MM

Exam 1 Review

Lecture 1: Forces in Molecules

  • Difference between Intramolecular and Intermolecular Forces:

    • Intramolecular Forces:

    • Forces that hold atoms together within a molecule.

    • Types include:

      • Covalent bonding

      • Ionic bonding

      • Metallic bonding

    • Generally stronger than intermolecular forces (IMF).

    • Intermolecular Forces (IMF):

    • Attractions between molecules.

    • Weaker than intramolecular forces with varying strengths.

    • Strength hierarchy:

      • London Dispersion Forces < Dipole-Dipole < Hydrogen Bonding < Ion-Dipole < Covalent < Ionic < Metallic

    • Stronger IMF lead to:

      • Higher melting/freezing/boiling points

      • Higher viscosity

      • Greater surface tension

      • Higher enthalpies of fusion, vaporization, sublimation

      • Lower vapor pressure

  • Important Concepts:

    • Lewis Structure: Key to understanding molecular structure and behavior.

Types of Intermolecular Forces

  • London Dispersion Forces:

    • Weakest IMF, present in all molecules.

    • Caused by temporary dipoles due to electron movement.

    • Strength increases with molecular weight due to greater polarization potential.

  • Dipole-Dipole Interactions:

    • Occur between polar molecules.

    • Positive end of one molecule attracts the negative end of another.

  • Hydrogen Bonds:

    • Special case of dipole-dipole interaction.

    • Involves hydrogen atoms bonded to highly electronegative atoms (N, O, F).

    • Stronger than regular dipole-dipole interactions.

  • Ion-Dipole Forces:

    • Interactions between an ion and a polar molecule, crucial in solvation.

  • Collective Terms:

    • Dipole-induced dipoles and London Dispersion forces are referred to as Van der Waals forces.

    • Instantaneous dipoles can form when nonpolar molecules are close together.

Lecture 2: Heat and Phase Changes

  • Phase Diagrams: Understand how temperature and pressure affect phases.

  • Endothermic vs Exothermic Processes:

    • Endothermic: Absorbs heat. e.g., Solid → Liquid → Gas (bond breaking).

    • Exothermic: Releases heat. e.g., Gas → Liquid → Solid (bond forming).

  • Clausius-Clapeyron Equation:

    • R = 8.314 ext{ J/mol*K}

    • Pressure (P) is directly related to temperature during phase changes.

Cooling & Heating Curves

  • Temperature Change:

    • Q=mc\Delta T

    • where:

      • m = mass

      • c = specific heat

      • \Delta T = final temp - initial temp

  • Phase Change:

    • Q=m\cdot\Delta H

    • Remember the signs:

    • Endothermic: positive \Delta H

    • Exothermic: negative \Delta H

    • Types of \Delta H : Fusion, Evaporation, Sublimation.

Lecture 3: Unit Cells

  • Volume Calculation:

    • V=\left(edge\cdot leng\operatorname{th}\right)^3\left(a^3\right)

    • 1 Å = 10^{-10} m

    • 1 m = 10^{12} pm

Lecture 4: Solution Process

  • "Like Dissolves Like" Principle:

    • Polar solvents dissolve polar solutes, nonpolar solvents dissolve nonpolar solutes.

    • Requires breaking solute-solute and solvent-solvent interactions.

  • Enthalpy of Solution:

    • riangle H{soln} = riangle H1 + riangle H2 + riangle H3

Henry's Law

  • Solubility Factors:

    • Solids: Higher temperature increases solubility.

    • Gases: Higher pressure increases solubility; lower temperature helps gas solubility as well.

  • Henry’s Law Equation:

    • C=kP

    • where:

      • C = concentration of gas (M)

      • P = partial pressure (atm)

      • k = Henry’s law constant (M/atm).

Lecture 5: Concentration

  • Molarity (M):

    • =molesofsolute/litersofsolution

  • Molality (m):

    • =molesofsolute/kilogramsofsolvent

  • Volume Percent (%v/v):

    • =volumeofsolute/volumeofsolution*100

  • Weight Percent (%w/w):

    • =massofsolute/massofsolution*100

  • Weight by Volume Percent (%w/v):

    • =massofsolute/volumeofsolution*100

  • Mole Fraction (X):

    • =molesofsolute/molesoftotalsolution

  • ppm and ppb:

    • ppm=milligramsofsolute/litersofsolution

    • ppb=microgramsofsolute/litersofsolution

Lecture 6: Colligative Properties

  • Types:

    • Vapor pressure lowering

    • Boiling point elevation

    • Freezing point depression

    • Osmotic pressure

  • Calculations for water:

    • New boiling point: 100+\Delta T

    • New freezing point: 0-\Delta T

  • Van 't Hoff Factor (i):

    • Number of particles a solute breaks into upon dissolving.

  • Effect of Concentration:

    • Higher concentration leads to higher boiling points, lower freezing points, lower vapor pressures, and higher osmotic pressure.

Lecture 7: Colloids

  • Definition:

    • A suspension of tiny particles in a medium (not dissolving).

    • Intermediate between homogeneous and heterogeneous mixtures.

    • Particle size: 10^3 to 10^6

  • Coagulation:

    • Process where a colloid is destroyed, typically by heating or adding an electrolyte.