Pb isotope insight into the formation of the Earth's first stable continents

The formation of stable buoyant continental crust during the Archaean Eon was fundamental in establishing the planet's geochemical reservoirs. However, the processes that created Earth's first continents and the timescales over which they formed are debated. Here, we report the Pb isotope...

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Main Authors: Hartnady, Michael, Kirkland, Christopher, Smithies, R. Hugh, Johnson, S.P., Johnson, Tim
Format: Journal Article
Language:English
Published: ELSEVIER 2022
Subjects:
Online Access:http://purl.org/au-research/grants/arc/DP200101104
http://hdl.handle.net/20.500.11937/90872
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author Hartnady, Michael
Kirkland, Christopher
Smithies, R. Hugh
Johnson, S.P.
Johnson, Tim
author_facet Hartnady, Michael
Kirkland, Christopher
Smithies, R. Hugh
Johnson, S.P.
Johnson, Tim
author_sort Hartnady, Michael
building Curtin Institutional Repository
collection Online Access
description The formation of stable buoyant continental crust during the Archaean Eon was fundamental in establishing the planet's geochemical reservoirs. However, the processes that created Earth's first continents and the timescales over which they formed are debated. Here, we report the Pb isotope compositions of K-feldspar grains from 52 Paleoarchaean to Neoarchaean granites from the Pilbara Craton in Western Australia, one of the world's oldest and best-preserved granite–greenstone terranes. The Pb isotope composition of the Pilbara K-feldspars is variable, implying the granites were derived from crustal precursors of different age and/or variable time-integrated 238U/204Pb and 232Th/204Pb compositions. Trends to sub-mantle 207Pb/206Pb ratios preclude the influence of 4.3 Ga crustal precursors. In order to estimate crustal residence times we derive equations to calculate source model ages in a linearized Pb isotope evolution system. The best agreement between the feldspar Pb two-stage source model ages and those derived from zircon initial Hf isotope compositions requires crustal precursors that separated from a chondritic mantle source between 3.2 and 3.8 Ga, and rapidly differentiated to continental crust with 238U/204Pb and 232Th/238U ratios of ∼14 and 4.2–4.5, respectively. The preservation of Pb isotope variability in the Pilbara Paleoarchaean granites indicates their early continental source rocks were preserved for up to 500 Ma after their formation. The apparent longevity of these early continental nuclei is consistent with the incipient development of buoyant melt-depleted cratonic lithosphere during the Eoarchaean to Paleoarchaean.
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spelling curtin-20.500.11937-908722023-05-09T04:24:30Z Pb isotope insight into the formation of the Earth's first stable continents Hartnady, Michael Kirkland, Christopher Smithies, R. Hugh Johnson, S.P. Johnson, Tim Science & Technology Physical Sciences Geochemistry & Geophysics early Earth Pb isotopes crustal evolution Pilbara Craton Eoarchaean MC-ICP-MS IN-SITU ANALYSIS PILBARA CRATON HF ISOTOPES OXYGEN ISOTOPES CORE FORMATION LU-HF CRUST ZIRCON CONSTRAINTS The formation of stable buoyant continental crust during the Archaean Eon was fundamental in establishing the planet's geochemical reservoirs. However, the processes that created Earth's first continents and the timescales over which they formed are debated. Here, we report the Pb isotope compositions of K-feldspar grains from 52 Paleoarchaean to Neoarchaean granites from the Pilbara Craton in Western Australia, one of the world's oldest and best-preserved granite–greenstone terranes. The Pb isotope composition of the Pilbara K-feldspars is variable, implying the granites were derived from crustal precursors of different age and/or variable time-integrated 238U/204Pb and 232Th/204Pb compositions. Trends to sub-mantle 207Pb/206Pb ratios preclude the influence of 4.3 Ga crustal precursors. In order to estimate crustal residence times we derive equations to calculate source model ages in a linearized Pb isotope evolution system. The best agreement between the feldspar Pb two-stage source model ages and those derived from zircon initial Hf isotope compositions requires crustal precursors that separated from a chondritic mantle source between 3.2 and 3.8 Ga, and rapidly differentiated to continental crust with 238U/204Pb and 232Th/238U ratios of ∼14 and 4.2–4.5, respectively. The preservation of Pb isotope variability in the Pilbara Paleoarchaean granites indicates their early continental source rocks were preserved for up to 500 Ma after their formation. The apparent longevity of these early continental nuclei is consistent with the incipient development of buoyant melt-depleted cratonic lithosphere during the Eoarchaean to Paleoarchaean. 2022 Journal Article http://hdl.handle.net/20.500.11937/90872 10.1016/j.epsl.2021.117319 English http://purl.org/au-research/grants/arc/DP200101104 http://purl.org/au-research/grants/arc/LP180100199 http://creativecommons.org/licenses/by/4.0/ ELSEVIER fulltext
spellingShingle Science & Technology
Physical Sciences
Geochemistry & Geophysics
early Earth
Pb isotopes
crustal evolution
Pilbara Craton
Eoarchaean
MC-ICP-MS
IN-SITU ANALYSIS
PILBARA CRATON
HF ISOTOPES
OXYGEN ISOTOPES
CORE FORMATION
LU-HF
CRUST
ZIRCON
CONSTRAINTS
Hartnady, Michael
Kirkland, Christopher
Smithies, R. Hugh
Johnson, S.P.
Johnson, Tim
Pb isotope insight into the formation of the Earth's first stable continents
title Pb isotope insight into the formation of the Earth's first stable continents
title_full Pb isotope insight into the formation of the Earth's first stable continents
title_fullStr Pb isotope insight into the formation of the Earth's first stable continents
title_full_unstemmed Pb isotope insight into the formation of the Earth's first stable continents
title_short Pb isotope insight into the formation of the Earth's first stable continents
title_sort pb isotope insight into the formation of the earth's first stable continents
topic Science & Technology
Physical Sciences
Geochemistry & Geophysics
early Earth
Pb isotopes
crustal evolution
Pilbara Craton
Eoarchaean
MC-ICP-MS
IN-SITU ANALYSIS
PILBARA CRATON
HF ISOTOPES
OXYGEN ISOTOPES
CORE FORMATION
LU-HF
CRUST
ZIRCON
CONSTRAINTS
url http://purl.org/au-research/grants/arc/DP200101104
http://purl.org/au-research/grants/arc/DP200101104
http://hdl.handle.net/20.500.11937/90872