Hostname: page-component-848d4c4894-r5zm4 Total loading time: 0 Render date: 2024-06-27T13:05:03.562Z Has data issue: false hasContentIssue false

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: nedelcu@aira.astro.ro, petre@aira.astro.ro, paras@aira.astro.ro, octavian@aira.astro.ro
J. Souchay
Affiliation:
SYRTE Observatoire de Paris, 61, avenue de l'Observatoire 75014, Paris, France email: jean.souchay@obspm.fr
M. Birlan
Affiliation:
IMCCE Observatoire de Paris, 61, avenue de l'Observatoire 75014, Paris, France email: mirel.birlan@obspm.fr
P. P. Popescu
Affiliation:
Astronomical Institute of the Romanian Academy, Cutitul de Argint 5, RO-040557, Bucharest, Romania email: nedelcu@aira.astro.ro, petre@aira.astro.ro, paras@aira.astro.ro, octavian@aira.astro.ro
P. V. Paraschiv
Affiliation:
Astronomical Institute of the Romanian Academy, Cutitul de Argint 5, RO-040557, Bucharest, Romania email: nedelcu@aira.astro.ro, petre@aira.astro.ro, paras@aira.astro.ro, octavian@aira.astro.ro
O. Badescu
Affiliation:
Astronomical Institute of the Romanian Academy, Cutitul de Argint 5, RO-040557, Bucharest, Romania email: nedelcu@aira.astro.ro, petre@aira.astro.ro, paras@aira.astro.ro, octavian@aira.astro.ro
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Andrei, A. H., Fienga, A., Assafin, M., Penna, J. L., da Silva Neto, D. N., & Vieira Martins, R. 2004, Journées 2004 - systèmes de reférénce spatio-temporels., p. 228Google Scholar
Assafin, M., Nedelcu, D. A., Badescu, O., Popescu, P., Andrei, A. H., Camargo, J. I. B., da Silva Neto, D. N., & Vieira Martins, R. 2007, A&A, in pressGoogle Scholar
Bowell, E., Muinonen, K., & Wasserman, L. H. 1994, Asteroids, comets, meteors 1993, p. 477CrossRefGoogle Scholar
Vèron-Cetty, M.-P. & Vèron, P. 2006, A&A, 455, 733Google Scholar