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The results of photographic observations of Galilean satellites with 26-inch refractor at Pulkovo

Published online by Cambridge University Press:  25 May 2016

T.P. Kisseleva
T.P. Kisseleva*
Affiliation:
The Main Astronomical Observatory Russian Academy of Science, Pulkovskoe shosse, 65-1, St. Petersburg, 196140, Russia

Abstract

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Photographic observations of the Galilean satellites of Jupiter have been made in Pulkovo with 26-inch refractor during two periods 1976–1981 and 1986–1993. The internal mean square errors of jovicentric coordinates and mutual distances is equal to 0.10 arcsec. The external errors are equal to 0.08 and 0.17 arcsec in AR and Decl. The systematic errors were analysed. The errors of the theory G-5 of J.E. Arlot do not exceed 0.1 arcsec.

Type
Part X - Solar System Astrometry
Information
Symposium - International Astronomical Union , Volume 172: Dynamics, Ephemerides and Astrometry of the Solar System , 1996 , pp. 427 - 430
Copyright
Copyright © Kluwer 1996 

References

Pascu, D. (1980). “Methods of astrometric observations of natural satellites.” In Planetary satellites (Burns, J.A., ed.) Mir, Moscow, p.71–105.Google Scholar
Kisselev, A.A. (1989). The theoretical foundations of the photographic- astrometry Nauka, Moscow.Google Scholar
Arlot, J.-E. (1982). “New constants for Sampson-Lieske Theory of the Galilean Satellites of Jupiter.” Astron. and Astrophys. 107, 305.Google Scholar