title: Investigation of the Moon rotation in the relativistic approximation
metadata.name: dc.contributor.author
metadata.value: Pashkevich, Vladimir V.
metadata.lang: -
metadata.name: dc.date.accessioned
metadata.value: 2017-12-27T14:46:00Z
metadata.lang: -
metadata.name: dc.date.available
metadata.value: 2017-12-27T14:46:00Z
metadata.lang: -
metadata.name: dc.date.issued
metadata.value: 2017-12
metadata.lang: -
metadata.name: dc.identifier.citation
metadata.value: Pashkevich V.V. Investigation of the Moon rotation in the relativistic approximation. Vestnik SPbSU. Mathematics. Mechanics. Astronomy, 2017, vol. 4 (62), issue 4, pp. 681–694.
metadata.lang: en_GB
metadata.name: dc.identifier.other
metadata.value: 10.21638/11701/spbu01.2017.416
metadata.lang: -
metadata.name: dc.identifier.uri
metadata.value: http://hdl.handle.net/11701/8813
metadata.lang: -
metadata.name: dc.description.abstract
metadata.value: The Moon rotation problem for the relativistic approximation, in which the geodetic perturbations (the
  most essential relativistic perturbations) in the Moon rotation are taken into account is studied. The
  discrepancies of the comparison between the high-precision numerical solutions and the semi-analytical
  solutions the Moon rotation problem are investigated by the numerical and analytical methods with respect
  to the fixed ecliptic of epoch J2000. As the result of this research in the first time are constructed the
  high-precision Moon Rotation Series MRS2016 in the relativistic approximation. The residuals between
  the numerical integration and MRS2016 in the perturbing terms of the physical librations do not surpass
  64 mas over 2000 and 8 arc seconds over 6000 years. Refs 21. Figs 4. Table 1.
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 Александра 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. Mathematics. Mechanics. Astronomy;Volume 4(62); Issue 4
metadata.lang: -
metadata.name: dc.subject
metadata.value: the Moon rotation
metadata.lang: en_GB
metadata.name: dc.subject
metadata.value: ephemeris
metadata.lang: en_GB
metadata.name: dc.subject
metadata.value: the numerical and the semi-analytical solutions
metadata.lang: en_GB
metadata.name: dc.subject
metadata.value: the relativistic approximation
metadata.lang: en_GB
metadata.name: dc.title
metadata.value: Investigation of the Moon rotation in the relativistic approximation
metadata.lang: en_GB
metadata.name: dc.type
metadata.value: Article
metadata.lang: en_GB
resources.filename: 16-Pashkevich.pdf
resources.url: https://dspace.spbu.ru/bitstream/11701/8813/1/16-Pashkevich.pdf
resources.format: Adobe PDF
resources.size: 1,43 MB