Results 81 to 90 of about 19,604,258 (169)
JWST has provided unprecedented access to ultracool brown dwarfs and has pushed the boundaries of directly imaging temperate giant planets. As we continue to push toward detecting sub-Saturn and Neptune-like planets, it is crucial to develop atmospheric ...
James Mang +9 more
doaj +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
Simultaneous formation of solar system giant planets [PDF]
Context.In the last few years, the so-called Nice model has become increasingly significant for studying the formation and evolution of the solar system.
Brunini, Adrián +3 more
core
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
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
Changes in the metallicity of gas giant planets due to pebble accretion
We run numerical simulations to study the accretion of gas and dust grains on to gas giant planets embedded into massive protoplanetary discs. The outcome is found to depend on the disc cooling rate, planet mass, grain size, and irradiative feedback from
S. Nayakshin (7603412) +1 more
core +2 more sources
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
88th Annual Meeting of the Meteoritical Society 2026: Abstracts
Meteoritics &Planetary Science, Volume 61, Issue S1, Page S48-S551, August 2026.
wiley +1 more source

