AP®︎ Chemistry: Unit 3 Flashcards

Master key terms and definitions for Unit 3 of AP Chemistry – Properties of Substances and Mixtures to help you prep for quizzes and the AP exam.


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Term

Intermolecular Vs. Intramolecular Forces

Definition

Between molecules: dispersion, dipole-dipole, hydrogen bonding, ion-dipole; within particles: covalent, ionic, metallic bonding.

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Intermolecular Vs. Intramolecular Forces
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Between molecules: dispersion, dipole-dipole, hydrogen bonding, ion-dipole; within particles: covalent, ionic, metallic bonding.

3.1.A
London Dispersion Forces
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Attractions from Coulombic interactions between temporary, fluctuating dipoles in all atoms and molecules.

3.1.A3.1.A.1
Polarizability
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How easily an electron cloud is distorted; it increases with more electrons, larger size, and pi bonding.

3.1.A3.1.A.1
Contact Area and Dispersion Strength
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Greater surface contact between molecules increases dispersion attractions by allowing more electron-cloud interactions.

3.1.A3.1.A.1
London Dispersion Forces Vs. Van Der Waals Forces
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Dispersion is one specific weak attraction; van der Waals is a broader category and not synonymous.

3.1.A3.1.A.1
Dipole-Induced Dipole Interactions
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Attractions between a polar molecule and a nonpolar molecule whose electron cloud becomes temporarily distorted.

3.1.A3.1.A.2
Ion-Dipole Forces
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Attractions between an ion and the oppositely charged end of a polar molecule.

3.1.A3.1.A.2
Orientation Dependence Of Dipole-Dipole And Ion-Dipole Forces
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Opposite charges aligned closer give stronger attraction; like-charge alignment gives weaker or repulsive interactions.

3.1.A3.1.A.3
Intermolecular Vs. Intramolecular Hydrogen Bonding
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Between separate molecules or between different regions of the same large molecule containing suitable N, O, or F sites.

3.1.A3.1.A.5
Noncovalent Interactions In Biomolecules
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Hydrogen bonding, ionic attractions, dipole interactions, and dispersion forces within or between large biomolecules.

3.1.A3.1.A.5
Relative Strength Of Intermolecular Forces
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Generally ion-dipole and hydrogen bonding exceed dipole-dipole, while dispersion varies with size and polarizability.

3.1.A
Dipole Moments And Dipole-Dipole Interactions
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A permanent molecular dipole creates attractions between polar molecules when opposite partial charges align.

3.1.A3.1.A.2
Temporary Dipole
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A momentary uneven electron distribution that creates partial charges in an atom or molecule.

3.1.A3.1.A.1
Hydrogen Bonding
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A strong intermolecular attraction between H covalently bonded to N, O, or F and a lone pair on N, O, or F.

3.1.A3.1.A.4
Crystalline Solids
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Solids with particles arranged in a regular, repeating pattern called a crystal lattice.

3.2.A
Particulate-Level Representations of Solids
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Diagrams showing atoms, ions, or molecules arranged to reveal forces and solid structure.

3.2.A3.2.A.2
Intermolecular Force Strength and Phase Change Properties
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Stronger attractions give lower vapor pressure and generally higher boiling and melting points.

3.2.A3.2.A.1
Types of Solids
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Ionic: ions; molecular: molecules with IMFs; covalent network: bonded networks; metallic: metal atoms with mobile electrons.

3.2.A
Ionic Solid Brittleness
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Shifting layers place like charges adjacent, causing repulsion and fracture.

3.2.A3.2.A.3
Diamond and Graphite
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Diamond is a hard 3D network insulator; graphite is layered, soft, and electrically conductive.

3.2.A3.2.A.4
Ionic Solids
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Crystalline solids of cations and anions with high melting points, brittleness, and conductivity only when ions move.

3.2.A3.2.A.3
Metallic Solids
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Solids of metal cores in a sea of mobile, delocalized valence electrons.

3.2.A3.2.A.6
Properties of Metallic Solids
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They conduct heat and electricity and are malleable and ductile because mobile electrons maintain bonding.

3.2.A3.2.A.6
Alloys
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Metal mixtures form substitutional or interstitial structures, and interstitial atoms make the lattice more rigid.

3.2.A3.2.A.6
Molecular Solids
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Solids of discrete molecules held by intermolecular forces, usually with low melting points and poor conductivity.

3.2.A3.2.A.5
Covalent Network Solids
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Solids of atoms covalently bonded in 2D or 3D networks, giving very high melting points and hardness.

3.2.A3.2.A.4
Biomolecules and Polymers in Solids
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Their shapes and properties depend on noncovalent interactions within one molecule or between molecules.

3.2.A3.2.A.7
Crystal Lattice and Unit Cell
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A crystal lattice is a regular, repeating three-dimensional arrangement of particles in a crystalline solid; the unit cell is the smallest repeating structural unit that builds the entire lattice.

