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The mass of PhobosRadio tracking data associated with the February 1977 encounters between the Martian satellite Phobos and the Viking Orbiter I spacecraft have been analyzed to determine the gravitational constant of Phobos. A linear error analysis was conducted to determine the selection of data and the parameter solution set which would yield the best estimate of the gravitational constant. This error analysis indicated that the optimal data set was a data arc beginning just prior to the closest encounter and spanning three consecutive spacecraft orbits; data near periapsis were deleted. The most feasible parameter solution set consisted of the Phobos gravitational constant and the spacecraft initial conditions. The result of the data analysis was an estimate of (7.3 plus or minus 0.7) x 10 to the -4th cu km/sq sec for the gravitational constant of Phobos.
Document ID
19780034967
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Tolson, R. H.
(NASA Langley Research Center Hampton, VA, United States)
Blackshear, W. T.
(NASA Langley Research Center Hampton, VA, United States)
Mason, M. L.
(NASA Langley Research Center Atmospheric Environmental Sciences Div., Hampton, Va., United States)
Kelly, G. M.
(Analytical Mechanics Associates, Inc. Hampton, Va., United States)
Date Acquired
August 9, 2013
Publication Date
December 1, 1977
Publication Information
Publication: Geophysical Research Letters
Volume: 4
Subject Category
Lunar And Planetary Exploration
Accession Number
78A18876
Distribution Limits
Public
Copyright
Other

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