Chapter 6- Electronic Structure & Periodic Table Flashcards

1
Q

electromagnetic radiation

A

radiation consisting of electric and magnetic waves that travel at the speed of light

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2
Q

wavelength

A
  • distance between two consecutive peaks in a wave

- unit: m

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3
Q

frequency

A
  • number of waves (cycle) per second that pass a given point in space
  • unit: 1/s = hertz (Hz)
  • frequency = speed of light (c)/ wavelength
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4
Q

Max Planck’s Quantum Theory

A
  • light must be emitted and absorbed in discrete amounts

- light was before considered as a continuous electromagnetic wave

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5
Q

Equation for light

A
  • E = hv
  • h = 6.63 x 10^-34 J-s
    v = frequency
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6
Q

de Broglie’s wave equation

A

wavelength = h / mv (mass x velocity)

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7
Q

Lyman’s Series

A
  • results in ultraviolet emission of lines

- electron goes from n>=2 to n=1

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8
Q

Balmer series

A
  • results in visible emission of lines

- electron goes from n>=3 to n=2

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9
Q

Paschhen series

A
  • results in infrared emission of lines

- electron goes from n>=4 to n=3

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10
Q

Brackett series

A
  • results in infrared emission of lines

- electron goes from n>= 5 to n=4

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11
Q

Schrodinger Equation

A

predicts analytically and precisely the probability of events or outcome, predicts the probability of finding the particle

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12
Q

Heisenberg Uncertainty Principle

A

it is impossible to calculate both the momentum and the speed of an electron in an atom, only possible to calculate the probability of finding an electron

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13
Q

orbital

A

indicates electron’s probable location

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14
Q

node

A

an area of an orbital having zero electron probability

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15
Q

ground state

A

lowest possible energy state of an atom or molecule

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16
Q

excited state

A

any state of a particle or system of particles that has a higher energy than that of its ground state

17
Q

Pauli Exclusion Principle

A

no two electrons can have the same set of four quantum numbers

18
Q

Aufbau Principle

A

electrons fill orbitals starting at the lowest available energy state before filling higher states

19
Q

Hund’s Rule

A

single electron with the same spin must occupy each equal energy orbital before additional electrons with opposite spins can occupy the same orbital

20
Q

paramagnetic

A
  • atom has unpaired electrons

- attracted to a magnetic field due to unpaired electron

21
Q

diamagnetic

A
  • all electrons are paired

- weakly repelled by magnetic fields

22
Q

principal quantum number (n)

A

as n increases, the orbital becomes larger- electron has a higher energy level and is less tightly bounded to the nucleus

23
Q

angular momentum number (l)

A
  • values from 0 to n-1
  • defines shape of orbitals
  • 0 is S. 1 is P, 2 is D, and 3 is F
24
Q

magnetic quantum number

A
  • determines orientation of orbital

- values from -l to +l

25
Q

spin quantum number

A

either -1/2 or +1/2

26
Q

atomic radius

A
  • increases as you move down

- decreases as you move right

27
Q

shielding effect

A

lessening of attractive electrostatic charge difference between the nuclear protons and valence electrons by partially or fully filled inner shells

28
Q

effective nuclear charge

A

attractive positive charge of nuclear protons acting on valence electrons

29
Q

anion radius

A
  • larger than respective atoms

- electron electron repulsion forces them to spread further apart

30
Q

cation radius

A
  • smaller than respective atoms

- less electron electron repulsion, come closer together

31
Q

first ionization energy

A

energy required to remove the most loosely bound electron from a neutral atom in its GASEOUS state

32
Q

ionization energy

A
  • decreases as you move down (larger atomic radius)

- increases as you move right (smaller atomic radius)

33
Q

electron affinity

A
  • energy released when an atom gains an electron and becomes a negative ion
  • decreases as you move down (atomic radius increases)
  • increases as you move right (atomic radius decreases)
  • greater electron affinity = more negative