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Astrometry by asteroid occultations

Published online by Cambridge University Press:  25 May 2016

L. Kahl Kristensen
L. Kahl Kristensen*
Affiliation:
Institute of Physics and Astronomy University of Aarhus, DK-8000 Aarhus, Denmark

Abstract

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For the determination of the dynamical equinox in fundamental star catalogues observed by astrometric satellites it is proposed to observe occultations of stars by selected asteroids. Being a long term programme now is the time for planning. Quadrature observations and photometric back-up are essential.

Type
Part X - Solar System Astrometry
Information
Symposium - International Astronomical Union , Volume 172: Dynamics, Ephemerides and Astrometry of the Solar System , 1996 , pp. 443 - 446
Copyright
Copyright © Kluwer 1996 

References

Brouwer, D.: 1935, Astron. Journ. 44, 57–63.Google Scholar
Dyson, F.: 1929, Trans. I.A.U. 3, 227.Google Scholar
Kristensen, L.K.: 1980, Mitt. d. Astron. Ges. 48, 50–55.Google Scholar
Kristensen, L.K.: 1981, Astron. Astrophys. Suppl. Ser. 44, 375.Google Scholar
Newcomb, S.: 1878, Motion of the Moon. Washington Observations for 1875. Washington, Appendix II.Google Scholar
Numerov, M.B.: 1932, Bull. l'Inst. Astron. (Leningrad) 32, 139–147.Google Scholar
Strömgren, B.: 1950, Trans. I.A.U. 7, 220.Google Scholar