Pitted Terrain on Vesta and Implications for the Presence of Volatiles

@article{Denevi2012PittedTO,
  title={Pitted Terrain on Vesta and Implications for the Presence of Volatiles},
  author={B. Denevi and D. Blewett and D. Buczkowski and F. Capaccioni and M. Capria and M. D. De Sanctis and W. Garry and R. Gaskell and L. Le Corre and J.-Y. Li and S. Marchi and T. McCoy and A. Nathues and D. O'Brien and N. Petro and C. Pieters and F. Preusker and C. Raymond and V. Reddy and C. Russell and P. Schenk and J. Scully and J. Sunshine and F. Tosi and D. Williams and D. Wyrick},
  journal={Science},
  year={2012},
  volume={338},
  pages={246 - 249}
}
Vesta to the Core Vesta is one of the largest bodies in the main asteroid belt. Unlike most other asteroids, which are fragments of once larger bodies, Vesta is thought to have survived as a protoplanet since its formation at the beginning of the solar system (see the Perspective by Binzel, published online 20 September). Based on data obtained with the Gamma Ray and Neutron Detector aboard the Dawn spacecraft, Prettyman et al. (p. 242, published online 20 September) show that Vesta's reputed… Expand
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