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Coomes, E.P.; Cuta, J.M.; Webb, B.J.; King, D.Q.; Patterson, M.J.; Berkopec, F.; Jet Propulsion Lab., Pasadena, CA)
Manned Mars Mission. Working group papers, volume 2, section 5 - appendix1986
Manned Mars Mission. Working group papers, volume 2, section 5 - appendix1986
AbstractAbstract
[en] A propulsion system (PEGASUS) consisting of an electric thruster driven by a multimegawatt nuclear power system is proposed for a manned Mars mission. Magnetoplasmadynamic and mercury-ion thrusters are considered, based on a mission profile containing a 510-day burn time (for a mission time of approximately 1000 days). Both thrusters are capable of meeting the mission parameters. Electric propulsion systems have significant advantages over chemical systems, because of high specific impulse, lower propellant requirements, and lower system mass. The power for the PEGASUS system is supplied by a boiling liquid-metal fast reactor. The power system consists of the reactor, reactor shielding, power conditioning subsystems, and heat rejection subsystems. It is capable of providing a maximum of 8.5 megawatts of electrical power of which 6 megawatts is needed for the thruster system, leaving 1.5 megawatts available for inflight mission applications
Primary Subject
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Duke, M.B.; Keaton, P.W.; National Aeronautics and Space Administration, Huntsville, AL (USA). George C. Marshall Space Flight Center; vp; May 1986; vp; Manned mars mission workshop; Huntsville, AL (USA); 10-14 Jun 1985; Available from NTIS, PC A24/MF A01
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[en] Various issues associated with getting technology development of nuclear power systems moving at a pace which will support the anticipated need for such systems in later years is discussed. The projected power needs of such advanced space elements as growth space stations and lunar and planetary vehicles and bases are addressed briefly, and the relevance of nuclear power systems is discussed. A brief history and status of the U.S. nuclear reactor systems is provided, and some of the problems (real and/or perceived) are dealt with briefly. Key areas on which development attention should be focused in the near future are identified, and a suggested approach is recommended to help accelerate the process
Primary Subject
Source
Duke, M.B.; Keaton, P.W.; National Aeronautics and Space Administration, Huntsville, AL (USA). George C. Marshall Space Flight Center; vp; May 1986; vp; Manned mars mission workshop; Huntsville, AL (USA); 10-14 Jun 1985; Available from NTIS, PC A24/MF A01
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[en] There are specific risks to the crew of the manned Mars mission from energetic particles generated by solar activity. Therefore, mission planning must provide for solar monitoring and solar activity forecasts. The main need is to be able to anticipate the energetic particle events associated with some solar flares and, occasionally, with erupting filaments. A second need may be for forecasts of solar interference with radio communication between the manned Mars mission (during any of its three phases) and Earth. These two tasks are compatible with a small solar observatory that would be used during the transit and orbital phases of the mission. Images of the Sun would be made several times per hour and, together with a solar x-ray detector, used to monitor for the occurrence of solar activity. The data would also provide a basis for research studies of the interplanetary medium utilizing observations covering more of the surface of the Sun than just the portion facing Earth
Primary Subject
Source
Duke, M.B.; Keaton, P.W.; National Aeronautics and Space Administration, Huntsville, AL (USA). George C. Marshall Space Flight Center; vp; May 1986; vp; Manned mars mission workshop; Huntsville, AL (USA); 10-14 Jun 1985; Available from NTIS, PC A24/MF A01
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[en] The feasibility of rebuilding and testing a nuclear thermal rocket (NTR) for the Mars mission was investigted. Calculations indicate that an NTR would substantially reduce the Earth-orbit assemble mass compared to LOX/LH2 systems. The mass savings were 36 and 65% for the cases of total aerobraking and of total propulsive braking respectively. Consequently, the cost savings for a single mission of using an NTR, if aerobraking is feasible, are probably insufficient to warrant the NTR development. If multiple missions are planned or if propulsive braking is desired at Mars and/or at Earth, then the savings of about $7 billion will easily pay for the NTR. Estimates of the cost of rebuilding a NTR were based on the previous NERVA program's budget plus additional costs to develop a flight ready engine. The total cost to build the engine would be between $4 to 5 billion. The concept of developing a full-power test stand at Johnston Atoll in the Pacific appears very feasible. The added expense of building facilities on the island should be less than $1.4 billion
Primary Subject
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Duke, M.B.; Keaton, P.W.; National Aeronautics and Space Administration, Huntsville, AL (USA). George C. Marshall Space Flight Center; vp; May 1986; vp; Manned mars mission workshop; Huntsville, AL (USA); 10-14 Jun 1985; Available from NTIS, PC A24/MF A01
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Bents, D.; Patterson, M.J.; Berkopec, F.; Myers, I.; Presler, A.
