On the relativistic theory of astrometric observations. II - Determination of the positions of remote sources from the earth's surface

Astronomy and Astrophysics – Astronomy

Scientific paper

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Astrometry, Celestial Reference Systems, Position (Location), Relativistic Theory, Celestial Sphere, Equinoxes

Scientific paper

Relativistic equations for the horizontal coordinates of remote cosmic sources are obtained on the basis of observational relations derived previously. The accuracy in calculating the relativistic corrections is 0.001 arcsec. The quadratic relativistic corrections to the apparent annual motion of three hypothetical stars located in the directions of the ecliptic north pole, the celestial north pole, and the point of the vernal equinox are calculated as an illustration.

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