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Mars Methane Spectroscopy


Conceptual animation demonstrating the process of spectroscopy. The first animation demonstrates the general concept of visible-light spectroscopy by which white light is separated into its component wavelengths (colors) using a prism. The second animation demonstrates how this idea is applied to the discovery of methane in Mars' atmosphere. Because it absorbs specific wavelengths of electromagnetic energy, methane has a 'fingerprint' that can be seen as missing lines on the resulting spectograph.    Conceptual animation demonstrating the process of spectroscopy. The first animation demonstrates the general concept of visible-light spectroscopy by which white light is separated into its component wavelengths (colors) using a prism. The second animation demonstrates how this idea is applied to the discovery of methane in Mars' atmosphere. Because it absorbs specific wavelengths of electromagnetic energy, methane has a 'fingerprint' that can be seen as missing lines on the resulting spectograph.
Duration: 29.0 seconds
Available formats:
  1280x720 (30 fps) QT         9 MB
  640x360 (29.97 fps) MPEG-4   3 MB
  320x180 (29.97 fps) MPEG-4   1017 KB
  320x240 (29.97 fps) MPEG-4   658 KB
  640x360 (29.97 fps) MPEG-1   6 MB
  512x288 (29.97 fps) MPEG-1   4 MB
  1280x720 (29.97 fps) QT         140 MB
  1280x720 (29.97 fps) QT         6 MB
  320x180     PNG           60 KB
  160x80       PNG           19 KB
  80x40         PNG           6 KB
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Animation Number:10360
Completed:2008-12-23
Animator:Chris Smith (UMBC) (Lead)
Producer:Chris Smith (UMBC)
Scientist:Michael Mumma (NASA/GSFC)
Series:Mars Methane
Keywords:
SVS >> HDTV
SVS >> Mars
SVS >> Methane
More Information on this topic available at:
http://www.nasa.gov/mission_pages/mars/news/marsmethane.html
 
 
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NASA/Goddard Space Flight Center


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