Martian and terrestrial paleoclimatology - Relevance of solar variability

Details Martian and terrestrial paleoclimatology - Relevance of solar variability Martian and terrestrial paleoclimatology - Relevance of solar variability

Jul 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974icar...22..301h&link_type=abstract

Icarus, vol. 22, July 1974, p. 301-311. Research supported by the Science Applications, Inc.

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4

Climatology, Earth Atmosphere, Mars Atmosphere, Paleoclimatology, Secular Variations, Solar Activity Effects, Climate Change, Craters, Geomorphology, Luminous Intensity, Mars Surface, Neutrinos, Spaceborne Photography

Scientific paper

Certain assertions related to the interpretation of arroyo-like features observed on Mars are considered, giving attention to the deficiency in solar neutrinos which would indirectly imply that the sun was more luminous in the past than now. A review is given of the terrestrial geological evidence for climatic changes driven by solar changes. A working hypothesis of solar variation is developed by adopting terrestrial and Martian observations. The possibility is considered that solar variations on a time-scale of some 100 m.y. might be responsible for the transformation of Mars from a state in which liquid volatiles are presented to arid and/or frozen conditions.

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