title: Geodetic (relativistic) rotation of the solar system bodies
metadata.name: dc.contributor.author
metadata.value: Pashkevich, Vladimir V.
metadata.lang: -
metadata.name: dc.date.accessioned
metadata.value: 2016-09-28T16:20:29Z
metadata.lang: -
metadata.name: dc.date.available
metadata.value: 2016-09-28T16:20:29Z
metadata.lang: -
metadata.name: dc.date.issued
metadata.value: 2016-09
metadata.lang: -
metadata.name: dc.identifier.citation
metadata.value: Pashkevich V.V. Geodetic (relativistic) rotation of the solar system bodies. Vestnik of Saint Petersburg University. Series 1. Mathematics. Mechanics. Astronomy, 2016, vol. 3 (61), issue 3, pp. 506–516.
metadata.lang: en_GB
metadata.name: dc.identifier.other
metadata.value: 10.21638/11701/spbu01.2016.319
metadata.lang: -
metadata.name: dc.identifier.uri
metadata.value: http://hdl.handle.net/11701/3921
metadata.lang: -
metadata.name: dc.description.abstract
metadata.value: This investigation is continuation of our studies of the geodetic (relativistic) rotation of the Solar system
  bodies. For each body (the Moon, the Sun, the major planets and Pluto) the files of the values of the
  components of the angular velocity of the geodetic rotation are constructed over the time span from
  AD1000 to AD3000 with one day spacing, by using JPL DE422/LE422 ephemeris, with respect to the
  proper coordinate systems of the bodies. New method for calculation the values of the geodetic rotation
  any bodies of the Solar system was received. This method has a good confirmation of the results for the
  Earth case. In the first time in the perturbing terms of the physical librations for the Moon and in Euler
  angles for other bodies of the Solar system the most essential terms of the geodetic rotation are found
  by means of the least squares method and spectral analysis methods. For the Sun, giant planets and
  Pluto the geodetic rotation is insignificant. For the terrestrial planets and the Moon the geodetic rotation
  is significant and has to be taken into account for the construction of the high-precision theories of the
  rotational motion of these bodies. Refs 14. Figs 1. Tables 2.
metadata.lang: en_GB
metadata.name: dc.description.sponsorship
metadata.value: Работа выполнена при финансовой поддержке в рамках сотрудничества между Польской
  и Российской академиями наук (тема №34) и персонального гранта А.Бжезиньского (№ DEC-2012/05/B/ST10/02132).
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: geodetic (relativistic) rotation of the Solar system bodies
metadata.lang: en_GB
metadata.name: dc.subject
metadata.value: ephemeris
metadata.lang: en_GB
metadata.name: dc.title
metadata.value: Geodetic (relativistic) rotation of the solar system bodies
metadata.lang: en_GB
metadata.name: dc.type
metadata.value: Article
metadata.lang: en_GB
resources.filename: Pashkevich.pdf
resources.url: https://dspace.spbu.ru/bitstream/11701/3921/1/Pashkevich.pdf
resources.format: Adobe PDF
resources.size: 407,92 kB