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Density Formula
d= (p*MM)/RT
Gas Laws
p1V1=p2V2 p1/T1=p2/T2
total pressure
sum of all partial pressures
Calculating ΔH
final energy-initial exo: ΔH of the system is negative endo: ΔH of the system is positive
Breaking Bonds is.... Forming Bonds is...
breaking: endothermic forming: exothermic
Exothermic Reactions
combination (can be endo), single displacement, combustion
Endothermic Reactions
decomposition (can be exo), vaporization, melting
What is ΔH?
heat transferred when the reaction is carried out under conditions of constant pressure
specific heat of water
4.18 J/gCelsius
q always refers to what?
the surroundings
relationship between wavelength and frequency if c is constant
inversely proportional
wavelength for: red light blue light
red: 700nm blue: 400 nm
photon
smallest unit of light energy energy of photon=hv
Visible Light (Infrared to UV)
wavelength decreases frequency increases Ephoton increases
When light is absorbed by matter...
individual atoms or molecules absorb 1 photon at a time
3 Labels to characterize an orbital
n, l, ml
n
quantum number determines energy and size of orbital
l
quantum number defines overall shape of electron cloud
ml
quantum number defines orientation of the orbital
Differences between H and other atom
energies of orbitals decrease as protons added energies depend on n and l
Magnetic properties
you have to have one or more unpaired electron
paramagnetic
with one or more unpaired electron and it's magnetic
diamagnetic
with no unpaired electron
Exceptions to electron configuration
Cu, Ag, Au, Cr
Ionization Energy
-energy needed to remove highest energy electron from the atom -ranges from 400 - 2400 kJ/mol -always an endothermic process -increases as you move up and to the right of periodic table
Electron Affinity
-energy needed to add an electron to an atom -often exothermic -halogens have most exothermic EA -noble gases have endothermic values -small compared to IE -ranges from 350 to -50 kJ/mol -increases as you move up and to the right to the periodic table
Atomic Size
related to size of the largest valence orbital of the atom large orbital=large atomic size=small IE small orbital=small atomic size=large IE increases as you move down and to the left of the periodic table
Electronegativity
ability of an atom to attract an electron to it from another atom to which it is bonded -increases as you move up and to the right to periodic table
Large and Small EN
Large: high electron attracting power -active non-metals Small: low electron attracting power -active metals
EN: 0.7-1.5 2.5-4.0 2.0 2.1
0.7-1.5: fairly active metal 2.5-4.0: fairly active non-metal 2.0: metalloids 2.1: hydrogen
Exceeds Octet rule
3rd and 4th period
-ane -ene -yne
-ane: single bond -ene: double bond -yne: triple bond
Bond length and dissociation energy
bond length decreases from single to triple dissociation energy increases from single to triple
Exceptions to Octet Rule
-species with odd number of electrons -elements beyond 2nd period -electron deficient species
1 atm=
76cmHg = 760 mmHg
Atmospheric pressure and altitude
pressure decreases when altitude increases
at constant n and T: p and V are...
inversely proportional
at constant n and V: p and T are...
directly proportional
molecular speed increases with... and decreases with...
temperature and increasing mass
Hess's Law
No matter how many steps you go through to get a reaction, the enthalpy change is always the same
Boyle's Law
pressure and volume are inversely related when at a given temperature
Kinetic Theory of Ideal Gas
1. Molecules spread out in space so separation > molecular size 2. Molecules moving rapidly 3. Pressure due to molecules bouncing off walls of container 4. Gas molecules collide and are elastic
mole fraction
Xa= (Na/Ntotal)=(Pa/Ptotal)
Hund's Rule
In a set of orbitals with the same energy, electrons tend to occupy different orbitals with the same spin.
paulie exclusion principle
states that a max of 2 electrons can occupy a sungle orbital , but only if the electrons have opposite spins
Gas Laws in General:
(P1*V1)/(n1/T1)=(P2*V2)/(n2/T2)
Rules for determining delta H from bond energies
bonds broken-bonds formed
y2
y2 is the probability of finding the electron in a small volume at a distance r from the nucleus -part of Schrodinger equation
Diamagnetic
all spins are paired, not attracted to a magnetic field
paramagnetic
unpaired spins, attracted to a magnetic field

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