Degassing Driving Magma Hybridization in Plutons: Structural Evidence from the Famatinian Arc in the Puna Plateau, Argentina
- Autores
- Weinberg, Roberto; Ortiz Joya, Guillermo; Vernon, Ron; Araujo, Lucas; Morfulis Geipel, Marcos Nicolas; Sola, Alfonso Manuel; Suzaño, Nestor Omar; Becchio, Raul Alberto
- Año de publicación
- 2026
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Arc magmas are rich in fluids that exsolve forming a volatile phase at some point during ascent and crystallization. Despite expectations that this phase could have a significant impact on the evolution of magma reservoirs, there is relatively little recorded evidence of this impact or even of their passage, other than the upper reaches of the chamber. We hypothesize that this mismatch could be due to a lack of recognition of possible magmatic structures associated with this process. Here, we use meso- and microstructures found in variably disrupted dioritic sills and dykes, forming microdioritic and microgranitic enclaves of a large range of sizes, to explore features that could record the passage of a volatile phase and to argue that its passage facilitated hybridization between the two magmas. We focus on structures formed in three plutons of the Early Paleozoic Famatinian Arc in Argentina.The diorites in these plutons are commonly heterogeneous at cm- to dm-scale and have open and filled miaroles, indicative of the presence of a volatile phase. These miaroles tend to form swarms in the heterogeneous rock that also has quartz ocelli and feldspars with rapakivi texture – features indicative of magma hybridization. These heterogeneous rocks are also associated with a number of curious magmatic structures that we speculate record degassing processes and facilitate hybridization by intensifying melt flow and reactivity between the magmas. These structures indicate that the volatile phase caused bubbly diapirs, gas-driven filter-pressing, local catastrophic transfer of crystals across magmatic contacts, and it likely facilitated pervasive flow of invading leucogranitic melt through the pore space of a mushy diorite. Despite the speculative nature of these conclusions, we argue that there is a range of magmatic structures that remain unexplained and that require magma dynamics that could be explained by flow related to degassing.
Fil: Weinberg, Roberto. Monash University; Australia
Fil: Ortiz Joya, Guillermo. Monash University; Australia
Fil: Vernon, Ron. Macquarie University; Australia
Fil: Araujo, Lucas. Monash University; Australia
Fil: Morfulis Geipel, Marcos Nicolas. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Salta. Instituto de Bio y Geociencias del NOA. Universidad Nacional de Salta. Facultad de Ciencias Naturales. Museo de Ciencias Naturales. Instituto de Bio y Geociencias del NOA; Argentina
Fil: Sola, Alfonso Manuel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Salta. Instituto de Bio y Geociencias del NOA. Universidad Nacional de Salta. Facultad de Ciencias Naturales. Museo de Ciencias Naturales. Instituto de Bio y Geociencias del NOA; Argentina
Fil: Suzaño, Nestor Omar. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Salta. Instituto de Bio y Geociencias del NOA. Universidad Nacional de Salta. Facultad de Ciencias Naturales. Museo de Ciencias Naturales. Instituto de Bio y Geociencias del NOA; Argentina
Fil: Becchio, Raul Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Salta. Instituto de Bio y Geociencias del NOA. Universidad Nacional de Salta. Facultad de Ciencias Naturales. Museo de Ciencias Naturales. Instituto de Bio y Geociencias del NOA; Argentina - Materia
-
degassing
epizonal plutons
magma hybridization
magma mixing
volatile phase - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/290122
Ver los metadatos del registro completo
