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Asteroid astrometry as a link between ICRF and the Dynamical Reference Frames

Published online by Cambridge University Press:  01 October 2007

D. A. Nedelcu
Affiliation:
Astronomical Institute of the Romanian Academy, Cutitul de Argint 5, RO-040557, Bucharest, Romania email: [email protected], [email protected], [email protected], [email protected]
J. Souchay
Affiliation:
SYRTE Observatoire de Paris, 61, avenue de l'Observatoire 75014, Paris, France email: [email protected]
M. Birlan
Affiliation:
IMCCE Observatoire de Paris, 61, avenue de l'Observatoire 75014, Paris, France email: [email protected]
P. P. Popescu
Affiliation:
Astronomical Institute of the Romanian Academy, Cutitul de Argint 5, RO-040557, Bucharest, Romania email: [email protected], [email protected], [email protected], [email protected]
P. V. Paraschiv
Affiliation:
Astronomical Institute of the Romanian Academy, Cutitul de Argint 5, RO-040557, Bucharest, Romania email: [email protected], [email protected], [email protected], [email protected]
O. Badescu
Affiliation:
Astronomical Institute of the Romanian Academy, Cutitul de Argint 5, RO-040557, Bucharest, Romania email: [email protected], [email protected], [email protected], [email protected]
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Abstract

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Highly accurate astrometry of asteroids in the frame of QSOs will provide the direct link between the Dynamical Reference Frame and the International Celestial Reference Frame. We propose a procedure that implies a selection of events for asteroids with accurately determined orbits crossing the CCD field containing the selected quasars. For asteroid ephemerides, a numerical integration method coupled with precise modelling of asteroid brightness will be used for analyzing our observations. A list of predictions for this type of “close approaches” will be presented.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2008

References

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