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Inertial Frame Determination from Hipparcos Observations of Minor Planets

Published online by Cambridge University Press:  07 August 2017

D. Hestroffer*
Affiliation:
Bureau des longitudes 77 Avenue Denfert Rochereau 75014 Paris France

Abstract

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Observations of 48 minor planets by Hipparcos should lead to a good determination of the inertial reference frame. Analysis of one year observations showed periodic effects in the o-c due to a rotation between the Hipparcos system and the inertial system. By extending this result to a 2.5 years simulation and by studying the impact of added ground-based observations, it appears that the orbital elements of the Earth and the parameters of a rotation of the system can be obtained with an accuracy better than 5 mas.

Type
Space Optical Astrometry
Copyright
Copyright © Kluwer 

References

Bec-Borsenberger, A.:1990 Astron. Astrophys. Sup. Ser. 86, 299349 Google Scholar
Bretagnon, P.:1982 Astron. Astrophys. 114, 278288 Google Scholar
Morando, B., Lindegren, L.:1989 ESA SP-1111, 3, 269281 Google Scholar
Numerov, B.V.:1936 Astron. J 45, 105111 CrossRefGoogle Scholar
Söderhjelm, S., Lindegren, L.:1982 Astron. Astrophys. 110,156162 Google Scholar