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Abstract

Dinosaurs dominated the land surface. Ammonites are the main fossils for correlating marine deposits. Pangea supercontinent began to break up, and at the end of the Middle Jurassic the Central Atlantic was born. Organic-rich sediments in several locations eventually became the source rocks helping to fuel modern civilization. HISTORY AND SUBDIVISIONS Overview of the Jurassic The term “Jura Kalkstein” was applied by Alexander von Humboldt (1799) to a series of carbonate shelf deposits exposed in the mountainous Jura region of northernmost Switzerland, and he first recognized that these strata were distinct from the German Muschelkalk (middle Triassic), although he erroneously considered his unit to be older. Alexander Brongniart (1829) coined the term “Terrains Jurassiques” when correlating the “Jura Kalkstein” to the Lower Oolite Series (now assigned to Middle Jurassic) of the British succession.

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... The uncertainties in the inter-regional biostratigraphic correlation constitute a major classic problem for this time interval across the world, and absolute data are still scarce and conflicting with each other (e.g., Remane, 1991;Wimbledon, 2008;Wimbledon et al., 2011Wimbledon et al., , 2013P alfy et al., 2000;P alfy, 2008;Vennari et al., 2014;Wimbledon, 2017). Cyclostratigraphy has become an important tool in measuring Jurassic -Cretaceous geologic time and establishing floating astronomical time scales (Ogg and Hinnov, 2012a;. Almost the entire Jurassic and Cretaceous have been calibrated using astronomical cycles, especially the long-term and short-term excentricity cycle. ...
... Almost the entire Jurassic and Cretaceous have been calibrated using astronomical cycles, especially the long-term and short-term excentricity cycle. However, the Tithonian (uppermost Upper Jurassic) remains still somewhat uncertain, and should be even carefully reviewed and compared with magnetostratigraphy and absolute dating (e.g., P alfy et al., 2000;P alfy, 2008;Huang et al., 2010;Ogg and Hinnov, 2012a). ...
... Our cyclostratigraphic data suggest a time span of 5.67 myr for the Tithonian and 5.27 myr for the Berriasian. However, if we take into consideration that the Tithonian most likely spans 7.1 myr (Ogg and Hinnov, 2012a), it would imply that c. four low-frequency eccentricity cycles An accurate astromomical time scale (ATS) for the TithonianeBerriasian is possible from the comparison and combination of available studies (Fig. 9). The lowermost Lower Tithonian was studied by Weedon et al. (1999Weedon et al. ( , 2004 using magnetic-susceptibility measures made on exposures, core material and down boreholes from the Kimmeridge Clay Formation (Kimmeridgiane Tithonian). ...
Chapter
Detailed cyclostratigraphical analyses have been made from five TithonianeBerriasian sections of the Vaca Muerta Formation, exposed in the Neuquén Basin, Argentina. The Vaca Muerta Formation is characterized by decimetre-scale rhythmic alternations of marlstones and limestones, showing a well-ordered hierarchy of cycles, where elementary cycles, bundles of cycles and superbundles have been recognized. According to biostratigraphic data, elementary cycles have a periodicity of 21 ky, which correlates with the precession cycle of Earth’s axis. Spectral analysis based on time series of elementary cycle thicknesses allows us to identify frequencies of w400 ky and w90e120 ky, which we interpret as the modulation of the precessional cycle by the Earth’s orbital eccentricity. Correlation between studied sections allowed us to estimate a minimum duration for each Andean ammonite zone. Moreover, cyclostratigraphic data allowed us to build the first continuous floating astronomical time scale for the Tithonian e Berriasian, which is anchored to the geological time scale through magnetostratigraphy. We estimated a minimum duration of 5.67 myr for the Tithonian and 5.27 myr for the Berriasian. The resulted durations of some polarity chrones are also different with respect to the GTS2016, however such differences could be due to condensation or discontinuities not detected in the studied sections.
... The definition of Jurassic-Cretaceous boundary represents a drawback at a global scale, since the Cretaceous is the only system/period of the Phanerozoic that so far, has not been defined by a basal boundary stratotype. This is mainly due to the lack of significant evolutionary or physical/chemical event on either at regional or global scale within the commonly used boundary interval, coupled with the difficulty of correlating any biostratigraphic datum due to the pronounced provincialism of marine fauna (Ogg and Hinnov 2012;Ogg et al. 2016). After long years of debate, the Berriasian Working Group has concluded the boundary is marked by the explosion of Calpionella alpina, which is placed in the middle of Subchron M19n.2n. ...
... It enables correlation of rock strata of diverse depositional and faunal realms as well as the assignment of geologic ages to anomalies of marine magnetic intensities. For Middle Jurassic to present, magnetic anomalies of the ocean floor with their calibrations to biostratigraphy serve as a template against which magnetic polarities isolated, either on-land or in deep-sea sections, can be determined (Ogg and Hinnov 2012). Accordingly, magnetostratigraphy affords the employment of the reference Geomagnetic Polarity Time Scale (GTS) to the highresolution correlation of marine magnetic anomalies, and the use of the calibrated reference pattern of polarity changes to correlate polarity zones among sections (Ogg and Hinnov 2012). ...
