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PROTOSOLAR AMMONIA AS THE UNIQUE SOURCE OF TITAN’s NITROGEN
The origin of Titan’s nitrogen-rich atmosphere is thought to be ammonia ice, but this has not yet been confirmed. Furthermore, it is uncertain whether the building blocks of Titan formed within the Saturnian subnebula or in the colder protosolar nebula (PSN). Recent measurements of the nitrogen isot...
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| 發表在: | Astrophys J Lett |
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| Main Authors: | , , , |
| 格式: | Artigo |
| 語言: | Inglês |
| 出版: |
2014
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| 主題: | |
| 在線閱讀: | https://ncbi.nlm.nih.gov/pmc/articles/PMC6501209/ https://ncbi.nlm.nih.gov/pubmed/31069045 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1088/2041-8205/788/2/L24 |
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