BIOSCI 106 Lecture 1

Course Logistics & Pep Talk
  • Initial reassurance: course has a 93%93\% overall pass rate; laboratories have a 98%98\% pass rate with an average mark of 91%91\% – “very passable, don’t panic.”

  • First two modules are chemistry-heavy; class contains students with widely different science backgrounds (some strong in chemistry, others in biology/physics).
    • Catch-up tools provided; staff encourage you to “always tell us” if you struggle – help is available.

  • Class representative needed for both morning and afternoon streams (announcement by Julie).

Support & Extra Resources
  • “Diagnostic Quiz” (≈25 Qs) covers very basic chemistry/biology to locate knowledge gaps; no marks attached; immediate feedback with explanations.

  • Additional reading & even a (discouraged) research paper link for the curious.

  • Module pages:
    • Slides (pre-lecture + updated post-lecture)
    • Comprehensive worksheet for entire section (includes functional groups, protein structure, etc.)
    • Extra background materials appear in an “Additional Stuff” folder after first week.
    • Discussion notes + worksheet answers released ≈2–2.5 wks before test.

  • Weekly online quizzes: unlimited attempts, only best 10 count toward grade. Some quiz items require worksheet prep.

  • Tutorial session still to be scheduled.

  • Lecture recordings: morning session posted when complete; if morning overruns, afternoon version (faster, “gets act together”) is uploaded by 9 p.m.

Big Picture Questions & Learning Objectives
  • Lecture theme: “Aliens like us – a 14 billion-year history of biochemistry.”

  • Guiding questions:
    • Are we alone?
    • What evidence would we seek on Mars?
    • Would aliens look/biochemically behave like us?

  • Formal objectives

    1. Argue that biochemistry is governed by universal physical laws.

    2. Outline a plausible origin for chemical elements and, later, biological molecules.

    3. Explain why biology must be efficient and how modular evolution achieves that.

Key Chemical Vocabulary (must know)
  • Element: pure substance of one atom type.

  • Molecule: ≥2 atoms bonded.

  • Monomer → Polymer (Residues): Small repeating unit incorporated into biopolymers; once linked, each unit is called a residue.

  • Functional group: specific atom cluster conferring predictable chemical behavior (e.g., hydroxyl –OH–OH, carboxyl –COOH–COOH, amine –NH<em>2–NH<em>2, phosphate –PO</em>43−–PO</em>4^{3-}).

Origin of the Elements (14 Ga ➜ Present)
  1. ∼14 Ga\sim14\,\text{Ga} : Big Bang → only H2H_2 & HeHe.

  2. Gas clouds condense → 1st-generation stars.

  3. Stellar fusion under high heat/pressure forges heavier nuclei (C,N,O,P,S,C, N, O, P, S, metals…).

  4. Supernova explosions scatter elements across space.

  5. Dust & gas reconsolidate → 2nd-generation stars (our Sun) and planets; Earth forms in habitable zone.

Periodic Table of Life (textbook graphic)
  • Tier-1 “bulk” atoms: H,C,N,OH, C, N, O (+ P,SP, S).
    • Abundance correlates with ability to form strong, versatile covalent bonds.
    • HH and OO dominant due to prevalence of water (H2OH_2O ~90 % of human body mass).

  • Tier-2/3/4 trace atoms (e.g., Na,K,Ca,Mg,Fe,Cu,Zn,CrNa, K, Ca, Mg, Fe, Cu, Zn, Cr) enable catalysis, electron transfer, signalling; some are toxic in large doses (e.g., chromium).

Central Role & Geometry of Carbon
  • Valence = 4 → can create single, double, or triple bonds; scaffold for complex, diverse structures.

  • Typical geometries
    • Tetrahedral: 109.5∘109.5^{\circ}
    • Trigonal planar: 120∘120^{\circ}
    • Linear: 180∘180^{\circ}

  • Example drug molecule displayed (anticancer candidate) illustrates mixture of C–C single/double/triple bonds with hetero-atom decorations (N, O, S) for functional diversity.

Requirements for the Emergence of Life on Early Earth (≈4 Ga)
  1. Liquid water – universal solvent, medium for reactions.

