title: The hill stability of planetary motion under stellar approaches
metadata.name: dc.contributor.author
metadata.value: Mammadli, Azad Hidayat oglu
metadata.lang: -
metadata.name: dc.date.accessioned
metadata.value: 2016-09-28T16:18:18Z
metadata.lang: -
metadata.name: dc.date.available
metadata.value: 2016-09-28T16:18:18Z
metadata.lang: -
metadata.name: dc.date.issued
metadata.value: 2016-09
metadata.lang: -
metadata.name: dc.identifier.citation
metadata.value: Mammadli A.H. The hill stability of planetary motion under stellar approaches. Vestnik of Saint Petersburg University. Series 1. Mathematics. Mechanics. Astronomy, 2016, vol. 3 (61), issue 3, pp. 498–505.
metadata.lang: en_GB
metadata.name: dc.identifier.other
metadata.value: 10.21638/11701/spbu01.2016.318
metadata.lang: -
metadata.name: dc.identifier.uri
metadata.value: http://hdl.handle.net/11701/3920
metadata.lang: -
metadata.name: dc.description.abstract
metadata.value: A planetary motion under the influence of a star passing near the Solar system is examined in the
  framework of the three-dimensional restricted three-body problem. The exact expression of the force
  function without expansion it in series is used. An integral invariant relation —quasi-integral —is found,
  and regions of possible motion of a passively gravitating body are determined. Surfaces of minimal energy
  which are generalizations of surfaces of zero velocity are plotted. The Hill stability of planetary motion is
  investigated when a star with a mass between one and five solar masses approaches the Solar system at a
  minimum distance of 50 AU up to 100 AU. The results obtained are shown in the form of tables. Refs 10.
  Tables 2.
metadata.lang: en_GB
metadata.name: dc.description.sponsorship
metadata.value: Работа выполнена при финансовой поддержке Фонда развития науки при президенте Азербайджанской Республики (грант №EIF- 2013-9(15)-46/14/1).
metadata.lang: en_GB
metadata.name: dc.language.iso
metadata.value: ru
metadata.lang: en_GB
metadata.name: dc.publisher
metadata.value: St Petersburg State University
metadata.lang: en_GB
metadata.name: dc.relation.ispartofseries
metadata.value: Vestnik of St Petersburg University. Series 1. Mathematics. Mechanics. Astronomy;Vol. 3 (61); Issue 3
metadata.lang: -
metadata.name: dc.subject
metadata.value: celestial mechanics
metadata.lang: en_GB
metadata.name: dc.subject
metadata.value: restricted three-body problem
metadata.lang: en_GB
metadata.name: dc.subject
metadata.value: quasi-integral
metadata.lang: en_GB
metadata.name: dc.subject
metadata.value: law of conservation of energy
metadata.lang: en_GB
metadata.name: dc.subject
metadata.value: surfaces of minimal energy
metadata.lang: en_GB
metadata.name: dc.subject
metadata.value: Hill stability
metadata.lang: en_GB
metadata.name: dc.title
metadata.value: The hill stability of planetary motion under stellar approaches
metadata.lang: en_GB
metadata.name: dc.type
metadata.value: Article
metadata.lang: en_GB
resources.filename: Mammadli.pdf
resources.url: https://dspace.spbu.ru/bitstream/11701/3920/1/Mammadli.pdf
resources.format: Adobe PDF
resources.size: 226,36 kB