3.2.A
States of Matter: Solid, Liquid, and Gas
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Solid: fixed shape and volume; liquid: fixed volume only; gas: neither fixed shape nor volume.

3.3.A3.3.A.4
Crystalline vs. Amorphous Solids
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Crystalline solids have ordered 3-D particle arrangements; amorphous solids lack long-range regular order.

3.3.A3.3.A.1
Particle Motion in Solids
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Particles stay in fixed positions and only vibrate, with no overall translational motion.

3.3.A3.3.A.1
Packing and Interparticle Forces in Solids
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Solid structure depends on how strongly particles attract and how efficiently they can pack together.

3.3.A3.3.A.1
Liquid Particle Model
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Particles remain close together but move continuously, collide often, and slide past one another.

3.3.A3.3.A.2
Fluidity
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The ability of particles in a substance, especially a liquid or gas, to flow past one another.

3.3.A
Molar Volume of Solids vs. Liquids
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For one substance, solid and liquid phases usually have similar molar volumes because particles stay closely packed.

3.3.A3.3.A.3
Gas Particle Model
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Particles are far apart, move constantly in straight lines, and experience minimal intermolecular attractions.

3.3.A3.3.A.4
Temperature, Pressure, and Volume Effects on Gases
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These variables change particle spacing and collision frequency in a gas.

3.3.A3.3.A.4
Compressibility
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The extent to which a substance's volume decreases when pressure is applied.

3.3.A3.3.A.4
Diffusion in Solids, Liquids, and Gases
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Mixing is extremely slow in solids, slow in liquids, and rapid in gases.

3.3.A
Surface Tension
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A liquid minimizes surface area; stronger intermolecular forces increase it, while higher temperature decreases it.

3.3.A3.3.A.2
Viscosity
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A liquid's resistance to flow increases with stronger intermolecular forces and decreases with higher temperature.

3.3.A3.3.A.2
Cohesive and Adhesive Forces
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Attractions within a liquid and to surfaces determine capillary action and meniscus shape.

3.3.A3.3.A.2
Ideal Gas Law
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PV = nRT, relating pressure, volume, moles, and temperature for an ideal gas.

3.4.A3.4.A.1
Gas Variables and Units in The Ideal Gas Law
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P in atm, V in L, n in mol, T in K, and R = 0.08206 L·atm/mol·K.

3.4.A3.4.A.1
Standard Temperature and Pressure (STP)
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Conditions of 1 atm pressure and 273.15 K temperature.

3.4.A
Pressure and Particle Collisions
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Pressure comes from gas particles colliding with the walls of their container.

3.4.A
Boyle's Law
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At constant temperature, pressure and volume are inversely related: P1V1 = P2V2.

3.4.A3.4.A.3
Charles's Law
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At constant pressure, volume and temperature are directly related: V1/T1 = V2/T2.

3.4.A3.4.A.3
Gay-Lussac's Law
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At constant volume, pressure and temperature are directly related: P1/T1 = P2/T2.

3.4.A3.4.A.3
Avogadro's Law
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At constant pressure and temperature, volume is directly proportional to moles: V1/n1 = V2/n2.

3.4.A3.4.A.3
Combined Gas Law
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P1V1/T1 = P2V2/T2, combining pressure, volume, and temperature when moles stay constant.

3.4.A3.4.A.1
Dalton's Law of Partial Pressures
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Total pressure equals the sum of each gas's partial pressure in a mixture.

3.4.A3.4.A.2
Partial Pressure
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The pressure exerted by one gas component in a mixture, independent of other gases.

3.4.A3.4.A.2
Mole Fraction
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The ratio of moles of one gas to total moles in a mixture.

3.4.A3.4.A.2
Partial Pressure from Mole Fraction
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For gas A, PA = XA × Ptotal, where XA is its mole fraction.

3.4.A3.4.A.2
Graphical Gas Relationships
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P, V, T, and n can be graphed to show direct or inverse proportional relationships.

3.4.A3.4.A.3
Standard Pressure
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Atmospheric pressure under standard conditions is 1.00 atm, 760 torr, 760 mm Hg, or 101.3 kPa.

3.4.A
Kelvin Conversion
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Temperature in Celsius is converted to Kelvin by adding 273.15.

3.4.A3.4.A.1
Continuous Random Motion
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All particles in a sample of matter are always moving in random directions.

3.5.A3.5.A.2
Elastic Collisions
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Collisions in which particles transfer energy without any net loss of total kinetic energy.

3.5.A
Negligible Particle Volume
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Gas particles occupy very little space compared with the total volume of the container.

3.5.A
No Intermolecular Forces in an Ideal Gas
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Ideal gas particles neither attract nor repel one another between collisions.

