Chapter 3 Test Flashcards
(25 cards)
1
Q
Rutherford’s Contribution
A
- Electrons move in space randomly around the nucleus, beehive model
- e- account for the volume of atom
- nucleus accounts for mass of atom
2
Q
Rydberg’s Equation
A
- En = -RH/n^2
- RH is a constant value
- Calculates energy of e- in an energy level
3
Q
Electromagnetic spectrum concepts
A
- Radio, micro, infrared, UV, X-Ray, Gamma
- Longer wavelength (lambda) = lower frequency (nu) = lower energy
- Energy is proportional to frequency
- Frequency is inversely proportional to wavelength
- c = λv (c is speed of light, given)
4
Q
Visible length spectrum concepts
A
- (Red) 700nm to 400 nm (Violet)
- Colours of the rainbow from the least to most energetic: ROYGBIV
5
Q
Discontinuous spectrum
A
- Quantum: fixed amount of energy
- Energy quantized to specific levels…
- Separation and gaps
- Compare to a staircase
6
Q
Continuous spectrum
A
- All wavelengths of light are represented
- No gaps
- Compare to a ramp
7
Q
Emmision spectrum
A
- Spectrum of frequency of EM Radiatoin due to e- moving from high to low energy levels
- e- releases quantum energy as light as it moves down (6 to 1, 5 to 1, …)
8
Q
Emission series
A
- Different series depending on final energy level value
- Represented through emmision line spectrums for elements
- Lyman series: E(n) to E(n=1) - UV
- Balmer series: E(n) to E(n=2) - Visible
- Paschen series: E(n) to E(n=3) - Infrared Radiation
- Brackett series: E(n) to E(n=4) - Infrared Radiation
high E –> low E
Little BAbies Paint BRains
9
Q
Emmission Line Spectrum
A
- Ladder of energies
- Each element has own signature
10
Q
What are the four quantum numbers?
A
- Principle quantum number, n
- Angular momentum momentum quantum number, l
- Magnetic quantum number, ml
- Magnetic spin quantum number, ms
11
Q
Orbit model
A
- e- travel around nucleus in 2d pathway
- fixed distance
- No evidence exists
12
Q
Orbital model
A
- Region of probability where e- can be found
- 95% probability to find e-
- Can hold maximum 2 e-
- Different orbitals exist for different energy states, described by quantum numbers
13
Q
Principle quantum number
A
- Represented by n
- Represents energy level of e-
- Distance between e- and nucleus
- greater n = greater energy
14
Q
Angular momentum quantum number
A
- Represented by l
- Represents types and shapes of orbitals within each quantum level
- Restriction l<n
- s, p, d, f orbitals! s=0, p=1, d=2, f=3
- s orbitals: 1 spherical orbital (2e- max)
- p orbitals: 3 degenerate perpendicular/dumbbell orbitals (6e- max)
*d orbitals: 5 degenerate diffuse orbitals (10e- max) - f orbitals: 7 degenerate fundamental orbitals (14e- max)
- Relative energy of orbitals: s<p<d<f
15
Q
Magnetic quantum number
A
- Represented by ml
- Indicates 3D orientation/specific plane the e- in an orbital is found in
- Restriction: -l<=ml<=l
- s orbitals have 1 ml = 0
- p orbitals have 3 ml = -1, 0, 1 (x,y,z)
etc.
16
Q
Magnetic spin quantum number
A
- Represented by ms
- Direction of e- spin
- Can either be ms = 1/2 (up) or ms = -1/2 (down)
- Each orbital can hold max 2 electrons w/ opposite spin
17
Q
Afbau principle
A
- e- will fill lowest energy levels before higher ones are filled
- ex: 4s is filled first because it has less energy than 3d
- FOLLOW PERIODIC TABLE TO MAKE DIAGRAM!
18
Q
Pauli exclusion principle
A
- each orbital holds a max of two e- w opposite spin
- connects with ms
- 2e- of the same spin in one orbital cannot be true
19
Q
Hund’s rule
A
- When there are degenerate orbitals in a sublevel (ml), electrons will half fill each orbital before pairing up
- e= dont want to be together unless they have to!
19
Q
Electron configuration for ions
A
- Cation/+: electrons are lost from outermost shell/highest n value from highest energy orbital
- Anions/-: electrons are gained to nearest orbitals that are nolt yet full
20
Q
Paramagnetic
A
- Elements with unpaired electrons
- attracted to a magnetic field
21
Q
Diamagnetic
A
- Elements with paired electrons
- Repelled by a magnetic field
22
Q
Ground state
A
- Valence electrons are found in order we would predict
- 1s2,2s2,2p6, etc
- close to the nucleus as possible
23
Q
Excited state
A
- Electron configuration is out of order and unpredicted
- energy levels further from the nucleus
- Look for a gap while following periodic table
24
Exceptions to the electron configurations
* Group 6: Chromium (Cr), Molybdenum (Mo)
* Group 11: Copper (Cu), Silver (Ag), Gold (Au)
* d orbitals become filled (10e-) or half filled (5e-)
* s2 orbitals become s1 (loses an e- to a d orbital)