Phases and Phase Equilibria Flashcards
Convert between Kelvin and Celsius
K = °C + 273
Convert between Farenheight and Celsius
F = °C x 1.8 + 32
Pressure
Pressure is the force exerted over an area: P = F/A
What happens to pressure at higher elevations?
Pressure decreases at higher elevations
Simple mercury barometers were historically particularly useful because the high density of mercury allows a barometer to be only approximately 1 m tall to measure normal fluctuations in atmospheric pressure, which determined the height of the mercury. If a barometer reads a height of 1000 mmHg, what height would be read on a barometer using water instead? The density of mercury is 13.5 g/mL and that of water is 1 g/mL
A simple barometer setup has the height of the mercury controlled by the atmospheric pressure. We’re told that the reading of a barometer is 1000 mmHg, which means, using P = ρgh, that the pressure is P = (13.5 kg/L)(10 m/s2)(1 m) = 135 N/m2. That is the same pressure that a water barometer would experience. The issue is that water has a lower density. So we can set it up as 135 = (1)(10)h and therefore h = 13.5 m. This should make sense since mercury is 13.5 times denser so the water would need to be 13.5 higher to achieve the same pressure.
Ideal Gases
ideal gases occupy 22.4 L per mol of molecules.
Definition of Ideal Gas
- An ideal gas consists of pointy dots moving about randomly and colliding with one another and with the container wall. The ideal gas obeys the kinetic molecular theory of gases and has the following properties.
- Random molecular motion.
- No intermolecular forces.
- No (negligible) molecular volume.
- Perfectly elastic collisions (conservation of total kinetic energy).
At what pressures and temperatures can you treat gases as ideal gases?
- You can treat gases as ideal gases at:
- Low pressures
- High temperatures
Ideal Gas Law
PV=nRT, where P is pressure, V is volume, n is # mols of gas, R is the gas constant, and T is temperature
Combined Gas Law
Boyle’s Law
Boyle’s law: at constant temperature, P1V1 = P2V2
Charles Law
Charles’ law: at constant pressure
Kinetic molecular theory of gases - Assumptions
- Random molecular motion.
- No intermolecular forces.
- No (negligible) molecular volume.
- Perfectly elastic collisions (conservation of total kinetic energy).
The kinetic theory holds the following concepts about pressure and temperature:
- Pressure is equally distributed over the walls of the container because molecular motion is random.
- Higher temperature means the molecules are traveling faster, lower temperatures means slower molecules.
Diffusion
random molecular motion, causing a substance to move from an area of higher concentration to an area of lower concentration (diffusion down its concentration gradient).
Effusion
random molecular motion, causing a substance to escape a container through a very small openning.
Graham’s Law
(Rate1/Rate2) = √(M2/M1)
Kinetic Theory in terms of temperature and mass
(v1/v2) = √(m2/m1)
Van der Waals’ equation
b for bounce. The term with the constant b is the repulsion term. The greater b is, the more repulsion, which leads to greater pressure.
a for attraction. The term with the constant a is the attraction term. The greater a is, the more attraction, which leads to less pressure.
Partial pressure
Partial pressure = a component of the total pressure exerted by a species in a gas mixture.
The total pressure of a mixture of gas = The sum of all the partial pressures.
Mole Fraction
Mole fraction = a component (fraction) of the total # mols that belongs to a species in a gas mixture. Mole fraction for species A = # mols of A / # mols of the entire gas mixture. = # mols of A / Σ # mols of A, B, C …
Dalton’s law relating partial pressure to composition
Pi = χi·Ptotal
Ptotal = ΣPi = Σχi·Ptotal
Hydrogen bonding
Hydrogen bonding is a weak interaction between a partially positive H and a partially negative atom.
Technically, hydrogen bonds are a special type of dipole-dipole interaction.
Hydrogen bonding increases the boiling point.
Partially positive H are also called hydrogen bond donors. They are hydrogens that are bonded to either F, O, or N.
Partially negative atoms are also called hydrogen bond acceptors. They are most commonly F, O, or N.
Dipole-Dipole Interactions
All polar molecules exhibit dipole-dipole interactions. This is where the polar molecules align such that opposites attract.
Dipole-dipole interactions increase the boiling point, though not as significantly as hydrogen bonding.
Dipole interactions are stronger the more polar the molecule is.
Ion-Dipole Interactions
Ion-dipole interactions are similar to dipole-dipole interactions, but it’s stronger because it is no longer an interaction involving just partial charges. Instead, it is an interaction between a full charge (ion) and a partial charge (dipole).
Ion-dipole interactions get stronger when you have larger charge magnitude of the ion, and large polarity of the dipole molecule.
Van der Waals’ forces (London dispersion forces)
Dispersion forces exists for all molecules, but are only significant for non-polar molecules. For polar molecules, dipole forces are predominant.
Dispersion forces result from induced and instantaneous dipoles.
- Induced dipoles: when a polar molecule interacts with a non-polar molecule, then polar molecule induces a dipole in the non-polar molecule.
- Instantaneous dipoles: Non-polar molecules have randomly fluctuating dipoles that tend to align with one another from one instant to the next.
Phase Diagram
Molality
Molality = mols of solute / mass (in kg) of solvent.
Colligative properties
Colligative properties = properties that depend on the # of solute particles, but not on the type.
Van’t Hoff Factor (i)
all colligative properties take into consideration of the Van’t Hoff factor. Basically, it means convert concentration to reflect the total number of particles in solution. For example, glucose has i of 1 because it doesn’t break up in solution. NaCl has i of 2, because in solution, it breaks up into 2 particles Na+ and Cl-.
vapor pressure lowering (Raoult’s law)
ΔP = χsolute·P°solvent
boiling point elevation
ΔTb = kb·m·i
freezing point depression
ΔTf = -kf·m·i
osmotic pressure
π = MRT *i
π is the osmotic pressure; M is the molarity in mol/L; R is ideal gas constant; T is the temperature in K.
Osmosis
Osmosis is the movement of solvent across a semi-permeable membrane from an area of low solute concentration (high solvent concentration) to an area of high solute concentration (low solvent concentration).
Henry’s Law
Psolute = k [solute]