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Microreactor System Design for a NASA In Situ Propellant Production Plant on MarsThe NASA In Situ Resource Utilization (ISRU) program is planning near-term missions to Mars that will include chemical processes for converting the carbon dioxide (CO2) and possibly water from the Martian environment to propellants, oxygen, and other useful chemicals. The use of indigenous resources reduces the size and weight of the payloads from Earth significantly, representing enormous cost savings that make human exploration of Mars affordable. Extraterrestrial chemical processing plants will need to be compact, lightweight, highly efficient under reduced gravity, and extraordinarily reliable for long periods. Microchemical and thermal systems represent capability for dramatic reduction in size and weight, while offering high reliability through massive parallelization. In situ propellant production (ISPP), one aspect of the ISRU program, involves collecting and pressurizing atmospheric CO2, conversion reactions, chemical separations, heat exchangers, and cryogenic storage. A preliminary system design of an ISPP plant based on microtechnology has demonstrated significant size, weight, and energy efficiency gains over the current NASA baseline. Energy management is a strong driver for Mars-based processes, not only because energy is a scarce resource, but because heat rejection is problematic; the low pressure environment makes convective heat transfer ineffective. Energy efficiency gains are largely achieved in the microchemical plant through extensive heat recuperation and energy cascading, which has a small size and weight penalty because the added micro heat exchangers are small. This leads to additional size and weight gains by reducing the required area of waste heat radiators. The microtechnology-based ISPP plant is described in detail, including aspects of pinch analysis for optimizing the heat exchanger network. Three options for thermochemical compression Of CO2 from the Martian atmosphere, adsorption, absorption, and cryogenic freezing, are presented, as well as three options for water decomposition, low temperature electrolysis, high temperature electrolysis, and thermochemical decomposition. Other elements of the plant include Sabatier and reverse water gas shift reactors, water recovery, chemical separations, and cryogenic storage. Data are presented supporting preliminary sizing of components, and results of the system design are compared to the existing NASA baseline that is based on conventional technologies.
Document ID
20000110563
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
TeGrotenhuis, W. E.
(NASA Johnson Space Center Houston, TX United States)
Wegeng, R. S.
(NASA Johnson Space Center Houston, TX United States)
Vanderwiel, D. P.
(Pacific Northwest National Lab. Richland, WA United States)
Whyatt, G. A.
(Pacific Northwest National Lab. Richland, WA United States)
Viswanathan, V. V.
(Pacific Northwest National Lab. Richland, WA United States)
Schielke, K. P.
(Pacific Northwest National Lab. Richland, WA United States)
Sanders, G. B.
(Pacific Northwest National Lab. Richland, WA United States)
Peters, T. A.
(NASA Johnson Space Center Houston, TX United States)
Nicholson, Leonard S.
Date Acquired
August 19, 2013
Publication Date
January 1, 2000
Subject Category
Propellants And Fuels
Meeting Information
Meeting: 4th International Conferenc eon Microreaction Technology
Location: Atlanta, GA
Country: United States
Start Date: March 5, 2000
End Date: March 9, 2000
Sponsors: Dechema-Inst., American Inst. of Chemical Engineers, Battelle
Funding Number(s)
PROJECT: RTOP 953-20-632-70
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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