Periodic Insolation Variations on Mars

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 re...

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Veröffentlicht in:Science (American Association for the Advancement of Science) 1973-05, Vol.180 (4086), p.638-640
Hauptverfasser: Murray, Bruce C., Ward, William R., Yeung, Sze C.
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creator Murray, Bruce C.
Ward, William R.
Yeung, Sze C.
description 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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source JSTOR Archive Collection A-Z Listing; American Association for the Advancement of Science
subjects Axial tilt
Insolation
Mars
Murine leukemia virus
Numerical eccentricity
Perihelions
Planetary meteorology
Planetary orbits
Planets
Viruses
title Periodic Insolation Variations on Mars
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