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The origin of inner Solar System water
Of the potential volatile sources for the terrestrial planets, the CI and CM carbonaceous chondrites are closest to the planets' bulk H and N isotopic compositions. For the Earth, the addition of approximately 2–4 wt% of CI/CM material to a volatile-depleted proto-Earth can explain the abundanc...
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| Argitaratua izan da: | Philos Trans A Math Phys Eng Sci |
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| Egile nagusia: | |
| Formatua: | Artigo |
| Hizkuntza: | Inglês |
| Argitaratua: |
The Royal Society Publishing
2017
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| Sarrera elektronikoa: | https://ncbi.nlm.nih.gov/pmc/articles/PMC5394251/ https://ncbi.nlm.nih.gov/pubmed/28416723 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1098/rsta.2015.0384 |
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