Origin of magnetic highs at ultramafic hosted hydrothermal systems: Insights from the Yokoniwa site of Central Indian Ridge
High-resolution vector magnetic measurements were performed on an inactive ultramafic-hosted hydrothermal vent field, called Yokoniwa Hydrothermal Field (YHF), using a deep-sea manned submersible Shinkai6500 and an autonomous underwater vehicle r2D4. The YHF has developed at a non-transform offset m...
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description | High-resolution vector magnetic measurements were performed on an inactive ultramafic-hosted hydrothermal vent field, called Yokoniwa Hydrothermal Field (YHF), using a deep-sea manned submersible Shinkai6500 and an autonomous underwater vehicle r2D4. The YHF has developed at a non-transform offset massif of the Central Indian Ridge. Dead chimneys were widely observed around the YHF along with a very weak venting of low-temperature fluids so that hydrothermal activity of the YHF was almost finished. The distribution of crustal magnetization from the magnetic anomaly revealed that the YHF is associated with enhanced magnetization, as seen at the ultramafic-hosted Rainbow and Ashadze-1 hydrothermal sites of the Mid-Atlantic Ridge. The results of rock magnetic analysis on seafloor rock samples (including basalt, dolerite, gabbro, serpentinized peridotite, and hydrothermal sulfide) showed that only highly serpentinized peridotite carries high magnetic susceptibility and that the natural remanent magnetization intensity can explain the high magnetization of Yokoniwa. These observations reflect abundant and strongly magnetized magnetite grains within the highly serpentinized peridotite. Comparisons with the Rainbow and Ashadze-1 suggest that in ultramafic-hosted hydrothermal systems, strongly magnetized magnetite and pyrrhotite form during the progression of hydrothermal alteration of peridotite. After the completion of serpentinization and production of hydrogen, pyrrhotites convert into pyrite or nonmagnetic iron sulfides, which considerably reduces their levels of magnetization. Our results revealed origins of the magnetic high and the development of subsurface chemical processes in ultramafic-hosted hydrothermal systems. Furthermore, the results highlight the use of near-seafloor magnetic field measurements as a powerful tool for detecting and characterizing seafloor hydrothermal systems.
•The ultramafic-hosted inactive Yokoniwa Hydrothermal Field has an enhanced magnetic anomaly.•Highly serpentinized peridotite has strong NRM and magnetic susceptibility.•Strongly magnetized magnetite forms within the peridotite during serpentinization. |
doi_str_mv | 10.1016/j.epsl.2016.02.018 |
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•The ultramafic-hosted inactive Yokoniwa Hydrothermal Field has an enhanced magnetic anomaly.•Highly serpentinized peridotite has strong NRM and magnetic susceptibility.•Strongly magnetized magnetite forms within the peridotite during serpentinization.</description><subject>Hydrothermal systems</subject><subject>magnetic minerals formation model</subject><subject>Magnetite</subject><subject>Magnetization</subject><subject>near-seafloor magnetic anomaly</subject><subject>Origins</subject><subject>Peridotite</subject><subject>Pyrrhotite</subject><subject>Rainbows</subject><subject>Ridges</subject><subject>rock magnetic properties</subject><subject>serpentinization</subject><subject>Yokoniwa Hydrothermal Field</subject><issn>0012-821X</issn><issn>1385-013X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><recordid>eNp9kE9r3DAQxUVIoZs_X6AnHXuxO6ONbbnkEpamDQQCJYXkJBRrvKuNbW012oSlX74y23NPM7x578H8hPiEUCJg_WVb0o6HUuW9BFUC6hOxwKWuCsDl06lYAKAqtMKnj-KMeQsAdVW3C_HnIfq1n2To5WjXEyXfyY1fb1jaJPdDina0_awFTuTk5uBiSBuKox0kH7I28ld5N3GOJJZ9DKPMZ_kcXsPk361kn2guX9GUu4Zsdd5O8qd3a7oQH3o7MF3-m-fi1-23x9WP4v7h-93q5r6wVwCpQF212NgawWHfkqpqRxqoqVSnnH4hTY2CHrUl6BBJvzStU41S1ikLV7ZanovPx95dDL_3xMmMnjsaBjtR2LNBDRqaFqDNVnW0djEwR-rNLvrRxoNBMDNpszUzaTOTNqBMJp1D18cQ5SfePEXDnaepI-cjdcm44P8X_wusz4kx</recordid><startdate>20160501</startdate><enddate>20160501</enddate><creator>Fujii, Masakazu</creator><creator>Okino, Kyoko</creator><creator>Sato, Taichi</creator><creator>Sato, Hiroshi</creator><creator>Nakamura, Kentaro</creator><general>Elsevier B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20160501</creationdate><title>Origin of magnetic highs at ultramafic hosted hydrothermal systems: Insights