thompson
plum pudding model
rutherford
sea of electrons
bohr
planetary model
wave velocity =
frequency*wavelength
emission line spectrum
shows how many times an electron transitioned from a higher to lower energy state; more lines means more energy
electromagnetic spectrum
balmer series
shows visible light
s sublevel
sphere shaped, 1 orbital
p sublevel
dumbbell shaped, 3 orbitals (px, py, pz), all the dumbbells together form a sphere
d sublevel
clover shaped, 5 orbitals, all the clovers together forms a sphere
f sublevel
flower shaped, 7 orbitals, all the flower
hund's rule
electrons fill unoccupied degenerate orbitals before pairing
pauli's exclusion principle
no two electrons can have the same 4 quantum numbers
plank's hypothesis
worked with electromagnetic waves; E = hv = plank's constant * frequency
plank's constant
6.626x10^-34
atomic spectra
produced when an electron moves from a higher to lower energy level, giving off light in the process; delta E = Ehi - Elo = hv = h*c/λ
bohr model
electrons move around the nucleus with a fixed radius, they absorb energy as as they get farther from the nucleus, and gives off energy yas it gets closer to the nucleus. this resulted in the emission spectra, which only happens as certain visible wavelengths.
wave/particle duality
plank said waves can act like particles
de broglie said E = hv = mc^2
experiments can only demonstrate one of these particles at a time
hiesnburg uncertainty principle: the momentum & position of a particle cannot be known at the same exact time. therefore, we can only refer to the probability of finding an electron in a region; we cannot specify the path
schrodinger
wave equations (ψ2) can be used to predict the region of probability for locating an electron
particle behavior
photoelectric effect (solar powered calculator)
wave behavior
refraction (changes speed in different media), defraction (bends around barriers), reflection
exceptions to the auf bau
electron promotion; an electron can be promoted from the s sublevel to the d sublevel for stability (half or full)
elements in the same group have
similar chemical properties & outer electron config
elements in the same period have
similar physical properties
coulombs law
strength of a bond
types of bonds
strong nuclear, weak nuclear, electromagnetic, gravitational
periodic trends
explained by Z effective force (how strong the nucleus is); represented by the numerator (q1 * q2)
groups trends
explained by quantum energy & shielding effect - electron penetration; represented by the denominator (r^2)
trends of the periodic table
shielding effect
the attraction between outer electrons and the nucleus decreases as the number of electrons between them and the nucleus increases, causing bonding situations
Z effective force
how strong a nucleus is; # of protons - # core electrons
ionization energy
the energy required to remove one electron from one gaseous atom
electron affinity
atoms ability to attract additional electrons; metals have a high electron affinty, non-metals have a low electron affinty
multiple ionization energies
looking at the table - remove valence electrons take less energy and removing core electrons take a lot more energy, as they are more stable. 2nd and 3rd ionization energys can give clues as to the atomic structure