File:Absorption of Light by Hydrogen (01F8GFAYSYR6RP6EM83ZQ10XZ2).png
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[edit]DescriptionAbsorption of Light by Hydrogen (01F8GFAYSYR6RP6EM83ZQ10XZ2).png |
English: The relationship between a hydrogen atom and its absorption spectrum. (Left) A simple model of a hydrogen atom showing four of the many possible “jumps” the electron could make when it absorbs light. (Right) The relationship between the electron jumps and the specific wavelengths of light that the atom absorbs. An electron jumps from one energy level to another only when it absorbs a very specific wavelength of light (i.e., when it absorbs a photon with a specific energy). The shorter the wavelength, the higher the energy, and the greater the jump. Wavelengths that are absorbed appear as black lines in the spectrum. This illustration shows a set of jumps that correspond to absorption of visible wavelengths (the Balmer Series). |
Date | 2 July 2021, 19:30:00 (upload date) |
Source | Absorption of Light by Hydrogen |
Author | ILLUSTRATION: NASA, ESA, Leah Hustak (STScI) |
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[edit]Public domainPublic domainfalsefalse |
This file is in the public domain because it was created by NASA, ESA and CSA. NASA Webb material is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA/CSA is credited as the source of the material. This license does not apply if source material from other organizations is in use. The material was created for NASA by Space Telescope Science Institute under Contract NAS5-03127. Copyright statement at webbtelescope.org. For material created by the European Space Agency on the esawebb.org site, use the {{ESA-Webb}} tag. |
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