carbonate
CO₃²⁻
bicarbonate
HCO₃⁻
phosphate
PO₄⁻³
hydoxide
OH⁻
peroxide
O₂²⁻
cyanide
CN⁻
sulfate
SO₄²⁻
sulfite
SO₃²⁻
nitrate
NO₃⁻
nitrite
NO₂⁻
ammonium
NH₄⁺
acetate
C₂H₃O₂⁻ or CH₃COO⁻
charles law
V₁/T₁=V₂/T₂
avagadros law
V₁/n₁=V₂/n₂
boyles law
P₁V₁=P₂V₂
Lussac's Law
P₁/T₁ = P₂/T₂
Liters per mole at STP
22.4
density units
g/L
Density equation
p(mm)/RT or n(mm)/V
total pressure
((n1+n2)(RT))/V
daltons law
Ptotal=P₁+P₂+P₃...
mole fraction equation
(#moles)/total moles=Xa
partial pressure
Pa = (Ptotal)(Xa)
Kinetic Molecular Theory
gases are very small and spaced far apart 2.molecules are in constant random straight line motion
any collisions are perfectly elastic and no energy is lost or gained
the gas particles do not attract each other there are no intermolecular forces
kinetic energy formula
KE = 1/2 MV² (V= speed) mass is in kg V is in m/s and KE is in J
kinetic energy
KE=3/2 RT
root mean square velocity
Vrms = sqrt(3RT/MolarMass) molar mass is in kg/mol, use this for diffusion/effusion problems
Graham's law of effusion
V1/V2 = square root of mm2/mm1 2 gases must be at the same temp can be in grams per mol or rate of cold/rate of hot=sqrt Tcold/T-hot 1 gas, 2 temp temp is in kelvin
Hard Sphere Model
p(v-nb)=nrt larger molecules will have larger b
van der waals equation
(P+n²a/V²)(V-nb)=nRT a is for attractions
at high temp
KMT breaks down
molarity of 2 gases at the same temp and pressure
will be the same