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Sensitivity of Lunar Resource Economic Model to Lunar Ice ConcentrationLunar Prospector mission data indicates sufficient concentration of hydrogen (presumed to be in the form of water ice) to form the basis for lunar in-situ mining activities to provide a source of propellant for near-Earth and solar system transport missions. A model being developed by JPL, Colorado School of Mines, and CSP, Inc. generates the necessary conditions under which a commercial enterprise could earn a sufficient rate of return to develop and operate a LEO propellant service for government and commercial customers. A combination of Lunar-derived propellants, L-1 staging, and orbital fuel depots could make commercial LEO/GEO development, inter-planetary missions and the human exploration and development of space more energy, cost, and mass efficient.
Document ID
20020074657
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
Authors
Blair, Brad
(Colorado School of Mines Golden, CO United States)
Diaz, Javier
(Colorado School of Mines Golden, CO United States)
Date Acquired
August 20, 2013
Publication Date
January 1, 2002
Publication Information
Publication: The Moon Beyond 2002: Next Steps in Lunar Science and Exploration
Subject Category
Lunar And Planetary Science And Exploration
Funding Number(s)
CONTRACT_GRANT: JPL-1237006
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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