Telemetry data from three 445 N engine burns of the Cassini spacecraft are used to characterize the high-g slosh characteristics of bipropellants in cylindrical tanks with spherical end domes. Comparisons between flight data and theoretical results indicate that high-g clean tank slosh frequency and high-g sector mode frequency could be predicted with errors of 3–5%. However, at lower tanks’ fill fractions of <35%, when most of the propellants reside in the spherical end domes of the tanks, the prediction errors deteriorated to >5%. Also, high-g full-tank slosh mode in a tank with an eight-panel propellant management device could be modeled using an annular cylindrical tank. Again, prediction error of full-tank slosh frequency degraded with decreasing fill fractions. Based on these results, the high-g sector and full-tank propellant slosh frequencies could be well predicted using simple analytical techniques before these predictions are refined by liquid slosh computer modeling tools. A set of small-amplitude oscillatory motions of the spacecraft attitude was detected during 13 science observations conducted in 2007–2008. Their frequencies matched well the low-g slosh frequency predicted analytically for uncompartmented tank. The root cause and analytical prediction of the observed spacecraft oscillatory motion in low-g condition is an interesting topic for future research.


    Access

    Access via TIB

    Check availability in my library

    Order at Subito €


    Export, share and cite



    Title :

    In-Flight Characterization of the Cassini Spacecraft Propellant Slosh Modes


    Contributors:


    Publication date :

    2017




    Type of media :

    Article (Journal)


    Type of material :

    Print


    Language :

    English



    Classification :

    BKL:    55.60 Raumfahrttechnik
    Local classification TIB:    770/7040