Constraining Ocean and Ice Shell Thickness on Miranda from Surface Geological Structures and Stress Modeling
Images from the Voyager 2 mission revealed the small Uranian satellite Miranda to be a complex, dynamic world. This is exemplified by signs of recent geological activity, including an extensive fault system and the mysterious coronae. This has led to speculation that Miranda may have been tectonical...
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| Autors principals: | , , , |
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| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
IOP Publishing
2024-01-01
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| Col·lecció: | The Planetary Science Journal |
| Matèries: | |
| Accés en línia: | https://doi.org/10.3847/PSJ/ad77d7 |
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