The Hadean–Archaean transition at 4 Ga: From magma trapping in the mantle to volcanic resurfacing of the Earth
The Hadean–Archaean transition is poorly known because of the dearth of Hadean rocks. A new conceptual model is presented based on variations in mantle potential temperature ( T p ) with time. The critical issue is the depth of melting with respect to a negatively buoyant magma sink between 410 and...
Ausführliche Beschreibung
Autor*in: |
Nédélec, Anne [verfasserIn] |
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Format: |
Artikel |
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Sprache: |
Englisch |
Erschienen: |
2017 |
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Rechteinformationen: |
Nutzungsrecht: © 2017 John Wiley & Sons Ltd |
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Systematik: |
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Übergeordnetes Werk: |
Enthalten in: Terra nova - Oxford : Blackwell Scientific Publ., 1989, 29(2017), 4, Seite 218-223 |
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Übergeordnetes Werk: |
volume:29 ; year:2017 ; number:4 ; pages:218-223 |
Links: |
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DOI / URN: |
10.1111/ter.12266 |
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10.1111/ter.12266 doi PQ20171228 (DE-627)OLC1996281917 (DE-599)GBVOLC1996281917 (PRQ)w766-cf4d05de2be3e98b523253451fbda5ae07fdd06af916444eae72b47a5e17c0c40 (KEY)0178714420170000029000400218hadeanarchaeantransitionat4gafrommagmatrappinginth DE-627 ger DE-627 rakwb eng 550 DNB TE 1000 AVZ rvk Nédélec, Anne verfasserin aut The Hadean–Archaean transition at 4 Ga: From magma trapping in the mantle to volcanic resurfacing of the Earth 2017 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The Hadean–Archaean transition is poorly known because of the dearth of Hadean rocks. A new conceptual model is presented based on variations in mantle potential temperature ( T p ) with time. The critical issue is the depth of melting with respect to a negatively buoyant magma sink between 410 and 330 km (14–11 GP a). Hadean plume magmatism begins below the magma sink, leading to generation of a refractory upper mantle reservoir and the minor production of boninite‐like magmas near the surface. With cooling, the onset of melting migrates above the magma sink, a situation likely occurring since 3.9 Ga and corresponding to T p s of ~1870°C or less. Therefore, a burst of mafic to ultramafic volcanism was produced at 3.9–3.8 Ga. This extensive volcanism may have triggered gravitational instabilities and favoured the recycling of the Hadean crust into the mantle. Results of this model are discussed in the light of existing isotopic data. Nutzungsrecht: © 2017 John Wiley & Sons Ltd Monnereau, Marc oth Toplis, Michael J oth Enthalten in Terra nova Oxford : Blackwell Scientific Publ., 1989 29(2017), 4, Seite 218-223 (DE-627)130758817 (DE-600)1000080-X (DE-576)023035099 0954-4879 nnns volume:29 year:2017 number:4 pages:218-223 http://dx.doi.org/10.1111/ter.12266 Volltext http://onlinelibrary.wiley.com/doi/10.1111/ter.12266/abstract GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OPC-GGO SSG-OPC-GEO GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_4112 TE 1000 AR 29 2017 4 218-223 |
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10.1111/ter.12266 doi PQ20171228 (DE-627)OLC1996281917 (DE-599)GBVOLC1996281917 (PRQ)w766-cf4d05de2be3e98b523253451fbda5ae07fdd06af916444eae72b47a5e17c0c40 (KEY)0178714420170000029000400218hadeanarchaeantransitionat4gafrommagmatrappinginth DE-627 ger DE-627 rakwb eng 550 DNB TE 1000 AVZ rvk Nédélec, Anne verfasserin aut The Hadean–Archaean transition at 4 Ga: From magma trapping in the mantle to volcanic resurfacing of the Earth 2017 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The Hadean–Archaean transition is poorly known because of the dearth of Hadean rocks. A new conceptual model is presented based on variations in mantle potential temperature ( T p ) with time. The critical issue is the depth of melting with respect to a negatively buoyant magma sink between 410 and 330 km (14–11 GP a). Hadean plume magmatism begins below the magma sink, leading to generation of a refractory upper mantle reservoir and the minor production of boninite‐like magmas near the surface. With cooling, the onset of melting migrates above the magma sink, a situation