Tidal evolution of habitable planets

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Tidal evolution of habitable planets

Post by Lazarus on 12th January 2011, 4:37 pm

Tidal obliquity evolution of potentially habitable planets

Planets in the insolation habitable zone of stars with <0.25 solar masses are likely to be volcanic, and the potentially-habitable planets at Gliese 581 (d and g) are likely to have lost any axial tilt very early on.
dF star
dF star

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