3.5.A
Particle Motion and Gas Pressure
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Faster particles collide with container walls more often and more forcefully, increasing pressure.

3.5.A3.5.A.1
Kinetic Molecular Theory
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A model describing gases as tiny particles moving randomly with negligible volume, no forces, and elastic collisions.

3.5.A3.5.A.1
Maxwell-Boltzmann Distribution
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A graph showing particle energies or speeds, where higher temperature broadens the curve and shifts it right.

3.5.A3.5.A.4
Average Kinetic Energy and Temperature
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The average kinetic energy of particles is directly proportional to the Kelvin temperature, and at the same temperature all gases have the same average kinetic energy.

3.5.A3.5.A.3
Effect of Attractions on Measured Pressure
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Real-gas pressure is lower than ideal pressure because attractions reduce wall-collision frequency and force.

3.6.A3.6.A.1
Effect of Particle Volume at High Pressure
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At very high pressure, real gases occupy more volume than ideal gases predict.

3.6.A3.6.A.1
Causes of Real Gas Deviation
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Real gases deviate because particles attract each other and occupy finite volume.

3.6.A3.6.A.1
Factors That Increase Non-Ideal Behavior
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Low temperature, high pressure, polarity, and larger size make gases less ideal.

3.6.A3.6.A.1
Van Der Waals Equation and Constants
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This real-gas model corrects pressure for attractions and volume for particle size.

3.6.A3.6.A.1
Homogeneous Mixture / Solution
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A mixture with uniform composition whose macroscopic properties are the same throughout the sample.

3.7.A3.7.A.1
Heterogeneous Mixture
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A mixture with nonuniform composition whose macroscopic properties vary from one location to another.

3.7.A3.7.A.1
Types of Solutions
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Solutions can be solid, liquid, or gas, as long as composition is uniform throughout.

3.7.A3.7.A.1
Aqueous
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Dissolved in water, written as aq in a chemical equation.

3.7.A
Solvation and Hydration
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Solvation is solvent attraction around solute particles; hydration is this process specifically in water.

3.7.A
Volume of Solution vs. Volume of Solvent
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Molarity uses total solution volume, not just the volume of the solvent.

3.7.A3.7.A.2
Dilution
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Lowering concentration by adding solvent while keeping the amount of solute constant.

3.7.A
Dilution Equation
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Use M1V1 = M2V2 because moles of solute stay constant during dilution.

3.7.A3.7.A.2
Molarity
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Moles of solute per liter of solution, used to calculate amount, volume, or concentration.

3.7.A3.7.A.2
Solute and Solvent
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The dissolved substance is the solute, and the dissolving medium is the solvent.

3.7.A
Particulate Representation of a Solution
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A particle-level diagram showing component amounts, distribution, and interactions in a solution.

3.8.A3.8.A.1
Representing Concentration in Particulate Diagrams
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Show concentration by the number of solute particles per equal volume of solution.

3.8.A3.8.A.1
Dilute, Concentrated, and Saturated Solutions
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Dilute has few solute particles, concentrated has many, saturated has the maximum dissolved amount.

3.8.A3.8.A.1
Equal-Volume Comparison in Solution Diagrams
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Concentrations should be compared using the same volume so particle counts are meaningful.

3.8.A3.8.A.1
Solvation Shell
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A layer of solvent molecules surrounding and stabilizing a dissolved particle.

3.8.A3.8.A.1
Electrolyte and Nonelectrolyte
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One forms ions in water and conducts electricity; the other forms no ions and does not.

3.8.A
Strong and Weak Electrolytes
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One dissociates completely into ions in water; the other dissociates only partially.

3.8.A
Dissociation
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The separation of an ionic compound or electrolyte into ions in solution.

3.8.A
Molecular Solute Representation in Water
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Show intact molecules, with water oriented toward polar regions if intermolecular attractions exist.

3.8.A3.8.A.1
Ion-Dipole Interactions in Water
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An ion attracts polar water molecules, with oxygen toward cations and hydrogens toward anions.

3.8.A3.8.A.1
Ionic vs Molecular Solute Representation
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Ionic solutes separate into ions, while molecular solutes remain intact particles in solution.

3.8.A3.8.A.1
Filtration
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Separates an insoluble solid from a liquid by passing the mixture through a porous barrier.

3.9.A3.9.A.1
Chromatography
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Separates mixture components by different attractions to a mobile phase and a stationary phase.

3.9.A3.9.A.1
Stationary Phase and Mobile Phase
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Stationary phase stays fixed; mobile phase moves and carries dissolved substances through or across it.

3.9.A3.9.A.1
Paper, Thin-Layer, and Column Chromatography
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Paper uses cellulose, TLC uses coated silica plates, and column uses packed solid adsorbent in a tube.

3.9.A3.9.A.1
Chromatography and Polarity
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More polar substances usually stick more to polar stationary phases and travel shorter distances.

