Connecting the dynamical frame to the ICRF by use NEAs observations

Details Connecting the dynamical frame to the ICRF by use NEAs observations Connecting the dynamical frame to the ICRF by use NEAs observations

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008jsrs.meet...50y&link_type=abstract

"Proceedings of the "Journées Systèmes de Référence Spatio-temporels 2007". Observatoire de Paris, 17-19 September 2007. Editor:

Mathematics

Dynamical Systems

Scientific paper

ICRF (practical realization of ICRS) is now adopted as the fundamental celestial frame in astronomy. The Hipparcos catalogue is a primary realization of the ICRF at optical wavelengths. In spite of the fact that the ICRF is a quasi-inertial system there are a great number of problems associated with the use of the ICRF, the main of them being the connection of ICRF to dynamical systems. The parameters of this connection are known with insufficient accuracy and further work is necessary on the problem of mutual orientation of this systems at new level of accuracy using different new observations of different solar system objects.

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