Results 171 to 180 of about 152,640 (256)
Puffy Venuses: The Mass–Radius Impact of Carbon-rich Atmospheres on Lava Worlds
The recent advancements in exoplanet observations enable the potential detection of exo-Venuses, rocky planets with carbon-rich atmospheres. How extended these atmospheres can be, given high carbon abundances, has not been studied.
Bo Peng, Diana Valencia
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Photochemically produced SO2 in the atmosphere of WASP-39b. [PDF]
Tsai SM+84 more
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Analogous response of temperate terrestrial exoplanets and Earth's climate dynamics to greenhouse gas supplement. [PDF]
Hochman A, Komacek TD, De Luca P.
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Some sub-Neptune planets may host habitable conditions; for example “Hycean” worlds with H _2 envelopes over liquid water oceans can maintain potentially hospitable pressures and temperatures at their surface.
Michaela Leung+4 more
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No thick carbon dioxide atmosphere on the rocky exoplanet TRAPPIST-1 c. [PDF]
Zieba S+18 more
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Previous attempts have been made to characterize the atmospheres of directly imaged planets at low resolution ( R ∼ 10–100 s), but the presence of clouds has often led to degeneracies in the retrieved atmospheric abundances with cloud opacity and ...
Julie Inglis+9 more
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Synergies Between Venus & Exoplanetary Observations: Venus and Its Extrasolar Siblings. [PDF]
Way MJ+11 more
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An ultra-short-period super-Earth with an extremely high density and an outer companion. [PDF]
Livingston JH+20 more
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A qualitative assessment of limits of active flight in low density atmospheres. [PDF]
Pajusalu M+3 more
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