Passive decay heat removal enhances the safety of a nuclear propelled spacecraft and could increase its Isp by up to 4 percent. The large height‐to‐diameter ratio (≳1.5) of the PeBR provides an effective means for passive removal of decay heat from the reactor core after firing. A multi‐dimensional transient heat conduction/radiation model of the PeBR core and surrounding structures is developed to investigate the potential for passive decay heat removal. The effective conductance of the core region includes both conduction and radiation contributions and the thermophysical properties of the fuel and core structure materials are taken to be temperature dependent. Results indicate that passive decay heat removal, following a short period of active cooling (600–1000 seconds), would maintain the PeBR core safely coolable with the peak fuel temperature well below 3400 K.
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15 January 1992
Proceedings of the ninth symposium on space nuclear power systems
12−16 Jan 1992
Albuquerque, New Mexico (USA)
Research Article|
January 15 1992
Passive decay heat removal in the PeBR concept for nuclear thermal propulsion Available to Purchase
Nicholas J. Morley;
Nicholas J. Morley
Institute for Space Nuclear Power Studies, Chemical and Nuclear Engineering Department, The University of New Mexico, Albuquerque, New Mexico 87131
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Mohamed S. El‐Genk
Mohamed S. El‐Genk
Institute for Space Nuclear Power Studies, Chemical and Nuclear Engineering Department, The University of New Mexico, Albuquerque, New Mexico 87131
Search for other works by this author on:
Nicholas J. Morley
Institute for Space Nuclear Power Studies, Chemical and Nuclear Engineering Department, The University of New Mexico, Albuquerque, New Mexico 87131
Mohamed S. El‐Genk
Institute for Space Nuclear Power Studies, Chemical and Nuclear Engineering Department, The University of New Mexico, Albuquerque, New Mexico 87131
AIP Conf. Proc. 246, 955–966 (1992)
Citation
Nicholas J. Morley, Mohamed S. El‐Genk; Passive decay heat removal in the PeBR concept for nuclear thermal propulsion. AIP Conf. Proc. 15 January 1992; 246 (1): 955–966. https://doi.org/10.1063/1.41854
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