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Degassing Driving Magma Hybridization in Plutons: Structural Evidence from the Famatinian Arc in the Puna Plateau, ArgentinaWeinberg, RobertoOrtiz Joya, GuillermoVernon, RonAraujo, LucasMorfulis Geipel, Marcos NicolasSola, Alfonso ManuelSuzaño, Nestor OmarBecchio, Raul Albertodegassingepizonal plutonsmagma hybridizationmagma mixingvolatile phasehttps://purl.org/becyt/ford/1.5https://purl.org/becyt/ford/1Arc magmas are rich in fluids that exsolve forming a volatile phase at some point during ascent and crystallization. Despite expectations that this phase could have a significant impact on the evolution of magma reservoirs, there is relatively little recorded evidence of this impact or even of their passage, other than the upper reaches of the chamber. We hypothesize that this mismatch could be due to a lack of recognition of possible magmatic structures associated with this process. Here, we use meso- and microstructures found in variably disrupted dioritic sills and dykes, forming microdioritic and microgranitic enclaves of a large range of sizes, to explore features that could record the passage of a volatile phase and to argue that its passage facilitated hybridization between the two magmas. We focus on structures formed in three plutons of the Early Paleozoic Famatinian Arc in Argentina.The diorites in these plutons are commonly heterogeneous at cm- to dm-scale and have open and filled miaroles, indicative of the presence of a volatile phase. These miaroles tend to form swarms in the heterogeneous rock that also has quartz ocelli and feldspars with rapakivi texture – features indicative of magma hybridization. These heterogeneous rocks are also associated with a number of curious magmatic structures that we speculate record degassing processes and facilitate hybridization by intensifying melt flow and reactivity between the magmas. These structures indicate that the volatile phase caused bubbly diapirs, gas-driven filter-pressing, local catastrophic transfer of crystals across magmatic contacts, and it likely facilitated pervasive flow of invading leucogranitic melt through the pore space of a mushy diorite. Despite the speculative nature of these conclusions, we argue that there is a range of magmatic structures that remain unexplained and that require magma dynamics that could be explained by flow related to degassing.Fil: Weinberg, Roberto. Monash University; AustraliaFil: Ortiz Joya, Guillermo. Monash University; AustraliaFil: Vernon, Ron. Macquarie University; AustraliaFil: Araujo, Lucas. Monash University; AustraliaFil: Morfulis Geipel, Marcos Nicolas. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Salta. Instituto de Bio y Geociencias del NOA. Universidad Nacional de Salta. Facultad de Ciencias Naturales. Museo de Ciencias Naturales. Instituto de Bio y Geociencias del NOA; ArgentinaFil: Sola, Alfonso Manuel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Salta. Instituto de Bio y Geociencias del NOA. Universidad Nacional de Salta. Facultad de Ciencias Naturales. Museo de Ciencias Naturales. Instituto de Bio y Geociencias del NOA; ArgentinaFil: Suzaño, Nestor Omar. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Salta. Instituto de Bio y Geociencias del NOA. Universidad Nacional de Salta. Facultad de Ciencias Naturales. Museo de Ciencias Naturales. Instituto de Bio y Geociencias del NOA; ArgentinaFil: Becchio, Raul Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Salta. Instituto de Bio y Geociencias del NOA. Universidad Nacional de Salta. Facultad de Ciencias Naturales. Museo de Ciencias Naturales. Instituto de Bio y Geociencias del NOA; ArgentinaOxford University Press2026-03info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/290122Weinberg, Roberto; Ortiz Joya, Guillermo; Vernon, Ron; Araujo, Lucas; Morfulis Geipel, Marcos Nicolas; et al.; Degassing Driving Magma Hybridization in Plutons: Structural Evidence from the Famatinian Arc in the Puna Plateau, Argentina; Oxford University Press; Journal Of Petrology; 67; 4; 3-2026; 1-220022-3530CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/petrology/advance-article/doi/10.1093/petrology/egag024/8506967info:eu-repo/semantics/altIdentifier/doi/10.1093/petrology/egag024info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2026-08-25T15:12:27Zoai:ri.conicet.gov.ar:11336/290122instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982026-08-25 15:12:27.972CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
Degassing Driving Magma Hybridization in Plutons: Structural Evidence from the Famatinian Arc in the Puna Plateau, Argentina |
| title |
Degassing Driving Magma Hybridization in Plutons: Structural Evidence from the Famatinian Arc in the Puna Plateau, Argentina |
