The violent collisional history of aqueously evolved (2) Pallas

@article{Marsset2020TheVC,
  title={The violent collisional history of aqueously evolved (2) Pallas},
  author={Micha{\"e}l Marsset and Miroslav Bro{\vz} and Pierre Vernazza and Alexis Drouard and Julie C. Castillo‐Rogez and Josef Hanu{\vs} and M. Viikinkoski and N. Rambaux and Beno{\^i}t Carry and Laurent Jorda and Pavel {\vS}eve{\vc}ek and Mirel Birlan and Franck Marchis and Edyta Podlewska-Gaca and Erik Asphaug and Przemysław Bartczak and J{\'e}r{\^o}me Berthier and Fabrice Cipriani and F. Colas and Grzegorz Dudziński and Christophe Dumas and Josef Ďurech and Marin Ferrais and Romain F{\'e}tick and Thierry Fusco and Emmanuel Jehin and Mikko Kaasalainen and Agnieszka Kryszczyńska and Philippe Lamy and H. Le Coroller and Anna Marciniak and Tadeusz Michałowski and Patrick Michel and Derek C. Richardson and Toni Santana-Ros and Paolo Tanga and Fr{\'e}d{\'e}ric Vachier and Arthur Vigan and Olivier G. Witasse and Bin Yang},
  journal={Nature Astronomy},
  year={2020},
  volume={4},
  pages={569-576}
}
Asteroid (2) Pallas is the largest main-belt object not yet visited by a spacecraft, making its surface geology largely unknown and limiting our understanding of its origin and collisional evolution. Previous ground-based observational campaigns returned different estimates of its bulk density that are inconsistent with one another, one measurement 1 being compatible within error bars with the icy Ceres (2.16 ± 0.01 g cm −3 ) 2 and the other 3 compatible within error bars with the rocky Vesta… 
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