Units 24-28 Flashcards
Energy Levels
the orbitals electrons move in
-quantized energy levels
Bohr Model of the Atom
describes the electron as orbiting at a set of discrete radii
Energy of Hydrogen eq
En=(-2.180 x 10^-18 J)/n^2
Emission line spectrum
the different light emission from a hot gas, containing different x
unique to elements
Balmer Lines
transitions between n=2 energy levels and higher levels
Continuous spectrum
atoms must be packed so that electron energy levels are altered so each atom can interact with photons of different energies therefore allowing photons of all lambda to be emitted
emission line spectrum
isolated atoms and molecules emit light only at certain wavelengths
produced by hot low density gas
absorption line spectrum
produced when light from a hot dense body passes through cooler gas. All colors are present but light at certain wavelengths is missing
radial velocity
an object moving directly away from us
Doppler formula
Vr=( delta lambda/lambda) x c
Redshifts
longer wavelength
Blueshifts
Shorter wavelength
Doppler Broadening
if atoms in a gas are moving, spectral lines will be spread over a wider range of wavelengths
Rest frame
A coordinate system tied to the solar system’s position and motion in which it appears we are at rest
Galilean relativity
how motions add to and subtract from one another
motions depend on rest frame