likely occurring since 3.9 Ga and corresponding to T p s of ~1870°C or less. Therefore, a burst of mafic to ultramafic volcanism was produced at 3.9–3.8 Ga. This extensive volcanism may have triggered gravitational instabilities and favoured the recycling of the Hadean crust into the mantle. Results of this model are discussed in the light of existing isotopic data. Nutzungsrecht: © 2017 John Wiley & Sons Ltd Monnereau, Marc oth Toplis, Michael J oth Enthalten in Terra nova Oxford : Blackwell Scientific Publ., 1989 29(2017), 4, Seite 218-223 (DE-627)130758817 (DE-600)1000080-X (DE-576)023035099 0954-4879 nnns volume:29 year:2017 number:4 pages:218-223 http://dx.doi.org/10.1111/ter.12266 Volltext http://onlinelibrary.wiley.com/doi/10.1111/ter.12266/abstract GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OPC-GGO SSG-OPC-GEO GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_4112 TE 1000 AR 29 2017 4 218-223 |
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10.1111/ter.12266 doi PQ20171228 (DE-627)OLC1996281917 (DE-599)GBVOLC1996281917 (PRQ)w766-cf4d05de2be3e98b523253451fbda5ae07fdd06af916444eae72b47a5e17c0c40 (KEY)0178714420170000029000400218hadeanarchaeantransitionat4gafrommagmatrappinginth DE-627 ger DE-627 rakwb eng 550 DNB TE 1000 AVZ rvk Nédélec, Anne verfasserin aut The Hadean–Archaean transition at 4 Ga: From magma trapping in the mantle to volcanic resurfacing of the Earth 2017 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The Hadean–Archaean transition is poorly known because of the dearth of Hadean rocks. A new conceptual model is presented based on variations in mantle potential temperature ( T p ) with time. The critical issue is the depth of melting with respect to a negatively buoyant magma sink between 410 and 330 km (14–11 GP a). Hadean plume magmatism begins below the magma sink, leading to generation of a refractory upper mantle reservoir and the minor production of boninite‐like magmas near the surface. With cooling, the onset of melting migrates above the magma sink, a situation likely occurring since 3.9 Ga and corresponding to T p s of ~1870°C or less. Therefore, a burst of mafic to ultramafic volcanism was produced at 3.9–3.8 Ga. This extensive volcanism may have triggered gravitational instabilities and favoured the recycling of the Hadean crust into the mantle. Results of this model are discussed in the light of existing isotopic data. Nutzungsrecht: © 2017 John Wiley & Sons Ltd Monnereau, Marc oth Toplis, Michael J oth Enthalten in Terra nova Oxford : Blackwell Scientific Publ., 1989 29(2017), 4, Seite 218-223 (DE-627)130758817 (DE-600)1000080-X (DE-576)023035099 0954-4879 nnns volume:29 year:2017 number:4 pages:218-223 http://dx.doi.org/10.1111/ter.12266 Volltext http://onlinelibrary.wiley.com/doi/10.1111/ter.12266/abstract GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OPC-GGO SSG-OPC-GEO GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_4112 TE 1000 AR 29 2017 4 218-223 |
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10.1111/ter.12266 doi PQ20171228 (DE-627)OLC1996281917 (DE-599)GBVOLC1996281917 (PRQ)w766-cf4d05de2be3e98b523253451fbda5ae07fdd06af916444eae72b47a5e17c0c40 (KEY)0178714420170000029000400218hadeanarchaeantransitionat4gafrommagmatrappinginth DE-627 ger DE-627 rakwb eng 550 DNB TE 1000 AVZ rvk Nédélec, Anne verfasserin aut The Hadean–Archaean transition at 4 Ga: From magma trapping in the mantle to volcanic resurfacing of the Earth 2017 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The Hadean–Archaean transition is poorly known because of the dearth of Hadean rocks. A new conceptual model is presented based on variations in mantle potential temperature ( T p ) with time. The critical issue is the depth of melting with respect to a negatively buoyant magma sink between 410 and 330 km (14–11 GP a). Hadean plume magmatism begins below the magma sink, leading to generation of a refractory upper mantle reservoir and the minor production of boninite‐like magmas near the surface. With cooling, the onset of melting migrates above the magma sink, a situation likely occurring since 3.9 Ga and corresponding to T p s of ~1870°C or less. Therefore, a burst of mafic to ultramafic volcanism was produced at 3.9–3.8 Ga. This extensive volcanism may have triggered gravitational instabilities and favoured the recycling of the Hadean crust into the mantle. Results of this model are discussed in the light of existing isotopic data. Nutzungsrecht: © 2017 John Wiley & Sons Ltd Monnereau, Marc oth Toplis, Michael J oth Enthalten in Terra nova Oxford : Blackwell Scientific Publ., 1989 29(2017), 4, Seite 218-223 (DE-627)130758817 (DE-600)1000080-X (DE-576)023035099 0954-4879 nnns volume:29 year:2017 number:4 pages:218-223 http://dx.doi.org/10.1111/ter.12266 Volltext http://onlinelibrary.wiley.com/doi/10.1111/ter.12266/abstract GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OPC-GGO SSG-OPC-GEO GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_4112 TE 1000 AR 29 2017 4 218-223 |
