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Science 17 December 1976:
Vol. 194. no. 4271, pp. 1339 - 1341
DOI: 10.1126/science.194.4271.1339
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Articles

Mars: Northern Summer Ice Cap—Water Vapor Observations from Viking 2

CROFTON B. FARMER 1, DONALD W. DAVIES 1, and DANIEL D. LAPORTE 2

1 Jet Propulsion Laboratory, California Institute of Technology, Pasadena 91103
2 Santa Barbara Research Center Goleta, California 93017

Observations of the latitude dependence of water vapor made from the Viking 2 orbiter show peak abundances in the latitude band 70° to 80° north in the northern midsummer season (planetocentric longitude sim 108°). Total column abundances in the polar regions require near-surface atmospheric temperatures in excess of 200°K, and are incompatible with the survival of a frozen carbon dioxide cap at martian pressures. The remnant (or residual) north polar cap, and the outlying patches of ice at lower latitudes, are thus predominantly water ice, whose thickness can be estimated to be between 1 meter and 1 kilometer.

Submitted on October 18, 1976


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