This study was conducted to evaluate several propulsion system options for the Global Precipitation Measurement (GPM) core satellite. Orbital simulations showed clear benefits for the scientific data to be obtained at a constant orbital altitude rather than with a decay/reboost approach. An orbital analysis estimated the drag force on the satellite will be 1 to 12 mN during the five-year mission. Four electric propulsion systems were identified that are able to compensate for these drag forces and maintain a circular orbit. The four systems were the UK-10/TS and the NASA 8 cm ion engines, and the ESA RMT and RITl0 EVO radio-frequency ion engines. The mass, cost, and power requirements were examined for these four systems. The systems were also evaluated for the transfer time from the initial orbit of 400 x 650 km altitude orbit to a circular 400 km orbit. The transfer times were excessive, and as a consequence a dual system concept (with a hydrazine monopropellant system for the orbit transfer and electric propulsion for drag compensation) was examined. Clear mass benefits were obtained with the dual system, but cost remains an issue because of the larger power system required for the electric propulsion system. An electrodynamic tether was also evaluated in this trade study.


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    Title :

    Propulsion Options for the Global Precipitation Measurement Core Satellite


    Contributors:
    E. H. Cardiff (author) / G. T. Davis (author) / D. C. Folta (author)

    Publication date :

    2003


    Size :

    11 pages


    Type of media :

    Report


    Type of material :

    No indication


    Language :

    English




    Propulsion Options for the Global Precipitation Measurement Core Satellite

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    Propulsion Options for the Global Precipitation Measurement Core Satellite

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    Small Satellite Propulsion Options

    R. M. Myers / S. R. Oleson / F. M. Curran et al. | NTIS | 1994


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    Small Satellite Propulsion Options

    Myers, R. M. / Oleson, S. R. / Curran, F. M. et al. | British Library Conference Proceedings | 1994