Blowin’ in the Nonisothermal Wind: Core-powered Mass Loss with Hydrodynamic Radiative Transfer
The mass loss rates of planets undergoing core-powered escape are usually modeled using an isothermal Parker-type wind at the equilibrium temperature, T _eq .
William Misener +3 more
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A young progenitor for the most common planetary systems in the Galaxy. [PDF]
Livingston JH +41 more
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On the coincidence between the close passage of HD7977 and the Pliocene-Pleistocene transition. [PDF]
Cao Z, Loeb A, MacLeod M.
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A universal brown dwarf desert formed between planets and stars. [PDF]
Cui K +12 more
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Exo-Geoscience Perspectives Beyond Habitability. [PDF]
Spohn T +7 more
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Large-amplitude variability driven by giant dust storms on a planetary-mass companion. [PDF]
Tan X +19 more
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Upper Atmosphere Dynamics and Drivers of Volatiles Loss from Terrestrial-Type (Exo)Planets. [PDF]
Kubyshkina D +9 more
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Shock compression of FeOOH and implications for iron-water interactions in super-earth magma oceans. [PDF]
Zhang Y +21 more
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Prospects for detecting signs of life on exoplanets in the JWST era. [PDF]
Seager S +4 more
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Exploring the chaotic future and the deterministic past of the Solar System: an interview with Jacques Laskar. [PDF]
Li M, Zhao W.
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