11. Bob is traveling in a space ship and observes emission from a cloud of atomic hydrogen gas a few light years away. He identifies the Balmer-beta emission line (from the n = 4 to n = 2 transition) and measures its wavelength to be 322 nm. How fast is Bob moving relative to the cloud of hydrogen? Is he getting closer or further away from the hydrogen cloud? (You may assume that Bob is moving directly toward or away from the hydrogen gas cloud. Recall that the ground state energy of hydrogen is -13.6 eV.)

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Chapter1: Units, Trigonometry. And Vectors
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11. Bob is traveling in a space ship and observes emission from a cloud of atomic hydrogen
gas a few light years away. He identifies the Balmer-beta emission line (from the n = 4
to n = 2 transition) and measures its wavelength to be 322 nm. How fast is Bob
moving relative to the cloud of hydrogen? Is he getting closer or further away from the
hydrogen cloud? (You may assume that Bob is moving directly toward or away from
the hydrogen gas cloud. Recall that the ground state energy of hydrogen is -13.6 eV.)
Transcribed Image Text:11. Bob is traveling in a space ship and observes emission from a cloud of atomic hydrogen gas a few light years away. He identifies the Balmer-beta emission line (from the n = 4 to n = 2 transition) and measures its wavelength to be 322 nm. How fast is Bob moving relative to the cloud of hydrogen? Is he getting closer or further away from the hydrogen cloud? (You may assume that Bob is moving directly toward or away from the hydrogen gas cloud. Recall that the ground state energy of hydrogen is -13.6 eV.)
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