Other
Scientific paper
Dec 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufm.p13a1264e&link_type=abstract
American Geophysical Union, Fall Meeting 2009, abstract #P13A-1264
Other
[1034] Geochemistry / Hydrothermal Systems, [1039] Geochemistry / Alteration And Weathering Processes, [5415] Planetary Sciences: Solid Surface Planets / Erosion And Weathering, [5464] Planetary Sciences: Solid Surface Planets / Remote Sensing
Scientific paper
Recent orbital investigations have revealed that aqueous alteration on early Mars took place in diverse alteration environments indicated by distinctive assemblages of minerals (Murchie et al., 2009, JGR). There is growing evidence for past diagenetic or low-temperature/pressure hydrothermal activity on Mars at neutral to alkaline pH, indicated by the presence of Fe/Mg smectites, chlorite, prehnite, serpentine, opaline silica, and zeolites such as analcime in Noachian terrains (Ehlmann et al., 2009, JGR). In recent investigations of terrestrial Mars analog sites, neutral to alkaline pH alteration of basalt, both pedogenic and hydrothermal, has been understudied in favor of sulfur-rich, acidic systems including those at the Hawaiian volcanoes and Rio Tinto, Spain. We began study of the alteration of basalt lava flows in Iceland as a geochemical analog for Noachian Mars. Because the basaltic bedrock is recently formed (<16Ma) with few localities of more highly evolved composition and has poorly formed soils and spare vegetation, the ground and surface waters are broadly similar to those which might have existed on Noachian Mars. Iceland has a variety of geothermal spring systems--low T, low S; low T, high S; and high T, high S--each of which creates distinctive mineralogic assemblages. Here we examine rocks of the Hvalfjordur peninsula, collected from basalt flows that were in some places altered at the surface by pedogenesis and in other locations were hydrothermally altered by non-sulfurous groundwater circulation (low T, low S) following the emplacement of a later hot basalt flow. Rock samples were surveyed in the field using a portable VNIR spectrometer. Altered and unaltered rocks that were typical for the locality were collected as were altered rocks whose spectra were most similar to those measured by CRISM from Mars orbit. Ten rocks were ultimately selected for detailed laboratory analyses: zeolitized basaltic rocks bearing minerals including analcime and thomsonite, basalts with silica/quartz-bearing veins, basalts bearing celadonite, and basalts partially altered to montmorillonite, Fe/Mg smectite, or mixed smectite-chlorite. Analyses included: (1) measurement of reflectance spectra of the whole rock by the ASD; (2) measurement of VNIR and TIR spectra in RELAB of particle-size separates (<25um and <125um) derived from the bulk rock and from precipitated minerals extracted from the vesicles; (3) measurement of X-ray diffraction (XRD) patterns, including quantitative XRD; and (4) electron microprobe chemical analyses. These data emulate orbital data from CRISM, OMEGA, and TES, which detect the infrared active components, linked to in-situ data on whole rock modal mineralogy such as will be measured by the ChemMin instrument on the MSL rover.
Bish David L.
Ehlmann Bethany L.
Mustard John F.
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