Corrigendum to “Serpentinite fluids and slab-melting in the Aleutian arc: Evidence from molybdenum isotopes and boron systematics” [Earth and Planetary Science Letters, Volume 603, 2023, 1-12/117970]

0579213 - GLÚ 2025 RIV NL eng J - Journal Article
Rojas-Kolomiets, E. - Jensen, O. - Bizimis, M. - Yogodzinski, G. - Ackerman, Lukáš
Corrigendum to “Serpentinite fluids and slab-melting in the Aleutian arc: Evidence from molybdenum isotopes and boron systematics” [Earth and Planetary Science Letters, Volume 603, 2023, 1-12/117970].
Earth and Planetary Science Letters. Roč. 625, 1 January 2024 (2024), č. článku 118474. ISSN 0012-821X. E-ISSN 1385-013X
Institutional support: RVO:67985831
Keywords : molybdenum isotopes * boron * subduction zones * arc magmas * serpentinite fluids * sediments
OECD category: Geology
Impact factor: 5.3, year: 2022
Method of publishing: Limited access
https://www.sciencedirect.com/science/article/pii/S0012821X23004879

After publication of our paper Rojas-Kolomiets et al. (2023), we discovered that Aleutian lavas powdered in the University of South Carolina between 2004 and 2009 were contaminated with Mo. The issue was discovered in June-July 2023 when we re-powdered a subset of samples twice by grinding them in agate containers in a planetary ball mill and in tungsten carbide containers in a benchtop ring mill. Analyses of both sets of new rock powders showed significantly lower Mo concentrations than data from Rojas-Kolomiets et al. (2023). We subsequently re-powdered and re-analyzed all samples that were originally prepared at the University of South Carolina following the methods outlined in the paper. This included all samples from Rojas-Kolomiets et al. (2023) except those from the Korovin, Seguam and Yunaska locations. Despite this issue, most of our conclusions (particularly the presence of serpentinite-derived fluids in Aleutian lavas near the Amlia Fracture Zone) remain unchanged, and only one ought to be slightly modified.
Permanent Link: https://hdl.handle.net/11104/0348874