Results 41 to 50 of about 252 (123)

A New 2D Energy Balance Model for Simulating the Climates of Rapidly and Slowly Rotating Terrestrial Planets

open access: yesThe Planetary Science Journal
Energy balance models (EBMs), alongside radiative–convective climate models and global climate models (GCMs), are useful tools for simulating planetary climates.
Ramses M. Ramirez
doaj   +1 more source

Absence of a Runaway Greenhouse Limit on Lava Planets

open access: yesThe Astrophysical Journal
Climate transitions on exoplanets offer valuable insights into the atmospheric processes governing planetary habitability. Previous pure-steam atmospheric models show a thermal limit in outgoing long-wave radiation, which has been used to define the ...
Iris D. Boer   +2 more
doaj   +1 more source

Large planets may not form fractionally large moons. [PDF]

open access: yesNat Commun, 2022
Nakajima M, Genda H, Asphaug E, Ida S.
europepmc   +1 more source

Anatomy of Empirical Transit Spectra of Mars Based on TGO/NOMAD

open access: yesThe Astronomical Journal
Transit spectroscopy is a powerful tool for probing atmospheric structures of exoplanets. Accurately accounting for the effects of aerosols is key to reconstructing atmospheric properties from transit spectra, yet this remains a significant challenge. To
Shohei Aoki   +12 more
doaj   +1 more source

Toward Reliable Interpretations of Small-exoplanet Compositions: Comparisons and Considerations of Equations of State and Materials Used in Common Rocky Planet Models

open access: yesThe Planetary Science Journal
The bulk compositions of small planets ( R _p < 2 R _⊕ ) are directly linked to their formation histories, making reliable compositional constraints imperative for testing models of planet formation and evolution.
Joseph G. Schulze   +3 more
doaj   +1 more source

Haze Optical Depth in Exoplanet Atmospheres Varies with Rotation Rate: Implications for Observations

open access: yesThe Astronomical Journal
Transmission spectroscopy supports the presence of uncharacterized, light-scattering and -absorbing hazes in the atmospheres of many exoplanets. The complexity of factors influencing the formation, 3D transport, radiative impact, and removal of hazes ...
Maureen Cohen   +4 more
doaj   +1 more source

Synergies Between Venus & Exoplanetary Observations: Venus and Its Extrasolar Siblings. [PDF]

open access: yesSpace Sci Rev, 2023
Way MJ   +11 more
europepmc   +1 more source

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