Interhemispheric time scale for the Hauterivian and its implications for the carbon cycle in the Berriasian-Barremian times

Autores
Martinez, Mathieu; Aguirre Urreta, Beatriz; Schmitz, Mark; Lescano, Marina; Omarini, Julieta; Tunik, Maisa Andrea; Kuhnert, Henning; Concheyro, Andrea; Rawson, Peter; Ramos, Victor; Reboulet, Stéphane; Noclin, Nicolás; Frederichs, Thomas; Nickl, Anna-Leah; Palike, Heiko
Año de publicación
2018
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
Fil: Martinez, Mathieu. Univ. Rennes,CNRS, Geosciences, France.
Fil: Aguirre Urreta, Beatriz. Instituto de Estudios Andinos Don Pablo Groeber, CONICET, Universidad de Buenos Aires; Argentina.
Fil: Schmitz, Mark. Department of Geosciences, Boise State University; USA.
Fil: Lescano, Marina. Instituto de Estudios Andinos Don Pablo Groeber, CONICET, Universidad de Buenos Aires; Argentina.
Fil: Omarini, Julieta. Universidad Nacional de Río Negro. Instituto de Investigación en Paleobiología y Geología. Río Negro, Argentina.
Fil: Tunik, Maisa. Universidad Nacional de Río Negro. Instituto de Investigación en Paleobiología y Geología. Río Negro, Argentina.
Fil: Kuhnert, Henning. MARUM – Center for Marine Environmental Sciences, Universität Bremen; Germany.
Fil: Concheyro, Andrea. Instituto de Estudios Andinos Don Pablo Groeber, CONICET, Universidad de Buenos Aires; Argentina.
Fil: Rawson, Peter. School of Environmental Sciences, University of Hull; UK.
Fil: Ramos, Victor. Instituto de Estudios Andinos Don Pablo Groeber, CONICET, Universidad de Buenos Aires; Argentina.
Fil: Reboulet, Stéphane. Université de Lyon, UCBL, ENSL, CNRS, LGL TPE. France.
Fil: Noclin, Nicolas. Université de Lyon, UCBL, ENSL, CNRS, LGL TPE. France.
Fil: Frederichs, Thomas. MARUM – Center for Marine Environmental Sciences, Universität Bremen; Germany.
Fil: Nickl, Anna-Leah. MARUM – Center for Marine Environmental Sciences, Universität Bremen; Germany.
Fil: Palike, Heiko. MARUM – Center for Marine Environmental Sciences, Universität Bremen; Germany.
Discrepancies in the ages and durations of the Berriasian to Barremian stages still exist between geological data and the proposed geological time scale 2016 (Ogg et al., 2016; Lena et al., 2018). The Hauterivian Stage suffers from these discrepancies as its duration is proposed at 3.92 myr (Ogg et al., 2016), while astrochronology in the Tethyan area (SE France and SE Spain) led to a duration of 5.9 ± 0.4 myr (Martinez et al., 2015). In order to reconcile these durations, we investigated the Agrio Formation in the Neuquén Basin (Argentina). A total of 2,200 samples were collected every 0.25 cm and measured in magnetic susceptibility with a Kappabridge KLY-2. From spectral analyses realised on these MS signals, it appears that the 100-kyr eccentricity is continuously recorded throughout the Agrio Formation, allowing duration calculations. In addition, a new U-Pb age measured on zircons was provided in the upper part of the Agrio Formation using the CA-ID-TIMS method. Thus, four U-Pb ages are now available in the Agrio Formation measured with the U-Pb CA-ID-TIMS (Aguirre-Urreta et al., 2015, 2017). Notably, the astrochronological durations fit with three of the U-Pb ages. A fourth age appears 300 kyr elder than suggested by astrochronology, which may be due to protracted crystallization of zircons in the magmatic chamber. This new data in the Agrio Formation, together with correlations to the Tethyan area, highlights a revision to the duration of the Hauterivian Stage of 5.22 ± 0.11 myr starting at 131.29 ± 0.25 Ma and ending at 126.07 ± 0.25 Ma. The previous overestimate of the duration of the Hauterivian Stage was likely due to distortion of the 405-kyr eccentricity in the sedimentary record, as recent studies document (Laurin et al., 2017; Martinez, 2018). Thanks to these revised ages and previous astsochronological frameworks, we were able to revise the ages and durations of stages from the Late Berriasian to the Barremian-Aptian boundary. A synthesis of δ13C measured on belemnites (Martinez and Dera, 2015) indicate a clear 2.4-myr cycle in the carbon cycle record which fit with the main paleoceanographic events. Higher amplitudes of this cycle are notably observed during major volcanic episodes, suggesting that acceleration of the hydraulic cycle lead to a reinforcement of the long-Milankovitch cycles.