... For Middle Jurassic to present, magnetic anomalies of the ocean floor with their calibrations to biostratigraphy serve as a template against which magnetic polarities isolated, either on-land or in deep-sea sections, can be determined (Ogg and Hinnov 2012). Accordingly, magnetostratigraphy affords the employment of the reference Geomagnetic Polarity Time Scale (GTS) to the highresolution correlation of marine magnetic anomalies, and the use of the calibrated reference pattern of polarity changes to correlate polarity zones among sections (Ogg and Hinnov 2012). From present to the Kimmeridgian (Chron M25r), polarities from the GTS are directly derived from sea-surface marine magnetic anomalies, whereas from the Kimmeridgian to the Bajocian (Chrons M27 to M44), polarities are modeled from deep-tow surveys. ...
Chapter
The first magnetostratigraphic scales for the Jurassic through Early Cretaceous from the Southern Hemisphere have been constructed over the last decades from marine sections in the Neuquén Basin. Paleomagnetic sites were tied to ammonite zones in order to achieve well-refined ages of studied sections. Diverse field tests for the paleomagnetic stability proved the primary origin of isolated magnetizations. In the case of Upper Jurassic–Lower Cretaceous studies, magnetostratigraphic and biostratigraphic data were combined with cyclostratigraphy. Finally, polarities were tied to Andean ammonite zones and from their correlation with the standard zones, calibrated to the GTS2016 (Geomagnetic Polarity Time Scale 2016). For the Early Jurassic, a composite magnetostratigraphic scale was derived out of five sections spanning the Hettangian–Toarcian. The magnetostratigraphic scale portrays 16 reverse (Jr1–Jr16) and 16 normal (Jn1–Jn16) polarity zones that encompass at least 19 ammonite zones. A major difference between both scales rises in the Hettangian encompassing Jr1–Jr3 polarity zones. For the Middle Jurassic, the resultant magnetostratigraphy obtained in the Lajas Formation is a pattern of dominantly reverse polarity. According to the correlation with the GTS2016, the studied section is assigned to the Lower-uppermost Middle Bathonian (Chrons M41 through M39). For the Late Jurassic–Early Cretaceous, the magnetostratigraphic scale obtained in the Vaca Muerta Formation comprises Subchrons M22r.2r through M15r, spanning the V. andesensis (Lower Tithonian)–S. damesi Zones (Upper Berriasian). The use of diverse chronostratigraphic tools such as biostratigraphy, magnetostratigraphy and cyclostratigraphy, enabled to determine with unprecedented precision the position of the Jurassic–Cretaceous boundary, as well as to assess durations of ammonite zones.
... In contrast to most geological systems, the Jurassic/Cretaceous transition is characterized by the absence of a significant faunal turnover, as well as by the remarkable increase of faunal provinciality, especially in ammonites (e.g., Remane, 1991;Wimbledon, 2008;Michalík and Reh akov a, 2011;Wimbledon et al., 2011Wimbledon et al., , 2013Ogg and Hinnov, 2012, and references cited there). The uncertainties in the inter-regional correlation constitute a major classic problem for this time interval across the world. ...
... Since polarity reversals are recorded simultaneously in all type of rocks all over the world, they provide a distinctive pattern or finger-print for a certain time interval. Marine magnetic anomalies and their calibrations to biostratigraphy make up the reference against which magnetostratigraphic sequences, either on land or in deep-sea cores, are correlated (Ogg and Hinnov, 2012). Thus, one fundamental requisite to attempt a non-ambiguous paleomagnetic correlation between a section on-land and the GPTS is a good biostratigraphic definition (e.g. ...
... Thus, one fundamental requisite to attempt a non-ambiguous paleomagnetic correlation between a section on-land and the GPTS is a good biostratigraphic definition (e.g. Ogg and Hinnov, 2012). In the Jurassic, biostratigraphic, magnetostratigraphic, chemostratigraphic and other events are calibrated typically to the standard ammonite zones in Europe, although during the Oxfordian and Tithonian other paleogeographic realms take place such as the Boreal (Arctic and northernmost Europe), sub-Boreal (northern Europe), sub-Mediterranean (southern Europe) and Tethyan (southernmost Europe). ...
Article
A systematic sedimentologic and paleomagnetic study was carried out in the Vaca Muerta Formation, cropping out in the northern Neuquén Basin, west-central Argentina. The studied section is c.280 m-thick and represents a carbonate ramp system bearing ammonites that indicate Late Jurassic–Early Cretaceous ages. The Vaca Muerta Formation is one of the most important unconventional hydrocarbon reservoirs in the world and its thorough study has become a relevant target in Argentina. The J-K boundary is comprised within this unit, and although it is well-dated through biostratigraphy -mainly ammonites-, the position of particularly the boundary is yet a matter of hot debate. Therefore, the systematic paleomagnetic and cyclostratigraphic study in the Vaca Muerta Formation was considered relevant in order to obtain the first Upper Jurassic–Lower Cretaceous magnetostratigraphy of the southern hemisphere on the first place and to precise the position of the J-K boundary in the Neuquén Basin, on the other. Biostratigraphy is well studied in the area, so that paleomagnetic sampling horizons were reliably tied, particularly through ammonites. Almost 450 standard specimens have been processed for this study distributed along 56 paleomagnetic sampling horizons that were dated using ammonites. Paleomagnetic behaviours showed to be very stable, and their quality and primary origin have been proved through several paleomagnetic field tests The resultant magnetostratigraphic scale is made up of 11 reverse and 10 normal polarity zones, spanning the Andean Virgatosphinctes mendozanus (lower Tithonian) to Spiticeras damesi Zones (upper Berriasian). These polarity zones were correlated with those of the International Geomagnetic Polarity Time Scale 2012 and 2016 through the correlation between Andean and Tethyan ammonite zones. Cyclostratigraphy on the other hand, proved to be quite consistent with the magnetostratigraphy. Through the correlation of the resultant paleomagnetic and cyclostratigraphic data, it was possible to date the section with unprecedented precision, and therefore, to establish the position of the Jurassic-Cretaceous boundary. The paleomagnetic pole calculated from the primary magnetization is located at: Lon= 191.6°E, Lat= 76.2°S, A95= 3.5°, indicating a c. 24° clockwise rotation for the studied section, which is consistent with structural data of the region.
