Weak S-type asteroids compared to C-type explain the observed size distribution of the main belt
The main belt, the region between the orbits of Mars and Jupiter, is home to more than 1 million asteroids. These asteroids form orbital groups, (i.e., asteroid families formed by collisions) and also spectral groups (taxonomies) with different chemical compositions, in particular carbonaceous (C-ty...
-д хадгалсан:
| Үндсэн зохиолчид: | , |
|---|---|
| Формат: | Artigo |
| Хэл сонгох: | Inglês |
| Хэвлэсэн: |
EDP Sciences
2026-03-01
|
| Цуврал: | Astronomy & Astrophysics |
| Нөхцлүүд: | |
| Онлайн хандалт: | https://www.aanda.org/articles/aa/full_html/2026/03/aa57725-25/aa57725-25.html |
| Шошгууд: |
Шошго байхгүй, Энэхүү баримтыг шошголох эхний хүн болох!
|