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Summary: Essential Cell Biology (Alberts et al) - First part

Summary: Essential Cell Biology (Alberts et al) - First part

This summary is based on the 3rd edition of Essential Cell Biology from Alberts et al. The remaining chapters can be accessed here: Second part of the summary

1. Introduction to cells

Unity and diversity of cells

Cells are the fundamental units of life; all living things are made of cells. The present-day cells are believed to have evolved from an ancestral cell that excited more than 3 billion years age. Cells vary enormous in appearance and function, however all living cells have a similar basic chemistry.

With the invention of the microscope, it became clear that plants and animals are assemblies of cells, that cells can also exist as independent organisms, and that cells individually are living in the sense that they can grow, reproduce, convert energy from one form into another, respond to their environment, and so on. Although cells are varied when viewed from the outside, all living things are fundamentally similar inside. And in all living things, genetic instructions, called genes, are stored in DNA molecules. In every cell, the instructions in the DNA are read out, or transcribed, into a chemically related set of molecules made of RNA. The messages carried by the RNA molecules are in turn translated into yet another chemical form: they are used to direct the synthesis of a huge variety of large protein molecules that dominate the behaviour of the cell. In sum, the reproduction process exists of replication (DNA synthesis), transcription (RNA synthesis) and translation (protein synthesis). Unfortunately, the copying of DNA is not always perfect, and the instructions are occasionally corrupted. Later is this summary we will discuss this further.

Cells are enclosed by a plasma membrane that separates the inside of the cell from the environment. And all cells contain DNA as a store of genetic information and use it to guide the synthesis of proteins. Cells in a multicellular organism, though the all contain the same DNA, can be very different. They use their genetic information to direct their biochemical activities according to cues they receive from their environment.

Cells under the microscope

Cells of animal and plant tissues are typically 5-20 micrometer in diameter and can be seen with a light microscope, which also reveals some of their internal components (organelles). The electron microscope permits the smaller organelles and even individual molecules to be seen, but specimens require elaborate preparation and cannot be viewed alive. So, the invention of the light microscope led to the discovery of cells

The presence or absence of a nucleus is used as the basis for a simple but fundamental classification of all living things. Organisms whose cells have a nucleus are called eukaryotes. Organisms whose cells do not have a nucleus are called prokaryotes. Bacteria, the simplest of present-day living cells, are prokaryotes. Different species of prokaryotes are diverse in their chemical capabilities and inhabit an amazingly wide range of habitats. Prokaryotes are divided into two groups: eubacteria and archaea. As mentioned above eukaryotic cells possess a nucleus. They probably evolved in a series of stages from cells more similar to bacteria. An important step appears to have been the acquisition of mitochondria, origination as engulfed bacteria living in symbiosis with larger anaerobic cells.

There are a lot of organelles found in eukaryotic cells: the nucleus is the most prominent organelle in most plant and animal cells. It contains the genetic information of the organism, stored in DNA molecules. The rest of the cell’s contents, apart from the nucleus, constitute the cytoplasm. Chloroplasts are green organelles found only in the cells of plants and algae, not in the cells of animals or fungi. They perform photosynthesis and in the process they release oxygen as a molecular by-product. Other organelles are the mitochondria, which are generators of chemical energy for the cell. Mitochondria contain their own DNA and reproduce by dividing in two. Furthermore, they take the energy from the oxidation of food molecules to produce adenosine triphosphate (ATP). The endoplasmatic reticulum (ER) is the site at which most cell membrane components, as well as materials destined for export from the cell, are made.  The Golgi apparatus often modifies chemically the molecules made in the ER and directs them to various locations of the cell. Lysosomes are organelles in which intracellular digestion occurs and peroxisomes generate a dangerously reactive chemical, hydrogen peroxide. Finally, the cytoskeleton is responsible for directed cell movements.

Model organisms

Free-living single-celled eucaryotic micro organisms include some of the most complex eucaryotic cells known, and they are able to swim, mate, hunt and devour food. Other types of eukaryotic cells, derived from a fertilized egg, cooperate to form large, complex multicellular organisms composed of thousands of billions of cells.

Biologists have chosen a small number of organisms as a focus for intense investigation. These include the bacterium E. coli, brewer’s yeast, a nematode worm, a fly, a small plant, a mouse and the human species itself.
Although the minimum number of genes needed for a viable cell is probably less than 400, most cells contain significantly more. Yet even such a complex organism as a human has only about 30.000 genes – twice as many as a fly, seven times many as E. coli.

2. Chemical components of cells

Chemical bonds

The cell is the structural and functional unit of all known living organisms, but the smallest particle of an element that still retains its distinctive chemical properties is an atom. Each atom has as center a positively charged nucleus, which is surrounded by a cloud of negatively charged electrons. The nucleus consists of two kinds of particles:

  • positively charged protons

  • neutrons, which are electrically neutral

The number of protons present in an atomic nucleus determines its atomic number. Because the whole atom is electrically neutral, the number of negatively charged electron surrounding the nucleus is equal to the number of positively charged protons that the nucleus contains. Isotopes of an element have nuclei with the same number of protons (the same atomic number) but different numbers of neutrons.

The atomic weight of an atom, or the molecular weight of a molecule, is its mass relative to that of a hydrogen atom. The mass of an atom or a molecule is often specified in daltons. If a substance has a molecular weight of M, a mass of M grams of the substance will contain 6 x 10^23 molecules. This quantity is called one mole of the substance. The concept of mole is used widely in chemistry as a way to represent the number of molecules that are available to participate in chemical reactions. There are 92 naturally occurring elements, each differing from the others in the number of protons and electrons in its atoms. Living organisms are made of only a small selection of these elements.

The outermost electrons determine how atoms interact. The number and arrangement of its electrons determine the chemical properties of an atom. An atom is most stable when all of its electrons are at their lowest possible energy level and when each electron shell is completely filled. The number of electrons an atom must acquire of lose to attain a filled outer shell is known as its valence. Chemical bonds form between atoms as electrons move to reach a more stable arrangement. Clusters of two or more atoms held together by covalent bonds are known as molecules. There are two ways to create chemical bonds:

  • An ionic bond is formed when electrons are donated by one atom to another.
  • A covalent bond is formed when two atoms share a pair of electrons. If two pairs of electrons are shared, a double bond is formed. Double bonds are shorter and stronger than single bonds.

Also covalent and noncovalent chemical bonds have different strengths and lengths. Noncovalent bonds as a rule are much weaker.

Another noncovalent bond is the hydrogen bond, by which water is held together. These bonds are much weaker than covalent bonds. Molecules carrying positive or negative charges (ions) dissolve readily in water and are called hydrophilic, meaning that the are ‘water-loving’. Hydrophobic (water fearing) molecules on the other hand, are uncharged and form few or no hydrogen bonds, and so do not dissolve in water.

Substances that release protons when they dissolve in water and thus forming H3O+, are termed acids. The higher the concentration of H3O+, the more acidic the solution. The opposite of an acid is a base; any molecule capable of accepting a proton is called a base or alkaline. The concentration of H3O+ is expressed using the pH scale.

Molecules in Cells

Living organisms contain a distinctive and restricted set of small carbon-based molecules that are essentially the same for every living species. The main categories are:

  • Sugars: a primary source of chemical energy for cells and can be incorporated intro polysaccharides for energy storage

  • Fatty acids: also important for energy storage, but their most essential functions is in the formation of cell membranes. There are two kinds of fatty acids saturated and non-saturated. The first has no double bounds between its carbon atoms and contains the maximum possible numbers of hydrogens. The non-saturated fatty acids have tails with one or more double bounds. These double bounds create kinks in the molecules, interfering with their ability to pack together in a solid mass. How tightly the fatty acids, found in cell membranes, pack affects the fluidity of the membrane.

  • Amino acids: the subunits of proteins. The covalent linkage between two adjacent amino acids in a protein chain is called a peptide bound, the chain of amino acids is also known as a polypeptide.

  • Nucleotides: the subunits of DNA and RNA

These four families of small organic molecules, together with the macromolecules made by linking them into long chains, account for a large fraction of a cell’s mass.

Macromolecules in Cells

The vast majority of the dry mass of al cell consists of macromolecules, formed as polymers of sugars, amino acids, or nucleotides. Macromolecules are intermediated both in size and complexity between small molecules and cell organelles. They have many remarkable properties that are not easily deduced from the subunits from which they are made. Their remarkable diversity arises from the fact that each macromolecule has a unique sequence of subunits.

Noncovalent bounds specify the precise shape of a macromolecule: weak noncovalent bonds form between different regions of a macromolecule. Two types of noncovalent bounds are discussed earlier: ionic bounds and hydrogen bounds, but there is a third type of weak bound that result from ‘van der Waals attractions’. These attractions are a form of electrical attraction caused by fluctuating electric charges that whenever two atoms come within a very short distance of each other. These weak noncovalent bounds can cause the macromolecule to fold into a unique three-dimensional shape with a special chemistry, as seen in proteins.

3. Energy, catalysis and biosynthesis

Living organisms are able to exist because of a continual input of energy. Part of this energy is used to carry out essential functions, like reactions that support cellular metabolism, growth and reproduction, and the remainder is lost in the form of heat.

Catalysis and the use of energy

All animals live on energy stored in the chemical bonds of organic molecules made by other organisms, which they take as in food. Animals obtain food by eating plants or by eating animals that feed on plants. But ultimately, the primary source of energy for most living organisms is the sun.

Plants and photosynthetic bacteria use solar energy to produce organic molecules from carbon dioxide. They use the energy they derive from sunlight to form chemical bonds between atoms, linking them into small chemical building blocks such as sugar, amino acids, nucleotides and fatty acids. These small molecules in turn are converted into the macromolecules that form the plant.
The reactions of photosynthesis take place in two stages:

  1. In the light-dependent stage energy for the sunlight is captured and transiently stored as chemical bond energy in specialized small molecules that carry energy in their reactive chemical groups. Oxygen is released as a by-product of the first stage.

  2. In the second stage the molecules that serve as energy carriers are used to help drive a carbon-fixation process in which sugars are manufactured from carbon dioxide gas and water. By producing sugars, these light-independent reactions generate a critical source of stored chemical bond energy and materials.

The net result of the entire process of photosynthesis is:

Light energy + CO2 + H20 ® sugars + O2 + energy

To use to energy to live, grow and reproduce, organisms must extract it in a usable form. In both plants and animals, energy is extracted from food molecules by a process of oxidation, or controlled burning. Next to oxidation there is a process called cellular respiration.  Photosynthesis and cellular respiration are complementary processes; cellular respiration uses the O2 to form CO2 from the same carbon atoms that had been taken up as CO2 and converted into sugars by photosynthesis. In this process, the organisms obtain the chemical bond energy that they need to survive.

Oxidation refers to the removal of electrons and reduction (the converse of oxidation) refers to the addition of electrons. Because the number of electrons is conserved in a chemical reaction – there is no net loss or gain – oxidation and reduction always occur simultaneously.

Cells use enzymes to catalyze the oxidation of organic molecules in small steps, through a sequence of reactions that allows useful energy to be harvested.

Enzymes lower the barriers that block chemical reactions

Each of the many hundreds of chemical reactions that occur in a cell is specifically catalyzed by an enzyme. Large numbers of different enzymes work in sequence to form chains of reactions, called metabolic pathways, each performing a particular set of functions in the cell.

Catabolic reactions break down food molecules through oxidative pathways and release energy. Anabolic reactions generate the many complex molecules needed by the cell, and they require an energy input. In animal cells, both the building blocks and the energy required for the anabolic reactions are obtained by catabolism.

Enzymes catalyze reactions by binding to particular substrate molecules in a way that lowers the activation energy required for making and breaking specific covalent bonds. The rate at which an enzyme catalyzes a reaction depends on how rapidly it finds its substrate and how quickly the product forms and then diffuses away. These rates vary widely from one enzyme to another, and they can be measured after mixing purified enzymes and substrates together under a set of defined conditions. In general, the stronger the binding of the enzyme and substrate, the slower their rate of dissociation.

If a reactions leads to a release of free-energy, this energy can be harnessed to do work or drive chemical reactions. Chemical reactions proceed only in the direction that leads to a loss of free energy; in other words, the spontaneous direction for any reaction is the direction that goes ‘downhill’. This kind of reaction is often said to be energetically favorable. But even energetically favorable reactions require activation energy to get them started!

As mentioned above, the push over the energy barrier is greatly aided by enzymes. A substance that can lower the energy barrier, and hence the activation energy of a reaction is termed a catalysts. Like all other catalysts, enzyme molecules themselves remain unchanged after participating in a reaction and therefore can function over and over again.

If the concentration of the substrate is increased progressively from a very low value, the concentration of the enzyme-substrate complex, and therefore the rate at which product is formed, initially increases in a linear fashion in direct proportion to substrate concentration. But at a very high concentration of substrate it reaches a maximum value, termed Vmax. At this point, the active sites of all enzyme molecules in the sample are fully occupied with substrate, and the rate of product formation depends only on how rapidly the substrate molecule can be processed; also called the turnover number.

The concentration of substrate needed to make the enzyme work efficiently is often measured by a different parameter, the Michaelis’ constant (Km). An enzyme’s Km is the concentration of substrate at which the enzyme works at half its maximum speed (0.5 Vmax). A low value of Km indicated that a substrate binds very tightly to the enzyme, and a large value corresponds to weak binding. But enzymes cannot change the equilibrium point for reactions!

The free-energy change for a reaction determines whether it can occur

Although enzymes speed up reactions, they cannot by themselves force energetically unfavorable reactions to occur. But this can be done through enzymes that directly couple energetically favorable reactions, which release energy and produce heat, to energetically unfavorable reactions, which use this energy. But (according to the second law of thermodynamics) a chemical reaction can proceed only if it results in a net increase of the disorder in the universe. The criterion for an increase of disorder can be expressed most conveniently in term of free energy (G) of a system. The free-energy change for a reaction, ∆G, measures the disorder, and it must be less than zero for a reaction to proceed.

Energetically favorable reactions are those that create disorder by decreasing the free energy of a system to which the belong; in other words, they have a negative ∆G. Conversely, energetically unfavorable reactions, with a positive ∆G, create order in the universe. Because energetically unfavorable reactions require energy, they can take place only if they are coupled to a second reaction with a negative ∆G so large that the net ∆G of the entire process is negative.

In concluding, by creating a reaction pathway that couples an energetically favorable reaction to an energetically unfavorable one, enzymes cause otherwise impossible chemical transformations to occur.

The free-energy change for a chemical reaction, ∆G, depends on the concentration of the reacting molecules, and it may be calculated from these concentrations if the equilibrium constant (K) of the reaction (of the standard free-energy change ∆Gº for the reactants) is known. Because the equilibrium constant of a reaction is related directly to the standard free energy change (∆Gº), it is often employed as a measure of the binding strength between molecules. This value is very useful as it indicates the specificity of the interactions between molecules.

Equilibrium constants govern all of the associations (and dissociations) that occur between macromolecules and small molecules in the cell. The equilibrium constant becomes larger as the binding energy between the two molecules increases, and the more likely that these molecules will be paired.

Activated carrier molecules and biosynthesis

In living systems energy capture is achieved by means of a couple reactions, in which an energetically favorable reaction is used to drive and energetically unfavorable one that produces an activated carrier molecule. Coupling mechanisms require enzymes, and they are fundamental to all of the energy transactions in the cell. The most important of the activated carrier molecules are ATP, NADH and NADPH. ATP carries high-energy phosphate groups, whereas NADH an NADPH carry high-energy electrons.

1) ATP

The most important of the activated carrier molecules in cells is ATP (adenosine 5’-triphosphate). ATP is synthesized in an energetically unfavorable phosphorylation reaction in which a phosphate group is added to ADP (adenosine 5’-diphosphate). When required, ATP gives up this energy packet in an energetically favorable hydrolysis to ADP and inorganic phosphate. The regenerated ADP is then available to be used for another round of the phosphorylation reaction that forms ATP, creating an ATP cycle in the cell. Therefore, an energetically unfavorable biosynthetic reaction can be driven by ATP hydrolysis. For example, the synthesis of a polynucleotide likes RNA and DNA.

2) NADH an NADPH

NAD+ and NADP+ each pick up a ‘packet of energy’ in the form of two high-energy electrons plus a proton (H+), becoming NADH and NADPH, respectively. Like ATP, NADPH is an activated carrier that participates in many important biosynthetic reactions that would otherwise be energetically unfavorable. NADH, by contrast, has a special role as an intermediate in the catabolic system of reactions that generate ATP through the oxidation of food molecules.

Food molecules provide the carbon skeletons for the formation of larger molecules. The covalent bonds of these larger molecules are typically produced in reactions that are coupled to energetically favorable bond changes in activated carrier molecules such as ATP and NADPH.

4. Protein structure and function

Proteins are by far the most structurally complex and functionally sophisticated molecules known. Proteins are assembled from a set of 20 different amino acids, each with different chemical properties. A protein molecule is made from a long chain of these amino acids, each linked to its neighbor through a covalent peptide bond. Proteins, therefore, are also called polypeptides. Each polypeptide chain consists of a backbone that supports the different amino acid side chain. The polypeptide backbone if formed from the repeating sequence of atoms along the polypeptide chain. Attached tot this repetitive chain are any of the 20 different amino acid side chains. These side chains give each amino acid its unique properties, for example hydrophobic, nonpolar or positively charged.

Shape and structure of proteins

Each type of protein has a unique amino acid sequence that determines both its three-dimensional shape and its biological activity. Long peptides are very flexible and therefore proteins can fold in enormous number of ways. The folded structure of a protein is stabilized by noncovalent interactions between different parts of the polypeptide chain.

The final folded structure, of conformation, is the one in which the free energy (G) is minimized. A protein can be unfolded, or denatured, by treatment with certain solvents that disrupt the noncovalent interactions holding the folded chain together. When the denaturing solvent is removed, the protein often refolds spontaneously, or renatures, into its original conformation.

When proteins fold improperly, the can form aggregates that can damage cells and even whole tissue. Aggregated proteins underlie a number of neurodegenerative disorders, including Alzheimer’s disease and Huntington’s disease. Although a protein chain can fold into its correct conformation without outside help, protein folding in a living cell in generally assisted by special proteins called molecular chaperones. These proteins bind to partly folded chains and help them to fold along the most energetically favorable pathway.  However, the final three-dimensional shape of the protein is still specified by its amino acid sequence: chaperones merely make the folding process more efficient and reliable.

Although the overall conformation of each protein is unique, two regular folding patterns are often found in parts of them. Hydrogen bonds between neighboring regions of the polypeptide backbone can give rise to regular folding patterns, known as a helices and b sheets. In an a helix the N-H of every peptide bond is hydrogen-bonded to the C=O of a neighboring peptide bond located four peptide bonds away in the same chain. In the case of the b sheet the individual polypeptide chains in the sheet are held together by hydrogen-bonding between peptide bonds in different strands, and the amino acid side chains in each strand project alternately above and below the plane of the sheet.

A a helix is generated when a single polypeptide chain turns around itself to form a structurally rigid cylinder. Sometimes a pair of a helices will wrap around one another to form a particularly stable structure, known as coiled-coil. This structure forms when the two a helices have most of their nonpolar (hydrophobic) side chains on one side, so that they can twist around each other with these side chains facing inwards. b Sheets are made when hydrogen bonds form between segments of polypeptide chains lying side by side. When the structure consists of neighboring polypeptide chains that run in the same orientation, it is considered a parallel b sheet; when it forms from a polypeptide chain that fold back and forth upon itself the structure is an antiparallel b sheet. b Sheets provide an ideal ice-binding surface in an antifreeze protein.

Levels of organization

The structure of many proteins can be subdivided into smaller globular regions of compact three-dimensional structure, known as protein domain. So, a protein’s structure begins with its amino acid sequence, which is thus considered its primary structure. The next level of organization includes the a helices and b sheets that form within certain segments of polypeptide chain; these folds are elements of the protein’s secondary structure. The full, three-dimensional conformation formed by an entire polypeptide chain is referred as the tertiary structure. Finally, if a particular protein molecule is formed as a complex of more than one polypeptide chain, than the complete structure is designed its quaternary structure.

The same weak noncovalent bonds that enable a polypeptide chain to fold into a specific conformation also allows proteins to bind to each other to produce larger structures in the cell. Any region on a protein’s surface that interacts with another molecule through sets of noncovalent bonds is termed a binding site. If a binding site recognizes the surface of a second protein, the tight binding of two folded polypeptide chains at this site will create a larger protein molecule with a precisely defined geometry. Each polypeptide chain in such a protein is called a subunit. Each of these protein subunits may contain more than one domain.

There are different types of proteins:

  1. Globular proteins: in which the polypeptide chain folds up into a compact shape like a ball with an irregular surface. Enzymes tend to be globular proteins.

  2. Fibrous proteins: these have a relatively simple, elongated three-dimensional structure. These proteins are especially abundant outside the cell, where they form the gel-like extracellular matrix that helps cells bind together to form tissues. These proteins are secreted by cells into their surface roundings, where they often assemble into sheets of long fibrils. Collagen is the most abundant of these fibrous proteins in animal tissues, and another example is elastin.

To help maintain their structures, the polypeptide chains in such proteins are often stabilizes by covalent cross-linkages. The most common cross-links in proteins are covalent sulfur-sulfur bonds. These disulfide bonds (also called S-S bonds) form as proteins are being exported from cells. Their formation is catalyzed in the endoplasmatic reticulum by a special enzyme that links together two –SH groups from cysteine side chains that are adjacent in the folded protein.

How proteins work

The biological function of a protein depends on the detailed chemical properties of its surface and how it binds to other molecules, called ligands. The ability of a protein to bind selectively and with high affinity to a ligand is due to the formation of a set of weak, noncovalent bonds and favorable hydrophobic interactions. Each individual bond is weak, so that an effective interaction requires that many weak bonds be formed simultaneously. The region of a protein that associates with a ligand, known as its binding sites, usually consists of a cavity in the protein surface formed by a particular arrangement of amino acids. These amino acids belong to widely separated regions of the polypeptide chain that are brought together when the proteins fold.

