# Weissert Event

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{{Short description|Hyperthermal event during the Early Cretaceous epoch}}

The '''Weissert Event''', also referred to as the '''Weissert Thermal Excursion''' ('''WTX'''),<ref name="ChristopherScoteseIsAwesome">{{Cite journal |last1=Scotese |first1=Christopher R. |last2=Song |first2=Haijun |last3=Mills |first3=Benjamin J. W. |last4=van der Meer |first4=Douwe G. |date=1 April 2021 |title=Phanerozoic paleotemperatures: The earth's changing climate during the last 540 million years |url=https://www.sciencedirect.com/science/article/pii/S0012825221000027 |journal=[Earth-Science Reviews](/source/Earth-Science_Reviews) |volume=215 |article-number=103503 |doi=10.1016/j.earscirev.2021.103503 |bibcode=2021ESRv..21503503S |s2cid=233579194 |issn=0012-8252 |access-date=5 November 2023|url-access=subscription }}</ref> was a [hyperthermal event](/source/hyperthermal_event) that occurred in the [Valanginian](/source/Valanginian) [stage](/source/stage_(geology)) of the [Early Cretaceous](/source/Early_Cretaceous) epoch.<ref name="MartinezEtAl2015" /> This thermal excursion occurred amidst the relatively cool Tithonian-early Barremian Cool Interval (TEBCI).<ref name="ChristopherScoteseIsAwesome" /> Its termination marked an intense cooling event,<ref name="CavalheiroEtAl2021" /> potentially even an [ice age](/source/ice_age).<ref name="MartinezEtAl2013" />

== Duration ==
The start of the WTX has been astrochronologically dated by one study to 134.50 ± 0.19 million years ago (Ma), with its positive [δ<sup>13</sup>C](/source/%CE%9413C) excursion being found to last until 133.96 ± 0.19 Ma and the plateau phase of elevated δ<sup>13</sup>C values until 132.44 ± 0.19 Ma.<ref>{{Cite journal |last1=Martinez |first1=Mathieu |last2=Aguirre-Urreta |first2=Beatriz |last3=Dera |first3=Guillaume |last4=Lescano |first4=Marina |last5=Omarini |first5=Julieta |last6=Tunik |first6=Maisa |last7=O'Dogherty |first7=Luis |last8=Aguado |first8=Roque |last9=Company |first9=Miguel |last10=Bodin |first10=Stéphane |date=1 April 2023 |title=Synchrony of carbon cycle fluctuations, volcanism and orbital forcing during the Early Cretaceous |url=https://www.sciencedirect.com/science/article/pii/S0012825223000454 |journal=[Earth-Science Reviews](/source/Earth-Science_Reviews) |volume=239 |article-number=104356 |doi=10.1016/j.earscirev.2023.104356 |bibcode=2023ESRv..23904356M |s2cid=256880421 |issn=0012-8252 |access-date=5 November 2023}}</ref> However, astrochronological studies of sediments in the Vocontian Basin have yielded a duration of 2.08 Myr, with the positive δ<sup>13</sup>C excursion being 0.94 Myr in duration and the δ<sup>13</sup>C plateau being 1.14 Myr.<ref>{{Cite journal |last1=Charbonnier |first1=Guillaume |last2=Boulila |first2=Slah |last3=Gardin |first3=Silvia |last4=Duchamp-Alphonse |first4=Stéphanie |last5=Adatte |first5=Thierry |last6=Spangenberg |first6=Jorge E. |last7=Föllmi |first7=Karl B. |last8=Colin |first8=Christophe |last9=Galbrun |first9=Bruno |date=1 October 2013 |title=Astronomical calibration of the Valanginian "Weissert" episode: The Orpierre marl–limestone succession (Vocontian Basin, southeastern France) |url=https://www.sciencedirect.com/science/article/pii/S0195667113001122 |journal=[Cretaceous Research](/source/Cretaceous_Research) |volume=45 |pages=25–42 |doi=10.1016/j.cretres.2013.07.003 |bibcode=2013CrRes..45...25C |issn=0195-6671 |access-date=5 November 2023|url-access=subscription }}</ref> A different study concludes the WTX lasted for about 1.4 million years (Myr) based on the chronological length of the high δ<sup>13</sup>C plateau observed over its course in the Bersek Marl Formation of [Hungary](/source/Hungary).<ref>{{Cite journal |last1=Bajnai |first1=Dávid |last2=Pálfy |first2=József |last3=Martinez |first3=Mathieu |last4=Price |first4=Gregory D. |last5=Nyerges |first5=Anita |last6=Főzy |first6=István |date=1 July 2017 |title=Multi-proxy record of orbital-scale changes in climate and sedimentation during the Weissert Event in the Valanginian Bersek Marl Formation (Gerecse Mts., Hungary) |url=https://www.sciencedirect.com/science/article/pii/S0195667116302221 |journal=[Cretaceous Research](/source/Cretaceous_Research) |volume=75 |pages=45–60 |doi=10.1016/j.cretres.2017.02.021 |bibcode=2017CrRes..75...45B |issn=0195-6671 |access-date=5 November 2023|hdl=10026.1/8696 |hdl-access=free }}</ref>