Manned Mars Mission. Working group papers, volume 2, section 5 - appendix1986
Manned Mars Mission. Working group papers, volume 2, section 5 - appendix1986
AbstractAbstract
[en] The high impulse of electric propulsion makes it an attractive option for manned interplanetary missions such as a manned mission to Mars. This option is, however, dependent on the availability of high energy sources for propulsive power in addition to that required for the manned interplanetary transit vehicle. Two power system technologies are presented: nuclear and solar. The ion thruster technology for the interplanetary transit vehicle is described for a typical mission. The power management and distribution system components required for such a mission must be further developed beyond today's technology status. High voltage-high current technology advancements must be achieved. These advancements are described. In addition, large amounts of waste heat must be rejected to the space environment by the thermal management system. Advanced concepts such as the liquid droplet radiator are discussed as possible candidates for the manned Mars mission. These thermal management technologies have great potential for significant weight reductions over the more conventional systems
Primary Subject
Source
Duke, M.B.; Keaton, P.W.; National Aeronautics and Space Administration, Huntsville, AL (USA). George C. Marshall Space Flight Center; vp; May 1986; vp; Manned mars mission workshop; Huntsville, AL (USA); 10-14 Jun 1985; Available from NTIS, PC A24/MF A01
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[en] Several different types of propulsion concepts are discussed: pulsed fission; continuous nuclear fission; chemical; and chemical boost with advanced nuclear fission. Some of the key characteristics of each type are provided, and typical concepts of each are shown
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Duke, M.B.; Keaton, P.W.; National Aeronautics and Space Administration, New York (USA). Goddard Inst. for Space Studies; vp; May 1986; vp; Manned mars mission workshop; Huntsville, AL (USA); 10-14 Jun 1985; Available from NTIS, PC A24/MF A01
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[en] Potential radiation hazards to crew members on manned Mars missions are discussed. It deals briefly with radiation sources and environments likely to be encountered during various phases of such missions, providing quantitative estimates of these environments. Also provided are quantitative data and discussions on the implications of such radiation on the human body. Various sorts of protective measures are suggested. Recent re-evaluation of allowable dose limits by the National Council of Radiation Protection is discussed, and potential implications from such activity are assessed
Primary Subject
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Duke, M.B.; Keaton, P.W.; National Aeronautics and Space Administration, Huntsville, AL (USA). George C. Marshall Space Flight Center; vp; May 1986; vp; Manned mars mission workshop; Huntsville, AL (USA); 10-14 Jun 1985; Available from NTIS, PC A24/MF A01
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Howe, S.D.; Hynes, M.V.
Manned Mars Mission. Working group papers, volume 2, section 5 - appendix1986
Manned Mars Mission. Working group papers, volume 2, section 5 - appendix1986
AbstractAbstract
[en] The use of advanced propulsion techniques must be considered if the currently envisioned launch date of the manned Mars mission were delayed until 2020 or later. Within the next thirty years, technological advances may allow such methods as beaming power to the ship, inertial-confinement fusion, or mass-conversion of antiprotons to become feasible. A propulsion system with an ISP of around 5000 s would allow the currently envisioned mission module to fly to Mars in 3 months and would require about one million pounds to be assembled in Earth orbit. Of the possible methods to achieve this, the antiproton mass-conversion reaction offers the highest potential, the greatest problems, and the most fascination. Increasing the production rates of antiprotons is a high priority task at facilities around the world. The application of antiprotons to propulsion requires the coupling of the energy released in the mass-conversion reaction to thrust-producing mechanisms. Recent proposals entail using the antiprotons to produce inertial confinement fusion or to produce negative muons which can catalyze fusion. By increasing the energy released per antiproton, the effective cost, (dollars/joule) can be reduced. These proposals and other areas of research can be investigated now. These short term results will be important in assessing the long range feasibility of an antiproton powered engine
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Duke, M.B.; Keaton, P.W.; National Aeronautics and Space Administration, Huntsville, AL (USA). George C. Marshall Space Flight Center; vp; May 1986; vp; Manned mars mission workshop; Huntsville, AL (USA); 10-14 Jun 1985; Available from NTIS, PC A24/MF A01
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Hall, S.B.; Mccann, M.E.
Manned Mars Mission. Working group papers, volume 2, section 5 - appendix1986
Manned Mars Mission. Working group papers, volume 2, section 5 - appendix1986
AbstractAbstract
[en] The problem of shielding a crew during early manned Mars missions is discussed. Requirements for shielding are presented in the context of current astronaut exposure limits, natural ionizing radiation sources, and shielding inherent in a particular Mars vehicle configuration. An estimated range for shielding weight is presented based on the worst solar flare dose, mission duration, and inherent vehicle shielding
Primary Subject
Source
Duke, M.B.; Keaton, P.W.; National Aeronautics and Space Administration, Huntsville, AL (USA). George C. Marshall Space Flight Center; vp; May 1986; vp; Manned mars mission workshop; Huntsville, AL (USA); 10-14 Jun 1985; Available from NTIS, PC A24/MF A01
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Letaw, J.R.; Silberberg, R.; Tsao, C.H.
Manned Mars Mission. Working group papers, volume 2, section 5 - appendix1986
Manned Mars Mission. Working group papers, volume 2, section 5 - appendix1986
AbstractAbstract
[en] The hazards of the natural radiation environment (cosmic rays and solar energetic particles) on a manned mission to Mars are considered. These hazards are addressed in three different settings: the flight to Mars where the astronauts are shielded only by the spacecraft; on the surface of Mars under an atmosphere of about 10 g/sq cm carbon dioxide; and under the surface of Mars where additional shielding would result
Primary Subject
Source
Duke, M.B.; Keaton, P.W.; Naval Research Lab., Washington, DC (USA); vp; May 1986; vp; Manned mars mission workshop; Huntsville, AL (USA); 10-14 Jun 1985; Available from NTIS, PC A24/MF A01
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