dc.contributor.author
Geilert, Sonja
dc.contributor.author
Albers, Elmar
dc.contributor.author
Frick, Daniel A.
dc.contributor.author
Hansen, Christian T.
dc.contributor.author
Blanckenburg, Friedhelm von
dc.date.accessioned
2021-11-29T10:08:27Z
dc.date.available
2021-11-29T10:08:27Z
dc.identifier.uri
https://refubium.fu-berlin.de/handle/fub188/32888
dc.identifier.uri
http://dx.doi.org/10.17169/refubium-32614
dc.description.abstract
The Mariana forearc is a unique location for exploring the role serpentinization plays in the marine Si cycle by means of Si stable isotope variations. Here, active mud volcanism transports deep, serpentinized mantle wedge material to the surface and thus offers a natural window to slab dehydration processes in dependence of changing temperature and pressure with depth. Si isotopes were measured in situby femtosecond laser ablation MC-ICPMS in serpentine within ultramafic clasts from three mud volcanoes (Yinazao, Fantangisna, and Asut Tesoru) sampled during International Ocean Discovery Program Expedition 366. To corroborate the results, serpentinization of olivine was studied in batch experiments. The Si isotope ratios show large variations between the mud volcanoes and between individual serpentine generations within a given mud volcano. Serpentine that formed early under low water/rock ratios exhibits delta Si-30 of -0.41 +/- 0.04 parts per thousand (1SD) similar to unaltered olivine which agrees well with experimental findings predicting no significant isotope fractionation during early serpentinization. In contrast, late serpentine veins formed under higher water/rock ratios span a wide range of Si isotope ratios that differ significantly between the individual mud volcanoes. With increasing distance to the trench, delta Si-30 of late veins are -0.10 +/- 0.07 parts per thousand, -1.94 +/- 0.13 parts per thousand, and -0.80 +/- 0.22 parts per thousand and -0.93 +/- 0.21 parts per thousand. These delta Si-30 values are interpreted to record the isotopic composition of the fluid source, namely subducted biogenic silica and pore fluids, clays, and altered oceanic crust that dehydrate as consequence of rising pressure and temperature with depth. We show that Si isotopes of mantle wedge serpentinites can be used as a reliable new proxy for slab dehydration processes. They may be used in paleo-forearc systems to unravel oceanic sediment and silica biomineralization evolution through geological time.
en
dc.format.extent
13 Seiten
dc.rights.uri
https://creativecommons.org/licenses/by/4.0/
dc.subject
Mariana forearc
en
dc.subject
serpentinization
en
dc.subject
in situ Si isotopes
en
dc.subject
slab dehydration
en
dc.subject
sediment proxy
en
dc.subject.ddc
500 Naturwissenschaften und Mathematik::550 Geowissenschaften, Geologie::550 Geowissenschaften
dc.title
Systematic changes in serpentine Si isotope signatures across the Mariana forearc – a new proxy for slab dehydration processes
dc.type
Wissenschaftlicher Artikel
dcterms.bibliographicCitation.articlenumber
117193
dcterms.bibliographicCitation.doi
10.1016/j.epsl.2021.117193
dcterms.bibliographicCitation.journaltitle
Earth and Planetary Science Letters
dcterms.bibliographicCitation.volume
575
dcterms.bibliographicCitation.url
https://doi.org/10.1016/j.epsl.2021.117193
refubium.affiliation
Geowissenschaften
refubium.affiliation.other
Institut für Geologische Wissenschaften / Fachrichtung Geochemie, Hydrogeologie, Mineralogie

refubium.resourceType.isindependentpub
no
dcterms.accessRights.openaire
open access
dcterms.isPartOf.eissn
1385-013X
refubium.resourceType.provider
WoS-Alert