Mars 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.
Gravity field determination for Mars Observer
AIAA/AAS Astrodynamics Conference ; 1990 ; Portland, OR, United States
1990-01-01
Conference paper
No indication
English
Mars Observer orbit determination analysis
NTRS | 1991
|Mars Observer orbit determination analysis
AIAA | 1991
|NTRS | 1991
|NTIS | 1991
|TIBKAT | 1985
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