... Particularly, the studies of calcareous nannofossils (Bown and Ellison 1995, Scasso and Concheyro 1999, Bown and Concheyro 2004, Lescano and Concheyro 2009, Vennari et al. 2014, as well as other Tethyan calcareous microfossils, such as calpionellids, saccocomid microcrinoids and calcareous dinoflagellate cysts (Fernández Carmona et al. 1996, Fernández Carmona and Riccardi 1998, Kietzmann and Palma 2009, Kietzmann et al. 2011a, Kietzmann 2017, Ivanova and Kietzmann 2017. The remarkable increase of faunal provinciality, as well as the uncertainties in the inter-regional correlation constitutes a major classic problem for the Tithonian-Berriasian across the world (e.g., Ogg and Hinnov 2012). The definition of the base of the Cretaceous System is still controversial. ...
... One interval at c. 30 m from the base bears no polarity, were a Cenozoic sill was intruded. Based on the correlation between ammonite zones from the Andean and Tethys Regions, these polarities were calibrated according to the last Geomagnetic Polarity Time Scale (GPTS) compiled by Ogg and Hinnov (2012). Results show a good correlation between both magnetostratigraphic scales. ...
Article
Full-text available
Detailed systematic studies have been carried out in the Vaca Muerta Formation in order to achieve an integrated multidisciplinary calibration of the Jurassic/Cretaceous transition in the Neuquén Basin. Although this unit has a very well-established ammonite biostratigraphy, the temporal distribution of biozones is yet a matter of hot debate. In this contribution we present the results of a well constrained integrated data from the Arroyo Loncoche section (southern Mendoza), where comprehensive cyclostratigraphic, paleomagnetic and biostratigraphic sampling/data allowed us to elaborate a very strong chronostratigraphic scheme for the Titho-nian-Berriasian interval. The proposed stratigraphic calibration of the Tithonian-Berriasian Andean succession brings foward two key points: 1) The base of the Vaca Muerta Formation shows a polarities pattern which would only be compatible to the uppermost part of Hybonotum Zone (lowermost Lower Tithonian). 2) The position of the Jurassic-Cretaceous boundary is located within the lower third of the S. koeneni Zone. RESUMEN Calibración estratigráfica multidisciplinaria de la transición Jurásico-Cretácico en la Cuenca Neuquina Se realizaron estudios sistemáticos de detalle en la Formación Vaca Muerta con el fin de lograr una calibración multidisciplinaria integrada de la transición jurásico/cretácica en la Cuenca Neuquina. Aunque esta unidad se caracteriza por presentar una bioestra-tigrafía basada en amonites, la distribución temporal de las biozonas es todavía un tema de importante debate. En esta contribución se presentan los resultados integrados de la sección Arroyo Loncoche (sur de Mendoza), en donde exhaustivos estudios cicloestra-tigráficos, paleomagnéticos y bioestratigráficos han permitido elaborar un robusto esquema de correlación cronoestratigráfico para el intervalo Tithoniano-Berriasiano. La calibración estratigráfica propuesta para la sucesión tithoniano-berriasiana andina presenta dos puntos clave: 1) La base de la Formación Vaca Muerta muestra un patrón de polaridades que solo sería compatible con la parte superior de la Zona de Hybonotum (Tithoniano Inferior bajo). 2) La posición del límite Jurásico-Cretáceo está ubicada dentro del tercio inferior de la Zona de S. koeneni.
... Particularly, the studies of calcareous nannofossils (Bown and Ellison 1995, Scasso and Concheyro 1999, Bown and Concheyro 2004, Lescano and Concheyro 2009, Vennari et al. 2014, as well as other Tethyan calcareous microfossils, such as calpionellids, saccocomid microcrinoids and calcareous dinoflagellate cysts (Fernández Carmona et al. 1996, Fernández Carmona and Riccardi 1998, Kietzmann and Palma 2009, Kietzmann et al. 2011a, Kietzmann 2017, Ivanova and Kietzmann 2017. The remarkable increase of faunal provinciality, as well as the uncertainties in the inter-regional correlation constitutes a major classic problem for the Tithonian-Berriasian across the world (e.g., Ogg and Hinnov 2012). The definition of the base of the Cretaceous System is still controversial. ...
