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An Extremely High Isp Spacecraft Propulsion SystemSpecific Impulse, Isp, is a measure of a rocket engine’s efficiency. It is calculated relative to the Earth’s gravitational field, where Isp = ve/ go, with go= 9.8 m/s2 and the escape velocity of the propellant, ve, in m/s. Chemical rockets have ve < 4.4x103 m/s and Isp < 450 seconds. As an alternative, the NASA Glenn Research Center developed multiple generations of Solar Electric Propulsion (SEP), high Isp, ion engines using Xe gas as a propellant. Consequently, over 100 SEP Ion Thrusters provide geo-synchronous station keeping along with deep space probes like Deep Space One and Dawn. These
have ve » 2.9 x 104 m/s with Isp = 3x103 seconds. These thrusters have continuous operating lifetimes of thousands of hours allowing continuous acceleration making up for the very low thrust.

Chang-Diaz’ Variable Specific Impulse Magnetoplasma Rocket (VASIMR) has the potential for four times the propellant escape velocity and four times the specific impulse1. Unfortunately, this comes at a tremendous electrical power cost, estimated at 200 kWe for maintaining the International Space Station in Low Earth Orbit (LEO). Although nuclear fission and fusion reactors2 have been suggested for powering nuclear thermal propulsion (NTP) it only doubles the Isp over chemical rockets but with comparable thrust. Instead, we propose using Lattice Confinement Fusion (LCF) reactions.
Document ID
20220006853
Acquisition Source
Glenn Research Center
Document Type
Presentation
Authors
L P Forsley
(JWK Corporation (United States) Annandale, Virginia, United States)
T L Benyo
(Glenn Research Center Cleveland, Ohio, United States)
P A Mosier-Boss
(GEC LLC)
L A Dudzinski
(National Aeronautics and Space Administration Washington D.C., District of Columbia, United States)
Date Acquired
May 3, 2022
Subject Category
Spacecraft Propulsion And Power
Energy Production And Conversion
Meeting Information
Meeting: American Nuclear Society NETS-22
Location: Cleveland, OH
Country: US
Start Date: May 8, 2022
End Date: May 12, 2022
Sponsors: American Nuclear Society
Funding Number(s)
WBS: 138494.01.99.01
Distribution Limits
Public
Copyright
Public Use Permitted.
Technical Review
NASA Peer Committee
Keywords
High Isp Propulsion
Nuclear Fusion
Lattice Confinement Fusion
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