BackLiquids, Solids, and Intermolecular Forces: Study Guide
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Liquids, Solids, and Intermolecular Forces
Molecular Polarity
Molecular polarity describes the distribution of electrical charge across a molecule, which affects its physical and chemical properties. Polarity arises from the unequal sharing of electrons between atoms due to differences in electronegativity.
Nonpolar Molecule: Any hydrocarbon or molecule with a symmetrical ("perfect") shape. Examples include linear molecules with the same surrounding elements and no lone pairs, or square planar molecules with the same surrounding elements.
Polar Molecule: Any molecule whose Lewis Dot Structure does not have a perfect shape, often due to lone pairs or different surrounding elements.
Example: Carbon tetrachloride (CCl4) is nonpolar because it has a symmetrical tetrahedral shape with identical surrounding atoms.
Intermolecular Forces
Intermolecular forces are the attractive forces that exist between molecules and influence their physical properties. They are generally weaker than intramolecular forces (chemical bonds).
Intramolecular Forces: Exist within a molecule, bond atoms together, and influence chemical properties. Examples: ionic and covalent bonds.
Intermolecular Forces: Exist between molecules and influence physical properties such as boiling point, melting point, viscosity, and surface tension.
Types of Intermolecular Forces: There are five main types: London dispersion forces, dipole-dipole forces, hydrogen bonding, ion-dipole forces, and dipole/induced-dipole forces.
London Dispersion Forces: Present in all molecules, especially nonpolar ones.
Example: N2 (nonpolar) exhibits London dispersion forces; CH3OH (polar) exhibits hydrogen bonding.
Intermolecular Forces and Physical Properties
Physical properties such as boiling point, melting point, surface tension, and viscosity are influenced by the strength of intermolecular forces.
Direct Relationships: Stronger intermolecular forces lead to higher boiling points, melting points, and surface tension.
Indirect Relationships: Stronger intermolecular forces lead to lower vapor pressure and slower flow (higher viscosity).
Example: CaS in H2O has a higher melting point due to strong ion-dipole forces.

Vapor Pressure
Vapor pressure is the pressure exerted by a vapor at the surface of a liquid. It represents an equilibrium between evaporation and condensation.
As temperature increases, vapor pressure increases.
Equilibrium: The rate of evaporation equals the rate of condensation at equilibrium.

Heating and Cooling Curves
Heating and cooling curves show the amount of heat absorbed or released by a substance during phase changes. They help calculate the energy required for transitions between solid, liquid, and gas phases.
Heating Curve: Endothermic process (+q), heat absorbed.
Cooling Curve: Exothermic process (-q), heat released.
Formulas:
Specific Heat Capacity:
Enthalpy (Phase Change):
Total Energy:
Example: To convert 55.8 g of ice at -5°C to gas at 100°C, use the specific heat and enthalpy values for each phase.

Phase Diagrams
Phase diagrams map the physical state of a pure substance as a function of pressure and temperature. They show regions for solid, liquid, gas, and supercritical fluid.
Triple Point: Unique set of conditions where all three states of matter are in equilibrium.
Critical Point: Final set of pressure and temperature conditions where liquid and gas are indistinguishable.
Normal Pressure: Standard pressure of 1 atm or 760 mmHg.
Normal Melting Point: Transition from solid to liquid at normal pressure.
Normal Boiling Point: Transition from liquid to gas at normal pressure.




Clausius-Clapeyron Equation
The Clausius-Clapeyron equation relates the vapor pressure of liquids to temperature, allowing calculation of enthalpy of vaporization.
Linear Form:
Two-Point Form:
Variables: R = 8.314 J/(mol·K), P = vapor pressure, T = temperature in K, = enthalpy of vaporization.
Example: Calculate the vapor pressure of water at 60°C using the two-point form.
Property | Value |
|---|---|
Specific Heat of Ice (c) | 2.09 J/g·°C |
ΔHFusion | 334 J/g |
Specific Heat of Water (c) | 4.184 J/g·°C |
ΔHVaporization | 2260 J/g |
*Additional info: Academic context and formulas were expanded for completeness and clarity.*