Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005padeu..15..221s&link_type=abstract
In: Proceedings of the British-Romanian-Hungarian N+N+N Workshop for Young Researchers on Plasma- and Astrophysics: from laborat
Astronomy and Astrophysics
Astrophysics
Scientific paper
Zero velocity surfaces are deduced in the gravitational restricted three-body problem by using the Jacobi-integral. These surfaces are the boundaries of the Hill's regions: regions where the motion of the third, massless particle around the two primaries is possible. V. Szebehely generalized this result for the planar elliptic restricted three-body problem. In a recent paper the authors presented a generalization of this result for the spatial elliptic restricted three-body problem, where the existence of an invariant relation was proved. From this invariant relation the equation of the zero velocity surfaces can be deduced. In this paper we discuss the pulsation and the change of the type of these zero velocity surfaces and we present applications to the phenomenon of the gravitational capture. In the model of the spatial elliptic restricted three-body problem criteria of the capture are deduced by using the pulsating Hill's regions.
Makó Zoltán
Szenkovits Ferenc
No associations
LandOfFree
Pulsating zero velocity surfaces and capture in the elliptic restricted three-body problem does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Pulsating zero velocity surfaces and capture in the elliptic restricted three-body problem, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Pulsating zero velocity surfaces and capture in the elliptic restricted three-body problem will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1165600