Both nuclear electric propulsion (NEP) and nuclear thermal propulsion (NTP) systems show great potential to facilitate the human exploration of Mars with significant advantages relative to chemical propulsion. The two systems, however, have very different heritages. The development of high-power NTP systems benefits from the robust ground-based testing of many NTP reactors during the Rover/Nuclear Engine for Rocket Vehicle Application (NERVA) programs, but NTP systems require reactor operating temperatures about 1500 K higher than NEP systems. NASA, the Department of Energy (DOE), and the Department of Defense (DoD) are currently supporting substantive NTP research and development programs. Even so, an NTP system has never flown in space. In contrast, advanced electric propulsion technologies are deployed routinely in operational spacecraft. Such systems have demonstrated long life and high reliability, but only at power levels far below those needed for a megawatt electric-class system, and only in a solar-powered mode. Over the past decade, there has been very little advancement in NEP technology at the scale and power-level required for the baseline mission. Given this imbalance in technology maturity, system trades are difficult to make.
NTP systems and NEP systems (which include a chemical propulsion system) are composed of many technologies, including the following:
For those technologies that are used in both NEP and NTP systems, the engineering challenges are very different because of different operating temperatures, operational lifetimes, startup regimens, and requirements for integration with other system elements. For example, while both concepts use a nuclear reactor, as shown in Table 1.3, the operational requirements and design specifications for an NTP reactor are very different than those for an NEP reactor. As a result, different approaches may be needed to address some safety assurance requirements (see the discussion of safety assurance, below). Similarly, propellant storage temperature requirements greatly vary: 20 K for LH2 (NTP), 110 K for LOX (NEP), 90 K for liquid methane (NEP), and supercritical storage of xenon (NEP). The propellant mass of an NTP system will far exceed the propellant mass for the electric thrusters in an NEP system; the latter, however, will need to store a sizeable mass of propellant for its ancillary chemical propulsion system. System complexity is another consideration. NTP systems have a smaller number of subsystems to integrate, whereas the nature of NEP enables initial subsystem separability for ground testing.
Given the above circumstances, meaningful and objective trade studies will require expertise in all the above technologies as they apply to NTP and NEP systems scaled to meet the needs of the baseline mission.
FINDING. Trade Studies. Recent, apples-to-apples trade studies comparing NEP and NTP systems for a crewed mission to Mars in general and the baseline mission in particular do not exist.
RECOMMENDATION. Trade Studies. NASA should develop consistent figures of merit and technical expertise to allow for an objective comparison of the ability of nuclear electric propulsion and nuclear thermal propulsion systems to meet requirements for a 2039 launch of the baseline mission.
Despite the many differences between NEP and NTP systems and subsystems, there are some areas of synergy, including the following:
FINDING. NEP and NTP Commonalities. NEP and NTP systems require, albeit to different levels, significant maturation in areas such as nuclear reactor fuels, materials, and additional reactor technologies; cryogenic fluid management; M&S; testing; safety; and regulatory approvals. Given these commonalities, some development work in these areas can proceed independently of the selection of a particular space nuclear propulsion system.
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1 An NTP or NEP reactor only builds up appreciable fission products when operated at power for a period of time.
2 A.C. Marshall, et al., “Nuclear Safety Policy Working Group Recommendations on Nuclear Propulsion Safety for the Space Exploration Initiative,” NASA Technical Memorandum 105705, Final Report of the Joint NASA/DOE/DoD Nuclear Safety Policy Working Group, National Aeronautics and Space Administration, April 1993.
3 J.A. Sholtis, Jr., “Proposed Safety Functional Guidelines for Space Reactors,” Proceedings of the ANS Embedded Topical Meeting - Space Nuclear Conference 2005, LaGrange Park, IL, June 2005.
4 J.A. Sholtis, Jr., et al., “U.S. Space Nuclear Safety: Past, Present, and Future,” pp. 269-303 in A Critical Review of Space Nuclear Power and Propulsion 1984-1993, American Institute of Physics Publishing, New York, NY, 1994.
5 Johns Hopkins University–Applied Physics Laboratory, Nuclear Power Assessment Study – Final Report, TSSD-23122, Chapter 4, 2015.
6 A.C. Marshall, F.E. Haskin, and V.A. Usov, Space Nuclear Safety, Krieger Publishing Company, Malabar, FL, 2008.
7 Y. Chang, “Considerations for Implementing Presidential Memorandum-20 Guidelines for Nuclear Safety Launch Authorization for Future Civil Space Missions,” Nuclear Technology, 207(6): 844-850 2021, doi:10.1080/00295450.2020.1855946.
The decision between highly enriched uranium (HEU) (in this context, uranium with an enrichment greater than 90 percent)8 and HALEU (less than 20 percent enrichment) fuel involves more than feasibility and system performance. No such comprehensive assessment that compares the fuel types head-to-head (as distinct from a standalone assessment of the feasibility of an HALEU system) for either an NTP or NEP system was available to the committee. Key factors to be included in a comparative assessment of HEU and HALEU for both systems are as follows:
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8 HEU refers to uranium enriched to the point that it contains at least 20 percent uranium-235. HEU fuels used in space nuclear propulsion and power systems would likely be enriched to greater than 90 percent uranium-235.
