This NIAC (NASA Advanced Innovative Concepts) work will focus on Mars and will build on previous efforts at analyzing atmospheric mining at Earth and the outer solar system. Spacecraft systems concepts will be evaluated and traded, to assess feasibility. However the study will primarily examine the architecture and associated missions to explore the closure, constraints and critical parameters through sensitivity studies. The Mars atmosphere consists of 95.5 percent CO2 gas which can be converted to methane fuel (CH4) and Oxidizer (O2) for chemical rocket propulsion, if hydrogen is transported from electrolyzed water on the Mars surface or from Earth. By using a highly elliptical Mars Molniya style orbit, the CO2 atmosphere can be scooped, ram-compressed and stored while the spacecraft dips into the Mars atmosphere at periapsis. Successive orbits result in additional scooping of CO2 gas, which also serves to aerobrake the spacecraft, resulting in a decaying Molniya orbit.


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    Titel :

    Mars Molniya Orbit Atmospheric Resource Mining


    Beteiligte:
    Mueller, Robert P. (Autor:in) / Braun, Robert D. (Autor:in) / Sibille, Laurent (Autor:in) / Sforzo, Brandon (Autor:in) / Gonyea, Keir (Autor:in) / Ali, Hisham (Autor:in)

    Kongress:

    NIAC Orientation Meeting - Phase 1 ; 2016 ; Washington, DC, United States


    Erscheinungsdatum :

    2016-06-14


    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch




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    A PC based tool for Molniya orbit analysis

    Gunning, G. / Chao, C. | AIAA | 1996