The temporal evolution of back-arc magmas from the Auca Mahuida shield volcano (Payenia Volcanic Province, Argentina)
In order to better constrain the temporal volcanic activity of the back-arc context in Payenia Volcanic Province (PVP, Argentina), we present new K–Ar dating, petrographic data, major and trace elements from 23 samples collected on the Auca Mahuida shield volcano. Our new data, coupled with publishe...
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description | In order to better constrain the temporal volcanic activity of the back-arc context in Payenia Volcanic Province (PVP, Argentina), we present new K–Ar dating, petrographic data, major and trace elements from 23 samples collected on the Auca Mahuida shield volcano. Our new data, coupled with published data, show that this volcano was built from about 1.8 to 1.0Ma during five volcanic phases, and that Auca Mahuida magmas were extracted from, at least, two slightly different OIB-type mantle sources with a low partial melting rate. The first one, containing more garnet, was located deeper in the mantle, while the second contains more spinel and was thus shallower. The high-MgO basalts (or primitive basalts) and the low-MgO basalts (or evolved basalts), produced from the deeper and shallower lherzolite mantle sources, respectively, are found within each volcanic phase, suggesting that both magmatic reservoirs were sampled during the 1Myr lifetime of the Auca Mahuida volcano. However, a slight increase of the proportion of low-MgO basalts, as well as of magmas sampled from the shallowest source, can be observed through time. Similar overall petrological characteristics found in the Pleistocene–Holocene basaltic rocks from Los Volcanes and Auca Mahuida volcano suggest that they originated from the same magmatic source. Consequently, it can be proposed that the thermal asthenospheric anomaly is probably still present beneath the PVP. Finally, our data further support the hypothesis that the injection of hot asthenosphere with an OIB mantle source signature, which was triggered by the steepening of the Nazca subducting plate, induced the production of a large volume of lavas within the PVP since 2Ma.
•New K–Ar ages constrain the timing of the OIB-type Auca Mahuida volcano.•Auca Mahuida volcano was built during five volcanic-phases from 1.8 to 1.0Ma.•Geochemical data suggest the presence of two distinct mantle sources.•Similar petrologic features with Payún area point to a similar magmatic source.•Injection of OIB-type hot asthenosphere induced the PVP volcanism since 2Ma. |
doi_str_mv | 10.1016/j.jvolgeores.2016.04.043 |
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•New K–Ar ages constrain the timing of the OIB-type Auca Mahuida volcano.•Auca Mahuida volcano was built during five volcanic-phases from 1.8 to 1.0Ma.•Geochemical data suggest the presence of two distinct mantle sources.•Similar petrologic features with Payún area point to a similar magmatic source.•Injection of OIB-type hot asthenosphere induced the PVP volcanism since 2Ma.</description><identifier>ISSN: 0377-0273</identifier><identifier>EISSN: 1872-6097</identifier><identifier>DOI: 10.1016/j.jvolgeores.2016.04.043</identifier><language>eng</language><publisher>Elsevier B.V</publisher><subject>Argentina ; Auca Mahuida volcano ; Basalt ; Evolution ; K–Ar ages ; Los Volcanes ; Magma ; Mantle ; OIB-type magmas ; Payenia Volcanic Province ; Phases ; Sciences of the Universe ; Shields ; Volcanic activity ; Volcanoes</subject><ispartof>Journal of volcanology and geothermal research, 2016-09, Vol.323, p.19-37</ispartof><rights>2016 Elsevier B.V.</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a491t-e9da71d2872d5fd8bf92a556ff978d242105891d8518c745ca3ad7d23fcaf6293</citedby><cites>FETCH-LOGICAL-a491t-e9da71d2872d5fd8bf92a556ff978d242105891d8518c745ca3ad7d23fcaf6293</cites><orcidid>0000-0002-9964-5161 ; 0000-0001-8425-0047</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://dx.doi.org/10.1016/j.jvolgeores.2016.04.043$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>230,314,780,784,885,3550,27924,27925,45995</link.rule.ids><backlink>$$Uhttps://hal.science/hal-01320354$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Pallares, Carlos</creatorcontrib><creatorcontrib>Quidelleur, Xavier</creatorcontrib><creatorcontrib>Gillot, Pierre-Yves</creatorcontrib><creatorcontrib>Kluska, Jean-Michel</creatorcontrib><creatorcontrib>Tchilinguirian, Paul</creatorcontrib><creatorcontrib>Sarda, Philippe</creatorcontrib><title>The temporal evolution of back-arc magmas from the Auca Mahuida shield volcano (Payenia Volcanic Province, Argentina)</title><title>Journal of volcanology and geothermal research</title><description>In order to better constrain the temporal volcanic activity of the back-arc context in Payenia Volcanic Province (PVP, Argentina), we present new K–Ar dating, petrographic data, major and trace elements from 23 samples collected on the Auca Mahuida shield volcano. Our new data, coupled with published data, show that this volcano was built from about 1.8 to 1.0Ma during five volcanic phases, and that Auca Mahuida magmas were extracted from, at least, two slightly different OIB-type mantle sources with a low partial melting rate. The first one, containing more garnet, was located deeper in the mantle, while the second contains more spinel and was thus shallower. The high-MgO basalts (or primitive basalts) and the low-MgO basalts (or evolved basalts), produced from the deeper and shallower lherzolite mantle sources, respectively, are found within each volcanic phase, suggesting that both magmatic reservoirs were sampled during the 1Myr lifetime of the Auca Mahuida volcano. However, a slight increase of the proportion of low-MgO basalts, as well as of magmas sampled from the shallowest source, can be observed through time. Similar overall petrological characteristics found in the Pleistocene–Holocene basaltic rocks from Los Volcanes and Auca Mahuida volcano suggest that they originated from the same magmatic source. Consequently, it can be proposed that the thermal asthenospheric anomaly is probably still present beneath the PVP. Finally, our data further support the hypothesis that the injection of hot asthenosphere with an OIB mantle source signature, which was triggered by the steepening of the Nazca subducting plate, induced the production of a large volume of lavas within the PVP since 2Ma.