All proteins must bind to particular ligands to carry out their various functions. But this binding capacity seems to have been most highly developed for proteins in the antibody family. Antibodies, or immunoglobulins, are proteins produced by the immune system in response to foreign molecules. Each antibody binds to a particular target molecule, either inactivating that target directly or marking it for destruction. An antibody is Y-shaped and has two identical binding sites for its antigen, one on each arm of the Y.

For many proteins, binding to another molecule is their only function, but there are some proteins for which ligand binding is simply a necessary first step in their functions. This class of proteins is called enzymes. Enzymes are proteins that first bind tightly to specific molecules, called substrates, and then catalyze the formation or breakage of covalent bonds in these molecules. At the active site of an enzyme, the amino acid side chains of the folded protein are precisely positioned so that they favor the formation of the high-energy transition states that the substrates must pass through to be converted to product.
The three-dimensional structure of many proteins has evolved so that the binding of a small ligand can induce a significant change in protein shape.

Although the order of amino acids in proteins gives molecules their shape and the versatility to perform different functions, sometimes the amino acids by themselves are not enough. So proteins often employ small nonprotein molecules to perform functions that would be difficult or impossible using amino acids alone. Examples of these proteins are retinal (the light-sensitive molecule attached to rhodopsin in our eyes) and heme (gives hemoglobin and blood its red color, and enables hemoglobin to pick up oxygen in the lungs and release it in the tissues).

How proteins are controlled

Inside the cell most proteins and enzymes do not work continuously or at full speed. Instead, their activity is regulated so that the cell can maintain itself in a state of equilibrium, generating only those molecules it requires to thrive under the current conditions. To achieve this balans, the activities of cellular proteins are controlled in an integrated fashion, with consideration of what reactions are occurring in other parts of the cell. By coordinating when and how proteins function, the cell ensures that it does not deplete its energy reserves by accumulating molecules it does not require.

Regulation of enzyme activity occurs at many levels. At one level, the cell controls how many molecules of each enzyme it makes by regulating the expression of the gene that encodes that protein. At another level, the cell controls enzymatic activities by confining sets of enzymes to particular subcellular compartments, enclosed by distinct membranes (both mechanisms are discussed later in this summary). But the most rapid and general process used to adjust reactions rates operated at the level of the enzyme itself. In this case, an enzyme’s activity changes in response to other specific molecules that it encounters.

  • Feedback inhibition (negative feedback): it prevents an enzyme from acting
  • Positive regulation (positive feedback): the enzyme’s activity is stimulated

The interaction between sites that are located on separate regions of a protein molecule is known to depend on a conformational change in the protein: binding at one of the sites causes a shift in the protein’s structure from one folded shape to a slightly different folded shape. Feedback inhibition, for example, triggers a conformational change. Many, if not most, protein molecules are allosteric: they can adopt two or more slightly different conformations that differ in catalytic activity, and by a shift from one to another, their activity can be regulated. This is true not only for enzymes but for many other proteins like receptors, structural proteins, and motor proteins. The enzyme can be turned on or off by ligands that bind to a distinct regulatory site to stabilize either the active or the inactive conformation.

Phosphorylation can control protein activity by triggering a conformational change

Enzymes are not only regulated by the binding of small molecules. A second method commonly used by eukaryotic cells to regulate protein activity involves attaching a phosphate group covalenty to one of its amino acids side chains. Removal of the phosphate group by a second enzyme returns the protein to its original conformation and restores its initial activity. This reversible protein phosphorylation controls the activity of many different types of proteins in eukaryotic cells.

Protein phosphorylation involves the enzyme-catalyzed transfer of the terminal phosphate group of ATP to the hydroxyl group on a serine, threonine, of tyrosine said chain of the protein. This reaction is catalyzed by a protein kinase. The reverse reaction – removal of the phosphate group, or dephosphorylation – is catalyzed by a protein phosphatase. Cells contain hundreds of different protein kinases, each responsible for phosphorylating a different protein or set of proteins. Cells also contain many different protein phosphatases.

For many proteins, a phosphate group is added to a particular side chain and then removed in a continuous cycle. Phosphorylation cycles of this kind allow proteins to switch rapidly from one state to another. The energy required to drive this cycle is derived from the free energy of hydrolysis of ATP.

GTP-Binding proteins are also regulated by cyclic gain and loss of a phosphate group

Eucaryotic cells have another way to regulate protein activity by phosphate addition and removal. Instead of being enzymatically transferred from ATP to the protein, the phosphate is part of a guanine nucleotide (either GTP or GDP) that is bound tightly to the protein. Such GTP-binding proteins are in their active conformations with GTP bound; the protein itself then hydrolyses this GTP to GDP, by releasing a phosphate, and flips to an inactive conformation. As with protein phosphorylation, this process is reversible.

The GTP-binding proteins often bind to other proteins to control enzyme activities, and their crucial role in intracellular pathways will be discussed later in this summary.

In concluding, many thousands of proteins in a typical eucaryotic cell are regulated either by cycles of phosphorylation and dephosphorylation, or by the binding and hydrolysis of GTP by a GTP-binding protein.

Nucleotide hydrolysis

As mentioned above, conformational changes in proteins play a central part in enzyme regulation and cell signaling. But conformational changes also play another important role in the operation of the cell: they enable proteins whose major function is to move other molecules, the motor proteins, to generate the forces responsible for muscle contraction and the movements of the cell. The hydrolysis of ATP to ADP by motor proteins produces directed movements in the cell.

Proteins often form large complexes that function as protein machines

Highly efficient proteins machines are formed by assemblies of allosteric proteins. In most protein machines the hydrolysis of bound nucleoside triphosphates (ATP or GTP) drives an ordered series of conformational changes in some of the individual protein subunits, enabling the ensemble of proteins to move coordinately. In this way, the appropriate enzymes can be moved directly into the positions where they are needed to carry out successive reactions in a series as, for example, protein synthesis or DNA replication.

5. DNA and chromosomes

The structure and function of DNA

Life depends on stable and compact storage of genetic information. Genetic information is carried by very long deoxyribonucleic acid (DNA) molecules and encoded in the linear sequence of nucleotides A, T, G and C.
A DNA molecule consists of two long polynucleotide chains known as DNA chains, or DNA strands. Each of these chains is composed of four types of nucleotide subunits, and the two chains are held together by hydrogen bonds between the base portions of the nucleotides, nucleotides are composed of a five-carbon sugar to which are attached one or more phosphate groups and a nitrogen-containing base. In the case of the nucleotides in DNA, the sugar is deoxyribose attached to a single phosphate group, and the base may by adenine (A), cytosine (C), guanine (G), or thymine (T). The nucleotides are covalently linked together in a chain through the sugars and phosphates, which thus form a ‘backbone’ of alternating sugar-phosphate-sugar-phosphate.

The two polynucleotide chains in the DNA double helix are held together by hydrogen-bonding between the bases on the different strands; G-C and A-T. All the bases are therefore on the inside of the helix, with the sugar-phosphate backbones on the outside.
Each strand of DNA has a chemical polarity due to the linkage of alternating sugars and phosphates in its backbone The members of each base pair can fit together within the double helix only if the two strands of the helix are antiparallel, that is, only if the polarity of one strand is oriented opposite to that of the other strand. A consequence of these base-pairing requirements is that each strand of a DNA molecule contains a sequence of nucleotides that is exactly complementary to the nucleotide sequence of its partner strand. This is crucial importance for the copying of DNA, as we will see later in the summary.

The structure of eukaryotic chromosomes

Large amounts of DNA are required to encode all the information needed to make just a single-celled bacterium, and far more DNA is needed to encode the instructions for the development of multicellular organisms like ourselves.

In eukaryotic cells, enormously long double-stranded DNA molecules are package into chromosomes can be easily apportioned between the two daughter cells at each cell division. In eucaryotes the DNA in the nucleus is distributed among a set of different chromosomes. Each chromosome consists of a single, enormously long, linear DNA molecule associated with proteins that fold and pack the fine thread of DNA into a more compact structure. The complex of DNA and protein is called chromatin.
With the exception of the germ cells (sperm and eggs) and highly specialized cells that lack DNA entirely, human cells each contain two copies of each chromosome, one inherited from the mother and one from the father; the maternal and paternal chromosomes of a pair are called homologous chromosomes (homologs). The only nonhomologous chromosome pairs are the sex chromosomes in males, where a Y chromosome is inherited from the father and an X chromosome from the mother.

A display of the full set of 46 chromosomes is called the human karyotype. Cytogeneticists use alterations in banding patterns to detect chromosomal abnormalities that are associated with some inherited defects and with certain types of cancer.

The genetic material of a eukaryotic cell is contained within one or more chromosomes, each formed from a single, enormously long DNA molecule that contains many genes. In general, the more complex an organism is, the larger its genome. Furthermore, how the DNA is apportioned over chromosomes also differ from one species to another. Humans have 46 chromosomes, but a species of small deer has only 6 chromosomes. Thus, although gene number is roughly correlated with species complexity, there is no simple relationship between gene number, chromosome number and total genome size.

‘Life-cycle of chromosomes’

To form a functional chromosome, a DNA molecule must be able to replicate, and the replicated copies must be separated and partitioned reliably into daughter cells at each cell division. These processes occur through an ordered series of stages, known collectively as the cell cycle.

Two stages are important:

  1. the interphase, when chromosomes are duplicated;
  2. and mitosis, when they are distributed to the two daughter nuclei.

During interphase, the cell is actively expressing its genes, and during this stage the chromosomes are extended as long, thin, tangled threads of DNA in the nucleus. Still during the interphase and before cell division, the DNA is replicated and the chromosomes are duplicated. Once DNA replication is complete, the cell can enter M phase, when mitosis occurs. Mitosis is the division of the nucleus. During this stage, the chromosomes condense, gene expression largely ceases, the nuclear envelope breaks down, and the mitotic spindle forms from microtubules and other proteins. The condensed chromosomes are captured by the mitotic spindle, and one complete set of chromosomes is pulled to each end of the cell. A nuclear envelope form around each chromosome set, and in the final step of M phase, the cell divides to produces two daughter cells.

Three DNA sequence elements are needed to produce a eukaryotic chromosome that can be replicated and then segregated at mitosis. These sequences ensure that the chromosome can be replicated efficiently and passed on to daughter cells.

  1. Telomere: contain repeated nucleotide sequences that enable the ends of chromosomes to be replicated. They also protect the end of the chromosome from being mistaken by the cell as a broken DNA molecule in need of repair. But the function of telomeres is discussed later in this summary.

  2. Replication origin

  3. Centromere: this allows one copy of each duplicated chromosome to be apportioned to each daughter cell.

The nucleus is delimited by a nuclear envelope formed by two concentric membranes. The nuclear envelope is supported by two networks of protein filaments: one, the nuclear lamina, forms a thin layer underlying and supporting the inner nuclear membrane; while the other, less regularly organized, surrounds the outer nuclear membrane. The two membranes are punctured at intervals by nuclear pores, which actively transport selected molecules to and from the cytosol.

The most obvious example of chromosome organization in the interphase nucleus is the nucleolus. This is a region where the parts of different chromosomes carrying genes for ribosomal RNA cluster together. Here, ribosomal RNAs are synthesized and combined with proteins to form ribosomes, the cell’s protein-synthesizing machines.

Chromosomes and DNA

Chromosomes in eukaryotic cells consist of DNA tightly bound to a roughly equal mass of specialized proteins. These proteins fold the DNA into a more compact form so that it can fit into a cell nucleus.

The proteins that bind to the DNA to form eukaryotic chromosomes are traditionally divided into two general classes: the histones and the nonhistone chromosomal proteins. The complex of DNA and both classes of protein in chromosomes is called chromatin. Histones are responsible for the first and most fundamental level of chromatin packing: they pack DNA into a repeating array of DNA-protein particles called nucleosomes.

An individual nucleosome core particle consists of a complex of eight histone proteins (two molecules each of the histone H2A, H2B, H3 and H4) and a double stranded DNA of about 146 nucleotide pairs that winds around this histone octamer. Each nucleosome core particle is separated from the next by a region of linker DNA.

All four of the histones that make up the nucleosome core are relatively small proteins with a high proportion of positively charged amino acids. The positive charges help the histones bind tightly to the negatively charged sugar-phosphate backbone of DNA. Each of the core histones also has a long N-terminal amino acid ‘tail’, which extends out from the DNA histone core. These histone tails are subject to several types of covalent modification that control many aspects of chromatin structure.

Nucleosomes are further packed upon one another to generate a more compact structure, the 30-nm fiber. This happens with the aid of histone H1 molecules, which is thought to pull the nucleosomes together into a regular repeating array. This fiber can be further coiled and folded, producing more compact chromatin structures. But, some forms of chromatin are so highly compacted that the packaged genes cannot be expressed into protein.

As daughter cells complete their separation following mitosis, the mitotic chromosomes unfold into a more extended form: the interphase chromosomes. However, the chromatin in an interphase chromosome is not in the same packing state throughout the chromosome. In general, regions of the chromosome that contain genes that are being expressed are more extended, while those that contain quiescent genes are more compact. The most highly condensed form of interphase chromatin is called heterochromatin. Heterochromatin typically makes up about 10% of an interphase chromosome, and in mammalian chromosomes, it is typically concentrated around the centromere region and in the telomeres at the ends of the chromosomes. Most DNA that is folded into heterochromatin does not contain genes. However, genes that do become packaged into heterochromatin usually become resistant to being expressed because heterochromatin is unusually compact. The rest of the interphase chromatin, which is in a variety of more extended states, is called euchromatin.

Changes in nucleosome structure allow access to DNA

Eucaryotic cells have several ways to rapidly adjust the local structure of their chromatin. One approach takes advantage of chromatin remodeling complexes, protein machines that use the energy of ATP hydrolysis to change the structure of nucleosomes.

In concluding, chromatin structure is dynamic: by temporarily altering its structure (using chromatin remodeling complexes and enzymes that modify histone tails) the cell can ensure that proteins involved in gene expression, replication, and repair have rapid, localized access to the necessary DNA sequences.

6. DNA replication, repair and recombination

The ability of a cell to maintain order in a chaotic environment depends on the accurate duplication of the vast quantity of genetic information carried in its DNA. This duplication process, called DNA replication, must occur before a cell can produce two genetically identical daughter cells.

Despite systems for protecting the genetic instructions form copying errors and accidental damage, permanent changes, or mutations, sometimes do occur. Mutations in the DNA often affect the information it encodes. Occasionally, this can benefit the organism in which a mutation occurs. However, mutations are often detrimental: they are responsible for thousands of inherited diseases and many types of cancer. Without the cellular systems that are continually monitoring and repairing damage to DNA, it is questionable whether life could exist at all.

DNA replication

As mentioned earlier, each strand of the DNA double helix contains a sequence of nucleotides that is exactly complementary to the nucleotide sequence of its partner strand. Each strand can therefore act as a template for the synthesis of a new complementary strand.
The ability of each strand of a DNA molecule to act as a template for producing a complementary strand enables a cell to copy, or replicate, its genes before passing them on to its descendants. This replication is performed by a cluster of proteins that together form a ‘replication machine’. In each round of replication, each of the two strands of DNA is used as a template for the formation of a complementary DNA strand. The original strands, therefore, remain intact through many cell generations. DNA replication is called ‘semiconservative’ because each daughter DNA double helix is composed of one conserved strand and one newly synthesized strand.

DNA synthesis

1) DNA synthesis begins at replication origins

The DNA double helix is normally very stable, because the two DNA strands are locked together by the large numbers of hydrogen bonds between the bases on both strands. The process of DNA replication begins by initiator proteins that bind to the DNA and pulled the two strands apart, by breaking the hydrogen bonds between the bases. Although the hydrogen bonds collectively make the DNA helix very stable, individually each hydrogen bond is weak. Separating a short length of DNA does not therefore require a large energy input. The positions at which the DNA is first opened are called replication origins, and they are usually marked by a particular sequence of nucleotides. An A-T base pair is held together by fewer hydrogen bonds than is a G-C base pair, therefore DNA rich in A-T base pairs is relatively easy to pull apart, and A-T-rich stretches of DNA are typically found at replication origins.
Once an initiator protein binds to DNA at the replication origin and locally opens up the double helix, it attracts a group a proteins that carry out DNA replication. This group operates as a protein machine, with each member carrying out a specific function.

2) New DNA synthesis occurs at replication forks

As a DNA molecule replicates, its two strands are pulled apart to form one or more Y-shaped replication forks. At these forks, the replication machine is moving along the DNA, opening up the two strands of the double helix and using each strand as a template to make a new daughter strand. The enzyme DNA polymerase, situated in the fork, catalyzes the addition of nucleotides to the 3’ end of a growing DNA strand by forming a phosphodiester bond between this end and the 5’-phosphate group of the incoming nucleotide.

In concluding, DNA polymerase can catalyze the growth of the DNA chain in only one direction: the 5’-to-3’ direction. This problem is solved by the use of a ‘backstitching’ maneuver. The DNA strand whose 5’ end must grow is made discontinuously, in successive separate small pieces, with the DNA polymerase working backward from the replication fork in the 5’-to-3’ direction for each new piece. These pieces, called Okazaki fragments, are later ‘stitched’ together (by the enzyme ligase) to form a continuous new strand. The DNA strand that is synthesized discontinuously in this way is called the lagging strand; the strand that is synthesized continuously is called the leading strand. Because both of the new strands are synthesized in the 5’-to-3’ direction, the DNA replication forks are asymmetrical.

DNA polymerase

DNA polymerase replicated a DNA template with remarkable fidelity, making less tan one error in every 10^7 bases read. This is possible because the enzyme removes its own polymerization errors as it moves along the DNA (proofreading). Before the enzyme adds a nucleotide to a growing DNA chain, it checks whether the previous nucleotide added is correctly base-paired to the template strand. If so, the polymerase adds the next nucleotide; if not, the polymerase removes the mispaired nucleotide by cutting the phosphodiester bond it has just made, releases the nucleotide, and tries it again. Thus, DNA polymerase possess both a 5’-to-3’ polymerization activity and a 3’-to-5’ exonuclease (nucleic acid-degrading) activity.

This proofreading mechanism explains why DNA polymerase synthesize DNA only in the 5’-to-3’ direction. If DNA is synthesized in the 3’-to-5’ direction is would be unable to proofread: because if it removed an incorrectly paired nucleotide, the polymerase would create a chain end that is dead and unable to elongate.

Because the polymerase can join a nucleotide only to a base-paired nucleotide in a DNA double helix, it cannot start a completely new DNA strand. A different enzyme is needed and it is called primase. This enzyme makes short lengths of RNA, called primers, which are subsequently erased and replaced with DNA.

For the leading strand, an RNA primer is needed only to start replication at a replication origin; once a replication fork has been established, the DNA polymerase is continuously present with a base-paired 3’ end as it tracks along the template strand. But on the lagging strand, where DNA synthesis is discontinuous, new primers are needed continually.

To produce a continuous new DNA strand from the many separate pieces of RNA and DNA made on the lagging strand, three additional enzymes are needed. These act quickly to remove the RNA primer (nuclease), replace it with DNA (repair polymerase), and join the DNA fragments together (ligase).

Proteins at a replication fork

DNA replication requires the cooperation of many proteins: at the head of the replication machine is a helicase, a protein that uses the energy of ATP hydrolysis to speed along DNA, unzipping the double helix as it moves. Another component of the replication machine, the single-strand binding proteins clings to the single-stranded DNA exposed by the helicase and transiently prevents is from re-forming base pairs. Yet another protein, called a sliding clamp, keeps the DNA polymerase firmly attached to the DNA template; on the lagging strand, the sliding clamp releases the polymerase from the DNA each time an Okazaki fragment is completed. This clamp proteins forms a ring around the DNA helix and binds polymerase, allowing it to slide along a template strand as it synthesis new DNA.

Most of the proteins involved in DNA replication are thought to be held together in a large multienzyme complex that moves as a unit along the DNA, enabling DNA to be synthesized on both strands in a coordinated manner.  

Genetic information can be stored stably in DNA sequences only because a variety of DNA repair enzymes continuously scan the DNA and correct replication mistakes and replace damaged nucleotides. DNA can be repaired easily because one strand can be corrected using the other strand as a template.

Telomerase replicates the ends of eukaryotic chromosomes

In eucaryotes, a special enzyme called telomerase replicated the DNA at the ends of the chromosomes. Telomerase adds multiple copies of the same telomere DNA sequence to the ends of the chromosomes, thereby producing a template that allows replication of the lagging strand to be completed.

DNA repair

To survive and reproduce, individuals must be genetically stable. This stability is achieved not only through the extremely accurate mechanism for replicating DNA, but also through mechanisms for correcting the rare copying mistakes made by the replication machinery and for repairing the accidental damage that continually occurs to the DNA. Most of these changes in DNA are only temporary because they are immediately corrected by processes collectively called DNA repair.

Only rarely do the cell’s DNA replication and repair processes fail and allow a permanent change in the DNA. Such a permanent change is called a mutation. For example, a single nucleotide change causes the inherited disease sickle-cell anemia. It is very important to protect reproductive cells (germ cells) against mutation, because a mutation in one of these cells will be passed on to all the cells in the body of the multicellular organism that develops from it, including the germ cells for production of the next generation. However, the other cells (somatic cells) must also be protected from genetic change to safeguard the health and well-being of the individual. Therefore, cells have acquired an elegant set of mechanisms to reduce the number of mutations that occur in their DNA.

DNA mismatch repair system

The rare copying mistakes that slip through the DNA replication machinery are dealt with by the mismatch repair proteins, which monitor newly replicated DNA and repair copying mistakes. The overall accuracy of DNA replication, including mismatch repair, is one mistake per 10^9 nucleotides copied.

A complex of mismatch repair proteins recognizes the DNA mismatches, removes (excises) one of the two strands of DNA involved in the mismatch, and resynthesizes the missing strand. To be effective in correcting replication mistakes, this mismatch repair system must always excise only the newly synthesized DNA, and thus, eliminating the mutation by using the original (old) template strand as the template. The importance of mismatch repair in humans was recognized when it was discovered that an inherited predisposition to certain cancers (especially some types of colon cancer) is caused by a mutation in the gene responsible for producing one of the mismatch repair proteins.

