Jr. Johnson et al., Geological characterization of remote field sites using visible and infrared spectroscopy: Results from the 1999 Marsokhod field test, J GEO R-PLA, 106(E4), 2001, pp. 7683-7711
Upcoming Mars Surveyor lander missions will include extensive spectroscopic
capabilities designed to improve interpretations of the mineralogy and geo
logy of landing sites on Mars. The 1999 Marsokhod Field Experiment (MFE) wa
s a Mars rover simulation designed in part to investigate the utility of vi
sible/near-infrared and thermal infrared field spectrometers to contribute
to the remote geological exploration of a Mars analog field site in the Cal
ifornia Mojave Desert. The experiment simultaneously investigated the abili
ties of an off-site science: team to effectively analyze and acquire useful
imaging and spectroscopic data and to communicate efficiently with rover e
ngineers and an on-site field team to provide meaningful input to rover ope
rations and traverse planning. Experiences gained during the MFE regarding
effective communication between different mission operation teams will be u
seful to upcoming Mars mission teams. Field spectra acquired during the MFE
mission exhibited features interpreted at the time as indicative of carbon
ates (both dolomitic and calcitic), mafic rocks and associated weathering p
roducts, and silicic rocks with desert varnish-like coatings. The visible/n
ear-infrared spectra also suggested the presence of organic compounds, incl
uding chlorophyll in one rock. Postmission laboratory petrologic and spectr
al analyses of returned samples confirmed that all rocks identified as carb
onates using field measurements alone were cafe-silicates and that chloroph
yll associated with endolithic organisms was present in the one rock for wh
ich it was predicted. Rocks classified from field spectra as silicics and w
eathered mafics were recognized in the laboratory as metamorphosed monzonit
es and diorite schists. This discrepancy was likely due to rock coatings sa
mpled by the field spectrometers compared to fresh rock interiors analyzed
petrographically, in addition to somewhat different surfaces analyzed by la
boratory thermal spectroscopy compared to field spectra.