== Causes ==
An addition of [carbon dioxide into the atmosphere](/source/Carbon_dioxide_in_Earth's_atmosphere) via the activity of the [Paraná-Etendeka Large Igneous Province](/source/Paran%C3%A1_and_Etendeka_traps) (PE-LIP) is generally accepted as the leading candidate for what sparked the WTX,<ref name="MartinezEtAl2015">{{Cite journal |last1=Martinez |first1=Mathieu |last2=Deconinck |first2=Jean-François |last3=Pellenard |first3=Pierre |last4=Riquier |first4=Laurent |last5=Company |first5=Miguel |last6=Reboulet |first6=Stéphane |last7=Moiroud |first7=Mathieu |date=1 August 2015 |title=Astrochronology of the Valanginian–Hauterivian stages (Early Cretaceous): Chronological relationships between the Paraná–Etendeka large igneous province and the Weissert and the Faraoni events |url=https://www.sciencedirect.com/science/article/pii/S0921818115001113 |journal=[Global and Planetary Change](/source/Global_and_Planetary_Change) |volume=131 |pages=158–173 |doi=10.1016/j.gloplacha.2015.06.001 |bibcode=2015GPC...131..158M |issn=0921-8181 |access-date=5 November 2023|url-access=subscription }}</ref> although this is not universally accepted, with some reconstructed geochronologies showing a lack of causality between the emplacement of the PE-LIP and the onset of the WTX.<ref name="MartinezEtAl2013">{{Cite journal |last1=Martinez |first1=Mathieu |last2=Deconinck |first2=Jean-François |last3=Pellenard |first3=Pierre |last4=Reboulet |first4=Stéphane |last5=Riquier |first5=Laurent |date=15 April 2013 |title=Astrochronology of the Valanginian Stage from reference sections (Vocontian Basin, France) and palaeoenvironmental implications for the Weissert Event |url=https://www.sciencedirect.com/science/article/pii/S0031018213000977 |journal=[Palaeogeography, Palaeoclimatology, Palaeoecology](/source/Palaeogeography%2C_Palaeoclimatology%2C_Palaeoecology) |volume=376 |pages=91–102 |doi=10.1016/j.palaeo.2013.02.021 |bibcode=2013PPP...376...91M |issn=0031-0182 |access-date=5 November 2023|url-access=subscription }}</ref> The prolonged, drawn out manner in which the PE-LIP erupted has been brought up as a further argument against its emplacement as the driving perturbation causing the WTX.<ref name="PriceEtAl2018">{{Cite journal |last1=Price |first1=Gregory D. |last2=Janssen |first2=Nico M. M. |last3=Martinez |first3=Mathieu |last4=Company |first4=Miguel |last5=Vandevelde |first5=Justin H. |last6=Grimes |first6=Stephen T. |date=8 October 2018 |title=A High-Resolution Belemnite Geochemical Analysis of Early Cretaceous (Valanginian-Hauterivian) Environmental and Climatic Perturbations |journal=[Geochemistry, Geophysics, Geosystems](/source/Geochemistry%2C_Geophysics%2C_Geosystems) |language=en |volume=19 |issue=10 |pages=3832–3843 |doi=10.1029/2018GC007676 |issn=1525-2027 |doi-access=free |bibcode=2018GGG....19.3832P |hdl=10026.1/12437 |hdl-access=free }}</ref>