... One interval at c. 30 m from the base bears no polarity, were a Cenozoic sill was intruded. Based on the correlation between ammonite zones from the Andean and Tethys Regions, these polarities were calibrated according to the last Geomagnetic Polarity Time Scale (GPTS) compiled by Ogg and Hinnov (2012). Results show a good correlation between both magnetostratigraphic scales. ...
Article
Detailed systematic studies have been carried out in the Vaca Muerta Formation in order to achieve an integrated multidisciplinary calibration of the Jurassic/Cretaceous transition in the Neuquén Basin. Although this unit has a very well-established ammonite biostratigraphy, the temporal distribution of biozones is yet a matter of hot debate. In this contribution we present the results of a well constrained integrated data from the Arroyo Loncoche section (southern Mendoza), where comprehensive cyclostratigraphic, paleomagnetic and biostratigraphic sampling/data allowed us to elaborate a very strong chronostratigraphic scheme for the Titho-nian-Berriasian interval. The proposed stratigraphic calibration of the Tithonian-Berriasian Andean succession brings foward two key points: 1) The base of the Vaca Muerta Formation shows a polarities pattern which would only be compatible to the uppermost part of Hybonotum Zone (lowermost Lower Tithonian). 2) The position of the Jurassic-Cretaceous boundary is located within the lower third of the S. koeneni Zone.
... Within the Iznalloz section, the Polymorphum Zone is much thinner than any other biozone of the section but this is affected by the hiatus located in the Pliensbachian-Toarcian boundary and in the Polymorphum-Serpentinum zone boundary also recorded in other sections of the Subbetic (e.g., Nieto et al. 2008;Reolid et al. 2014a). The Serpentinum Zone has a duration of 1.08 Ma from Ogg and Hinnov (2012), 1.5-1.62 Ma from Boulila et al. (2014) and 1.31 Ma from Ruebsam et al. (2014) and is 2.62 m thick, but it is not represented by ammonitico rosso facies (sedimentation rate ranging from 0.24 to 0.16 cm/kyr; Table 1). ...
... Ma from Boulila et al. (2014) and 1.31 Ma from Ruebsam et al. (2014) and is 2.62 m thick, but it is not represented by ammonitico rosso facies (sedimentation rate ranging from 0.24 to 0.16 cm/kyr; Table 1). The Aalensis Zone, represented by ammonitico rosso facies, is 3.00 m thick for a duration of 1 Ma from Gradstein et al. (2004), 0.13 Ma from Ogg and Hinnov (2012) and 0.44-0.51 Ma from Boulila et al. (2014), (2.31-0.59 ...
Article
The Toarcian ammonitico rosso facies were widespread in the Mediterranean Tethys (between 15 and 30°N latitude) in the North Gondwana Paleomargin (Apulian promontory and North African Margin) and southern Iberian Paleomargin (Betic Cordillera). These facies were associated with epi-oceanic slopes of a sedimentary swell-trough system related to the extensional phase of continental rifting. In the Median Subbetic (southern Iberian Paleomargin), ammonitico rosso facies show a progressive change through the Toarcian on the hemipelagic swells after the fragmentation of a carbonate platform. During the latest Pliensbachian to the Bifrons Zone (middle Toarcian), sedimentation was dominated by epi-oceanic limestone and marl with a high influence of neighboring shallow-water environments represented by common turbidite–tempestite beds (with foraminifera and ooids). Microfossils and trace fossils provide no evidence of oxygen-restricted conditions. In the Gradata Zone (middle Toarcian), the ammonitico rosso facies appear (red nodular limestone and marly-limestone rich in the trace fossils Phycodes, Planolites, Thalassinoides, and Chondrites). Progressively more pelagic conditions and a restricted influence of emergent lands and carbonate platforms are reflected by the reduced input of turbidite–tempestite beds and increase of ammonitellas and radiolaria. A sea-level fall affected the hemipelagic swell during the middle–late Toarcian and favored sediment-winnowing by currents, with subsequent nodulation. The combined action of burrowing, compaction, and dissolution controlled nodulation, which ranges from diffuse nodules to sharp-edged nodules. The sedimentation rate conditioned the time available for nodule growth, the migration of the Ca2+ and HCO3− precipitation horizon, and the degree of nodulation (from horizons with diffuse-edged nodules to semi-continuous to continuous layers formed by the coalescence of sharp-edged nodules).
... Applegate & Bergen (1988) used the FO of L. bollii as a marker for the base of CC4-A. The CC4-A and CC4-B boundary has been considered Early Hauterivian in the Tethyan Realm, and has been correlated with the Crioceratites loryi ammonite zone (Bergen, 1994) and with Polarity Chron CM9 (Ogg & Hinnov, 2012b). However, in several sections of the Neuquén Basin, the FO of L. bollii occurs at a higher level, near the base of the Upper Hauterivian (Aguirre-Urreta et al. 2005). ...
... The LO of L. bollii has been used as a reliable marker within the CC5 Zone. In the Tethyan region, it occurs within the Pseudothurmannia ohmi ammonite zone (Bergen, 1994), at the top of the Hauterivian (Aguado et al. 2014;Reboulet et al. 2014) and within the Polarity Chron CM5 (Ogg & Hinnov, 2012b). In the Neuquén Basin, this bioevent is recorded high in the Agua de la Mula Member, in beds included in the Paraspiticeras groeberi ammonite zone, which in turn is correlated with part of the Pseudothurmannia ohmi Zone (Fig. 4). ...
