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Mars sample return by orbital rendezvousThe return of Mars surface samples by the orbital rendezvous mode would require smaller, lighter vehicles than the direct return mode and would limit the exposure of the earth return systems to possible contamination by Martian biota. The reference mission considered would use a single Titan IIIE/Centaur launch vehicle, carry a 1 kg sample, and be launched in late 1981. The spacecraft would consist of an orbiter, a Mars lander, a Mars ascent vehicle, an earth return vehicle, and an earth entry capsule. The Mars ascent vehicle is the only all-new vehicle required, the others being derived from Viking and other programs. A key consideration is the feasibility of automatic rendezvous and sample transfer between the ascent vehicle and orbiter in Mars orbit. The maneuvers required and the maneuver algorithm developed in a NASA feasibility study are described in detail. The possibility of international cooperation on a Mars orbital rendezvous mission is discussed.
Document ID
19750032551
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Moore, J. W.
(California Institute of Technology, Jet Propulsion Laboratory, Advanced Technical Studies Office, Pasadena Calif., United States)
Scofield, W. T.
(Martin Marietta Aerospace Denver, Colo., United States)
Date Acquired
August 8, 2013
Publication Date
January 1, 1975
Publication Information
Publication: Astronautics and Aeronautics
Volume: 13
Subject Category
Lunar And Planetary Exploration
Accession Number
75A16623
Distribution Limits
Public
Copyright
Other

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