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Group 1
Alkali Metals
Group 2
Alkaline Earth Metals
Group 3-12
Transition Metals
Group 17
Halogens
Group 18
Noble Gases
Isotope
Elements w/ diff numbers of neutrons
Coulombās Law
F is proportional to q1*q2/r² => q1:nucleus, q2:electron, r:distance between
Electrostatic Force
The attraction between opposite charges; calculated w/ coulombās law
ionization/binding energy
energy needed to remove an electron from an atom
aufbau principle
electrons are placed in shells, subshells, and orbitals in order of increasing energy
pauli exclusion principle
two electrons sharing an orbital must have opposite spins
hundās rule
when an electron is added to a subshell, it will occupy a free orbital. electrons will only pair up if there are no more free orbitals.
dipole
a pair of opposite electric charges sepparated by some distance
lattice energy
bond energy required to break ions out of ionic compounts
interstitial alloy
alloy made from atoms of vastly different radii; smaller atoms occupy the gaps between the larger ones
substitutional alloy
alloy made from alloys of similar radii
bond energy
energy required to pull apart bonded atoms
interneuclear distance
distance between nuclei of atoms
resonant structures
lewis structures that vary only in placement of lone electrons and double/triple bonds
formal charge
assigned electrons - valence eletrons of neutral atom (to judge most preferable lewis structure)
dipole moment
measurement of the separation between two oppositely charged atoms?
polarizability
tendency to distort electron density (causing a temporary dipole)
vapor pressure
pressure exerted by vapors (determined by IMF strength and temp: high IMF => lots of energy to escape into vapor phase => low pressure, high temp. => easier to break IMF => higher vapor pressure)
boiling point
temperature neessary to raise a substanceās vapor pressure up to the atmospheric pressure
partial pressure
x=moles of gas a/total moles of gas; partial pressure=x*total pressure
effusion
gas movement through tiny holes (ex: balloon deflating)
density
D=m/V or w/ ideal gas equation, D=P(Molar Mass)/RT
Daltonās Law
total pressure = sum of all the partial pressures
absorbance
amount of light at a certain wavelength absorbed by a molecule in a solution (calculated w/ Beerās law)
Beerās Law
Absorbtion=(molar absorbity, a constant depending on the molecule and wavelength used)(length of the bath of light through the solution - cm)(concentration of the solution) => A=ebc