Nitrogen isotope evidence for Earth’s heterogeneous accretion of volatiles
How and when Earth acquired its major volatiles N-C-H-S remains unclear. Here the authors show that Earth may have acquired its major volatiles from both reduced and oxidized impactors before and during the Moon-forming giant impact.
Autors principals: | Lanlan Shi, Wenhua Lu, Takanori Kagoshima, Yuji Sano, Zenghao Gao, Zhixue Du, Yun Liu, Yingwei Fei, Yuan Li |
---|---|
Format: | Article |
Idioma: | English |
Publicat: |
Nature Portfolio
2022-08-01
|
Col·lecció: | Nature Communications |
Accés en línia: | https://doi.org/10.1038/s41467-022-32516-5 |
Ítems similars
-
Volatile accretion history of the Earth.
per: Wood, B, et al.
Publicat: (2010) -
Thallium isotope constraints on Earth's accretion
per: Baker, R, et al.
Publicat: (2007) -
Isotopic evidence for internal oxidation of the Earth's mantle during accretion
per: Williams, H, et al.
Publicat: (2012) -
NanoSIMS Analysis of Rare Earth Elements in Silicate Glass and Zircon: Implications for Partition Coefficients
per: Lanlan Shi, et al.
Publicat: (2022-03-01) -
Implications of Differentiated Late Accretion for the Volatile Inventory of the Bulk Silicate Earth
per: Damanveer S. Grewal, et al.
Publicat: (2025-01-01)