The Bajada del Diablo astrobleme-strewn field, central Patagonia Argentina: Extending the exploration to surrounding areas
- Autores
- Acevedo, Rogelio Daniel; Rabassa, Jorge Oscar; Ponce, Juan Federico; Martínez, Oscar Alfredo; Orgeira, Maria Julia; Prezzi, Claudia Beatriz; Corbella, Jorge Hugo; Gonzalez Guillot, Mauricio Alberto; Rocca, Maximiliano; Subías, Ignacio; Vasquez, Carlos Alberto
- Año de publicación
- 2012
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The Bajada del Diablo astrobleme-strewn field is a huge domain of enigmatic circular structures located in Central Patagonia. Three more localities are herein described, adding to the first area studied so far (Acevedo et al., 2009). Taking into consideration the four areas, a single, blurred crater dispersion ellipse has been identified. The four sectors have been now investigated, mapped and georeferred, and their circular structures,with a total of 189, some of them partially obliterated by erosion or sediment accumulation, were identified by remote sensing techniques, but many of them have been evaluated in situ and interpreted as impact craters. Moreover, two of the structures have been surveyed in detail in the field using a total station instrument. In addition to the previously known occurrence of circular structures on the Eruptive Complex Quiñelaf (Miocene basalts), the Pampa Sastre Fm. (Pliocene conglomerates) and the Pleistocene pediment gravels and sands, and the geomorphological inferences that have suggested the extraterrestrial origin of this event (since no other natural Earth surface process could be responsible of their formation), it should be now added the recurrent absence of the Pliocene stratigraphic unit at the bottom of the craters found on the pediment gravel and sands . Its removal has been interpreted as directly related to the impact, according to the magnetometric record of existing magnetic anomalies. Other preliminary observations on the collected samples, glass, breccias and, most relevant, Fe-Nibearing spherules picked up within the impact zones, are herein discussed. Two hypotheses have been put forward about the nature of the possible impacting object that formed these astroblemes which, fragmented in hundreds of pieces, hit the surface of the Earth perhaps in Middle Pleistocene times. One of them is related to a desintegrated asteroid of the rubble-pile type, whereas the second hypothesis refers to the collision of a split comet with the Earth surface, being this the most probable since no meteorite fragments have been found so far.
Fil: Acevedo, Rogelio Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Austral de Investigaciones Científicas; Argentina
Fil: Rabassa, Jorge Oscar. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Austral de Investigaciones Científicas; Argentina. Universidad Nacional de la Patagonia "San Juan Bosco"; Argentina. Universidad Nacional de Tierra del Fuego; Argentina
Fil: Ponce, Juan Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Austral de Investigaciones Científicas; Argentina
Fil: Martínez, Oscar Alfredo. Universidad Nacional de la Patagonia "San Juan Bosco"; Argentina
Fil: Orgeira, Maria Julia. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires; Argentina
Fil: Prezzi, Claudia Beatriz. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires; Argentina
Fil: Corbella, Jorge Hugo. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Parque Centenario. Museo Argentino de Ciencias Naturales "Bernardino Rivadavia"; Argentina. Universidad Nacional de la Patagonia Austral; Argentina
Fil: Gonzalez Guillot, Mauricio Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Austral de Investigaciones Científicas; Argentina
Fil: Rocca, Maximiliano. Mendoza 2779; Argentina
Fil: Subías, Ignacio. Universidad de Zaragoza; España
Fil: Vasquez, Carlos Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires; Argentina - Materia
-
Meteoritos
Cráteres de Impacto
Patagonia
Geofísica - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/268842
