Notes on Chapter 2: Cell Chemistry and Bioenergetics (Key Concepts, Equations, and Connections)

The Chemical Components of a Cell

  • Living organisms are chemical systems governed by chemistry and physics; no “vital force” needed, but life is chemical in nature.
  • Three broad distinctive features of biochemistry:
    • Predominantly carbon-based (organic chemistry).
    • Cells are ~70% water; life hinges on reactions in aqueous solution.
    • Cells are extraordinarily complex; even the simplest cell contains huge polymeric macromolecules whose properties enable growth, reproduction, and life processes.
  • Major point: most carbon atoms in cells are in enormous polymers built from subunits; these macromolecules drive growth, reproduction, and function.
  • The main elements in cells (Figure 2–1) and weights:
    • Four elements (C, H, N, O) make up 96.5% of weight of organisms.
    • Elements are linked by covalent bonds to form molecules; covalent bonds are typically ~100× stronger than thermal energies in cells and are broken mainly in specific reactions.
  • Noncovalent interactions also play crucial roles in binding, recognition, and assembly: electrostatic (ionic), hydrogen bonds, van der Waals, and hydrophobic effects.
  • The chemistry of life is predominantly formed from lighter elements; atomic weights shown reflect common isotopes; C, N, O, H dominate bonding patterns.
  • A cell’s chemistry relies on large polymers whose properties emerge from repeating subunits: monomers link end-to-end to form macromolecules.

Water and the Nature of Biological Interactions

  • Water as solvent is central: reactions in an aqueous environment, with life’s oceanic origins imprinting water’s chemistry on biology.
  • Water structure: each H–O–H is bent; O is highly electronegative, giving water a strong polarity.
  • Hydrogen bonds: attractive interactions between a hydrogen attached to an electronegative atom (donor) and an electronegative atom with a lone pair (acceptor); bonds are weaker than covalent bonds but numerous bonds sum to strong effects.
  • Water forms an extensive hydrogen-bond network; each water molecule can form bonds with multiple neighbors, giving water unique properties (high boiling point, surface tension).
  • Hydrophilic vs hydrophobic: polar or charged molecules interact favorably with water and dissolve (e.g., sugars, DNA, RNA, proteins); hydrophobic molecules (nonpolar, e.g., hydrocarbons) do not dissolve well in water and tend to aggregate.
  • The four major noncovalent attractions that help bring molecules together in cells (Panel 2–3):
    • Electrostatic (ionic) attractions
    • Hydrogen bonds
    • van der Waals attractions
    • Hydrophobic force (driven by water exclusion of nonpolar surfaces)
  • Hydrogen bonds are directional and strongest when atoms align linearly.
  • Polar molecules can act as acids or bases in water through proton transfer and the hydronium/hydroxide equilibrium; pH and buffering are critical for cellular neutrality.
  • Water’s role in acid-base chemistry sets the stage for cellular pH control and buffer systems; pH scale is logarithmic in H3O+ concentration.
  • Important conversions and units:
    • 1 J = energy to move 1 N a distance of 1 m; 1 kJ = 1000 J; 1 kcal = 4.18 kJ; 1 kJ = 0.239 kcal.
    • pH related: extpH=extlog10[extH+].ext{pH} = -\, ext{log}_{10} [ ext{H}^+].
    • Water at neutral pH has [H+] = [OH−] = 10^−7 M.

Small Carbon-Based Molecules: The Four Major Families

  • Cells largely rely on four families of small organic molecules: sugars, fatty acids, nucleotides, and amino acids.
  • These small molecules serve multiple roles:
    • Monomer subunits to build macromolecules (proteins, nucleic acids, polysaccharides).
    • Energy sources and intermediates in metabolism.
    • Some act in more than one role (e.g., sugar as energy source and polymer subunit).
  • Macromolecules are dominant in dry cell mass; small molecules account for a smaller fraction but are chemically related and interconvertible within pathways.
  • Major points about macromolecular synthesis:
    • Macromolecules are polymers formed from monomers via covalent bonds; growth occurs by addition to the chain end in a condensation (water is released).
    • Most polymers are made from a limited set of monomers (e.g., 20 amino acids in proteins).
    • Subunit order (sequence) is precise, enabling a unique function and structure; ordering is controlled by enzymes (7–11 in subsequent chapters).

