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Paul Douglas Archer Jr., Heather B. Franz, Brad Sutter, Ricardo D. Arevalo Jr., Patrice Coll, Jennifer L. Eigenbrode, Daniel P. Glavin, John J. Jones, Laurie A. Leshin, Paul R. Mahaffy, Amy C. McAdam, Christopher P. McKay, Douglas W. Ming, Richard V. Morris, Rafael Navarro-González, Paul B. Niles, Alex Pavlov, Steven W. Squyres, Jennifer C. Stern, Andrew Steele and James J. Wray Abundances and implications of volatile-bearing species from evolved gas analysis of the Rocknest aeolian deposit, Gale Crater, Mars Journal of Geophysical Research: Planets 119

Version of Record online: 29 JAN 2014 | DOI: 10.1002/2013JE004493

Key Points

  • Major volatiles detected by SAM were H2O, SO2, CO2, and O2
  • Minor volatiles include HCl, H2S, NH3, NO, and HCN
  • Calculating abundances from counts per second is explained

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