Titanium and iron isotopic records of granitoid crust production in diverse Archean cratons

Archean granitoid provides critical clues on how Earth's felsic crust was established and its geodynamics evolved. In this study, we present Fe-Ti isotope and trace-element data for granitoids (mostly TTGs) from the ∼3.8-3.6 Ga Itsaq Gneiss Complex and ∼3.3 Ga East Pilbara Terrane, Pilbara Crat...

Full description

Bibliographic Details
Published in:Earth and Planetary Science Letters
Main Authors: Zhang, Zhe J., Dauphas, Nicolas, Johnson, Aleisha C., Aarons, Sarah M., Bennett, Vickie C., Nutman, Allen P., MacLennan, Scott, Schoene, Blair
Format: Text
Language:unknown
Published: Research Online 2023
Subjects:
TTG
Online Access:https://ro.uow.edu.au/test2021/9171
https://doi.org/10.1016/j.epsl.2023.118342
id ftunivwollongong:oai:ro.uow.edu.au:test2021-14718
record_format openpolar
spelling ftunivwollongong:oai:ro.uow.edu.au:test2021-14718 2023-10-09T21:52:02+02:00 Titanium and iron isotopic records of granitoid crust production in diverse Archean cratons Zhang, Zhe J. Dauphas, Nicolas Johnson, Aleisha C. Aarons, Sarah M. Bennett, Vickie C. Nutman, Allen P. MacLennan, Scott Schoene, Blair 2023-10-15T07:00:00Z https://ro.uow.edu.au/test2021/9171 https://doi.org/10.1016/j.epsl.2023.118342 unknown Research Online https://ro.uow.edu.au/test2021/9171 doi:10.1016/j.epsl.2023.118342 https://doi.org/10.1016/j.epsl.2023.118342 Scopus Harvesting Series Archean continental crust Ti isotopes TTG text 2023 ftunivwollongong https://doi.org/10.1016/j.epsl.2023.118342 2023-09-18T22:24:48Z Archean granitoid provides critical clues on how Earth's felsic crust was established and its geodynamics evolved. In this study, we present Fe-Ti isotope and trace-element data for granitoids (mostly TTGs) from the ∼3.8-3.6 Ga Itsaq Gneiss Complex and ∼3.3 Ga East Pilbara Terrane, Pilbara Craton. TTGs from those localities and several other cratons follow the same Ti isotopic fractionation trend as modern calc-alkaline rocks. This similarity hides important petrogenetic differences as partial melting could have played a much more important role in establishing the felsic character of TTGs compared to modern granites of calc-alkaline affinity. Our thermodynamics-based modeling of isotopic fractionation shows that partial melting of hydrated metabasite can explain the Fe and Ti isotopic compositions of many TTGs but reworking of tonalite crust is needed to explain the most extreme compositions. The same Ti isotopic fractionation trends have been found now in several cratons (West Greenland, Slave, Pilbara, and Kaapvaal cratons) in granitoids formed in different geothermal gradients, meaning that it was likely a global signature of the Archean crust. Sediment provenance studies that use those TTG compositions and point to a primarily felsic crust in the Archean are therefore valid. Text Greenland University of Wollongong, Australia: Research Online Greenland Earth and Planetary Science Letters 620 118342
institution Open Polar
collection University of Wollongong, Australia: Research Online
op_collection_id ftunivwollongong
language unknown
topic Archean
continental crust
Ti isotopes
TTG
spellingShingle Archean
continental crust
Ti isotopes
TTG
Zhang, Zhe J.
Dauphas, Nicolas
Johnson, Aleisha C.
Aarons, Sarah M.
Bennett, Vickie C.
Nutman, Allen P.
MacLennan, Scott
Schoene, Blair
Titanium and iron isotopic records of granitoid crust production in diverse Archean cratons
topic_facet Archean
continental crust
Ti isotopes
TTG
description Archean granitoid provides critical clues on how Earth's felsic crust was established and its geodynamics evolved. In this study, we present Fe-Ti isotope and trace-element data for granitoids (mostly TTGs) from the ∼3.8-3.6 Ga Itsaq Gneiss Complex and ∼3.3 Ga East Pilbara Terrane, Pilbara Craton. TTGs from those localities and several other cratons follow the same Ti isotopic fractionation trend as modern calc-alkaline rocks. This similarity hides important petrogenetic differences as partial melting could have played a much more important role in establishing the felsic character of TTGs compared to modern granites of calc-alkaline affinity. Our thermodynamics-based modeling of isotopic fractionation shows that partial melting of hydrated metabasite can explain the Fe and Ti isotopic compositions of many TTGs but reworking of tonalite crust is needed to explain the most extreme compositions. The same Ti isotopic fractionation trends have been found now in several cratons (West Greenland, Slave, Pilbara, and Kaapvaal cratons) in granitoids formed in different geothermal gradients, meaning that it was likely a global signature of the Archean crust. Sediment provenance studies that use those TTG compositions and point to a primarily felsic crust in the Archean are therefore valid.
format Text
author Zhang, Zhe J.
Dauphas, Nicolas
Johnson, Aleisha C.
Aarons, Sarah M.
Bennett, Vickie C.
Nutman, Allen P.
MacLennan, Scott
Schoene, Blair
author_facet Zhang, Zhe J.
Dauphas, Nicolas
Johnson, Aleisha C.
Aarons, Sarah M.
Bennett, Vickie C.
Nutman, Allen P.
MacLennan, Scott
Schoene, Blair
author_sort Zhang, Zhe J.
title Titanium and iron isotopic records of granitoid crust production in diverse Archean cratons
title_short Titanium and iron isotopic records of granitoid crust production in diverse Archean cratons
title_full Titanium and iron isotopic records of granitoid crust production in diverse Archean cratons
title_fullStr Titanium and iron isotopic records of granitoid crust production in diverse Archean cratons
title_full_unstemmed Titanium and iron isotopic records of granitoid crust production in diverse Archean cratons
title_sort titanium and iron isotopic records of granitoid crust production in diverse archean cratons
publisher Research Online
publishDate 2023
url https://ro.uow.edu.au/test2021/9171
https://doi.org/10.1016/j.epsl.2023.118342
geographic Greenland
geographic_facet Greenland
genre Greenland
genre_facet Greenland
op_source Scopus Harvesting Series
op_relation https://ro.uow.edu.au/test2021/9171
doi:10.1016/j.epsl.2023.118342
https://doi.org/10.1016/j.epsl.2023.118342
op_doi https://doi.org/10.1016/j.epsl.2023.118342
container_title Earth and Planetary Science Letters
container_volume 620
container_start_page 118342
_version_ 1779315154830229504