BackWater and Carbon: The Chemical Basis of Life (Chapter 2 Study Notes)
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Water and Carbon: The Chemical Basis of Life
Introduction to Chemical Evolution
Chemical evolution is the leading explanation for the origin of life on Earth. It describes the process by which simple molecules formed increasingly complex carbon-containing substances, eventually leading to molecules capable of self-replication and the transition from chemical to biological evolution.
Chemical evolution: Formation of complex molecules from simpler ones, setting the stage for life.
Biological evolution: Began when molecules could replicate, become metabolically active, and acquire membranes, fulfilling the five characteristics of life.
2.2 Properties of Water and the Early Oceans
Water as the Basis of Life
Water is essential for life, making up about 75% of a cell's mass. Its unique properties as a solvent facilitate the chemical reactions necessary for life.
Solvent: The substance in which solutes dissolve to form a solution.
Substances are more likely to react when dissolved in water.
Structural Properties of Water
Water's structure gives rise to its unique chemical and physical properties.
Small molecular size
Bent shape
Highly polar covalent bonds
Overall polarity
Covalent and Ionic Bonding
Covalent bonds: Atoms share electrons (e.g., two hydrogen atoms form H2 by sharing electrons).
Ionic bonds: Formed when one atom donates an electron to another, resulting in oppositely charged ions (e.g., NaCl).
Polarity and Hydrogen Bonding
Water is polar: Oxygen has a partial negative charge, hydrogen has a partial positive charge.
Hydrogen bonds form between the partial charges of water molecules, contributing to water's unique properties.
Water as an Efficient Solvent
Hydrophilic molecules: "Water-loving"; ions and polar molecules that dissolve in water due to interactions with water's partial charges.
Hydrophobic molecules: "Water-fearing"; uncharged and nonpolar compounds that do not dissolve in water. They interact via hydrophobic interactions and van der Waals forces.
Cohesion, Adhesion, and Surface Tension
Cohesion: Attraction between like molecules (e.g., water molecules stick together due to hydrogen bonds).
Adhesion: Attraction between unlike molecules (e.g., water adheres to glass).
Surface tension: Cohesive force at the surface of a liquid, making water surfaces act like elastic membranes.
Density of Water
Water is denser as a liquid than as a solid due to the open crystal structure of ice, which is why ice floats.
Ice forms an insulating layer on water surfaces, protecting aquatic life in cold environments.
Water's Capacity for Absorbing Energy
Specific heat: The energy required to raise the temperature of 1 gram of a substance by 1°C. Water has a high specific heat due to hydrogen bonding.
Heat of vaporization: The energy required to convert 1 gram of a substance from liquid to gas. Water's high heat of vaporization explains why sweating cools the body.
The Role of Water in Acid-Base Chemical Reactions
Acids, Bases, and pH
Acids: Substances that donate protons (H+) and increase hydronium ion concentration ().
Bases: Substances that accept protons and decrease hydronium ion concentration.
pH: Logarithmic scale expressing proton concentration in solution.
Acids have pH < 7; bases have pH > 7; neutral solutions have pH ≈ 7 (e.g., inside living cells).
Buffers: Compounds that minimize changes in pH, helping maintain homeostasis.
2.3 Chemical Reactions, Energy, and Chemical Evolution
Origins of Chemical Evolution
Atmosphere hypothesis: Early Earth's atmosphere contained water vapor, CO2, N2, and small amounts of H2 and CO.
Hydrothermal vent hypothesis: Deep-sea vents provided heat, gases, and reactive minerals for chemical evolution.
Spontaneity of Chemical Reactions
Spontaneous reactions proceed without continuous external energy.
Two key factors for spontaneity:
Products have lower potential energy than reactants.
Products are less ordered (higher entropy) than reactants.
Entropy (): A measure of disorder in a system.
2.4 Investigating Chemical Evolution
Stanley Miller's Experiment
Tested whether complex organic compounds could be synthesized from simple molecules in Earth's early atmosphere.
Used heat and electrical sparks to simulate early Earth conditions.
Produced amino acids, the building blocks of proteins, demonstrating that chemical evolution is plausible under prebiotic conditions.
2.5 Life is Carbon Based
Importance of Carbon
Carbon is the backbone of almost all biological molecules (except water).
Forms four covalent bonds, allowing for a variety of molecular shapes and complexity.
Organic compounds: Molecules containing carbon bonded to other elements, with diverse structures due to single and double bonds.
Functional Groups in Organic Molecules
Amino groups (–NH2): Act as bases, attract protons.
Carboxyl groups (–COOH): Act as acids, donate protons.
Carbonyl groups (–CO): Sites for linking molecules into more complex compounds.
Hydroxyl groups (–OH): Act as weak acids.
Phosphate groups (–PO4): Carry two negative charges.
Sulfhydryl groups (–SH): Form disulfide bonds, stabilizing protein structure.
Macromolecules and Polymerization
Macromolecules: Large molecules made of smaller subunits (monomers) joined by polymerization.
Condensation (dehydration) reactions: Link monomers, releasing water.
Hydrolysis: Breaks polymers into monomers by adding water.
Polymerization is favored only at high monomer concentrations; equilibrium favors free monomers.
Additional info: Macromolecules such as proteins, nucleic acids, and carbohydrates are essential for life and may have formed during early chemical evolution.