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Stellar astronomy / Planetary science / Nebular hypothesis / Planets / Photoevaporation / Protoplanetary disk / Circumstellar disk / Accretion / Planetary migration / Astronomy / Space / Solar System


January 3, 2014 Preprint typeset using LATEX style emulateapj v[removed]MODELS OF JUPITER’S GROWTH INCORPORATING THERMAL AND HYDRODYNAMIC CONSTRAINTS† Jack J. Lissauer, Olenka Hubickyj1 , Gennaro D’Angelo2 NASA A
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Document Date: 2014-12-10 16:17:43


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Company

Marley / Hp / /

Country

United States / /

Currency

pence / /

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Facility

UCO/Lick Observatory / University of California / /

IndustryTerm

gas Σg / gas drag / gas flow / gas accretion / gas molecules / narrow gas feeding zone / grid systems / gas surface density / gas mass / gas flow limits / gas pressure gradient / accrete gas / constant maximum gas accretion rate / instantaneous gas loss rate / gas accretion rate / gas density / Gas velocities / thermal energy / runaway gas accretion / linear gas surface density drop-off rate / thermal pressure pushing gas / gas loss rate / gas proceeds / gas pressure gradients / energy / energy transport / bound material gas / regulated gas accretion / gas rate / gas runaway / surface gas density decreases / gas feeding zone / rapid gas flow / slow gas accretion / unbound protoplanetary disk gas flowing / sufficient energy / distant gas / overall gas removal / interstellar gas / gas accretion rates / gas accretion zone / accrete additional gas / /

NaturalFeature

Growth Hill / /

Organization

Department of Astronomy and Astrophysics / Space Science and Astrobiology Division / University of California / Santa Cruz / Gennaro D’Angelo2 NASA Ames Research Center / African Union / National Aeronautics and Space Administration / /

Person

Jack J. Lissauer / Peter Bodenheimer / Angelo Models / Kary / /

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Position

Mp / XY Mp Mp / /

ProvinceOrState

California / /

PublishedMedium

Icarus / Astronomy and Astrophysics / /

Technology

X-ray / 3-D / Mp3 / secondorder Runge-Kutta algorithm / simulation / /

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