40Ar/39Ar dating of the eruptive history of Mount Erebus, Antarctica: volcano evolution
Mt. Erebus, a 3,794-meter-high active polygenetic stratovolcano, is composed of voluminous anorthoclase-phyric tephriphonolite and phonolite lavas overlying unknown volumes of poorly exposed, less differentiated lavas. The older basanite to phonotephrite lavas crop out on Fang Ridge, an eroded remna...
Gespeichert in:
Veröffentlicht in: | Bulletin of volcanology 2004-12, Vol.66 (8), p.671-686 |
---|---|
Hauptverfasser: | , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | 686 |
---|---|
container_issue | 8 |
container_start_page | 671 |
container_title | Bulletin of volcanology |
container_volume | 66 |
creator | ESSER, Richard P KYLE, Philip R MCINTOSH, William C |
description | Mt. Erebus, a 3,794-meter-high active polygenetic stratovolcano, is composed of voluminous anorthoclase-phyric tephriphonolite and phonolite lavas overlying unknown volumes of poorly exposed, less differentiated lavas. The older basanite to phonotephrite lavas crop out on Fang Ridge, an eroded remnant of a proto-Erebus volcano and at other isolated locations on the flanks of the Mt. Erebus edifice. Anorthoclase feldspars in the phonolitic lavas are large (~10 cm), abundant (~30-40%) and contain numerous melt inclusions. Although excess argon is known to exist within the melt inclusions, rigorous sample preparation was used to remove the majority of the contaminant. Twenty-five sample sites were dated by the ^sup 40^Ar/^sup 39^Ar method (using 20 anorthoclase, 5 plagioclase and 9 groundmass concentrates) to examine the eruptive history of the volcano. Cape Barne, the oldest site, is 1,311±16 ka and represents the first of three stages of eruptive activity on the Mt. Erebus edifice. It shows a transition from sub-aqueous to sub-aerial volcanism that may mark the initiation of proto-Erebus eruptive activity. It is inferred that a further ~300 ky of basanitic/phonotephritic volcanism built a low, broad platform shield volcano. Cessation of the shield-building phase is marked by eruptions at Fang Ridge at ~1,000 ka. The termination of proto-Erebus eruptive activity is marked by the stratigraphically highest flow at Fang Ridge (758±20 ka). Younger lavas (~550-250 ka) on a modern-Erebus edifice are characterized by phonotephrites, tephriphonolites and trachytes. Plagioclase-phyric phonotephrite from coastal and flank flows yield ages between 531±38 and 368±18 ka. The initiation of anorthoclase tephriphonolite occurred in the southwest sector of the volcano at and around Turks Head (243±10 ka). A short pulse of effusive activity marked by crustal contamination occurred ~160 ka as indicated by at least two trachytic flows (157±6 and 166±10 ka). Most anorthoclase-phyric lavas, characteristic of Mt. Erebus, are less than 250 ka. All Mt. Erebus flows between about 250 and 90 ka are anorthoclase tephriphonolite in composition.[PUBLICATION ABSTRACT] |
doi_str_mv | 10.1007/s00445-004-0354-x |
format | Article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_journals_613238664</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2083128541</sourcerecordid><originalsourceid>FETCH-LOGICAL-c298t-e084fbd9c103ae68e822f0b414f7f50bffa8ae826a119b2ef1f99bcde9fbdea43</originalsourceid><addsrcrecordid>eNpFUE1LAzEUDKJgrf4Ab0HwZuzLJrtNvC1SP6DiRfEYsmlit9RNTbKl_fdmacHLvMe8mXkwCF1TuKcA00kE4LwkGQmwkpPdCRpRzgoCgspTNIKiFERIgHN0EeMKIB-r6Qh9cajDhMk64IVObfeNvcNpabEN_Sa1W4uXbUw-7Af-zfddwrNgmz7e4bpLOpjUGv2At35tdOexzUufWt9dojOn19FeHecYfT7NPh5fyPz9-fWxnhNTSJGIBcFds5CGAtO2ElYUhYOGU-6mroTGOS10JitNqWwK66iTsjELK7PLas7G6OaQuwn-t7cxqZXvQ5dfqoqygomqGkT0IDLBxxisU5vQ_uiwVxTUUJ861KcyqqE-tcue22OwjkavXdCdaeO_sWJMlFPJ_gAo-HCU</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>613238664</pqid></control><display><type>article</type><title>40Ar/39Ar dating of the eruptive history of Mount Erebus, Antarctica: volcano evolution</title><source>SpringerLink Journals</source><creator>ESSER, Richard P ; KYLE, Philip R ; MCINTOSH, William C</creator><creatorcontrib>ESSER, Richard P ; KYLE, Philip R ; MCINTOSH, William C</creatorcontrib><description>Mt. Erebus, a 3,794-meter-high active polygenetic stratovolcano, is composed of voluminous anorthoclase-phyric tephriphonolite and phonolite lavas overlying unknown volumes of poorly exposed, less differentiated lavas. The older basanite to phonotephrite lavas