Carbonates in fractures of martian meteorite ALH84001: Petrologic evidence for impact origin

Details Carbonates in fractures of martian meteorite ALH84001: Petrologic evidence for impact origin Carbonates in fractures of martian meteorite ALH84001: Petrologic evidence for impact origin

Jul 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998m%26ps...33..709s&link_type=abstract

Meteoritics & Planetary Science, vol. 33, no. 4, pp. 709-719.

Mathematics

Logic

29

Scientific paper

Carbonates in martian meteorite ALH84001 occur as grains on pyroxene grain boundaries, in crushed zones, and as disks, veins, and irregularly shaped grains in healed pyroxene fractures. Some carbonate disks have tapered Mg-rich edges and are accompanied by smaller, thinner and relatively homogeneous, magnesite microdisks. Except for the microdisks, all types of carbonate grains show the same unique chemical zoning pattern on MgCO3-FeCO3-CaCO3 plots. This chemical characteristic and the close spatial association of diverse carbonate types show that all carbonates formed by a similar process. The heterogeneous distribution of carbonates in fractures, tapered shapes of some disks, and the localized occurrence of Mg-rich microdisks appear to be incompatible with growth from an externally derived CO2-rich fluid that changed in composition over time. These features suggest instead that the fractures were closed as carbonates grew from an internally derived fluid and that the microdisks formed from a residual Mg-rich fluid that was squeezed along fractures. Carbonate in pyroxene fractures is most abundant near grains of plagioclase glass that are located on pyroxene grain boundaries and commonly contain major or minor amounts of carbonate. We infer that carbonates in fractures formed from grain boundary carbonates associated with plagioclase that were melted by impact and dispersed into the surrounding fractured pyroxene. Carbonates in fractures, including those studied by McKay et al. (1996), could not have formed at low temperatures and preserved mineralogical evidence for martian organisms.

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