Observed Spectral Classes (TES)
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 |