L2: Bohr's Model and Atomic Spectra

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7 Terms

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Problems with Rutherford’s Model

  • Orbiting electrons were acceleration, but there is no emission of EMR

  • Electrons are losing energy, but they are not spiralling towards the nucleus

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Continuous Spectrum

  • Heated solids, liquids, and dense gases

  • Emit light with a continuous spectrum (contains all frequencies)

  • There are no gaps in EMR due to the collisions between atoms

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Bright Line Spectrum (Studied)

  • Low pressure (rarefied) gases exposed to high voltages give off specific colours

  • Emitted EMR is due to the excited atoms themselves

  • Each element has a unique emission spectrum (classical theory could not explain why most frequencies were missing)

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Dark Line Spectrum (Evidence)

  • When white light passes through unexcited gas, there are dark lines in the spectrum

  • Wavelengths absorbed matched wavelengths emitted

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Bohr’s Energy Level Model

  • The spectra lines corresponded to differences between quantized energy levels in the hydrogen atom

  • Orbits in an atom are quantized

    • Each orbit corresponds to a particular energy level for the electron since the energy of an electron is quantized

    • Electrons can move between energy levels by emitting or absorbing energy equal to the difference between energy levels

  • Only light with certain frequencies &

    wavelengths can be emitted or absorbed by an atom

  • Energies of an electron within an atom are most often

    given relative to ionization

    • The zero point for energy is when electron is an infinite

      distance from nucleus

    • The negative sign means electron needs that much

      energy to be removed from atom (ie: to ionize atom)

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Transition Energy

  • Energy of the photon that an atom absorbs or emits

  • Conservation of Energy (PP5)

    • ΔEe- = Ephoton

    • Ef (energy in final orbit) - Ei (energy in initial orbit) = hf

  • Positive E = Photon emitted

  • Negative E = Photon absorbed

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Evaluate Bohr’s Model

  • Positive: Explained emission and absorption spectra for hydrogen (and other 1 electron atoms)

  • Negative:

    • Could not explain the spectra for more complex atoms and why only certain orbits are allowed

    • Could not explain why orbiting electrons did not emit EMR and why some lines were brighter than others