Conditions for the Long‐Term Preservation of a Deep Brine Reservoir in Ceres-Reference-Cited by-同舟云学术

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

Published:2019-02-19 Issue:4 Volume:46 Page:1963-1972
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophys. Res. Lett.

Author:

Castillo‐Rogez Julie C.¹^ORCID,Hesse M. A.²^ORCID,Formisano M.³^ORCID,Sizemore H.⁴^ORCID,Bland M.⁵^ORCID,Ermakov A. I.¹^ORCID,Fu R. R.⁶^ORCID

Affiliation:

1. Jet Propulsion Laboratory, California Institute of Technology Pasadena CA USA

2. Department of Geological SciencesThe University of Texas at Austin Austin TX USA

3. INAF‐IAPS, Istituto di Astrofisica e Planetologia Spaziali di Roma Italy

4. Planetary Science Institute Tucson AZ USA

5. United States Geological Survey Flagstaff AZ USA

6. Department of Earth and Planetary SciencesHarvard University Cambridge MA USA

Funder

Connecticut Space Grant College Consortium

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2018GL081473

Reference50 articles.

1. Distribution of phyllosilicates on the surface of Ceres

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

3. Bland M. T. Sizemore H. G. Buczkowski D. L. Sori M. M. Raymond C. A. King S. D. &Russell C. T.(2018).Why is Ceres lumpy? Surface deformation induced by solid‐state subsurface flow. In49th Lunar and Planetary Science Conference 19‐23 March 2018 The Woodlands. Texas LPI Contribution No. 2083 id.1627.

4. Post-impact thermal structure and cooling timescales of Occator crater on asteroid 1 Ceres

5. Floor‐Fractured Craters on Ceres and Implications for Interior Processes

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