Materia
Ciencias Exactas y Naturales
Interhemispheric Time
Hauterivian
Carbon Cycle
Berriasian-Barremian Times
Ciencias Exactas y Naturales
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
RID-UNRN (UNRN)
Institución
Universidad Nacional de Río Negro
OAI Identificador
oai:rid.unrn.edu.ar:20.500.12049/5745

id RIDUNRN_5c3d0db7da6e5660e43e77860bc20b07
oai_identifier_str oai:rid.unrn.edu.ar:20.500.12049/5745
network_acronym_str RIDUNRN
repository_id_str 4369
network_name_str RID-UNRN (UNRN)
spelling Interhemispheric time scale for the Hauterivian and its implications for the carbon cycle in the Berriasian-Barremian timesMartinez, MathieuAguirre Urreta, BeatrizSchmitz, MarkLescano, MarinaOmarini, JulietaTunik, Maisa AndreaKuhnert, HenningConcheyro, AndreaRawson, PeterRamos, VictorReboulet, StéphaneNoclin, NicolásFrederichs, ThomasNickl, Anna-LeahPalike, HeikoCiencias Exactas y NaturalesInterhemispheric TimeHauterivianCarbon CycleBerriasian-Barremian TimesCiencias Exactas y NaturalesFil: Martinez, Mathieu. Univ. Rennes,CNRS, Geosciences, France.Fil: Aguirre Urreta, Beatriz. Instituto de Estudios Andinos Don Pablo Groeber, CONICET, Universidad de Buenos Aires; Argentina.Fil: Schmitz, Mark. Department of Geosciences, Boise State University; USA.Fil: Lescano, Marina. Instituto de Estudios Andinos Don Pablo Groeber, CONICET, Universidad de Buenos Aires; Argentina.Fil: Omarini, Julieta. Universidad Nacional de Río Negro. Instituto de Investigación en Paleobiología y Geología. Río Negro, Argentina.Fil: Tunik, Maisa. Universidad Nacional de Río Negro. Instituto de Investigación en Paleobiología y Geología. Río Negro, Argentina.Fil: Kuhnert, Henning. MARUM – Center for Marine Environmental Sciences, Universität Bremen; Germany.Fil: Concheyro, Andrea. Instituto de Estudios Andinos Don Pablo Groeber, CONICET, Universidad de Buenos Aires; Argentina.Fil: Rawson, Peter. School of Environmental Sciences, University of Hull; UK.Fil: Ramos, Victor. Instituto de Estudios Andinos Don Pablo Groeber, CONICET, Universidad de Buenos Aires; Argentina.Fil: Reboulet, Stéphane. Université de Lyon, UCBL, ENSL, CNRS, LGL TPE. France.Fil: Noclin, Nicolas. Université de Lyon, UCBL, ENSL, CNRS, LGL TPE. France.Fil: Frederichs, Thomas. MARUM – Center for Marine Environmental Sciences, Universität Bremen; Germany.Fil: Nickl, Anna-Leah. MARUM – Center for Marine Environmental Sciences, Universität Bremen; Germany.Fil: Palike, Heiko. MARUM – Center for Marine Environmental Sciences, Universität Bremen; Germany.Discrepancies in the ages and durations of the Berriasian to Barremian stages still exist between geological data and the proposed geological time scale 2016 (Ogg et al., 2016; Lena et al., 2018). The Hauterivian Stage suffers from these discrepancies as its duration is proposed at 3.92 myr (Ogg et al., 2016), while astrochronology in the Tethyan area (SE France and SE Spain) led to a duration of 5.9 ± 0.4 myr (Martinez et al., 2015). In order to reconcile these durations, we investigated the Agrio Formation in the Neuquén Basin (Argentina). A total of 2,200 samples were collected every 