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Propellant production from the Martian atmosphereResults are presented from a calculation of the specific impulses that can be generated through the combustion of cryogenic CO and O2 over a range of fuel/oxidizer ratios, chamber pressures, nozzle expansion ratios, freestream pressures representative of Mars, and the limiting conditions of equilibrium and frozen nozzle flow. For an expansion ratio of 80 and 100-atm. chamber pressure, a specific impulse of 298 sec was obtained; this is comparable to the best solid rocket propellants.
Document ID
19920061903
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Bowles, J. V.
(NASA Ames Research Center Moffett Field, CA, United States)
Tauber, M. E.
(NASA Ames Research Center Moffett Field, CA, United States)
Anagnost, A. J.
(Stanford University CA, United States)
Whittaker, T.
(Sterling Software, Inc. Palo Alto, CA, United States)
Date Acquired
August 15, 2013
Publication Date
August 1, 1992
Publication Information
Publication: Journal of Propulsion and Power
Volume: 8
Issue: 4, Ju
ISSN: 0748-4658
Subject Category
Propellants And Fuels
Accession Number
92A44527
Distribution Limits
Public
Copyright
Other

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