Semi-analytical Model for the Dynamical Evolution of Planetary Systems via Giant Impacts
In the standard model of terrestrial planet formation, planets are formed through giant impacts of planetary embryos after the dispersal of the protoplanetary gas disk. Traditionally, N -body simulations have been used to investigate this process. However, they are computationally too expensive to g...
| الحاوية / القاعدة: | The Astrophysical Journal |
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| المؤلفون الرئيسيون: | , , , , |
| التنسيق: | مقال |
| اللغة: | الإنجليزية |
| منشور في: |
IOP Publishing
2025-01-01
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| الموضوعات: | |
| الوصول للمادة أونلاين: | https://doi.org/10.3847/1538-4357/ade992 |