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Abstract

Previously unrecognized insolation variations on Mars are a consequence of periodic variations in eccentricity, first established by the theory of Brouwer and Van Woerkom (1950). Such annual insolation variations, characterized by both 95,000-year and 2,000,000-year periodicities, may actually be recorded in newly discovered layered deposits in the polar regions of Mars. An additional north-south variation in seasonal insolation, but not average annual insolation, exists with 51,000-year and 2,000,000-year periodicities.

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Published In

Science
Volume 180 | Issue 4086
11 May 1973

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Published in print: 11 May 1973

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Bruce C. Murray
Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena 91109
William R. Ward
Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena 91109
Sze C. Yeung
Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena 91109

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