Macromolecules and the Rules of Polymerization

  • Macromolecules in cells are built from repeating subunits (monomers) via covalent linkages to form polymers:
    • Proteins (amino acids), Nucleic acids (nucleotides), and Polysaccharides (sugars).
  • Polymer growth occurs by condensation reactions; each added monomer causes loss of a water molecule.
  • Polymerization requires energy input; hydrolysis is energetically favorable and often drives polymer breakdown.
  • The polymerization process is not random; subunits are added in a specific, ordered sequence determined by enzymes.
  • The four major small-molecule families are depicted in Figure 2–6 (sugars, fatty acids, nucleotides, amino acids).
  • Macromolecules (proteins, nucleic acids, polysaccharides) are the major dry-mass components and assemble into larger macromolecular machines (e.g., ribosome).

Noncovalent Forces and Macromolecular Structure

  • Noncovalent bonds, though individually weak, collectively endow macromolecules with defined shapes and binding specificities:
    • The same four noncovalent forces previously discussed (electrostatic, hydrogen bonds, van der Waals, hydrophobic expulsion) govern folding and interactions.
  • Role of noncovalent interactions in folding:
    • Folding into a unique, functional conformation relies on multiple weak interactions; the sequence of monomers strongly biases the final fold.
    • Protein folding creates specific surfaces enabling selective binding to other molecules, crucial for catalysis and complex assembly (e.g., ribosome assembly; DNA-protein interactions).
  • The concept of “conformation” and tight binding is explained with examples of macromolecular recognition (Figure 2–3, 2–4).
  • Hydrophobic effect is central to protein folding and membrane formation; nonpolar surfaces avoid water, driving compact structures and membrane assembly.
  • Noncovalent binding creates specificity: number of bonds correlates with binding strength and the possibility of rapid association/dissociation.
  • Folding and binding are not static—binding can be dynamic, enabling catalysis and molecular motors.

Catalysis and the Use of Energy by Cells

  • Living systems maintain order in a universe tending toward disorder (second law of thermodynamics) by continually performing chemical reactions powered by energy input.
  • Enzymes are biological catalysts (mostly proteins; some ribozymes) that accelerate specific reactions, reducing activation energy barriers.
  • Key ideas about enzyme-catalyzed reactions:
    • Enzymes do not change the equilibrium of a reaction; they accelerate both forward and reverse reactions equally, but they steer the pathway by providing a preferred reaction route via active sites.
    • Enzymes are highly specific for substrates and often catalyze only one reaction type; sets of enzymes can channel substrates along defined metabolic pathways.
    • Substrate molecules find enzymes via rapid diffusion and Brownian motion; collisions lead to enzyme–substrate complex formation.
  • Activation energy concept: reactions have an energy barrier; enzymes lower this barrier, dramatically increasing reaction rates (up to 10^14-fold for some reactions).
  • How enzymes couple reactions: exergonic (energetically favorable) reactions can drive endergonic (unfavorable) reactions when linked to a favorable step via shared intermediates, carriers, or metabolic pathways; the coupling makes the overall ΔG negative.
  • The notion of energy transfer: activated carrier molecules store energy from exergonic steps and shuttle it to endergonic biosynthetic steps (e.g., ATP, NADH, NADPH, acetyl CoA, FADH2).
  • Temperature vs enzyme-catalyzed rate: increasing temperature nonselectively speeds all reactions, whereas enzymes provide selective acceleration.
  • Activation energy diagrams illustrate uncatalyzed vs enzyme-catalyzed paths and how catalysts change barriers without altering equilibrium.

