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Terrestrial planet and asteroid belt formation by Jupiter–Saturn chaotic excitation
The terrestrial planets formed by accretion of asteroid-like objects within the inner solar system’s protoplanetary disk. Previous works have found that forming a small-mass Mars requires the disk to contain little mass beyond ~ 1.5 au (i.e., the disk mass was concentrated within this boundary). The...
| Autores principales: | , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
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Nature Publishing Group UK
2023
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| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10042868/ https://www.ncbi.nlm.nih.gov/pubmed/36973305 http://dx.doi.org/10.1038/s41598-023-30382-9 |