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The Bajada del Diablo astrobleme-strewn field, central Patagonia Argentina: Extending the exploration to surrounding areasAcevedo, Rogelio DanielRabassa, Jorge OscarPonce, Juan FedericoMartínez, Oscar AlfredoOrgeira, Maria JuliaPrezzi, Claudia BeatrizCorbella, Jorge HugoGonzalez Guillot, Mauricio AlbertoRocca, MaximilianoSubías, IgnacioVasquez, Carlos AlbertoMeteoritosCráteres de ImpactoPatagoniaGeofísicahttps://purl.org/becyt/ford/1.5https://purl.org/becyt/ford/1The Bajada del Diablo astrobleme-strewn field is a huge domain of enigmatic circular structures located in Central Patagonia. Three more localities are herein described, adding to the first area studied so far (Acevedo et al., 2009). Taking into consideration the four areas, a single, blurred crater dispersion ellipse has been identified. The four sectors have been now investigated, mapped and georeferred, and their circular structures,with a total of 189, some of them partially obliterated by erosion or sediment accumulation, were identified by remote sensing techniques, but many of them have been evaluated in situ and interpreted as impact craters. Moreover, two of the structures have been surveyed in detail in the field using a total station instrument. In addition to the previously known occurrence of circular structures on the Eruptive Complex Quiñelaf (Miocene basalts), the Pampa Sastre Fm. (Pliocene conglomerates) and the Pleistocene pediment gravels and sands, and the geomorphological inferences that have suggested the extraterrestrial origin of this event (since no other natural Earth surface process could be responsible of their formation), it should be now added the recurrent absence of the Pliocene stratigraphic unit at the bottom of the craters found on the pediment gravel and sands . Its removal has been interpreted as directly related to the impact, according to the magnetometric record of existing magnetic anomalies. Other preliminary observations on the collected samples, glass, breccias and, most relevant, Fe-Nibearing spherules picked up within the impact zones, are herein discussed. Two hypotheses have been put forward about the nature of the possible impacting object that formed these astroblemes which, fragmented in hundreds of pieces, hit the surface of the Earth perhaps in Middle Pleistocene times. One of them is related to a desintegrated asteroid of the rubble-pile type, whereas the second hypothesis refers to the collision of a split comet with the Earth surface, being this the most probable since no meteorite fragments have been found so far.Fil: Acevedo, Rogelio Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Austral de Investigaciones Científicas; ArgentinaFil: Rabassa, Jorge Oscar. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Austral de Investigaciones Científicas; Argentina. Universidad Nacional de la Patagonia "San Juan Bosco"; Argentina. Universidad Nacional de Tierra del Fuego; ArgentinaFil: Ponce, Juan Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Austral de Investigaciones Científicas; ArgentinaFil: Martínez, Oscar Alfredo. Universidad Nacional de la Patagonia "San Juan Bosco"; ArgentinaFil: Orgeira, Maria Julia. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires; ArgentinaFil: Prezzi, Claudia Beatriz. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires; ArgentinaFil: Corbella, Jorge Hugo. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Parque Centenario. Museo Argentino de Ciencias Naturales "Bernardino Rivadavia"; Argentina. Universidad Nacional de la Patagonia Austral; ArgentinaFil: Gonzalez Guillot, Mauricio Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Austral de Investigaciones Científicas; ArgentinaFil: Rocca, Maximiliano. Mendoza 2779; ArgentinaFil: Subías, Ignacio. Universidad de Zaragoza; EspañaFil: Vasquez, Carlos Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires; ArgentinaElsevier Science2012-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfapplication/pdfapplication/pdfapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/268842Acevedo, Rogelio Daniel; Rabassa, Jorge Oscar; Ponce, Juan Federico; Martínez, Oscar Alfredo; Orgeira, Maria Julia; et al.; The Bajada del Diablo astrobleme-strewn field, central Patagonia Argentina: Extending the exploration to surrounding areas; Elsevier Science; Geomorphology; 169-170; 10-2012; 151-1640169-555XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/abs/pii/S0169555X12001936info:eu-repo/semantics/altIdentifier/doi/10.1016/j.geomorph.2012.04.020info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:19:53Zoai:ri.conicet.gov.ar:11336/268842instacron: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:34982025-09-29 10:19:53.545CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
The Bajada del Diablo astrobleme-strewn field, central Patagonia Argentina: Extending the exploration to surrounding areas |
title |
The Bajada del Diablo astrobleme-strewn field, central Patagonia Argentina: Extending the exploration to surrounding areas |
spellingShingle |