DNA is continually suffering damage in cells. There are many ways in which the DNA can be damaged, and these require other mechanism, than mismatch repair proteins, for their repair. Depurination and deamination are the most frequent chemical reactions known to create serious DNA damage in the cell. Furthermore, the ultraviolet radiation in sunlight causes also DNA damage.
The basic mechanism of DNA repair involved three steps:

  • Excision
  • Resynthesis
  • Ligation

In step one (excision), the damage is recognized and removed by one of a variety of different nuclease, which cleave the covalent bond that join the damaged nucleotides to the rest of the DNA molecule, leaving a small gap on one of the DNA double helix in this region. In step two (resynthesis), a repair DNA polymerase binds to the 3’-hydroxyl ends of the cut DNA strand. In then fills the gap by making a complementary copy of the information stored in the undamaged strand. In step three (ligation), DNA ligase seals the nick left in the sugar-phosphate backbone of the repaired strand. Nick sealing requires energy from ATP hydrolysis, remakes the broken phosphodiester bond between the adjacent nucleotides.

teps two and three are nearly the same for most types of DNA repair, including mismatch repair. However, step one uses a series of different enzymes, each specialized for removing different types of DNA damage.

DNA recombination

Homologous recombination is the process by which two double-stranded DNA molecules of similar nucleotide sequence can cross over to create DNA molecules of novel sequence. Homologous recombination begins with a double-strand break in a chromosome, creating a complete break in the DNA molecule. The 5’ ends at the break are then chewed back by a DNA-digesting enzyme, creating protruding single-stranded 3’ ends. Each of these single strands then searches for a homologous, complementary DNA helix with which to pair, leading to the formation of a ‘joint-molecule’ between the two chromosomes. The nicks in the DNA strands are then sealed and this is known as a cross-strand exchange or ‘Holliday junction’. To regenerate two separate DNA molecules, the two crossing strands must be cut. The structure undergoes a series of rotational movements so that the two original noncrossing strands become crossing and vice versa.

Homologous recombination provides many advantages to cells and organisms:

  • The process allows an organism to repair DNA that is damaged on both strands of the double helix
  • It can fix other genetic accidents that occur during nearly every round of DNA replication
  • It is essential for the accurate chromosome segregation that occurs during meiosis in fungi, plants and animals.

In homologous recombination, DNA rearrangements occur between DNA segments that are very similar in sequence. A second type of recombination, called site-specific recombination, allows DNA exchange to occur between DNA double helices that are not similar in nucleotide sequences. Mobile genetic elements are thought to play a crucial role in this process. Mobile genetic elements are DNA sequences that can move from place to place in the genomes of their host. This movement creates change in the host genome provides a source of genetic variation.

More than 50% of the human genome consists of DNA that is repeated many times in the genome. Approximately two-thirds of this repeated DNA (about 34% of the total genome) consists of two classes of transposons that have multiplied to especially high copy numbers in the genome. Retrotransposons move via an RNA intermediate, instead of a DNA intermediate. One type of retrotransposon, the L1 element (or LINE-1), is a highly repeated sequence that constitutes about 15% of the total mass of the human genome.

Viruses are mobile genetic elements that can escape from cells
Viruses are little more than genes packaged in protective protein coats. They require host cells in order to reproduces themselves. Viral genomes can be made of DNA or RNA and can be single-stranded or double-stranded. One group of RNA viruses – the retrovirus – must copy their RNA genomes into DNA in order to replicate. The human immunodeficiency virus (HIV), which is the cause of AIDS, is a retrovirus.

7. From DNA to protein

When a particular protein is needed by the cell, the nucleotide sequences of the appropriate portion of the immensely long DNA molecule in a chromosome is first copies into another type of nucleic acid – RNA (ribonucleic acid). It is these RNA copies of short segments of the DNA that are used as templates to direct the synthesis of the protein.

The flow of genetic information in all living cells is therefore from DNA ® RNA ® protein. The conversation of the genetic instructions in DNA into RNAs and proteins is termed gene expression.

From DNA to RNA

To express the genetic information carried in DNA, the nucleotide sequence of a gene is first transcribed into RNA. Like DNA, RNA is a linear polymer made of four different types of nucleotide subunits linked together by phosphodiester bonds. It differs from DNA chemically in two ways:

  1. The nucleotides in RNA are ribonucleotides; they contain the sugar ribose rather than deoxyribose

  2. Although RNA and DNA both contain the bases adenine (A), guanine (G), and cytosine (C), RNA contains uracil (U) instead of thymine (T) found in DNA.

Next to the chemical differences, there are also important differences in overall structure. Whereas DNA always occurs in cells as a double-stranded helix, RNA is single-stranded. This difference has important functional consequences; because RNA is single-stranded it can fold up into a variety of three-dimensional shapes. As we will see later in this summary, this ability allows RNA to carry out different functions, like for example catalytic functions.

All of the RNA in a cell is made by transcription. The enzymes that carry out transcription are called RNA polymerase. RNA polymerases catalyze the formation of phosphodiester bonds that link the nucleotides together and form the sugar-phosphate backbone of the RNA chain. The RNA polymerase moves stepwise along the DNA, unwinding the DNA helix to expose a new region of the template strand for complementary base-pairing. Nucleotide sequences in the DNA molecule indicate to the RNA polymerase where to start and stop transcribing. A promotor contains a sequence of nucleotides indicating the starting point for RNA synthesis. A subunit of bacterial polymerase, called sigma (s) factor, is primarily responsible for recognizing the promotor sequence on DNA.

RNA polymerase make about one mistake for every 10^4 nucleotides copied into RNA, compared with an error rate for DNA polymerase of about one in 10^7 nucleotides. Although RNA polymerase catalyzes essentially the same chemical reactions as DNA polymerase, there are some important differences between the two enzymes:

  • RNA polymerase catalyzes the linkage of ribonucleotides, not deoxyribonucleotides
  • Unlike the DNA polymerase involved in DNA replication, RNA polymerase can start an RNA chain without a primer

Several types of RNA are produces in cells

Cells make several different functional types of RNA, including messenger RNA (mRNA), which carries the instructions for making proteins, ribosomal RNA (rRNA), which is a component of ribosome’s; and transfer RNA (tRNA), which acts as an adaptor molecule in proteins synthesis.

Although the templating principle by which DNA is transcribed into RNA is the same in all organisms, the way in which the RNA transcripts are handled before the can be used by the cell differs a great deal between bacteria and eucaryotes. Bacterial DNA lies directly exposed to the cytoplasm, which contains the ribosomes on which protein synthesis takes places. In eukaryotic cells, by contrast, DNA is enclosed within the nucleus. Transcription takes place in the nucleus, but protein synthesis takes place on ribosomes in cytoplasm. So, before mRNA can be translated, it must be transported out of the nucleus. In addition, before RNA exists in the nucleus, it must go through several different RNA processing steps. Two processing steps that occur only on transcripts destines to become mRNA molecules are:

  • RNA capping
  • Polyadenylation

These two modifications are thought to increase the stability of the eukaryotic mRNA molecule, to aid its export from the nucleus to the cytoplasm, and to generally identify the RNA molecule as an mRNA. They are also used by the protein-synthesis machinery as an indication that both ends of the mRNA are present and that the message is therefore completed.

Genes are interrupted by noncoding sequences

In eukaryotic DNA most genes are composed of a number of smaller coding regions (exons) interspersed with noncoding regions (introns). When a eukaryotic gene is transcribed from DNA into RNA, both exons and introns are copied. After capping, as the RNA polymerase continues to transcribe the gene, the process of RNA splicing begins, in which the intron sequences are removed from the newly synthesized RNA and the exons are stitched together. RNA splicing is performed by RNA molecules that recognize intron-exon boundaries and participate in the chemistry of splicing. These RNA molecules, called small nuclear RNAs (snRNAs), bind with additional proteins to form small nuclear ribonucleoprotein particles (snRNPs). These snRNPs form the core of the spliceosome, the largely assembly of RNA and protein molecules that performs RNA splicing in the cell. To splice an RNA, a group of snRNPs assemble at an intron-exon boundary, cut out the intron, and rejoin the RNA chain.

In concluding, eucaryotic mRNAs go through several additional RNA processing steps before the leave the nucleus, including RNA capping and polyadenylation. These reactions, along with splicing, are tightly coupled to transcription and take place as the RNA is being transcribed. The mature mRNA then moves to the cytoplasm. Furthermore, RNA splicing enables eucaryotes to increase the already enormous coding potential of their genomes.

From RNA to protein

Translation is the ‘transfer of the information’ in RNA into proteins. Because there are only 4 different nucleotides in mRNA and 20 different types of amino acids in a protein, this translation cannot be accounted for by a direct one-to-one correspondence between a nucleotide in RNA and an amino acid in protein. The rules by which the nucleotide sequence of a gene, through the medium of mRNA, is translated into the amino acid sequence of a protein are known as the genetic code.

Translation of the nucleotide sequence of mRNA into a protein takes place in the cytoplasm on large ribonucleoprotein assemblies called ribosomes. These attach to the mRNA and move stepwise along the mRNA chain, translating the message into protein. The nucleotide sequence in mRNA is read in sets of three nucleotides (codons), each codon corresponding to one amino acid. The correspondence between amino acids and codons is specified by the genetic code. The possible combinations of the 4 different nucleotides in RNA give 64 (4x4x4) different codons in the genetic code. Most amino acids are specified by more than one codon.

Transfer RNAs

The codons in an mRNA do not directly recognize the amino acids they specify. Rather, the translation of mRNA into proteins depends on adaptor molecules that can recognize and bind both to the codon and to the amino acid. These adaptors consist of a set of small RNA molecules known as transfer RNAs (tRNAs).

tRNA acts as an adaptor molecule in protein synthesis and enzymes called aminoacyl-tRNA synthetases link amino acids to their appropriate tRNAs. Each tRNA contains a sequence of three nucleotides, the anticodon, which matches a codon in mRNA by complementary base-pairing between codon and anticodon.

Recognition and attachment of the correct amino acid depends on enzymes called aminoacyl-tRNA synthetases, which covalently couple each amino acid to its appropriate set of tRNA molecules. There is a different synthetase enzyme for each amino acid. The synthetase-catalyzed reaction that attaches the amino acid to the 3’ end of the tRNA is one of the many cellular reactions coupled to the energy-releasing hydrolysis of ATP. And it produces a high-energy bond between the charged tRNA and the amino acid. The energy of this bond is used at a later stage in protein synthesis to covalently link the amino acid to the growing polypeptide chain.

Decoding of the RNA message

Each ribosome has a binding site for mRNA and three binding sites for tRNA. The tRNA sites are designated the A-, P-, and E-sites. Protein synthesis begins when a ribosome assembles at an initiation condon (AUG) in mRNA, a process that is regulated by proteins called translation initiation factors. Of all the charged tRNAs in the cell, only the charged initiator tRNA is capable of tightly binding to the P-site of the small ribosome subunit. The completed protein chain is released from the ribosome when a stop codon (UUA, UAG, of UGA) is reached. Proteins known as release factors bind to any stop codon that reaches the A-site on the ribosome, and this binding alters the activity of the peptidyl transferase in the ribosome, finally causing the release of the protein into the cytoplasm.
The stepwise linking of amino acids into a polypeptide chain is catalyzes by an rRNA molecule in the large ribosomal subunit. Thus the ribosome is an example of a ribozyme, an RNA molecule that can catalyze a chemical reaction.

Protein breakdown

The degradation of proteins in the cell is carefully controlled. Cells possess specializes pathways to enzymatically break proteins down into their constituent amino acids – a process called proteolysis. The enzymes that degrade proteins are known collectively as proteases. Proteases act by hydrolyzing the peptide bonds between amino acids. One function of the proteolytic pathways is to rapidly degrade those proteins whose lifetimes must be short. Another is to recognize and eliminate proteins that are damaged or misfolded. Eliminating improperly folded proteins is critical for an organism, because neurodegenerative disorders such as Huntington’s and Alzheimer’s are caused by the aggregation of misfolded proteins. Some proteins are degraded in the cytosol by large protein complexes called proteasomes. Proteasomes act primarily on proteins that have been marked for destruction by the covalent attachment of a small protein called ubiquitin.

RNA and the origins of life

From our knowledge of present-day organisms and their molecules, it seem likely that living systems began with the evolution of RNA molecules that could catalyze their own replication. We have seen that a protein is able to catalyze a biochemical reaction because is has a special surface on which a given substrate can react. In the same way, RNA molecules, with their unique folded three-dimensional shapes, can serve as enzymes. Although the fact that they are constructed of only four different subunits limits their catalytic efficiency and the range of chemical reactions they can catalyze compared with proteins. So, most catalytic functions in present-day cells have been taken over by proteins.

It has been proposed that, as cells evolved, the DNA double helix replaced RNA as a more stable molecule for storing increased amounts of genetic information, and proteins replaced RNAs as major catalytic and structural components.

The flow of information in present-day living cells is DNA ® RNA ® protein, with RNA serving primarily as a go-between. Some important reactions, however, are still catalyzed by RNA; these are thought to provide a glimpse into the ancient, RNA-based world.

8. Control of gene expression

An overview of gene expression

A typical eukaryotic cell expresses only a fraction of it genes, and the distinct types of cells in multicellular organisms arise because different sets of genes are expressed as a cell differentiates. So, the different cell types of a multicellular organism contain the same DNA and, therefore all the genetic instructions necessary to direct the formation of a complete organism. Hence, the cells of an organism differ not because they contain different genes, but because they express them differently.

Although all of the steps involved in expressing a gene can in principle be regulated, for most genes the initiation of transcription is the most important point of control. Thus a cell can control the proteins it makes by:

  • Controlling when and how often a given gene is transcribed
  • Controlling how the primary RNA transcript is spliced or otherwise processed
  • Selecting which mRNAs are translated by ribosomes
  • Selectively activating or inactivating proteins after they have been made

How transcription switches work

We saw earlier that the promoter region of a gene attracts the enzyme RNA polymerase and correctly orients the enzyme to begin its task of making an RNA copy of the gene. The promoters of both bacterial and eukaryotic genes include an initiation site, where transcription begins. In addition to the promoter, nearly all genes have regulatory DNA sequences that are used to switch the gene on or off. Regulatory DNA sequences do not work by themselves; to have any effect these sequences must be recognized by proteins called gene regulatory proteins that bind to the DNA. It is the combination of a DNA sequence and its associated protein molecules that acts as the switch to control transcription.

Although each gene regulatory protein has unique features, most bind to DNA using one of a small number of protein structure motifs. The precise amino acid sequence that is folded into the DNA-binding motif determines the particular DNA sequence that is recognized. The DNA-binding motifs are the homeodomain that consists of three linked α helices; the zinc finger that is built from an α helix and a β sheet held together by a molecule of zinc; and the leucine zipper that is formed by two α helices.

Repressors turn genes off, activators turn them on

RNA polymerase binds to the DNA and initiates transcription at a site called promoter. However, within the promoter is a short DNA sequence that is recognized by a gene regulatory protein. When the regulatory protein binds to this nucleotide sequence, termed the operator, it blocks access of RNA polymerase to the promoter. This prevents transcription of the operon and production of the tryptophan-producing enzymes; it switches genes off. The gene regulatory protein is known as the tryptophan repressor, and it is regulated in a clever way: the repressor can bind only to DNA if it has also bound several molecules of the amino acid tryptophan. Therefore, the tryptophan repressor in an allosteric protein: the binding of tryptophan causes subtle change in its three-dimensional structure so that it can now bind to the operator DNA.

Other bacterial gene regulatory  proteins operate in the opposite manner by switching genes on, or activating them. These activator proteins bind to a regulatory sequence on the DNA and then interacts with the RNA polymerase to help it initiate transcription. Without the activator, the promoter fails to initiate transcription efficiently.

Differences in regulation of transcription

Regulation of transcription in eucaryotes differs in four important ways from that in bacteria:

  1. While bacteria contain a single type of RNA polymerase, eukaryotic cells have three: RNA polymerase I / II / III. These polymerases are responsible for transcribing different types of genes. RNA polymerases III and I transcribe the genes encoding tRNA, rRNA and small RNAs. RNA polymerase II transcribes the vast majority of eukaryotic genes.

  2. Bacterial RNA polymerase is able to initiate transcription without the help of additional proteins. However, eucaryotic RNA polymerases require the assembly of proteins called general transcription factors. The general are thought to position the RNA polymerase correctly at the promoter, to aid in pulling apart the two strands of DNA to allow transcription to begin, and to allow RNA polymerase to leave the promoter as transcription begins.

  3. In bacteria, regulatory proteins usually bind to regulatory DNA sequences close to where RNA polymerase binds and then either activate or repress transcription of the gene. In eucaryotes, these regulatory DNA sequences are often separated from the promoter by many thousands of nucleotide pairs. So, in eucaryotes gene activation occurs at a distance.

  4. Initiation of transcription in eukaryotic cells must also take into account the packing of DNA into nucleosomes and more compact forms of chromatin structure.

Eucaryotic gene regulatory proteins act in two fundamental ways:

  1. They can directly affect the assembly process of RNA polymerase and the general transcription factors at the promoter
  2. They can locally modify the chromatin structure of promoter regions

The molecular mechanisms that create specialized cell types

In eucaryotes, the expression of a gene is generally controlled by a combination of gene regulatory proteins. The regulatory proteins do not each function individually, but they work together as a ‘committee’ to control gene expression.

In multicellular plants and animals, the production of different gene regulatory proteins in different cell types ensures the expression of only those genes appropriate to the particular type of cell. Although all cells must be able to switch genes on and off, multicellular organisms require special gene switching mechanisms for generating and maintaining their different types of cells. Once a cell in a multicellular organism has become differentiated into a particular cell type, it will generally remain differentiated, and if it is able to divide, all it progeny cells will be of that same cell type. This means that the changes in gene expression that give rise to a differentiated cell must be remembered and passed on to its daughter cells through all subsequent cell divisions. Cells have several ways of ensuring that daughter cells remember what kind of cells they are supposed to be:

  1. Trough a positive feedback loop, where a key gene regulatory protein activates transcription of its own gene in addition to that of other cell-type-specific genes

  2. Trough the propagation of a condensed chromatin structure from parent to daughter cell even though DNA replication intervenes

A single gene regulatory protein, if expressed in the appropriate precursor cell, can trigger the formation of a specialized cell type or even an entire organ.

9. How genes and genomes evolve

The vast diversity of life we see around us has arisen through changes in DNA sequences that have accumulated since the first cells on earth arose some 3.5 billion years ago.

Generating genetic variation

Genetic changes that offer an organism a selective advantage or those that are selectively neutral are the most likely to be perpetuated. Changes that seriously compromise an organism’s fitness are eliminated through natural selection.

Genetic variation (the raw material for evolutionary change) occurs by a variety of mechanisms and each of these forms of genetic variation has played an important part in the evolution of modern organisms:

  1. Mutations within a gene: an existing gene can be modified by mutations that change a single nucleotide or that delete or duplicate on or more nucleotides in its DNA sequence. These so called point mutations typically arise from small errors in DNA replication or repair.

  2. Gene duplication: an existing gene, a larger segment of DNA, or even a whole genome can be duplicated, creating a set of closely related genes within a single cell. Gene duplication is one of the most important sources of genetic diversity. Once a gene has been duplicated, one of the two gene copies is free to mutate and become specialized to perform a different function. Repeated rounds of this process of duplication and divergence can allow one gene to give rise to a whole family of genes within a single genome.

  3. Gene deletion: individual genes, or whole blocks of genes can be lost through chromosome breakage and failures of repair.  

  4. Exon shuffling: the evolution of new proteins is thought to have been greatly facilitated by the organization of eukaryotic genes as relatively short exons separated by long, noncoding introns. The presence of introns greatly increases the probability that a chance recombination event generate a functional hybrid gene by joining together two initially separate exons coding for quite different protein domains; this process called exon shuffling.

  5. Horizontal (intracellular) gene transfer: a piece of DNA can be transferred from the genome of one cell to that of another, even to that of another species. This process is rare among eucaryotes, but common among procaryotes.

Reconstructing life’s family tree

By comparing the nucleotide or amino acid sequences of contemporary organisms, we are beginning to able to reconstruct how genomes have evolved in the billions of years that elapsed since the appearance of the first cells.

Examining the human genome

The human genome contains 3.2 x 10^9 nucleotide pairs divided among 22 autosomes and 2 sex chromosomes. The human genome sequence refers to the complete nucleotide sequence of the DNA contained in these 24 chromosomes.
Individual human differ from one another by an average of 1 nucleotide pair in every 1000; this variation underlies our individuality and provides the basis for identifying individuals by DNA analysis.

The first characteristic feature of the human genome is how little of it (only a few percent) codes for proteins or for structural or catalytic RNAs. Much of the remaining DNA is made up of transposable elements that have gradually colonized our genome over evolutionary time. A second feature of the human genome is the very large average size of 27.000 nucleotide pairs. Only about 1300 nucleotide pairs are required to encode a protein of average size, and most of the remaining DNA is a gene consists of long stretches of noncoding DNA that interrupt the relatively short protein-coding exons. Finally, the nucleotide sequence of the human genome has revealed that the critical information it carries seems to be in an alarming state of disarray.

A major obstacle in interpreting the nucleotide sequences of human chromosomes is the fact that much of the sequence appears unimportant. Comparative genome analyses provide a valuable tool for indentifying genes as well as functionally important regulatory sequences. Knowing the location, and possibly the function, of a gene in one genome consequently makes it easier to identify and predict the function of the corresponding gene in the other genome. Such comparisons have revealed that mice and humans share most of the same genes, and that large blocks of the mouse and human genomes contain these genes in the same order.

Even with the human genome in hand, many questions will continue to challenge cell biologists throughout the next century. Perhaps most puzzling is to determine how organisms built from essentially the same set of proteins can be so different. This will require understanding how genes are regulated and alternatively spliced to define each organism’s developmental programs.

