Obliquity Evolution of Earth-Like Exoplanets in Systems with Large Inclinations

Abstract : In order to properly assess the potential for habitability and prioritize target selection for the characterization of exoplanets, we need to understand the limits of orbital and rotational dynamics. Large satellites may be rare and very difficult to detect. Consequently, it is necessary to quantify the likelihood of a planet's having extreme obliquity cycles in the absence of a moon and to model the potential impact on the planet's climate. We explore the obliquity evolution of (1) known exoplanet systems that could contain Earth-like planets in the habitable zone and (2) hypothetical planets in mutually inclined, chaotic resonant configurations that experience some of the most extreme orbital evolution possible. We use a secular obliquity model coupled to either an N-body models or a 4th order secular orbital model.We find that in some known systems, planets' obliquity variations are small and unlikely to have a major effect on climate, unless undetected planets are present. Systems with three or more planets are significantly more dynamically rich, with planets that undergo obliquity changes of ~10° over 50,000 years and >30° over a few million years. In resonant configurations, Earth-like exoplanets can undergo dramatic and chaotic evolution in eccentricity and inclination while remaining stable for over 10 Gyr. In configurations in which eccentricities and inclinations stay below ~0.1 and ~10°, respectively, obliquities oscillate quasi-periodically with amplitudes similar to the non-resonant, three-planet configurations. In more dynamically active configurations, in which eccentricities and inclinations evolve to e > 0.3 and i > 15°, obliquities can extend from ~0° to well past 90°. In extreme cases eccentricities can reach >0.9999 and inclinations >179.9 degrees, driving precession rates in excess of degrees per year. However, these planets can graze or impact the stellar surface and are probably not habitable.
Type de document :
Communication dans un congrès
American Astronomical Society, DDA meeting #46, #100.03 - 46th Meeting of the AAS Division for Planetary Sciences held in Tucson-AZ 9-14 november 2014, Nov 2014, Tucson, United States. 46, pp.100.03, 2015
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https://hal.archives-ouvertes.fr/hal-01149645
Contributeur : Marie-Paule Pomies <>
Soumis le : jeudi 7 mai 2015 - 14:11:07
Dernière modification le : lundi 15 juin 2015 - 15:08:35

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Russell, Deitrick, Rory, Barnes, Richard, Greenberg, Thomas R., Quinn, Sean N. Raymond. Obliquity Evolution of Earth-Like Exoplanets in Systems with Large Inclinations. American Astronomical Society, DDA meeting #46, #100.03 - 46th Meeting of the AAS Division for Planetary Sciences held in Tucson-AZ 9-14 november 2014, Nov 2014, Tucson, United States. 46, pp.100.03, 2015. <hal-01149645>

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