The Bajada del Diablo astrobleme-strewn field, central Patagonia Argentina: Extending the exploration to surrounding areas Acevedo, Rogelio Daniel Meteoritos Cráteres de Impacto Patagonia Geofísica |
title_short |
The Bajada del Diablo astrobleme-strewn field, central Patagonia Argentina: Extending the exploration to surrounding areas |
title_full |
The Bajada del Diablo astrobleme-strewn field, central Patagonia Argentina: Extending the exploration to surrounding areas |
title_fullStr |
The Bajada del Diablo astrobleme-strewn field, central Patagonia Argentina: Extending the exploration to surrounding areas |
title_full_unstemmed |
The Bajada del Diablo astrobleme-strewn field, central Patagonia Argentina: Extending the exploration to surrounding areas |
title_sort |
The Bajada del Diablo astrobleme-strewn field, central Patagonia Argentina: Extending the exploration to surrounding areas |
dc.creator.none.fl_str_mv |
Acevedo, Rogelio Daniel Rabassa, Jorge Oscar Ponce, Juan Federico Martínez, Oscar Alfredo Orgeira, Maria Julia Prezzi, Claudia Beatriz Corbella, Jorge Hugo Gonzalez Guillot, Mauricio Alberto Rocca, Maximiliano Subías, Ignacio Vasquez, Carlos Alberto |
author |
Acevedo, Rogelio Daniel |
author_facet |
Acevedo, Rogelio Daniel Rabassa, Jorge Oscar Ponce, Juan Federico Martínez, Oscar Alfredo Orgeira, Maria Julia Prezzi, Claudia Beatriz Corbella, Jorge Hugo Gonzalez Guillot, Mauricio Alberto Rocca, Maximiliano Subías, Ignacio Vasquez, Carlos Alberto |
author_role |
author |
author2 |
Rabassa, Jorge Oscar Ponce, Juan Federico Martínez, Oscar Alfredo Orgeira, Maria Julia Prezzi, Claudia Beatriz Corbella, Jorge Hugo Gonzalez Guillot, Mauricio Alberto Rocca, Maximiliano Subías, Ignacio Vasquez, Carlos Alberto |
author2_role |
author author author author author author author author author author |
dc.subject.none.fl_str_mv |
Meteoritos Cráteres de Impacto Patagonia Geofísica |
topic |
Meteoritos Cráteres de Impacto Patagonia Geofísica |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.5 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
The Bajada del Diablo astrobleme-strewn field is a huge domain of enigmatic circular structures located in Central Patagonia. Three more localities are herein described, adding to the first area studied so far (Acevedo et al., 2009). Taking into consideration the four areas, a single, blurred crater dispersion ellipse has been identified. The four sectors have been now investigated, mapped and georeferred, and their circular structures,with a total of 189, some of them partially obliterated by erosion or sediment accumulation, were identified by remote sensing techniques, but many of them have been evaluated in situ and interpreted as impact craters. Moreover, two of the structures have been surveyed in detail in the field using a total station instrument. In addition to the previously known occurrence of circular structures on the Eruptive Complex Quiñelaf (Miocene basalts), the Pampa Sastre Fm. (Pliocene conglomerates) and the Pleistocene pediment gravels and sands, and the geomorphological inferences that have suggested the extraterrestrial origin of this event (since no other natural Earth surface process could be responsible of their formation), it should be now added the recurrent absence of the Pliocene stratigraphic unit at the bottom of the craters found on the pediment gravel and sands . Its removal has been interpreted as directly related to the impact, according to the magnetometric record of existing magnetic anomalies. Other preliminary observations on the collected samples, glass, breccias and, most relevant, Fe-Nibearing spherules picked up within the impact zones, are herein discussed. Two hypotheses have been put forward about the nature of the possible impacting object that formed these astroblemes which, fragmented in hundreds of pieces, hit the surface of the Earth perhaps in Middle Pleistocene times. One of them is related to a desintegrated asteroid of the rubble-pile type, whereas the second hypothesis refers to the collision of a split comet with the Earth surface, being this the most probable since no meteorite fragments have been found so far. Fil: Acevedo, Rogelio Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Austral de Investigaciones Científicas; Argentina Fil: Rabassa, Jorge Oscar. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Austral de Investigaciones Científicas; Argentina. Universidad Nacional de la Patagonia "San Juan Bosco"; Argentina. Universidad Nacional de Tierra del Fuego; Argentina Fil: Ponce, Juan Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Austral de Investigaciones Científicas; Argentina Fil: Martínez, Oscar Alfredo. Universidad Nacional de la Patagonia "San Juan Bosco"; Argentina Fil: Orgeira, Maria Julia. