A Fizeau optical interferometer astrometric satelliteThe proposed design and construction of the Fizeau astrometric mapping explorer (FAME), a small astrometric instrument for use on an artificial satellite, is reported on. The instrument and spacecraft are designed to slowly spin and will repeatedly scan great circles on the sky so that, over a period of time, it will cover the complete sky and repeat in a manner similar to that of the Hipparcos satellite. The instrument will use the two fixed dilute aperture telescopes to measure a fixed angle between stars and detect the positions, magnitude and color of all stars crossing its field of view to a visual magnitude of approximately 15 mag. The aim of the instrument is to obtain a catalog of positions, proper motions and parallaxes of all stars down to about 15 mag, with a magnitude dependent accuracy of positions of 20 to 800 micro arcsec, proper motions of 20 to 800 micro arcsec per year and parallaxes of 20 to 800 micro arcsec.
Document ID
19960012032
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Seidelmann, P. Kenneth (Naval Observatory Washington, DC., United States)
Johnston, K. J. (Naval Observatory Washington, DC., United States)
Urban, S. (Naval Observatory Washington, DC., United States)
Germain, M. (Naval Observatory Washington, DC., United States)
Corbin, T. (Naval Observatory Washington, DC., United States)
Shao, M. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Yu, J. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Fanson, J. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Rickard, L. J. (Naval Research Lab. Washington, DC., United States)
Weiler, K. (Naval Research Lab. Washington, DC., United States)
Date Acquired
August 17, 2013
Publication Date
September 1, 1995
Publication Information
Publication: ESA, Future Possibilities for Astrometry in Space