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Evolution of the Oceanic Lithosphere in the Equatorial Atlantic From Rayleigh Wave Tomography, Evidence for Small‐Scale Convection From the PI‐LAB Experiment
The oceanic lithosphere is a primary component of the plate tectonic system, yet its evolution and its asthenospheric interaction have rarely been quantified by in situ imaging at slow spreading systems. We use Rayleigh wave tomography from noise and teleseismic surface waves to image the shear wave...
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Published in: | Geochemistry, geophysics, geosystems : G3 geophysics, geosystems : G3, 2020-09, Vol.21 (9), p.n/a |
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description | The oceanic lithosphere is a primary component of the plate tectonic system, yet its evolution and its asthenospheric interaction have rarely been quantified by in situ imaging at slow spreading systems. We use Rayleigh wave tomography from noise and teleseismic surface waves to image the shear wave velocity structure of the oceanic lithosphere‐asthenosphere system from 0 to 80 My at the equatorial Mid‐Atlantic Ridge using data from the Passive Imaging of the Lithosphere‐Asthenosphere Boundary (PI‐LAB) experiment. We observe fast lithosphere (VSV > 4.4 km/s) that thickens from 20–30 km near the ridge axis to ~70 km at seafloor >60 My. We observe several punctuated slow velocity anomalies (VSV 400 km from the ridge. We observe a high velocity lithospheric downwelling drip beneath 30 My seafloor that extends to 80–130 km depth. The asthenospheric slow velocities likely require partial melt. Although melt is present off axis, the lack of off‐axis volcanism suggests the lithosphere acts as a permeability boundary for deeper melts. The punctuated and off‐axis character of the asthenospheric anomalies and lithospheric drip suggests small‐scale convection is active at a range of seafloor ages. Small‐scale convection and/or more complex mantle flow may be aided by the presence of large offset fracture zones and/or the presence of melt and its associated low‐viscosities and enhanced buoyancies.
Plain Language Summary
Tectonic plates are created at mid‐ocean ridges. As the plates age and move over the weaker asthenosphere below, they thicken and subside. Yet there are few high‐resolution images of this process. We deployed 39 ocean bottom seismometers in the equatorial Mid‐Atlantic to image the seismic velocity of the tectonic plate and the asthenosphere below. We observe a tectonic plate that generally thickens with age, but the thickening is not simple and monotonic everywhere, and there may be evidence of drips coming off the base of the plate. We also see evidence for small pockets of melt and rising mantle far away from the ridge axis. Taken together this suggests that flow in the mantle is more complicated than previously thought. Small‐scale convection may occur beneath a range of seafloor ages, which may also affe |
doi_str_mv | 10.1029/2020GC009174 |
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Plain Language Summary
Tectonic plates are created at mid‐ocean ridges. As the plates age and move over the weaker asthenosphere below, they thicken and subside. Yet there are few high‐resolution images of this process. We deployed 39 ocean bottom seismometers in the equatorial Mid‐Atlantic to image the seismic velocity of the tectonic plate and the asthenosphere below. We observe a tectonic plate that generally thickens with age, but the thickening is not simple and monotonic everywhere, and there may be evidence of drips coming off the base of the plate. We also see evidence for small pockets of melt and rising mantle far away from the ridge axis. Taken together this suggests that flow in the mantle is more complicated than previously thought. Small‐scale convection may occur beneath a range of seafloor ages, which may also affect the way the lithosphere cools and ages. Thus, our result has implications for how tectonic plates evolve and interact with the mantle below and how plate tectonics works to cool the earth since its formation billions of years ago.
