1 Atomic Structure Flashcards
valence electrons
outermost shell of electrons –> higher energy
have strongest interactions with surroundings
isotopes
varying mass numbers
atomic weight
weighted average of different, naturally occurring, isotopes
Avogadro’s number
1 mole = number of whatever “things” one is concerned about
= 6.02 x 10^23
Planck relation
energy omitted as electromagnetic radiation from matter
comes in discrete bundles called quanta
Planck’s equation
E = hf
h = Planck’s constant = 6.626 x 10^(-34) J s
Bohr’s model
angular momentum of electrons orbiting hydrogen nucleus
Bohr’s equation
L = n h / 2 pi
energy of electron orbiting hydrogen nucleus
E = -R(H) / n^2
ground state
state of lowest energy of atom
(all electrons in lowest possible orbitals)
all systems tend towards minimal energy)
excited state
at least 1 electron moves to subshell of higher than normal energy
atomic emission spectra
fingerprints of electron transition
identifies element by line spectra
application of Bohr’s model
equation for energy of emitted photon
E = hc / lambda = -R(H) [(1/n(i)^2) - (1/n(f)^2)]
atomic absorption spectra
at specific wavelengths
accurate to make electro transition to “excited”
also a fingerprint (element-specific)
required when element is in gas phase
application of Bohr’s model
orbitals
electrons move rapidly around nucleus – localized to regions