Results 171 to 180 of about 55,109 (308)
Hot Jupiters Are Asynchronous Rotators
The Astrophysical Journal LettersHot Jupiters are typically assumed to be synchronously rotating, from tidal locking. Their thermally driven atmospheric winds experience Lorentz drag on the planetary magnetic field anchored at depth.
Marek Wazny, Kristen Menou
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Non-solar noble gas abundances in the atmosphere of Jupiter [PDF]
The thermodynamic stability of clathrate hydrate is calculated to predict the formation conditions corresponding to a range of solar system parameters. The calculations were performed using the statistical mechanical theory developed by van der Waals and
Lunine, Jonathan I., Stevenson, David J.
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Impact of Jupiter’s Heating and Self-shadowing on the Jovian Circumplanetary Disk Structure
The Planetary Science JournalDeciphering the structure of the circumplanetary disk (CPD) that surrounded Jupiter at the end of its formation is key to understanding how the Galilean moons formed.
Antoine Schneeberger, Olivier Mousis
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High-temperature condensate clouds in super-hot Jupiter atmospheres [PDF]
, 2016 Hannah R. Wakeford +6 more
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The Hubble PanCET Program: A Metal-rich Atmosphere for the Inflated Hot Jupiter HAT-P-41b [PDF]
, 2021 Kyle Sheppard +16 more
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The behavior of fragments of comet Shoemaker-Levy 9 in the atmosphere of Jupiter
, 1995 G. Field, A. Ferrara
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HST hot-Jupiter transmission spectral survey: haze in the atmosphere of WASP-6b [PDF]
, 2014 Nikolay Nikolov +16 more
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Behavior of metal-containing species during entries of meteoroids into atmospheres of Mars, Jupiter, and Titan [PDF]
, 2011 A. A. Berezhnoy
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Modeled Temperature-dependent Clouds with Radiative Feedback in Hot Jupiter Atmospheres [PDF]
, 2019 Michael T. Roman, Emily Rauscher
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