Saturday, 11 June 2011

What is the cause of the variation from high and low mean obliquity periods of Mars?

It is reasonably well known that Mars has a greater obliquity range than Earth, due to Mars lacking a stabilising influence of a large moon. However, the Martian obliquity seems to have gone through periods of high and low mean obliquity, as shown in the top chart below:



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Image source: Mars Climate Modeling Group



What is the current accepted theory as to why there are periodic high and low mean obliquities on Mars?



(Please note, I am not asking about orbital eccentricity)

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