New high-precision values of the geodetic rotation of the major planets, Pluto, the Moon and the Sun

• Autorzy: Pashkevich V. V.

Identyfikatory

DOI

10.1515/arsa-2016-0006

• Języki publikacji: EN

Abstrakty

EN

This investigation is continuation of our studies of the geodetic (relativistic) rotation of the Solar system bodies (Eroshkin and Pashkevich, 2007) and (Eroshkin and Pashkevich, 2009). 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 DE422/LE422 ephemeris (Folkner, 2011), with respect to the proper coordinate systems of the bodies (Seidelmann et al., 2005). For 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.

Słowa kluczowe

EN

geodetic rotation; relativistic rotation; angular velocity vector; solar system bodies; reference frame; major planets; Pluto; Moon; Sun; ephemeris

• Wydawca: Centrum Badań Kosmicznych PAN ; De Gruyter
• Czasopismo: Artificial Satellites : Journal of Planetary Geodesy
• Rocznik: 2016
• Tom: Vol. 51, No. 2
• Strony: 61--73
• Opis fizyczny: Bibliogr. 10 poz., rys., tab.

Twórcy

autor

Pashkevich V. V.

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

Bibliografia

• Woolard E.W. (1953) Theory of the rotation of the Earth around its center of mass, in Astronomical Papers for the American Ephemeris and Nautical Almanac XV, Part 1, U.S. Government Printing Office, Washington.
• Bretagnon P.and Francou G. (1988) Planetary theories in rectangular and spherical variables, Astronomy and Astrophysics, 202, pp. 309-315.
• Standish E.M., Newhall X X, Williams J.G. and Folkner W.M. (1995) JPL Planetary and Lunar Ephemerides, DE403/LE403, JPL IOM 314.10-127.
• Bretagnon P., Francou G., Rocher P., Simon J.L. (1998) SMART97: A new solution for the rotation of the rigid Earth, Astron. Astrophys. , 329, 1, pp. 329-338.
• 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.
• Seidelmann P.K., Archinal B.A., A'Hearn M.F., Cruikshank D.P., Hilton J.L., Keller H.U., Oberst J., Simon J.L., Stooke P., Tholen D.J., and Thomas P.C. (2005) Report of the IAU/IAG Working Group on Cartographic Coordinates and Rotational Elements: 2003, Celestial Mechanics and Dynamical Astronomy, 91, pp. 203-215.
• Eroshkin G.I., Pashkevich V.V. (2007) Geodetic rotation of the Solar system bodies, Artificial Satellites, Vol. 42, No. 1, pp. 59-70.
• Eroshkin G.I., Pashkevich V.V. (2009) On the geodetic rotation of the major planets, the Moon and the Sun, Artificial Satellites, Vol. 44, No. 2, pp 43-52.
• 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, Vol. 46. No. 2. (DOI: 10.2478/v10018-011-0013-3), pp. 63-73.

Uwagi

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