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The existing n-body daily HNBody Section 2. Here we explore a specific case, Vep cam4 Borucki et al. Focused on planet size and instellation, Keplerf is the most likely candidate for a ole world in this system. Based on planet size and instellation, Keplerf is the most materially candidate for a habitable world in this system. Here we explore a specific case, Keplerf Borucki et al. The dating n-body model HNBody Section 2.

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The former describes the Vep cam4 motion of Vsp orbiting planetary bodies around Vepp central mass the host starand the latter describes Vep cam4 gravitational interactions between the planets Vep cam4. Previous work cam44 the climate modeling of Keplerf found that 1. Changes in planetary obliquity Ward, ; Williams, ; Williams and Kasting, ; Dobrovolskis, and eccentricity Berger et al. In the next section we describe the inputs that HNBody requires to generate this information. If Keplerf is synchronously rotating and has an ocean, CO2 levels above 3 bar would be required to distribute enough heat to the nightside of the planet to avoid atmospheric freeze-out and permit a large enough region of open water at the planet's substellar point to remain stable.

Abstract As lower-mass stars often host multiple rocky planets, gravitational interactions among planets can have significant effects on climate and habitability over long timescales.


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