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Observation of solar system bodies on board the future russian astrometric satellite

Published online by Cambridge University Press:  25 May 2016

V.N. Yershov
V.N. Yershov*
Affiliation:
Pulkovo Observatory, 196140 St Petersburg, Russia e-mail: yersh@gao.spb.su

Abstract

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A future Russian astrometric satellite (Struve) is aimed at an extension of the fundamental coordinate system down to 18-th magnitude stars. The positional accuracy of observations is planned to be about 0.6 mas. Many of the Solar System objects will be observed by the Struve satellite. Problems of registration and reduction of these observations are discussed.

Type
Part X - Solar System Astrometry
Information
Symposium - International Astronomical Union , Volume 172: Dynamics, Ephemerides and Astrometry of the Solar System , 1996 , pp. 415 - 418
Copyright
Copyright © Kluwer 1996 

References

Kisselev, A.A., Bykov, O.P. (1976) Determination of the elliptical orbit of a satellite with the use of parameters of its apparent motion, Astron. J., 53(4), 879–888.Google Scholar
Yershov, V.N., Kanayev, I.I. (1994) Development of the Russian Space Astrometric Satellite, Third International Workshop on Positional Astronomy and Celestial Mechanics, ed. López García, A., Cuenca.Google Scholar