Ceres’ Broad‐Scale Surface Geomorphology Largely Due To Asymmetric Internal Convection

Ceres’ Broad‐Scale Surface Geomorphology Largely Due To Asymmetric Internal Convection

Abstract While we now know much about the volatile‐rich world of Ceres from the Dawn mission, the deep interior remains something of an enigma, shrouded by a crust composed of water ice, carbonates, phyllosilicates, salts and clathrate hydrates. While smaller than most active moons or planets, Ceres...

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Bibliographic Details
Main Authors: Scott D. King, Michael T. Bland, Simone Marchi, Carol A. Raymond, Christopher T. Russell, Jennifer E. C. Scully, Hanna G. Sizemore
Format: Article
Language:English
Published: Wiley 2022-06-01
Series:AGU Advances
Subjects:
Ceres
mantle convection
Hanami Planum
icy bodies
Online Access:https://doi.org/10.1029/2021AV000571

Internet

https://doi.org/10.1029/2021AV000571

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