Replication Data for: Lack of late-accreted material as the origin of 182W excesses in the Archean mantle: Evidence from the Pilbara Craton, Western Australia
收藏DataCite Commons2023-04-14 更新2025-04-15 收录
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https://planetary-data-portal.org/citation?persistentId=doi:10.35003/F0ITDI
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资源简介：
• 182W and HSE indicate partial lack late-accreted material in Pilbara source. • Only of normal amount of late-accreted material present at 3.3 Ga. • Similar 182W characteristics of other mantle sources indicates common process. • 182W–HSE mismatch for other sources caused by dissimilar behaviors of HSE vs. W. • Moon and pre-late accretion BSE had similar 182W.
提供机构：
TRR170-DB
创建时间：
2021-01-19
