A study of low velocities regions near the Roche lobe during the gas giant planets formation


Autoria(s): Moraes, Ricardo A.; Vieira Neto, Ernesto; IOP
Contribuinte(s)

Universidade Estadual Paulista (UNESP)

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