| spellingShingle |
Degassing Driving Magma Hybridization in Plutons: Structural Evidence from the Famatinian Arc in the Puna Plateau, Argentina Weinberg, Roberto degassing epizonal plutons magma hybridization magma mixing volatile phase |
| title_short |
Degassing Driving Magma Hybridization in Plutons: Structural Evidence from the Famatinian Arc in the Puna Plateau, Argentina |
| title_full |
Degassing Driving Magma Hybridization in Plutons: Structural Evidence from the Famatinian Arc in the Puna Plateau, Argentina |
| title_fullStr |
Degassing Driving Magma Hybridization in Plutons: Structural Evidence from the Famatinian Arc in the Puna Plateau, Argentina |
| title_full_unstemmed |
Degassing Driving Magma Hybridization in Plutons: Structural Evidence from the Famatinian Arc in the Puna Plateau, Argentina |
| title_sort |
Degassing Driving Magma Hybridization in Plutons: Structural Evidence from the Famatinian Arc in the Puna Plateau, Argentina |
| dc.creator.none.fl_str_mv |
Weinberg, Roberto Ortiz Joya, Guillermo Vernon, Ron Araujo, Lucas Morfulis Geipel, Marcos Nicolas Sola, Alfonso Manuel Suzaño, Nestor Omar Becchio, Raul Alberto |
| author |
Weinberg, Roberto |
| author_facet |
Weinberg, Roberto Ortiz Joya, Guillermo Vernon, Ron Araujo, Lucas Morfulis Geipel, Marcos Nicolas Sola, Alfonso Manuel Suzaño, Nestor Omar Becchio, Raul Alberto |
| author_role |
author |
| author2 |
Ortiz Joya, Guillermo Vernon, Ron Araujo, Lucas Morfulis Geipel, Marcos Nicolas Sola, Alfonso Manuel Suzaño, Nestor Omar Becchio, Raul Alberto |
| author2_role |
author author author author author author author |
| dc.subject.none.fl_str_mv |
degassing epizonal plutons magma hybridization magma mixing volatile phase |
| topic |
degassing epizonal plutons magma hybridization magma mixing volatile phase |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.5 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
Arc magmas are rich in fluids that exsolve forming a volatile phase at some point during ascent and crystallization. Despite expectations that this phase could have a significant impact on the evolution of magma reservoirs, there is relatively little recorded evidence of this impact or even of their passage, other than the upper reaches of the chamber. We hypothesize that this mismatch could be due to a lack of recognition of possible magmatic structures associated with this process. Here, we use meso- and microstructures found in variably disrupted dioritic sills and dykes, forming microdioritic and microgranitic enclaves of a large range of sizes, to explore features that could record the passage of a volatile phase and to argue that its passage facilitated hybridization between the two magmas. We focus on structures formed in three plutons of the Early Paleozoic Famatinian Arc in Argentina.The diorites in these plutons are commonly heterogeneous at cm- to dm-scale and have open and filled miaroles, indicative of the presence of a volatile phase. These miaroles tend to form swarms in the heterogeneous rock that also has quartz ocelli and feldspars with rapakivi texture – features indicative of magma hybridization. These heterogeneous rocks are also associated with a number of curious magmatic structures that we speculate record degassing processes and facilitate hybridization by intensifying melt flow and reactivity between the magmas. These structures indicate that the volatile phase caused bubbly diapirs, gas-driven filter-pressing, local catastrophic transfer of crystals across magmatic contacts, and it likely facilitated pervasive flow of invading leucogranitic melt through the pore space of a mushy diorite. Despite the speculative nature of these conclusions, we argue that there is a range of magmatic structures that remain unexplained and that require magma dynamics that could be explained by flow related to degassing. Fil: Weinberg, Roberto. Monash University; Australia Fil: Ortiz Joya, Guillermo. Monash University; Australia Fil: Vernon, Ron. Macquarie University; Australia Fil: Araujo, Lucas. Monash University; Australia Fil: Morfulis Geipel, Marcos Nicolas. