CHE Final Exam Flashcards
Alpha and beta particles
Positively and negatively charged particles, respectively
Gamma rays
Neutral charge, high-energy radiation
Nuclear theory
Supported by Rutherford’s experiment:
nucleus = most of atom’s mass w/protons & neutrons
empty space = most of atom’s space w/electrons
Polyatomic molecules in nature
P4
S4
Se4
O3
Noble metals
Ag, Pt, Au
Transition metals with predictable charge (3)
Ag (1B = 1+)
Zn (2B = 2+)
Cd (2B = 2+)
1 prefix (HC)
meth-
2 prefix (HC)
eth-
3 prefix (HC)
prop-
4 prefix (HC)
but-
HC suffixes (single, double, & triple bonds)
-ane, -ene, -yne
Alkanes
Hydrocarbons with only single bonds (-anes)
Percent yield
% yield = ( actual / theoretical ) * 100%
*NOT PERCENT ERROR!
Dilution formula
M1V1 = M2V2
M = molarity, V = volume (liters)
Dissociation
Ions of a salt separate when dissolved
Ionization
Process of ion formation in solution
(acids, bases)
Arrhenius acids & bases
Acids produce H+ (H3O+) in water
Bases produce OH- in water
Brønsted acids & bases
Acid = proton donor
Base = proton acceptor
Monoprotic, diprotic, and tripotic acids
Each unit of acid yields one, two, and H+ ion(s) respectively
Neutralization reaction result
salt + water + heat
Gas-evolving reactions & compounds (4)
Acid + salt –> salt + gas + water
Sulfides
Bicarbonates
Bisulfites
Ammonium
Oxidation half-reaction
Shows loss of electrons (OIL)
Reduction half-reaction
Shows the gain of electrons (RIG)
Oxidizing agents
Are reduced (RIG)
Reduction agents
Are oxidized (OIL)
Disproportionation reaction
Same element is simultaneously oxidized & reduced
Modified dilution equation
MacidVacid(# of H+) = MbaseVbase(# of OH-)
Pressure unit conversion
760 mmHg = 760 torr = 1 atm = 101,325 Pa
Molar mass of gas formula
M = dRT/P
molar mass = (density) * R * (Kelvin) / (atm)
D = PM/RT
= pressure * molar mass / R * temp
Average KE
Constant tempterature: gases have same average KE
Root mean square velocity
urms = (3RT/M)1/2
R = J/mol K T = Kelvin M = kg/mol
Graham’s law of effusion
ra/rb = (M<span>b</span>/M<span>a</span>)1/2
Real gases
Behavior differse at high pressure/low temperature
Energy unit conversion (4 equalities)
1 J = 1 kg*m2/s2
1 cal = 4.184 J
1 Cal = 1kcal
1 L*atm = 101.3 J
Internal energy & change in internal energy
E (internal energy) = KE + PE
ΔE = Eproducts - Ereactants
ΔE = q + w
*+w work done ON system, -w work done BY system
ΔEsystem = -ΔEsurroundings
Pressure-volume work
w = -PΔV
work = negative of external pressure * change in volume
Enthalpy/change in enthalpy formula
Enthalpy = H
H = E + PV
(internal energy + pressure*volume)
ΔH = ΔE + PΔV
ΔH = Hproducts - Hreactants
Heat capacity
q = C * Δt
Amount of heat to raise temperature by 1°C
C = J/°C or J/K
System absorbs heat = temperature increasse
Specific heat capacity
q = m * Cs * Δt
Measure of substance’s ability to absorb heat/amount of heat required to raise 1 g of substance by 1°C
Bomb calorimeter
Constant-volume calorimetry
ΔErxn = qv = qrxn = -qcal
qcal = Ccal * ΔT = -qrxn
Coffee-cup calorimetry
Constant-pressure calorimetry
ΔHrxn = qp = qrxn = -qsoln
qsoln = msoln * Cs, soln * ΔT = -qrxn
Standard enthalpy of formation
ΔHf°
Heat change when one mole is formed from elements at 1 atm
Most stable = 0
Stable liquids: Hg, Br
Stable gases: H2, N2, O2, F2, Cl2, noble gases
Graphite is stable, diamond is not
S8 rhombic is stable
Standard enthalpy of a reaction
The enthalpy of a reaction carried out at 1 atm
ΔHrxn° = ΣnproductsΔHf° - ΣnreactantsΔHf°
Hess’ law
ΔHrxn° = ΔH1° + ΔH2°
Frequency formula
v = c / λ
Electromagnetic spectrum
Low energy to high:
radio
microwave
infared
visible light
ultraviolet
X-ray
gamma ray
Photoelectric effect
Many metals emit electrons when light shines on surface
Number of photons formula
Number of photons = Epulse / Ephoton
*Ephoton = hc/λ
Energy & frequency combined formula
v = c / λ
E = hv
E = hc/λ
Wavelength formula
λ = h/mv
Planck’s constant / mass * velocity
Energy of electron orbital change formula
ΔEH atom = -R (1/n2final - 1/n2initial)
R = Joules
1 Hz = ? s-1
1 Hz = 1 s-1
Pauli exclusion principle
No two electrons can have same four quantum numbers
Orbital = 2 electrons max
Aufbau principle
Lower energy orbitals fill before higher energy orbitals to minimize energy of atom
Hund’s rule
Electrons first occupy orbitals of equal energy singly with parallel spins
Transition elements with irregular electron configurations (10)
- Cr (Chromium) 24
- Cu (Copper) 29
- Nb (Niobium) 41
- Mo (Molybdenur) 42
- Ru (Rutherium) 44
- Rh (Rhodium) 45
- Pd (Palladium) 46
- Ag (Silver) 47
- Pt (Platinum) 78
- Au (Gold) 79
Van der Waals radius
Nonbonding radius of an atom
Cation v. anion radius size
Cations < anions
Except Rb+ and Cs+ are larger than F- and O2-
Periodic trends in first ionization energy
The larger the Zeff, the more energy it takes to remove it.
*IE1 increases to the right
**Except: Group 2A to 3A & Group 5A to 6A
The farther the electron is from the nucleus, the less energy it takes to remove it
*IE1 decreases toward the bottom
Electron affinity
X (g) + e- → X- (g) + EA
The energy released (-kJ/mol) when a neutral gaseous atom gains an electron
The more energy released when electron is gained, the more negative the EA (-kJ/mol)
*INCREASES TO THE RIGHT
Diagonal relationship
- Li & Mg
- Be & Al (Al is a metal like 2A)
- B & Si (metalloids)
Similar because of charge density (ion charge / volume)
Properties of oxides across a period (3)
- Metals/Groups 1A/2A form basic oxides
- Nonmetals form acidic oxides
- Al form amphoteric oxides (both basic/acidic)
Formal charge (4)
Charge an atom would have if all bonding electrons were shared equally
FC of an atom = Valence e- - nonbonding e- - (1/2)(bonding e-)
- Sum of all formal charges in neutral molecule = 0
- Sum of all formal charges in ion = ion charge
- Small (or zero) formal charges on individual atoms are better than large ones
- When formal charge cannot be avoided, negative formal charge should reside on the most electronegative atom
The Clausius-Clapeyron Equation
ln P2/P1 = (-ΔHvap/R) (1/T2-T1)
R = 8.314 J/mol K
T = in Kelvin
Equation for heat involved in completion of a phase change
q = nΔHtransition
heat = # of mols * heat of [transition]
Equation for heat involved in temperature change
q = (m) (Cs) (ΔT)