Article
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Two tuffs in the Lower Cretaceous Agrio Formation, Neuquén Basin, provided U–Pb zircon radioisotopic ages of 129.09±0.16 Ma and 127.42±0.15 Ma. Both horizons are well constrained biostratigraphically by ammonites and nannofossils and can be correlated with the ‘standard’ sequence of the Mediterranean Province. The lower horizon is very close to the base of the Upper Hauterivian and the upper horizon to the Hauterivian/Barremian boundary, indicating that the former lies at c . 129.5 Ma and the latter at c . 127 Ma. These new radioisotopic ages fill a gap of over 8 million years in the numerical calibration of the current global Early Cretaceous geological time scale.
... According to the chronostratigraphic Mesozoic timescale of Ogg (2004), the boundaries of the Tithonian are, at the base, 150.8 + 4 Ma and, at the top, 145.5 + 4 Ma (Fig. 2), the latter being the present absolute age for the Jurassic -Cretaceous boundary accepted by the International Commission of Stratigraphy of the IUGS (Ogg 2004). Recent studies by Ogg & Hinnov (2012), moved the base of the Tithonian to an older age, and propose a limit at 152.1 Ma. However, in the Tordillo Formation, the U -Pb detrital zircon ages indicate a statistically robust measure of the maximum depositional age at c. 144 Ma. ...
... We used the youngest graphical age peak and this is defined by a prominent peak composed of 37 concordant zircon ages at c. 144 Ma. This younger age indicates a discrepancy of at least 7 Ma with the absolute ages for the Kimmeridgian and Tithonian boundaries from the chronostratigraphic timescale of Ogg & Hinnov (2012). This also raises questions about the true absolute age of the Jurassic -Cretaceous boundary. ...
Article
Full-text available
New U–Pb detrital zircon ages are presented for the Tordillo Formation. The ages indicate that the most important source region of sediment supply was the Jurassic Andean arc (peaks at c. 144, 153 and 178 Ma), although two secondary sources were defined at c. 218 and 275 Ma. Temporal variation in the provenance indicates that at the beginning of the sedimentation, Carboniferous to Lower Jurassic magmatic rocks and Lower Palaeozoic metamorphic rocks were the most important sources. Towards the top, the data suggest that the Andean arc becomes the main source region. The comparison between provenance patterns of the Tordillo Formation and of the Avilé Member (Agrio Formation) showed some differences. In the former, the arc region played a considerable role as a source region, but this is not identified in the latter. The results permit a statistically robust estimation of the maximum deposition age for the Tordillo Formation at c. 144 Ma. This younger age represents a discrepancy of at least 7 Ma from the absolute age of the Kimmeridgian and Tithonian boundary (from the chronostratigraphic timescale accepted by the International Commission of Stratigraphy, IUGS), and has strong implications for the absolute age of the Jurassic–Cretaceous boundary. Supplementary material Sample coordinates, values of the sandstone compositional framework and U–Pb (LAM-MC-ICP-MS) age measurements of zircons grains are available at http://www.geolsoc.org.uk/SUP18718
... Myr vs. 0.3 Myr in GTS2004), our cyclostratigraphic estimates could be used in the future generation of GTS. The recent GTS2012 used our estimate of ∼8.3 Myr from preliminary results (Huang et al., 2010a(Huang et al., , 2010b and added a 200 kyr duration assuming a condensation at the basal Tenuicostatum Zone in Sancerre, for a total duration of ∼8.6 Myr (Ogg and Hinnov, 2012, their Table 26.3). ...
... Also, a duration of 0.8 Myr for the Polymorphum Zone was inferred from the Peniche section, Portugal , although a problem in their cyclostratigraphic interpretation is likely (Kemp et al., 2011; see below, Section 5.1.2). In place of adding an arbitrary 200 kyr duration to the basal Toarcian Stage to compensate for a possible condensation (Ogg and Hinnov, 2012) we suggest future high-resolution cyclostratigraphic studies from thick Lower Toarcian sections (e.g., the Amellago section, Morocco) to constrain the chronology of the Tenuicostatum Zone. ...
Article
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The Toarcian Oceanic Anoxic Event (T-OAE) of the early Jurassic period involves one of the largest perturbations of the carbon cycle in the past 250 Ma, recorded by a pronounced negative carbon-isotope excursion (CIE). Numerous studies have focused on potential causes of the T-OAE and CIE, but are hampered by an uncertain timescale. Here we present high-resolution (∼2 kyr∼2 kyr) magnetic susceptibility (MS) measurements from the marine marls of the Sancerre-Couy drill-core, southern Paris Basin, spanning the entire Toarcian Stage. The MS variations document a rich series of sub-Milankovitch to Milankovitch frequencies (precession, obliquity and eccentricity) with the periodic g2–g5 (405 kyr) and quasi-periodic g4–g3 (∼2.4 Myr∼2.4 Myr Cenozoic mean periodicity) eccentricity terms being the most prominent. The MS-related g4–g3 variation reflects third-order eustatic sequences, and constrains the sequence stratigraphic framework of the Toarcian Stage. In addition, MS variations reveal a modulation of g2–g5 by g4–g3 eccentricity related cycles, suggesting that sea-level change was the main control on the deposition of the Toarcian Sancerre marls, in tune with the astro-climatic frequencies. The stable 405 kyr cyclicity constrains a minimum duration of the Toarcian Stage to ∼8.3 Myr∼8.3 Myr, and the well documented CIE, associated with the T-OAE, to ∼300 to 500 kyr. The 405 kyr MS timescale calibrates the periodicity of the prominent high-frequency δC13 cycles that occur in the decreasing part of the CIE to 30 to 34 kyr, consistent with the Toarcian obliquity period predicted for an Earth experiencing sustained tidal dissipation.
