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The mass, gravity field, and ephemeris of MercuryIn the present gravity analysis of Mariner 10/Deep Space Network radio Doppler and range data for Mercury encounters in March 1974 and March 1975, a combined least-squares fit to the Doppler data has determined two second-degree gravity harmonics that are referred to a 2439-km equatorial radius. It is noted that the 1-sigma error limits on the gravity results encompass the possibility that harmonics other than J2 and C22 significantly differ from zero. The Deep Space Network radio range data obtained with Mariner 10 are primarily applicable to such improvements of Mercury's ephemeris as the more precise determination of perihelion precession.
Document ID
19880026537
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Anderson, John D.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Esposito, Pasquale B.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Lau, Eunice L.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Trager, Gayle B.
(California Institute of Technology Jet Propulsion Laboratory, Pasadena, United States)
Colombo, Giuseppe
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
August 13, 2013
Publication Date
September 1, 1987
Publication Information
Publication: Icarus
Volume: 71
ISSN: 0019-1035
Subject Category
Lunar And Planetary Exploration
Accession Number
88A13764
Distribution Limits
Public
Copyright
Other

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