Photochemical and climate consequences of sulfur outgassing on early Mars

Feng Tian, Mark W. Claire, Jacob D. Haqq-Misra, Megan Smith, David C. Crisp, David Catling, Kevin Zahnle, James F. Kasting

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Abstract

Ancient Mars might have been warm and wet compared to today, but climate models have trouble reproducing this warmth, partly because of the faintness of the young Sun and partly because of inherent limitations to CO2-H2O greenhouse warming. In particular, Rayleigh scattering of incoming sunlight by a dense, CO2-rich atmosphere leads to a high planetary albedo, thereby reducing the amount of sunlight absorbed by the planet. It has been recently suggested that the presence of 1-100ppmv SO2 in Mars' early atmosphere might have provided enough additional greenhouse warming to maintain a warm, wet early Mars. We show, however, that this warming should have been more than offset by cooling from sulfate and sulfur aerosols in early martian atmosphere. Hence, the paradox of Mars' early climate remains unresolved.

Original languageEnglish (US)
Pages (from-to)412-418
Number of pages7
JournalEarth and Planetary Science Letters
Volume295
Issue number3-4
DOIs
StatePublished - Jul 1 2010

All Science Journal Classification (ASJC) codes

  • Geophysics
  • Geochemistry and Petrology
  • Earth and Planetary Sciences (miscellaneous)
  • Space and Planetary Science

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    Tian, F., Claire, M. W., Haqq-Misra, J. D., Smith, M., Crisp, D. C., Catling, D., Zahnle, K., & Kasting, J. F. (2010). Photochemical and climate consequences of sulfur outgassing on early Mars. Earth and Planetary Science Letters, 295(3-4), 412-418. https://doi.org/10.1016/j.epsl.2010.04.016