TY - JOUR
T1 - Noble gas isotopic compositions of seamount lavas from the central Chile trench
T2 - Implications for petit-spot volcanism and the lithosphere asthenosphere boundary
AU - Yamamoto, Junji
AU - Hirano, Naoto
AU - Kurz, Mark D.
N1 - Funding Information:
The manuscript benefited from comments by D. Graham and an anonymous reviewer. We appreciate Joshua Curtice for his assistance in analyzing noble gases. We also thank the crews and the scientific party of R/V Mirai's MR08-06 cruise. This study was supported by Grants-in-Aid for Scientific Research (Nos. 20H02000 , 18H03733 , 17K05715 , and 16H04079 ) from the Japan Society for the Promotion of Science .
Publisher Copyright:
© 2020
PY - 2020/12/15
Y1 - 2020/12/15
N2 - We report new noble gas isotopic compositions of submarine basaltic glasses sampled from two seamounts discovered offshore of Chile, and inferred to have erupted as petit-spot volcanoes near the Juan Fernández hotspot. The samples have 3He/4He of 1–15 times atmosphere (Ra). Their neon isotope compositions are similar to those of the Hawaiian Islands and Réunion Island. Their 40Ar/36Ar range from atmospheric to 2300. Although the lavas are likely to be influenced by a hotspot-related component, the cause of the 3He/4He variation must be clarified to ascertain the mantle source. Variations in 3He/4He are not attributable to processes occurring at the Earth's surface such as degassing fractionation, mixing with atmosphere dissolved in seawater, or in-situ post-eruptive addition of 4He. A combination of the Ne-Ar isotope ratios corrected for atmospheric influence and He isotope ratios indicates that the noble gas isotopes of the lavas are a mixture of a hotspot magma, MORB-source, and radiogenic components. The lower 3He/4He are attributed to assimilation with the oceanic lithosphere, suggesting that the pristine 3He/4He of the lavas is hotspot-like. These features can be interpreted as indicating that part of the Juan Fernández plume infiltrated the lithosphere–asthenosphere boundary (LAB), and that the ponding magma has erupted as petit-spot volcanoes because of plate bending. The noble gas data indicate that LAB can be a reservoir for exotic melts, which might have lubricated plate tectonics.
AB - We report new noble gas isotopic compositions of submarine basaltic glasses sampled from two seamounts discovered offshore of Chile, and inferred to have erupted as petit-spot volcanoes near the Juan Fernández hotspot. The samples have 3He/4He of 1–15 times atmosphere (Ra). Their neon isotope compositions are similar to those of the Hawaiian Islands and Réunion Island. Their 40Ar/36Ar range from atmospheric to 2300. Although the lavas are likely to be influenced by a hotspot-related component, the cause of the 3He/4He variation must be clarified to ascertain the mantle source. Variations in 3He/4He are not attributable to processes occurring at the Earth's surface such as degassing fractionation, mixing with atmosphere dissolved in seawater, or in-situ post-eruptive addition of 4He. A combination of the Ne-Ar isotope ratios corrected for atmospheric influence and He isotope ratios indicates that the noble gas isotopes of the lavas are a mixture of a hotspot magma, MORB-source, and radiogenic components. The lower 3He/4He are attributed to assimilation with the oceanic lithosphere, suggesting that the pristine 3He/4He of the lavas is hotspot-like. These features can be interpreted as indicating that part of the Juan Fernández plume infiltrated the lithosphere–asthenosphere boundary (LAB), and that the ponding magma has erupted as petit-spot volcanoes because of plate bending. The noble gas data indicate that LAB can be a reservoir for exotic melts, which might have lubricated plate tectonics.
KW - crustal assimilation
KW - Juan Fernández Islands
KW - lithosphere–asthenosphere boundary
KW - noble gas isotopic ratio
KW - petit-spot
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U2 - 10.1016/j.epsl.2020.116611
DO - 10.1016/j.epsl.2020.116611
M3 - Article
AN - SCOPUS:85092043278
SN - 0012-821X
VL - 552
JO - Earth and Planetary Science Letters
JF - Earth and Planetary Science Letters
M1 - 116611
ER -