Indigenous Organic Matter Associated with Unusual Low Temperature Aqueous Secondary Phases in the Mars Meteorite Nakhla
The Martian meteorite Nakhla provides demonstrates evidence of mineral-water interactions that occurred in the Martian regolith within the last 1 Ga, as well as the presence of trace indigenous organic matter. The aim of our research is threefold: [1] provide a context in which to interpret alteration features; [2] determine the physical and chemical environment during alteration; and, [3] investigate the hypothesis that the formation of alteration phases was intimately involved in the accumulation and/or preservation of organic matter. In freshly fractured chips of the Mars meteorite Nakhla, we found carbonaceous matter intimately associated with secondary aqueous alteration phases interpreted to have formed through the low-temperature, mineral-water dissolution of the host Martian basalt. We have characterized the nature of carbonaceous matter and spatially associated secondary phases within Nakhla using a multidisciplinary suite of analytical instrumentation. The aim of our research is to provide a context to interpret the formation of secondary alteration assemblages within the Mars meteorite Nakhla and determine whether, and if so the extent to which, these phases participated in the accumulation and preservation of Martian organic matter.