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💧 Unit 3 · Intermolecular Forces & Properties 🏠 Unit Hub 🗂 Flashcards 🗺 Cheat Sheet Essentials 🎨 Visual Review 📝 MC Practice ✍️ SAQ Practice

AP Chemistry Unit 3 Essentials

The must-know terms and big ideas for Unit 3: Intermolecular Forces & Properties. Every vocabulary word and concept you need to master.

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Big Idea 1
Intermolecular forces explain almost every macroscopic property you can measure
Boiling point, melting point, viscosity, surface tension, and vapor pressure all come down to one question: how strongly do neighboring molecules attract each other? Stronger IMFs (hydrogen bonding > dipole-dipole > London dispersion) mean more energy is needed to separate molecules, which raises boiling and melting points and lowers vapor pressure. The molecular shape and polarity you predicted in Unit 2 are exactly what you need to identify which IMFs apply.
IMFs Boiling Point Structure-Property
Big Idea 2
The ideal gas law is a model, and real gases deviate from it predictably
PV = nRT assumes gas particles have no volume and no attraction to each other — a useful simplification, but not reality. Real gases deviate most from ideal behavior at high pressure (molecules are forced close together, so their actual volume matters) and low temperature (molecules move slowly enough for intermolecular attractions to matter). Notice the pattern: the same intermolecular forces from Big Idea 1 are exactly what cause real-gas deviations.
Ideal Gas Law Kinetic Molecular Theory Real Gases
Big Idea 3
"Like dissolves like" is IMF compatibility, not magic
A solute dissolves in a solvent when the new solute-solvent IMFs that form are strong enough to compensate for the solute-solute and solvent-solvent IMFs being broken. Polar and ionic substances dissolve well in polar solvents (like water) because they can form strong dipole-dipole, ion-dipole, or hydrogen-bonding interactions; nonpolar substances dissolve in nonpolar solvents because only weak London dispersion forces need to be matched.
Solubility Solutions Polarity
Big Idea 4
Spectroscopy turns light absorption into information about concentration and structure
Different regions of the electromagnetic spectrum interact with matter in different ways — and the amount of light a sample absorbs (its absorbance) is directly proportional to its concentration, according to the Beer-Lambert law. This single relationship is what allows chemists to determine an unknown concentration just by shining light through a solution and measuring how much comes out the other side.
Spectroscopy Beer-Lambert Law Absorbance
Intermolecular force (IMF)
An attractive force between molecules (or between ions and molecules), much weaker than the intramolecular (covalent or ionic) bonds within a molecule.
IMFs
London dispersion force
A temporary, weak attraction caused by momentary, fluctuating electron distributions creating instantaneous dipoles. Present in all molecules; the only IMF in nonpolar molecules. Strength increases with molecular size and surface area (polarizability).
IMFs
Dipole-dipole force
An attraction between the positive end of one polar molecule and the negative end of a neighboring polar molecule.
IMFs
Hydrogen bonding
An especially strong type of dipole-dipole force that occurs when hydrogen is bonded to a small, highly electronegative atom (N, O, or F) and attracted to a lone pair on a neighboring N, O, or F.
IMFs
Polarizability
A measure of how easily an atom or molecule's electron cloud can be distorted to form a temporary dipole. Larger atoms/molecules with more electrons are more polarizable, leading to stronger London dispersion forces.
IMFs
Vapor pressure
The pressure exerted by a substance's gas phase in equilibrium with its liquid phase at a given temperature. Weaker IMFs lead to higher vapor pressure (more molecules escape into the gas phase).
States of Matter
Viscosity
A liquid's resistance to flow. Stronger IMFs between molecules increase viscosity.
States of Matter
Surface tension
The energy required to increase a liquid's surface area, caused by IMFs pulling surface molecules inward. Stronger IMFs mean higher surface tension.
States of Matter
Crystalline solid
A solid with a highly ordered, repeating particle arrangement. Types include ionic, metallic, covalent network, and molecular solids, each with distinct properties.
Solids
Amorphous solid
A solid lacking a long-range ordered structure (e.g., glass or rubber), resulting in variable, less-defined physical properties compared to crystalline solids.
Solids
Covalent network solid
A solid (like diamond or quartz) held together entirely by covalent bonds extending through the whole structure, giving extremely high melting points and hardness.
Solids
Phase diagram
A graph of pressure versus temperature showing the conditions under which a substance exists as a solid, liquid, or gas, including the triple point and critical point.
States of Matter
Ideal gas law
PV = nRT — relates pressure, volume, moles, and temperature of an ideal gas, where R is the gas constant.
Gas Laws
Kinetic molecular theory (KMT)
A model describing gas particles as point masses in constant random motion with no intermolecular attraction, whose average kinetic energy is directly proportional to absolute temperature.
Gas Laws
Real gas deviation
The departure of actual gas behavior from the ideal gas law, most significant at high pressure (molecular volume becomes significant) and low temperature (intermolecular attractions become significant).
Gas Laws
Partial pressure / Dalton's law
The pressure a single gas in a mixture would exert if it alone occupied the container. Dalton's law states that total pressure equals the sum of all partial pressures.
Gas Laws
Solute / solvent
The solute is the substance being dissolved (present in smaller amount); the solvent is the substance doing the dissolving (present in larger amount).
Solutions
Molarity
A concentration unit defined as moles of solute per liter of solution (mol/L).
Solutions
"Like dissolves like"
The general solubility rule that polar/ionic solutes dissolve well in polar solvents, and nonpolar solutes dissolve well in nonpolar solvents, because similar IMFs allow new solute-solvent interactions to replace the ones being broken.
Solubility
Chromatography
A separation technique exploiting differences in how strongly mixture components interact with a stationary phase versus a mobile phase.
Separation
Electromagnetic spectrum
The full range of electromagnetic radiation, from low-energy radio waves to high-energy gamma rays, including visible light, infrared, and ultraviolet — each interacting differently with matter.
Spectroscopy
Beer-Lambert law
A = εlc — absorbance (A) is directly proportional to molar absorptivity (ε), path length (l), and concentration (c). Used to determine unknown concentrations from absorbance measurements.
Spectroscopy