The Free Energy and Thermodynamics of Cellular Reactions

  • Free energy (G) concept and the direction of reactions:
    • Reactions proceed spontaneously in the direction that lowers free energy (ΔG < 0).
    • The universe’s disorder is the sum of changes in system (box) and surroundings (sea); ΔSuniverse = ΔSsea + ΔSbox; ΔG is a measure of this overall change.
  • The first and second laws of thermodynamics in biology:
    • 1st law: energy is conserved; it can be transformed but not created/destroyed.
    • 2nd law: systems tend toward higher probability states (greater disorder); entropy increases overall.
  • Definitions and relationships:
    • Enthalpy H = E + PV; heat exchange at constant pressure is h = ΔH; most biological reactions occur with negligible volume change, so ΔH ≈ Δq (heat exchange).
    • Gibbs free energy: G=HTS.G = H - T S. For a reaction, ΔG = ΔH - T ΔS.
    • For reactions in a cellular “box”: ΔG = ΔG° + RT \,
      abla \,
      olinebreak \, frac{[X]}{[Y]} (RT is about
      olinebreak 2.58 kJ mol⁻¹ at 37°C).
    • Standard free-energy change (ΔG°) is defined under standard conditions ([A] = [B] = 1 M). The relationship to the equilibrium constant K is:oxed{ \Delta G = \,oxed{ \Delta G^
      abla}} [Note: the standard form is oxed{ \Delta G^ ext{o} = -RT \, \ln K} or equivalently oxed{ \Delta G^ ext{o} = -RT \, \ln K = - RT (2.303) \, \log K = -5.94 \, \log K ext{ at 37°C}}.]
  • Coupled reactions: the total free energy change of coupled steps is additive:oxed{ \Delta G_ ext{total} = \sumi \Delta Gi }. This allows unfavorable steps to proceed when paired with favorable ones.
  • Equilibrium constant and ΔG° relation for complex reactions: for a reaction aA + bB ⇌ cC + dD, K=[C]c[D]d[A]a[B]bK = \frac{[C]^c[D]^d}{[A]^a[B]^b} and ΔGexto=RTlnK\Delta G^ ext{o} = - RT \, \ln K; in base-10 form, ΔGexto=RTlnK=5.94logK\Delta G^ ext{o} = - RT \,\ln K = -5.94 \, \log K (at 37°C with RT ≈ 2.58 kJ/mol).
  • Practical takeaway: the magnitude of ΔG° reflects intrinsic chemistry; large negative ΔG° means the equilibrium favors products; increasing [X]/[Y] intensifies ΔG in the forward direction until equilibrium is reached.
  • Energetics in biology emphasize that ATP hydrolysis is a major energy source for biosynthesis; typical hydrolysis free energy is in the range: oxed{\Delta G_ ext{hydrolysis} \approx -46 \text{ to } -54 \text{ kJ/mol}}.

Activated Carriers and Energy Currency

  • To couple energetically favorable and unfavorable reactions, cells use activated carrier molecules that store energy in readily transferable bonds:
    • ATP (adenosine triphosphate): primary energy currency; formed by phosphorylation of ADP; hydrolysis to ADP + Pi releases energy used to drive biosynthesis and transport; typical hydrolysis energy cited as ΔGextoexthyd46 to 54 kJ/mol.\Delta G^ ext{o}_{ ext{hyd}} \approx -46 \text{ to } -54 \text{ kJ/mol}.
    • NADH and NADPH: carriers of electrons (hydride transfer, H−) for oxidation-reduction chemistry; NADH mainly in catabolic reactions; NADPH mainly in anabolic (biosynthetic) reactions.
    • Acetyl CoA (acetyl coenzyme A): carries acetyl groups for biosynthesis and oxidation.
    • FADH2: another electron carrier supporting redox reactions.
  • Balance of carriers in cells:
    • The cell maintains a high NAD+/NADH ratio to favor oxidation (accepting electrons) in catabolic pathways; and a high NADP+/NADPH ratio is kept low to favor NADPH as a reducing agent in biosynthesis.
    • Activated carriers diffuse and shuttle energy and chemical groups to where they’re needed, enabling diverse biosynthetic processes.
  • Other activated carriers include biotin (carboxyl transfer), S-adenosylmethionine (methyl transfer), UDP-glucose (glucose transfer), acetyl CoA (acetyl transfer), and more (Table 2–3).
  • ATP synthesis and transfer examples:
    • ATP is formed from ADP + Pi via phosphorylation; energy from ATP hydrolysis can be directly transferred to other molecules via phosphorylation (phosphoester bond formation, or phosphotransfer to substrates).
    • Phosphate transfer reactions can produce high-energy intermediates that drive subsequent steps (e.g., formation of 1,3-bisphosphoglycerate in glycolysis).
  • Two illustrative coupling mechanisms: direct coupling via enzyme-catalyzed steps or indirect coupling via activated carriers; a mechanical analogy (rocks falling powering a paddle wheel) helps visualize how an exergonic step can drive an endergonic one (Figure 2–32).

