T213 Planetary Exploration through Remote Compositional Analysis: The G.K. Gilbert Award Session
Tuesday, 2 November 2010
1:30 PM - 5:30 PM
Mile High Ballroom Prefunction
MINERALOGY OF MAWTH VALLIS, MARS, AS DETERMINED THROUGH ANALYSES OF CRISM IMAGES
Paper number: T213-10
Program: Technical Sessions
Time: 4:00 PM – 4:15 PM
Authors
-
Lee M. SaperBrown University, Providence, RI
-
Nancy K. McKeownGrant MacEwan University, Edmonton, AB
-
Mario ParenteBrown University, Providence, RI
-
Francois PouletInstitut d' Astrophysique Spatiale (IAS), Orsay
-
John F. MustardBrown University, Providence, RI
Abstract
Spectral analyses of the ferrous component in the CRISM images of Mawrth Vallis indicate that this material most frequently occurs together with the nontronite unit below it, that it sometimes occurs in combination with the Al-phyllosilciate unit above it and that in other cases it occurs with both the Fe/Mg-OH and the Al/Si-OH features. Analyses of lab spectra of phyllosilicates and phyllosilicate mixtures suggest that some Mg/Fe2+-chlorite minerals could be mixed with nontronite and not contribute changes to the spectral feature near 2.3 µm. Other clay minerals such as illite mixed with nontronite would change the spectral features and are inconsistent with our observations at Mawrth Vallis.
Detailed examination of the Mawrth Vallis spectra is showing the presence of smaller outcrops of phyllosilicates and hydrated components. We are continuing to analyze these in order to constrain likely formation scenarios for the Mawrth Vallis region including sedimentary and pedogenic processes.