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  • Potential regions for finding small satellites and dust particles in the Pluto's system: Implications for the New Horizons Mission

    Paper number

    IAC-11,A3,5,11,x11111

    Author

    Dr. Silvia Giuliatti-Winter, Saõ Paulo State University (UNESP), Brazil

    Year

    2011

    Abstract
    Pluto and Charon form a binary system and, along with the  recent discovered satellites Nix 
    and Hydra, will be imaged by the New Horizons spacecraft  in 2015. In this work we  analysed the effects that small and large particles can suffer due to different perturbative effects through a sample of numerical simulations. For  cm-sized particles we identified  stable regions for  particles in S and P-types  orbits under the gravitational perturbations  of Pluto, Charon, Nix and Hydra. Some of the internal stable regions are located very close  to the orbital path of the New Horizons mission posing as a potential hazard for this mission. 
    
    	We also analysed the effects of hypothetical satellites, with sizes varyng from 1-50km in radius,  on the orbital evolution of Nix and Hydra in order to constrain an upper limit size. Our results, derived from a sample of numerical simulations, show that some hypothetical satellites can be coorbital to Nix or Hydra, and they can also be located  in specific  regions  between the orbits of  them without provoking any significant gravitational effects on the orbital elements of Nix and Hydra.  These  regions   are potential regions to look for undiscovered satellites at the time the mission passes by Pluto-Charon system.
    
    	Although Pluto's system is far away from the Sun, the effects of the solar radiation pressure are do important for  dust particles  with sizes ranging from 1-30$\mu$m.  The effects of this dissipative force, combined with the gravitational effects of the four massive bodies, provoke   collisions and ejections of these tiny particles in a time much less than 1000years.  Only a small fraction of particles survived for the entire time span of the integration. Therefore,  if  Pluto has a tenuous ring  it  has to be continuously  replenished.
    Abstract document

    IAC-11,A3,5,11,x11111.brief.pdf

    Manuscript document

    (absent)