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Experimental determination of Mercury's mass and oblatenessThe ratio of the mass of the sun to that of Mercury deduced from the first and third flybys of Mercury by Mariner 10 is 6,023,600 plus or minus 600 and 6,023,700 plus or minus 300, respectively. Additional analysis should improve these uncertainties by a factor of 2 to 5. Assuming an equatorial radius of 2439 km, the mean density of the planet is 5.44 g/cu cm. The gravitational oblateness deduced from the first encounter is discussed. Data received from the third encounter are better suited for this determination and yield J2 of 0.00008 plus or minus 0.00006. In addition, the third-encounter data are sensitive to local gravity effects or anomalies.
Document ID
19770038123
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Esposito, P. B.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Anderson, J. D.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Ng, A. T. Y.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Date Acquired
August 9, 2013
Publication Date
June 1, 1976
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Plenary Meeting
Location: Philadelphia, PA
Start Date: June 8, 1976
End Date: June 19, 1976
Sponsors: COSPAR
Accession Number
77A20975
Funding Number(s)
CONTRACT_GRANT: NAS7-100
Distribution Limits
Public
Copyright
Other

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