Results 91 to 100 of about 464 (180)
Past work has shown that ocean salinity and planetary obliquity both influence the climates of Earth-like exoplanets throughout the habitable zone of Sun-like stars.
Kyle Batra +2 more
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
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
With the recent discoveries of hundreds of extrasolar planets, the search for planets like Earth and life in the universe is quickly gaining momentum. In the future, large space observatories could directly detect the light scattered from rocky planets ...
M Vazquez +4 more
core
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
Revealing the atmospheres of highly irradiated exoplanets: from ultra-hot Jupiters to rocky worlds. [PDF]
Mansfield M.
europepmc +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
doaj +1 more source
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
Synergies Between Venus & Exoplanetary Observations: Venus and Its Extrasolar Siblings. [PDF]
Way MJ +11 more
europepmc +1 more source