10. Manipulating genes and cells

Isolating cells and growing them in culture

Several approaches can be used to separate a particular type of cell from the cells that surround it in the body. If the cells are part of a compact tissue, they must first be dissociated from each other. This is often accomplished using proteolytic enzymes and other agent that disrupt the adhesive bonds between cells. Next, the different types of cells in the tissue must be isolated from each other. A fluorescence-activated cell sorter allows the isolation of specific types of cells. The isolated cells can be used for biochemical analysis or for establishing cell cultures.

Many animal and plant cells survive and proliferate in culture provided they have suitable medium containing nutrients and the necessary growth factor proteins. Experiments performed using cultured cells are said to be carried out in vitro (‘in glass’) to contrast them with experiments on intact organisms, which are said to be carried out in vivo (‘in the living’).

Most vertebrate cells cease to proliferate after a finite number of cell divisions. Like most human somatic cells, these cells do not express the enzyme telomerase, whose renew the ends of chromosomes at each cell division. As a result the chromosomes of human somatic cells progressively shrink at each cell division, and cell division stops when critical information is lost from the ends of chromosomes. This feature ensures that somatic cells do not divide indiscriminately and develop into cancerous cells. Cells that can divide indefinitely as the result of a genetic change are said to be immortalized and can be propagated in culture as a cell line. Immortalized cell lines can be regenerated by providing the cells with the gene that encodes the catalytic subunit of telomerase. The cell lines provide a convenient source of homogeneous cells.

Among the most promising cell lines to be developed are the human embryonic stem (ES) cell lines. The critical importance of these cell lines is the fact that the cells are undifferentiated; and given the appropriate treatment, they can give rise to any tissue in the body.

How DNA molecules are analyzed

Recombinant DNA technology has revolutionized the study of the cell, making it possible for researchers to pick any gene at will from the thousands of genes in a cell, and after an amplification step, to determine the exact molecular structure of the gene. A crucial element in this technology is the ability to cut a large DNA molecule into a specific and reproducible set of DNA fragments using restriction nucleases, each of which cuts the DNA double helix only at a particular nucleotide sequence. In general, a nuclease catalyzes the hydrolysis of a phosphodiester bond in a nuclei acid. The restriction nucleases used in DNA technology come mainly from bacteria.

After a large DNA molecule is cleaved into smaller pieces using restriction nuclease, it is often desirable to separate the DNA fragments from one another. This is usually accomplished using gel electrophoresis, which separates the fragments on the basis of their length. When a voltage is applied across the gel slab, the DNA fragments migrate toward the positive electrode (DNA is negatively charged); the larger fragments migrate more slowly and after several hours the DNA fragments become spread out across the gel according to size. Isolating a particular DNA fragment is simple: a small section of the gel can now be cut out. Techniques are now available for rapidly determining the nucleotide sequence of any isolated DNA fragment.

In 1970 researchers developed methods that allows the nucleotide sequence of any purified DNA fragment to be determined simply and quickly. These techniques have made it possible to determine the complete nucleotide sequences of the genomes of dozens of single-celled organisms (including bacteria, archaea, and yeasts), as well as several more complex organisms.

Several schemes for sequencing DNA have been developed, but the enzymatic or dideoxy method is the most commonly used technique. The process of interpreting a genome sequence by locating its genes and assigning functions to them is called annotation. Identifying genes is easiest when the DNA sequence is from a simple genome that lacks introns and other nonessential DNA.

Nucleic acid hybridization

We have seen that the two strands of a double helix DNA are held together by weak hydrogen bonds that can be broken by heating the DNA to around 90°C or by subjecting it to extremes of pH. These treatments release the two strands from each other but do not break the covalent bonds between the nucleotides. If this process is slowly reversed (slowly lowering the temperature to normal body temperature of by bringing the pH back to neutral), the complementary strands will readily re-form double helices. This process is called hybridization or renaturation, and its results from a restoration of the complementary hydrogen bonds.

Nucleic acid hybridization can detect any given DNA or RNA sequence in a mixture of nucleic acid fragments. This technique relies on the fact that a single strand of DNA or RNA will form a double helix only with another nucleic acid strand of the complementary nucleotide sequence. Single-stranded DNAs of known sequences and labeled with fluorescent dyes or radioisotopes are used as probes in hybridization reactions. Nucleic acid hybridization can be used to detect the precise location of genes in chromosomes, or RNAs in cells and tissues.

DNA hybridization facilitates the diagnosis of genetic diseases

To search for a nucleotide sequence by hybridization, a piece of nucleic acid is needed to search with. This DNA probe is a single-stranded DNA molecule that is used in hybridization reactions to detect nucleic acid molecules containing a complementary sequence. In the past, scientists were limited to using probed that could be obtained from natural sources. Today, short DNA strands of any sequence can be made by chemical (nonenzymatic) synthesis in the laboratory. Of the many uses of DNA probes, one of the most important is in identifying carriers of genetic diseases. More than 3000 different human genetic diseases are caused by mutations in single genes, including sickle-cell anemia. For some of these diseases, it is now possible to identify early in a pregnancy fetuses that carry two copies of a defective gene; this information may be the factor in decisions relating to possible termination of the pregnancy. A common laboratory procedure used to visualize the hybridization is called Soutern blotting.

The same techniques can also be used to ascertain an individual’s susceptibility to future diseases. For example, they can identify individuals who have inherited abnormal copies of a DNA mismatch repair gene.

Hybridization and microarrays

Another important use of nucleic acid hybridization is to determine, for a population of cells, exactly which genes are being transcribed into mRNA and which genes are transcriptionally silent. DNA microarrays have revolutioned they way of analyzing genes by allowing the RNA products of thousands of genes to be monitored at the same time. By examining the expression of so many genes simultaneously, it is possible to identify and study the complex gene expression patterns that underlie cellular physiology, like responses to hormones.

DNA cloning

DNA cloning techniques enable a DNA sequence to be selected from millions of other sequences and produced in unlimited amounts in pure form. DNA ligase reseals the nicks in the DNA backbone that arise during DNA replication and DNA repair. So, DNA fragments can be joined together in vitro using DNA ligase to form recombinant DNA molecules not found in nature.

The first step in a typical cloning procedure is to insert the DNA fragments to be cloned into a DNA molecule capable of replication, such as a plasmid or a viral genome. This recombinant DNA molecule is then introduced into a rapidly dividing host cell, usually a bacterium, so that the DNA is replicated at each cell division. The bacteria are then lysed, and the plasmid DNA is purified from the rest of the cell contents. The purified preparation of plasmid DNA will contain millions of copies of the original DNA fragment.

Human genes are isolated by DNA cloning

A collection of cloned fragments of chromosomal DNA representing the complete genome of an organism is known as a genomic library. The library is often maintained as clones of bacteria, each clone carrying a different DNA fragment.  Complementary DNA (cDNA) libraries contain cloned DNA copies of the total mRNA of a particular cell type or tissue. cDNA is synthesized from mRNA and unlike genomic DNA clones, cloned cDNAs contain only protein-coding sequences; they lack introns, gene regulatory sequences and promoters. They are thus most suitable for use when the cloned gene is to be expressed to make a protein.

The polymerase chain reaction

Cloning via DNA libraries was once the only route the gene isolation. However, a method known as the polymerase chain reaction (PCR) provides a quicker alternative for many cloning applications, particularly for those organisms whose complete genome sequence is known. PCR is based on the use of DNA polymerase to copy a DNA template in repeated rounds of replication. But because the oligonucleotide primers have to be chemically synthesized, PCR can be used only to clone DNA whose beginning and end sequences are known. Guided by these primers, DNA polymerase is then used to make many copies of the sequences required.
There are several useful applications of PCR:

  1. PCR is now the method of choice for cloning relatively short DNA fragments from a cell.

  2. PCR is able to detect infections by pathogens at very early stages. Short sequences complementary to the pathogen’s genome are used as primers, following many cycles of amplification, the presence or absence of even a few copies of an invading genome in a sample of blood can be ascertained. In this way PCR can be used to detect the presence of a viral genome in a sample of blood.

  3. PCR is used in forensic science. Its extreme sensitivity makes it possible to work with a very small sample and still obtain a DNA fingerprint of the person from whom it came. The genome of each human differs in DNA sequence from the genome of every other human; the DNA amplified by PCR using a particular primer pair is therefore quite likely to differ in sequence from one individual to another.

DNA engineering

Genetic engineering has far-reaching consequences. Bacteria, yeasts, and mammalian cells can be engineered to synthesize a particular protein from any organism in large quantities, thus making it possible to study proteins that are otherwise rare or difficult to isolate.

There are more than 10.000 human genes whose functions are unknown. Clues to a protein’s function can be obtained by examining when and where its gene is expressed in the cell or in the organism. Determining the pattern and timing of a gene’s expression can be accomplished by joining the regulatory region of the gene under study to a reporter gene, one whose activity can be easily monitored. One of the most popular reporter proteins used today is green fluorescent protein (GFP), whose allows the tracking of its movements inside the cell. In the case of GFP, the protein can be monitored over time in living organisms.

Animals can be genetically altered

The ultimate test of the function of a mutated gene is to insert it into the genome of an organism and see what effect it has. Organisms into which a new gene has been introduced, or those whose genomes have been altered in other ways using recombinant DNA techniques, are known as transgenic organisms. Several types of gene alterations can be made in genetically engineered organisms:

  1. Gene replacement: the normal gene is completely replaced by a mutant copy of the gene. This will provide information on the activity of the mutant gene, without interference from the normal gene, and thus the effect of small and subtle mutations can be determined

  2. Gene knockout: the normal gene is completely inactivated. This is used to obtain information on the possible function of the normal gene in the whole animal

  3. Gene addition: a mutant gene is added to the genome. Even this alteration can still provide useful information when the introduced mutant gene overrides the function of the normal gene

There is another way discovered to inactivate genes, known as RNA interference (RNAi). This technique relies on introducing intro a cell or organism a double stranded RNA molecule whose nucleotide sequence matches that of the gene to be inactivated. The RNA molecule hybridizes with the mRNA produced by the target gene en direct its degradation. Small fragments of this degraded RNA are subsequently used by the cell to produce more double-stranded RNA which directs the continued elimination of the target mRNA. Because these short RNA fragments can be passed on to progency cells, RNAi can cause heritable changes in gene expression.

In concluding, cloned genes can be permanently inserted into the genome of a cell or an organism by the techniques of genetic engineering. Cloned DNA can be altered in vitro to create mutant genes that can then be reinserted into a cell or an organism to study gene function.

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Summary: Essential Cell Biology (Alberts et al) - Second part

Summary: Essential Cell Biology (Alberts et al) - Second part

This summary is based on the 3rd edition of Essential Cell Biology from Alberts et al. The first 10 chapters are open access and can be found here: First part of the summary

11. Membrane structure

Cell membranes enable a cell to create barriers that confine particular molecules to specific compartments. The simplest bacteria have only a single membrane, the plasma membrane. Eucaryotic cells, however, contain in addition a profusion of internal membranes that enclose intracellular compartments. All cell membranes are composed of lipids and proteins and share a common general structure. The lipid component consists of many millions of lipid molecules forming a lipid bilayer. This lipid bilayer gives the membrane its basic structure and serves as a permeability barrier.

The lipid bilayer

The lipids in cell membranes combine two very different properties in a single molecule: each lipid has a hydrophilic (‘water-loving’) has and one or two hydrophobic (‘water-hating’) hydrocarbon tails. There are three major classes of membrane lipid molecules:

  1. Phospholipids
  2. Sterols
  3. Glycolipids

The most abundant lipids in cell membranes are phospholipids, and the most common type of phosphoslipid in most cell membranes is phosphatidylcholine. Molecules with both hydrophilic and hydrophobic properties are termed amphipathic. This chemical property plays a crucial part in driving these lipid molecules to assemble into bilayers. They assemble spontaneously into bilayers when placed in water, forming closed compartments that reseals of torn.

Amphipathic molecules re subject to two conflicting forces: the hydrophilic head is attracted to water, while the hydrophobic tail shuns water and seeks to aggregate with other hydrophobic molecules. This conflict is resolved by the formation of a lipid bilayer, because the hydrophilic heads face the water at each of the two surfaces of the sheet of molecules and the hydrophobic tails are all shielded from the water and lie next to one another in the interior of this ‘sandwich’. Finally, the phospholipid bilayers spontaneously close in on themselves to form sealed compartments.

The fluidity of a lipid bilayer

The lipid bilayer is fluid, and individual lipid molecules are able to diffuse within their own monolayer; they do not, however, spontaneously flip from one monolayer to the other. The two layers of the lipid bilayer have different lipid compositions, reflecting the different functions of the two faces of a cell membrane.

The fluidity of a cell membrane (the ease with which its lipid molecules move within the plane of the bilayer) is important for membrane function and has to be maintained within certain limits. The fluidity of a bilayer depends on its phospholipid composition and on the nature of the hydrocarbon tails. The closer and more regular the packing of the tails, the more viscous and less fluid the bilayer will be. The two properties length and degree of unsaturation determine how tightly packed the bilayer is.

  • A shorter chain length reduces the tendency of the hydrocarbon tails to interact with one another and therefore increases the fluidity of the bilayer.

  • Each double bond in an unsaturated tail (saturated tails have no double bonds) creates a small kink in the hydrocarbon tail that makes it more difficult for the tails to pack against one another. For this reason, lipid bilayers that contain a large proportion of unsaturated hydrocarbon tails are more fluid than those with lower proportions.

In animals, membrane fluidity is modulated by the inclusion of the sterol cholesterol. Cholesterol molecules fill the spaces between neighboring phospholipid molecules left by the kinks in the unsaturated hydrocarbon tails. In this way cholesterol tends to stiffen the bilayer, making it more rigid and less permeable.  

Membrane fluidity is important for many reasons:

  1. It enables membrane proteins to diffuse rapidly in the plane of the bilayer and to interact with one another

  2. It permits membrane lipids and proteins to diffuse from sites where they are inserted into the bilayer after their synthesis to other regions of the cell

  3. It allows membranes to fuse with one another and mix their molecules

  4. It ensures that membrane molecules are distributed evenly between daughter cells when a cell divides

Cells adjust their membrane fluidity by modifying the lipid composition of their membranes. Flippases play a role in synthesizing the lipid bilayer.

Membrane proteins

Although the lipid bilayer provides the basic structure of all cell membranes and serves as a permeability barrier to the molecules on either side of it, most membrane functions are carried out by membrane proteins. Plasma membrane proteins have a variety of functions: first they take care of transportation of nutrients, metabolites, and ions across the lipid bilayer. Some anchor the membrane to macromolecules on either side. Others function as receptors that detect chemical signals in the cell’s environment and relay them to the cell’s interior; and still others work as enzymes to catalyze specific reactions.

Proteins can be associated with the lipid bilayer of a cell membrane in several ways:

  1. Transmembrane: transmembrane proteins extend across the lipid bilayer, usually as one or more a helices but sometimes as a b sheet curved into the form of a barrel

  2. Membrane-associated: some membrane proteins are anchored to the cytosolic surface by an amphipathic a helix

  3. Lipid-linked: membrane proteins that are attached to either side of the bilayer solely by a covalent attachment to a lipid molecule

  4. Protein-attached: many proteins are attached to the membrane only by relatively weak, noncovalent interactions with other membrane proteins

Proteins that are directly attached to membranes can be removed only by disrupting the lipid bilayer detergents. Such proteins are known as integral membrane proteins. The remaining membrane proteins are know as peripheral membrane proteins; they can be released from the membrane by extraction procedures that interface with protein-protein interactions but leave the lipid bilayer intact.

Before an individual protein can be studied in detail, it must be separated from all the other cellular proteins. For most membrane proteins, the first step in this separation process involves solubilizing the membrane with agents that destroy the lipid bilayer by disrupting hydrophobic associations. The most widely used disruptive agents are detergents. Sodium dodecyl sulfate (SDS) and Trition X-100 are two commonly used detergents. The detergent disrupts the lipid bilayer and brings the protein into solution as protein-detergent complexes.

The cell surface

A cell membrane by itself is enormously thin and fragile. Most cell membranes are therefore strengthened and supported by a framework of proteins, attached to the membrane via transmembrane proteins. The shape of the cell and the mechanical properties of the plasma membrane are determined by a meshwork of fibrous proteins, called the cell cortex, which is attached to the cytosolic surface of the membrane.

Many of the proteins and some of the lipids exposed on the surface of cells have attached chains of sugars which help protect and lubricate the cell surface and are involved in cell-cell recognition. Some proteins, called lectins, are specialized to recognize particular oligosaccharide side chains and bind to them.

Although many membrane proteins can diffuse rapidly in the plane of the membrane, cells have ways of confining proteins to specific membrane domains and of immobilizing particular proteins by attaching them to intracellular or extracellular macromolecules.

12. Membrane transport

The lipid bilayer of cell membranes is permeable to small nonpolar molecules such as oxygen and carbon dioxide and to very small polar molecules such as water. It is highly impermeable to most large, water-soluble molecules and all ions. Transfer of nutrients, metabolites, and ions across the plasma membrane and internal cell membranes is carried out by membrane transport proteins. Cell membranes contain a variety of transport proteins, each of which is responsible for transferring a particular type of solute across the membrane. There are two classes of membrane transport proteins:

  1. Carrier proteins
  2. Channel proteins; most let through inorganic ions and are therefore called ion channels

The basic difference between carrier proteins and channel proteins is the way they discriminate between solutes. A channel protein discriminates mainly on the basis of size and electric charge; if the channel is open, molecules small enough and carrying the appropriate charge can slip through. A carrier protein, on the other hand, allows passage only to solute molecules that fit into a binding site on the protein; it then transfers these molecules across the membrane one at a time by changing its own conformation.  

Principles of membrane transport

Living cells maintain an internal ion composition that is very different from the ion composition in the fluid around them. Na+ is the most plentiful positively charged ion (cation) outside the cell, while K+ is the most plentiful of all the solutes in a cell’s environment. The high concentration of Na+ outside the cell is balanced by extracellular Cl-. The high concentration of K+ inside is balanced by a variety of negatively charged intracellular ions (anions). This differential distribution of ions inside and outside the cell is controlled in part by the activity of membrane transport proteins, and in part by the permeability characteristics of the lipid bilayer itself.

The electrochemical gradient represents the net driving force on an ion due to its concentration gradient, and a charged solute (an ion) moves spontaneously down its electrochemical gradient. Such movements are called passive transport (or facilitated diffusion), because they need no other driving forces. All channel proteins and many carrier proteins can act as a conduit for such passive transport. In active transport an uncharged solute or an ion is transported against its concentration or electrochemical gradient in an energy-requiring process. This is carried out only by special types of carrier proteins that can harness some energy source to the transport process.

Carrier proteins and their function

Although the detailed molecular mechanisms that underlie transport are known for only a few carrier proteins, the general principles are well understood. Solutes can cross the membrane by passive and active transport, and carrier proteins are capable of facilitating both types of movement. Carrier proteins bind specific solutes (inorganic ions, small organic molecules, or both) and transfer them across the lipid bilayer by undergoing conformational changes that expose the solute-binding site first on one side of the membrane and then on the other.

Cells carry out active transport in three main ways:

  1. Coupled transport; they couple the uphill transport of one solute across the membrane to the downhill transport of another
  2. ATP-driven pumps; they couple uphill transport to the hydrolysis of ATP
  3. Light-driven pumps; they are found mainly in bacterial cells and couple uphill transport to an input of energy from light

The Na+-K+ pump in the plasma membrane of animal cells is an ATPase that actively transports Na+ out of the cell and K+ in, maintaining the steep Na+ gradient across the plasma membrane that is used to drive other active transport processes and to convey electrical signals. The downhill movement of the first soluble down its gradient provides the energy to drive the uphill transport of the second. The carrier proteins that do this are called coupled transporters. If the transporters moves both solutes in the same direction across the membrane, it is called a symport. If it moves them in opposite directions, it is called an antiport. A carrier protein that ferries only one type of solute across the membrane (and is therefore not a coupled transporter) is called a uniport.

In animal cells an especially important role is played by symports that use they inward flow of Na+ down its steep electrochemical gradient to drive the import of other solutes into the cell. The epithelial cells that line the gut, for example, transfer glucose from the gut across the gut epithelium. In this way animals use the Na+ gradient to take up nutrients.

Furthermore, the Na+-K+ pump helps to maintain the osmotic balance of animal cells. Movement of water from a region of low solute concentration (high water concentration) to a region of high solute concentration (low water concentration) is called osmosis. The driving forces for the water movement is equivalent to a difference in water pressure and is called the osmotic pressure. In the absence of any counter-acting pressure, the osmotic movement of water into a cell will cause it to swell. Such effects are a severe problem for animal cells, which have no rigid external wall to prevent them from swelling. In animal cells the osmotic balance is regulated by the Na-K+- pump, which pumps out the Na+ that leaks in. At the same time, by helping to maintain a membrane potential, the Na+-K+-pump also tends to prevent the entry of Cl-, which is negatively charged.

Other cells cope with their osmotic problems in different ways. Plant cells are prevented from swelling and bursting by their tough cell wall and so can tolerate a large osmotic difference across their plasma membrane. The protozoan avoids swelling by periodically ejecting the water that moves into the cell.

Ion channels and the membrane potential

Channel proteins form aqueous pores across the lipid bilayer through which solutes can diffuse. Whereas transport by carrier proteins can be active or passive, transport by channel proteins is always passive. Most channel proteins are selective ion channels that allow inorganic ions of appropriate size and charge to cross the membrane down their electrochemical gradients. Transport through ion channels is al least 1000 times faster than transport through any known carrier protein.

There are more than a hundred types of ion channels and they mainly differ from one another with respect to their ion selectivity (the type of ions they allow to pass) and gating (the conditions that influence their opening and closing). For a voltage-gated channel, the probability of being open is controlled by the membrane potential. For a ligand-gated channel, it is controlled by the binding of some molecules (the ligand) to the channel protein. For a stress-activated channel, opening is controlled by a mechanical force applied to the channel. Even when opened by their specific stimulus, ion channels do not remain continuously open: they flicker randomly between open and closed conformations. An activating stimulus increases the proportion of time the channel spends in the open state.