•New K–Ar ages constrain the timing of the OIB-type Auca Mahuida volcano.•Auca Mahuida volcano was built during five volcanic-phases from 1.8 to 1.0Ma.•Geochemical data suggest the presence of two distinct mantle sources.•Similar petrologic features with Payún area point to a similar magmatic source.•Injection of OIB-type hot asthenosphere induced the PVP volcanism since 2Ma.</description><subject>Argentina</subject><subject>Auca Mahuida volcano</subject><subject>Basalt</subject><subject>Evolution</subject><subject>K–Ar ages</subject><subject>Los Volcanes</subject><subject>Magma</subject><subject>Mantle</subject><subject>OIB-type magmas</subject><subject>Payenia Volcanic Province</subject><subject>Phases</subject><subject>Sciences of the Universe</subject><subject>Shields</subject><subject>Volcanic activity</subject><subject>Volcanoes</subject><issn>0377-0273</issn><issn>1872-6097</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><recordid>eNqNkU9rGzEQxZfQQt2030HHBLqO_qxW2qMbmqbg0hySXMVEGtlyd1eutGvIt69ch_TYwsDA4zdvpHlVRRhdMsraq91yd4j9BmPCvORFWdKmlDirFkwrXre0U2-qBRVK1ZQr8a56n_OOUsqopotqvt8imXDYxwQ9wWI1TyGOJHryBPZnDcmSATYDZOJTHMhU8NVsgXyH7RwckLwN2DtSBi2MkVzcwTOOAcjjHyFYcpfiIYwWP5FV2uA4hREuP1RvPfQZP7708-rh5sv99W29_vH12_VqXUPTsanGzoFijpd_OOmdfvIdBylb7zulHW84o1J3zGnJtFWNtCDAKceFt-Bb3onz6vLku4Xe7FMYID2bCMHcrtbmqFEmOBWyObDCXpzYfYq_ZsyTGUK22PcwYpyzYVpKoYVsxX-gQvGubaUuqD6hNsWcE_rXZzBqjgGanfkboDkGaGhT6rjl82kUy4UOAZPJNmC5pAsJ7WRcDP82-Q39TakN</recordid><startdate>20160901</startdate><enddate>20160901</enddate><creator>Pallares, Carlos</creator><creator>Quidelleur, Xavier</creator><creator>Gillot, Pierre-Yves</creator><creator>Kluska, Jean-Michel</creator><creator>Tchilinguirian, Paul</creator><creator>Sarda, Philippe</creator><general>Elsevier B.V</general><general>Elsevier</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7ST</scope><scope>7TG</scope><scope>7UA</scope><scope>C1K</scope><scope>F1W</scope><scope>H96</scope><scope>KL.</scope><scope>L.G</scope><scope>SOI</scope><scope>8FD</scope><scope>FR3</scope><scope>H8D</scope><scope>KR7</scope><scope>L7M</scope><scope>1XC</scope><orcidid>https://orcid.org/0000-0002-9964-5161</orcidid><orcidid>https://orcid.org/0000-0001-8425-0047</orcidid></search><sort><creationdate>20160901</creationdate><title>The temporal evolution of back-arc magmas from the Auca Mahuida shield volcano (Payenia Volcanic Province, Argentina)</title><author>Pallares, Carlos ; Quidelleur, Xavier ; Gillot, Pierre-Yves ; Kluska, Jean-Michel ; Tchilinguirian, Paul ; Sarda, Philippe</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a491t-e9da71d2872d5fd8bf92a556ff978d242105891d8518c745ca3ad7d23fcaf6293</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2016</creationdate><topic>Argentina</topic><topic>Auca Mahuida volcano</topic><topic>Basalt</topic><topic>Evolution</topic><topic>K–Ar ages</topic><topic>Los Volcanes</topic><topic>Magma</topic><topic>Mantle</topic><topic>OIB-type magmas</topic><topic>Payenia Volcanic Province</topic><topic>Phases</topic><topic>Sciences of the Universe</topic><topic>Shields</topic><topic>Volcanic activity</topic><topic>Volcanoes</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Pallares, Carlos</creatorcontrib><creatorcontrib>Quidelleur, Xavier</creatorcontrib><creatorcontrib>Gillot, Pierre-Yves</creatorcontrib><creatorcontrib>Kluska, Jean-Michel</creatorcontrib><creatorcontrib>Tchilinguirian, Paul</creatorcontrib><creatorcontrib>Sarda, Philippe</creatorcontrib><collection>CrossRef</collection><collection>Environment Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Water Resources Abstracts</collection><collection>Environmental Sciences and Pollution Management</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>Environment