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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 1.

Geometry used in the obliquity model DISTROT. The light gray represents the planet’s orbital plane, while the darker gray represents a plane of reference. The important orbital angles are the inclination, i, the longitude of ascending node, Ω, and the argument of pericenter, ω. The longitude of pericenter is a “dog-leg” angle, ﹩\varpi ={\rm{\Omega }}+\omega ﹩. The angle Λ is measured from the vernal point ϒ at time t to the ascending node, Ω. The precession angle is defined as ﹩\psi ={\rm{\Lambda }}-{\rm{\Omega }}﹩ (also a dog-leg angle). The reference point for Ω is usually chosen as the vernal point at some known date for the solar system, but there is probably a more sensible choice for exoplanetary systems.

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