3.9.A3.9.A.1
Chromatogram
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The separation pattern showing component positions after chromatography, used to compare relative polarity.

3.9.A3.9.A.1
Distillation
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Separates liquids by heating so the more volatile component vaporizes first and then condenses.

3.9.A3.9.A.1
Simple Distillation vs. Fractional Distillation
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Simple uses one vaporization-condensation step for larger boiling-point differences; fractional uses many steps for closer boiling points.

3.9.A3.9.A.1
Boiling Point, Vapor Pressure, and Intermolecular Forces in Distillation
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Weaker intermolecular forces give higher vapor pressure and lower boiling point, so that component distills first.

3.9.A3.9.A.1
Rf Value
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The ratio of a substance’s travel distance to the solvent front’s distance.

3.9.A3.9.A.1
Solubility
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The maximum amount of solute that dissolves in a given solvent under specific conditions.

3.10.A
Miscibility
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The ability of two liquids to mix completely and form one homogeneous phase.

3.10.A3.10.A.1
Saturated, Unsaturated, and Supersaturated Solutions
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At maximum dissolved solute, below that amount, and above that amount in an unstable state, respectively.

3.10.A
Pressure and Gas Solubility
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Increasing pressure increases the solubility of gases, but has little effect on solids or liquids.

3.10.A
Intermolecular Forces and Solubility
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Solubility is greatest when solute-solvent attractions closely match or exceed particle-particle attractions.

3.10.A3.10.A.1
Solubility Curve
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A graph showing how a substance's solubility changes with temperature.

3.10.A
Electromagnetic Radiation / Radiant Energy
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Energy that travels through space as oscillating electric and magnetic waves.

3.11.A
Wave-Particle Duality
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The idea that light behaves as both a wave and a particle.

3.11.A
Electromagnetic Spectrum
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The full range of electromagnetic radiation, ordered by wavelength or frequency.

3.11.A
Spectroscopy
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The study of how matter absorbs, emits, or interacts with electromagnetic radiation.

3.11.A
Absorption and Emission Spectra
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Patterns formed when matter absorbs specific wavelengths or emits photons at specific wavelengths.

3.11.A
Wavelength, Frequency, and c = λν
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Wavelength and frequency are inversely related and connected by c = λν.

3.11.A
Spectral Regions and Energy Transitions
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Microwaves cause rotational changes, infrared causes vibrational changes, and UV-visible causes electronic changes.

3.11.A3.11.A.1
Planck's Equation
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E = hν, relating photon energy to frequency through Planck's constant.

3.12.A3.12.A.2
Planck's Constant
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The proportionality constant 6.626 × 10^-34 J·s used in E = hν.

3.12.A3.12.A.2
Electronic Transitions and Photons
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Electrons change energy levels by absorbing or emitting photons with matching energy.

3.12.A3.12.A.1
Frequency, Wavelength, and Photon Energy
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Frequency and wavelength are inversely related, and higher frequency means higher photon energy.

3.12.A3.12.A.2
Photoelectric Effect and Threshold Frequency
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Electrons are emitted from metals only when light reaches a minimum frequency.

3.12.A
Photon
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A discrete packet of electromagnetic energy absorbed or emitted by matter during a transition.

3.12.A3.12.A.1
Monochromator
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The spectrophotometer component that isolates a narrow band of wavelengths from white light.

3.13.A
Cuvette / Path Length
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A transparent sample holder whose width sets the light-travel distance, usually measured in centimeters.

3.13.A3.13.A.1
Incident Light and Transmitted Light
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I0 is light entering the sample; I is light leaving after some has been absorbed.

3.13.A
Absorbance
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A unitless measure of how much light a sample absorbs at a given wavelength.

3.13.A3.13.A.1
Molar Absorptivity
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A wavelength-specific constant showing how strongly a substance absorbs light, symbolized by epsilon.

3.13.A3.13.A.1
Beer-Lambert Law / Beer's Law
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A = epsilonbc, relating absorbance to molar absorptivity, path length, and concentration.

3.13.A3.13.A.1
Direct Proportionality in Beer-Lambert Law
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With wavelength and path length constant, absorbance increases linearly as concentration increases.

3.13.A3.13.A.2
Complementary Colors and Absorption
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Solutions absorb light best in the color opposite their observed color on the visible spectrum.

3.13.A
Solving for Concentration with Beer-Lambert Law
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Rearrange A = epsilonbc to c = A divided by epsilon times b.

3.13.A3.13.A.1
Spectrophotometry and Spectrophotometer
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A method using an instrument to measure transmitted light and determine sample absorbance.

3.13.A3.13.A.2
Wavelength of Maximum Absorbance
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The wavelength at which a substance absorbs most strongly, giving the greatest measurement sensitivity.

3.13.A3.13.A.2