Results 91 to 100 of about 26,515 (184)
Exoplanetary Geophysics -- An Emerging Discipline
Thousands of extrasolar planets have been discovered, and it is clear that the galactic planetary census draws on a diversity greatly exceeding that exhibited by the solar system's planets.
Adachi +225 more
core +1 more source
Constraints on the Long-term Existence of Dilute Cores in Giant Planets
Post-Cassini ring seismology analysis suggests the existence of a stable stratification inside Saturn that extends from the center to ∼60% of its radius, in what is recognized today as Saturn’s dilute core.
A. Tulekeyev +3 more
doaj +1 more source
We examine how the late divergent migration of Jupiter and Saturn may have perturbed the terrestrial planets. We identify six secular resonances between the nu_5 apsidal eigenfrequency of Jupiter and Saturn and the four eigenfrequencies of the ...
Adams +39 more
core +1 more source
Penetrative Convection in Rotating Tilted f-plane with Multiple Radiative and Convective Layers
In this paper, we conducted a linear instability analysis to investigate penetrative convection in rotating, tilted f -planes with multiple convectively stable and unstable layers. Our findings indicate that penetrative distance decreases with increasing
Sethulakshmy Edathara Sreenivasan +1 more
doaj +1 more source
Elemental ratios in stars vs planets
Context. The chemical composition of planets is an important constraint for planet formation and subsequent differentiation. While theoretical studies try to derive the compositions of planets from planet formation models in order to link the composition
Alibert, Yann +4 more
core +1 more source
On the Meaning of the Dynamo Radius in Giant Planets with Stable Layers
Current structure models of Jupiter and Saturn suggest that helium becomes immiscible in hydrogen in the outer part of the planets’ electrically conducting regions.
Paula N. Wulff +2 more
doaj +1 more source
It is widely accepted that Titan and the mid-sized regular satellites around Saturn were formed in the circum-Saturn disk. Thus, if these mid-sized satellites were simply accreted by collisions of similar ice-rock satellitesimals in the disk, the ...
Agnor +56 more
core +1 more source
Thermal Emission and Confirmation of the Frigid White Dwarf Exoplanet WD 1856+534 b
We report the detection of thermal emission from and confirm the planetary nature of WD 1856+534 b, the first transiting planet known to orbit a white dwarf (WD) star.
Mary Anne Limbach +14 more
doaj +1 more source
Isolated planetary-mass objects share their mass range with planets but do not orbit a star. They lack the necessary mass to support fusion in their cores and thermally radiate their heat from formation as they cool, primarily at infrared wavelengths ...
Allison M. McCarthy +19 more
doaj +1 more source
Jupiter Evolutionary Models Incorporating Stably Stratified Regions
We address the issue of which broad set of initial conditions for the planet Jupiter best matches the current presence of a “fuzzy core” of heavy elements, while at the same time comporting with measured parameters such as its effective temperature ...
Roberto Tejada Arevalo +3 more
doaj +1 more source

