Results 91 to 100 of about 134,248 (173)
Spin Dynamics of Planets in Resonant Chains
About a dozen exoplanetary systems have been discovered with three or more planets participating in a sequence of mean-motion resonances. The unique and complex architectures of these so-called “resonant chains” motivate efforts to characterize their ...
Sarah C. Millholland +2 more
doaj +1 more source
On a Possible Solution to the Tidal Realignment Problem for Hot Jupiters. [PDF]
Anderson KR, Winn JN, Penev K.
europepmc +1 more source
87th Annual Meeting of the Meteoritical Society 2025: Abstracts
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley +1 more source
The Effect of Ocean Salinity on Climate and Its Implications for Earth's Habitability. [PDF]
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
TOI-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
Ocean Tides on Asynchronously Rotating Planets Orbiting Low-mass Stars
Planets 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]
Thomas N.
europepmc +1 more source
TOI-1266 is a benchmark system of two temperate (
Michael Greklek-McKeon +40 more
doaj +1 more source
Long-Term Earth-Moon Evolution With High-Level Orbit and Ocean Tide Models. [PDF]
Daher H +17 more
europepmc +1 more source

