Effect of impactor oblateness on the formation of lunar simple craters
Context. Simple craters are ubiquitous on the Moon and are mainly formed by impactors of <1 km in diameter. Prevailing knowledge suggested that gravity-dominated simple craters follow uniform morphometric scaling, which is routinely employed to probe lunar subsurface structures and compositions. How...
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| Autori principali: | , , , , |
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| Natura: | Artigo |
| Lingua: | Inglês |
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EDP Sciences
2026-06-01
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| Serie: | Astronomy & Astrophysics |
| Soggetti: | |
| Accesso online: | https://www.aanda.org/articles/aa/full_html/2026/06/aa59315-26/aa59315-26.html |
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