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Mars Observer orbital accuracy analysisAttention is given to the orbital accuracy of the Mars Observer (MO) spacecraft throughout its 687 days of mapping (scheduled to commence in 1991). The MO's short period and near circular orbit necessitate a multiorbit analysis in which the spacecraft's motion is strongly perturbed by the local and global gravity field of Mars. This analysis attests to the feasibility of achieving an orbital position accuracy at the level of 2-3 km within the data interval. It is found that Very Long Baseline Interferometric data can rectify a situation in which the position accuracy degrades significantly.
Document ID
19860063211
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Esposito, P. B.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Demcak, S.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Santee, M. L.
(California Institute of Technology Jet Propulsion Laboratory, Pasadena, United States)
Date Acquired
August 12, 2013
Publication Date
August 1, 1986
Subject Category
Astrodynamics
Report/Patent Number
AIAA PAPER 86-2057
Report Number: AIAA PAPER 86-2057
Accession Number
86A47949
Distribution Limits
Public
Copyright
Other

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