Results 81 to 90 of about 10,001 (169)
86th Annual Meeting of the Meteoritical Society (2024)
Meteoritics &Planetary Science, Volume 59, Issue S1, Page A1-A468, August 2024.
wiley +1 more source
The Coupled Impacts of Atmospheric Composition and Obliquity on the Climate Dynamics of TRAPPIST-1e
Planets in multiplanet systems are expected to migrate inward as near-resonant chains, thus allowing them to undergo gravitational planet–planet interactions and possibly maintain a nonzero obliquity.
Tobi Hammond, Thaddeus D. Komacek
doaj +1 more source
Planetary population synthesis and the emergence of four classes of planetary system architectures. [PDF]
Emsenhuber A, Mordasini C, Burn R.
europepmc +1 more source
Energy balance models (EBMs), alongside radiative–convective climate models and global climate models (GCMs), are useful tools for simulating planetary climates.
Ramses M. Ramirez
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Absence of a Runaway Greenhouse Limit on Lava Planets
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
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Revealing the atmospheres of highly irradiated exoplanets: from ultra-hot Jupiters to rocky worlds. [PDF]
Mansfield M.
europepmc +1 more source
Anatomy of Empirical Transit Spectra of Mars Based on TGO/NOMAD
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
Carbon Cycle Imbalances on Arid Terrestrial Planets with Implications for Venus
Arid terrestrial exoplanets are potentially abundant and are thus interesting targets in the search for life. In particular, M-dwarf planets such as those in the TRAPPIST-1 system may possess limited surface water, whereas early solar system terrestrials
Haskelle T. White-Gianella +1 more
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Synergies Between Venus & Exoplanetary Observations: Venus and Its Extrasolar Siblings. [PDF]
Way MJ +11 more
europepmc +1 more source
The standard formation model of close-in low-mass planets involves efficient inward migration followed by growth through giant impacts after the protoplanetary gas disk disperses.
Tadahiro Kimura +4 more
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