== Effects ==
The WTX resulted in a rapid global temperature increase during the otherwise mild TEBCI.<ref name="ChristopherScoteseIsAwesome" /> The sharp jump in global temperatures during this hyperthermal event was accompanied by [oceanic anoxia](/source/Oceanic_anoxic_event).<ref>{{Cite journal |last1=Erba |first1=Elisabetta |last2=Bartolini |first2=Annachiara |last3=Larson |first3=Roger L. |date=1 February 2004 |title=Valanginian Weissert oceanic anoxic event |url=https://pubs.geoscienceworld.org/geology/article/32/2/149-152/103728 |journal=[Geology](/source/Geology_(journal)) |language=en |volume=32 |issue=2 |page=149 |doi=10.1130/G20008.1 |bibcode=2004Geo....32..149E |issn=0091-7613 |access-date=5 November 2023|url-access=subscription }}</ref> However, unlike other oceanic anoxic events, the WTX is not associated with widespread [black shale](/source/Shale) deposits.<ref>{{Cite journal |last1=Bornemann |first1=André |last2=Erbacher |first2=Jochen |last3=Blumenberg |first3=Martin |last4=Voigt |first4=Silke |date=15 June 2023 |title=A first high-resolution carbon isotope stratigraphy from the Boreal (NW Germany) for the Berriasian to Coniacian interval—implications for the timing of the Aptian–Albian boundary |journal=[Frontiers in Earth Science](/source/Frontiers_in_Earth_Science) |volume=11 |pages=1–14 |doi=10.3389/feart.2023.1173319 |issn=2296-6463 |doi-access=free |bibcode=2023FrEaS..1173319B }}</ref> Nannoconids experienced a decline at the onset of the WTX resulting from [marine regression](/source/marine_regression), but bloomed in abundance later on in the event as ocean productivity skyrocketed.<ref>{{Cite journal |last1=Shmeit |first1=M. |last2=Giraud |first2=F. |last3=Jaillard |first3=E. |last4=Reboulet |first4=S. |last5=Masrour |first5=M. |last6=Spangenberg |first6=J. E. |last7=El-Samrani |first7=A. |date=1 August 2022 |title=The Valanginian Weissert Event on the south Tethyan margin: A dynamic paleoceanographic evolution based on the study of calcareous nannofossils |url=https://www.sciencedirect.com/science/article/pii/S0377839822000500 |journal=Marine Micropaleontology |volume=175 |article-number=102134 |doi=10.1016/j.marmicro.2022.102134 |s2cid=249325228 |issn=0377-8398 |access-date=5 November 2023|doi-access=free }}</ref> In the Vocontian Basin, the WTX is associated with an increase in [marlstones](/source/Marl).<ref>{{Cite journal |last1=Martinez |first1=Mathieu |last2=Guillois |first2=Landry |last3=Boulvais |first3=Philippe |last4=Deconinck |first4=Jean-François |date=8 May 2020 |title=Inverted Responses of the Carbon Cycle to Orbital Forcing in Mesozoic Periplatform Marginal Basins: Implications for Astrochronology |url=https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2019PA003705 |journal=[Paleoceanography and Paleoclimatology](/source/Paleoceanography_and_Paleoclimatology) |language=en |volume=35 |issue=6 |pages=1–19 |doi=10.1029/2019PA003705 |bibcode=2020PaPa...35.3705M |s2cid=218939500 |issn=2572-4517 |access-date=5 November 2023}}</ref> At the end of the WTX, temperatures cooled by ~1–2 °C based on the results of [palaeothermometry](/source/Paleothermometer) done in southern France, whereas the Boreal Ocean and its surroundings cooled by as much as 4 °C.