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires; Argentina Fil: Prezzi, Claudia Beatriz. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires; Argentina Fil: Corbella, Jorge Hugo. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Parque Centenario. Museo Argentino de Ciencias Naturales "Bernardino Rivadavia"; Argentina. Universidad Nacional de la Patagonia Austral; Argentina Fil: Gonzalez Guillot, Mauricio Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Austral de Investigaciones Científicas; Argentina Fil: Rocca, Maximiliano. Mendoza 2779; Argentina Fil: Subías, Ignacio. Universidad de Zaragoza; España Fil: Vasquez, Carlos Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires; Argentina |
description |
The Bajada del Diablo astrobleme-strewn field is a huge domain of enigmatic circular structures located in Central Patagonia. Three more localities are herein described, adding to the first area studied so far (Acevedo et al., 2009). Taking into consideration the four areas, a single, blurred crater dispersion ellipse has been identified. The four sectors have been now investigated, mapped and georeferred, and their circular structures,with a total of 189, some of them partially obliterated by erosion or sediment accumulation, were identified by remote sensing techniques, but many of them have been evaluated in situ and interpreted as impact craters. Moreover, two of the structures have been surveyed in detail in the field using a total station instrument. In addition to the previously known occurrence of circular structures on the Eruptive Complex Quiñelaf (Miocene basalts), the Pampa Sastre Fm. (Pliocene conglomerates) and the Pleistocene pediment gravels and sands, and the geomorphological inferences that have suggested the extraterrestrial origin of this event (since no other natural Earth surface process could be responsible of their formation), it should be now added the recurrent absence of the Pliocene stratigraphic unit at the bottom of the craters found on the pediment gravel and sands . Its removal has been interpreted as directly related to the impact, according to the magnetometric record of existing magnetic anomalies. Other preliminary observations on the collected samples, glass, breccias and, most relevant, Fe-Nibearing spherules picked up within the impact zones, are herein discussed. Two hypotheses have been put forward about the nature of the possible impacting object that formed these astroblemes which, fragmented in hundreds of pieces, hit the surface of the Earth perhaps in Middle Pleistocene times. One of them is related to a desintegrated asteroid of the rubble-pile type, whereas the second hypothesis refers to the collision of a split comet with the Earth surface, being this the most probable since no meteorite fragments have been found so far. |
publishDate |
2012 |
dc.date.none.fl_str_mv |
2012-10 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/268842 Acevedo, Rogelio Daniel; Rabassa, Jorge Oscar; Ponce, Juan Federico; Martínez, Oscar Alfredo; Orgeira, Maria Julia; et al.; The Bajada del Diablo astrobleme-strewn field, central Patagonia Argentina: Extending the exploration to surrounding areas; Elsevier Science; Geomorphology; 169-170; 10-2012; 151-164 0169-555X CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/268842 |
identifier_str_mv |
Acevedo, Rogelio Daniel; Rabassa, Jorge Oscar; Ponce, Juan Federico; Martínez, Oscar Alfredo; Orgeira, Maria Julia; et al.; The Bajada del Diablo astrobleme-strewn field, central Patagonia Argentina: Extending the exploration to surrounding areas; Elsevier Science; Geomorphology; 169-170; 10-2012; 151-164 0169-555X CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/abs/pii/S0169555X12001936 info:eu-repo/semantics/altIdentifier/doi/10.1016/j.geomorph.2012.04.020 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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application/pdf application/pdf application/pdf application/pdf application/pdf application/pdf application/pdf application/pdf application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
Elsevier Science |
publisher.none.fl_str_mv |
Elsevier Science |
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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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