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GAIA and beyond: The perspective from the milliarcseconds of Hubble and HipparcosAstrometry with the Hubble space telescope and Hipparcos satellite advanced the optical astrometric accuracies to the milliarcsec level. The global astrometric interferometer for astrophysics (GAIA) satellite and other proposed optical interferometry space missions would advance the optical astrometric accuracy to better than 10 microarcsec. A catalog figure of merit is defined which allows a quantitative comparison to be carried out for astrometric catalogs. Using two specific astrophysical problems, the level of the expected scientific contribution from a GAIA-type mission is assessed. The two problems are: the age of the globular clusters in relation to the age of the Universe, and the initial mass function compared with fluctuations in the star formation rate with time.
Document ID
19960012025
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Hemenway, Paul D.
(Texas Univ. Austin, TX, United States)
Date Acquired
August 17, 2013
Publication Date
September 1, 1995
Publication Information
Publication: ESA, Future Possibilities for Astrometry in Space
Subject Category
Astrophysics
Accession Number
96N18262
Funding Number(s)
CONTRACT_GRANT: NAGW-3111
Distribution Limits
Public
Copyright
Other

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