0.25 cm and measured in magnetic susceptibility with a Kappabridge KLY-2. From spectral analyses realised on these MS signals, it appears that the 100-kyr eccentricity is continuously recorded throughout the Agrio Formation, allowing duration calculations. In addition, a new U-Pb age measured on zircons was provided in the upper part of the Agrio Formation using the CA-ID-TIMS method. Thus, four U-Pb ages are now available in the Agrio Formation measured with the U-Pb CA-ID-TIMS (Aguirre-Urreta et al., 2015, 2017). Notably, the astrochronological durations fit with three of the U-Pb ages. A fourth age appears 300 kyr elder than suggested by astrochronology, which may be due to protracted crystallization of zircons in the magmatic chamber. This new data in the Agrio Formation, together with correlations to the Tethyan area, highlights a revision to the duration of the Hauterivian Stage of 5.22 ± 0.11 myr starting at 131.29 ± 0.25 Ma and ending at 126.07 ± 0.25 Ma. The previous overestimate of the duration of the Hauterivian Stage was likely due to distortion of the 405-kyr eccentricity in the sedimentary record, as recent studies document (Laurin et al., 2017; Martinez, 2018). Thanks to these revised ages and previous astsochronological frameworks, we were able to revise the ages and durations of stages from the Late Berriasian to the Barremian-Aptian boundary. A synthesis of δ13C measured on belemnites (Martinez and Dera, 2015) indicate a clear 2.4-myr cycle in the carbon cycle record which fit with the main paleoceanographic events. Higher amplitudes of this cycle are notably observed during major volcanic episodes, suggesting that acceleration of the hydraulic cycle lead to a reinforcement of the long-Milankovitch cycles.2018info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfhttps://www.thejk.org.uk/jk2018/https://php5.univ-brest.fr/conference/ocs/index.php/JK2018/JK2018/paper/view/515http://rid.unrn.edu.ar/handle/20.500.12049/5745engJK2018info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/4.0/reponame:RID-UNRN (UNRN)instname:Universidad Nacional de Río Negro2025-10-23T11:17:33Zoai:rid.unrn.edu.ar:20.500.12049/5745instacron:UNRNInstitucionalhttps://rid.unrn.edu.ar/jspui/Universidad públicaNo correspondehttps://rid.unrn.edu.ar/oai/snrdrid@unrn.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:43692025-10-23 11:17:34.331RID-UNRN (UNRN) - Universidad Nacional de Río Negrofalse
dc.title.none.fl_str_mv Interhemispheric time scale for the Hauterivian and its implications for the carbon cycle in the Berriasian-Barremian times
title Interhemispheric time scale for the Hauterivian and its implications for the carbon cycle in the Berriasian-Barremian times
spellingShingle Interhemispheric time scale for the Hauterivian and its implications for the carbon cycle in the Berriasian-Barremian times
Martinez, Mathieu
Ciencias Exactas y Naturales
Interhemispheric Time
Hauterivian
Carbon Cycle
Berriasian-Barremian Times
Ciencias Exactas y Naturales
title_short Interhemispheric time scale for the Hauterivian and its implications for the carbon cycle in the Berriasian-Barremian times
