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Observed Spectral Classes (TES)
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Caption:
Surface, atmospheric dust, and atmospheric water-ice clouds have been observed as approximate spectral end-members as well as in combinations. Note the deep 15-micron line for atmospheric CO 2 and the near 7 micron water vapor lines.
Cataloging Keywords:
| Name | Value | Additional Values |
|---|---|---|
| Target | Mars | |
| System | ||
| Target Type | Planet | |
| Mission | Mars Global Surveyor (MGS) | |
| Instrument Host | Mars Global Surveyor | |
| Host Type | Orbiter | |
| Instrument | Thermal Emission Spectrometer (TES) | |
| Detector | ||
| Extra Keywords | Atmosphere, Color, Dust, Water | |
| Acquisition Date | ||
| Release Date | 1999-06-23 | |
| Date in Caption | ||
| Image Credit | NASA/JPL/ASU | |
| Source | photojournal.jpl.nasa.gov/catalog/PIA02062 | |
| Identifier | PIA02062 | |
