Stability analysis of the martian obliqu
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Ramon Brasser; Kevin J. Walsh
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Article
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2011
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Elsevier Science
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English
⚖ 505 KB
We performed numerical simulations of the obliquity evolution of Mars during the Noachian era, at which time the giant planets were on drastically different orbits than today. For the preferred primordial configuration of the planets we find that there are two large zones where the martian obliquity