Abstract
International programs of observations of selected minor planets have lasted about 50 years and the last one comes to the end in 2000. The main aim of these observational programs consists in obtaining the orientation of the stellar reference frame with respect to the dynamical one using observations of the bright minor planets. The observations are also useful for the orbital improvements of the asteroids themselves. They are available from the author via e-mail at the address <cya@quasar.ipa.nw.ru>.
During the above mentioned period more than 23 000 observations of minor planets, referred to different reference star catalogues, have been obtained. The reduction procedure of observations to the PPM star catalogue is described. The orientation parameters are given and discussed.
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References
Batrakov, Yu. V. and Shor, V. A.: 1989, ‘On the programme of ground-based observations of bright selected minor planets for 1991-2000’, In: J. H. Lieske and V. K. Abalakin (eds), Inertial Coordinate System on the Sky pp. 69-71.
Batrakov, Yu. V., Chernetenko, Yu. A., Gorel', G. K. and Gudkova, L. A.: 1999, ‘Hipparcos catalogue orientation as obtained from observations of minor planets’, Astron. Astrophys. 352, 703–711.
Brouwer, D.: 1935, ‘On the determination of systematic correction to stars position from observations of minor planets’, Astron. J. 44, 57–63.
Dyson, F.W.: 1928, ‘Usefulness of minor planets for checking the equator point’, Trans. IAU 3, 227.
ESA.: 1997, The Hipparcos and Tycho Catalogues, ESA SP-1200.
Folkner, W.M., Charlot, P., Finger,M. H., Williams, J. G., Sovers, O. J., Newhall, X. X. and Stand ish, E. M.: 1994, ‘Determination of the extragalactic-planetary frame tie from joint analysis of radio interferometric and lunar laser ranging measurements’, Astron. Astrophys. 287, 279–289.
Makarova, E. N.: 1999, ‘Catalogue of photographic observations of selected minor planets’, In: Astrometry, Geodynamics and Celestial Mechanics, Trudy IPA, 4, 128–134 (in Russian).
Mignard, F. and Froeschle, M.: 1997, Comparison of the FK5 frame to Hipparcos. In: 'Hipparcos-Venice 97',Venice, Italy May 13-16. ESA SP-402, 57–60.
Newcomb, S.: 1895, The Elements of the Four Inner Planets and the Fundamental Constants of Astronomy. Washington, Government Printing Office. p. 202.
Numerov, B. V.: 1933, On the problem of determination of systematic errors of declination of fundamental stars. Bull. Astron. Inst. 32, 139–147 (in Russian).
Numerov, B. V.: 1935, On the question of simultaneous determination of corrections to elements of the planets and the Earth. Astron. Zh XII 6, 584–593 (in Russian).
Orelskaya, V. I.: 1981, Improvement of the FK4 zero-points using photographic observations of asteroids. In: Astrometric Researches. Kiev. Naukova dumka. 48–53 (in Russian).
Pierce, D. A.: 1971, Star catalogue corrections-determined from photographic observations of selected minor planets. Astron. J. 76, 177–181.
Podobed, V. V.: 1962, Fundamental Astrometry. Moskau. p. 273 (in Russian).
Stand ish, E. M.: 2000, Private communication.
Yagudina, E. I.: 2000, Usage of radar and optical observations of Near-Earth Asteroids and main belt minor planets for astrometry (this issue).
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Chernetenko, Y.A. International program of observations of selected minor planets: first results. Celestial Mechanics and Dynamical Astronomy 80, 185–194 (2001). https://doi.org/10.1023/A:1012031821629
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DOI: https://doi.org/10.1023/A:1012031821629