Synthesis of Biological Polymers

  • Macromolecules are built by repetitive condensation reactions that form polymers from monomers:
    • Proteins: polymerize amino acids via peptide bonds; polymerization is directional (N-terminus to C-terminus) and often the chain grows by head polymerization in which the growing chain carries a high-energy bond that is used for the next addition.
    • Nucleic acids: polynucleotide synthesis uses nucleoside triphosphates; growth can be head (new nucleotide adds to the 3′ end) or tail polymerization depending on mechanism.
    • Polysaccharides: sugar subunits linked by glycosidic bonds; glycogen (branched) vs starch (less branched) storage polysaccharides.
  • Energy coupling in polymer synthesis:
    • Condensation reactions are energetically unfavorable on their own; energy from ATP hydrolysis (or other activated carriers) is used to activate monomers or to form high-energy intermediates that drive polymerization.
    • For proteins and polysaccharides, the final hydrolysis steps are energetically favorable; energy input is required to activate monomers and/or intermediates; the net process is driven by coupling to ATP hydrolysis or other activated carriers (Figure 2–41).
  • General summary of polymerization:
    • Macromolecules form from limited sets of monomers (e.g., 20 amino acids in proteins).
    • Subunits are added in a precise order, with folding driven by noncovalent interactions that stabilize the final three-dimensional conformation.
    • Macromolecules form higher-order assemblies through noncovalent interactions, enabling complex cellular machines (e.g., ribosome).

Why Macromolecules Fold and Bind: Noncovalent Forces in Action

  • The folded structure of a macromolecule is determined by the sequence of monomers and reinforced by multiple noncovalent interactions; this defines the molecule’s shape and binding properties.
  • The four main weak noncovalent interactions remain central:
    • Electrostatic attractions (ionic interactions)
    • Hydrogen bonds
    • Van der Waals attractions
    • Hydrophobic effect (expulsion of nonpolar surfaces from water)
  • Hydrophobic forces: nonpolar surfaces cluster to minimize disruption to the water network; important in protein folding and membrane formation.
  • Noncovalent interactions underlie specific binding necessary for catalysis, signaling, assembly of macromolecular machines, and molecular recognition.
  • Hydration and solvent effects: water competes for hydrogen bonds with many partners; this competition weakens some noncovalent bonds in water but the cumulative effect remains powerful for selectivity and binding.

Cellular Catalysis and Reaction Kinetics

  • Enzymes dramatically accelerate reaction rates by lowering activation barriers; they do not alter the ultimate equilibrium of a reaction.
  • Enzymes provide active sites where substrates bind, forming an enzyme–substrate complex and reducing the energy needed to reach the transition state.
  • Kinetics in cells are driven by diffusion and rapid molecular motions; substrates collide with enzymes, forming transient complexes at high frequencies (often 10^5–10^6 collisions per second per enzyme at typical cellular concentrations).
  • A key concept is that enzymes couple energetically favorable and unfavorable reactions; the overall free energy change is what determines whether a process proceeds.
  • Activation energy diagrams illustrate how enzymes favor particular reaction pathways by lowering barriers; the uncatalyzed path and the enzyme-catalyzed path converge at the same equilibrium point (Figure 2–23).
  • Enzymes are highly selective: a given enzyme typically catalyzes only one reaction, allowing the cell to engineer specific reaction pathways (Figure 2–24).
  • The speed at which enzymes find substrates is aided by the rapid molecular motions (translation, rotation, and vibration) and diffusion; large proteins tumble rapidly, while small molecules diffuse quickly through cytosol.
  • The role of enzymes in energy transduction and metabolism is central: they enable organic molecules to be oxidized in a controlled, stepwise fashion to harvest energy as ATP and activated carriers (e.g., NADH, NADPH).

