Affordable Development and Demonstration of a Small NTR Engine and Stage: How Small is Big Enough?

摘要

The Nuclear Thermal Rocket (NTR) derives its energy from fission of uranium-235 atoms contained within fuel elements that comprise the engine's reactor core. It generates high thrust and has a specific impulse potential of ～900 seconds - a 100% increase over today's best chemical rockets. The Nuclear Thermal Propulsion (NTP) project, funded by NASA's AES program, includes five key task activities: (1) Recapture, demonstration, and validation of heritage graphite composite (GC) fuel (selected as the "Lead Fuel" option); (2) Engine Conceptual Design; (3) Operating Requirements Definition; (4) Identification of Affordable Options for Ground Testing; and (5) Formulation of an Affordable Development Strategy. During FY '14, a preliminary DDT&E plan and schedule for NTP development was outlined by GRC, DOE and industry that involved significant system-level demonstration projects that included GTD tests at the NNSS, followed by a FTD mission. To reduce cost for the GTD tests and FTD mission, small NTR engines, in either the 7.5 or 16.5 klbr thrust class, were considered. Both engine options used GC fuel and a "common" fuel element (FE) design. The small ～7.5 klbr "criticality-limited" engine produces -157 megawatts of thermal power (MWt) and its core is configured with parallel rows of hexagonal-shaped FEs and tie tubes (TTs) with a FE to TT ratio of ～1:1. The larger ～16.5 klbr Small Nuclear Rocket Engine (SNRE), developed by LANL at the end of the Rover program, produces ～367 MWt and has a FE to TT ratio of ～2:1. Although both engines use a common 35 inch (～89 cm) long FE, the SNRE's larger diameter core contains ～300 more FEs needed to produce an additional 210 MW_t of power. To reduce the cost of the FTD mission, a simple "1-burn" lunar flyby mission was considered to reduce the LF_2 propellant loading, the stage size and complexity. Use of existing and flight proven liquid rocket and stage hardware (e.g., from the RL10B-2 engine and Delta Cryogenic Second Stage) was also maximized to further aid affordability. This paper examines the pros and cons of using these two small engine options, including their potential to support future human exploration missions to the Moon, near Earth asteroids, and Mars, and recommends a preferred size. It also provides a preliminary assessment of the key activities, development options, and schedule required to affordably build, ground test and fly a small NTR engine and stage within a 10-year timeframe.