Relativistic theory of astrometric observations. I Determination of the positions of remote sources from the surfaces of solar-system bodies

Details Relativistic theory of astrometric observations. I Determination of the positions of remote sources from the surfaces of solar-system bodies Relativistic theory of astrometric observations. I Determination of the positions of remote sources from the surfaces of solar-system bodies

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984azh....61..385p&link_type=abstract

(Astronomicheskii Zhurnal, vol. 61, Mar.-Apr. 1984, p. 385-392) Soviet Astronomy (ISSN 0038-5301), vol. 28, Mar.-Apr. 1984, p. 2

Astronomy and Astrophysics

Astronomy

1

Astrometry, Astronomical Coordinates, Relativistic Effects, Solar System, Celestial Reference Systems, Correction, Position (Location), Relativistic Theory

Scientific paper

Equations for the rectangular components of the unit vector in the apparent direction toward a remote cosmic source are obtained within the framework of the post-Newtonian approximation of the GTR. It is assumed that the astronomical observations are made from the surface of a celestial body which is in an arbitrary heliocentric orbit. All relativistic corrections due to the solar gravitational field and the motion of the observer are taken into account in the resulting observational relations within the limits of the adopted accuracy of the calculations.

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