  2. Simple reducing gases: CH<em>4,NH</em>3,H2,CO,CH<em>4, NH</em>3, H_2, CO, etc.

  3. Energy source – lightning, UV, geothermal/volcanic heat (→\text{→} electrical discharge).

  4. Reducing atmosphere (very little O2O_2) – prevents oxidative destruction, facilitates bond formation.

Laboratory Test of the Hypothesis: Miller–Urey (1953)
  • Apparatus: boiling flask (water steam) → gas chamber containing the reducing mix CH<em>4,NH</em>3,H<em>2,H</em>2O{CH<em>4, NH</em>3, H<em>2, H</em>2O} → continuous electrical spark (E≈60 000 V)\big(E \approx 60\,000\,\text{V}\big) → condenser → aqueous “primordial soup” trap.

  • Results: within a week produced a rich mixture of organic molecules, notably ALL 20 proteinogenic amino acids plus several non-natural ones.

  • Later variants (2007 re-analysis, phosphate-buffered systems) also yield nucleobases and simple sugars.

  • Demonstrates plausibility of prebiotic synthesis without enzymes.

Modularity & Biological Efficiency
  • Building macromolecules atom-by-atom would exceed the universe’s age; evolution solved this via prefabricated parts (monomers) — analogous to shipping-container architecture.

  • Four major macromolecule classes

    1. Polypeptides (proteins) – polymers of amino-acid residues.

    2. Polynucleotides (DNA/RNA) – polymers of nucleotide residues.

    3. Polysaccharides (cellulose, glycogen) – polymers of monosaccharide residues.

    4. Lipids – do not polymerise but self-assemble into membranes/compartments (critical for cellular life).

  • Polymer formation mechanism: condensation (dehydration) reaction → monomer₁ + monomer₂ →\rightarrow polymer + H2OH_2O.
    • Same chemical logic across proteins (peptide bond), nucleic acids (phosphodiester bond), carbohydrates (glycosidic bond).

Key Bond & Functional Examples
  • Peptide bond:  –C(O)NH–\mathrm{\ –C(O)NH–} link between amino-acid –COOH–COOH & –NH2–NH_2.

  • Glycosidic bond in cellulose: β (1→4)\beta\,(1\rightarrow4) linkage between glucose residues.

  • Phosphodiester bond in DNA: –PO42−\mathrm{–PO_4^{2-}} bridges 3′3'-OH to 5′5'-OH of adjacent sugars.

Functional-Group Recognition vs Memorisation Philosophy
  • Course will provide structural figures in assessments; emphasis on interpreting chemical behavior (polarity, hydrogen-bonding, hydrophobicity, acidity/basicity, aromaticity) rather than rote name recall.
    • Eg. Recognise tyrosine side chain: aromatic ring = hydrophobic, –OH–OH can H-bond.

Water – Why It Matters (worksheet pp. 18–19)
  • High dielectric constant: dissolves ions, stabilises charges.

  • Cohesion & adhesion: support capillary action, blood flow.

  • High specific heat & heat of vaporisation: thermal buffering.

  • Participates directly in hydrolysis/condensation.

Searching for Extraterrestrial Life
  • Mars rovers seek evidence of past liquid water, organic molecules, and redox-active minerals rather than “little green heads.”

  • If life is elsewhere, expectation: carbon-based chemistry operating in aqueous environments, using proteins (or analogues) for catalysis, nucleic-acid-like polymers for information, lipid-like assemblies for compartmentalisation, and energy currencies analogous to ATP.

Class Poll & Humour Highlights
  • Majority believe aliens exist; mixed views on similarity to humans. Answers ranged from serious (shared carbon chemistry) to comedic (Mark Zuckerberg cameo, licking communication, fear of POPHL 111).

Take-Home Messages
  • The laws of chemistry/physics are universal, hence biochemistry should be similar everywhere (universality principle).

  • Stellar evolution supplies the elemental toolkit; prebiotic chemistry can spontaneously build life’s monomers under plausible early-Earth conditions.

  • Efficiency via modularity is essential; life constructs complexity by linking ready-made parts.

  • Studying functional groups, reaction mechanisms, and structure–function relationships is far more valuable than memorising molecule names.

  • You are literally “made of stardust” – every atom in your body was forged in ancient stars, a reminder of our cosmic connection.

“Fear nothing. You have a little piece of stardust in you – every single one of you.” – Lecture closing quote

Exam & Study Tips (implicit from lecture)
  • Do diagnostic quiz to pinpoint weak chemistry areas early.

  • Use worksheet problems both during and after lectures; some quiz items rely on them.

  • Focus revision on:
    • Recognising bond types/angles, functional groups, condensation vs hydrolysis.
    • Explaining why certain atoms dominate biomolecules.
    • Applying the universality argument to hypothetical extraterrestrial scenarios.

  • Expect a few more mid-semester test questions from Lecture 1 this year – easy marks if concepts above are clear.