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Fission or fusion for Mars missions : Expectations and challenges

dc.contributor.authorKammash, Terry B.en_US
dc.date.accessioned2006-04-10T17:50:27Z
dc.date.available2006-04-10T17:50:27Z
dc.date.issued1994-10en_US
dc.identifier.citationKammash, Terry (1994/10)."Fission or fusion for Mars missions : Expectations and challenges." Acta Astronautica 34(): 17-23. <http://hdl.handle.net/2027.42/31267>en_US
dc.identifier.urihttp://www.sciencedirect.com/science/article/B6V1N-47WTRK5-3W/2/a3b8b250502bd9c6ef89afa055c62b6cen_US
dc.identifier.urihttps://hdl.handle.net/2027.42/31267
dc.description.abstractA fission based system in the form of the Gas Core Nuclear Rocket (GCR) and a laser-driven inertial fusion system that utilizes a self-generated magnetic field (MICF) are compared as potential propulsion systems for manned planetary travel. The first generates thrust by a hydrogen propellant that is heated by radiation emitted from a critical reactor with a uranium fuel in plasma form, to take advantage of high achievable temperatures. The fusion system produces attractive propulsion characteristics through energy magnification of a hot hydrogenous plasma which is guided by a magnetic nozzle that allows thermal energy to be converted into thrust. Although both systems are capable of producing several thousand seconds of specific impulse, and tens to hundreds of kilonewtons of thrust, each faces some formidable physics and engineering problems that must be addressed if they are to become viable propulsion systems. With the aid of an appropriate set of fluid and plasma equations, we assess the dynamics of each system and identify those issues that could detract from their performance. In the case of GCR, thermal hydraulic considerations reveal deterioration of propulsive capability when wall heat flux limitations and turbulent mixing are taken into account. Moreover, hydrodynamics and acoustic instabilities could also adversely affect its performance, although they may be amenable to stabilization by magnetic fields. For MICF, large energy multiplication at modest input laser energies appears to be a major concern, but if anti-hydrogen can be used to initiate the fusion reactions, this concept can be truly an outstanding propulsion device.en_US
dc.format.extent605016 bytes
dc.format.extent3118 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherElsevieren_US
dc.titleFission or fusion for Mars missions : Expectations and challengesen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelAtmospheric, Oceanic and Space Sciencesen_US
dc.subject.hlbsecondlevelAerospace Engineeringen_US
dc.subject.hlbtoplevelScienceen_US
dc.subject.hlbtoplevelEngineeringen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumUniversity of Michigan, Ann Arbor, MI, U.S.A.en_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/31267/1/0000173.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1016/0094-5765(94)90238-0en_US
dc.identifier.sourceActa Astronauticaen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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