crop out on Fang Ridge, an eroded remnant of a proto-Erebus volcano and at other isolated locations on the flanks of the Mt. Erebus edifice. Anorthoclase feldspars in the phonolitic lavas are large (~10 cm), abundant (~30-40%) and contain numerous melt inclusions. Although excess argon is known to exist within the melt inclusions, rigorous sample preparation was used to remove the majority of the contaminant. Twenty-five sample sites were dated by the ^sup 40^Ar/^sup 39^Ar method (using 20 anorthoclase, 5 plagioclase and 9 groundmass concentrates) to examine the eruptive history of the volcano. Cape Barne, the oldest site, is 1,311±16 ka and represents the first of three stages of eruptive activity on the Mt. Erebus edifice. It shows a transition from sub-aqueous to sub-aerial volcanism that may mark the initiation of proto-Erebus eruptive activity. It is inferred that a further ~300 ky of basanitic/phonotephritic volcanism built a low, broad platform shield volcano. Cessation of the shield-building phase is marked by eruptions at Fang Ridge at ~1,000 ka. The termination of proto-Erebus eruptive activity is marked by the stratigraphically highest flow at Fang Ridge (758±20 ka). Younger lavas (~550-250 ka) on a modern-Erebus edifice are characterized by phonotephrites, tephriphonolites and trachytes. Plagioclase-phyric phonotephrite from coastal and flank flows yield ages between 531±38 and 368±18 ka. The initiation of anorthoclase tephriphonolite occurred in the southwest sector of the volcano at and around Turks Head (243±10 ka). A short pulse of effusive activity marked by crustal contamination occurred ~160 ka as indicated by at least two trachytic flows (157±6 and 166±10 ka). Most anorthoclase-phyric lavas, characteristic of Mt. Erebus, are less than 250 ka. All Mt. Erebus flows between about 250 and 90 ka are anorthoclase tephriphonolite in composition.[PUBLICATION ABSTRACT]</description><identifier>ISSN: 0258-8900</identifier><identifier>EISSN: 1432-0819</identifier><identifier>DOI: 10.1007/s00445-004-0354-x</identifier><identifier>CODEN: BUVOEW</identifier><language>eng</language><publisher>Heidelberg: Springer</publisher><subject>Contaminants ; Crystalline rocks ; Earth sciences ; Earth, ocean, space ; Engineering and environment geology. Geothermics ; Exact sciences and technology ; Igneous and metamorphic rocks petrology, volcanic processes, magmas ; Mineralogy ; Natural hazards: prediction, damages, etc ; Sample preparation ; Volcanoes ; Volcanology</subject><ispartof>Bulletin of volcanology, 2004-12, Vol.66 (8), p.671-686</ispartof><rights>2005 INIST-CNRS</rights><rights>Springer-Verlag 2004</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c298t-e084fbd9c103ae68e822f0b414f7f50bffa8ae826a119b2ef1f99bcde9fbdea43</citedby><cites>FETCH-LOGICAL-c298t-e084fbd9c103ae68e822f0b414f7f50bffa8ae826a119b2ef1f99bcde9fbdea43</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=16338579$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>ESSER, Richard P</creatorcontrib><creatorcontrib>KYLE, Philip R</creatorcontrib><creatorcontrib>MCINTOSH, William C</creatorcontrib><title>40Ar/39Ar dating of the eruptive history of Mount Erebus, Antarctica: volcano evolution</title><title>Bulletin of volcanology</title><description>Mt. Erebus, a 3,794-meter-high active polygenetic stratovolcano, is composed of voluminous anorthoclase-phyric tephriphonolite and phonolite lavas overlying unknown volumes of poorly exposed, less differentiated lavas. The older basanite to phonotephrite lavas crop out on Fang Ridge, an eroded remnant of a proto-Erebus volcano and at other isolated locations on the flanks of the Mt. Erebus edifice. Anorthoclase feldspars in the phonolitic lavas are large (~10 cm), abundant (~30-40%) and contain numerous melt inclusions. Although excess argon is known to exist within the melt inclusions, rigorous sample preparation was used to remove the majority of the contaminant. Twenty-five sample sites were dated by the ^sup 40^Ar/^sup 39^Ar method (using 20 anorthoclase, 5 plagioclase and 9 groundmass concentrates) to examine the eruptive history of the volcano. Cape Barne, the oldest site, is 1,311±16 ka and represents the first of three stages of eruptive activity on the Mt. Erebus edifice. It shows a transition from sub-aqueous to sub-aerial volcanism that may mark the initiation of proto-Erebus eruptive