title_full Interhemispheric time scale for the Hauterivian and its implications for the carbon cycle in the Berriasian-Barremian times
title_fullStr Interhemispheric time scale for the Hauterivian and its implications for the carbon cycle in the Berriasian-Barremian times
title_full_unstemmed Interhemispheric time scale for the Hauterivian and its implications for the carbon cycle in the Berriasian-Barremian times
title_sort Interhemispheric time scale for the Hauterivian and its implications for the carbon cycle in the Berriasian-Barremian times
dc.creator.none.fl_str_mv Martinez, Mathieu
Aguirre Urreta, Beatriz
Schmitz, Mark
Lescano, Marina
Omarini, Julieta
Tunik, Maisa Andrea
Kuhnert, Henning
Concheyro, Andrea
Rawson, Peter
Ramos, Victor
Reboulet, Stéphane
Noclin, Nicolás
Frederichs, Thomas
Nickl, Anna-Leah
Palike, Heiko
author Martinez, Mathieu
author_facet Martinez, Mathieu
Aguirre Urreta, Beatriz
Schmitz, Mark
Lescano, Marina
Omarini, Julieta
Tunik, Maisa Andrea
Kuhnert, Henning
Concheyro, Andrea
Rawson, Peter
Ramos, Victor
Reboulet, Stéphane
Noclin, Nicolás
Frederichs, Thomas
Nickl, Anna-Leah
Palike, Heiko
author_role author
author2 Aguirre Urreta, Beatriz
Schmitz, Mark
Lescano, Marina
Omarini, Julieta
Tunik, Maisa Andrea
Kuhnert, Henning
Concheyro, Andrea
Rawson, Peter
Ramos, Victor
Reboulet, Stéphane
Noclin, Nicolás
Frederichs, Thomas
Nickl, Anna-Leah
Palike, Heiko
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Ciencias Exactas y Naturales
Interhemispheric Time
Hauterivian
Carbon Cycle
Berriasian-Barremian Times
Ciencias Exactas y Naturales
topic Ciencias Exactas y Naturales
Interhemispheric Time
Hauterivian
Carbon Cycle
Berriasian-Barremian Times
Ciencias Exactas y Naturales
dc.description.none.fl_txt_mv Fil: Martinez, Mathieu. Univ. Rennes,CNRS, Geosciences, France.
Fil: Aguirre Urreta, Beatriz. Instituto de Estudios Andinos Don Pablo Groeber, CONICET, Universidad de Buenos Aires; Argentina.
Fil: Schmitz, Mark. Department of Geosciences, Boise State University; USA.
Fil: Lescano, Marina. Instituto de Estudios Andinos Don Pablo Groeber, CONICET, Universidad de Buenos Aires; Argentina.
Fil: Omarini, Julieta. Universidad Nacional de Río Negro. Instituto de Investigación en Paleobiología y Geología. Río Negro, Argentina.
Fil: Tunik, Maisa. Universidad Nacional de Río Negro. Instituto de Investigación en Paleobiología y Geología. Río Negro, Argentina.
Fil: Kuhnert, Henning. MARUM – Center for Marine Environmental Sciences, Universität Bremen; Germany.
Fil: Concheyro, Andrea. Instituto de Estudios Andinos Don Pablo Groeber, CONICET, Universidad de Buenos Aires; Argentina.
Fil: Rawson, Peter. School of Environmental Sciences, University of Hull; UK.
Fil: Ramos, Victor. Instituto de Estudios Andinos Don Pablo Groeber, CONICET, Universidad de Buenos Aires; Argentina.
Fil: Reboulet, Stéphane. Université de Lyon, UCBL, ENSL, CNRS, LGL TPE. France.
Fil: Noclin, Nicolas. Université de Lyon, UCBL, ENSL, CNRS, LGL TPE. France.
Fil: Frederichs, Thomas. MARUM – Center for Marine Environmental Sciences, Universität Bremen; Germany.
