The effects of orbital and climatic variations on Martian surface heat flow

Details The effects of orbital and climatic variations on Martian surface heat flow The effects of orbital and climatic variations on Martian surface heat flow

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992georl..19.2393m&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 19, no. 24, p. 2393-2396.

Mathematics

Logic

4

Climate Change, Equatorial Regions, Heat Transmission, Mars Surface, Orbital Resonances (Celestial Mechanics), Polar Regions, Carbon Dioxide, Perihelions, Regolith, Surface Temperature

Scientific paper

We have examined the effects of climate changes, induced by orbital oscillations, on Martian surface heat flow. It was found that the climatological component of the surface heat flow can be larger than the expected internal geothermal heat flow. We suggest that measurements of surface heat flow be targeted for equatorial and south polar regions to avoid climatic effects and that care be taken in interpreting measurements in mid-latitude and north polar regions.

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