The Energetics of Cellular Reactions: Free Energy and Equilibrium

  • The direction of a reaction depends on the sign of ΔG:
    • Energetically favorable (spontaneous) if ΔG < 0; unfavorable if ΔG > 0; at equilibrium ΔG = 0.
  • Concentration dependence: ΔG = ΔG° + RT ln([X]/[Y]); changing concentrations shifts the direction of the reaction.
  • Standard free-energy change ΔG° depends only on intrinsic properties of reactants at standard conditions; it relates to the equilibrium constant as:oxed{ \Delta G^ ext{o} = - RT \, \ln K }. In base-10 form at 37°C: oxed{ \Delta G^ ext{o} = -5.94 \, \log K }.
  • The concept of activation energy: many biological reactions require a kinetic kick; enzymes lower the activation energy, enabling reactions to occur at physiological temperatures.
  • The concept of energy coupling: energetically favorable reactions can power energetically unfavorable ones, by tying the two together and sharing energy via intermediates or carriers; the overall ΔG must be negative for the coupled process to proceed.

Activation Carriers: ATP, NADH, NADPH, and More

  • ATP is the primary activated carrier used to drive biosynthesis and work in cells; hydrolysis of the terminal phosphate yields significant energy to drive endergonic steps.
  • NADH and NADPH are electron carriers; NADH is primarily associated with catabolic energy production; NADPH is primarily used for anabolic biosynthesis.
  • The balance between NAD+/NADH and NADP+/NADPH is carefully regulated to direct electrons to the correct pathway (catabolic vs anabolic).
  • Other activated carriers include acetyl CoA (acetyl groups), FADH2 (electrons and hydrogens), coenzyme A derivatives, biotin-linked carboxyl groups, S-adenosylmethionine (methyl groups), UDP-glucose (glucose transfer), and more (Table 2–3).
  • The energy from ATP hydrolysis (ΔG ≈ −46 to −54 kJ/mol) can be used directly or via intermediate high-energy bonds to drive biosynthetic reactions.
  • ATP can energize biosynthesis by forming high-energy intermediates or by phosphate-transfer reactions (Figure 2–34).
  • The activation of biosynthetic steps often involves ATP-driven formation of an activated intermediate, which then reacts with a substrate to form a bond (e.g., A–H + B–OPO3 → A–B + Pi).

The Synthesis of Biological Polymers

  • Biological polymers (proteins, nucleic acids, polysaccharides) are formed by condensation reactions driven by activated carriers; hydrolysis reverses polymer formation.
  • Synthesis of nucleic acids (RNA/DNA): nucleoside triphosphates drive polynucleotide synthesis via phosphodiester bonds; two ATP equivalents typically activate a monomer (formation of a high-energy intermediate) before insertion.
  • Proteins and polysaccharides also rely on ATP hydrolysis to power activation steps that enable polymerization.
  • The two modes of polymerization:
    • Head polymerization: the growing polymer chain carries the reactive bond for the next addition; common for proteins and fatty acids.
    • Tail polymerization: the monomer provides its own reactive bond for its addition; typical for DNA/RNA and some polysaccharides.
  • Energy budgets for polymer synthesis emphasize that though condensation is energetically unfavorable, coupling to ATP hydrolysis and other activated carriers makes polymerization thermodynamically favorable overall.

