Propagation of a melting anomaly along the ultraslow Southwest Indian Ridge between 46°E and 52°20′E: interaction with the Crozet hotspot?

International audience Regional axial depths, mantle Bouguer anomaly values, geochemical proxies for the extent of partial melting and tomographic models along the Southwest Indian Ridge (SWIR) all concur in indicating the presence of thicker crust and hotter mantle between the Indomed and Gallieni...

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Published in:Geophysical Journal International
Main Authors: Sauter, Daniel, Cannat, Mathilde, Meyzen, Christine, Bézos, Antoine, Patriat, Philippe, Humler, Eric, Debayle, Eric
Other Authors: Institut de physique du globe de Strasbourg (IPGS), Université de Strasbourg (UNISTRA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Géosciences Marines (LGM), Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Paris Diderot - Paris 7 (UPD7)-Institut de Physique du Globe de Paris (IPG Paris)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Sciences de la Terre (LST), École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Planétologie et Géodynamique de Nantes UMR 6112 (LPGN), Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2009
Subjects:
Online Access:https://insu.hal.science/insu-01828244
https://insu.hal.science/insu-01828244/document
https://insu.hal.science/insu-01828244/file/gji-sauter-2009-179-2-687.pdf
https://doi.org/10.1111/j.1365-246X.2009.04308.x
id ftsorbonneuniv:oai:HAL:insu-01828244v1
record_format openpolar
institution Open Polar
collection HAL Sorbonne Université
op_collection_id ftsorbonneuniv
language English
topic Magnetic anomalies: modelling and interpretation
Mid-ocean ridge processes
Hotspots
Indian Ocean
[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]
spellingShingle Magnetic anomalies: modelling and interpretation
Mid-ocean ridge processes
Hotspots
Indian Ocean
[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]
Sauter, Daniel
Cannat, Mathilde
Meyzen, Christine
Bézos, Antoine
Patriat, Philippe
Humler, Eric
Debayle, Eric
Propagation of a melting anomaly along the ultraslow Southwest Indian Ridge between 46°E and 52°20′E: interaction with the Crozet hotspot?
topic_facet Magnetic anomalies: modelling and interpretation
Mid-ocean ridge processes
Hotspots
Indian Ocean
[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]
description International audience Regional axial depths, mantle Bouguer anomaly values, geochemical proxies for the extent of partial melting and tomographic models along the Southwest Indian Ridge (SWIR) all concur in indicating the presence of thicker crust and hotter mantle between the Indomed and Gallieni transform faults (TFs; 46 • E and 52 • 20 E) relative to the neighbouring ridge sections. Accreted seafloor between these TFs over the past ∼10 Myr is also locally much shallower (>1000 m) and corresponds to thicker crust (>1.7 km) than previously accreted seafloor along the same ridge region. Two large outward facing topographic gradients mark the outer edges of two anomalously shallow off-axis domains on the African and Antarctic plates. Their vertical relief (>2000 m locally) and their geometry, parallel to the present-day axis along a >210-km-long ridge section, suggest an extremely sudden and large event dated between ∼8 (magnetic anomaly C4n) and ∼11 Ma (magnetic anomaly C5n). Asymmetric spreading and small ridge jumps occur at the onset of the formation of the anomalously shallow off-axis domains, leading to a reorganization of the ridge segmentation. We interpret these anomalously shallow off-axis domains as the relicts of a volcanic plateau due to a sudden increase of the magma supply. This event of enhanced magmatism started in the central part of the ridge section and then propagated along axis to the east and probably also to the west. However, it did not cross the Gallieni and Indomed TFs suggesting that large offsets can curtail or even block along-axis melt flow. We propose that this melting anomaly may be ascribed to a regionally higher mantle temperature provided by mantle outpouring from the Crozet hotspot towards the SWIR.
author2 Institut de physique du globe de Strasbourg (IPGS)
Université de Strasbourg (UNISTRA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Laboratoire de Géosciences Marines (LGM)
Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Paris Diderot - Paris 7 (UPD7)-Institut de Physique du Globe de Paris (IPG Paris)-Centre National de la Recherche Scientifique (CNRS)
Laboratoire de Sciences de la Terre (LST)
École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL)
Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Laboratoire de Planétologie et Géodynamique de Nantes UMR 6112 (LPGN)
Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)
format Article in Journal/Newspaper
author Sauter, Daniel
Cannat, Mathilde
Meyzen, Christine
Bézos, Antoine
Patriat, Philippe
Humler, Eric
Debayle, Eric
author_facet Sauter, Daniel
Cannat, Mathilde
Meyzen, Christine
Bézos, Antoine
Patriat, Philippe
Humler, Eric
Debayle, Eric
author_sort Sauter, Daniel
title Propagation of a melting anomaly along the ultraslow Southwest Indian Ridge between 46°E and 52°20′E: interaction with the Crozet hotspot?
title_short Propagation of a melting anomaly along the ultraslow Southwest Indian Ridge between 46°E and 52°20′E: interaction with the Crozet hotspot?
title_full Propagation of a melting anomaly along the ultraslow Southwest Indian Ridge between 46°E and 52°20′E: interaction with the Crozet hotspot?
title_fullStr Propagation of a melting anomaly along the ultraslow Southwest Indian Ridge between 46°E and 52°20′E: interaction with the Crozet hotspot?
