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Exo-Milankovitch Cycles. I. Orbits and Rotation States

  • Authors: Russell Deitrick, Rory Barnes, Thomas R. Quinn, John Armstrong, Benjamin Charnay, and Caitlyn Wilhelm

2018 The Astronomical Journal 155 60.

  • Provider: AAS Journals

Caption: Figure 12.

Evolution of the obliquity and the angle ﹩\psi +{\rm{\Omega }}﹩ for points a (left), b (middle), and c (right) from Figure 11. Point a approaches Cassini state 2 wherein the obliquity oscillation is smaller than the surrounding regions. Point b is librating about Cassini state 2 with a large amplitude, and its obliquity oscillation is large. Point c is near Cassini state 4.

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