BackChem 2A Exam 3 Study Guide (Chapters 9–13): Electrons, Bonding, Gases, Liquids, and Solutions
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Chapter 9: Electrons in Atoms and the Periodic Table
Energy, Wavelength, and Frequency
The relationship between energy, wavelength, and frequency is fundamental to understanding electromagnetic radiation.
Energy (E) is directly proportional to frequency (ν) and inversely proportional to wavelength (λ).
The equation relating these quantities is:
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Where h is Planck's constant and c is the speed of light.
Electromagnetic Spectrum and Visible Light
The electromagnetic spectrum includes all types of electromagnetic radiation, from gamma rays to radio waves.
Visible light is a small portion of this spectrum, with wavelengths approximately from 400 nm (violet) to 700 nm (red).
Atomic Orbitals and Electron Configurations
Electrons occupy orbitals, which are regions of space where the probability of finding an electron is high.
Each orbital can hold a maximum of two electrons with opposite spins.
Electron configurations describe the arrangement of electrons in an atom.
Orbital Diagrams
Orbital diagrams use boxes or lines to represent orbitals and arrows to represent electrons.
Hund's Rule: Electrons fill degenerate orbitals singly before pairing.
Periodic Trends
Electron configurations explain trends in atomic size, ionization energy, and chemical reactivity.
Chapter 10: Chemical Bonding
Lewis Structures and Bonding
Lewis structures are diagrams that show the bonding between atoms and the lone pairs of electrons in a molecule.
Valence electrons are represented as dots around the chemical symbols.
Shared pairs of electrons (bonds) are shown as lines.
Polarity and Molecular Geometry
Molecular polarity depends on the difference in electronegativity between atoms and the geometry of the molecule.
Electronegativity is a measure of an atom's ability to attract electrons in a bond.
VSEPR (Valence Shell Electron Pair Repulsion) theory is used to predict molecular shapes.
Bond Order and Resonance
Bond order is the number of chemical bonds between a pair of atoms.
Resonance structures are different Lewis structures for the same molecule that show delocalized electrons.
Chapter 11: Gases
Gas Laws and Properties
Gases have unique properties and are described by several laws relating pressure, volume, temperature, and amount.
Boyle's Law: (at constant temperature)
Charles's Law: (at constant pressure)
Avogadro's Law: (at constant temperature and pressure)
Ideal Gas Law:
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Where P is pressure, V is volume, n is moles, R is the gas constant, and T is temperature in Kelvin.
Partial Pressure and Dalton's Law
The total pressure of a gas mixture is the sum of the partial pressures of each component.
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Chapter 12: Liquids, Solids, and Intermolecular Forces
Types of Intermolecular Forces
Dispersion forces (London forces): Present in all molecules, due to temporary dipoles.
Dipole-dipole forces: Occur between polar molecules.
Hydrogen bonding: A strong type of dipole-dipole interaction, occurs when H is bonded to N, O, or F.
Properties of Liquids and Solids
Intermolecular forces affect boiling points, melting points, and solubility.
Stronger forces lead to higher boiling and melting points.
Phase Changes
Energy is required to change states (e.g., melting, vaporization).
Phase diagrams show the conditions under which different phases exist.
Chapter 13: Solutions
Types of Solutions and Solubility
A solution is a homogeneous mixture of two or more substances.
The solute is dissolved in the solvent.
Solubility depends on temperature, pressure, and the nature of the solute and solvent.
Electrolytes and Nonelectrolytes
Electrolytes are substances that conduct electricity when dissolved in water (e.g., salts, acids, bases).
Nonelectrolytes do not conduct electricity (e.g., sugar).
Concentration Units
Molarity (M): Moles of solute per liter of solution.
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Solution Stoichiometry and Dilution
Stoichiometry involves calculations based on balanced chemical equations.
Dilution equation:
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Where M is molarity and V is volume before and after dilution.
Diffusion and Osmosis
Diffusion is the movement of particles from high to low concentration.
Osmosis is the movement of solvent through a semipermeable membrane.
Example: Calculating the final concentration after dilution using .
Additional info: Some context and explanations have been expanded for clarity and completeness based on standard introductory chemistry curricula.