<ref name="CavalheiroEtAl2021">{{Cite journal |last1=Cavalheiro |first1=Liyenne |last2=Wagner |first2=Thomas |last3=Steinig |first3=Sebastian |last4=Bottini |first4=Cinzia |last5=Dummann |first5=Wolf |last6=Esegbue |first6=Onoriode |last7=Gambacorta |first7=Gabriele |last8=Giraldo-Gómez |first8=Victor |last9=Farnsworth |first9=Alexander |last10=Flögel |first10=Sascha |last11=Hofmann |first11=Peter |last12=Lunt |first12=Daniel J. |last13=Rethemeyer |first13=Janet |last14=Torricelli |first14=Stefano |last15=Erba |first15=Elisabetta |date=13 September 2021 |title=Impact of global cooling on Early Cretaceous high pCO2 world during the Weissert Event |journal=[Nature Communications](/source/Nature_Communications) |language=en |volume=12 |issue=1 |page=5411 |doi=10.1038/s41467-021-25706-0 |pmid=34518550 |pmc=8437947 |issn=2041-1723 |doi-access=free }}</ref> Geochemical records of <sup>187</sup>Os/<sup>188</sup>Os point to an increase in unradiogenic osmium flux into the ocean, suggesting the occurrence of [silicate weathering](/source/Carbonate%E2%80%93silicate_cycle) of PE-LIP basalts during this slice of time, providing the most likely explanation for the temperature drop.<ref>{{Cite journal |last1=Percival |first1=Lawrence M. E. |last2=Ownsworth |first2=E. |last3=Robinson |first3=S. A. |last4=Selby |first4=D. |last5=Goderis |first5=S. |last6=Claeys |first6=P. |date=1 August 2023 |title=Valanginian climate cooling and environmental change driven by Paraná-Etendeka basalt erosion |url=https://pubs.geoscienceworld.org/gsa/geology/article/51/8/753/623905/Valanginian-climate-cooling-and-environmental |journal=[Geology](/source/Geology_(journal)) |language=en |volume=51 |issue=8 |pages=753–757 |doi=10.1130/G51202.1 |bibcode=2023Geo....51..753P |issn=0091-7613 |access-date=22 December 2023 |via=GeoScienceWorld}}</ref> Some studies have suggested that a transient ice age with limited but significant [polar ice caps](/source/Polar_ice_cap) occurred in the aftermath of the WTX,<ref name="MartinezEtAl2013" /><ref>{{Cite journal |last1=Gröcke |first1=Darren R. |last2=Price |first2=Gregory D. |last3=Robinson |first3=Stuart A. |last4=Baraboshkin |first4=Evgenij Y. |last5=Mutterlose |first5=Jörg |last6=Ruffell |first6=Alastair H. |date=1 December 2005 |title=The Upper Valanginian (Early Cretaceous) positive carbon–isotope event recorded in terrestrial plants |url=https://www.sciencedirect.com/science/article/pii/S0012821X05005546 |journal=[Earth and Planetary Science Letters](/source/Earth_and_Planetary_Science_Letters) |volume=240 |issue=2 |pages=495–509 |doi=10.1016/j.epsl.2005.09.001 |issn=0012-821X |access-date=5 November 2023|url-access=subscription }}</ref> although the lack of a positive [δ<sup>18</sup>O<sub>seawater</sub>](/source/%CE%9418O) excursion during the latest Valanginian interval of cooling and the presence instead of a very slightly negative excursion calls into question the existence of any significant polar ice growth.<ref name="PriceEtAl2018" />

== References ==
{{reflist}}

Category:Anoxic events
Category:Valanginian Stage
{{improve categories|date=November 2023}}

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Adapted from the Wikipedia article [Weissert Event](https://en.wikipedia.org/wiki/Weissert_Event) by Wikipedia contributors ([contributor history](https://en.wikipedia.org/wiki/Weissert_Event?action=history)). Available under [Creative Commons Attribution-ShareAlike 4.0 International](https://creativecommons.org/licenses/by-sa/4.0/). Changes may have been made.
