CHARACTERIZING THE EXTENT OF HYDROTHERMAL ACTIVITY IN GUSEV CRATER, MARS
To better understand the extent of past hydrothermal activity, we have analyzed the full suite of Pancam multispectral images of all bright soil exposures. Previously, the soils Arad, Paso Robles, Gertrude Weise, Tyrone and Ulysses were found to have spectra indicating potentially hydrothermal mineralogies, with opaline silica and Fe-, Mg- and Ca-sulfates. In our analysis of six additional bright soil exposures, we found evidence of similar mineralogies, in addition to new spectral endmembers that have yet to be fully modeled. We have also studied all available CTX and HiRISE images of Gusev crater to search for additional hydrovolcanic features (e.g., candidate vent structures and “Home Plate-like” features). Beyond the Columbia Hills, no further features have been identified that resemble “Home Plate” or other candidate vent structures. While we have found a diverse mineralogy indicating hydrothermal deposits within the Inner Basin of the Columbia Hills, we have not found evidence from orbital mapping that there was widespread hydrothermal activity within Gusev crater.