Fil: Nickl, Anna-Leah. MARUM – Center for Marine Environmental Sciences, Universität Bremen; Germany.
Fil: Palike, Heiko. MARUM – Center for Marine Environmental Sciences, Universität Bremen; Germany.
Discrepancies in the ages and durations of the Berriasian to Barremian stages still exist between geological data and the proposed geological time scale 2016 (Ogg et al., 2016; Lena et al., 2018). The Hauterivian Stage suffers from these discrepancies as its duration is proposed at 3.92 myr (Ogg et al., 2016), while astrochronology in the Tethyan area (SE France and SE Spain) led to a duration of 5.9 ± 0.4 myr (Martinez et al., 2015). In order to reconcile these durations, we investigated the Agrio Formation in the Neuquén Basin (Argentina). A total of 2,200 samples were collected every 0.25 cm and measured in magnetic susceptibility with a Kappabridge KLY-2. From spectral analyses realised on these MS signals, it appears that the 100-kyr eccentricity is continuously recorded throughout the Agrio Formation, allowing duration calculations. In addition, a new U-Pb age measured on zircons was provided in the upper part of the Agrio Formation using the CA-ID-TIMS method. Thus, four U-Pb ages are now available in the Agrio Formation measured with the U-Pb CA-ID-TIMS (Aguirre-Urreta et al., 2015, 2017). Notably, the astrochronological durations fit with three of the U-Pb ages. A fourth age appears 300 kyr elder than suggested by astrochronology, which may be due to protracted crystallization of zircons in the magmatic chamber. This new data in the Agrio Formation, together with correlations to the Tethyan area, highlights a revision to the duration of the Hauterivian Stage of 5.22 ± 0.11 myr starting at 131.29 ± 0.25 Ma and ending at 126.07 ± 0.25 Ma. The previous overestimate of the duration of the Hauterivian Stage was likely due to distortion of the 405-kyr eccentricity in the sedimentary record, as recent studies document (Laurin et al., 2017; Martinez, 2018). Thanks to these revised ages and previous astsochronological frameworks, we were able to revise the ages and durations of stages from the Late Berriasian to the Barremian-Aptian boundary. A synthesis of δ13C measured on belemnites (Martinez and Dera, 2015) indicate a clear 2.4-myr cycle in the carbon cycle record which fit with the main paleoceanographic events. Higher amplitudes of this cycle are notably observed during major volcanic episodes, suggesting that acceleration of the hydraulic cycle lead to a reinforcement of the long-Milankovitch cycles.
description Fil: Martinez, Mathieu. Univ. Rennes,CNRS, Geosciences, France.
publishDate 2018
dc.date.none.fl_str_mv 2018
dc.type.none.fl_str_mv info:eu-repo/semantics/conferenceObject
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_5794
info:ar-repo/semantics/documentoDeConferencia
format conferenceObject
status_str publishedVersion
dc.identifier.none.fl_str_mv https://www.thejk.org.uk/jk2018/
https://php5.univ-brest.fr/conference/ocs/index.php/JK2018/JK2018/paper/view/515
http://rid.unrn.edu.ar/handle/20.500.12049/5745
url https://www.thejk.org.uk/jk2018/
https://php5.univ-brest.fr/conference/ocs/index.php/JK2018/JK2018/paper/view/515
http://rid.unrn.edu.ar/handle/20.500.12049/5745
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv JK2018
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/4.0/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/4.0/
dc.format.none.fl_str_mv application/pdf
dc.source.none.fl_str_mv reponame:RID-UNRN (UNRN)
instname:Universidad Nacional de Río Negro
reponame_str RID-UNRN (UNRN)
collection RID-UNRN (UNRN)
instname_str Universidad Nacional de Río Negro
repository.name.fl_str_mv RID-UNRN (UNRN) - Universidad Nacional de Río Negro
repository.mail.fl_str_mv rid@unrn.edu.ar
_version_ 1846787726375911424
score 12.982451