Results 81 to 90 of about 19,604,258 (169)

The Sonora Substellar Atmosphere Models. VII. Flame Skimmer: Cloud-free Atmospheric and Evolutionary Models for the Coldest Substellar Objects

open access: yesThe Astrophysical Journal
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

open access: yesThe Planetary Science Journal
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]

open access: yes, 2019
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

open access: yesThe Astrophysical Journal
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

open access: yesThe Astrophysical Journal
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

open access: yes, 2018
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

open access: yesThe Astrophysical Journal Letters
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

The JWST Weather Report from the Isolated Exoplanet Analog SIMP 0136+0933: Pressure-dependent Variability Driven by Multiple Mechanisms

open access: yesThe Astrophysical Journal Letters
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

open access: yes
Meteoritics &Planetary Science, Volume 61, Issue S1, Page S48-S551, August 2026.
wiley   +1 more source

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