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Gravity field determination for Mars ObserverMars Observer will be the first near circular, low altitude and short-periodic orbiter of Mars. From previous Mars orbiters, such as Mariner 9 and Vikings 1 and 2, a large gravitational oblateness and in general a gravity field ten times stronger than the earth's field have been determined. Because of these, the gravity field will dominate the evolution of the spacecraft's orbital motion and is the principal error source for reconstructing the spacecraft's motion. Thus a gravity calibration (GC) period has been established prior to the mapping phase in order to refine the gravitational field model. This paper describes the plan being made by Navigation to implement the GC strategy. By analyzing simulated Doppler data acquired during the seven day GC period, we give (1) the expected improvement in the gravity field model and (2) the resulting improvement in reconstructed spacecraft orbital motion. In addition, we have developed a strategy for converging the GC gravity model.
Document ID
19900065967
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Esposito, Pasquale B.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Demcak, Stuart
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Roth, Duane
(JPL Pasadena, CA, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1990
Subject Category
Space Communications, Spacecraft Communications, Command And Tracking
Report/Patent Number
AIAA PAPER 90-2945
Report Number: AIAA PAPER 90-2945
Meeting Information
Meeting: AIAA/AAS Astrodynamics Conference
Location: Portland, OR
Country: United States
Start Date: August 20, 1990
End Date: August 22, 1990
Accession Number
90A53022
Distribution Limits
Public
Copyright
Other

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