Fluid–sediment interactions at Eastern Mediterranean mud volcanoes: a stable isotope study from ODP Leg 160
Pore fluids from two ODP sites at Eastern Mediterranean mud volcanoes have been analyzed for their Cl concentration and their δ 18O and δD isotopic composition. The Cl data span a wide range of concentrations, from extremely depleted with respect to seawater (as low as 60 mM) at the crest of Milano...
Gespeichert in:
Veröffentlicht in: | Earth and planetary science letters 2003-07, Vol.212 (3), p.377-391 |
---|---|
Hauptverfasser: | , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | 391 |
---|---|
container_issue | 3 |
container_start_page | 377 |
container_title | Earth and planetary science letters |
container_volume | 212 |
creator | Dählmann, A de Lange, G.J |
description | Pore fluids from two ODP sites at Eastern Mediterranean mud volcanoes have been analyzed for their Cl concentration and their δ
18O and δD isotopic composition. The Cl data span a wide range of concentrations, from extremely depleted with respect to seawater (as low as 60 mM) at the crest of Milano dome (site 970) to strongly enriched (up to 5.4 M) at Napoli dome (site 971). Chloride enrichment is known to be due to dissolving Messinian evaporites, whereas the source of the low-Cl fluid is deduced from stable isotope data presented here. The isotopic composition of the endmember fluid is found to be +10‰ for δ
18O and −32‰ for δD for low- as well as for high-Cl waters. From this signature it can be concluded that neither gas hydrates nor meteoric water play a significant role in the freshening of the pore water. Several other processes altering the δ
18O/δD composition of pore waters are discussed and considered to be of only negligible influence. The process characterizing the isotopic composition of the fluid is found to be clay mineral dehydration (mainly smectite–illite transformation), corresponding to a depth range of 3.5–7 km and an elevated temperature of about 120–165°C. A quantitative estimate shows that this reaction is capable of producing the observed extreme Cl depletion. |
doi_str_mv | 10.1016/S0012-821X(03)00227-9 |
format | Article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_18021621</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><els_id>S0012821X03002279</els_id><sourcerecordid>18021621</sourcerecordid><originalsourceid>FETCH-LOGICAL-a479t-94316963c328da7425889046f266138bf738ecf4cf64c35d681b5f8db8683fd3</originalsourceid><addsrcrecordid>eNqFkMlKBDEURYMo2A6fIGQluijNUJVOuRFxhhYFXbgL6eRFIlWVNkkJ7vwH_9AvMdri1tUbuPfx7kFoh5IDSqg4vCeEskoy-rhH-D4hjE2rdgVNKJdNRSh_XEWTP8k62kjpmRAiGtFOUH_Rjd5-vn8ksL6HIWM_ZIjaZB-GhHXG5zqVxYBviqA0UQ-gB9yPFr-GzughQDrCGqes5x1gn0IOCyjjaN-wi6HHt2d3eAZPmAqyhdac7hJs_9ZN9HBx_nB6Vc1uL69PT2aVrqdtrtqaU9EKbjiTVk9r1kjZklo4JkQJNXdTLsG42jhRG95YIem8cdLOpZDcWb6JdpdnFzG8jJCy6n0y0HXl9zAmRSVhVDBahM1SaGJIKYJTi-h7Hd8UJeqbrfphq77BKcLVD1vVFt_x0gclxKuHqJLxMJiCKILJygb_z4UvBPSCFg</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>18021621</pqid></control><display><type>article</type><title>Fluid–sediment interactions at Eastern Mediterranean mud volcanoes: a stable isotope study from ODP Leg 160</title><source>Access via ScienceDirect (Elsevier)</source><creator>Dählmann, A ; de Lange, G.J</creator><creatorcontrib>Dählmann, A ; de Lange, G.J</creatorcontrib><description>Pore fluids from two ODP sites at Eastern Mediterranean mud volcanoes have been analyzed for their Cl concentration and their δ
18O and δD isotopic composition. The Cl data span a wide range of concentrations, from extremely depleted with respect to seawater (as low as 60 mM) at the crest of Milano dome (site 970) to strongly enriched (up to 5.4 M) at Napoli dome (site 971). Chloride enrichment is known to be due to dissolving Messinian evaporites, whereas the source of the low-Cl fluid is deduced from stable isotope data presented here. The isotopic composition of the endmember fluid is found to be +10‰ for δ
18O and −32‰ for δD for low- as well as for high-Cl waters. From this signature it can be concluded that neither gas hydrates nor meteoric water play a significant role in the freshening of the pore water. Several other processes altering the δ
