Chapters 6 & 7 Flashcards

1
Q

electronic structure (of atoms)

A

arrangement and energy of electrons

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2
Q

Electromagnetic radiation (radiant energy)

A

carries energy through space
- moves at speed of light (c)

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3
Q

C =

A

c = λv
c = 3.00 x 10^8 m/s

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4
Q

wavelength (λ)

A

distance b/w 2 wave peaks
- meters (or nm)

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5
Q

Frequency(v)

A

of complete cycles (wavelengths) that pass a given point/second
- v = 1 s^-1

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6
Q

Electromagnetic Spectrum

A

electromagnetic radiation arranged in increasing wavelength

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7
Q

blackbody radiation

A

emission of light from hot objects

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8
Q

photoelectric effect

A

emission of electrons from metal surfaces which light in shone

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9
Q

emission spectra

A

emission of light from electronically excited gas atoms

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10
Q

Quantum physics

A

physics to describe atoms

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11
Q

Quantum theory

A

to describe electronic structure of atoms

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12
Q

Photoelectric effect

A

every metal has diff energy level which ejects e-

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13
Q

Planck’s constant: E=

A

E = hv
- to calculate the energy required to remove an electron

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14
Q

Emission spectra

A

observed energy emitted when electric current is passed thru
- radiation–>component wavelengths

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15
Q

Continuous spectrum

A

(the “rainbow”) from white light source

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16
Q

Line spectrum

A

radiation of only specific wavelengths; discrete wavelengths observed
- each element = unique line spectrum

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17
Q

Rydberg formula

A

1/λ = (RH)x((1/n1^2) - (1/n2^2))
- RH = 1.096 x 10^7 m^-1

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18
Q

Bohr equation

A

∆E = Ef-Ei
- ∆E = (-2.18 x 10^-18 J)(1/n^2-1/n^2)

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19
Q

ground state

A

lowest energy state of atom
- n=1

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20
Q

excited state

A

higher energy state of atom
- n=2+

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21
Q

λ =

A

h / mv

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22
Q

Heisenberg Uncertainty Principle

A

can’t know both momentum and position of a particle

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23
Q

Wave functions

A

describes the electron (orbital) and its energy

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24
Q

electron density

A

probability e- can be found in specific location

25
Q

orbitals

A

hold 2 electrons

26
Q

electron shell (n)

A

orbitals w/ same n value
- ex: all orbitals w/ n=3 = third orbital

27
Q

subshell

A

diff orbital types w/in shell

28
Q

s orbital

A

L = 0
- spherical

29
Q

p orbital

A

L = 2
- 2 lobes w/ 1 node

30
Q

f orbital

A

L = 3

31
Q

degenerate orbitals

A

orbitals at same energy level; n =

32
Q

electron spin

A

describes magnetic field; (+/-) 1/2

33
Q

pauli exclusion principle

A

each electron in atom must have distinct quantum numbers; need image to describe

34
Q

electron configurations

A

way electrons are distributed in an atom
- orbitals filled in order of increasing energy
- n = energy level
- letter = type of orbital
- superscript = number of electrons in orbitals

35
Q

ground state

A

most stable organization at lowest possible energy

36
Q

orbital diagram

A

each orbital denoted by box and electron by half arrow

37
Q

Hund’s rule

A

“sharing is caring”
- there must be 1 e- (w/ same spin) per orbital before pairing with 2nd opposite spin

38
Q

Valence electrons

A

same group (↓) have same # of e- in outer shell; part after [ ]

39
Q

core electrons

A

filled inner-shell electrons; part in [ ]

40
Q

transition elements

A

10 elements touching step-line
- d-block

41
Q

Lanthanide elements

A

4f

42
Q

Actinide elements

A

5f

43
Q

Periodicity

A

repetitive pattern of property for elements based on atomic number

44
Q

effective nuclear charge (Zeff)

A

Zeff = Z – S
feel pull of nucleus more:
- changes w/ # of protons
- increase Zeff = increase nucleus size = incr. pull
- decrease Zeff = decr. nucleus size = decr. pull

45
Q

Slater’s Rules

A

ignore all outer e- beyond one of interest

46
Q

Nonbonding radius (van der Waals radius)

A

½ shortest distance separating 2 nuclei during collision of atoms

47
Q

Bonding atomic radius (covalent radius)

A

½ distance b/w nuclei in a bond
- Can’t get any closer bc of core e- repulsion
- Bonding radius < nonbonding radius

48
Q

cations

A
  • smaller than parent atoms
  • e- removed
  • repulsions b/w e- = reduced
49
Q

anions

A
  • larger than parent atoms
  • e- added
  • repulsions b/w e- = increased
50
Q

isoelectronic series

A

ions have the same # e-, diff # of protons
- calculate number of ions and compare

51
Q

Ionization energy

A

energy required to remove 1 e- from ground state of a gaseous atom or ion
- larger ionization energy # = more difficult to remove e-

52
Q

first ionization energy

A
  • removing e- from gaseous element
    ex: Al (g) –> e- + Al+ (g)
53
Q

Electron affinity

A

measures attraction/affinity of atom for added electron

54
Q

Ionization energy measures energy change when atom __ e-

A

loses

55
Q

Electron affinity measures energy change when atom __ e-

A

gains

56
Q

increasing atomic radius

A

Increasing:
- right to left
- top to bottom
(same as increasing metallic character)

57
Q

increasing ionization energy

A

Increasing:
- left to right
- bottom to top
(same as increasing electron affinity)

58
Q

increasing electron affinity

A

Increasing:
- left to right
- bottom to top
(same as increasing ionization energy)

59
Q

increasing metallic character

A

Increasing:
- right to left
- top to bottom
(same as increasing atomic radius)