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Determination of Position of Jupiter From Very-Long Baseline Interferometry Observations of UlyssesVery-long baseline interferometry (VLBI) observations of the Ulysses spacecraft near its encounter with Jupiter on 1992 February 8 were made to determine the angular position of Jupiter with respect to well known extragalactic radio sources. Spacecraft range and Doppler data were used to determine the position of the spacecraft with respect to Jupiter. Thirty-one VLBI observations of the spacecraft were made within 30 days of Ulysses closest approach to Jupiter, using the California-Spain and California-Australia baselines of NASA's Deep Space Network. When combined, these data determine the position of Jupiter at the time of encounter with an accuracy of 0.003 min in right ascension and 0.005 sec in declination. In addition, the Earth-Jupiter distance was determined with 20 m accuracy.
Document ID
19990019471
Acquisition Source
Headquarters
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Folkner, W. M.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
McElrath, T. P.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Mannucci, A. J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Date Acquired
August 19, 2013
Publication Date
September 1, 1996
Publication Information
Publication: Astronomical Journal
Publisher: American Astronautical Society
Volume: 112
Issue: 3
ISSN: 0004-6256
Subject Category
Astronomy
Distribution Limits
Public
Copyright
Other

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