Mars: Influence of Topography on Formation of Temporary Bright Patches

Details Mars: Influence of Topography on Formation of Temporary Bright Patches Mars: Influence of Topography on Formation of Temporary Bright Patches

Jan 1967

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1967sci...155..317o&link_type=abstract

Science, Volume 155, Issue 3760, pp. 317-319

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6

Scientific paper

The mountains of Mitchel and other temporary bright patches observed on
the Martian disk may be carbon-dioxide condensations in depressions
rather than a water-ice mixture on mountains as previously thought. This
interpretation supports the hypothesis that the Martian deserts, that
is, the light areas, are lower than their surroundings.

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