Oct 2nd 1 hour Exam
Chapter 9- Thermodynamics
KE= ½ mv2
w= F∆x w= force × distance
∙ A state function refers to a property of the system that depends only on its present state.
∙Internal Energy = heat + work
∆E = q + w
∙Pressure = Force/Area = P = F/A
∙Work= - external pressure × change in volume w = - P∆V
Enthalpy
H = E + PV qp = ∆E + P∆V
∆H = qp
∆H = H products H reactants
Ideal Gas Law
PV = nRT
Energy "heat" = 3/2 R∆T
Cv = 3/2 R = "heat" required to change the temp of 1 mol of gas by 1K at constant volume Energy required = "heat" energy needed - energy needed to do to change the translational the …show more content…
∙ As n increases, the size of the orbital increases, and the electron is easier to remove.
∙ Exceptions :
Be to B decrease in IE shows that the electrons in 2s orbital effectively shield the 2p electron.
N to O- drop in IE because of addition of electron in first p orbital that results in a pair that repel each other and make either of them easier to remove.
Electron Affinity
X(g) + e-→ X- (g)
∙ Down a group more positive since electron is added at increasing distances from the nucleus.
∙ Increase across period because effective nuclear charge is increasing.
Electronegativity = (Electron Affinity + Ionization Potential)/2
Lattice Energy
Li+ (g)+ Cl- (g) → LiCl(s)
Lattice Energy = k(Q1Q2)/r
∆H = ∑ D(Bonds broken) - ∑D(Bonds