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• W3100148376 abstract "Previous studies have demonstrated that continental carbon-silicate weathering is important to the continued habitability of a terrestrial planet. Despite this, few studies have considered the influence of land on the climate of a tidally-locked planet. In this work we use the Met Office Unified Model, coupled to a land surface model, to investigate the climate effects of a continent located at the sub-stellar point. We choose to use the orbital and planetary parameters of Proxima Centauri B as a template, to allow comparison with the work of others. A region of the surface where $T_{text{s}} > 273.15,text{K}$ is always retained, and previous conclusions on the habitability of Proxima Centauri B remain intact. We find that sub-stellar land causes global cooling, and increases day-night temperature contrasts by limiting heat redistribution. Furthermore, we find that sub-stellar land is able to introduce a regime change in the atmospheric circulation. Specifically, when a continent offset to the east of the sub-stellar point is introduced, we observe the formation of two mid-latitude counterrotating jets, and a substantially weakened equatorial superrotating jet." @default.
• W3100148376 created "2020-11-23" @default.
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• W3100148376 date "2018-02-26" @default.
• W3100148376 modified "2023-10-13" @default.
• W3100148376 title "The Influence of a Substellar Continent on the Climate of a Tidally Locked Exoplanet" @default.
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• W3100148376 doi "https://doi.org/10.3847/1538-4357/aaad0a" @default.
• W3100148376 hasPublicationYear "2018" @default.
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