Results 131 to 140 of about 349,003 (221)

Detecting an Ocean Inside Callisto With Geodetic Measurements From Europa Clipper and Juice

open access: yesGeophysical Research Letters
Determining whether Callisto hosts a subsurface ocean, and the implications for material and energy transport through its hydrosphere, is of high interest to NASA's Europa Clipper and ESA's Juice missions. A recent reanalysis of Galileo magnetometer data
Flavio Petricca   +2 more
doaj   +1 more source

The Formation of Ultra-short-period Planets under the Influence of the Nearby Planetary Companions

open access: yesThe Astrophysical Journal
Ultra-short-period (USP) planets, defined as those with orbital periods shorter than 1 day, provide valuable insights into planetary evolution under strong stellar tidal interactions.
Jiajun Zhu   +3 more
doaj   +1 more source

Tidal Heating in a Subsurface Magma Ocean on Io Revisited

open access: yesGeophysical Research Letters
We investigate the tidal dissipation in Io's hypothetical fluid magma ocean using a new approach based on the solution of the 3D Navier‐Stokes equations.
B. Aygün, O. Čadek
doaj   +1 more source

Tidal dissipation in the dense anelastic core of giant planets

open access: yes, 2014
International audienceThe prescriptions used today in celestial mechanics to describe dynamical processes, such as tidal interactions, are somewhat crude. In particular, the quality factor Q, quantifying the tidal dissipation, is often taken as constant,
Remus, Françoise   +2 more
core   +2 more sources

Amplifying Resonant Repulsion with Inflated Young Planets, Overlooked Inner Planets, and Nonzero Initial Δ

open access: yesThe Astrophysical Journal
Most multiplanet systems around mature (∼5 Gyr old) host stars are nonresonant. Even the near-resonant planet pairs still display 1%–2% positive deviation from perfect period commensurabilities (Δ) near first-order mean motion resonances (MMRs). Resonant
Yuancheng Xu, Fei Dai
doaj   +1 more source

Tidal dissipation in binary systems

open access: yes, 2005
International audienceTo first approximation, a binary system conserves its angular momentum while it evolves to its state of minimum kinetic energy: circular orbit, all spins aligned, and components rotating in synchronism with the orbital motion.
Zahn, Jean-Paul
core   +1 more source

Patient-Specific Computational Fluid Dynamics Modeling of Airway Collapse in Infants With Robin Sequence. [PDF]

open access: yesInt J Numer Method Biomed Eng
Jalori G   +5 more
europepmc   +1 more source

Good vibrations: Exploring how orbital resonance shapes the Galilean moons. [PDF]

open access: yesNat Commun
Veenstra A   +4 more
europepmc   +1 more source

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