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Oxidant enhancement in martian dust devils and storms: implications for life and habitability.

Publication ,  Journal Article
Atreya, SK; Wong, A-S; Renno, NO; Farrell, WM; Delory, GT; Sentman, DD; Cummer, SA; Marshall, JR; Rafkin, SCR; Catling, DC
Published in: Astrobiology
June 2006

We investigate a new mechanism for producing oxidants, especially hydrogen peroxide (H2O2), on Mars. Large-scale electrostatic fields generated by charged sand and dust in the martian dust devils and storms, as well as during normal saltation, can induce chemical changes near and above the surface of Mars. The most dramatic effect is found in the production of H2O2 whose atmospheric abundance in the "vapor" phase can exceed 200 times that produced by photochemistry alone. With large electric fields, H2O2 abundance gets large enough for condensation to occur, followed by precipitation out of the atmosphere. Large quantities of H2O2 would then be adsorbed into the regolith, either as solid H2O2 "dust" or as re-evaporated vapor if the solid does not survive as it diffuses from its production region close to the surface. We suggest that this H2O2, or another superoxide processed from it in the surface, may be responsible for scavenging organic material from Mars. The presence of H2O2 in the surface could also accelerate the loss of methane from the atmosphere, thus requiring a larger source for maintaining a steady-state abundance of methane on Mars. The surface oxidants, together with storm electric fields and the harmful ultraviolet radiation that readily passes through the thin martian atmosphere, are likely to render the surface of Mars inhospitable to life as we know it.

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Published In

Astrobiology

DOI

EISSN

1557-8070

ISSN

1531-1074

Publication Date

June 2006

Volume

6

Issue

3

Start / End Page

439 / 450

Related Subject Headings

  • Wind
  • Mars
  • Hydrogen Peroxide
  • Exobiology
  • Astronomy & Astrophysics
  • 5101 Astronomical sciences
  • 0403 Geology
  • 0402 Geochemistry
  • 0201 Astronomical and Space Sciences
 

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Atreya, S. K., Wong, A.-S., Renno, N. O., Farrell, W. M., Delory, G. T., Sentman, D. D., … Catling, D. C. (2006). Oxidant enhancement in martian dust devils and storms: implications for life and habitability. Astrobiology, 6(3), 439–450. https://doi.org/10.1089/ast.2006.6.439
Atreya, Sushil K., Ah-San Wong, Nilton O. Renno, William M. Farrell, Gregory T. Delory, Davis D. Sentman, Steven A. Cummer, John R. Marshall, Scot C. R. Rafkin, and David C. Catling. “Oxidant enhancement in martian dust devils and storms: implications for life and habitability.Astrobiology 6, no. 3 (June 2006): 439–50. https://doi.org/10.1089/ast.2006.6.439.
Atreya SK, Wong A-S, Renno NO, Farrell WM, Delory GT, Sentman DD, et al. Oxidant enhancement in martian dust devils and storms: implications for life and habitability. Astrobiology. 2006 Jun;6(3):439–50.
Atreya, Sushil K., et al. “Oxidant enhancement in martian dust devils and storms: implications for life and habitability.Astrobiology, vol. 6, no. 3, June 2006, pp. 439–50. Epmc, doi:10.1089/ast.2006.6.439.
Atreya SK, Wong A-S, Renno NO, Farrell WM, Delory GT, Sentman DD, Cummer SA, Marshall JR, Rafkin SCR, Catling DC. Oxidant enhancement in martian dust devils and storms: implications for life and habitability. Astrobiology. 2006 Jun;6(3):439–450.
Journal cover image

Published In

Astrobiology

DOI

EISSN

1557-8070

ISSN

1531-1074

Publication Date

June 2006

Volume

6

Issue

3

Start / End Page

439 / 450

Related Subject Headings

  • Wind
  • Mars
  • Hydrogen Peroxide
  • Exobiology
  • Astronomy & Astrophysics
  • 5101 Astronomical sciences
  • 0403 Geology
  • 0402 Geochemistry
  • 0201 Astronomical and Space Sciences