Hostname: page-component-586b7cd67f-dlnhk Total loading time: 0 Render date: 2024-11-27T10:45:06.308Z Has data issue: false hasContentIssue false

The Stellar Reference Frame from Space Observations

Published online by Cambridge University Press:  12 April 2016

C. A. Murray*
Affiliation:
Royal Greenwich Observatory

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.

The HIPPARCOS Satellite, to be launched by the European Space Agency, will provide a stellar reference frame over the whole celestial sphere with an average accuracy of ± 0002 in each coordinate and component of annual proper motion, for some 100,000 stars.

The origin of coordinates will be arbitrary. Absolute rotation of the system of proper motions can be obtained by measuring quasars relative to stars in the HIPPARCOS catalogue, either with the NASA Space Telescope or by conventional ground based astrometric observations.

Type
Research Article
Copyright
Copyright © Reidel 1981

References

European Space Agency 1979a HIPPARCOS. Space Astrormetry. Report on Phase A Study (SC1(79)10)Google Scholar
European Space Agency 1979b HIPPARCOS. Spacecraft design and development (PF 616)Google Scholar
van Altena, W. F. 1979 IAU Colloquium No 48. “Modern Astrometry” (eds. Prochazka, F. V. and Tucker, R. H., Vienna, ), pp.561571 Google Scholar