Glycolysis, Fermentation, and Cellular Energy from Sugars

  • Glycolysis is the central ATP-producing pathway in the cytosol; it converts one glucose (6 carbons) into two pyruvates (3 carbons each) with a net gain of 2extATP2 ext{ ATP} and 2extNADH2 ext{ NADH} per glucose, without requiring O2.
  • Pathway outline (10 steps): glucose → glucose-6-phosphate → fructose-6-phosphate → fructose-1,6-bisphosphate → glyceraldehyde-3-phosphate (G3P) × 2 → 1,3-bisphosphoglycerate → 3-phosphoglycerate → 2-phosphoglycerate → phosphoenolpyruvate → pyruvate; energy investments occur in early steps; energy payoffs occur in steps 6 and 7.
  • Key enzyme-catalyzed steps producing energy:
    • Step 6: G3P is oxidized; NAD+ is reduced to NADH; a high-energy acyl phosphate is formed on glyceraldehyde-3-phosphate–dehydrogenase complex (step 6).
    • Step 7: The high-energy phosphate is transferred to ADP to form ATP (phosphoglycerate kinase step).
    • Net result of steps 6 and 7: generation of NADH and ATP from oxidation of glyceraldehyde-3-phosphate; overall glycolysis yields: 2extATPext(net)2 ext{ ATP} ext{ (net)} and 2extNADH2 ext{ NADH} per glucose.
  • Fermentation (anaerobic): In the absence of oxygen, pyruvate is reduced to lactate (in animals) or converted to ethanol and CO2 (in yeasts), regenerating NAD+ so glycolysis can continue. These pathways allow ATP generation without oxidative phosphorylation but yield less total energy.
  • If oxygen is present, pyruvate enters mitochondria for aerobic oxidative metabolism: pyruvate → acetyl-CoA → citric acid cycle; NADH/FADH2 produced feed into oxidative phosphorylation to generate most ATP.
  • Overall energy yield from glucose oxidation (glycolysis + TCA + oxidative phosphorylation) is about 30extATPperglucose30 ext{ ATP per glucose} in many eukaryotic cells, though exact numbers vary by tissue and shuttle mechanisms.
  • The glucose-to-CO2/H2O energy transfer occurs via stepwise oxidation that stores energy first in ATP and NADH; the coupling to NADH and subsequent oxidative phosphorylation yields the majority of ATP.
  • A comparison of direct burning of glucose with stepwise cellular oxidation highlights that enzymes allow controlled, energy-efficient extraction of energy rather than a single, explosive release.
  • Glycolysis as a model of enzyme-coupled energy harvesting: steps 6–7 illustrate how oxidation energy can be stored in an activated intermediate and then used to form ATP, a classic example of coupling energetically favorable and unfavorable steps (see Figure 2–48).

Glucose Storage and Plant/Fatty Acid Storage in Cells

  • Organisms store energy for times of need: glycogen (short-term storage in animals and plants) and fats (long-term energy store).
  • Glycogen: highly branched glucose polymer stored in liver and muscle; breakdown yields glucose-1-phosphate, then glucose-6-phosphate for glycolysis.
  • Fat storage: triacylglycerols (triglycerides) are energy-dense and stored in adipocytes; oxidation of fat yields more energy per gram than glycogen and fat’s water content is low, making it an efficient store.
  • Plants store energy as starch and fats; chloroplasts produce sugars via photosynthesis and convert some sugars to fats and starch; starch granules accumulate in chloroplasts.
  • In seeds, energy storage is critical for germination; seeds contain large stores of fats and starch which feed growing embryos.
  • In animals, after a meal, energy comes from sugars; glycogen stores replenish; during fasting, fatty acids become the main energy source; fatty acids are mobilized from adipose tissue, transported via blood, and oxidized in mitochondria.
  • The oxidation of sugars and fats both converge on acetyl-CoA, which enters the citric acid cycle in mitochondria for maximal energy harvest.

The Citric Acid Cycle and Oxidative Phosphorylation

  • The citric acid cycle (Krebs cycle) is central to aerobic metabolism, oxidizing acetyl-CoA to CO2 while generating high-energy carriers (NADH, FADH2) and GTP (or ATP in some organisms).
  • Per turn, the cycle generates: 3 NADH, 1 FADH2, and 1 GTP (or ATP) and releases 2 CO2; oxaloacetate is regenerated to continue the cycle.
  • Each glucose (which yields 2 acetyl-CoA) drives two turns of the cycle, giving total outputs of 6 NADH, 2 FADH2, 2 GTP, and 4 CO2 per glucose.
  • The NADH and FADH2 produced feed the electron transport chain (ETC) in the inner mitochondrial membrane, where electrons are transferred through a series of carriers to O2, pumping protons and generating a proton-mmotive force.
  • Oxidative phosphorylation uses the proton gradient to drive ATP synthesis via ATP synthase; this is the major source of ATP in aerobic respiration.
  • The complete oxidation of one glucose molecule (to CO2 and H2O) yields about 30 ATPs, with substantial ATP production arising from NADH/FADH2 oxidation in the ETC; glycolysis yields 2 ATP directly, whereas the majority of ATP comes from the ETC and oxidative phosphorylation.
  • The oxygen we breathe is required as the final electron acceptor in the ETC; water is produced as a byproduct when O2 accepts electrons.

