On the relation between zero-points of the dynamical (DE200) and catalogue (FK5) reference frames from observations of the Sun 1941 - 1982.

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The authors discuss the relation between catalogue and dynamical zero-points from observations of the Sun using the geometrical and analytical approaches. The comparative analysis of equations used is carried out. Washington (1941 - 1977) and Greenwich (1942 - 1982) observations of the Sun have been reduced to the FK4 and FK5 systems. The angles of mutual orientation of axes of dynamical (DE200) and catalogue (FK5) reference frames have been estimated. The results based on the geometrical approach are characterized by better convergence and higher accuracy. The assumption is made that the effect of the non-precessional equinox motion may be a consequence of an imperfection of the technique of its study as well as of the incomplete theory of the Sun motion.

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