Properties of Substances and Mixtures
Intermolecular Forces (IMFs)
- London Dispersion Forces (LDF):
- Present in all substances; sole force in nonpolar substances.
- Temporary dipoles due to random electron motion induce dipoles in neighboring molecules, leading to Coulombic attraction.
- Increase with greater contact area, more electrons/larger electron cloud, and pi bonding (polarizability).
- Dipole-Induced Dipole:
- Occurs between polar and nonpolar molecules.
- Increases with polarity of the polar molecule and polarizability of the nonpolar molecule.
- Dipole-Dipole:
- Occurs between two polar molecules.
- Strength increases with greater polarity and favorable orientations.
- Typically stronger than LDF, but data should be checked.
- Hydrogen Bonding:
- Strong form of dipole-dipole interaction.
- Requires a partially positive hydrogen atom attached to N, O, or F on one molecule, attracted to a partially negative N, O, or F on another molecule.
- Ion-Dipole:
- Occurs between an ion and a polar molecule.
- Usually stronger than dipole-dipole interactions.
Properties of Solids
- Properties depend on the strength and type of IMFs (boiling point (BP), vapor pressure (VP), melting point (MP)).
- When boiling, all IMFs must be overcome to vaporize a substance.
- Ionic Solids:
- Strong interactions between ions result in low VP and high MP/BP.
- Brittle due to repulsions between like charges.
- Conduct electricity when ions are mobile (solutions or molten state).
- Covalent Network Solids:
- 3D (or 2D for graphite) covalent bonds throughout the structure.
- Very strong, leading to very high MP/BP.
- Hard/rigid due to fixed bond angles.
- Examples: diamond, Buckyball (C60), graphite, SiC, SiO2.
- Molecular Solids:
- Individual molecules held together by relatively weak IMFs.
- High VP and low MP/BP.
- Do not conduct electricity.
- Metallic Solids:
- Metal atoms in a sea of valence electrons.
- Can form alloys (interstitial and substitutional).
- Conduct heat and electricity.
- Biomolecules/Polymers:
- Large molecules with intramolecular forces affecting shape/properties.
Solids, Liquids, and Gases
- Solids:
- Particles in regular, crystalline arrangements or amorphous structures.
- Limited particle motion; no translational kinetic energy.
- Structure determined by interparticle attractions.
- Liquids:
- Particles close together but able to move and collide.
- Arrangement and movement depend on polarity, hydrogen bonding, and temperature.
- Molar volume similar to corresponding solid.
- Gases:
- Constant random motion in straight lines until collision.
- Frequency of collisions depends on volume, pressure, and temperature.
- Limited IMFs; no definite shape or volume.
Ideal Gas Law
- Relates pressure (P), volume (V), moles (n), and absolute temperature (T) of a gas: PV = nRT
- R is the Universal Gas Constant (0.08206 Latm/molK).
- Combined Gas Law derivation: \frac{PV}{nT} = R = \frac{PV}{nT}
- Dalton's Law of Partial Pressures: Total pressure is the sum of individual pressures (P = P1 + P2 + P_3…).
- Application: Gases collected by bubbling through water require accounting for water vapor pressure.
- Mole Fraction (X):
- Represents the fraction of the sample (in moles) for one of the gases.
- Mole fraction * total pressure = pressure of the gas in question.
Kinetic Molecular Theory (KMT)
- Based on postulates for an IDEAL gas:
- Gas particle size is negligible compared to the space between particles.
- Constant random motion with perfectly elastic collisions (energy transferred, not lost).
- No attractive or repulsive forces between gas particles.
- Temperature is a measure of average kinetic energy (KE = \frac{1}{2} mv^2).
- Graham's law: smaller molecules move faster than larger molecules at the same temperature.
Deviation from Ideal Gas Law
- Real gases deviate from ideal behavior at high pressure or low temperature.
- Factors causing deviation:
- Volume of particles: Significant for larger particles, increases the P*V term.
- Intermolecular Forces: Increase with stronger IMFs, decreases the P*V term.
- Maxwell-Boltzmann distribution: Describes particle energies at different temperatures.
Solutions and Mixtures
- Solutions: Homogeneous mixtures where a solute is dissolved in a solvent.
- Heterogeneous mixtures: Non-uniform composition.
- Molarity:
- Common unit for solution concentration: Molarity = \frac{moles \, of \, solute}{Liter \, of \, solution}
- Ion concentration depends on the ratio of atoms in the formula.
Representations of Solutions
- Considerations:
- Whether the solute forms ions or not.
- Relative sizes, amounts, and orientation of water to ions.
- Solution concentration and number of particles represented.
- Changes in volume or states of matter (precipitate or gas formation).
- Types of IMFs between solute and solvent.
Separation of Solutions and Mixtures
- Chromatography:
- Separates components based on differences in IMFs.
- Types: Paper, Column, and Thin-Layer Chromatography (TLC).
- Mobile phase (solvent) and stationary phase.
- Column chromatography: Use for material recovery.
- R_f \, value = \frac{distance \, traveled \, by \, dye}{distance \, traveled \, by \, solvent}
- Distillation:
- Separates mixtures based on differences in boiling points.
- Repeated boiling and condensation of vapors.
Solubility
- Miscible: Solute and solvent will mix.
- Immiscible: Solute and solvent do not mix.
- Substances with similar IMFs tend to be miscible.
- Solution formation steps:
- Solute separation (requires energy).
- Solvent separation (requires energy).
- Solvent-solute attraction (releases energy).
Spectroscopy and the Electromagnetic Spectrum
- Spectroscopy: Study of matter's interaction with electromagnetic radiation.
- Microwave Rotational Spectroscopy:
- Microwaves cause molecules to rotate due to interaction with molecular dipole.
- Infrared (IR) Vibrational Spectroscopy:
- Measures atomic vibrations, determines functional groups.
- Ultraviolet-Visible (UV-Vis) Light Spectroscopy:
- Photons excite electrons to higher energy levels.
- Energy released as EM radiation during transitions in electronic energy levels.
Properties of Photons
- Photoelectric Effect:
- Light shone on a material's surface ejects electrons if energy exceeds binding energy (or shorter wavelength/higher frequency than threshold).
- Photon absorption/emission changes atom/molecule energy.
- Photon energy:
- E = hv
- h (Planck's constant) = 6.626 \times 10^{-34} m/second
- v (frequency) in Hertz (1/sec).
- Electron energy: E = \frac{1}{2} mv^2
- Combined equations:
- E = \frac{hc}{\lambda}
- c (speed of light) = 3.00 \times 10^8 m/sec
- λ = wavelength (m).
Beer-Lambert Law
- Relates UV-Vis light absorbance to solution concentration.
- Increased concentration increases absorbance and decreases % transmittance.
- A = \epsilon bc
- A = Absorbance.
- ε = Molar absorptivity constant.
- b = path length (usually 1 cm).
- c = concentration (molarity).
- Wavelength selection: Choose complementary color for absorbance around 1.