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spelling ftinsu:oai:HAL:hal-00112779v1 2023-06-18T03:38:06+02:00 Constraints on age and construction process of the Foundation chain submarine volcanoes from magnetic modeling Maia, Marcia Dyment, Jérôme Jouannetaud, David Domaines Océaniques (LDO) Institut national des sciences de l'Univers (INSU - CNRS)-Université de Brest (UBO)-Observatoire des Sciences de l'Univers-Institut d'écologie et environnement-Centre National de la Recherche Scientifique (CNRS) Institut de Physique du Globe de Paris (IPGP) Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Université de La Réunion (UR)-Institut de Physique du Globe de Paris (IPG Paris)-Centre National de la Recherche Scientifique (CNRS) 2005-06-30 https://hal.science/hal-00112779 https://doi.org/10.1016/j.epsl.2005.02.044 en eng HAL CCSD Elsevier info:eu-repo/semantics/altIdentifier/doi/10.1016/j.epsl.2005.02.044 hal-00112779 https://hal.science/hal-00112779 doi:10.1016/j.epsl.2005.02.044 ISSN: 0012-821X Earth and Planetary Science Letters https://hal.science/hal-00112779 Earth and Planetary Science Letters, 2005, 235 (1-2), pp.183-199. ⟨10.1016/j.epsl.2005.02.044⟩ intraplate volcanism seamount magnetism hotspot seamount ages ridge–hotspot interactions [SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph] info:eu-repo/semantics/article Journal articles 2005 ftinsu https://doi.org/10.1016/j.epsl.2005.02.044 2023-06-06T01:23:39Z The interaction between the Foundation hotspot and the Pacific–Antarctic Ridge (South Pacific) is one of the two known cases where a ridge is approaching a hotspot. This ridge–hotspot relative movement results in a change in the morphology of the volcanoes along the chain as the age of the lithosphere at the time of edifice formation progressively diminishes. Four hundred kilometers west of the Pacific–Antarctic Ridge axis, volcanism is distributed along two sub-parallel lines of volcanoes, separated by distances diminishing from 100 km at the west to 50 km near the axis of the ridge. The magnetic anomalies mapped on this part of the chain show a pattern clearly dominated by the magnetic signature of the seamounts. The anomalies were forward modeled using a remanent magnetization of normal or reversed polarity within the volcano topography. The resulting pattern of normal and reversed magnetization is consistent with the intervals of the geomagnetic polarity time scale for the last 5 Ma, the age of the oldest studied volcano. These magnetic anomalies therefore represent an independent means of dating the volcanic edifices. The ages deduced from the modeling are consistent with the hypothesis of volcanoes built by a hotspot on the fast moving Pacific plate and are in good agreement with the published radiometric dates, although these dates tend to correspond to the late constructional stages of the edifices. The differences between magnetic and radiometric ages suggest that the average time span to build a volcano of the Foundation chain is about 1 million years, in agreement with other intraplate edifices. The difference between the magnetic ages of the seamounts and of the underlying crust, both deduced from the magnetic anomaly analysis, show that the ridge has approached the hotspot at a rate of 40 km/Ma. Article in Journal/Newspaper Antarc* Antarctic Institut national des sciences de l'Univers: HAL-INSU Antarctic Pacific Earth and Planetary Science Letters 235 1-2 183 199
institution Open Polar
collection Institut national des sciences de l'Univers: HAL-INSU
op_collection_id ftinsu
language English
topic intraplate volcanism
seamount magnetism
hotspot
seamount ages
ridge–hotspot interactions
[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]
spellingShingle intraplate volcanism
seamount magnetism
hotspot
seamount ages
ridge–hotspot interactions
[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]
Maia, Marcia
Dyment, Jérôme
Jouannetaud, David
Constraints on age and construction process of the Foundation chain submarine volcanoes from magnetic modeling
topic_facet intraplate volcanism
seamount magnetism
hotspot
seamount ages
ridge–hotspot interactions
[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]
description The interaction between the Foundation hotspot and the Pacific–Antarctic Ridge (South Pacific) is one of the two known cases where a ridge is approaching a hotspot. This ridge–hotspot relative movement results in a change in the morphology of the volcanoes along the chain as the age of the lithosphere at the time of edifice formation progressively diminishes. Four hundred kilometers west of the Pacific–Antarctic Ridge axis, volcanism is distributed along two sub-parallel lines of volcanoes, separated by distances diminishing from 100 km at the west to 50 km near the axis of the ridge. The magnetic anomalies mapped on this part of the chain show a pattern clearly dominated by the magnetic signature of the seamounts. The anomalies were forward modeled using a remanent magnetization of normal or reversed polarity within the volcano topography. The resulting pattern of normal and reversed magnetization is consistent with the intervals of the geomagnetic polarity time scale for the last 5 Ma, the age of the oldest studied volcano. These magnetic anomalies therefore represent an independent means of dating the volcanic edifices. The ages deduced from the modeling are consistent with the hypothesis of volcanoes built by a hotspot on the fast moving Pacific plate and are in good agreement with the published radiometric dates, although these dates tend to correspond to the late constructional stages of the edifices. The differences between magnetic and radiometric ages suggest that the average time span to build a volcano of the Foundation chain is about 1 million years, in agreement with other intraplate edifices. The difference between the magnetic ages of the seamounts and of the underlying crust, both deduced from the magnetic anomaly analysis, show that the ridge has approached the hotspot at a rate of 40 km/Ma.
author2 Domaines Océaniques (LDO)
Institut national des sciences de l'Univers (INSU - CNRS)-Université de Brest (UBO)-Observatoire des Sciences de l'Univers-Institut d'écologie et environnement-Centre National de la Recherche Scientifique (CNRS)
Institut de Physique du Globe de Paris (IPGP)
Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Université de La Réunion (UR)-Institut de Physique du Globe de Paris (IPG Paris)-Centre National de la Recherche Scientifique (CNRS)
format Article in Journal/Newspaper
author Maia, Marcia
Dyment, Jérôme
Jouannetaud, David
author_facet Maia, Marcia
Dyment, Jérôme
Jouannetaud, David
author_sort Maia, Marcia
title Constraints on age and construction process of the Foundation chain submarine volcanoes from magnetic modeling
title_short Constraints on age and construction process of the Foundation chain submarine volcanoes from magnetic modeling
title_full Constraints on age and construction process of the Foundation chain submarine volcanoes from magnetic modeling
title_fullStr Constraints on age and construction process of the Foundation chain submarine volcanoes from magnetic modeling
title_full_unstemmed Constraints on age and construction process of the Foundation chain submarine volcanoes from magnetic modeling
title_sort constraints on age and construction process of the foundation chain submarine volcanoes from magnetic modeling
publisher HAL CCSD
publishDate 2005
url https://hal.science/hal-00112779
https://doi.org/10.1016/j.epsl.2005.02.044
geographic Antarctic
Pacific
geographic_facet Antarctic
Pacific
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
op_source ISSN: 0012-821X
Earth and Planetary Science Letters
https://hal.science/hal-00112779
Earth and Planetary Science Letters, 2005, 235 (1-2), pp.183-199. ⟨10.1016/j.epsl.2005.02.044⟩
op_relation info:eu-repo/semantics/altIdentifier/doi/10.1016/j.epsl.2005.02.044
hal-00112779
https://hal.science/hal-00112779
doi:10.1016/j.epsl.2005.02.044
op_doi https://doi.org/10.1016/j.epsl.2005.02.044
container_title Earth and Planetary Science Letters
container_volume 235
container_issue 1-2
container_start_page 183
op_container_end_page 199
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