Ceres’ Broad‐Scale Surface Geomorphology Largely Due To Asymmetric Internal Convection-Reference-Cited by-同舟云学术

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

Published:2022-05-17 Issue:3 Volume:3 Page:
ISSN:2576-604X
Container-title:AGU Advances
language:en
Short-container-title:AGU Advances

Author:

King Scott D.¹^ORCID,Bland Michael T.²^ORCID,Marchi Simone³^ORCID,Raymond Carol A.⁴^ORCID,Russell Christopher T.⁵^ORCID,Scully Jennifer E. C.⁴^ORCID,Sizemore Hanna G.³^ORCID

Affiliation:

1. Department of Geosciences Virginia Tech Blacksburg VA USA

2. United States Geological Survey Flagstaff AZ USA

3. Planetary Science Institute Tucson AZ USA

4. Jet Propulsion Laboratory California Institute of Technology Pasadena CA USA

5. Department of Earth, Planetary, and Space Sciences University of California Los Angeles CA USA

Funder

Science Mission Directorate

Publisher

American Geophysical Union (AGU)

Subject

General Medicine

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2021AV000571

Reference55 articles.

1. Composition and structure of the shallow subsurface of Ceres revealed by crater morphology

2. Giant convecting mud balls of the early solar system

3. Seismic imaging of hotspot-related crustal underplating beneath the Marquesas Islands

4. Conditions for the Long‐Term Preservation of a Deep Brine Reservoir in Ceres

5. Ceres’ evolution and present state constrained by shape data

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