The Nitrogen and Sulfur Cycles in Biology

  • Nitrogen metabolism: nitrogen fixation converts atmospheric N2 into biologically usable forms; essential for amino acids and nucleotides; vertebrates obtain nitrogen mainly from dietary proteins and nucleic acids.
  • Amino acids: about half of the 20 amino acids are essential for vertebrates; plants synthesize them, but vertebrates must obtain essential amino acids from diet.
  • Nucleotides: nucleotides required for RNA and DNA can be synthesized in cells; no essential nucleotides must be supplied directly; the ribose/deoxyribose sugar is derived from glucose.
  • Nitrogen and sulfur atoms are incorporated into biomolecules through various pathways; nitrogen fixation and assimilation cycles continually circulate nitrogen between organisms and their environment.
  • Sulfur metabolism: sulfur is required for methionine and cysteine; sulfate must be reduced to sulfide in some organisms, allowing synthesis of sulfur-containing biomolecules; humans obtain sulfur via diet.

The Proteins: Structure, Folding, and Function

  • Proteins are the most abundant dry mass in cells and are responsible for a wide range of functions: enzymes, structural components, molecular motors, channels/pumps in membranes, signaling and regulation, immunity, etc.
  • Proteins are polymers of 20 standard amino acids linked by peptide (amide) bonds; the sequence determines the protein’s structure and function.
  • The amino terminus (N-terminus) and carboxyl terminus (C-terminus) mark the ends of the polypeptide; sequences are written N→C.
  • The peptide bond is planar and does not rotate; rotation occurs about the bonds adjacent to the peptide bond, notably the N–Cα and Cα–C bonds; this gives freedom to adopt many conformations.
  • Amino acid side chains vary greatly in chemical properties: acidic, basic, uncharged polar, and nonpolar; these properties influence folding, stability, and interactions.
  • The twenty standard amino acids have specific properties and identities (see Panel 3–1 and Figure 3–2).
  • Optical isomers: all protein amino acids are L-stereoisomers, which influences how they interact in biomolecules.
  • Protein folding is driven by noncovalent interactions among backbone atoms and side chains: hydrogen bonds, electrostatic interactions, van der Waals interactions, and hydrophobic effects (Figure 3–4 summarizes how these forces cooperate).
  • The three-dimensional shape of a protein is stabilized by cumulative noncovalent bonds; many simultaneous weak interactions produce a strong overall stabilization, supporting a stable, functional conformation.
  • The Ramachandran plot describes allowed combinations of backbone φ (phi) and ψ (psi) angles for amino acid residues; steric constraints limit feasible conformations and define secondary structure motifs.
  • Proteins also assemble into macromolecular machines via noncovalent interactions; folding and assembly create functional surfaces for catalysis, signaling, and mechanical work.
  • Disulfide bonds between cysteine residues can stabilize protein structure, especially in extracellular environments; these are covalent links that contribute to stability.

The Essential Amino Acids and Protein Architecture

  • The nine essential amino acids for humans cannot be synthesized and must be supplied by the diet: Threonine, Methionine, Lysine, Valine, Leucine, Isoleucine, Histidine, Phenylalanine, Tryptophan (Figure 2–62).
  • The 20 canonical amino acids fall into categories by side-chain properties: nonpolar, polar uncharged, acidic, and basic; these properties guide folding, interactions, and enzyme active sites (Figure 3–2).
  • The amino acid side chains confer unique chemistries that enable a protein’s function; their spacing and orientation in the polypeptide backbone determine the folded state and binding properties.
  • An example of the role of histidine in catalysis highlights how enzyme active-site chemistry depends on pH and the protonation state of functional groups in the active site (Question Q2–1 in end-of-chapter problems).

