A microphysical thermal model for the lunar regolith: Determining the lunar regolith properties using a combination of LRO/Diviner and Chang’E-2/MRM data
Context. The surface of the Moon is covered by regolith and its microphysical structure is not only linked to surface processes and regolith evolution, but is also important for in situ resource utilization and mission planning. Aims. We aim to uniquely constrain lunar regolith grain size and densit...
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| Autors principals: | , , , |
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| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
EDP Sciences
2026-06-01
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| Col·lecció: | Astronomy & Astrophysics |
| Matèries: | |
| Accés en línia: | https://www.aanda.org/articles/aa/full_html/2026/06/aa59897-26/aa59897-26.html |
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