Results 111 to 120 of about 65,635 (192)
The Effect of Ocean Salinity on Climate and Its Implications for Earth's Habitability. [PDF]
Geophys Res Lett, 2022 Olson S +4 more
europepmc +1 more source
The PFS View of TOI-677 b: A Spin–Orbit Aligned Warm Jupiter in a Dynamically Hot System
The Astronomical JournalTOI-677 b is part of an emerging class of “tidally detached” gas giants ( a / R _⋆ ≳ 11) that exhibit large orbital eccentricities and yet low stellar obliquities. Such sources pose a challenge for models of giant planet formation, which must account for
Qingru Hu +11 more
doaj +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
An exoplanet is a planet that orbits another star other than the Sun; since 1988, more than 4,300 of them have been confirmed. This catalogue provides a visual way to visualise exoplanets in their solar systems, together with their habitable zones.
Zucconi, Alan
core +3 more sources
Causes of Hot Jupiter Inflation from Causal Discovery
The Astronomical JournalHot Jupiters often have radii larger than predicted by standard cooling–contraction models, but it remains unclear which process supplies or preserves the extra internal heat. We analyze 328 short-period giant planets with measured M _p , R _p , P _orb ,
Zehao Jin +5 more
doaj +1 more source
, 2019 Inhalt: Acknowledgments; 1. Introductory concepts; 2. Tidal forcing; 3. Celestial motions; 4. Tidal constituents and the harmonic method; 5. Tidal wave propagation; 6. Tides in coastal seas and basins; 7.
Gerkema, Theo 1965-
core
Revised exoplanet radii and habitability using Gaia Data Release 2
, 2018 Accurate stellar properties are crucial for determining exoplanet characteristics. Gaia DR2 presents revised distances, luminosities, and radii for 1.6 billion stars. Here, we report the calculation of revised radii and densities for 320 exoplanets using
Johns, Daniel +6 more
core +1 more source
Ocean Tides on Asynchronously Rotating Planets Orbiting Low-mass Stars
The Astrophysical JournalPlanets in the liquid-water habitable zone of low-mass stars experience large tidal forces, 10 ^3 –10 ^4 times those on Earth, due to the small distance between the habitable zone and the host stars.
Jiaru Shi +5 more
doaj +1 more source
A comprehensive investigation of the Galilean moon, Io, by tracing mass and energy flows. [PDF]
Exp Astron (Dordr), 2022 Thomas N.
europepmc +1 more source
Atmospheric composition of exoplanets based on the thermal escape of gases and implications for habitability. [PDF]
Proc Math Phys Eng Sci, 2020 Konatham S, Martin-Torres J, Zorzano MP.
europepmc +1 more source