Found: 7
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Ceres' Broad‐Scale Surface Geomorphology Largely Due To Asymmetric Internal Convection.
- Published in:
- AGU Advances, 2022, v. 3, n. 3, p. 1, doi. 10.1029/2021AV000571
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- Article
Floor‐Fractured Craters on Ceres and Implications for Interior Processes.
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- Journal of Geophysical Research. Planets, 2018, v. 123, n. 12, p. 3188, doi. 10.1029/2018JE005632
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- Article
Ground ice at the Phoenix Landing Site: Stability state and origin.
- Published in:
- Journal of Geophysical Research. Planets, 2009, v. 114, n. E1, p. n/a, doi. 10.1029/2009JE003417
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- Article
The periglacial landscape at the Phoenix landing site.
- Published in:
- Journal of Geophysical Research. Planets, 2009, v. 114, n. E1, p. n/a, doi. 10.1029/2009JE003418
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- Article
A prelanding assessment of the ice table depth and ground ice characteristics in Martian permafrost at the Phoenix landing site.
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- Journal of Geophysical Research. Planets, 2008, v. 113, n. E3, p. n/a, doi. 10.1029/2007JE003067
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- Article
Geomorphological evidence for ground ice on dwarf planet Ceres.
- Published in:
- Nature Geoscience, 2017, v. 10, n. 5, p. 338, doi. 10.1038/ngeo2936
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- Article
A Geomorphic Analysis of Floor-fractured Craters on Ceres and a Study of Potential Formation Mechanisms.
- Published in:
- Geophysical Research Abstracts, 2018, v. 20, p. 7523
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- Article