Lecture 2 - Nature of science Chemistry of life

Introduction to the Molecular Understanding of Life (BIOL141)

  • The nature of science in biology, focusing on the chemical basis of life.

Learning Objectives

  • Facts, Laws, Theories, and Hypotheses: Understand their definitions and differences.

  • Atomic and Molecular Structure: Understand atoms, ions, and molecules, including determining valence.

  • Chemical Bonds: Differentiate between polar covalent, nonpolar covalent, and ionic bonds; predict bonding between elements.

  • Hydrogen Bonding: Describe how hydrogen bonding leads to unique properties of water.

  • pH Understanding: Explain and calculate pH and H+ concentration.

  • Stanley Miller’s Experiment: Know its significance to prebiotic atmospheric chemistry and the origin of life.

  • Wogan et al. Model (2023): Understand its relevance to Stanley Miller's experiment.

The Process of Science

Facts, Hypotheses, Theories, and Laws

  • Fact: A strongly supported observation accepted as true in science but without absolute certainty.

  • Hypothesis: A testable explanation for an observation.

  • Scientific Theory: A well-substantiated explanation based on evidence and repeatedly tested through experimentation.

  • Scientific Law: Describes natural phenomena that consistently occur under certain conditions.

Today's Roadmap

  • Overview of Chemistry's Role in Life: Examining the structure of atoms, ions, and molecules and how chemical reactions occur.

  • Carbon’s Role: Studying how the unique properties of carbon underpin the evolution of life.

  • Unique Properties of Water: Examining how water's properties influence life.

Atomic Structure and Electron Configuration

Diagrams of Atoms

  • Basic atomic components: protons (+), neutrons (neutral), electrons (–).

  • Illustrate various elements such as Hydrogen (H) and Carbon (C).

Electron Shells

  • The valence shell is the outermost electron shell, determining chemical bonding.

  • Valence indicates the number of unpaired electrons in the valence shell.

Chemical Bonds

Covalent Bonds

  • A covalent bond forms when outer-shell electrons are shared between atoms.

  • Example: H2 molecule with two shared electrons; stability occurs when valence shells are full.

Types of Covalent Bonds

  • Polar Covalent Bonds: Electrons are not shared equally; e.g., water (H2O) exhibits partial charges.

  • Nonpolar Covalent Bonds: Electrons are shared equally; e.g., H2 molecule.

Ionic Bonds

  • Formed through electron transfer between atoms, resulting in charged ions (cations and anions).

  • Sodium chloride (NaCl) is an example where sodium (Na+) and chloride (Cl–) ions form a crystal lattice.

Polar vs Nonpolar vs Ionic Bonds

  • Nonpolar Covalent: No charge on atoms; equal sharing of electrons (e.g., Methane, CH4).

  • Polar Covalent: Partial charges exist due to uneven sharing (e.g., Water, H2O).

  • Ionic: Full charges on atoms through electron transfer (e.g., Sodium Chloride).

Unique Properties of Water

Hydrogen Bonds

  • Water is polar; hydrogen bonds form when hydrogen is attracted to electronegative atoms (O, N, F).

  • Hydrogen bonds result in high boiling points and unique properties such as high surface tension.

Cohesion and Adhesion

  • Cohesion: Water molecules stick to each other due to hydrogen bonding.

  • Adhesion: Water molecules stick to other substances (e.g., glass), facilitating capillary action.

Density of Water

  • Ice is less dense than liquid water due to its crystal lattice structure, allowing it to float.

pH in Biology

  • pH Scale: Indicates acidity or alkalinity; calculated as pH = -log[H+].

  • Example: Neutral pH for pure water is 7.

Acid and Base Reactions

  • Acids produce protons (H+) in solutions; bases neutralize acids by acquiring H+.

  • Strong acids like HCl dissociate completely in water, affecting pH significantly.

Chemical Evolution and Early Life

Stanley Miller’s Experiment (1954)

  • Hypothesis: Chemical evolution of organic molecules simulates early-Earth conditions.

  • Findings: Organic compounds like amino acids formed from simple molecules energized by kinetic energy.

Wogan et al. (2023) Model

  • Suggests an iron-rich asteroid could have created a prebiotic atmosphere conducive to complex molecule formation.

Reminders

  • Homework due: Mastering by Sunday 11:59pm.

  • Pre-lab participation required before discussions next week.

  • Reading quizzes are scheduled prior to every class.