While there is some clarity on each of the criteria above, they are not equally important. Performance, security, and safety concerns are significantly more important than those related to the supply chain. This weighting must be considered prior to making a fuel enrichment decision.
FINDING. Enrichment of Nuclear Fuels. A comprehensive assessment of HALEU versus HEU for NTP and NEP systems that weighs the key considerations is not available. These considerations include technical feasibility and difficulty, performance, proliferation and security, safety, fuel availability, cost, schedule, and supply chain as applied to the baseline mission.
RECOMMENDATION. Enrichment of Nuclear Fuels. In the near term, NASA and the Department of Energy, with inputs from other key stakeholders, including commercial industry and academia, should conduct a comprehensive assessment of the relative merits and challenges of highly enriched uranium and high-assay, low-enriched uranium fuels for nuclear thermal propulsion and nuclear electric propulsion systems as applied to the baseline mission.
A growing number of private-sector companies are developing system concepts for space nuclear systems. These concepts include applications for orbital maneuvering, deep space exploration, and planetary surface electrical grids.
No single entity—public or private—has all the requisite expertise or facilities to develop a space nuclear propulsion system. As has been demonstrated in recent space launch initiatives, NASA can leverage private-sector expertise, interests, and investments, along with DOE and NASA facilities, to spur the development of necessary technologies.
Several engine manufacturing and launch services providers have developed or are developing LOX/LH2 engines for in-space propulsion. Many of the needed nonnuclear engine components have heritage from these product development and demonstration efforts, but additional investment is required to convert these systems for application to an NEP or NTP propulsion system.
Cryogenic fluid management, which is critical for both NEP/chemical and NTP systems, has primarily been a government-led development effort. Private-sector fuel tank and pressure vessel manufacturers exist, but the technically challenging nature of multiyear containment of cryogenic hydrogen (necessary for NTP) will require sustained government investment in the design, fabrication, and testing of these systems.
Very few private-sector entities have the capability to develop nuclear reactor fuels, cores, shields, and control systems. However, several are investing in these capabilities and can be expected to contribute directly to the design, manufacturing, and assembly of space nuclear propulsion systems.
If efforts to develop a space nuclear system are scaled up on an accelerated timeline, there may be shortfalls in the workforce needed for such systems. A significant space nuclear power development effort would benefit from concomitant efforts to enhance relevant aspects of the science, technology, engineering, and mathematics educational pipeline, particularly nuclear engineering. This pipeline faces the following three principal challenges:
Since 1961, the United States has launched 47 radioisotope power systems of eight different types in support of 30 navigational, meteorological, communications, and space science satellites, spacecraft, and planetary landers and rovers. In contrast, the United States has launched only one fission power system—the 500 We Systems for Nuclear Auxiliary Power (SNAP)-10A reactor power system was launched in 1965 as an experimental test of an NEP system concept. At least a dozen other programs have been initiated to develop fission systems for space applications. While none of these additional programs launched a nuclear reactor, several lessons have emerged from these efforts that are worth incorporating in future space nuclear propulsion development efforts.
As detailed in Chapters 2 and 3, there is uncertainty regarding the ability to predict whether a complete space nuclear propulsion system can be developed in time to launch cargo missions to Mars beginning in 2033 and to execute the baseline mission in 2039. The level of uncertainty is presently lower for NTP than for NEP. Each system is characterized by a small number of significant risks (see Table 4.1). The fundamental NTP challenge is to develop an NTP system that can heat its propellant to approximately 2700 K at the reactor exit for the duration of each burn. The fundamental NEP challenge is to scale up the operating power of each NEP subsystem and to develop an integrated NEP system suitable for the baseline mission.
The roadmaps of Sections 2.6 and 3.6 show the key milestones necessary to execute the baseline 2039 human Mars mission preceded by cargo missions beginning in the 2033 opportunity. These roadmaps assume that NASA accelerates development decisions and maturation of the requisite technologies through an aggressive and focused development program, beginning in 2021 (18 years before the planned departure of the first crew and 12 years prior to the flight of the first full-scale cargo mission). NASA previously demonstrated greater expediency from less of a technical base in the successful Mercury, Gemini, and Apollo programs (e.g., Mercury was announced in October 1958 with a first successful crewed flight 31 months later; Apollo was announced in 1961 with the
TABLE 4.1 Major Challenges for Developing Nuclear Electric Propulsion (NEP) and Nuclear Thermal Propulsion (NTP) Systems for the Baseline Mission
| Category | NTP | NEP |
|---|---|---|
| Reactor Core Fuel and Materials |
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| System Operational Parameters |
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| Scale |
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| Ground-Based Testing |
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| In-Space Propulsion Technology Needs |
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| System Complexity |
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first human lunar landing 8 years later, including programmatic recovery from a major failure that resulted in the death of three astronauts). The International Space Station (from Freedom proposal in 1984 to first sustained crew presence 16 years later) provides another comparable. The committee believes that should the federal government choose to invest aggressively in this space nuclear propulsion technology, there is sufficient schedule to achieve the baseline mission. In addition, as presented in Figure 1.2, over the 17-year synodic cycle, 9 of 10 Earth-departure opportunities are feasible within the propulsive capability of a space nuclear propulsion system sized for the 2039 opportunity. As such, the next opportunities of 2042, 2045, and 2047 provide fallback potential and schedule mitigation for the chosen path.