Rutherford, Planck and Bohr Flashcards

1
Q

Rutherford

A
  • postulated that the atom had a dense, positively charged nucleus that made up only a small fraction of the volume of the atom
  • first to show atom being mostly empty space
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2
Q

Planck

A
  • developed the first quantum theory
  • Energy emitted as electromagnetic radiation from matter comes in discrete bundles called quanta
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3
Q

Planck Relation

A
  • determines energy of a quantum
  • E=hf
  • h is Planck’s constant (60626 x 10-34J•s)
  • f is the frequency of the radiation (sometimes designated by the Greek letter nu, v)
    • frequency of emitted radiation is proprtional to the energy of that radiation
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4
Q

Planck’s constant

A
  • 6.626 x 10-34J•s
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5
Q

Bohr Model of the Atom

A
  • A dense, positively charged nucleus is surrounded by electrons revolving aroung the nucleus in orbits with distinct energy levels
  • Bohr placed restrictions on the possible values of angular momentum
  • Bohr created an important conceptualization of atomic behavior but we now know electrons are NOT restricted to specific pathways but tend to be localized in certain regions of space
  • proved inadequate to explain the structure and behavior of atoms containing more than 1 electron
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6
Q

Bohr Formulas

A
  • L=nh/2π
  • E = - RH/n2
  • Angular momentum of an electron is directly proprtional to it’s Principle Quantum number
  • The energy of the electron increases expontially with the Principle Quantum Number
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7
Q

ground state

A
  • atom at the state of lowest energy (smallest, lowest-energy radius)
  • n=1
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8
Q

excited state

A
  • when at least 1 electron has moved to a subshell higher than normal energy
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9
Q

Atomic Emission Spectra

A
  • When electrons return from the excited state to the ground state, they emit an amount of energy that is exactly equal to the energy difference between the 2 levels
  • sometimes the electromagnetic energy emitted corresponds to a frequency in the visible light range
  • used as a fingerprint for the elements

**moves higher to lower

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10
Q

AHED

A
  • As electrons go from a lower energy level to a higher energy level, they get AHED
  • Absorb Light
  • Higher potential
  • Excited
  • Distant (from nucleus)
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11
Q

Electro magnetic Energy Emission of Photons equation

A
  • E=hc/λ
    • h = Plancks constant (6.626 x 10-34J•s)
    • c = speed of light (3.00 x 108 m/s)
    • λ = wave length of the radiation
    • combination of E=hf and c=fλ
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12
Q

Name the 3 series of hydrogen emission spectrum

A
  1. Lyman Series
    • group of H emission lines transitioning from n ≥ 2 to n = 1
    • larger energy transitions; therefore has shorter photon wavelengths
    • UV light
  2. Balmer Series
    • transitions from energy levels n ≥ 3 to n = 2
    • visable light
  3. Paschen series
    • transitions from n ≥ 4 to n = 3
    • infared
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13
Q

Equation for energy associated with a change in the principal quantum number

A

E = hc/λ = -RH [1/n2i - 1/n2f]

  • RH = Rydberg Unit of energy = 2.18 x 10-18 J/electron
  • energy of the emitted photon corresponds to the difference in energy between the higher-energy initial state and the lower-energy final state
  • wavelength of emitted proton is inversely proportional to the energy of that photon
  • the energy emitted or absorbed by an atom will increase as the energy level of the excited electron increases (decreases as energy level decreases)
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14
Q

Atomic Absorption Spectra

A
  • The atomic absorption spectra of an element is unique
  • for an electron to jump from a lower energy level to a higher one, it must absorb an amount of energy equal to the energy difference of the 2 levels
  • These wavelengths correspond to the wavelengths of emission
  • Identification of elements in the gas phase requires absorption spectra

**moves lower to higher

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