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GalileoThe purpose of the Galileo missions is to make observations of Jupiter and its satellites using an orbiting spacecraft and an atmospheric entry probe. The mission will determine the chemical composition and physical state of the Jovian atmosphere and its satellites, and the topology and behavior of the magnetic field and energetic particle flux of Jupiter. The mission plan calls for a Venus Earth Earth Gravity Assist (VEEGA) trajectory having a launch to end of mission duration of approximately 8 years. The Galileo spacecraft was placed in Earth orbit by the Space Transportation System (STS) on October 18, 1989. The Inertial Upper Stage (IUS) placed the spacecraft on a trajectory to encounter Venus on February 10, 1990. Information is given in tabular form for coverage goals, Deep Space Network (DSN) support, frequency assignments, telemetry, command, and tracking support responsibility.
Document ID
19920003881
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Ausman, N. E.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Oneil, W. J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
September 6, 2013
Publication Date
October 1, 1991
Publication Information
Publication: JPL, California Inst. of Tech., Deep Space Network: Mission Support Requirements
Subject Category
Astronautics (General)
Accession Number
92N13099
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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