... In vertebrate groups, there is similar evidence for a faunal turnover in the marine (Steel, 1973; (1) Stratigraphic age of the J/K boundary Recently, there has been substantial progress in determining the age of the J/K stratigraphic boundary, along with attempts at a global correlation (Wimbledon et al., 2011). Mahoney et al. (2005) previously proposed an age of 145.5 ± 0.8Ma, a result that has since been widely accepted as the age of the J/K boundary (Ogg & Hinnov, 2012; although see below). Of particular note is the biostratigraphic use of calpionellids (calcareous microplankton), which have helped to refine the dating of the base of the Cretaceous (Blau & Grun, 1997;Hauser et al., 2007;Casellato, 2010;Pruner et al., 2010). ...
Preprint
The Late Jurassic to Early Cretaceous interval represents a time of environmental upheaval and cataclysmic events, combined with disruptions to terrestrial and marine ecosystems. Historically, the Jurassic/Cretaceous (J/K) boundary was classified as one of eight mass extinctions. However, more recent research has largely overturned this view, revealing a much more complex pattern of biotic and abiotic dynamics than has previously been appreciated. Here, we present a synthesis of our current knowledge of Late Jurassic–Early Cretaceous events, focusing particularly on events closest to the J/K boundary. We find evidence for a combination of short-term catastrophic events, large-scale tectonic processes and environmental perturbations, and major clade interactions that led to a seemingly dramatic faunal and ecological turnover in both the marine and terrestrial realms. This is coupled with a great reduction in global biodiversity which might in part be explained by poor sampling. Very few groups appear to have been entirely resilient to this J/K boundary ‘event’, which hints at a ‘cascade model’ of ecosystem changes driving faunal dynamics. Within terrestrial ecosystems, larger, more-specialised organisms, such as saurischian dinosaurs, appear to have suffered the most. Medium-sized tetanuran theropods declined, and were replaced by larger-bodied groups, and basal eusauropods were replaced by neosauropod faunas. The ascent of paravian theropods is emphasised by escalated competition with contemporary pterosaur groups, culminating in the explosive radiation of birds, although the timing of this is obfuscated by biases in sampling. Smaller, more ecologically diverse terrestrial non-archosaurs, such as lissamphibians and mammaliaforms, were comparatively resilient to extinctions, instead documenting the origination of many extant groups around the J/K boundary. In the marine realm, extinctions were focused on low-latitude, shallow marine shelf-dwelling faunas, corresponding to a significant eustatic sea-level fall in the latest Jurassic. More mobile and ecologically plastic marine groups, such as ichthyosaurs, survived the boundary relatively unscathed. High rates of extinction and turnover in other macropredaceous marine groups, including plesiosaurs, are accompanied by the origin of most major lineages of extant sharks. Groups which occupied both marine and terrestrial ecosystems, including crocodylomorphs, document a selective extinction in shallow marine forms, whereas turtles appear to have diversified. These patterns suggest that different extinction selectivity and ecological processes were operating between marine and terrestrial ecosystems, which were ultimately important in determining the fates of many key groups, as well as the origins of many major extant lineages. We identify a series of potential abiotic candidates for driving these patterns, including multiple bolide impacts, several episodes of flood basalt eruptions, dramatic climate change, and major disruptions to oceanic systems. The J/K transition therefore, although not a mass extinction, represents an important transitional period in the co-evolutionary history of life on Earth.
... In vertebrate groups, there is similar evidence for a faunal turnover in the marine (Steel, 1973; (1) Stratigraphic age of the J/K boundary Recently, there has been substantial progress in determining the age of the J/K stratigraphic boundary, along with attempts at a global correlation (Wimbledon et al., 2011). Mahoney et al. (2005) previously proposed an age of 145.5 ± 0.8Ma, a result that has since been widely accepted as the age of the J/K boundary (Ogg & Hinnov, 2012; although see below). Of particular note is the biostratigraphic use of calpionellids (calcareous microplankton), which have helped to refine the dating of the base of the Cretaceous (Blau & Grun, 1997;Hauser et al., 2007;Casellato, 2010;Pruner et al., 2010). ...
