Constraining the magnitude of climate extremes from time-varying instellation on a circumbinary terrestrial planet

Abstract

Planets that revolve around a binary pair of stars are known as circumbinary planets. The orbital motion of the stars around their center of mass causes a periodic variation in the total instellation incident upon a circumbinary planet. This study uses both an analytic and numerical energy balance model to calculate the extent to which this effect can drive changes in surface temperature on circumbinary terrestrial planets. We show that the amplitude of the temperature variation is largely constrained by the effective heat capacity, which corresponds to the ocean-to-land ratio on the planet. Planets with large ocean fractions should experience only modest warming and cooling of only a few degrees, which suggests that habitability cannot be precluded for such circumbinary planets. Planets with large land fractions that experience extreme periodic forcing could be prone to changes in temperature of tens of degrees or more, which could drive more extreme climate changes that inhibit continuously habitable conditions.

arXiv commentAccepted for publication in JGR-Planets

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Cited by in corpus (8)

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• Greater climate sensitivity and variability on TRAPPIST-1e than Earth
• An Energy Balance Model for Rapidly and Synchronously Rotating Terrestrial Planets
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• Planetary Rhythms: Synchronous Circulation on Variably Irradiated Asynchronous Planets