MRS2016: rigid Moon Rotation Series in the relativistic approximation

• Autorzy: Pashkevich V. V.

Identyfikatory

DOI

10.1515/arsa-2017-0001

• Języki publikacji: EN

Abstrakty

EN

The rigid Moon rotation problem is studied for the relativistic (kinematical) case, in which the geodetic perturbations in the Moon rotation are taken into account. As the result of this research the high-precision Moon Rotation Series MRS2016 in the relativistic approximation was constructed for the first time and the discrepancies between the highprecision numerical and the semi-analytical solutions of the rigid Moon rotation were investigated with respect to the fixed ecliptic of epoch J2000, by the numerical and analytical methods. The residuals between the numerical solution and MRS2016 in the perturbing terms of the physical librations do not exceed 80 mas and 10 arc seconds over 2000 and 6000 years, respectively.

Słowa kluczowe

EN

rigid Moon rotation; ephemerides; numerical solutions; semi-analytical solution; relativistic approximation

• Wydawca: Centrum Badań Kosmicznych PAN ; De Gruyter
• Czasopismo: Artificial Satellites : Journal of Planetary Geodesy
• Rocznik: 2017
• Tom: Vol. 52, No. 1
• Strony: 1--8
• Opis fizyczny: Bibliogr. 9 poz., rys., tab.

Twórcy

autor

Pashkevich V. V.

• Central (Pulkovo) Astronomical Observatory of RAS Pulkovskoe shosse, 65/1, 196140, St.Petersburg, Russia

Bibliografia

• Eckhardt D.H. (1981) Theory of Libration of the Moon, The Moon and the planets, 25, pp.3-49.
• Brumberg V.A., Bretagnon P. (2000) Kinematical Relativistic Corrections for Earth’s Rotation Parameters, in Proc. of IAU Colloquium 180, eds. K.Johnston, D. McCarthy, B. Luzum and G. Kaplan, U.S. Naval Observatory, pp. 293-302.
• Pashkevich V.V., Eroshkin G.I. (2005) Application of the spectral analysis for the mathematical modelling of the rigid Earth rotation, Artificial Satellites, Warszawa, 2005, Vol. 40, No 4, pp. 251-259.
• Eroshkin G.I., Pashkevich V.V. (2009) On the geodetic rotation of the major planets, the Moon and the Sun, Artificial Satellites, Warszawa, 2009, Vol. 44, No. 2, pp. 43-52.
• Pashkevich V.V., Eroshkin G.I. (2010) Application of the spectral analysis for modeling the rotations of the Moon, Artificial Satellites, Warszawa, 2010, Vol. 45, No 4, pp.153-162.
• Folkner W.F. (2011) JPL Planetary and Lunar Ephemerides: Export Information http://iaucomm4. jpl.nasa.gov/README.html.
• Pashkevich V.V., Eroshkin G.I. (2011) Construction of the new high-precision Moon rotation series at a long time intervals, Artificial Satellites, Warszawa, 2011, Vol. 46. No. 2. (DOI: 10.2478/v10018-011-0013-3), pp. 63-73.
• Pashkevich V.V. (2015) RERS2014 and MRS2014: new high-precision rigid Earth rotation and Moon rotation series, Artificial Satellites, Warszawa, 2015, Vol. 50, No. 1 (DOI: 10.1515/arsa-2015-0003), pp. 35-40.
• Pashkevich V.V. (2016) New high-precision values of the geodetic rotation of the major planets, Pluto, the Moon and the Sun, Artificial Satellites, Warszawa, 2016, Vol. 51, No. 2 (DOI: 10.1515/arsa-2016-0006), pp. 61-73.

Uwagi

Opracowanie rekordu ze środków MNiSW, umowa Nr 461252 w ramach programu "Społeczna odpowiedzialność nauki" - moduł: Popularyzacja nauki i promocja sportu (2020).