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...
Uloženo v:
| Hlavní autoři: | , , , |
|---|---|
| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
EDP Sciences
2026-06-01
|
| Edice: | Astronomy & Astrophysics |
| Témata: | |
| On-line přístup: | https://www.aanda.org/articles/aa/full_html/2026/06/aa59897-26/aa59897-26.html |
| Tagy: |
Žádné tagy, Buďte první, kdo vytvoří štítek k tomuto záznamu!
|