Periodic Insolation Variations on Mars
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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Science
Volume 180 | Issue 4086
11 May 1973
11 May 1973
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The American Association for the Advancement of Science.
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Published in print: 11 May 1973
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- Solar Neutrinos and Variations in the Solar Luminosity, Science, 190, 4215, (619-624), (1975)./doi/10.1126/science.190.4215.619
- Polar Wandering on Mars?, Science, 179, 4077, (997-1000), (1973)./doi/10.1126/science.179.4077.997
- Large-Scale Variations in the Obliquity of Mars, Science, 181, 4096, (260-262), (1973)./doi/10.1126/science.181.4096.260
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