NTP 101 Short Course
An Introductory Overview of Nuclear Science and Space Nuclear Power and Propulsion Systems ENERGY COMPARISON
Chemical: combustion, reaction Natural: solar (PV, thermal), EM tethers Nuclear: radioactive decay, fission Advanced nuclear: fusion, antimatter
Process Maturity Reaction Reaction Specific Specific Energy Energy Cost (eV) (J/kg) ($/kg)
6 -1 0 Combustion Proven CH4 + 2O2 → CO2 + 2H2O41010 –10 (CH4) -1 10 (O2) 7 0 Fuel Cell Proven 2H2 + O2 → 2H2O 10.2 10 10 (H2) -1 10 (O2) 6 12 6 Radioisotope Proven → 5.59 x 10 10 10 6 13 4 Fission Proven → 2 + γ 195 x 10 10 10 (XF > 93%) 6 14 3 Fusion Research → 17.57 x 10 10 10 (D) 6 6 3 → 18.35 x 10 10 ( He) Antimatter Research p + p- → γ 1.05 x 109 1016 1012 NUCLEAR = MISSION ENABLING
L = 46.9 m OD = 8.4 m Fission 341 mL of 235U = 50x MLOX = 630 MT
MH2 = 106 MT
Significantly extends mission capability by overcoming current technology limitations: Power Reliable, robust, long-duration, power dense Logistics (consumables) – Food, water, oxygen Time dependant Human Factors factors mitigated by – μg atrophy rapid propulsion decreasing transit – Psychological isolation Shielding decreases – Radiation dose crew dose RADIOSIOTOPE DECAY
U-234 Heat produced from natural alpha (α) decay 5.6 MeV
Pu-238 (He-4)
238Pu Decay
Service life activity (A) inversely proportional to
isotope half-life (t1/2)