18O/δD composition of pore waters are discussed and considered to be of only negligible influence. The process characterizing the isotopic composition of the fluid is found to be clay mineral dehydration (mainly smectite–illite transformation), corresponding to a depth range of 3.5–7 km and an elevated temperature of about 120–165°C. A quantitative estimate shows that this reaction is capable of producing the observed extreme Cl depletion.</description><identifier>ISSN: 0012-821X</identifier><identifier>EISSN: 1385-013X</identifier><identifier>DOI: 10.1016/S0012-821X(03)00227-9</identifier><language>eng</language><publisher>Elsevier B.V</publisher><subject>clay mineral dehydration ; clay mineral ion filtration ; gas hydrates ; hydrogen isotopes ; Marine ; Mediterranean ; mud volcanoes ; oxygen isotopes ; pore water</subject><ispartof>Earth and planetary science letters, 2003-07, Vol.212 (3), p.377-391</ispartof><rights>2003 Elsevier Science B.V.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a479t-94316963c328da7425889046f266138bf738ecf4cf64c35d681b5f8db8683fd3</citedby><cites>FETCH-LOGICAL-a479t-94316963c328da7425889046f266138bf738ecf4cf64c35d681b5f8db8683fd3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://dx.doi.org/10.1016/S0012-821X(03)00227-9$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>314,780,784,3550,27924,27925,45995</link.rule.ids></links><search><creatorcontrib>Dählmann, A</creatorcontrib><creatorcontrib>de Lange, G.J</creatorcontrib><title>Fluid–sediment interactions at Eastern Mediterranean mud volcanoes: a stable isotope study from ODP Leg 160</title><title>Earth and planetary science letters</title><description>Pore fluids from two ODP sites at Eastern Mediterranean mud volcanoes have been analyzed for their Cl concentration and their δ
18O and δD isotopic composition. The Cl data span a wide range of concentrations, from extremely depleted with respect to seawater (as low as 60 mM) at the crest of Milano dome (site 970) to strongly enriched (up to 5.4 M) at Napoli dome (site 971). Chloride enrichment is known to be due to dissolving Messinian evaporites, whereas the source of the low-Cl fluid is deduced from stable isotope data presented here. The isotopic composition of the endmember fluid is found to be +10‰ for δ
18O and −32‰ for δD for low- as well as for high-Cl waters. From this signature it can be concluded that neither gas hydrates nor meteoric water play a significant role in the freshening of the pore water. Several other processes altering the δ
18O/δD composition of pore waters are discussed and considered to be of only negligible influence. The process characterizing the isotopic composition of the fluid is found to be clay mineral dehydration (mainly smectite–illite transformation), corresponding to a depth range of 3.5–7 km and an elevated temperature of about 120–165°C. A quantitative estimate shows that this reaction is capable of producing the observed extreme Cl depletion.</description><subject>clay mineral dehydration</subject><subject>clay mineral ion filtration</subject><subject>gas hydrates</subject><subject>hydrogen isotopes</subject><subject>Marine</subject><subject>Mediterranean</subject><subject>mud volcanoes</subject><subject>oxygen isotopes</subject><subject>pore water</subject><issn>0012-821X</issn><issn>1385-013X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2003</creationdate><recordtype>article</recordtype><recordid>eNqFkMlKBDEURYMo2A6fIGQluijNUJVOuRFxhhYFXbgL6eRFIlWVNkkJ7vwH_9AvMdri1tUbuPfx7kFoh5IDSqg4vCeEskoy-rhH-D4hjE2rdgVNKJdNRSh_XEWTP8k62kjpmRAiGtFOUH_Rjd5-vn8ksL6HIWM_ZIjaZB-GhHXG5zqVxYBviqA0UQ-gB9yPFr-GzughQDrCGqes5x1gn0IOCyjjaN-wi6HHt2d3eAZPmAqyhdac7hJs_9ZN9HBx_nB6Vc1uL69PT2aVrqdtrtqaU9EKbjiTVk9r1kjZklo4JkQJNXdTLsG42jhRG95YIem8cdLOpZDcWb6JdpdnFzG8jJCy6n0y0HXl9zAmRSVhVDBahM1SaGJIKYJTi-h7Hd8UJeqbrfphq77BKcLVD1vVFt_x0gclxKuHqJLxMJiCKILJygb_z4UvBPSCFg</recordid><startdate>20030725</startdate><enddate>20030725</enddate><creator>Dählmann, A</creator><creator>de Lange, G.J</creator><general>Elsevier