Forming Mercury from Excited Initial Conditions
Mercury is notoriously difficult to form in Solar System simulations, due to its small mass and iron-rich composition. Smooth particle hydrodynamics simulations of collisions have found that a Mercury-like body could be formed by one or multiple giant impacts, but due to the chaotic nature of collis...
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| Главные авторы: | , , , |
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| Формат: | Artigo |
| Язык: | Inglês |
| Опубликовано: |
IOP Publishing
2024-01-01
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| Серии: | The Astrophysical Journal |
| Предметы: | |
| Online-ссылка: | https://doi.org/10.3847/1538-4357/ad39e6 |
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