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Hydrogen produces emission lines (colored lines on the spectrum) with the following wavelengths: 410 nm, 434 nm, 486 nm and 656 nm. Where would you expect to see the absorption lines (dark lines) for hydrogen on its absorption spectrum and why? The absorption lines for hydrogen would appear at exactly the same O wavelengths because the energies of the photons emitted and absorbed by hydrogen are the same. The absorption lines for hydrogen would appear at shorter wavelengths than O the emission lines because the energies of the photons absorbed are higher than the energies of the photons emitted by hydrogen. The absorption lines for hydrogen would appear at longer wavelengths than O the emission lines because the energies of the photons absorbed are lower than the energies of the photons emitted by hydrogen. The absorption lines for hydrogen would be red-shifted because of the doppler effect.

Hydrogen produces emission lines (colored lines on the spectrum) with the following wavelengths: 410 nm, 434 nm, 486 nm and 656 nm. Where would you expect to see the absorption lines (dark lines) for hydrogen on its absorption spectrum and why? The absorption lines for hydrogen would appear at exactly the same O wavelengths because the energies of the photons emitted and absorbed by hydrogen are the same. The absorption lines for hydrogen would appear at shorter wavelengths than O the emission lines because the energies of the photons absorbed are higher than the energies of the photons emitted by hydrogen. The absorption lines for hydrogen would appear at longer wavelengths than O the emission lines because the energies of the photons absorbed are lower than the energies of the photons emitted by hydrogen. The absorption lines for hydrogen would be red-shifted because of the doppler effect.

Chemistry for Engineering Students
Chemistry for Engineering Students
4th Edition
ISBN:9781337398909
Author:Lawrence S. Brown, Tom Holme
Publisher:Lawrence S. Brown, Tom Holme
Chapter6: The Periodic Table And Atomic Structure
Section: Chapter Questions
Problem 6.103PAE: 6.103 Atomic absorption spectroscopy is based on the atomic spectra of the elements being studied....
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Hydrogen produces emission lines (colored lines on the spectrum) with the following wavelengths: 410 nm, 434 nm, 486 nm and 656 nm. Where would you expect to see the absorption lines (dark lines) for hydrogen on its absorption spectrum and why? The absorption lines for hydrogen would appear at exactly the same wavelengths because the energies of the photons emitted and absorbed by hydrogen are the same. The absorption lines for hydrogen would appear at shorter wavelengths than the emission lines because the energies of the photons absorbed are higher than the energies of the photons emitted by hydrogen. The absorption lines for hydrogen would appear at longer wavelengths than O the emission lines because the energies of the photons absorbed are lower than the energies of the photons emitted by hydrogen. The absorption lines for hydrogen would be red-shifted because of the doppler effect. O
Transcribed Image Text:Hydrogen produces emission lines (colored lines on the spectrum) with the following wavelengths: 410 nm, 434 nm, 486 nm and 656 nm. Where would you expect to see the absorption lines (dark lines) for hydrogen on its absorption spectrum and why? The absorption lines for hydrogen would appear at exactly the same wavelengths because the energies of the photons emitted and absorbed by hydrogen are the same. The absorption lines for hydrogen would appear at shorter wavelengths than the emission lines because the energies of the photons absorbed are higher than the energies of the photons emitted by hydrogen. The absorption lines for hydrogen would appear at longer wavelengths than O the emission lines because the energies of the photons absorbed are lower than the energies of the photons emitted by hydrogen. The absorption lines for hydrogen would be red-shifted because of the doppler effect. O
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