All cells have an electrical potential difference, or membrane potential, across their plasma membrane. The membrane potential is determined by the unequal distribution of electric charge on the two sides of the plasma membrane and is altered when ions flow through open channels. In most animal cells, K+-selective leak channels hold the resting membrane potential at a negative value, close to the value where the driving force for movement of K+ across the membrane is almost zero.

A simple formula called the Nernst equation expresses the equilibrium quantitatively and makes it possible to calculate the theoretical resting membrane potential if the ratio of internal to external ion concentrations is known.

Ion channels and signaling in nerve cells

The fundamental task of a nerve cell (neuron) is to receive, conduct, and transmit signals. No matter what the meaning of the signal a neuron carries the form of the signal is always the same: it consists of changes in the electrical potential across the neuron’s plasma membrane. Neurons are often extremely elongated and the action potentials therefore have to travel long distances along an axon without weakening.

Every neuron consists of a cell body (containing the nucleus); a long axon, which conducts signals away form the cell body toward distant target cells; and dendrites, which extend from the cell body like antennae and provide an enlarged surface area to receive signals from the axons of other neurons. The axon divides at its far end into many branches, each of which ends in a nerve terminal; so that the neuron’s message can be passed simultaneously to many target cells.

Action potentials are usually mediated by voltage-gate Na+ channels that open in response to depolarization of the plasma membrane (a shift in the membrane potential to a less negatively value). Such a depolarization is caused by the action of signaling molecules, called neurotransmitters, released by other neurons. When the voltage-gate Na+ channels are open Na+ enters the cell, depolarizes the membrane further. The membrane potential swings past zero and reaches +40mV before it returns to its resting negatively value, as the action potential terminates. The membrane is helped to return to its resting value by inactivation of the Na+ channels, opening of voltage-gated K+ channels, and through the K+ leak channels.

When the action potential reaches the ends of the axon (the nerve terminals) the signal must be relayed to the target cells that the nerve terminals contact. The signal is transmitted at specialized junctions known as synapses. At most synapses the presynaptic and postsynaptic plasma membranes are separated from each other by a synaptic cleft, which the electrical signal cannot cross. For the message to be transmitted the electrical signal is converted into a chemical signal, known as a neurotransmitter. Neurotransmitters are stored in the nerve terminals, packaged in synaptic vesicles. When the action potential reaches the terminal, voltage-gated Ca2+ channels in nerve terminals couple electrical signals to transmitter release at synapses. Transmitter-gated ion channels convert these chemical signals back into electrical signals in the postsynaptic target cell.

The response produced by a neurotransmitter at a synapse can be either excitatory or inhibitory. Excitatory neurotransmitters, mainly acetylcholine and glutamate, open transmitter-gated channels that are permeable to Na+ and thereby depolarize the postsynaptic cell membrane toward the threshold potential for firing an action potential. Inhibitory neurotransmitters, mainly GABA and glycine, open transmitter-gated Cl- channels and thereby suppress firing by keeping the postsynaptic cell membrane polarized.

Transmitter-gated ion channels are major targets for psychoactive drugs.

13. How cells obtain energy from food

As mentioned earlier, cells require a constant supply of energy to generate and maintain the biological order that keeps them alive. Perhaps the most important fuel molecules are the sugars. Plants make their own sugars by photosynthesis, whereas animals obtain sugars by eating other organism. Nevertheless, the process whereby these sugars are oxidized to generate energy is very similar in both animals and plants.  Glucose and other food molecules are broken down by controlled stepwise oxidation to provide useful chemical energy in the form of the activated carriers ATP and NADH.

The breakdown of sugars and fats

The proteins, lipids and polysaccharides that make up most of the food we eat must be broken down into smaller molecules before our cells can use them; this happens in three stages:

Stage 1

In stage 1 the enzymatic breakdown of food molecules (digestion) occurs either outside the cells in our intestine or in a specialized organelle within cells called lysosome. In either case, digestive enzymes reduce the large polymeric molecules in food into their monomeric subunits (proteins into amino acids and polysaccharides into sugar). After digestion, the small organic molecules derived from the food enter the cytosol of a cell, where their gradual oxidation begins

Stage 2

The most important step of stage 2 is the degradation of glucose, a process called glycolysis. Glycolysis produces ATP without the involvement of molecular oxygen (O2 gas). It occurs in the cytosol of most cells, including many anaerobic microorganisms.

Glycolysis converts each molecule of glucose into two smaller molecules of pyruvate. During this formation two types of activated carrier molecules are produced: ATP and NADH. At the end of glycolysis, there is a net gain of two molecules ATP (4 produced, but 2 consumed during the process) and two molecules of NADH for each glucose molecule broken down. Next the pyruvate passes from the cytosol into mitochondria.

Stage 3

Stage 3 takes place in mitochondria. Here the pyruvate is converted into CO2 plus acetyl coenzyme A (CoA). The acetyl group enters a series of reactions called the citric acid cycle. The citric acid cycle accounts for about two-thirds of the total oxidation of carbon compounds in most cells, and its major products are CO2 and NADH. The CO2 is released as a waste product, while the high-energy electrons from NADH are passed to a membrane-bound electron-transport chain, eventually combining with O2 to produce H2O. Each turn of the citric acid cycle produces one molecule of GTP and one molecule of FADH2. The energy that is stored in the high-electrons of NADH and FADH2 will be used to drive a process that produces ATP and consumes molecular oxygen (O2). It is in these final steps that most of the energy released by oxidation is harnessed to produce most of the cell’s ATP. Because the energy for it ultimately derives from the oxidative breakdown of food molecules, the phosphorylation of ADP to form ATP in the mitochondrial inner membrane is known as oxidative phosphorylation.

As mentioned above, sugars are broken down by distinct sets of reactions: glycolysis (which occurs in the cytosol), the citric acid cycle (in the mitochondrial matrix), and oxidative phosphorylation (in the inner mitochondrial membrane). In total, the complete oxidation of a molecule of glucose to H20 and CO2 produces about 30 molecules of ATP (in contrast to glycolysis alone, which produces 2 molecules of ATP). Besides sugars, another major energy source in foods is fat. The fatty acids produced from fats are imported into mitochondria and converted to acetyl CoA molecules. These acetyl CoA molecules are then further oxidized through the citric acid cycle, producing NADH and FADH2, just like the acetyl CoA derived from pyruvate.

Anaerobic conditions

For most animal and plant cells, glycolysis is just a prelude to the final stage of the breakdown of food molecules. But for many anaerobic organisms, which do not use molecular oxygen and can grow and dived in its absence, glycolysis is the principle source of the cell’s ATP. In these anaerobic conditions, the pyruvate and the NADH electrons stay in the cytosol. The pyruvate is converted into products that are excreted from the cell, like for example lactate and ethanol. The NADH is converted back into NAD+; this is required to maintain the reactions of glycolysis.

Storing and utilizing food

Cells store food molecules in special reservoirs. Glucose subunits are stored as glycogen in animals and as starch in plants; both animals and plants store food as fats. The food reservoirs produced by plants are the major sources of food for animals, including humans.
Molecules ingested as food are used not only as sources of metabolic energy but also as raw material for biosynthesis. Thus many intermediates of glycolysis and the citric acid cycle are starting points for pathways that lead to the synthesis of proteins, nucleic acids, and the many other specialized molecules of the cell.

The thousands of different reactions carried out simultaneously by a cell are closely coordinated, enabling the cell to adapt and continue to function under a wide range of external conditions.

14. Energy generation in mitochondria and chloroplasts

The main energy currency in cells is ATP. In eukaryotic cells, small amounts of ATP are generated during glycolysis in the cytosol, but most ATP is produced by membrane-based processes in the mitochondria, using energy derived from oxidation of sugars and fatty acids. Similar processes also occur in the cell membrane of many bacteria. The mechanism for making ATP consists of two linked stages, both of which are carried out by protein complexes embedded in a membrane:

  1. Stage 1: electrons derived from the oxidation of food molecules are transferred along an electron-transport chain, which is embedded in the membrane. These electron transfers release energy that is used to pump protons (H+) across the membrane and thus generate an electron chemical proton gradient. This gradient is a form of stored energy that can be used when the ions flow back down their electrochemical gradient.

  2. Stage 2: H+ flows back down its electrochemical gradient through a protein complex called ATP synthase, which catalyzes the energy-requiring synthesis of ATP from ADP and inorganic phosphate (Pi).

The linkage of electron transport, proton pumping, and ATP synthesis is called chemiosmotic coupling. Chemiosmotic coupling first evolved in bacteria. Therefore, it is perhaps not surprising that aerobic eucaryotic cells appear to have adopted the bacterial chemiosmotic mechanisms by engulfing aerobic bacteria to form mitochondria and cyanobacteria to form chloroplasts.

Mitochondria and oxidative phosphorylation

Mitochondria are present in nearly all eucaryotic cells and contain their own DNA and RNA, and a complete transcription and translation system including ribosomes, which allows them to synthesize some of their own proteins. Defects in mitochondrial function can have serious repercussions for an organism. An inherited disorder called myoclonic epilepsy and ragged red fiber disease (MERRF) caused by a mutation in one of the mitochondrial transfer RNA genes, is characterized by a decrease in synthesis of the mitochondrial proteins required for electron transport and ATP production. As a result, patients with this disorder typically experience muscle weakness or hart problems (from the effect on cardiac muscle) and epilepsy or dementia (from the effects on nerve cells). Muscle and nervous tissue suffer most when mitochondria are defective because they need particularly large amounts of ATP to function optimally.

Composition of mitochondria

Mitochondria are enclosed by two concentric membranes. The outer and inner mitochondrial membranes create two mitochondrial compartments: a large internal space called the matrix and the intermembrane space. The matrix is a large internal space that contain a mixture of hundreds of enzymes, and it contains several identical copies of the mitochondrial DNA genome. The inner mitochondrial membrane is folded into numerous cristae, which greatly increase its total surface area. An electrochemical gradient of H+, which drives the ATP synthase, is established across this membrane. The inner membrane contains proteins with three types of function:

  1. Those that carry out the oxidation reactions of the electron-transport chain
  2. The ATP synthase that makes ATP in the matrix
  3. Transport proteins that allow the passage of metabolites into and out the matrix.

The outer membrane contains many molecules of a transport protein called porin, which forms wide aqueous channels through the lipids bilayer. As a result, the outer membrane is permeable to all molecules of 5000 dalton or less. Other proteins in this membrane include enzymes involved in mitochondrial lipid synthesis and enzymes that convert lipid substrates into forms that are subsequently metabolized in the matrix.

Citric acid cycle

Mitochondria can use both pyruvate and fatty acids as fuel. Pyruvate comes mainly from glucose and other sugars, and fatty acids come from fats. Pyruvate and fatty acids enter the mitochondrium and are converted into acetyl CoA. Then they are further metabolized by the citric acid cycle, which reduces NAD+ to NADH, and FAD to FADH2. In the process of oxidative phosphorylation, high-energy electrons from NADH and FADH2 are then passed along the electron-transport chain (the respiratory chain) in the inner membrane to oxygen. Much of the energy released by electron transfers along the respiratory chain is harnessed to pump H+ out of the matrix, thereby creating a transmembrane electrochemical proton (H+) gradient. The proton pumping is carried out by three large respiratory enzyme complexes embedded in the membrane. Each complex includes transmembrane proteins that hold the entire protein complex firmly in the inner mitochondrial membrane. The three respiratory enzyme complexes are:

  • NADH dehydrogenase complex
  • Cytochrome b-c1 complex
  • Cytochrome oxidase complex

The resulting electrochemical proton gradient across the inner mitochondrial membrane is used to drive the ATP synthesis in the process of oxidative phosphorylation. The device that makes this possible is a large membrane-bound enzyme called ATP synthase. This enzyme creates a hydrophilic pathway across the inner mitochondrial membrane that allows protons to flow down their electrochemical gradient. ATP synthase is a reversible coupling device. It can either harness the flow of protons down their electrochemical gradient to make ATP or use the energy of ATP hydrolysis to pump protons across a membrane, like H+ pumps. Whether the ATP synthase primarily makes or consumes ATP depends on the magnitude of the electrochemical proton gradient across the membrane in which it sits.
The synthesis of ATP is not the only process driven by the electrochemical proton gradient. The electrochemical gradient also drives the active transport of metabolites into and out the mitochondrion, or coupled transport processes.

Chloroplasts and photosynthesis

In plants, photosynthesis is carried out in a specialized intracellular organelle, the chloroplast. Chloroplasts perform photosynthesis during daylight hours and thereby produce ATP and NADPH, which in turn are used to convert CO2 into sugars inside the chloroplast. The sugars are then used to make ATP and as starting materials for many of the other organic molecules that the plant cell needs. Chloroplasts have a highly permeable outer membrane, a much less permeable inner membrane (in which membrane transport proteins are embedded) and a narrow intermembrane space in between. Together these membranes form the chloroplast envelope. The inner membrane surrounds a large space called the stroma, which is analogous to the mitochondrial matrix and contains many metabolic enzymes. Like the mitochondrium, the chloroplast evolved from an engulfed bacterium, and it still contains its own genome and genetic system. There is, however, an important difference between the organization of mitochondria and that of chloroplasts. Compared with mitochondria, chloroplasts are larger and have an extra compartment. A chloroplast contains, in addition to an inner and outer membrane, a thylakoid membrane enclosing a thylakoid space. The thylakoid membrane contains the light-capturing systems, the electron-transport chains and ATP synthase.

The many reactions that occur during photosynthesis in plants can be grouped into two broad categories:

  1. Photosynthetic electron-transfer reactions (also called the ‘light-reactions’): in this reactions is water oxidized and oxygen released

  2. Carbon-fixation reactions (also called the ‘dark reactions’): in this reactions, which begin in the chloroplast stroma and continue in the cytosol, carbon dioxide is assimilated (fixed) to produce sugars and a variety of other organic molecules

In photosynthesis high-energy electrons are generated when sunlight is absorbed by chlorophyll; this energy is captured by protein complexes known as photosystems, which are located in the thylakoid membranes of chloroplasts.

Electron-transport chains associated with photosystems transfer electrons from water to NADP+ to form NADPH, with the concomitant production of an electrochemical proton gradient across the thylakoid membrane. Molecular oxygen is generated as a by-product. As is mitochondria, the proton gradient across the thylakoid membrane is used by an ATP synthase embedded in the membrane to generate ATP. The ATP and the NADPH made by photosynthesis are used within the chloroplast to drive the carbon-fixation cycle in the chloroplast stroma, thereby producing carbohydrate from CO2. Carbohydrate is exported to the cell cytosol, where it is metabolized to provide organic carbon, ATP (mostly via mitochondria), and reducing power for the rest of the cell.

The origins of chloroplasts and mitochondria

Both mitochondria and chloroplasts are thought to have evolved from bacteria that were endocytosed by primitive eukaryotic cells. Each retains its own genome and divides by processes that resemble a bacterial cell division. Because mitochondria and chloroplasts have component proteins that are encoded by two separate genetic systems, their growth and proliferation is complicated.

Chemiosmotic coupling mechanisms are widespread and of ancient origin. Modern microorganisms that live in environments similar to those thought to have been present on the early Earth also use chemiosmotic coupling to produce ATP.

15. Intracellular compartments and transport

Membrane-enclosed organelles

Whereas a prokaryotic cell consists of a single compartment, the cytosol, enclosed by the plasma membrane, a eukaryotic cell is subdivides by internal membranes. These membranes create enclosed comportments in which sets of enzymes can operate without interference from reactions occurring in other compartments. They major membrane-enclosed organelles are:

  • Nucleus: this is generally the most prominent organelle in eukaryotic cells. It is surrounded by a double membrane, known as the nuclear envelope, and communicates with the cytosol via nuclear pores that perforate the envelope.

  • Endoplasmatic reticulum (ER): a system of interconnected sacs and tubes of membrane that often extends throughout most of the cell. The ER is the major site of new-membrane synthesis in the cell. Large areas of the system have ribosomes attached to the cytosolic surface and are called rough ER. The ribosomes are synthesizing proteins that are delivered into the ER lumen or ER membrane. The smooth ER is the site of steroid hormone synthesis and the site where a variety of organic molecules (including alcohol) are detoxified.

  • Golgi apparatus: receives proteins and lipids from the ER, modifies them, and then dispatches them to other destinations in the cell.

  • Lysosomes: small sacs of digestive enzymes that degrade worn-out organelles, as well as macromolecules and particles taken into the cell by endocytosis.

  • Endosomes: sort the ingested molecules and recycle some back to the plasma membrane.

  • Mitochondria: their main function is ATP synthesis by oxidative phosphorylation

  • Chloroplasts (in plant cells): by photosynthesis they produce ATP and carbon fixation

  • Peroxisomes: they contain enzymes that break down lipids and destroy toxic molecules.

Much can be learned about the composition and function of an organelle once it has been isolated from other cell structures; organelles are isolated by differential centrifugation. Many of the membrane-enclosed organelles, including the ER, Golgi apparatus, mitochondria, and chloroplasts, are held in their relative locations in the cell by attachment to the cytoskeleton, especially to microtubules.

To understand the relationship between the different compartments of a modern eukaryotic cell, it is useful to consider how they might have evolved. The precursors of the first eukaryotic cells are thought to have been simple microorganisms, which had a plasma membrane but no internal membranes. The plasma membrane in such cells would have provided all membrane-dependent functions, as does a plasma membrane in most bacteria. Membrane-enclosed organelles are thought to have arisen in evolution in at least two ways:

  1. The nuclear membrane and the membranes of the ER, Golgi apparatus, endosomes, and lysosomes are believed to have originated by invagination of the plasma membrane. These membranes, and the organelles they enclose, are all part of what is called the endomembrane system.

  2. Mitochondria and chloroplasts differ from all other organelles in that they possess their own small genomes and can make some of their own proteins. The similarity of these genomes to those of bacteria suggests that mitochondria and chloroplasts evolved from bacteria that were engulfed by primitive eukaryotic cells with which they initially lived in symbiosis. This would also explain why these organelles are enclosed by two membranes.

Protein sorting

Before a eukaryotic cell reproduces by dividing in two, it has to duplicates its membrane-enclosed organelles. As a cell grows, membrane-enclosed organelles enlarge by incorporation of new molecules. The organelles then divide and at cell division they are distributed between the two daughter cells. The nuclear envelope, ER and Golgi apparatus break up into small vesicles, which ten coalesce again as the two daughter cells are formed. Organelle growth requires a supply of new lipids to make more membrane and a supply of the appropriate proteins. These newly synthesized proteins must be accurately delivered to organelles.

The synthesis of all proteins in the cell begins of ribosomes in the cytosol. The exceptions are the few mitochondrial and chloroplasts proteins that are synthesized on ribosomes inside these organelles. However, most mitochondrial and chloroplasts proteins are made in the cytosol. The fate of any protein molecule synthesized in the cytosol depends on its amino acid sequence, which can contain a sorting signal that directs the protein to the organelle in which it is required. Proteins that lack such signals remain as permanent residents in the cytosol. The typical sorting signal on proteins is a stretch of amino acids sequence, 15-60 amino acids long. This signal sequence is often removed from the finished protein once the sorting decision has been executed.

Proteins are imported into the organelles by three mechanisms:

  1. Nuclear proteins contain nuclear localization signals that help direct their active transport from the cytosol into the nucleus through nuclear pores, which penetrate the double-membrane nuclear envelope. First, specialized proteins, called nuclear transport receptors, bind to the prospective nuclear protein. The resulting complex is guided to a nuclear pore by fibrils at extend from the pore into the cytosol. The binding of the nuclear proteins to the pore, opens the pore, and the complex is actively transported into the nucleus by a process that uses the energy provided by GTP hydrolysis. The receptors are then exported back through the pores into the cytosol for reuse. Proteins can enter the nucleus without being unfolded.

  2. Most mitochondrial and chloroplast proteins are made in the cytosol and are then actively transported into the organelles by protein translocators in their membranes. Proteins must be unfolded to allow them to snake through the chloroplast or mitochondrial membrane. Chaperone proteins inside the organelles help to pull the proteins across the two membranes and to refold the protein once it is inside. Subsequent transport to a particular site within the organelle usually requires further sorting signals in the protein, which are often only exposed after the first signal sequence in removed. Proteins moving from cytosol into the ER also use the mechanism of protein translocators.

  3. Proteins moving from the ER onward and from one compartment of the endomembrane system to another are transported by transport vesicles.

The outer nuclear membrane is continuous with the ER. The ER is the membrane factory of the cell; it makes most of the cell’s lipids and many of its proteins. The proteins are made by ribosomes bound to the surface of the rough ER. There are two separate populations of ribosomes in the cytosol. Membrane-bound ribosomes are attached to the cytosolic side of the ER membrane and are making proteins that are being translocated into the ER. Free ribosomes are unattached to any membrane and are making al of the other proteins encoded by nuclear DNA.

Ribosomes in the cytosol are directed to the ER if the protein they are making has an ER signal sequence, which is recognized by a signal-recognition particle (SRP) in the cytosol; the binding of the ribosome-SRP complex to a receptor on the ER membrane initiates the translocation process that threads the growing polypeptide across the ER membrane through a translocation channel. Soluble proteins destined for secretion or the lumen of an organelle pass completely into the ER lumen, while transmembrane proteins destined for the ER membrane or other cell membrane remain anchored in the lipid bilayer by one or more membrane-spanning a helices.

In the ER lumen, proteins fold up, assemble with other proteins, form disulfide bonds, and become decorated with oligosaccharide chains. Exit from the ER is an important quality-control step; proteins that either fail to fold properly or fail to assemble with their normal partners are retained in the ER and are eventually degraded.

Vesicular transport

Protein transport from the ER to the Golgi apparatus and from the Golgi apparatus to other destinations is mediated by transport vesicles that continually bud off from one membrane and fuse with another, a process called vesicular transport.

The vesicular traffic between membrane-enclosed compartments of the endomembrane system is highly organized. In the outward secretory pathway protein molecules are transported from the ER, through the Golgi apparatus, to the plasma membrane or lysosomes. In the inward endocytic pathway extracellular molecules are ingested in vesicles derived from the plasma membrane and are delivered to early endosomes and then to lysosomes.