B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TN</scope><scope>F1W</scope><scope>H96</scope><scope>L.G</scope></search><sort><creationdate>20030725</creationdate><title>Fluid–sediment interactions at Eastern Mediterranean mud volcanoes: a stable isotope study from ODP Leg 160</title><author>Dählmann, A ; de Lange, G.J</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a479t-94316963c328da7425889046f266138bf738ecf4cf64c35d681b5f8db8683fd3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2003</creationdate><topic>clay mineral dehydration</topic><topic>clay mineral ion filtration</topic><topic>gas hydrates</topic><topic>hydrogen isotopes</topic><topic>Marine</topic><topic>Mediterranean</topic><topic>mud volcanoes</topic><topic>oxygen isotopes</topic><topic>pore water</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Dählmann, A</creatorcontrib><creatorcontrib>de Lange, G.J</creatorcontrib><collection>CrossRef</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>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><jtitle>Earth and planetary science letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Dählmann, A</au><au>de Lange, G.J</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Fluid–sediment interactions at Eastern Mediterranean mud volcanoes: a stable isotope study from ODP Leg 160</atitle><jtitle>Earth and planetary science letters</jtitle><date>2003-07-25</date><risdate>2003</risdate><volume>212</volume><issue>3</issue><spage>377</spage><epage>391</epage><pages>377-391</pages><issn>0012-821X</issn><eissn>1385-013X</eissn><abstract>Pore fluids from two ODP sites at Eastern Mediterranean mud volcanoes have been analyzed for their Cl concentration and their δ
18O and δD isotopic composition. The Cl data span a wide range of concentrations, from extremely depleted with respect to seawater (as low as 60 mM) at the crest of Milano dome (site 970) to strongly enriched (up to 5.4 M) at Napoli dome (site 971). Chloride enrichment is known to be due to dissolving Messinian evaporites, whereas the source of the low-Cl fluid is deduced from stable isotope data presented here. The isotopic composition of the endmember fluid is found to be +10‰ for δ
18O and −32‰ for δD for low- as well as for high-Cl waters. From this signature it can be concluded that neither gas hydrates nor meteoric water play a significant role in the freshening of the pore water. Several other processes altering the δ
18O/δD composition of pore waters are discussed and considered to be of only negligible influence. The process characterizing the isotopic composition of the fluid is found to be clay mineral dehydration (mainly smectite–illite transformation), corresponding to a depth range of 3.5–7 km and an elevated temperature of about 120–165°C. A quantitative estimate shows that this reaction is capable of producing the observed extreme Cl depletion.</abstract><pub>Elsevier B.V</pub><doi>10.1016/S0012-821X(03)00227-9</doi><tpages>15</tpages></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0012-821X |
ispartof | Earth and planetary science letters, 2003-07, Vol.212 (3), p.377-391 |
issn | 0012-821X 1385-013X |
language | eng |
recordid | cdi_proquest_miscellaneous_18021621 |
source | Access via ScienceDirect (Elsevier) |
subjects | clay mineral dehydration clay mineral ion filtration gas hydrates hydrogen isotopes Marine Mediterranean mud volcanoes oxygen isotopes pore water |
title | Fluid–sediment interactions at Eastern Mediterranean mud volcanoes: a stable isotope study from ODP Leg 160 |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-01T17%3A28%3A21IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Fluid%E2%80%93sediment%20interactions%20at%20Eastern%20Mediterranean%20mud%20volcanoes:%20a%20stable%20isotope%20study%20from%20ODP%20Leg%20160&rft.jtitle=Earth%20and%20planetary%20science%20letters&rft.au=D%C3%A4hlmann,%20A&rft.date=2003-07-25&rft.volume=212&rft.issue=3&rft.spage=377&rft.epage=391&rft.pages=377-391&rft.issn=0012-821X&rft.eissn=1385-013X&rft_id=info:doi/10.1016/S0012-821X(03)00227-9&rft_dat=%3Cproquest_cross%3E18021621%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=18021621&rft_id=info:pmid/&rft_els_id=S0012821X03002279&rfr_iscdi=true |