Non-Chaotic Obliquity Variations of Mars

Details Non-Chaotic Obliquity Variations of Mars Non-Chaotic Obliquity Variations of Mars

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.2093b&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.2093

Physics

Scientific paper

In the absence of energy dissipation, obliquity variations of Mars would
likely be chaotic. However, relatively small amounts of dissipation
suffice to suppress chaotic variations. Spin pole estimates from a fully
damped model agree well with observation.

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