Abstract
Nuclear thermal propulsion (NTP) is an in-space propulsion technology capable of both high specific impulse (850–1000 s) and thrust (44–1112 kN), which can help reduce trip times for crewed missions beyond low Earth orbit. NTP technology has been demonstrated during historic programs. Over 20 ground test reactor experiments were performed, which demonstrated the prototypic reactor operations, during the Nuclear Engine for Rocket Vehicle Application (NERVA)/Rover program (1955–1972). Although historical programs have shown that NTP is a viable in-space propulsion technology, developing NTP in modern programs is contingent on the development and qualification of ultrahigh-temperature nuclear fuel technologies that can withstand engine operating conditions. In historical NTP development programs such as NERVA/Rover, prototypic reactor/engine schemes were ground tested to assess the overall system feasibility and to qualify the reactor fuel forms for eventual flight systems. Although this approach is effective to verify fuel performance under prototypic conditions, relying solely on full-scale NTP reactor tests as the pathway for verifying or qualifying fuel is inefficient and cost prohibitive today. Additionally, modern nuclear licensing requirements state that before test reactor approval, reactor components and fuel elements should be qualified via non-nuclear (out-of-pile) and nuclear (in-pile) testing under representative operating conditions. Using this methodology, fuel matures as production scale fabrication methods are established, and as produced fuel performance is demonstrated. This paper provides an overview of historical approaches to NTP fuel performance maturation, including fuel screening and qualification needs, and provides insight for establishing an efficient testing paradigm that can be implemented to rapidly and affordably develop NTP fuel forms for eventual qualification.
Original language | English |
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Article number | 110765 |
Journal | Nuclear Engineering and Design |
Volume | 367 |
DOIs | |
State | Published - Oct 2020 |
Funding
Notice: This manuscript has been authored by UT-Battelle, LLC, under contract DE-AC05-00OR22725 with the US Department of Energy (DOE). The US government retains and the publisher, by accepting the article for publication, acknowledges that the US government retains a nonexclusive, paid-up, irrevocable, worldwide license to publish or reproduce the published form of this manuscript, or allow others to do so, for US government purposes. DOE will provide public access to these results of federally sponsored research in accordance with the DOE Public Access Plan ( http://energy.gov/downloads/doe-public-access-plan ). Dr. Palomares was funded in part by a NASA Space Technology Research Fellowship [grant number NNX15AQ35H ] provided by the University of Tennessee Knoxville (UTK). Dr. Howard and Mr. Steiner were funded through the Oak Ridge National Laboratory (ORNL) executed, Department of Energy managed, and NASA funded NTP project [contract number DE-AC05-00OR22725]. The authors wish to acknowledge the contributions of Dr. L. Heilbronn (UTK) and Dr. T. J. Harrison (ORNL/UTK). The findings and conclusions expressed in this paper are opinion of the authors’ and not representative of ongoing NTP fuel development efforts.
Funders | Funder number |
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U.S. Department of Energy | |
National Aeronautics and Space Administration | NNX15AQ35H |
Oak Ridge National Laboratory | DE-AC05-00OR22725 |
University of Tennessee, Knoxville |