BIOSCI 106 Lecture 1
Course Logistics & Pep Talk
Initial reassurance: course has a overall pass rate; laboratories have a pass rate with an average mark of – “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
Argue that biochemistry is governed by universal physical laws.
Outline a plausible origin for chemical elements and, later, biological molecules.
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 , carboxyl , amine , phosphate ).
Origin of the Elements (14 Ga ➜ Present)
: Big Bang → only & .
Gas clouds condense → 1st-generation stars.
Stellar fusion under high heat/pressure forges heavier nuclei ( metals…).
Supernova explosions scatter elements across space.
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: (+ ).
• Abundance correlates with ability to form strong, versatile covalent bonds.
• and dominant due to prevalence of water ( ~90 % of human body mass).Tier-2/3/4 trace atoms (e.g., ) 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:
• Trigonal planar:
• Linear: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)
Liquid water – universal solvent, medium for reactions.
Simple reducing gases: etc.
Energy source – lightning, UV, geothermal/volcanic heat ( electrical discharge).
Reducing atmosphere (very little ) – 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 → continuous electrical spark → 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
Polypeptides (proteins) – polymers of amino-acid residues.
Polynucleotides (DNA/RNA) – polymers of nucleotide residues.
Polysaccharides (cellulose, glycogen) – polymers of monosaccharide residues.
Lipids – do not polymerise but self-assemble into membranes/compartments (critical for cellular life).
Polymer formation mechanism: condensation (dehydration) reaction → monomer₁ + monomer₂ polymer + .
• Same chemical logic across proteins (peptide bond), nucleic acids (phosphodiester bond), carbohydrates (glycosidic bond).
Key Bond & Functional Examples
Peptide bond: link between amino-acid & .
Glycosidic bond in cellulose: linkage between glucose residues.
Phosphodiester bond in DNA: bridges -OH to -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, 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.