Morphological Indicators of a Mascon Beneath Ceres's Largest Crater, Kerwan

Morphological Indicators of a Mascon Beneath Ceres's Largest Crater, Kerwan

Abstract Gravity data of Ceres returned by the National Aeronautics and Space Administration's Dawn spacecraft is consistent with a lower density crust of variable thickness overlying a higher density mantle. Crustal thickness variations can affect the long‐term, postimpact modification of impa...

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Bibliographic Details
Main Authors: M. T. Bland, A. I. Ermakov, C. A. Raymond, D. A. Williams, T. J. Bowling, F. Preusker, R. S. Park, S. Marchi, J. C. Castillo‐Rogez, R. R. Fu, C. T. Russell
Format: Article
Language:English
Published: Wiley 2018-02-01
Series:Geophysical Research Letters
Subjects:
Ceres
crater morphology
interior structure
gravity anomaly
mascon
Online Access:https://doi.org/10.1002/2017GL075526
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https://doi.org/10.1002/2017GL075526

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