Mechanisms leading to a warmer climate on high obliquity planets

Abstract

A consistent finding of high obliquity simulations is that they are warmer than their low obliquity counterparts when the climate is cold. Ice-albedo feedback has been suggested as a possible mechanism. In this study, we find that warmer climate under high obliquity holds with varying insolations, including almost ice-free conditions. We try to understand the mechanisms through a series of feedback suppression experiments. Turning off the ice-albedo feedback, the temperature contrast between high and low obliquity remains significant, but it vanishes when the cloud radiation effects or the seasonal variation is turned off. This suggests the warmer climate on high obliquity planets does not rely completely on the existence of ice, and therefore holds at high insolation. In that regime, the surface temperature, and hence the cloud formation, lags behind the substellar point, leading to inefficient sunlight reflection and warmer climate.

References in corpus (2)

• Effects of Extreme Obliquity Variations on the Habitability of Exoplanets
• Obliquity-Driven Sculpting of Exoplanetary Systems

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• Moderately High Obliquity Promotes Biospheric Oxygenation
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