A partially differentiated interior for (1) Ceres deduced from its gravity field and shape

  title={A partially differentiated interior for (1) Ceres deduced from its gravity field and shape},
  author={Ryan S. Park and Alex S. Konopliv and Bruce G. Bills and N. Rambaux and Julie C. Castillo‐Rogez and Carol A. Raymond and Andrew T. Vaughan and Anton I. Ermakov and Maria T. Zuber and Roger R. Fu and M. J. Toplis and Christopher T. Russell and Andreas Nathues and Frank Preusker},
Remote observations of the asteroid (1) Ceres from ground- and space-based telescopes have provided its approximate density and shape, leading to a range of models for the interior of Ceres, from homogeneous to fully differentiated. A previously missing parameter that can place a strong constraint on the interior of Ceres is its moment of inertia, which requires the measurement of its gravitational variation together with either precession rate or a validated assumption of hydrostatic… 

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