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Browsing LPI Contributions by Subject "Ceres (Dwarf planet)"

Browsing LPI Contributions by Subject "Ceres (Dwarf planet)"

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  • Schenk, Paul M.; Scully, J. E. C.; Buczkowski, Debra L.; Sizemore, Hanna G.; Schmidt, B.; Pieters, Carlé M.; Neesemann, A.; O’Brien, D. P.; Marchi, Simone; Williams, David A. (Planetary geologist); Nathues, A.; De Sanctis, M. Cristina; Tosi, F.; Russell, C. T. (Christopher T.); Castillo-Rogez, Julie; Raymond, Carol A. (Nature, 2020-08-10)
    Here we show using Dawn high-resolution stereo imaging and topography that Ceres’ unique composition has resulted in widespread mantling by solidified water- and salt-rich mud-like impact melts with scattered endogenic ...
  • Marchi, Simone; Ermakov, A. I.; Raymond, Carol A.; Fu, Roger R. (Roger Rennan); O’Brien, D. P.; Bland, M. T.; Ammannito, E.; De Sanctis, M. Cristina; Bowling, T.; Schenk, Paul M.; Scully, J. E. C.; Buczkowski, Debra L.; Williams, David A. (Planetary geologist); Hiesinger, H. (Harald); Russell, C. T. (Christopher T.) (Nature, 2016-07-26)
    Asteroids provide fundamental clues to the formation and evolution of planetesimals. Collisional models based on the depletion of the primordial main belt of asteroids predict 10–15 craters 4400 km should have formed on ...
  • Sizemore, Hanna G.; Schenk, Paul M. (American Geophysical Union, 2017-06-27)
    Prior to the arrival of the Dawn spacecraft at Ceres, the dwarf planet was anticipated to be ice‐rich. Searches for morphological features related to ice have been ongoing during Dawn's mission at Ceres. Here we report the ...
  • De Sanctis, M. Cristina;; Shaner, Andrew;; Webb, Sha'Rell; Portillo, Kevin (Lunar and Planetary Institute, 2019)
    The front of the graphic includes a picture of the planet, a histogram showing the abundance of the Top 5 elements at that planet, and an outline of the Periodic Table highlighting the location of those elements on the ...

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