Vesicles that bud from membranes usually have a distinctive protein coat on their cytosolic surface and are therefore called coated vesicles. After budding from its parent organelle, the vesicle sheds it coat, allowing its membrane to interact directly with the membrane to which it will fuse. Cells produce several kinds of coated vesicles, each with a distinctive protein coat; the assembly of the coat drives the budding process, and the coat proteins help incorporate receptors with their bound cargo molecules into the forming vesicle.
Best-studied vesicles are those that have coats made of the protein clathrin. These clathrin-coated vesicles bud from the Golgi apparatus on the outward secretory pathway and from the plasma membrane on the inward endocytic pathway. Clathrin molecules form basketlike cages that help shape membranes into vesicles. Clathrin itself plays no part in capturing specific molecules for transport. This is the function of a second class of coat proteins called adaptins, which both secure the clathrin coat to the vesicle membrane and help select cargo molecules for transport. Molecules for onward transport carry specific transport signals that are recognized by cargo receptors in the compartment membrane. Adaptins help capture specific cargo molecules by trapping the cargo receptors that bind them. In this way a selected set of cargo molecules, bound to their specific receptors, is incorporated into the lumen of each newly formed cathrin-coated vesicle.

Coated vesicles lose their protein coat soon after pinching off, enabling them to dock and fuse with a particular target membrane. Docking and fusion are thought to be mediated by proteins on the vesicle and on the target membranes, called v-SNAREs and t-SNAREs, respectively. Each organelle and each type of transport vesicle is believed to carry a unique SNARE, and the interactions between complementary SNAREs help ensure that transport vesicles fuse only with the correct membrane. Fusion not only delivers the contents of the vesicle into the interior of the target organelle, it also adds the vesicle membrane to the membrane of the organelle. Pairing of v-SNAREs and t-SNAREs forces the two lipid bilayers into close apposition. Lipids then flow between the two bilayers and the membranes fuse.

Secretory pathways

The Golgi apparatus receives newly made proteins from the ER; it modifies their oligosaccharides, sort proteins, and dispatches them from the trans Golgi network to the plasma membrane, lysosomes, or secretory vesicles. Some proteins are destined to function in the ER and they are retained in the ER by a C-terminal sequence of four amino acids called an ‘ER retention signal’, which is recognized by a membrane-bound receptor protein in the ER and Golgi apparatus. However, most proteins that enter the ER are destined for other locations. As mentioned above, exit from the ER is highly selective; chaperones prevent misfolded or partially assembled proteins from leaving the ER.

The mutation that causes the genetic disease cystic fibrosis, which causes severe degeneration of the lung, produces a plasma-membrane transport protein that is slightly misfolded. The devastating disease results not because the mutation inactivates an important protein, but because the active protein is discharged by the cell before it is given an opportunity to function.

After the exit from the ER, proteins are further modified and sorted in the Golgi apparatus. The Golgi apparatus consists of a collection of flattened, membrane-enclosed sacs (cisternae). Each Golgi stack has two distinct faces: an entry (or cis) fase and an exit (or trans) face. The cis face is adjacent to the ER, while the trans face points toward the plasma membrane. Soluble proteins and membrane enter the cis Golgi network via transport vesicles derived from the ER. The proteins travel through the cisternae in sequence by means of transport vesicles that bud from one cisterna and fuse with the next. Proteins exit from the trans Golgi network in transport vesicles destined for either the cell surface or another compartment. Both the cis and trans Golgi network are thought to be important for protein soring.

In all eukaryotic cells, transport vesicles continually bud from the trans Golgi network and fuse with the plasma membrane, a process called constitutive exocytosis; the process delivers plasma membrane lipids and proteins to the cell surface and also releases molecules from the cell, a process called secretion. In addition to the constitutive exocytosis pathway, which operated continually, there is also a regulated exocytosis pathway, which operates only in cells that are specialized for secretion. Specialized secretory cells produce large quantities of particular products, such as hormones or digestive enzymes, which are stored in secretory vesicles for later release. These vesicles bud off from the trans Golgi network and accumulate near the plasma membrane. There they wait for the extracellular signal that will stimulate them to fuse with the plasma membrane and release their contents to the cell exterior.

Endocytic pathway

Cells ingest fluid, molecules, and sometimes even particles, by endocytosis, in which regions of plasma membrane invaginate and pinch off to form endocytic vesicles. Two main types of endocytosis are distinguished on the basis of the size of the endocytic vesicles formed:

  1. Pinocytosis (‘cellular drinking’): this involves the ingestion of fluid and molecules via small vesicles (<150 nm in diameter)

  2. Phagocytosis (‘cellular eating’): this involves the ingestion of large particles, such as microorganisms and cell debris, via large vesicles called phagosomes (>250 nm in diameter)

Whereas all eukaryotic cells are continually ingesting fluid and molecules by pinocytosis, large particles are ingested mainly by specialized phagocytic cells. Phagocytic cells ingest large particles by taking them up into phagosomes; these phagosomes then fuse with lysosomes. Phagocytosis is important for digesting food molecules and defense against infections by ingesting invading microorganisms. Because during pinocytosis, a cell’s total surface area and volume remain unchanged, it is clear that as much membrane is being added to the cell surface by vesicle fusion (exocytosis) as is being removed by endocytosis.

Much of the material that is endocytosed is delivered to endosomes and then to lysosomes, where hydrolytic enzymes degrade it; most of the components of the endocytic vesicle membrane, however, are recycled in transport vesicles back to the plasma membrane for reuse.

16. Cell communication

Cells in multicellular organisms communicate through a large variety of extracellular chemical signals. And communication involves converting information signals from one form to another, a process called signal transduction. In a typical communication between cells, the signaling cell produces a particular type of signal molecule that is detected by the target cell. The target cells possess receptor proteins that recognized and respond specifically to the signal molecule. Signal transduction begins when the receptor protein on the target cell receives an incoming extracellular signal and converts it to the intracellular signals that alter cell behavior.

General principles of cell signaling

Single cells and cells in multicellular organisms use a variety of extracellular molecules to send signals to one another:

  1. Endocrine signals: hormones produced in endocrine glands are secreted into the bloodstream and are often distributed widely throughout the body

  2. Paracrine signals: the signaling molecules diffuse locally through the extracellular medium, remaining in the neighborhood of the cell that secretes them. Thus they act as local mediators on nearby cells.

  3. Neuronal signals: neurons can deliver messages across long distances, but in the case of neuronal signaling the message is not broadcast widely but is transmitted quickly along axons to remote target cells.

  4. Contact-dependent signals: this style of signaling does not require the release of a secreted molecule. Instead, the cells make direct contact through signaling molecules lodged in their plasma membranes. The message is delivered when a signal molecule anchored in the plasma membrane of the signaling cell binds to a receptor molecule embedded in the plasma membrane of the target cell.

Many of the signal molecules that regulate inflammation at the site of an infection or control cell proliferation in a healing wound function as paracrine signals. In embryonic development contact-dependent signaling plays an important role; for example it controls nerve-cell production.

A cell in a multicellular organism is exposed to hundreds of different signal molecules in its environment. Each cell must respond selectively to this mixture of signals, disregarding some and reacting to others, according to the cell’s specialized function. Whether a cell responds to a signal molecule depends first on whether is possesses a receptor for that signal. But one signal can still be used to control the behavior of the cell in complex ways:

  1. One signal, binding to one type of receptor protein, can cause a multitude of effect in the same target cell. Furthermore, different types of cells respond to the same signal in different ways.

  2. A cell possesses a collection of different receptors. Such variety makes the cell sensitive to many extracellular signals. These signal molecules work in combinations to regulate the behavior of the cell.

Cells are stimulated by an extracellular signal molecule when it binds to and activates a receptor protein. Each receptor protein recognizes a particular signal molecule. Receptor proteins act as transducers, converting signals from one physical form to another. However, most extracellular signal molecules cannot pass through the plasma membrane; first they must bind to cell-surface receptor proteins that transduce the extracellular signal into different intracellular signals.

Extracellular signal molecules fall into two classes:

  1. Signal molecules that are too large are too hydrophilic to cross the plasma membrane of the target cell. They bind on receptors on the surface of the target cell to relay their message across the membrane.

  2. Signal molecules that are small enough or hydrophobic enough to slip easily through the plasma membrane. Once inside, these signal molecules either activate intracellular enzymes or bind to intracellular receptor proteins that regulate gene expression. Steroid hormones (including cortisol and testosterone) and nitric oxide (NO) are examples of small hydrophobic extracellular signal molecules. Acetylcholine released by nerve terminals in the blood-vessel wall stimulates endothelial cells lining the blood vessel to make and release NO. The NO diffuses out of the endothelial cells and into adjacent smooth muscle cells, causing them to relax.  

In contrast to NO and the steroid hormones, the majority of signal molecules are too large or hydrophilic to cross the plasma membrane of the target. These signal molecules bind to receptor proteins on the target cell surface:

There are three main classes of cell-surface receptors:

  1. Ion-channel-linked receptors: this receptor opens in response to binding of its signal molecule. The result is a flow of ions across the membrane, which produces an electrical current

  2. G-protein-linked receptors: when a G-protein-linked receptor binds its extracellular signal molecule, the signal is passes first to a GTP-binding protein (a G-protein) that is associated with the receptor. The activated G-protein then leaves the receptor and turns on a target enzyme in the plasma membrane

  3. Enzyme-linked receptors: when binding of the signal molecule activates this receptor, enzyme activity is switched on at the other end of the receptor, which is inside the cell

In sum, G-protein-linked receptors and enzyme-linked receptors respond to extracellular signals by initiating cascades of intracellular signaling reactions that alter the behavior of the cell.

G-protein-linked receptors

G-protein-linked receptors form the largest family of cell-surface receptors. They mediate responses to an enormous diversity of extracellular signal molecules. These signal molecules are as varied in structure as they are in function. Despite the diversity of the signal molecules that bind to them, all G-protein-linked receptors possess a similar structure: each is made of a single polypeptide chain that threads back and forth across the lipid bilayer seven times. There are also several varieties of G proteins. All of these G proteins, however, have a similar general structure and operate in a similar way. All G proteins are composed of three protein subunits: the a, b and g subunits.

In the unstimulated state, the a subunit has GDP bound to it, and the G protein is purposeless. When an extracellular ligand binds to its receptor, the altered receptor activates a G protein by causing the a subunit to lose some of its affinity for GDP, which it exchanges for a molecule of GTP. This activation breaks up the G protein subunits: the switched-on a subunit detaches from the bg complex, giving rise to two separate molecules that now roam independently along the plasma membrane. The amount of time that the a- and bg subunits remain dissociated is limited by the behavior of the a subunit. The a subunit has an intrinsic GTP-hydrolyzing (GTPase) activity, and it eventually hydrolyzes its bound GTP back to GDP; the a subunit then reassociates with the bg complex. The reconstituted G protein is now ready to be reactivated by another activated receptor.

In concluding, when an extracellular signal molecule binds to a seven-pass transmembrane receptor, the receptor protein undergoes a conformational change that enables it to activate a G protein located on the underside of the plasma membrane. These G-proteins act as molecular switches, transmitting the signal onward for a short period and then switching themselves off by hydrolysis their bound GTP and GDP. This system demonstrates that the mechanisms that shut a signal off are as important as the mechanisms that turn it on. The disease cholera is caused by a bacterium that multiplies in the intestine where it produces a protein called cholera toxin. This protein enters the cells that line the intestine and modifies the a subunit of a G-protein in such way that it can no longer hydrolyze its bound GTP. The altered a subunit thus remains in the active state, continuously transmitting a signal to its target proteins. In intestinal cells, this causes a prolonged and excessive outflow of Cl- and water into the gut, resulting in catastrophic diarrhea and dehydration.

As mentioned above, there are many different G proteins:

  • Some G proteins directly regulate ion channels in the plasma membrane. For example, G proteins couple receptor activation to the opening of K+ channels in the plasma membrane of heart muscle cells.

  • Other G proteins activate membrane-bound enzymes. The most frequent target enzymes for G proteins are adenylyl cyclase, the enzyme responsible for production of the signaling molecule cyclic AMP, and phospholipase C, which generates the messenger molecules inositol trisphosphate (IP3) and diacylglycerol.

We take a closer look to G proteins that activate membrane-bound enzymes. Adenylyl cyclase and phospholipase C are activated by different types of G proteins, so that cells are able to couple production of the signaling molecules to different extracellular signals. Many extracellular signals acting via G protein-linked receptors affect the activity of adenyl cyclase. Most commonly, the activated G protein a subunit switches on the adenyl cyclase, causing an increase in the synthesis of cyclic AMP from ATP. To help eliminate the signal, a second enzyme, called cyclic AMP phoshodiesterase, converts cyclic AMP to ordinary AMP. Cyclic AMP exerts various effects by activating the enzyme protein kinase A (PKA). This enzyme is normally held inactive in a complex with another protein. The binding of cyclic AMP forces a conformational change that unleashes the active kinase. In some cases the effects of activating a cyclic AMP cascade are rapid; in others the effects are slow. A rise in intracellular cyclic AMP can activate gene transcription.

The inositol phospolipid pathway begins with the activation of the membrane-bound enzyme phospholipase C. This enzyme activates two signaling pathways: IP3 and diacylglycerol. IP3 opens ion channels in the membrane of the endoplasmatic reticulum, releasing a flood of free Ca2+ ions into the cytosol. Ca2+ itself acts as an intracellular messenger, altering the activity of a wide range of proteins. Together with this Ca2+, diacylglycerol helps recruit and activate an enzyme called protein kinase C (PKC).

In concluding, a rise in cyclic AMP activates protein kinase A (PKA), while CA2+ and diacylglycerol in combination activate protein kinase C (PKC). PKA and PKC phosphorylate secreted target proteins on serines and threonines, thereby altering protein activity. Different cell types contain different sets of target proteins and are affected in different ways.

In general, stimulation of G-proteins-linked receptors produces rapid and reversible cell responses!

Enzyme-linked receptors

Plants, like animals use enzyme-linked cell-surface receptors to control their growth and development. Like G-protein-linked receptors, enzyme-linked receptors are transmembrane proteins that display their ligand-binding domains on the outer surface of the plasma membrane. Instead of associating with a G protein, the cytoplasmatic domain of the receptor acts as an enzyme or forms a complex with another protein that acts as an enzyme. Most are receptor tyrosine kinase, which phosphorylate tyrosines on selected intracellular proteins. Activated receptor tyrosine kinases cause the assembly of an intracellular signaling complex on the intracellular tail of the receptor. A part of this complex serves to activate Ras, a small GTP-binding protein, which activates a cascade of protein kinases that relay the signal from the plasma membrane to the nucleus. This cascade is called a MAP-kinase cascade.

MAP-kinase is the final kinase in the chain and it phosphorylates certain gene regulatory proteins on serines and threonines, altering their ability to control gene transcription and thereby causing a change in the pattern of gene expression. This shift may stimulate cell proliferation, cell survival or induce cell differentiation. However, mutations that stimulate cell proliferation by making Ras constantly active are a common feature of many cancers.

Some enzyme-linked receptors activate a direct pathway to the nucleus. Instead of activating signaling cascades, they turn on gene regulatory proteins right at the plasma membrane. Unlike the receptor tyrosine kinases that stimulate signaling cascades, cytokine receptors have no intrinsic enzyme activity. Instead, they are associated with cytoplasmatic tyrosine kinases called JAKs that are activated when a cytokine binds to its receptor. Once activated, the JAKs phosphorylate and activate cytoplasmatic gene regulatory proteins called STATs, which then migrates to the nucleus, where they stimulate transcription of specific target genes.
An even more direct signaling pathway is used by the TGF-b receptors, which activate gene regulatory proteins directly at the plasma membrane.  

Different intracellular signaling pathways interact, enabling cells to produce an appropriate response to a complex combination of signals. Some combinations of signals will cause it to proliferate; and in the absence of any signals, most cells will kill themselves by undergoing apoptosis.

17. Cytoskeleton

The cytoskeleton is an intricate network of protein filaments that extend throughout the cytoplasm. It is responsible for large-scale movements, and without the cytoskeleton, wounds would never heal, muscles would be useless, and sperm would never reach the egg. The cytoskeleton is build on a framework of three types of protein filaments, and each type of filament has distinct mechanical properties and is formed from a different protein subunit.

  1. Intermediate filaments: these are ropelike fibers made of intermediate filament proteins. One type of intermediate filaments forms a meshwork called the nuclear lamina just beneath the inner nuclear membrane. Other types extend across the cytoplasm, giving cells mechanical strength and distributing the mechanical stresses in an epithelial tissue by spanning the cytoplasm from one cell to another.

  2. Microtubules: these are long, hollow cylinders made of the protein tubulin. They are more rigid than actin filaments or intermediate filaments. Microtubules have typically one end attached to a single microtubule-organizing center called a centrosome.

  3. Actin filaments: these are flexible structures made of the protein actin. Although actin filaments are dispersed throughout the cell, they are most highly concentrated in the cortex (the layer of cytoplasm just beneath the plasma membrane)

Intermediate filaments

The main function of intermediate filaments is to enable cells to withstand the mechanical stress that occurs when cells are stretched. Intermediate filaments are therefore present along the length of nerve cell axons, in muscle cells and in epithelial cells. In all these cells, intermediate filaments, by stretching and distributing the effect of locally applied forces, keep the cells and their membranes from breaking.

The filaments are called ‘intermediate’ because their diameter (10nm) is between that of the thin actin-containing filaments and the ticker myosin filaments of smooth muscle cells. Intermediate filaments are the toughest and most durable of the three types of cytoskeletal filaments. The intermediate filaments are found in the cytoplasm of most animal cells. They typically form a network throughout the cytoplasm, surrounding the nucleus and extending out to the cell periphery. Furthermore, intermediate filaments are also found within the nucleus as the nuclear lamina, which underlies and strengthens the nuclear envelope.
Intermediate filaments can be grouped intro four classes:

  1. Keratin filaments in epithelial cells. Keratin filaments typically span the interiors of epithelial cells from one side to the cell to the other, and filaments in adjacent epithelial cells are indirectly connected through cell-cell junctions called desmosomes. This network distributes the stress that occurs when the skin is stretched. The importance of this function is illustrated by the rare genetic disease epidermolysis bullosa simplex, in which mutations in the keratin genes interfere with the formation of keratin filaments in the epidermis. As a result, the skin is highly vulnerable to mechanical injury, and even a gentle pressure can rupture its cell, causing the skin to blister.

  2. Vimentin and vimentin-related filaments in connective-tissue, muscle and neuroglial cells

  3. Neurofilaments in nerve cells

  4. Nuclear lamins, which strengthen the nuclear membrane of all animal cells

Filaments of each class are formed by polymerization of their corresponding protein subunits. Plectin aids in the bundling of intermediate filaments and links these filaments to other cytoskeletal protein networks. Mutations in the gene for plectin cause a devastating disease that combines features of epidermolysis bullosa simplex, muscular dystrophy and neurodegeneration. Thus, although plectin may not be necessary for the initial formation of intermediate filaments, its cross-linking action is crucial to withstand the mechanical stress.  

Microtubules

Microtubules are stiff, hollow tubes formed by polymerization of tubulin dimer subunits. They are polarized structures with a slow-growing ‘minus’ end (the a-tubulin end) and a fast-growing ‘plus’ end (the b-tubulin end).  Microtubules are nucleated in, and grow out from, organizing centers such as the centrosome. The minus ends of the microtubules are embedded in the organizing center. Centrosomes contain hundreds of ring-shaped structured formed from another type of tubuline, g-tubulin, and each g-tubulin ring serves as the starting point (or nucleation site) for the growth of one microtubule.

Once a microtubule has been nucleated it has in a labile, dynamic state in which the microtubule alternate between a growing state and a shrinking state. These transitions, known as dynamic instability, are controlled by the hydrolysis of GTP bound to tubulin dimers. Each tubulin dimer has a tightly bound GTP molecule that is hydrolyzed to GDP after the tubulin assembles into a microtubule. GTP hydrolysis reduces the affinity of the subunit for its neighbors and decreases the stability of the polymer, causing it to dissemble. In this way, GTP hydrolysis controls the growth of microtubules.

The relative instability of microtubules allows them to undergo continual rapid remodeling, and this is crucial for microtubule function, as demonstrated by the effect of drugs that prevent polymerization or depolymerization of tubulin. If a cell in mitosis is exposed to the drug colchicine, which binds tightly to free tubulin and prevents its polymerization into microtubules, the mitotic spindle rapidly disappears and the cell is unable to partition its chromosomes into two groups. This shows that the mitotic spindle is normally maintained by a continuous balanced addition and loss of tubulin subunits. The inactivation or destruction of the mitotic spindle will eventually kill dividing cells.

Cells are able to modify the dynamic instability of their microtubules for particular purposes. When a cell has differentiated into a specialized cell type and taken on a definite fixed structure, the dynamic instability of its microtubules or along their length and stabilize them against disassembly. The stabilized microtubules then serve to maintain the organization of the cell. Proteins that capture the plus end can stabilize microtubules. Its important to realize that the microtubules in living cells do not act alone.

Intracellular transport is generated by motor proteins, which bind to actin filaments or microtubules and use the energy derived from repeated cycles of ATP hydrolysis to travel along the actin filament or microtubule in a single direction. Motor proteins move along microtubules using their globular heads and they belong to two families:

  1. The kinesins generally move toward the plus end of a microtubule; away from the centrosome
  2. The dyneins move toward the minus end, or toward the centrosome

Kinesins and dyneins both have two globular ATP-binding heads and a tail. The globular heads are enzymes with ATP-hydrolyzing (ATPase) activity. This reaction provides the energy for a cycle of conformational changes in the head that enable it to move along the microtubule by a cycle of binding, release, and rebinding to the microtubule. Finally, microtubules and their associated motor proteins play an important part in positioning membrane-enclosed organelles within a eukaryotic cell.

As mentioned earlier in this summary, many microtubules in cells are stabilized through their association with other proteins, and therefore no longer show dynamic instability. This is seen in cilia and flagella that contain a bundle of stable microtubules. Bending of the microtubules, driven by a motor protein called ciliary dynein, causes their beating.

