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20092026
most citedStabilizing Cloud Feedback Dramatically Expands the Habitable Zone of Tidally Locked Planets

399 citations · 2.6k across the 69 of their papers we have counts for

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Showing 2014 · astro-ph.EPShow all

5 papers · 2 filters

astro-ph.EP2014★ 87 cited

Deciphering thermal phase curves of dry, tidally locked terrestrial planets

Daniel D. B. Koll, Dorian S. Abbot

Next-generation space telescopes will allow us to characterize terrestrial exoplanets. To do so effectively it will be crucial to make use of all available data. We investigate whi…

astro-ph.EP2014★ 84 cited

Water Trapping on Tidally Locked Terrestrial Planets Requires Special Conditions

Jun Yang, Yonggang Liu, Yongyun Hu +1

Surface liquid water is essential for standard planetary habitability. Calculations of atmospheric circulation on tidally locked planets around M stars suggest that this peculiar o…

astro-ph.EP2014★ 256 cited

Strong Dependence of the Inner Edge of the Habitable Zone on Planetary Rotation Rate

Jun Yang, Gwenael Boue, Daniel C. Fabrycky +1

Planetary rotation rate is a key parameter in determining atmospheric circulation and hence the spatial pattern of clouds. Since clouds can exert a dominant control on planetary ra…

astro-ph.EP2014★ 50 cited

A Low-order Model of Water Vapor, Clouds, and Thermal Emission for Tidally Locked Terrestrial Planets

Jun Yang, Dorian S. Abbot

In the spirit of minimal modeling of complex systems, we develop an idealized two-column model to investigate the climate of tidally locked terrestrial planets with Earth-like atmo…

astro-ph.EP2014★ 78 cited

Water Cycling Between Ocean and Mantle: Super-Earths Need Not be Waterworlds

Nicolas B. Cowan, Dorian S. Abbot

Large terrestrial planets are expected to have muted topography and deep oceans, implying that most super-Earths should be entirely covered in water, so-called waterworlds. This is…