title: Detection of atomic deuterium in the upper atmosphere of Mars.
abstract: High-resolution spectroscopy of Mars' atmosphere with the Hubble Space Telescope revealed the deuterium Lyman alpha line at an intensity of 23 +/- 6 rayleighs. This measured intensity corresponds to HD/H2 = 1.5 +/- 0.6 x 10(-4), which is smaller by a factor of 11 than HDO/H2O. This indicates that fractionation of HD/H2 relative to that of HDO/H2O is not kinetically controlled by the rates of formation and destruction of H2 and HD but is thermodynamically controlled by the isotope exchange HD + H2O left and right arrow HDO + H2. Molecular hydrogen is strongly depleted in deuterium relative to water on Mars because of the very long lifetime of H2 (1200 years). The derived isotope fractionation corresponds to an estimate of a planetwide reservoir of water ice about 5 meters thick that is exchangeable with the atmosphere.
authors.affiliation: Department of Physics, Catholic University of America, Washington, DC 20064, USA. VKras@lepvx3.gsfc.nasa.gov
authors.forename: V A
authors.initials: VA
authors.lastname: Krasnopolsky
authors.forename: M J
authors.initials: MJ
authors.lastname: Mumma
authors.forename: G R
authors.initials: GR
authors.lastname: Gladstone
mesh_terms: D001272:Atmosphere; D003903:Deuterium / Q000032:analysis*; D005118:Extraterrestrial Environment; D006859:Hydrogen / Q000032:analysis*; D007053:Ice; D018535:Mars; D013696:Temperature; D014867:Water
chemical_list: D007053:Ice; D014867:Water; D006859:Hydrogen; D003903:Deuterium