The Organization and Regulation of Metabolism

  • Cells live in a dynamic, highly regulated metabolic network; thousands of reactions and many enzymes operate in concert to maintain energy balance and biosynthesis.
  • Metabolic pathways are organized into three broad zones:
    • Catabolic pathways (break down nutrients to generate energy and building blocks).
    • Anabolic pathways (biosynthetic routes that utilize energy to build macromolecules).
    • Intermediates of catabolic pathways serve as substrates for biosynthesis, illustrating the interconnected nature of metabolism.
  • The energy flow in metabolism: food molecules are oxidized to CO2 and H2O, releasing energy; part of this energy is captured in ATP and other carriers and used to drive biosynthesis, while part is lost as heat.
  • The carbon cycle and biogeochemical cycles interplay with metabolism: photosynthesis fixes carbon and releases O2; respiration and fermentation release CO2 back into the environment; this interdependence reflects life’s integration with planetary chemistry.
  • Metabolic regulation is complex and robust: cells balance energy production and consumption; perturbations trigger adaptive responses to reestablish homeostasis; regulation often occurs at key control points (e.g., allosteric regulation of enzymes).

End-of-Chapter Problems and Real-World Connections

  • The chapter poses problems that integrate concepts: pH calculations, diffusion, kinetics, and energy calculations; these reinforce quantitative intuition about cellular chemistry.
  • Broader questions raised include origins of energy transduction, minimal components for a living cell, and possibilities for other life chemistries; these prompt thinking about the universality and variability of biochemistry.
  • Real-world relevance: chloroplasts, mitochondria, glycogen, glycogenolysis, gluconeogenesis, fat storage, and lipid membranes are all tied to cellular energy balance and the structure of life.
  • The big picture: life requires a constant energy input to create ordered structures, with heat released to the environment ensuring the universe’s overall entropy increases; biology achieves this through tightly coupled, regulated metabolic networks.

Key Equations and Quantitative Details to Memorize

  • Water and pH:
    • extpH=log10[H+].ext{pH} = -\log_{10}[\text{H}^+].
    • Pure water: [H+] = [OH−] = 10^{−7} M.
  • Free energy and equilibrium:
    • ΔG=ΔG+RTln([X][Y]).\Delta G = \Delta G^\circ + RT \ln\left(\frac{[X]}{[Y]}\right).
    • At equilibrium: ΔG=0ΔG=RTlnK.\Delta G = 0 \quad\Rightarrow\quad \Delta G^\circ = -RT \ln K.)
    • In base-10 form: ΔG=RTlnK=5.94logK(at 37°C).\Delta G^\circ = -RT \ln K = -5.94 \log K\quad\text{(at 37°C)}. (With RT2.58 kJ/molRT\approx 2.58\text{ kJ/mol}.)
  • Activation energy and catalysis:
    • Enzymes lower activation barriers, increasing reaction rates without changing equilibrium.
  • Coupled reactions:
    • ΔG<em>total=</em>iΔGi.\Delta G<em>{total} = \sum</em>i \Delta G_i.
  • ATP hydrolysis energy:
    • ΔGhydrolysis  46 to 54  kJ/mol.\Delta G_{hydrolysis} \approx -\;46 \text{ to } -54\; \text{kJ/mol}.
  • Glycolysis yields per glucose:
    • Net: 2 ATP2\text{ ATP} and 2 NADH2\text{ NADH} (glucose → 2 pyruvate).
    • Steps 6–7 store energy as NADH and ATP in a coupled fashion: the net ΔG for steps 6–7 is negative (≈ −12.5 kJ/mol for the combined process).
  • Citric acid cycle per turn:
    • Produces 3  NADH,3\; NADH, 1  FADH2,1\; FADH_2, and 1  GTP1\; GTP (or ATP); per glucose (two turns) double these amounts.
  • ATP as energy currency and its transfer:
    • ATP hydrolysis to ADP + Pi provides energy for biosynthesis or work; phosphate transfer to substrates forms high-energy intermediates.
  • Synthesis of polymers (summary): energy from nucleoside triphosphate hydrolysis activates monomers, enabling condensation into polymers (proteins, nucleic acids, polysaccharides).

References to Foundational Concepts

  • Thermodynamics as the backbone of metabolism: energy transduction, heat release, entropy increases, and the central role of free energy in driving cellular processes.
  • The link between structure and function: a protein’s function is determined by its folded structure, which arises from its amino acid sequence and the ensemble of noncovalent bonds that stabilize it.
  • The integration of energy metabolism with biosynthesis underpins growth and reproduction in all living systems, with energy carriers acting as the currency of cellular life.