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Salta. Instituto de Bio y Geociencias del NOA. Universidad Nacional de Salta. Facultad de Ciencias Naturales. Museo de Ciencias Naturales. Instituto de Bio y Geociencias del NOA; Argentina Fil: Sola, Alfonso Manuel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Salta. Instituto de Bio y Geociencias del NOA. Universidad Nacional de Salta. Facultad de Ciencias Naturales. Museo de Ciencias Naturales. Instituto de Bio y Geociencias del NOA; Argentina Fil: Suzaño, Nestor Omar. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Salta. Instituto de Bio y Geociencias del NOA. Universidad Nacional de Salta. Facultad de Ciencias Naturales. Museo de Ciencias Naturales. Instituto de Bio y Geociencias del NOA; Argentina Fil: Becchio, Raul Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Salta. Instituto de Bio y Geociencias del NOA. Universidad Nacional de Salta. Facultad de Ciencias Naturales. Museo de Ciencias Naturales. Instituto de Bio y Geociencias del NOA; Argentina |
| description |
Arc magmas are rich in fluids that exsolve forming a volatile phase at some point during ascent and crystallization. Despite expectations that this phase could have a significant impact on the evolution of magma reservoirs, there is relatively little recorded evidence of this impact or even of their passage, other than the upper reaches of the chamber. We hypothesize that this mismatch could be due to a lack of recognition of possible magmatic structures associated with this process. Here, we use meso- and microstructures found in variably disrupted dioritic sills and dykes, forming microdioritic and microgranitic enclaves of a large range of sizes, to explore features that could record the passage of a volatile phase and to argue that its passage facilitated hybridization between the two magmas. We focus on structures formed in three plutons of the Early Paleozoic Famatinian Arc in Argentina.The diorites in these plutons are commonly heterogeneous at cm- to dm-scale and have open and filled miaroles, indicative of the presence of a volatile phase. These miaroles tend to form swarms in the heterogeneous rock that also has quartz ocelli and feldspars with rapakivi texture – features indicative of magma hybridization. These heterogeneous rocks are also associated with a number of curious magmatic structures that we speculate record degassing processes and facilitate hybridization by intensifying melt flow and reactivity between the magmas. These structures indicate that the volatile phase caused bubbly diapirs, gas-driven filter-pressing, local catastrophic transfer of crystals across magmatic contacts, and it likely facilitated pervasive flow of invading leucogranitic melt through the pore space of a mushy diorite. Despite the speculative nature of these conclusions, we argue that there is a range of magmatic structures that remain unexplained and that require magma dynamics that could be explained by flow related to degassing. |
| publishDate |
2026 |
| dc.date.none.fl_str_mv |
2026-03 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
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http://hdl.handle.net/11336/290122 Weinberg, Roberto; Ortiz Joya, Guillermo; Vernon, Ron; Araujo, Lucas; Morfulis Geipel, Marcos Nicolas; et al.; Degassing Driving Magma Hybridization in Plutons: Structural Evidence from the Famatinian Arc in the Puna Plateau, Argentina; Oxford University Press; Journal Of Petrology; 67; 4; 3-2026; 1-22 0022-3530 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/290122 |
| identifier_str_mv |
Weinberg, Roberto; Ortiz Joya, Guillermo; Vernon, Ron; Araujo, Lucas; Morfulis Geipel, Marcos Nicolas; et al.; Degassing Driving Magma Hybridization in Plutons: Structural Evidence from the Famatinian Arc in the Puna Plateau, Argentina; Oxford University Press; Journal Of Petrology; 67; 4; 3-2026; 1-22 0022-3530 CONICET Digital CONICET |
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eng |
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eng |
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Oxford University Press |
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Oxford University Press |
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CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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