Key Points
We image a lithosphere that increases from 20–30 to 50 km thick beneath 0–40 My old seafloor
We image punctuated slow velocity zones beneath the ridge and up to 400 km off‐axis in the asthenosphere that likely require melt
The pattern of anomalies suggests small‐scale convection may occur beneath a range of seafloor ages</description><identifier>ISSN: 1525-2027</identifier><identifier>EISSN: 1525-2027</identifier><identifier>DOI: 10.1029/2020GC009174</identifier><language>eng</language><publisher>Washington: John Wiley & Sons, Inc</publisher><subject>Anomalies ; Asthenosphere ; Atlantic Ocean ; Convection ; Downwelling ; Evolution ; Fracture zones ; Imaging techniques ; Lava ; Lithosphere ; Ocean bottom seismometers ; Ocean floor ; oceanic lithosphere ; Oceans ; Permeability ; PI‐LAB ; Plate tectonics ; Rayleigh waves ; Regions ; Ridges ; Seismic velocities ; Seismometers ; shear velocity ; Shear wave velocities ; surface wave tomography ; Tectonics ; Tomography ; Velocity ; Volcanism ; Wave velocity</subject><ispartof>Geochemistry, geophysics, geosystems : G3, 2020-09, Vol.21 (9), p.n/a</ispartof><rights>2020. The Authors.</rights><rights>2020. This article is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a4340-d88be424f3f377bbefcd4beef23f251bdbcdc538c5120756963eb79e120a91fc3</citedby><cites>FETCH-LOGICAL-a4340-d88be424f3f377bbefcd4beef23f251bdbcdc538c5120756963eb79e120a91fc3</cites><orcidid>0000-0002-2620-295X ; 0000-0001-5071-793X ; 0000-0003-1902-7476 ; 0000-0002-1486-3945 ; 0000-0002-0731-768X ; 0000-0002-1841-1911</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://onlinelibrary.wiley.com/doi/pdf/10.1029%2F2020GC009174$$EPDF$$P50$$Gwiley$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1029%2F2020GC009174$$EHTML$$P50$$Gwiley$$Hfree_for_read</linktohtml><link.rule.ids>314,780,784,11562,27924,27925,46052,46476</link.rule.ids></links><search><creatorcontrib>Harmon, Nicholas</creatorcontrib><creatorcontrib>Rychert, Catherine A.</creatorcontrib><creatorcontrib>Kendall, J. Michael</creatorcontrib><creatorcontrib>Agius, Matthew</creatorcontrib><creatorcontrib>Bogiatzis, Petros</creatorcontrib><creatorcontrib>Tharimena, Saikiran</creatorcontrib><title>Evolution of the Oceanic Lithosphere in the Equatorial Atlantic From Rayleigh Wave Tomography, Evidence for Small‐Scale Convection From the PI‐LAB Experiment</title><title>Geochemistry, geophysics, geosystems : G3</title><description>The oceanic lithosphere is a primary component of the plate tectonic system, yet its evolution and its asthenospheric interaction have rarely been quantified by in situ imaging at slow spreading systems. We use Rayleigh wave tomography from noise and teleseismic surface waves to image the shear wave velocity structure of the oceanic lithosphere‐asthenosphere system from 0 to 80 My at the equatorial Mid‐Atlantic Ridge using data from the Passive Imaging of the Lithosphere‐Asthenosphere Boundary (PI‐LAB) experiment. We observe fast lithosphere (VSV > 4.4 km/s) that thickens from 20–30 km near the ridge axis to ~70 km at seafloor >60 My. We observe several punctuated slow velocity anomalies (VSV < 4.1 km/s) in the asthenosphere between 50 and 150 km depth, not necessarily focused beneath the ridge axis. Some of the slow velocity regions are located within 100 km of the ridge axis, but other slow velocity regions are observed at distances > 400 km from the ridge. We observe a high velocity lithospheric downwelling drip beneath 30 My seafloor that extends to 80–130 km depth. The asthenospheric slow velocities likely require partial melt. Although melt is present off axis, the lack of off‐axis volcanism suggests the lithosphere acts as a permeability boundary for deeper melts. The punctuated and off‐axis character of the asthenospheric anomalies and lithospheric drip suggests small‐scale convection is active at a range of seafloor ages. Small‐scale convection and/or more complex mantle flow may be aided by the presence of large offset fracture zones and/or the presence of melt and its associated low‐viscosities and enhanced buoyancies.
