Bulk and stable isotopic compositions of carbonate minerals in Martian meteorite Allan Hills 84001: no proof of high formation temperature.
Understanding the origin of carbonate minerals in the Martian meteorite Allan Hills (ALH) 84001 is crucial to evaluating the hypothesis that they contain traces of ancient Martian life. Using arguments based on chemical equilibria among carbonates and fluids, an origin at >650 degrees C (inimical to life) has been proposed. However, the bulk and stable isotopic compositions of the carbonate minerals are open to multiple interpretations and so lend no particular support to a high-temperature origin. Other methods (possibly less direct) will have to be used to determine the formation temperature of the carbonates in ALH84001.
Treiman
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AH
Lunar and Planetary Institute, Houston, Texas 77058, USA. treiman@lpi.jsc.nasa.gov
Romanek
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CS
D002119:Calcium Carbonate / Q000032:analysis* / Q000737:chemistry; D002247:Carbon Isotopes; D002254:Carbonates / Q000032:analysis / Q000737:chemistry; D007501:Iron; D007554:Isotopes; D008274:Magnesium / Q000032:analysis* / Q000737:chemistry; D019110:Meteoroids; D008903:Minerals / Q000032:analysis* / Q000737:chemistry; D010103:Oxygen Isotopes; D013696:Temperature
D002247:Carbon Isotopes; D002254:Carbonates; D007554:Isotopes; D008903:Minerals; D010103:Oxygen Isotopes; C005479:magnesium carbonate; D007501:Iron; D002119:Calcium Carbonate; D008274:Magnesium; C028042:calcium magnesium carbonate