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hadean–archaean transition at 4 ga: from magma trapping in the mantle to volcanic resurfacing of the earth |
title_auth |
The Hadean–Archaean transition at 4 Ga: From magma trapping in the mantle to volcanic resurfacing of the Earth |
abstract |
The Hadean–Archaean transition is poorly known because of the dearth of Hadean rocks. A new conceptual model is presented based on variations in mantle potential temperature ( T p ) with time. The critical issue is the depth of melting with respect to a negatively buoyant magma sink between 410 and 330 km (14–11 GP a). Hadean plume magmatism begins below the magma sink, leading to generation of a refractory upper mantle reservoir and the minor production of boninite‐like magmas near the surface. With cooling, the onset of melting migrates above the magma sink, a situation likely occurring since 3.9 Ga and corresponding to T p s of ~1870°C or less. Therefore, a burst of mafic to ultramafic volcanism was produced at 3.9–3.8 Ga. This extensive volcanism may have triggered gravitational instabilities and favoured the recycling of the Hadean crust into the mantle. Results of this model are discussed in the light of existing isotopic data. |
abstractGer |
The Hadean–Archaean transition is poorly known because of the dearth of Hadean rocks. A new conceptual model is presented based on variations in mantle potential temperature ( T p ) with time. The critical issue is the depth of melting with respect to a negatively buoyant magma sink between 410 and 330 km (14–11 GP a). Hadean plume magmatism begins below the magma sink, leading to generation of a refractory upper mantle reservoir and the minor production of boninite‐like magmas near the surface. With cooling, the onset of melting migrates above the magma sink, a situation likely occurring since 3.9 Ga and corresponding to T p s of ~1870°C or less. Therefore, a burst of mafic to ultramafic volcanism was produced at 3.9–3.8 Ga. This extensive volcanism may have triggered gravitational instabilities and favoured the recycling of the Hadean crust into the mantle. Results of this model are discussed in the light of existing isotopic data. |
abstract_unstemmed |
The Hadean–Archaean transition is poorly known because of the dearth of Hadean rocks. A new conceptual model is presented based on variations in mantle potential temperature ( T p ) with time. The critical issue is the depth of melting with respect to a negatively buoyant magma sink between 410 and 330 km (14–11 GP a). Hadean plume magmatism begins below the magma sink, leading to generation of a refractory upper mantle reservoir and the minor production of boninite‐like magmas near the surface. With cooling, the onset of melting migrates above the magma sink, a situation likely occurring since 3.9 Ga and corresponding to T p s of ~1870°C or less. Therefore, a burst of mafic to ultramafic volcanism was produced at 3.9–3.8 Ga. This extensive volcanism may have triggered gravitational instabilities and favoured the recycling of the Hadean crust into the mantle. Results of this model are discussed in the light of existing isotopic data. |
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container_issue |
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title_short |
The Hadean–Archaean transition at 4 Ga: From magma trapping in the mantle to volcanic resurfacing of the Earth |
url |
http://dx.doi.org/10.1111/ter.12266 http://onlinelibrary.wiley.com/doi/10.1111/ter.12266/abstract |
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author2 |
Monnereau, Marc Toplis, Michael J |
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up_date |
2024-07-04T00:17:15.245Z |
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