activity. It is inferred that a further ~300 ky of basanitic/phonotephritic volcanism built a low, broad platform shield volcano. Cessation of the shield-building phase is marked by eruptions at Fang Ridge at ~1,000 ka. The termination of proto-Erebus eruptive activity is marked by the stratigraphically highest flow at Fang Ridge (758±20 ka). Younger lavas (~550-250 ka) on a modern-Erebus edifice are characterized by phonotephrites, tephriphonolites and trachytes. Plagioclase-phyric phonotephrite from coastal and flank flows yield ages between 531±38 and 368±18 ka. The initiation of anorthoclase tephriphonolite occurred in the southwest sector of the volcano at and around Turks Head (243±10 ka). A short pulse of effusive activity marked by crustal contamination occurred ~160 ka as indicated by at least two trachytic flows (157±6 and 166±10 ka). Most anorthoclase-phyric lavas, characteristic of Mt. Erebus, are less than 250 ka. All Mt. Erebus flows between about 250 and 90 ka are anorthoclase tephriphonolite in composition.[PUBLICATION ABSTRACT]</description><subject>Contaminants</subject><subject>Crystalline rocks</subject><subject>Earth sciences</subject><subject>Earth, ocean, space</subject><subject>Engineering and environment geology. Geothermics</subject><subject>Exact sciences and technology</subject><subject>Igneous and metamorphic rocks petrology, volcanic processes, magmas</subject><subject>Mineralogy</subject><subject>Natural hazards: prediction, damages, etc</subject><subject>Sample preparation</subject><subject>Volcanoes</subject><subject>Volcanology</subject><issn>0258-8900</issn><issn>1432-0819</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2004</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GNUQQ</sourceid><recordid>eNpFUE1LAzEUDKJgrf4Ab0HwZuzLJrtNvC1SP6DiRfEYsmlit9RNTbKl_fdmacHLvMe8mXkwCF1TuKcA00kE4LwkGQmwkpPdCRpRzgoCgspTNIKiFERIgHN0EeMKIB-r6Qh9cajDhMk64IVObfeNvcNpabEN_Sa1W4uXbUw-7Af-zfddwrNgmz7e4bpLOpjUGv2At35tdOexzUufWt9dojOn19FeHecYfT7NPh5fyPz9-fWxnhNTSJGIBcFds5CGAtO2ElYUhYOGU-6mroTGOS10JitNqWwK66iTsjELK7PLas7G6OaQuwn-t7cxqZXvQ5dfqoqygomqGkT0IDLBxxisU5vQ_uiwVxTUUJ861KcyqqE-tcue22OwjkavXdCdaeO_sWJMlFPJ_gAo-HCU</recordid><startdate>20041201</startdate><enddate>20041201</enddate><creator>ESSER, Richard P</creator><creator>KYLE, Philip R</creator><creator>MCINTOSH, William C</creator><general>Springer</general><general>Springer Nature B.V</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7TG</scope><scope>7TN</scope><scope>7XB</scope><scope>88I</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>F1W</scope><scope>GNUQQ</scope><scope>H96</scope><scope>HCIFZ</scope><scope>KL.</scope><scope>L.G</scope><scope>M2P</scope><scope>PCBAR</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>Q9U</scope></search><sort><creationdate>20041201</creationdate><title>40Ar/39Ar dating of the eruptive history of Mount Erebus, Antarctica: volcano evolution</title><author>ESSER, Richard P ; KYLE, Philip R ; MCINTOSH, William C</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c298t-e084fbd9c103ae68e822f0b414f7f50bffa8ae826a119b2ef1f99bcde9fbdea43</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2004</creationdate><topic>Contaminants</topic><topic>Crystalline rocks</topic><topic>Earth sciences</topic><topic>Earth, ocean, space</topic><topic>Engineering and environment geology. Geothermics</topic><topic>Exact sciences and technology</topic><topic>Igneous and metamorphic rocks petrology, volcanic processes, magmas</topic><topic>Mineralogy</topic><topic>Natural hazards: prediction, damages, etc</topic><topic>Sample preparation</topic><topic>Volcanoes</topic><topic>Volcanology</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>ESSER, Richard P</creatorcontrib><creatorcontrib>KYLE, Philip R</creatorcontrib><creatorcontrib>MCINTOSH, William C</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>ProQuest Central (Corporate)</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Oceanic Abstracts</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Science Database (Alumni Edition)</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Natural Science Collection</collection><collection>Earth, Atmospheric & Aquatic Science Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>ProQuest Central Student</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy & Non-Living Resources</collection><collection>SciTech