Abstracts</collection><collection>Technology Research Database</collection><collection>Engineering Research Database</collection><collection>Aerospace Database</collection><collection>Civil Engineering Abstracts</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Hyper Article en Ligne (HAL)</collection><jtitle>Journal of volcanology and geothermal research</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Pallares, Carlos</au><au>Quidelleur, Xavier</au><au>Gillot, Pierre-Yves</au><au>Kluska, Jean-Michel</au><au>Tchilinguirian, Paul</au><au>Sarda, Philippe</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The temporal evolution of back-arc magmas from the Auca Mahuida shield volcano (Payenia Volcanic Province, Argentina)</atitle><jtitle>Journal of volcanology and geothermal research</jtitle><date>2016-09-01</date><risdate>2016</risdate><volume>323</volume><spage>19</spage><epage>37</epage><pages>19-37</pages><issn>0377-0273</issn><eissn>1872-6097</eissn><abstract>In order to better constrain the temporal volcanic activity of the back-arc context in Payenia Volcanic Province (PVP, Argentina), we present new K–Ar dating, petrographic data, major and trace elements from 23 samples collected on the Auca Mahuida shield volcano. Our new data, coupled with published data, show that this volcano was built from about 1.8 to 1.0Ma during five volcanic phases, and that Auca Mahuida magmas were extracted from, at least, two slightly different OIB-type mantle sources with a low partial melting rate. The first one, containing more garnet, was located deeper in the mantle, while the second contains more spinel and was thus shallower. The high-MgO basalts (or primitive basalts) and the low-MgO basalts (or evolved basalts), produced from the deeper and shallower lherzolite mantle sources, respectively, are found within each volcanic phase, suggesting that both magmatic reservoirs were sampled during the 1Myr lifetime of the Auca Mahuida volcano. However, a slight increase of the proportion of low-MgO basalts, as well as of magmas sampled from the shallowest source, can be observed through time. Similar overall petrological characteristics found in the Pleistocene–Holocene basaltic rocks from Los Volcanes and Auca Mahuida volcano suggest that they originated from the same magmatic source. Consequently, it can be proposed that the thermal asthenospheric anomaly is probably still present beneath the PVP. Finally, our data further support the hypothesis that the injection of hot asthenosphere with an OIB mantle source signature, which was triggered by the steepening of the Nazca subducting plate, induced the production of a large volume of lavas within the PVP since 2Ma.
•New K–Ar ages constrain the timing of the OIB-type Auca Mahuida volcano.•Auca Mahuida volcano was built during five volcanic-phases from 1.8 to 1.0Ma.•Geochemical data suggest the presence of two distinct mantle sources.•Similar petrologic features with Payún area point to a similar magmatic source.•Injection of OIB-type hot asthenosphere induced the PVP volcanism since 2Ma.</abstract><pub>Elsevier B.V</pub><doi>10.1016/j.jvolgeores.2016.04.043</doi><tpages>19</tpages><orcidid>https://orcid.org/0000-0002-9964-5161</orcidid><orcidid>https://orcid.org/0000-0001-8425-0047</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Argentina Auca Mahuida volcano Basalt Evolution K–Ar ages Los Volcanes Magma Mantle OIB-type magmas Payenia Volcanic Province Phases Sciences of the Universe Shields Volcanic activity Volcanoes |
title | The temporal evolution of back-arc magmas from the Auca Mahuida shield volcano (Payenia Volcanic Province, Argentina) |
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