from the Yokoniwa site of Central Indian Ridge</title><author>Fujii, Masakazu ; Okino, Kyoko ; Sato, Taichi ; Sato, Hiroshi ; Nakamura, Kentaro</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a400t-185917a610d1f9e256de80e752c2d8be8e720f18ae0c11e8b79d2722ad2a04a53</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2016</creationdate><topic>Hydrothermal systems</topic><topic>magnetic minerals formation model</topic><topic>Magnetite</topic><topic>Magnetization</topic><topic>near-seafloor magnetic anomaly</topic><topic>Origins</topic><topic>Peridotite</topic><topic>Pyrrhotite</topic><topic>Rainbows</topic><topic>Ridges</topic><topic>rock magnetic properties</topic><topic>serpentinization</topic><topic>Yokoniwa Hydrothermal Field</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Fujii, Masakazu</creatorcontrib><creatorcontrib>Okino, Kyoko</creatorcontrib><creatorcontrib>Sato, Taichi</creatorcontrib><creatorcontrib>Sato, Hiroshi</creatorcontrib><creatorcontrib>Nakamura, Kentaro</creatorcontrib><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Earth and planetary science letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Fujii, Masakazu</au><au>Okino, Kyoko</au><au>Sato, Taichi</au><au>Sato, Hiroshi</au><au>Nakamura, Kentaro</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Origin of magnetic highs at ultramafic hosted hydrothermal systems: Insights from the Yokoniwa site of Central Indian Ridge</atitle><jtitle>Earth and planetary science letters</jtitle><date>2016-05-01</date><risdate>2016</risdate><volume>441</volume><spage>26</spage><epage>37</epage><pages>26-37</pages><issn>0012-821X</issn><eissn>1385-013X</eissn><abstract>High-resolution vector magnetic measurements were performed on an inactive ultramafic-hosted hydrothermal vent field, called Yokoniwa Hydrothermal Field (YHF), using a deep-sea manned submersible Shinkai6500 and an autonomous underwater vehicle r2D4. The YHF has developed at a non-transform offset massif of the Central Indian Ridge. Dead chimneys were widely observed around the YHF along with a very weak venting of low-temperature fluids so that hydrothermal activity of the YHF was almost finished. The distribution of crustal magnetization from the magnetic anomaly revealed that the YHF is associated with enhanced magnetization, as seen at the ultramafic-hosted Rainbow and Ashadze-1 hydrothermal sites of the Mid-Atlantic Ridge. The results of rock magnetic analysis on seafloor rock samples (including basalt, dolerite, gabbro, serpentinized peridotite, and hydrothermal sulfide) showed that only highly serpentinized peridotite carries high magnetic susceptibility and that the natural remanent magnetization intensity can explain the high magnetization of Yokoniwa. These observations reflect abundant and strongly magnetized magnetite grains within the highly serpentinized peridotite. Comparisons with the Rainbow and Ashadze-1 suggest that in ultramafic-hosted hydrothermal systems, strongly magnetized magnetite and pyrrhotite form during the progression of hydrothermal alteration of peridotite. After the completion of serpentinization and production of hydrogen, pyrrhotites convert into pyrite or nonmagnetic iron sulfides, which considerably reduces their levels of magnetization. Our results revealed origins of the magnetic high and the development of subsurface chemical processes in ultramafic-hosted hydrothermal systems. Furthermore, the results highlight the use of near-seafloor magnetic field measurements as a powerful tool for detecting and characterizing seafloor hydrothermal systems.
•The ultramafic-hosted inactive Yokoniwa Hydrothermal Field has an enhanced magnetic anomaly.•Highly serpentinized peridotite has strong NRM and magnetic susceptibility.•Strongly magnetized magnetite forms within the peridotite during serpentinization.</abstract><pub>Elsevier B.V</pub><doi>10.1016/j.epsl.2016.02.018</doi><tpages>12</tpages><oa>free_for_read</oa></addata></record> |
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subjects | Hydrothermal systems magnetic minerals formation model Magnetite Magnetization near-seafloor magnetic anomaly Origins Peridotite Pyrrhotite Rainbows Ridges rock magnetic properties serpentinization Yokoniwa Hydrothermal Field |
title | Origin of magnetic highs at ultramafic hosted hydrothermal systems: Insights from the Yokoniwa site of Central Indian Ridge |
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