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Mudstones from the Argiles de Châtillon Formation exposed in the Boulonnais region of Northern France represent a proximal lateral equivalent of the organic-rich Kimmeridge Clay Formation. The Argiles de Châtillon Formation is composed of two subunits that straddle the Kimmeridgian–Tithonian boundary. Each subunit contains an organic-rich interval. The two conspicuous organic-rich intervals have been linked to either periods of high sea level or greenhouse warming. Here, we use palynology to further understand climate and environmental mechanisms that drove organic matter enrichment. We use bulk organic carbon isotope records (δ ¹³ C org ) to correlate the Boulonnais sections with those of the Kimmeridge Clay Formation. The palynological results suggest that the stratigraphically lower organic-rich interval (Kimmeridgian) was deposited under suboxic to anoxic stratified conditions. A large-scale climate shift from cooler/humid to warmer/arid conditions marked the Kimmeridgian–Tithonian boundary, influencing organic matter enrichment in the stratigraphically higher organic-rich interval (Tithonian). In contrast with the lower organic-rich interval, there are no indications of stratified conditions for the higher organic-rich interval. Within this thicker organic-rich interval, cyclic variations in amorphous organic matter distribution, total organic carbon and δ ¹³ C org trends on a 2 m scale are observed. They co-occur with fluctuations of the palynological assemblages, indicative of more humid versus arid climate conditions, likely alternating on a ∼100 kyr eccentricity timescale. Our results show that under the most humid phases of these overall arid climate conditions, sulfurization of carbohydrates was the dominant control on organic matter preservation. This climate-controlled process that drives organic matter enrichment in the Tithonian can be recognized on a basin-wide scale.
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The discovery of Tethyan and Boreal fossils in Bathonian deposits of the Sokur section in the vicinity of Saratov (Central Russia) reopened the possibility of direct correlation of the Bathonian sections in different paleobiogeographic provinces, which require further integrated studies involving both paleontological (based on different groups of fauna) and physicochemical (paleomagnetic and isotope-geochemical) methods. Stable carbon isotope data for belemnite (Cylindroteuthididae) rostra from the Sokur section show that the Subboreal Oraniceras besnosovi Zone and Boreal Arcticoceras harlandi Subzone are correlated with the Zigzag Zone of the standard scale, whereas the Boreal A. ishmae Subzone can be correlated completely or, even partly, with the Tenuiplicatus Zone. We identified equivalents of chrons of the geomagnetic polarity time scale (GPTS): e-Bath N, m-Bath R, and lt-Bath N, corresponding to the Lower–Middle Bathonian and, possibly, lowermost Upper Bathonian. Article link, which provides free access to the article and is valid until April 05, 2017 https://authors.elsevier.com/a/1UZ1n3p12uWtra
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The source rock characteristics (e.g. thickness, lateral extension, richness) are known to be highly variable in both time and space. The Lower Jurassic formations of north-western Europe contain source rocks with organic-rich intervals showing different characteristics from one region to another: the Paris Basin differs from the South-East Basin of France, but organic content and hydrogen index also vary within a single basin. During the Early Jurassic, the overall depositional environment of north-western Europe corresponded to an epicontinental domain at the western extremity of the Tethys Ocean. The early transgressive phase of the Jurassic induced flooding of this European realm. Because of the evolution of the connections and threshold of the European basins and their associated sedimentary settings, this domain occupied a key position for the deposition of organic-rich layers. Using a forward modelling approach, we aim to predict the heterogeneous characteristics of such sediments. It is widely accepted that primary productivity and preservation are key factors favouring the accumulation of organic-rich layers. However, the roles of these factors remain to be assessed and the processes leading to accumulation and preservation need to be quantified.
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Mixed calcareous-agglutinated benthic foraminiferal assemblages have been obtained from five hydrocarbon seep carbonate structures in the upper Slottsmøya Member (Agardhfjellet Formation) in central Spitsbergen, Svalbard. The composition of the agglutinated component is comparable to faunas previously described from the surrounding dark shales of the Slottsmøya Member, as well as from deposits of Arctic Russia and other areas of the Boreal Realm. Calcareous foraminifera are observed only in thin-sections. The foraminifera date the hydrocarbon seep bodies as Late Volgian - Late Ryazanian; an age determination in part slightly divergent from ammonite datings previously recorded from these carbonates. This is the first systematic report of foraminifera from seep structures developed at the Jurassic-Cretaceous transition.
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We here briefly introduce the distribution, sedimentary characteristics and filling sequence of the Tuchengzi Formation in northern North China. On the basis of the uncertainty of the age of the Tuchengzi Formation, we analyzed all the isotopic dating data and constrained the age of Tuchengzi Formation to be 154-137 Ma. Previous biostratigraphy research is consistent with the age of Tuchengzi Formation. The International Commission on Stratigraphy (ICS) proposed 145 Ma to be the age of Jurassic-Cretaceous boundary in 2013, which is supported by recent studies in the Tethys-Himalaya and Andes, although more high-precision geochronology is still needed for the final establishment. This boundary age suggests that the Tuchengzi Formation is the Late Jurassic-Early Cretaceous in age, and the terrestrial Jurassic-Cretaceous boundary in China exists in the Tuchengzi Formation. The international stratigraphic boundary, especially for the J/K boundary, should be established by the marine biostratigraphy. The establishment of the J/K boundary in China should give priority to obey the symbol and achievement derived from the marine biostratigraphy and organic evolution.
