S1.3 Electron configurations Flashcards
1
Q
how are emission spectra produced
A
by atoms emitting photons when electrons in excited states return to lower energy levels
2
Q
continuous spectrum
A
- in the visible region
- all colours
- all wavelengths
- all frequencies
3
Q
line spectrum
A
- Only has specific wavelengths
- Only has specific frequencies
- Only has specific energies of light
- Tells us that emitted light from atoms can only be at fixed frequencies → quantised
- Electrons can only have certain energy amounts
4
Q
radio waves
A
low energy
long wavelength
low frequency
5
Q
gamma rays
A
high energy
short wavelength
high frequency
6
Q
relationship between frequency and wavelength + the supporting equation
A
Speed of light (c) = vλ → frequency and wavelength are inversely proportional
7
Q
hydrogen line emission spectrum
A
- Provides evidence for the existence of electrons in discrete energy levels, which converge at higher energies
- As energy increases (frequency increases, wavelength decreases), lines converge so the electron is reaching a maximum amount of energy → ionisation energy
- The visible lines correspond to the electron jumping from higher levels to n=2
8
Q
n∞ → n=3
A
- paschen
- infrared region
- low energy
9
Q
n∞ → n=2
A
- balmer
- visible region
- medium energy
10
Q
n∞ → n=1
A
- lyman
- UV region
- high energy
11
Q
how is energy related to frequency and wavelength
A
- Wavelength determines colour
- If constant energy, the same colour will always be emitted
12
Q
principal quantum number (n)
A
- main energy level
- number of energy levels/quantum shells
- can hold a maximum of 2n^2 electrons
13
Q
what is the main energy level divided into
A
- sublevels/subshells of successively higher energies
- s, p, d, f
14
Q
s atomic orbital
A
- spherical
- low energy
- most likely to find electrons
15
Q
p atomic orbitals
A
- 3: x, y, z
- dumbbell
- higher energy than s
- lobes are larger and longer as n increases