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  • Equilibrium configurations for attitude and orbital control by tether system.

    Paper number

    IAC-15,C1,6,3,x31509

    Author

    Dr. Denilson Paulo Souza dos Santos, Instituto Nacional de Pesquisas Espaciais - INPE (Brasil) \ Centre for Mechanical and Aerospace Science and Technologies (C-MAST), Portugal, Brazil

    Coauthor

    Prof. Anna Guerman, Centre for Mechanical and Aerospace Science and Technologies (C-MAST), Portugal

    Coauthor

    Dr. Alexander Burov, Dorodnitsyn Computing Center, Russian Academy of Sciences, Russian Federation

    Year

    2015

    Abstract
    The use of spacecraft’s shape change and mass re-distribution for attitude and orbital control has been proposed in several studies. For example, much research on tether systems suggests controlling system position and/or orientation by changing the tether length. Recently, we have examined dynamics of a two-body tethered system in an elliptic orbit and proved the possibility to keep the tether orientation with respect to the Earth using tether length control. There exist also a possibility to implement a uniform, with respect to the true anomaly $\nu$, rotation of such tether system; periodic control of the tether length for uniform rotations have been found and their stability studied.
    
    In more general case of a spatial spacecraft, it can be shown that if the spacecraft inertia tensor $I$ changes with true anomaly $\nu$ so as $(1+ecos$\nu$)^2I=const$, there exist 24 relative equilibria of the spacecraft. In these equilibria configurations, one of the spacecraft’s principal axes of inertia is aligned with the local vertical and another is orthogonal to the orbit plane. 
    
    The objective of the current study is to analyze the behavior of a 3D spacecraft in a central keplerian force field and possibility to cause spacecraft rotation via mass distribution control. We develop a model for dynamics of body whose tensor of inertia can be changed according to a prescribed control law and study control of its attitude motion when its center of mass moves along an elliptic orbit. We show that there exists periodic control for such motion and analyze its stability.
    Abstract document

    IAC-15,C1,6,3,x31509.brief.pdf

    Manuscript document

    (absent)