Actin filaments

Actin filaments are found in all eukaryotic cells and are essential for many of their movements, especially those involving the cell surface. Like microtubules, many actin filaments are unstable, but they can also form stable structures in cells, such as the contractile apparatus of muscle. The varied forms and functions of actin filaments in cells depends on multiple actin-binding proteins. These control the polymerization of actin filaments, cross-link the filaments into loose networks or stiff bundles, attach them to membranes, or move them relative to one another.

Composition of actin filaments

Actin filaments are helical polymers of actin molecules. They are thinner, more flexible, and shorter than microtubules. Furthermore, actin molecules rarely occur in isolation in the cell; they are generally found in cross-linked bundles and networks, which are much stronger then the individual filaments.

Actine filaments are polarized structures with a fast- and a slow-growing end; the rate of growth is faster at the plus end than at the minus end. A ‘naked’ actin filament is unstable and can disassemble from both ends. Each free actin monomer carriers a tightly bound ATP, which is hydrolyzed to ADP soon after the incorporation of the actin monomer into the filament. Hydrolyses of ATP to ADP reduces the strength of binding between monomers and decreases the stability of the polymer. This hydrolysis thereby promotes depolymerization, helping the cell to disassemble filaments after they have formed. As for microtubules, the ability to assemble and disassemble is required for many of the functions performed by actin filaments.

Drugs like cytochalasins prevent actin polymerization, and others like jasplakinolides stabilize actin filaments against depolymerization. Addition of these toxins freezes cell movements.

Function of actin filaments

Although actin is found throughout the cytoplasm of a eukaryotic cell, in most cells it is concentrated in the layer just beneath the plasma membrane, also known as the cell cortex. In this region actin filaments are linked by actin-binding proteins into a meshwork that supports the outer surface of the cell and gives it mechanical strength. In this way, actin filaments are responsible for the shape and movement of the cell surface, including the movements involved when a cell crawls along a surface. For this kind of movements are three interrelated processes required; all these three processes involve actin, but in different ways:

  1. The cell pushes out protrusions at its front, or leading edge; this is driven by actin polymerization. The leading edge of a crawling cell regularly extends thin, sheetlike lamellipodia, which contain a dense meshwork of actin filaments. Many cells also extend thin, stiff protrusions called filopodia, which also contains a bundle of actin filaments. The formation and growth of actin filaments at the leading edge of a cell is assisted by various actin-binding accessory proteins, one set of proteins, the actin-related proteins or ARPs, promote the formation of branched actin filaments. These proteins form a complex that binds to the existing actin filaments, where they nucleate the growth of a new filament, which grows out at an angle to form a side branch. With the aid of additional actin-binding proteins, this web of actin undergoes assembly at the front end and disassembly at the back, pushing the lamellipodia to the front.

  2. When the lamellipodia and filopodia touch down on a favorable patch of surface, the transmembrane proteins in their plasma membrane, known as integrins, adhere to molecules in the extracellular matrix on the surface of another cell over which the moving cell is crawling.

  3. Meanwhile, on the intracellular face of the membrane of the crawling cell, integrins capture actin filaments, thereby creating an anchorage for the system of actin filaments inside the cell. The rest of the cell drags itself forward by traction on these anchorage points. This too depends on actin, but through the interaction of actin filaments with motor proteins known as myosins.

A variety of actin-binding proteins are thus required to drive the leading edge of a migrating cell forward, to adhere to the substratum, and to retract its trailing edge. All of these processes are triggered by external stimuli working via small GTP-binding proteins.

Muscle contraction

Myosins are motor proteins that use the energy of ATP hydrolysis to move along actin filaments: they can carry organelles along actin-filament tracks or cause adjacent actin filaments to slide past each other in contractile bundles. There are several different types of myosins in cells, of which the myosin-I and myosin-II subfamilies are most abundant. Myosin-I is found in all types of cells, and the myosin-I molecules have only one head domain and a tail. The head domain interacts with actin filaments and has ATP-hydrolyzing motor activity; the tail varies among the different types of myosin-I.

Muscle myosin belongs to the myosin-II subfamily of myosins, all of which have two ATPase heads and a long, rodlike tail. Each myosin-II molecule is a dimmer composed of a pair of identical myosin molecules held together by their tails; it has two ATPase heads at one end and e single coiled-coil tail at the other. Clustering of myosin-II molecules bind to each other through their coiled-coil tails, forming a bipolor myosin filament in which the heads project from the side.

In muscle, huge arrays of overlapping actin filaments and myosin filaments generate contractions by sliding over one another. One set of heads binds to acting filaments in one orientation and moves them in one way; the other set of heads binds to other actin filaments in the opposite orientation and moves them in the opposite direction.

The long fibers of skeletal muscle are huge single cells formed by the fusion of many separate smaller cells. A skeletal muscle cell is packed with myofibrils, which consists of a chain of identical tiny contractile units, or sacromeres. Sacromeres are highly organized assemblies of two types of filaments: actin filaments and filaments of muscle-specific myosin-II. Myosin filaments are centrally positioned in each sacromere, whereas the actin filaments extend inward from each end of the sacromere and overlap the ends of the myosin filaments.
The contraction of a muscle cell is caused by simultaneous shortening of all the sacromeres, which in turn is caused by the actin filaments sliding past the myosin filaments, with no change in the length of either type of filament. When a muscle is stimulated to contract, the myosin heads start to walk along the actin filament in repeated cycles of attachment and detachment. During each cycle, a myosin head binds and hydrolyzes one molecule of ATP. After a contraction is completed, the myosin heads lose contact with the actin filaments completely, and the muscle relaxes.

The molecular interaction between myosin and actin filaments takes place only when the skeletal muscle receives a signal from the nervous system. The signal from a nerve terminal triggers an action potential, which caused a release of Ca2+ in the cytosol. As mentioned earlier in this summary, Ca2+ is widely used as an intracellular signal to rely a message from the exterior to the internal machinery of the cell. In the case of muscle, the Ca2+ interacts with a molecular switch made of specialized accessory proteins. One of these proteins is tropomyosin, a molecule that binds in the groove of the actin helix and prevents the myosin heads from associating with the actin filament. The other is troponin, a complex that includes a Ca2+-sensitive protein (troponin-C), which is associated with the end of a tropomyosin molecule. When the level of Ca2+ rises in the cytosol, Ca2+ binds to troponin and induces a change in its shape. This in turn causes the tropomyosin molecules to shift their position, allowing myosin heads to bind to the actin filament and initiating contraction.

18. Cell-cycle control and cell death

All living organisms are products of repeated rounds of cell growth and division extending back in time to the beginnings of life over three billion years ago. A cell reproduces by carrying out an orderly sequence of events in which it duplicates its contents and then divides in two. This cell cycle is the essential mechanism by which all living things reproduce. To ensure correct progression through the cell cycle, eukaryotic cells have evolved a complex network of regulatory proteins, known as the cell-cycle control system.

Overview of the cell cycle

The most basic function of the cell cycle is to duplicate accurately the vast amount of DNA in the chromosomes and then precisely distribute the copies into genetically identical daughter cells. The duration of the cell cycle varies greatly from one cell type to another.

The eukaryotic cell cycle consists of four distinct phases. In the M phase two events occur: dividing of the nucleus, a process called mitosis and dividing of the cytoplasm, a process called cytokinesis. The period between one M phase and the next is called interphase, in which the cell increases in size and encompass the remaining three phases of the cell cycle. During S phase (S=synthesis), the cell replicates its nuclear DNA. S phase is flanked by two phases in which the cell continues to grow. The G1 phase (G=gap) is the interval between the completion of M phase and the beginning of the S phase. The G2 phase in the interval between the end of S phase and the beginning of M phase. During these gap phases, the cell monitors the internal and external environments to ensure that conditions are suitable and preparations are complete. At particular points in G1 and G2 the cell decides whether to proceed to the next phase or pause to allow more time to prepare.

The first visible sign that a cell is about to enter the M phase is the progressive condensation of its chromosomes, which were replicated earlier during S phase. Chromosome condensation thus marks the end of the G2 phase, and at this stage in the cell cycle the replicated chromosomes become visible in the light microscope.

The essential processes of the cell cycle, such as DNA replication, mitosis, and cytokinesis, are triggered by a cell-cycle control system. The events of the cell cycle must occur in a particular sequence, and this sequence must be preserved even if one of the steps takes longer than usual. The cell-cycle control system achieves all of this by means of molecular brakes that can stop the cycle at various checkpoints. Two important checkpoints occur in G1 and G2:

  • The G1 checkpoint allows the cell to confirm that the environment is favorable for cell proliferation and its DNA is intact before committing to S phase. Cell proliferation depends of nutrients and specific signal molecules in the extracellular environment. If extracellular conditions are unfavorable cells can delay progress through G1 and may even enter a specialized resting state known as G0.

  • The G2 checkpoint ensures that cells do not enter mitosis until damaged DNA is repaired and DNA replication is completed.

The cell-cycle control system

The cell-cycle control system coordinates the events of the cell cycle by cyclically switching on the appropriate parts of the cell-cycle machinery and then switching them off. As discussed earlier in this summary, phosphorylation followed by dephosphorylation is one of the most common ways used by cells to switch the activity of a protein on and then off, and the cell-cycle control system uses this mechanism repeatedly. The phosphorylation reactions are carried out by a specific set of protein kinases, enzymes that transfer a phosphate group from ATP to a particular amino acid side chain of the target protein. Switching these protein kinases on and off at the appropriate times is regulated by a second set of protein components of the control system: cyclin-dependent protein kinases (Cdks).

Different cyclin-Cdk complexes trigger different steps of the cell cycle:

  • M-Cdk drives the cell into mitosis
  • G1-Cdk drives it through G1 toward S phase
  • G1/S-Cdk and S-Cdk drive it into S phase.

M-Cdk

Synthesis of M-cyclin starts immediately after cell division. Activated M-Cdk indirectly activates more M-Cdk; this explosive increase in M-Cdk activity drives the cell abruptly into M phase. Its rapid elimination then helps initiate the exit from mitosis. This elimination is the result of the ubiquitin-dependent proteolytic system. As mitosis nears completion, multiple molecules of the protein ubiquitin are attached to the M-cyclin molecules. This ubiquitination marks the cyclin for degradation in proteasomes, large proteolytic machines found in all eukaryotic cells. A protein complex called the anaphase promoting complex (APC) adds ubiquitin to the cyclin and to other proteins involved in the regulation of mitosis. Destruction of the cyclin inactivates the Cdk.

S-Cdk

As we discussed earlier, DNA replication begins at origins of replication. These sequences recruit specific proteins that control the initiation and completion of DNA replication. One multiprotein complex, the origin recognition complex (ORC), remains bound to the origins of replication throughout the cell cycle, where it serves as a sort landing pad for additional regulatory proteins that bind before the start of S phase. One of these regulatory proteins is called Cdc6, which concentration increases in early G1. When Cdc6 binds to ORCs in G1, it promotes the binding of additional proteins to form a pre-replicative complex. S-Cdk then triggers origin firing by causing the assembly of DNA polymerase and the initiation of DNA synthesis. S-Cdk also helps block replication by helping to phosphorylate Cdc6, which dissociated from the origin and is degraded.

The cell-cycle can be halted by at least two mechanisms:

  1. 1Cdk inhibitor proteins can block the assembly or activity of one or more cyclin-Cdk complexes. This is seen when checkpoints mechanisms halts the cell cycle in G1 if DNA is damaged, helping to ensure that a cell does not replicated damaged DNA. When DNA is damaged, the p53 protein, which is normally rapidly degraded, is stabilized and activated. This is partly because p53 becomes phosphorylated by specific protein kinases that are activated in response to DNA damage. Activated p53 accumulates and stimulates the transcription of the gene that encodes the Cdk inhibitor protein p21. The p21 protein binds to G1/S-Cdk and S-Cdk and inactivates them, so that the cell cycle arrests in G1. If p53 is missing of defective, the replication of damaged DNA leads to a high rate of mutations and the production of cells that tend to become cancerous. In fact, mutations in the p53 gene are found in about half of all human cancers.

  2. Components of the control system can stop being made, for example when cells enter G0. It seems to be a general rule that cells will multiply only if they are stimulated to do so by signals from other cells. If deprived of such signals, the cell cycle arrests at a G1 checkpoint and enters the G0 state.

Programmed cell death (apoptosis)

Animal cell numbers are not only regulated by controlling the rate of cell division, but also by controlling the rate of cell death. If cells are no longer needed, they commit suicide by activating an intracellular death program. This process is therefore called programmed cell death, although it is more commonly called apoptosis. In adult tissues, cell death exactly balances cell division. If this were not so, the tissue would grow or shrink.

Cells that die as a result of acute injury typically swell and burst, spilling their contents all over their neighbors, a process called cell necrosis. By contrast, a cell that undergoes apoptosis dies neatly, without damaging its neighbors. A cell in apoptosis shrinks and condenses. The cytoskeleton collapses, the nuclear envelope disassembles, and the nuclear DNA breaks up into fragments. Most important, the cell surface is altered in such a manner that it immediately attracts phagocytic cells, usually specialized phagocytic cells called macrophages. These cells engulf the apoptotic cell before it spills its contents. This rapid removal of the dying cell avoids the damaging consequences of cell necrosis, and also allows the organic components of the apoptotic cell to be recycled by the cell that ingests it.

Apoptosis is carried out by a family of proteases called caspases. The caspases are made as inactive precursors called procaspases, which are themselves activated by proteolytic cleavage in response to signals that induce apoptosis. The activated caspases cleave, and thereby activate, other members of the family, resulting in an amplifying proteolytic cascade.

The main proteins that regulate the activation of procaspases are members of the Bcl-2 family of intracellular proteins. Some members of this protein family promote procaspase activation and cell death, whereas others inhibit these processes. Two of the most important death-promoting family members are proteins called Bax and Bak. These proteins activate procaspases indirectly, by inducing the release of cytochrome c from mitochondria into the cytosol. Cytochrome c binds to an adaptor protein, which then activates a specific procaspase. This activated procaspases initiates the caspase cascade that leads to apoptosis.

Extracellular control of cell numbers and cell size

Most of the extracellular signal molecules that influence cell division, cell growth, and cell survival are soluble proteins secreted by other cells or proteins bound to the surface of other cells or the extracellular matrix. Although most act positively to stimulate one or more of these cell processes, some act negatively to inhibit a particular process. The positively acting signal proteins can be divided into three major classes based on their function:

  1. Mitogens: animal cells proliferate only if stimulated by mitogens, which activate intracellular signaling pathways to override the normal brakes that otherwise block cell-cycle progression; this mechanism ensures that a cell divides only when another cell is needed.

  2. Growth factors: for an organism or an organ to grow, cells must grow as well as divide. Animal cell growth depends on extracellular growth factors, which stimulate protein synthesis and inhibit protein degradation.

  3. Survival factors: most animal cells require continuous signaling from other cells to avoid apoptosis; and this may be a mechanism to ensure that cells survive only when and where they are needed.

Cancer cells fail to obey these normal ‘social’ controls on cell behavior and therefore outgrow, out-divide and out-survive their normal neighbors.

19. Cell division

We take a closer look to the final phase of the cell cycle, when the cell divides its nucleus (mitosis) and then its cytoplasm (cytokinesis). Together, mitosis and cytokinesis constitute M phase of the cell cycle.

An overview of M Phase

When the chromosomes are duplicated in S phase, the two copies of each duplicated chromosome (called sister chromatids) remain tightly bound together by cohesins. A set of protein complexes, called condensins, helps to carry out chromosome condensation when the cell is about to enter the M phase. Together, cohesins and condensins help reduce the mitotic chromosomes to small, condensed structures that can be easily segregated during mitosis. M phase is initiated by the phosphorylation triggered by activated M-Cdk.

To produce two identical daughter cells, a mitotic spindle is formed during M phase. This mitotic spindle is composed of microtubules and the various proteins that interact with them, including microtubule-associated motor proteins. In animal cells and many unicellular eucaryotes, a different cytoskeletal structure is responsible for cytokinesis. It is called the contractile ring because it consists mainly of actin filaments and myosin filaments arranged in a ring around the equator of the cell. As the ring contracts, it pulls the membrane inward, thereby dividing the cell in two. The microtubules bind to protein complexes called kinetochores, associated with the centromere of each sister chromatid.

However, before M phase begins two critical events must be completed: DNA must be fully replicated and the centrosome must be duplicated. Each centrosome consists of proteins that contain hundreds of g-tubulin rings. These ring complexes serve as nucleation sites for the growth of microtubules that radiate out from the centrosome. During interphase of each cell cycle, the centrosome is duplicated and as mitosis begins the two centrosomes separate, each of which nucleates its own aster. The two asters move to opposite sides of the nucleus to form the two poles of the mitotic spindle. When the nuclear envelope breaks down, the spindle microtubules invade the nuclear area and capture the replicated chromosomes. The process of centrosome duplication and separation is known as the centrosome cycle.

Although M phase proceeds as a continuous sequence of events, it is traditionally divided into six stages. The first five stages of M phase constitute mitosis, and cytokinesis occurs in the sixth stage, which overlaps with the end of mitosis.
The six stages are:

  1. Prophase: at the beginning of the prophase, the two daughter centrosomes separate. They now organize their own array of microtubules and being to move to opposite poles of the cell, driven by centrosome-associated motor proteins that use the energy of ATP hydrolysis to move along the microtubules. During prophase, some of the microtubules growing from one centrosome interact with the microtubules from the other centrosome; this interaction stabilizes the microtubules.

  2. Prometaphase: this starts abruptly with the disassembly of the nuclear envelope, which breaks up into small membrane vesicles. This process is triggered by the phosphorylation and consequent disassembly of the intermediate filament proteins of the nuclear lamina. Chromosomes can now attach to spindle microtubules via their kinetochores and undergo active movements.

  3. Metaphase: the chromosomes are aligned at the equator of the spindle, midway between the spindle poles. The paired kinetochore microtubules on each chromosome attach to opposite poles of the spindle.

  4. Anaphase: this begins abruptly with the release of the cohesin linkage that holds the sister chromatids together. This allows each chromatid (now called a daughter chromosome) to be gradually pulled to the spindle pole to which it is attached. This movement segregates the two identical sets of chromosomes to opposite ends of the spindle. The abrupt disruption of the cohesin linkage is triggered by the activation of the anaphase-promoting complex (APC). Once this proteolytic complex is activated, it cleaves an inhibitory protein, thereby releasing a proteolytic enzyme that breaks the cohesin linkage. The anaphase is separated in two processes: in anaphase A the kinetochore microtubules shorten by depolymerization, and the attached chromosomes move poleward. In anaphase B, the spindle poles themselves move apart, further contributing to the segregation of the two sets of daughter chromosomes.  

  5. Telophase: the two sets of daughter chromosomes arrive at the poles of the spindle. A new nuclear envelope reassembles around each set, completing the formation of two nuclei and marking the end of mitosis. The division of the cytoplasm begins with the assembly of the contractile ring.

  6. Cytokinesis: in animal cells, cytoplasmatic division is mediated by a contractile ring of actin filaments and myosin filaments, which assembles midway between the spindle poles and contracts to divide the cytoplasm in two; in plant cells, by contrast, cell division occurs by the formation of a new cell wall inside the cell, which divides the cytoplasm in two.

Together, the six stages form a dynamic sequence in which many independent cycles are coordinated to produce two genetically identical daughter cells.

The process of mitosis ensures that each daughter cell receives a full complement of chromosomes. But when a eucaryotic cell divides, each daughter cell must also inherit all of the other essential cell components, including the membrane-enclosed organelles. Therefore, large membrane-enclosed organelles such as the endoplasmatic reticulum and Golgi apparatus break into many smaller fragments during M phase. Other components of the cell, including all of the soluble proteins, are inherited randomly when the cell divides its cytoplasm in the final stage of the M phase.

20. Genetics, meiosis, and the molecular basis of heredity

The benefits of sex

Most of the organisms around us reproduce sexually. However, reproduction without sex is possible; bacteria and other single-celled organisms can reproduce by simple cell division. While asexual reproduction is simple en direct, it usually gives rise to offspring that are genetically identical to the parent organisms. Sexual reproduction, on the other hand, involves the mixing of genomes from two individuals to produce offspring that are genetically distinct from one another and from both their parents. This way of reproduction has great advantages. One advantage seems to be that the reshuffling of the genes through sexual reproduction can help a species survive in an unpredictably variable environment. If two parents produce many offspring with a wide variety of gene combinations, the chance that at least one of their progeny will have the combinations of features necessary for survival is increased.

Sexual reproduction occurs in diploid organisms, in which each cell contains two sets of chromosomes, one inherited from each parent. The specialized cells that carry out sexual reproduction (the germ cells, or gametes) are haploid: they each contain only one set of chromosomes. These haploid germ cells are generated when a diploid cell undergoes the process of cell division called meiosis. During meiosis the chromosomes of the double chromosome set are portioned out into single chromosome sets. The two different haploid gametes then fuse to make a diploid cell (the zygote) with a new combination of chromosomes. The zyg ote thus produces develops into a new individual with a diploid set of chromosomes, which differs from that of either parent. In this way, a distinction can be drawn between the cells of the germ line (from which the next generation of gametes will be derived) and the somatic cells (which form the rest of the body).
Sexual reproduction thus involves the cyclic alternation of diploid and haploid states: diploid cells divide by meiosis to form haploid gametes, and the haploid gametes from two individuals fuse as fertilization to form a new diploid cell.

Meiosis

During meiosis, the maternal and paternal chromosomes of a diploid cell are parceled out to gametes so that each gamete receives one copy of each chromosome. Because the assortment of the two members of each chromosome pair occurs at random, many genetically different gametes can be produced from a single individual.

Before a cell divides – by either meiosis or mitosis – it first duplicates all of its chromosomes. The twin copies of each fully replicated chromosome at first remain tightly linked along their length and are called sister chromatids. However, the way these replicated chromosomes are handled differs in meiosis and mitosis. In mitosis the replicated chromosomes line up at random order at the metaphase plate; as mitosis continues, the two previously joined sister chromatids then separate from each other to become individual chromosomes. The events that occur in the first meiotic cell division mirror the sequence of stages that a cell goes through in mitosis: in prophase, the replicated chromosomes condense; in metaphase, they align at the equator of the meiotic spindle; and in anaphase, they are segregated to the poles. In this first meiotic division the homologous maternal and paternal chromosomes have paired before lining up at the metaphase plate.

