Figure 10 from Exo-Milankovitch Cycles. I. Orbits and Rotation States

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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 10.

Same as Figure 5 but using mass set ﹩{ \mathcal B }﹩. The left panel has ﹩{(\psi +{\rm{\Omega }})}_{0}=0^\circ ﹩, the right ﹩{(\psi +{\rm{\Omega }})}_{0}=180^\circ ﹩. The secular resonances (and Cassini states) are shifted to longer rotation periods.

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