Plain Language Summary
Tectonic plates are created at mid‐ocean ridges. As the plates age and move over the weaker asthenosphere below, they thicken and subside. Yet there are few high‐resolution images of this process. We deployed 39 ocean bottom seismometers in the equatorial Mid‐Atlantic to image the seismic velocity of the tectonic plate and the asthenosphere below. We observe a tectonic plate that generally thickens with age, but the thickening is not simple and monotonic everywhere, and there may be evidence of drips coming off the base of the plate. We also see evidence for small pockets of melt and rising mantle far away from the ridge axis. Taken together this suggests that flow in the mantle is more complicated than previously thought. Small‐scale convection may occur beneath a range of seafloor ages, which may also affect the way the lithosphere cools and ages. Thus, our result has implications for how tectonic plates evolve and interact with the mantle below and how plate tectonics works to cool the earth since its formation billions of years ago.
Key Points
We image a lithosphere that increases from 20–30 to 50 km thick beneath 0–40 My old seafloor
We image punctuated slow velocity zones beneath the ridge and up to 400 km off‐axis in the asthenosphere that likely require melt
The pattern of anomalies suggests small‐scale convection may occur beneath a range of seafloor ages</description><subject>Anomalies</subject><subject>Asthenosphere</subject><subject>Atlantic Ocean</subject><subject>Convection</subject><subject>Downwelling</subject><subject>Evolution</subject><subject>Fracture zones</subject><subject>Imaging techniques</subject><subject>Lava</subject><subject>Lithosphere</subject><subject>Ocean bottom seismometers</subject><subject>Ocean floor</subject><subject>oceanic lithosphere</subject><subject>Oceans</subject><subject>Permeability</subject><subject>PI‐LAB</subject><subject>Plate tectonics</subject><subject>Rayleigh waves</subject><subject>Regions</subject><subject>Ridges</subject><subject>Seismic velocities</subject><subject>Seismometers</subject><subject>shear velocity</subject><subject>Shear wave velocities</subject><subject>surface wave tomography</subject><subject>Tectonics</subject><subject>Tomography</subject><subject>Velocity</subject><subject>Volcanism</subject><subject>Wave velocity</subject><issn>1525-2027</issn><issn>1525-2027</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><sourceid>24P</sourceid><sourceid>DOA</sourceid><recordid>eNp9kd9u0zAUhyPEJMbGHQ9gidsV_DeJL0uVhUqVhtgmLi3HOW5cuXHmpB294xF4BV6NJ8FrEdrVrmyf8-n7Hetk2XuCPxJM5SeKKa4XGEtS8FfZORFUzFKteP3s_iZ7O44bjAkXojzPflf74HeTCz0KFk0doBsDuncGrdzUhXHoIAJy_bFVPez0FKLTHs0nr_spYdcxbNE3ffDg1h36rveA7sI2rKMeusMVqvauhd4AsiGi2632_s_PX7dGe0CL0O_BHKOPkqeEr8vUXs0_o-rHANFtoZ8uszOr_Qjv_p0X2f11dbf4Mlvd1MvFfDXTnHE8a8uyAU65ZZYVRdOANS1vACxllgrStI1pjWClEYTiQuQyZ9AUEtJLS2INu8iWJ28b9EYNKVzHgwraqWMhxLXSMf3YgwIpQUvaJIPgZZFLSYmhWFiW55oVIrk-nFxDDA87GCe1CbvYp_EV5TwvMOMlS9TViTIxjGME-z-VYPW0UPV8oQlnJ_zReTi8yKq6ritKGcbsL1afpDo</recordid><startdate>202009</startdate><enddate>202009</enddate><creator>Harmon, Nicholas</creator><creator>Rychert, Catherine A.</creator><creator>Kendall, J. Michael</creator><creator>Agius, Matthew</creator><creator>Bogiatzis, Petros</creator><creator>Tharimena, Saikiran</creator><general>John Wiley & Sons, Inc</general><general>Wiley</general><scope>24P</scope><scope>WIN</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>7TN</scope><scope>F1W</scope><scope>H96</scope><scope>KL.