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The empty primordial asteroid belt
The asteroid belt contains less than a thousandth of Earth’s mass and is radially segregated, with S-types dominating the inner belt and C-types the outer belt. It is generally assumed that the belt formed with far more mass and was later strongly depleted. We show that the present-day asteroid belt...
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| Publicat a: | Sci Adv |
|---|---|
| Autors principals: | , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
American Association for the Advancement of Science
2017
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| Matèries: | |
| Accés en línia: | https://ncbi.nlm.nih.gov/pmc/articles/PMC5597311/ https://ncbi.nlm.nih.gov/pubmed/28924609 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1126/sciadv.1701138 |
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