title_full_unstemmed Propagation of a melting anomaly along the ultraslow Southwest Indian Ridge between 46°E and 52°20′E: interaction with the Crozet hotspot?
title_sort propagation of a melting anomaly along the ultraslow southwest indian ridge between 46°e and 52°20′e: interaction with the crozet hotspot?
publisher HAL CCSD
publishDate 2009
url https://insu.hal.science/insu-01828244
https://insu.hal.science/insu-01828244/document
https://insu.hal.science/insu-01828244/file/gji-sauter-2009-179-2-687.pdf
https://doi.org/10.1111/j.1365-246X.2009.04308.x
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
op_source ISSN: 0956-540X
EISSN: 1365-246X
Geophysical Journal International
https://insu.hal.science/insu-01828244
Geophysical Journal International, 2009, 179 (2), pp.687-699. ⟨10.1111/j.1365-246X.2009.04308.x⟩
op_relation info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-246X.2009.04308.x
insu-01828244
https://insu.hal.science/insu-01828244
https://insu.hal.science/insu-01828244/document
https://insu.hal.science/insu-01828244/file/gji-sauter-2009-179-2-687.pdf
doi:10.1111/j.1365-246X.2009.04308.x
op_rights info:eu-repo/semantics/OpenAccess
op_doi https://doi.org/10.1111/j.1365-246X.2009.04308.x
container_title Geophysical Journal International
container_volume 179
container_issue 2
container_start_page 687
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spelling ftsorbonneuniv:oai:HAL:insu-01828244v1 2024-09-15T17:47:47+00:00 Propagation of a melting anomaly along the ultraslow Southwest Indian Ridge between 46°E and 52°20′E: interaction with the Crozet hotspot? Sauter, Daniel Cannat, Mathilde Meyzen, Christine Bézos, Antoine Patriat, Philippe Humler, Eric Debayle, Eric Institut de physique du globe de Strasbourg (IPGS) Université de Strasbourg (UNISTRA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS) Laboratoire de Géosciences Marines (LGM) Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Paris Diderot - Paris 7 (UPD7)-Institut de Physique du Globe de Paris (IPG Paris)-Centre National de la Recherche Scientifique (CNRS) Laboratoire de Sciences de la Terre (LST) École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL) Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS) Laboratoire de Planétologie et Géodynamique de Nantes UMR 6112 (LPGN) Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS) 2009 https://insu.hal.science/insu-01828244 https://insu.hal.science/insu-01828244/document https://insu.hal.science/insu-01828244/file/gji-sauter-2009-179-2-687.pdf https://doi.org/10.1111/j.1365-246X.2009.04308.x en eng HAL CCSD Oxford University Press (OUP) info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-246X.2009.04308.x insu-01828244 https://insu.hal.science/insu-01828244 https://insu.hal.science/insu-01828244/document https://insu.hal.science/insu-01828244/file/gji-sauter-2009-179-2-687.pdf doi:10.1111/j.1365-246X.2009.04308.x info:eu-repo/semantics/OpenAccess ISSN: 0956-540X EISSN: 1365-246X Geophysical Journal International https://insu.hal.science/insu-01828244 Geophysical Journal International, 2009, 179 (2), pp.687-699. ⟨10.1111/j.1365-246X.2009.04308.x⟩ Magnetic anomalies: modelling and interpretation Mid-ocean ridge processes Hotspots Indian Ocean [SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph] info:eu-repo/semantics/article Journal articles 2009 ftsorbonneuniv https://doi.org/10.1111/j.1365-246X.2009.04308.x 2024-07-25T23:48:06Z International audience Regional axial depths, mantle Bouguer anomaly values, geochemical proxies for the extent of partial melting and tomographic models along the Southwest Indian Ridge (SWIR) all concur in indicating the presence of thicker crust and hotter mantle between the Indomed and Gallieni transform faults (TFs; 46 • E and 52 • 20 E) relative to the neighbouring ridge sections. Accreted seafloor between these TFs over the past ∼10 Myr is also locally much shallower (>1000 m) and corresponds to thicker crust (>1.7 km) than previously accreted seafloor along the same ridge region. Two large outward facing topographic gradients mark the outer edges of two anomalously shallow off-axis domains on the African and Antarctic plates. Their vertical relief (>2000 m locally) and their geometry, parallel to the present-day axis along a >210-km-long ridge section, suggest an extremely sudden and large event dated between ∼8 (magnetic anomaly C4n) and ∼11 Ma (magnetic anomaly C5n). Asymmetric spreading and small ridge jumps occur at the onset of the formation of the anomalously shallow off-axis domains, leading to a reorganization of the ridge segmentation. We interpret these anomalously shallow off-axis domains as the relicts of a volcanic plateau due to a sudden increase of the magma supply. This event of enhanced magmatism started in the central part of the ridge section and then propagated along axis to the east and probably also to the west. However, it did not cross the Gallieni and Indomed TFs suggesting that large offsets can curtail or even block along-axis melt flow. We propose that this melting anomaly may be ascribed to a regionally higher mantle temperature provided by mantle outpouring from the Crozet hotspot towards the SWIR. Article in Journal/Newspaper Antarc* Antarctic HAL Sorbonne Université Geophysical Journal International 179 2 687 699