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20112026
most citedThe inner edge of the habitable zone for synchronously rotating planets around low-mass stars using general circulation models

236 citations · 1.6k across the 60 of their papers we have counts for

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Showing 2017Show all

5 papers · 1 filter

astro-ph.EP2017★ 125 cited

Demarcating circulation regimes of synchronously rotating terrestrial planets within the habitable zone

Jacob Haqq-Misra, Eric. T. Wolf, Manoj Joshi +2

We investigate the atmospheric dynamics of terrestrial planets in synchronous rotation within the habitable zone of low-mass stars using the Community Atmosphere Model (CAM). The s…

physics.pop-ph2017★ 7 cited

The Drake Equation as a Function of Spectral Type and Time

Jacob Haqq-Misra, Ravi Kumar Kopparapu

This chapter draws upon astronomical observations and modeling to constrain the prevalence of communicative civilizations in the galaxy. We discuss the dependence of the Drake equa…

physics.pop-ph2017★ 30 cited

Why do we find ourselves around a yellow star instead of a red star?

Jacob Haqq-Misra, Ravi Kumar Kopparpu, Eric T. Wolf

M-dwarf stars are more abundant than G-dwarf stars, so our position as observers on a planet orbiting a G-dwarf raises questions about the suitability of other stellar types for su…

astro-ph.EP2017★ 205 cited

Habitable Moist Atmospheres On Terrestrial Planets Near the Inner Edge Of the Habitable Zone Around M-dwarfs

Ravi kumar Kopparapu, Eric T. Wolf, Giada Arney +4

Terrestrial planets in the habitable zones (HZs) of low-mass stars and cool dwarfs have received significant scrutiny recently because their shorter orbital periods increase their…

astro-ph.EP2017★ 95 cited

Constraints on Climate and Habitability for Earth-like Exoplanets Determined from a General Circulation Model

Eric T. Wolf, Aomawa L. Shields, Ravi K. Kopparapu +2

Conventional definitions of habitability require abundant liquid surface water to exist continuously over geologic timescales. Water in each of its thermodynamic phases interacts w…