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  • analysis of the external region of the Pluto system for different values of inclination and eccentricity of the particles

    Paper number

    IAC-17,C1,8,5,x36628

    Author

    Prof.Dr. Silvia Maria Giuliatti Winter, UNESP - Univ Estadual Paulista, Brazil

    Coauthor

    Mr. Daniel Gaslac, Brazil

    Coauthor

    Dr. Pryscilla Pires dos Santos, Univ. Federal Fluminense, Brazil

    Year

    2017

    Abstract
    Pluto and Charon form a binary system due to the large mass ratio ($\mu  = 0.12$) and the small
    distance (d = 19570km) between them. Four small satellites, discovered after the launch of
    the New Horizons spacecraft, are located exterior to Charon’s orbit. Styx, Nix, Kerberos
    and Hydra have very small eccentricity and are all coplanar with Charon’s orbital plane. In
    this work we analysed external regions for a set of particles with different values of
    eccentricity and inclination. From our numerical simulations, taking into account the
    gravitational effects of Pluto and its five satellites, we generate diagrams of $a$ versus $e$ and $a$
    versus $I$ (where $a$ is the semi major axis, $e$ is the eccentricity and $I$ is the inclination of the
    particles) after a timespan of $10^5$ orbital periods of Charon (about 650000days). The
    external region was divided into three: a) region 1 between $1.5d$ to $2.5d$ - Styx and Nix are
    located in this region; b) region 2 between $2.5d$ to $3.5d$ - Kerberos and Hydra are located in
    this region, and c) region 3 external to Hydra’s orbit. For particles with $I \leq $90^{\circ}$,
    our results show that less than $30\%$ of the initial set of particles remains in regions 2 and 3,
    while in region 1 less than $5\%$ survived after 650000days. However, about $30\%$ of particles
    located in region 1 survives when its $I > 90^{\circ}$. When the Solar Radiation
    Pressure is included in the system, only a small number of particles larger than $10\mu m$ 
    stays in the system. Smaller particles are ejected or collide with the massive bodies in a very
    short period of time.
    Abstract document

    IAC-17,C1,8,5,x36628.brief.pdf

    Manuscript document

    IAC-17,C1,8,5,x36628.pdf (🔒 authorized access only).

    To get the manuscript, please contact IAF Secretariat.