Premium Collection</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><collection>Science Database</collection><collection>Earth, Atmospheric & Aquatic Science Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central Basic</collection><jtitle>Bulletin of volcanology</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>ESSER, Richard P</au><au>KYLE, Philip R</au><au>MCINTOSH, William C</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>40Ar/39Ar dating of the eruptive history of Mount Erebus, Antarctica: volcano evolution</atitle><jtitle>Bulletin of volcanology</jtitle><date>2004-12-01</date><risdate>2004</risdate><volume>66</volume><issue>8</issue><spage>671</spage><epage>686</epage><pages>671-686</pages><issn>0258-8900</issn><eissn>1432-0819</eissn><coden>BUVOEW</coden><abstract>Mt. Erebus, a 3,794-meter-high active polygenetic stratovolcano, is composed of voluminous anorthoclase-phyric tephriphonolite and phonolite lavas overlying unknown volumes of poorly exposed, less differentiated lavas. The older basanite to phonotephrite lavas crop out on Fang Ridge, an eroded remnant of a proto-Erebus volcano and at other isolated locations on the flanks of the Mt. Erebus edifice. Anorthoclase feldspars in the phonolitic lavas are large (~10 cm), abundant (~30-40%) and contain numerous melt inclusions. Although excess argon is known to exist within the melt inclusions, rigorous sample preparation was used to remove the majority of the contaminant. Twenty-five sample sites were dated by the ^sup 40^Ar/^sup 39^Ar method (using 20 anorthoclase, 5 plagioclase and 9 groundmass concentrates) to examine the eruptive history of the volcano. Cape Barne, the oldest site, is 1,311±16 ka and represents the first of three stages of eruptive activity on the Mt. Erebus edifice. It shows a transition from sub-aqueous to sub-aerial volcanism that may mark the initiation of proto-Erebus eruptive activity. It is inferred that a further ~300 ky of basanitic/phonotephritic volcanism built a low, broad platform shield volcano. Cessation of the shield-building phase is marked by eruptions at Fang Ridge at ~1,000 ka. The termination of proto-Erebus eruptive activity is marked by the stratigraphically highest flow at Fang Ridge (758±20 ka). Younger lavas (~550-250 ka) on a modern-Erebus edifice are characterized by phonotephrites, tephriphonolites and trachytes. Plagioclase-phyric phonotephrite from coastal and flank flows yield ages between 531±38 and 368±18 ka. The initiation of anorthoclase tephriphonolite occurred in the southwest sector of the volcano at and around Turks Head (243±10 ka). A short pulse of effusive activity marked by crustal contamination occurred ~160 ka as indicated by at least two trachytic flows (157±6 and 166±10 ka). Most anorthoclase-phyric lavas, characteristic of Mt. Erebus, are less than 250 ka. All Mt. Erebus flows between about 250 and 90 ka are anorthoclase tephriphonolite in composition.[PUBLICATION ABSTRACT]</abstract><cop>Heidelberg</cop><pub>Springer</pub><doi>10.1007/s00445-004-0354-x</doi><tpages>16</tpages></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0258-8900 |
ispartof | Bulletin of volcanology, 2004-12, Vol.66 (8), p.671-686 |
issn | 0258-8900 1432-0819 |
language | eng |
recordid | cdi_proquest_journals_613238664 |
source | SpringerLink Journals |
subjects | Contaminants Crystalline rocks Earth sciences Earth, ocean, space Engineering and environment geology. Geothermics Exact sciences and technology Igneous and metamorphic rocks petrology, volcanic processes, magmas Mineralogy Natural hazards: prediction, damages, etc Sample preparation Volcanoes Volcanology |
title | 40Ar/39Ar dating of the eruptive history of Mount Erebus, Antarctica: volcano evolution |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-03T10%3A56%3A59IST&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=40Ar/39Ar%20dating%20of%20the%20eruptive%20history%20of%20Mount%20Erebus,%20Antarctica:%20volcano%20evolution&rft.jtitle=Bulletin%20of%20volcanology&rft.au=ESSER,%20Richard%20P&rft.date=2004-12-01&rft.volume=66&rft.issue=8&rft.spage=671&rft.epage=686&rft.pages=671-686&rft.issn=0258-8900&rft.eissn=1432-0819&rft.coden=BUVOEW&rft_id=info:doi/10.1007/s00445-004-0354-x&rft_dat=%3Cproquest_cross%3E2083128541%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=613238664&rft_id=info:pmid/&rfr_iscdi=true |