</scope><scope>L.G</scope><scope>DOA</scope><orcidid>https://orcid.org/0000-0002-2620-295X</orcidid><orcidid>https://orcid.org/0000-0001-5071-793X</orcidid><orcidid>https://orcid.org/0000-0003-1902-7476</orcidid><orcidid>https://orcid.org/0000-0002-1486-3945</orcidid><orcidid>https://orcid.org/0000-0002-0731-768X</orcidid><orcidid>https://orcid.org/0000-0002-1841-1911</orcidid></search><sort><creationdate>202009</creationdate><title>Evolution of the Oceanic Lithosphere in the Equatorial Atlantic From Rayleigh Wave Tomography, Evidence for Small‐Scale Convection From the PI‐LAB Experiment</title><author>Harmon, Nicholas ; Rychert, Catherine A. ; Kendall, J. Michael ; Agius, Matthew ; Bogiatzis, Petros ; Tharimena, Saikiran</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a4340-d88be424f3f377bbefcd4beef23f251bdbcdc538c5120756963eb79e120a91fc3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Anomalies</topic><topic>Asthenosphere</topic><topic>Atlantic Ocean</topic><topic>Convection</topic><topic>Downwelling</topic><topic>Evolution</topic><topic>Fracture zones</topic><topic>Imaging techniques</topic><topic>Lava</topic><topic>Lithosphere</topic><topic>Ocean bottom seismometers</topic><topic>Ocean floor</topic><topic>oceanic lithosphere</topic><topic>Oceans</topic><topic>Permeability</topic><topic>PI‐LAB</topic><topic>Plate tectonics</topic><topic>Rayleigh waves</topic><topic>Regions</topic><topic>Ridges</topic><topic>Seismic velocities</topic><topic>Seismometers</topic><topic>shear velocity</topic><topic>Shear wave velocities</topic><topic>surface wave tomography</topic><topic>Tectonics</topic><topic>Tomography</topic><topic>Velocity</topic><topic>Volcanism</topic><topic>Wave velocity</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Harmon, Nicholas</creatorcontrib><creatorcontrib>Rychert, Catherine A.</creatorcontrib><creatorcontrib>Kendall, J. Michael</creatorcontrib><creatorcontrib>Agius, Matthew</creatorcontrib><creatorcontrib>Bogiatzis, Petros</creatorcontrib><creatorcontrib>Tharimena, Saikiran</creatorcontrib><collection>Open Access: Wiley-Blackwell Open Access Journals</collection><collection>Wiley Free Archive</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Oceanic Abstracts</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy & Non-Living Resources</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><collection>DOAJ Directory of Open Access Journals</collection><jtitle>Geochemistry, geophysics, geosystems : G3</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Harmon, Nicholas</au><au>Rychert, Catherine A.</au><au>Kendall, J. Michael</au><au>Agius, Matthew</au><au>Bogiatzis, Petros</au><au>Tharimena, Saikiran</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Evolution of the Oceanic Lithosphere in the Equatorial Atlantic From Rayleigh Wave Tomography, Evidence for Small‐Scale Convection From the PI‐LAB Experiment</atitle><jtitle>Geochemistry, geophysics, geosystems : G3</jtitle><date>2020-09</date><risdate>2020</risdate><volume>21</volume><issue>9</issue><epage>n/a</epage><issn>1525-2027</issn><eissn>1525-2027</eissn><abstract>The oceanic lithosphere is a primary component of the plate tectonic system, yet its evolution and its asthenospheric interaction have rarely been quantified by in situ imaging at slow spreading systems. We use Rayleigh wave tomography from noise and teleseismic surface waves to image the shear wave velocity structure of the oceanic lithosphere‐asthenosphere system from 0 to 80 My at the equatorial Mid‐Atlantic Ridge using data from the Passive Imaging of the Lithosphere‐Asthenosphere Boundary (PI‐LAB) experiment. We observe fast lithosphere (VSV > 4.4 km/s) that