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Perchlorate on Mars - Overview and Implications

Authors :
Archer, P. D
Ming, D. W
Sutter, B
Hogancamp, J. V
Morris, R. V
Clark, B.C
Mahaffy, P.H
Navarro-González, R
McKay, C.P
Gough, R.V
Fairen, A.G
Publication Year :
2019
Publisher :
United States: NASA Center for Aerospace Information (CASI), 2019.

Abstract

Perchlorate was first detected on Mars by the Wet Chemistry Laboratory (WCL) instrument on the Phoenix lander at a concentration of ~0.5 wt% in northern plains soils. Since that initial detection, perchlorate (and likely chlorate) have been detected on Mars by both surface and orbital instruments. Perchlorate (ClO4-) is an oxidized chlorine compound and salts of perchlorate are kinetically stable (though very reactive at high temperature), very soluble, deliquescent, and have low eutectic temperature (which decreases the temperature for stable liquids on Mars). Chlorate (ClO3-) salts are similar, though they are less kinetically stable than perchlorates. Because many of the analytical signatures of perchlorate and chlorate are similar to the instruments we have used on Mars, we cannot always determine which species is present, so we will use the more generic term “oxychlorine” when referring to perchlorate and/or chlorate.

Details

Language :
English
Database :
NASA Technical Reports
Notes :
NNJ13HA01C
Publication Type :
Report
Accession number :
edsnas.20190028297
Document Type :
Report