After the duplicated homologs pair, genetic recombination is initiated, also called crossing-over. Crossing-over ensures the proper segregation of homologous chromosomes and enhances the genetic reassortment that occurs during meiosis by exchanging genes between them. The structure formed when homologous chromosomes pair is called a bivalent and consists of four chromatids. Cross-over events between a maternal and paternal chromatid in paired chromosomes forms a chiasma (a connection that corresponds to a crossover between two non-sister chromatids). The combination of the chiasmata and the tight attachment of the sister chromatids to each other mediated by cohesin proteins, holds the two duplicated homologs together until the spindle separates then at anaphase I. In most organisms, recombination during meiosis is required for the correct segregation of the two duplicated homologs into separate daughter nuclei.

The first meiotic division does not produce cells with a haploid amount of DNA. To achieve this goal, each cell proceeds through a second round of division, meiosis II, which occurs without further DNA replication and without any significant interphase period. A spindle forms, the chromosomes align at its equator, and the sister chromatids separate to produce daughter cells with a haploid DNA content. In meiosis II, as in mitosis, the kinetochores on each sister chromatid function independently and the cohesins holding the sister chromatids together at the centromere are degraded, allowing the two sister chromatids to be pulled to opposite poles.

Although most of the mechanical features of meiosis are similar to those of mitosis, the behavior of the chromosomes is different: meiosis produces four genetically dissimilar haploid cells by two consecutive cell divisions, whereas mitosis produces two genetically identical diploid cells by a single cell division. Whereas mitosis and division II of meiosis usually occur within hours, division I of meiosis can last days, month, or even years, due to the long time spent in prophase.

Occasionally, homologs fail to separate properly, a phenomenon known as nondisjunction. As a result, some of the haploid cells that are produced lack a particular chromosome, while others have more then one copy of it. Upon fertilization, such gametes form abnormal embryos, most of which die. However, some survive: Down syndrome, caused by an extra copy of Chromosome 21, is a human disease characterized by severe mental retardation. This extra copy results from nondisjunction of a Chromosome 21 pair during meiosis, giving rise to a gamete that contains two copies of Chromosome 21 instead of one copy. When this abnormal gamete fuses with a normal gamete at fertilization, the resulting embryo contains three copies of Chromosome 21 instead of two.
Regardless of whether the segregation error occurs in the sperm or the egg, nondisjunction is thought to be one of the reasons for the high rate of miscarriages (spontaneous abortion) in early pregnancy in humans.

Mendel and the laws of inheritance

Mendel unraveled the laws of heredity by studying the inheritance of a handful of discrete traits in garden peas. He supposed that for any pair of alleles, one allele is dominant and the other is recessive. The ideas of homozygosity and heterozygosity are also his. One important consequence of heterozygosity, and of dominance and recessiveness, is that not all of the alleles an individual carries can be detected in its phenotype. Humans have about 30.000 genes, and each of us is heterozygous for a very large number of these. Thus, we all carry a great deal of genetic information that remains hidden in our personal phenotype, but that can turn up in future generations.

Mendel’s first law

The law of segregation states that the maternal and paternal alleles for each trait separate from one another during gamete formation, then reunite at random during fertilization. This law permits us to predict the phenotypes that will result from a particular cross-breeding experiment. Mendel’s law of segregation also explains the 3:1 ratio that can be observed in the F2 generation of heterozygous inheritance. But his rules governing inheritance are not limited to reproduction in plants. Mendel’s concept of the gene and his law of segregation can be generalized to all sexually reproducing organisms, including humans.

Mendel’s second law

The law of independent assortment states that during gamete formation, different alleles segregate independently of each other. Furthermore, the behavior of chromosomes during meiosis explains Mendel’s laws. During meiosis, each set of paired homologs attaches to the spindle independently. This random arrangement of chromosomes on the metaphase spindle is reflected in Mendel’s law of independent assortment, since gene on different chromosomes will be inherited independently.

Mendel’s observation that different genes assort independently does not necessarily require that the genes lie on different chromosomes. Genes that are far enough away from one another on the same chromosome will also sort independently due to the recombination that occurs during prophase of meiosis I. In this way, if genes lie close together on a chromosome they tend to be inherited as a unit. By measuring how frequently genes are co-inherited, researchers can determine whether genes reside on the same chromosome and, if so, how far apart they lie. This type of information has been used to map the relative positions of the genes on each chromosome of many organisms. Such genetic maps have been crucial for cloning of human disease genes such as the gene for cystic fibrosis.

Gene mutations

Mutant alleles can be either dominant or recessive. If the heterozygous organism has a mutant phenotype, the mutant allel is dominant; if it has a normal phenotype, the mutant allel is recessive. So, the key to determining whether a particular allele is dominant or recessive lies in the phenotype of the heterozygote. 

Mutations have very different consequences, some confer a selective advantage, whether others cause defects and make the organisms less likely to survive. However, even deleterious mutations can benefit an organism, as individual genes can have multiple effects on phenotype. Take sickle-cell anemia in humans: this disorder is caused by a mutation in the gene encoding for b-globin, one of the polypeptides that make up hemoglobin. The sickle-cell mutation directs the formation of an abnormal polypeptide that causes red blood cells to adopt to a sickled shape. These misshapen cells clog small blood vessels, reducing the amount of oxygen that can reach different tissues, causing a variety of symptoms including muscle cramps and even heart failure. But the sickle-trait also has its benefits! Individuals who are heterozygous or homozygous for the sickle-mutation, are resistant to malaria. This is because the organism that causes the disease is unable to reproduce in sickle-shaped red blood cells, which fragment before the parasite has a chance to multiply.

Genetics as an experimental tool

Before the advent of recombinant DNA technology, most genes were identified by observing he processes disrupted when the gene was mutated. Although spontaneous mutations can sometimes be found by examining extremely large populations the process of identifying interesting mutants can be made much more efficient by generating mutations with agents that damage DNA, called mutagens. Different mutagens can generate different types of DNA alterations. And such mutants can then be screened to identify phenotypes of interest and, ultimately, to isolate the responsible genes.

Unlike worm and flies, humans are not suitable for experiments with mutagens, because they do not reproduce rapidly and any human with a serious defect in an essential process, such as DNA replication, would die long before birth. We study human genes, by studying less complex organisms which genes can reveal critical information about similar genes and processes in humans. And secondly, by analyses of the phenotypes of individuals with spontaneous mutations (like sickle-cell anemia), together with studies of their cultured cells, have provided many unique insights into important human gene function.

A large-scale genetic screen can turn up many different mutants that have the same phenotype. These defects might lie in different genes that function in the same process, or they might represent different mutations in the same gene. Complementation tests can be used to ascertain whether the mutations fall in the same or in different genes. In the simplest type of complementation test, an individual that is homozygous for one mutation is mated with an individual that is homozygous for the other mutation. If the two mutations are in the same gene, the offspring will show the mutant phenotype, because they carry only defective copies of the gene in question. If, in contrast, the mutations fall in different genes, the resulting offspring will show ‘the normal phenotype’ because they will have one normal copy (and one mutant copy) of each gene. The mutations thereby complement one another and restore a normal phenotype.

With the exception of identical twins, no two humans genomes are alike. Each of us carries a unique set of polymorphisms – changes in nucleotide sequence – that shapes our individual phenotypes. Single-nucleotide polymorphisms (SNPs) are DNA sequences that differ by a single nucleotide base between one portion of the population and another. They provide useful markers for performing genetic analyses that link a specific trait with a particular region of DNA. These polymorphisms can be used as markers for building genetic maps or for performing the genetic analyses that allow us to link particular polymorphisms with specific disease or predispositions to disease.

The problem is that any two humans differ about 0.1% in their nucleotide sequences. Theoretically, one would need to search through all 3 million of those polymorphisms to identify the one or two changes that are responsible for the differences. However, to reduce the number of polymorphisms one needs to examine, researchers are taking advantage of the recent discovery that human genes tend to be inherited in blocks. These haplotype blocks contain sets of alleles and SNPs that have been inherited as a group with little genetic rearrangement. The presence of such genetic clusters makes it easier to identify genes and mutations that are associated with human disease.

Many human traits run in families, have a genetically inherited component, but do not adhere strictly to Mendel’s laws. These complex traits are often polygenic; they arise from the interactions of multiple genes, each of which makes a small contribution to the phenotype. Although many human traits have a strong genetic basis, some are determined primarily by the environment. It is the interactions of our genetic makeup with our environment that make each of us unique.

21. Tissue and cancer

Cells are the building blocks of multicellular organisms. Most of the cells are organized into cooperative assemblies called tissues. However, tissues are composed not only of cells, with their internal framework of cytoskeletal filaments and extracellular matrix. It is this matrix that gives supportive tissues their strength.

Plants and animals have evolved their multicellular organization independently, and their tissues are constructed on different principles. Because the cytoskeleton of plants lacks the tension-bearing intermediate filaments found in animal cells, and it has virtually no tensile strength. An external cell wall, therefore, is essential. Animal tissues are more diverse. Like plants, they consists of extracellular matrix as well as cells, but these components are organized in many different ways, including bone, muscle, and epidermis.

Extracellular matrix and connective tissues

Plants

In plants, each cell surrounds itself with extracellular matrix in the form of a cell wall. Most newly formed cells in a multicellular plant initially make relatively then primary cell walls that are capable of slowly expanding to accommodate subsequent cell growth. The driving force for growth is a swelling pressure, called the turgor pressure, which develops due to an osmotic imbalance between the interior of the cell and its surroundings. Once growth stops and the wall no longer need to expand, a more rigid secondary cell wall is produced. Cellulose fibers give the plant cell wall its tensile strength. In woody tissue, a highly cross-linked lignin network is deposited within this matrix to make it more rigid and waterproof.

Because the cellulose fibers resist stretching, their orientation governs the direction in which the growing cell enlarges, or grows. Cellulose is synthesized on the outer surface of the cell by enzyme complexes embedded in the plasma membrane. These transport sugar monomers across the membrane and incorporate them into a set of growing polymer chains at their points of membrane attachment. Each set of chains forms a cellulose microfibril. The enzyme complexes move in the membrane, spinning out new polymers and laying down a trail of oriented cellulose fibers behind them. Just underneath the plasma membrane, microtubules are aligned exactly with the cellulose fiber outside the cell. These microtubules are thought to serve as tracks to guides the movement of the enzyme complexes. In this way, the orientation of the cytoskeleton controls shaping of the plant cell and the modeling of the plant tissue.

Cellulose fibers in the plant cell wall confer tensile strength; other cell wall components give resistance to compression.

Animals

There are four major types of tissues in animals: connective, epithelial, nervous, and muscular. But the basic distinction is between connective tissue and the rest. Animal connective tissues provide mechanical support and consist of extracellular matrix with sparsely scattered cells. In the extracellular matrix of animals, the tensile strength is provided not by a polysaccharide, as in plants, but by a fibrous protein called collagen. The various types of connective tissue owe their specific characters to the type of collagen that they contain, to its quantity, and to the other molecules that are interwoven it in varying proportions. The protein and polysaccharide components of the matrix are made by connective tissue cells embedded in it; in most connective tissues these cells are called fibroblasts; in bone they are called osteoblasts.

Some people have a genetic defect in the collagenase, so that their collagen fibrils do not assemble correctly. As a result, the skin and various other connective tissues have reduced tensile strength and are extraordinarily stretchable.

Cells must be able to attach to the matrix, but cells do not attach well to bare collagen. Another extracellular matrix protein, fibronectin, provides a linkage; one part of the fibronectin molecule binds to collagen, while another par forms an attachment site for a cell. The cell binds to the specific site by means of a receptor protein, called an integrin. While the extracellular domain of the integrin binds to fibronectine, the intracellular domain binds to actin filaments.

While collagen provides tensile strength to resist stretching; glycosaminoglycans (GAGs), covalenty linked to proteins to form proteoglycans, act as space-filters and provide resistance to compression.

Epithelial sheets and cell-cell junction

Cells joined together in epithelial sheets line all external and internal surfaces of the animal body. An epithelial sheet has two faces: the apical surface is free and exposed to the air or to a watery fluid; the basal surface rests on some other tissue to which it is attached. Supporting the basal surface of the epithelium there lies a thin tough sheet of extracellular matrix, called the basal lamina, composed of a specialized type of collagen and various other molecules, including a protein called laminin. Laminin provides adhesive site for integrin molecules in the plasma membrane of the epithelial cells. The apical and basal faces of an epithelium are chemically different, reflecting a polarized internal organization of the individual epithelial cells.

In epithelial sheets, in contrast to connective tissue, tension is transmitted directly from cell to cell via cell-cell junctions. Several types of cell-cell junctions are found in epithelia in animals:

  • Tight junction
  • Adherens junction
  • Desmosome
  • Gap junction
  • Hemidesmosome

Tight junctions seal neighboring cells together in an epithelial sheet to prevent leakage of molecules between them. The tight junctions are formed from proteins called claudins and occludins, which are arranged in strands along the lines of junction to create the seal. As we saw earlier in this summary, tight junctions also play a key part in maintaining the polarity of the individual epithelial cells.

The junctions that hold an epithelium together by forming mechanical attachments are of three main types. Adherens junctions and desmosome junctions bind one epithelial cell to another, while hemidesmosomes bind epithelial cells to the basal lamina. Adherens junctions and desmosome junctions are both build around transmembrane proteins belonging to the same family, called cadherins. A cadherin molecule in the plasma membrane of one cell binds directly to an identical cadherin molecule in the plasma membrane of its neighbor, this kind of binding is called homophilic.

Proteins of the cadherin family span the epithelial cell membrane and bind to similar cadherins in the adjacent epithelial cell. At an adherens junction, the cadherins are linked intercellularly to actin filaments; at a desmosome junction, they are linked to keratin filaments. Actin bundles connected from cell to cell across an epithelium can contract, causing the epithelium to bend.
Gap junctions form channels that allow passage of small molecules and ions from cell to cell. Curiously, plant tissues, though they lack all the other types of cell-cell junctions, have a functional counterpart of the gap junction. The cytoplasms of adjacent plant cells are connected via minute communicating chancels called plasmodesmata, which span the intervening cell walls.

Tissue maintenance and renewal

Although the final structure of an animal’s body may be enormously complex, it is generated by a limited repertoire of cell activities. Examples of all these activities have been discussed earlier in this summary. Trough cell division, cell growth, cell movement, and cell specialization, a fertilized egg cell gives rise to a multicellular animal. Almost every tissue in animals consists of a complex mixture of cell types that are subject to continual turnover. But throughout cell replacement and tissue renewal, the organization of the tissue must be preserved. Three key factors maintain the cellular organization of tissues:

  1. Cell communication: to survive most cells have to receive signals from their environment. These communications ensure that new cells are produced and survive only when and where they are required

  2. Selective cell-cell adhesion: because different cell types have different cadherins and other adhesion molecules in their plasma membranes, they tend to stick selectively (by homophilic binding) to other cells of the same type. Sometimes they form selective attachment to certain other cell types or to specific extracellular matrix components. The selectivity of adhesion prevents the different cell types in a tissue from becoming chaotically mixed

  3. Cell memory: specialized patterns of gene expression, evoked by signals that acted during embryonic development, are maintained so that cells preserve their distinctive character and pass it on to their progency

Cells in tissue vary enormously in their rate and pattern of turnover. At one extreme are nerve cells, most of which last a lifetime without replacement. At the other extreme are the cells that line the intestine, which are replaced every few days. Between these extreme there is of course a spectrum of different rates and styles of cell replacement and tissue renewal. Our life depends on these renewal processes. A large dose of ionizing radiation, by blocking cell division, halts renewal.

Many of the differentiated cells that need continual replacement are themselves unable to divide. Red blood cells, surface epidermal cells, and the absorptive and goblet cells of the gut lining are all of this type; also referred as terminally differentiated cells. Replacement for terminally differentiated cells are generated from a stock of proliferating precursor cells, which themselves usually derive from small numbers of more slowly dividing stem cells. The stem cells and proliferating precursors cells are retained in the corresponding tissues along with the differentiated cells. When a stem cell divides, each daughter can either remain a stem cell or go on to become terminally differentiated. The pattern of replacement varies from one stem-cell-based tissue to another. Often, a single type of stem cell gives rise to several types of differentiated progency; the process of blood-cell formation, or hemopoiesis, provides an extreme example of the phenomenon. All of the different cell types in the blood ultimately derive from the same hemopoietic stem cell that normally inhabits the bone marrow.

Embryonic stem cells (ES cells) can be maintained indefinitely in culture and remain capable of differentiating into any cell type in the body. Perhaps one day it may even become possible to grow entire organs from ES cells by recapitulation of embryonic development. There is, however, one major problem associated with the use of ES cells for tissue repair. If the transplanted cells are genetically different from the cells of the patient into whom they are grafted, they are likely to be rejected and destroyed by the immune system.
By nuclear transplantation, personalized ES cells can in principle be produced for any adult, a technique called ‘therapeutic cloning’. In therapeutic cloning only cells are produced; in reproductive cloning a whole new multicellular individual is generated.

Cancer

Foremost among the diseases of tissue renewal is cancer. In Europe and North America, one in four of us will die of cancer. Cancer cells fail to obey the social constraints that normally maintain tissue organization: they proliferate when they should not, survive where they should not, and invade regions that they should keep out of. It is the combination of these features that creates the lethal danger.

Epidemiology has provided strong evidence that the environment plays a part in the causation of most cases of cancer. Although it is still hard to discover which specific factors in the environment or life-style are critical, and many remain unknown, some of them have been identified quite precisely. Obesity, for example, is correlated with an increased cancer risk, and the relationship is suspected to be causal. By far the most important environmental cause of cancer, however, is tobacco-smoking, which is not only responsible for almost all cases of lung cancer, but also raises the incidence of several other cancers, such as those of the bladder.

Cancer is fundamentally a genetic disease: it arises as a consequence of pathological changes in the information carried by DNA. It differs from other genetic diseases in that the mutations underlying cancer are mainly somatic mutations as opposed to germ-line mutations. Most of the identified agents known to contribute to the causation of cancer are mutagens: they cause changes in the nucleotide sequence of DNA. But mutations can also occur spontaneously as a result of fundamental limitations on the accuracy of DNA replication and DNA repair. Nevertheless, it takes more than a single mutation to turn a normal cell into a cancer cell. In fact, cancer cells arise from the accumulation of many mutations in a single somatic cell lineage. And cancer, therefore, is typically a disease of old age.
To be successful, a cancer cell must acquire a whole range of abnormal properties as it evolves. Different cancers require different combinations of properties. Even though, there is a general list of key behaviors of cancer cells that distinguish them from normal cells:

  1. They have a reduced dependence on signals from other cells for their growth, survival, and division. A mutation in a ras gene can, for example, cause an intercellular signal for proliferation to be produced even in the absence of the extracellular signal that would normally be needed to trigger it.
  2. Cancer cells are less prone than normal cells to kill themselves by apoptosis. This is often caused by mutations in genes that regulate the intracellular death program, including the p53 protein. Mutations in the p53 gene, allowing them to survive and divide even when their DNA is damaged.
  3. Unlike most normal human cells, cancer cells can often proliferate indefinitely by reactivating production of the telomerase enzyme that maintains telomere length.
  4. Most cancer cells are genetically unstable, with a greatly increased mutation rate.
  5. Cancer cells are abnormally invasive, and this is often in part because they lack specific cell-adhesion molecules, such as cadherins, that hold normal cells in their proper place.
  6. Cancer cells can often survive and proliferate in foreign tissues to form metastases, whereas most normal cells die when misplaced.

Many diverse types of genes are critical for cancer. In some case, the dangerous mutations are ones that make the affected gene product hyperactive. These mutations have a dominant effect and the mutant gene is called an oncogene; the corresponding normal form of the gene is then called a proto-oncogene. For other genes, the danger lies in mutations that destroy gene function. These mutations are generally recessive and the affected gene is called a tumor suppressor gene. Tumor suppressor genes can sometimes be identified through studies of rare cancer-prone families in which a mutation of one gene copy is inherited.

Colorectal cancer illustrates how loss of a gene can lead to growth of a tumor. Colorectal cancer arises from the epithelium lining the colon and rectum; most cases are seen in old people and do not have any discernible hereditary cause. A small proportion of cases, however, occur in families that are exceptionally prone to the disease and show an early onset. In one set of families, the predisposition to cancer has been traced to an inherited mutation in a DNA repair enzyme. In another class of hereditary colorectal cancer patients, a different mutation is present, leading to a highly distinctive phenotype. The affected individuals develop colorectal cancer in early adult life, and the onset of their disease is foreshadowed by the development of hundreds of thousands of little tumorous growths, called polyps, in the lining of the colon and rectum. The abnormality can be traced to deletion or inactivation of a gene called the adenomatous polyposis coli (APC) gene. Affected individuals inherit one mutant copy of the gene and one normal copy; their cancers arise from cells that can be shown to have undergone a somatic mutation that inactivates the remaining good copy. All this identifies APC as a tumor suppressor gene. When APC is lost, the ‘Wnt pathway’ (which is involved in stimulating cell proliferation in crypts of the gut lining) is hyperactive and the cells proliferate to excess, generating a polyp. Within this growing mass of tissue, further mutations may occur, resulting in invasive cancer.

An understanding of cancer cell biology opens the way to new treatments. At this moment, surgery remains the most effective tactic in many cancer, and surgical techniques are continually improving. Where surgery fails, therapies based on the intrinsic peculiarities of cancer cells can be used. One promising strategy for the future is to block formation of the new blood vessels that normally invade a growing tumor, and so to choke tumor growth by depriving the cells of their blood supply. Another strategy aims to use antibodies that bind to the tumor-specific cell surface proteins; the antibodies can be coupled to toxins or toxin-generating enzymes that will kill the targeted cancer cells.

With our modern understanding of the molecular biology of cancer, we hoop it will be possible to dives effective methods of treatment for a still wider range of forms of cancer.

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