Results 101 to 110 of about 65,635 (192)
CoRoT-2b: a Tidally Inflated, Young Exoplanet?
, 2009 CoRoT-2b is among the most anomalously large transiting exoplanet known. Due to its large mass (3.3 Mjup), its large radius (~1.5 Rjup) cannot be explained by standard evolution models.
Guillot, Tristan, Havel, Mathieu
core
, 2020 This photo is an overhead shot of the waves breaking at Pine Point beach. This represents so much for me. In these times of uncertainty it gives me hope that the tides will eventually turn.
Eo, Paul S
core
Planet–Planet Scattering and Von Zeipel–Lidov–Kozai Migration—The Dynamical History of HAT-P-11
The Astrophysical JournalThe two planets of the HAT-P-11 system represent fascinating dynamical puzzles due to their significant eccentricities and orbital misalignments. In particular, HAT-P-11 b is in a close-in orbit in which tides should have circularized well within the age
Tiger Lu +6 more
doaj +1 more source
, 1977 Classic earth science textbooks present a rather generalized treatment of the topic of tides, but to the majority of mid-westerners the descriptions are largely without intrinsic meaning because of the lack of firsthand experience with marine tides.
Hoff, Darrel
core +1 more source
Planetary Obliquity Excitation through Pre-main-sequence Stellar Evolution
The Astrophysical JournalA planet’s axial tilt (“obliquity”) substantially affects its atmosphere and habitability. It is thus essential to comprehend the various mechanisms that can excite planetary obliquities, particularly at the primordial stage.
Sidhant Kumar Suar, Sarah C. Millholland
doaj +1 more source
, 2019 Tides on planet Earth are generated by the gravitational attraction of the Moon and Sun. In the global ocean the observed tides are strongly controlled by the responses of the oceans basins to the direct tidal forcing. Analysis of tidal measurements, and
David Pugh, Pugh, David
core +1 more source
Spin Dynamics of Planets in Resonant Chains
The Astrophysical JournalAbout 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]
Astrophys J, 2021 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
Tidal Migration of Exoplanets around M Dwarfs: Frequency-dependent Tidal Dissipation
The Astrophysical JournalThe orbital architectures of short-period exoplanet systems are shaped by tidal dissipation in their host stars. For low-mass M dwarfs whose dynamical tidal response comprises a dense spectrum of inertial modes at low frequencies, resolving the frequency
Samantha C. Wu +2 more
doaj +1 more source