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Our results show that eeta79001 shock veins and melt pockets represent local mineral melts formed by shock impedance contrasts, which can account for the observed compositional anomalies compared to the whole rock sample. Petrologic investigation of the shergottites has been hampered by the fact that most of these meteorites are partial cumulates. We examined two samples of eet 79001 that include shock melt pockets and basaltic wallrock (lith a)
We find that either a regolith or an excess sulfide component, along with excess plagioclase and residual olivine, can explain most of the major element and s abundances in the shock melt. Lithology a as an impact melt From these measurements, becker and coworkers concluded that the pahs in both alh 84001 and eet 79001 were contaminants, though they could not determine if the contamination occurred on mars or in antarctica.
A synthetic martian basaltic magma with the composition of the groundmass of eet 79001 lithology a has been used in a number of experiments to constrain martian parental magmas and to investigate the nature of martian basaltic magmatism (longhi and pan, 1989
As this study develops we aim to extract details of a potenal soil composion and to examine maran surface processes using elemental raos and correlaons. Isotopic evidence for a terrestrial source of organic compounds found in martian meteorites allan hills 84001 and elephant moraine 79001. A groundmass composition for eet 79001a using a novel microprobe technique for estimating bulk compositions
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