The Astronomical Theory of Climatic Change on Mars

@inproceedings{2002TheAT,
  title={The Astronomical Theory of Climatic Change on Mars},
  author={},
  year={2002}
}
  • Published 2002
We examine the response of Martian climate to changes in solar energy deposition caused by variations of the Martian orbit and obliquity. We systematically investigate the seasonal cycles of carbon dioxide, water, and dust to provide a complete picture of the climate for various orbital configurations. We find that at low obliquity (15 °) the atmospheric pressure will fall below 1 mbar; dust storms will cease; thick permanent CO2 caps will form; the regolith will release CO2; and H20 polar ice… CONTINUE READING