A study of low velocities regions near the Roche lobe during the gas giant planets formation
Contribuinte(s) |
Universidade Estadual Paulista (UNESP) |
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Data(s) |
03/12/2014
03/12/2014
01/01/2013
|
Resumo |
In this paper were studied regions close to the Roche lobe of a planet like Jupiter, in order to find regions with low velocities. We simulated a two dimensional and non-self-gravitating disk, where tidal and viscous torques are considered, using the hydrodynamic numerical integrator FARGO 2D. As stated earlier we are interested in find low velocities regions for in future works study the possibility of satellites formation in these regions. |
Formato |
6 |
Identificador |
http://dx.doi.org/10.1088/1742-6596/465/1/012015 Xvi Brazilian Colloquium On Orbital Dynamics. Bristol: Iop Publishing Ltd, v. 465, 6 p., 2013. 1742-6588 http://hdl.handle.net/11449/112104 10.1088/1742-6596/465/1/012015 WOS:000326877000015 WOS000326877000015.pdf |
Idioma(s) |
eng |
Publicador |
Iop Publishing Ltd |
Relação |
Xvi Brazilian Colloquium On Orbital Dynamics |
Direitos |
openAccess |
Tipo |
info:eu-repo/semantics/conferencePaper |