File:Spectroscopic Analysis of Three Planets (4183-Image).png

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English: Spectroscopy can identify planets capable of supporting life. Note the differences between the spectroscopic data of these three solar system planets; Mars, Earth, and Venus. Dips indicate varying types of gases in their atmospheres. Although all three planets show a significant dip in the spectroscopic data for carbon dioxide, only Earth clearly shows the presence of water, ozone, and carbon dioxide.
Date 21 May 2018 (upload date)
Source Spectroscopic Analysis of Three Planets
Author NASA and C. Godfrey (STScI)

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Public domain 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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current23:22, 25 November 2022Thumbnail for version as of 23:22, 25 November 20224,000 × 2,545 (2.38 MB)OptimusPrimeBot (talk | contribs)#Spacemedia - Upload of https://stsci-opo.org/STScI-01EVT0DW2RHZ0BX3KQ8H7886W2.png via Commons:Spacemedia

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