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Pyrolysis of Oxalate, Acetate, and Perchlorate Mixtures and the Implications for Organic Salts on Mars
Author(s) -
Lewis J. M. T.,
Eigenbrode J. L.,
Wong G. M.,
McAdam A. C.,
Archer P. D.,
Sutter B.,
Millan M.,
Williams R. H.,
Guzman M.,
Das A.,
Rampe E. B.,
Achilles C. N.,
Franz H. B.,
Andrejkovičová S.,
Knudson C. A.,
Mahaffy P. R.
Publication year - 2021
Publication title -
journal of geophysical research: planets
Language(s) - English
Resource type - Journals
eISSN - 2169-9100
pISSN - 2169-9097
DOI - 10.1029/2020je006803
Subject(s) - chemistry , perchlorate , oxalate , inorganic chemistry , pyrolysis , organic matter , acetic acid , acetone , ammonium oxalate , environmental chemistry , organic chemistry , ion
Organic salts, such as Fe, Ca, and Mg oxalates and acetates, may be widespread radiolysis and oxidation products of organic matter in Martian surface sediments. Such organic salts are challenging to identify by evolved gas analysis but the ubiquitous CO 2 and CO in pyrolysis data from the Sample Analysis at Mars (SAM) instrument suite on the Curiosity rover indirectly points to their presence. Here, we examined laboratory results from SAM‐like analyses of organic salts as pure phases, as trace phases mixed with silica, and in mixtures with Ca and Mg perchlorates. Pure oxalates evolved CO 2 and CO, while pure acetates evolved CO 2 and a diverse range of organic products dominated by acetone and acetic acid. Dispersal within silica caused minor peak shifting, decreased the amounts of CO 2 evolved by the acetate standards, and altered the relative abundances of the organic products of acetate pyrolysis. The perchlorate salts scrubbed Fe oxalate CO releases and shifted the CO 2 peaks to lower temperatures, whereas with Ca and Mg oxalate, a weaker CO release was observed but the initial CO 2 evolutions were largely unchanged. The perchlorates induced a stronger CO 2 release from acetates at the expense of other products. Oxalates evolved ∼47% more CO 2 and acetates yielded ∼69% more CO 2 when the perchlorates were abundant. The most compelling fits between our organic salt data and SAM CO 2 and CO data included Martian samples acquired from modern eolian deposits and sedimentary rocks with evidence for low‐temperature alteration.