thickens from 20–30 km near the ridge axis to ~70 km at seafloor >60 My. We observe several punctuated slow velocity anomalies (VSV < 4.1 km/s) in the asthenosphere between 50 and 150 km depth, not necessarily focused beneath the ridge axis. Some of the slow velocity regions are located within 100 km of the ridge axis, but other slow velocity regions are observed at distances > 400 km from the ridge. We observe a high velocity lithospheric downwelling drip beneath 30 My seafloor that extends to 80–130 km depth. The asthenospheric slow velocities likely require partial melt. Although melt is present off axis, the lack of off‐axis volcanism suggests the lithosphere acts as a permeability boundary for deeper melts. The punctuated and off‐axis character of the asthenospheric anomalies and lithospheric drip suggests small‐scale convection is active at a range of seafloor ages. Small‐scale convection and/or more complex mantle flow may be aided by the presence of large offset fracture zones and/or the presence of melt and its associated low‐viscosities and enhanced buoyancies.
Plain Language Summary
Tectonic plates are created at mid‐ocean ridges. As the plates age and move over the weaker asthenosphere below, they thicken and subside. Yet there are few high‐resolution images of this process. We deployed 39 ocean bottom seismometers in the equatorial Mid‐Atlantic to image the seismic velocity of the tectonic plate and the asthenosphere below. We observe a tectonic plate that generally thickens with age, but the thickening is not simple and monotonic everywhere, and there may be evidence of drips coming off the base of the plate. We also see evidence for small pockets of melt and rising mantle far away from the ridge axis. Taken together this suggests that flow in the mantle is more complicated than previously thought. Small‐scale convection may occur beneath a range of seafloor ages, which may also affect the way the lithosphere cools and ages. Thus, our result has implications for how tectonic plates evolve and interact with the mantle below and how plate tectonics works to cool the earth since its formation billions of years ago.
Key Points
We image a lithosphere that increases from 20–30 to 50 km thick beneath 0–40 My old seafloor
We image punctuated slow velocity zones beneath the ridge and up to 400 km off‐axis in the asthenosphere that likely require melt
The pattern of anomalies suggests small‐scale convection may occur beneath a range of seafloor ages</abstract><cop>Washington</cop><pub>John Wiley & Sons, Inc</pub><doi>10.1029/2020GC009174</doi><tpages>18</tpages><orcidid>https://orcid.org/0000-0002-2620-295X</orcidid><orcidid>https://orcid.org/0000-0001-5071-793X</orcidid><orcidid>https://orcid.org/0000-0003-1902-7476</orcidid><orcidid>https://orcid.org/0000-0002-1486-3945</orcidid><orcidid>https://orcid.org/0000-0002-0731-768X</orcidid><orcidid>https://orcid.org/0000-0002-1841-1911</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Anomalies Asthenosphere Atlantic Ocean Convection Downwelling Evolution Fracture zones Imaging techniques Lava Lithosphere Ocean bottom seismometers Ocean floor oceanic lithosphere Oceans Permeability PI‐LAB Plate tectonics Rayleigh waves Regions Ridges Seismic velocities Seismometers shear velocity Shear wave velocities surface wave tomography Tectonics Tomography Velocity Volcanism Wave velocity |
title | Evolution of the Oceanic Lithosphere in the Equatorial Atlantic From Rayleigh Wave Tomography, Evidence for Small‐Scale Convection From the PI‐LAB Experiment |
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