dc.contributor
Lehmann, Elfrun
dc.creator
Archer, Gregory J.
dc.creator
Brennecka, Gregory A.
dc.creator
Stracke, Andreas
dc.creator
Kleine, Thorsten
dc.date.accessioned
2023-05-23T15:19:57Z
dc.date.available
2023-05-23T15:19:57Z
dc.identifier
https://doi.org/10.35003/F0ITDI
dc.identifier.uri
https://refubium.fu-berlin.de/handle/fub188/39451
dc.identifier.uri
http://dx.doi.org/10.17169/refubium-39168
dc.description
• 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.
dc.subject
Earth and Environmental Sciences
dc.subject
Tungsten isotopes
dc.subject
Pilbara Craton
dc.title
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
dcterms.accessRights.openaire
metadata only access