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Integrative studies of sedimentary and palaeontological topics for unconformity surfaces are useful in basin analysis. A middle Bathonian unconformity surface in the Ammonitico Rosso facies cropping out in the La Mola Unit (Subbetic Domain, Betic External Zone) was studied by integrating ichnological, palaeotectonic, and sedimentological analyses to decipher sea-level, tectonic, and palaeogeographic conditions during its development. The trace-fossil assemblage mainly consists of the Glossifungites (Thalassinoides, Arenicolites, and Gastrochaenolites) and Trypanites ichnofacies elements. Probable Ophiomorpha represents previous softground stages, Thalassinoides and Arenicolites were formed in firmground, Gastrochaenolites reflects an evolved firmground or early hardground, and Trypanites can be attributed to an incipient hardground. The degree of firmness, relative sea-level position, and continuity of deposition were related. The softground stage corresponds to a fall in relative sea level and continued deposition. The firmground (semi-consolidated substrate) probably reflects an extremely low sea level characterized by non-deposition, whereas the incipient hardground stage indicates an initial phase of relative sea-level rise, with an increase in marine current energy. The presence of two neptunian dyke systems reflects significant tectonic activity related to the transtensional deformation that affected the South Iberian Palaeomargin. Lateral variations in sedimentological and ichnological features recorded at similar discontinuity surfaces in nearby areas were considered and related to differences in bottom topography, with associated changes in sedimentation, and to the variable duration of the hiatus.
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Ichthyosaur diversity near the Jurassic-Cretaceous boundary, particularly from high paleolatitudes, is poorly known. Two recently collected specimens of medium- to large-bodied ichthyosaurs from the Slottsmøya Member of the Agardhfjellet, Svalbard, Norway represent two new taxa of ophthalmosaurids. The holotype specimen of Cryopterygius kristiansenae gen et sp. nov., PMO 214.578, is a nearly complete and largely articulated skeleton. The specimen consists of a nearly complete skull, the entire presacral and preflexural vertebral series, numerous dorsal ribs and gastralia, an articulated pectoral girdle and nearly complete forelimb, and an articulated left pelvic girdle and hindlimb. The new taxon is diagnosed on a unique suite of features, including a robust and moderately elongate rostrum, a reduced supranarial process, an elongate maxilla that bears a high number of teeth, the absence of a lacrimal-external naris contact, and an anteroposteriorly broad postorbital bar possessing an unidentified element (supratemporal?) that lies posterior to the quadratojugal. Cryopterygius has 52 presacral vertebrae, a distinctive forelimb, including a humerus that bears only two facets at its distal end, and an articulated left pelvic girdle and hindlimb, which facilitates the unequivocal orientation of the ophthalmosaurid femur. The holotype specimen of Palvennia hoybergeti, SVB 1451, includes a nearly complete skull and fragmented postcranial remains. It is diagnosed on its relatively short rostrum, greatly enlarged orbit, narrow postorbital bar, very large pineal foramen, basioccipital with broad extracondylar area laterally, and a gracile stapedial shaft. The Slottsmøya Lagerstätte is established as one of the most productive horizons for Upper Jurassic ichthyosaurs and considerably expands our knowledge of ophthalmosaurid diversity and distribution in the latest Jurassic.
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The revision of the geochronological ranges of the Boreal genera Arctocephalites and Arcticoceras found in the Middle Volga region (Middle Povolzhye) together with Peri-Tethyan ammonites resulted in the revision of the stratigraphic position of several zones in the Middle Jurassic ammonite scale of Siberia. It is shown that the Arctic genus Arcticoceras appeared in the early Bathonian, rather than in the middle Bathonian, as is cited in the current Siberian zonal scale. The geochronology of zones preceding the zones with Arcticoceras also needs revision. The lower jugatus Subzone in the arcticus Zone (equivalent to the upper Bajocian niortense Zone in the northwestern European zonal standard) can be used as a correlation marker level. The upper arcticus Subzone is correlated to the two upper Bajocian zones, greenlandicus and harlandi zones, whereas the ishmae Zone correlates with the lower Bathonian zigzag Zone. The gracilis and borealis zones, considered as equivalents of the humphriesianum Zone, should be transferred to the lower Bajocian. No ammonites were found in the middle Bathonian.
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The Late Triassic was a prolonged interval of elevated extinction rates and low origination rates that manifested themselves in a series of extinctions during Carnian, Norian and Rhaetian time. Most of these extinctions took place in the marine realm, particularly affecting radiolarians, conodonts, bivalves, ammonoids and reef-building organisms. On land, the case for a Late Triassic mass extinction is much more tenuous and has largely focused on tetrapod vertebrates (amphibians and reptiles), though some workers advocate a sudden end-Triassic (TJB) extinction of land plants. Nevertheless, an extensive literature does not identify a major extinction of land plants at the TJB, and a comprehensive review of palynological records concluded that TJB vegetation changes were non-uniform (different changes in different places), not synchronous and not indicative of a mass extinction of land plants. Claims of a substantial perturbation of plant ecology and diversity at the TJB in East Greenland are indicative of a local change in the paleoflora largely driven by lithofacies changes resulting in changing taphonomic filters. Plant extinctions at the TJB were palaeogeographically localized events, not global in extent. With new and more detailed stratigraphic data, the perceived TJB tetrapod extinction is mostly an artifact of coarse temporal resolution, the compiled correlation effect. The amphibian, archosaur and synapsid extinctions of the Late Triassic are not concentrated at the TJB, but instead occur stepwise, beginning in the Norian and extending into the Hettangian. There was a disruption of the terrestrial ecosystem across the TJB, but it was more modest than generally claimed. The ecological severity of the end-Triassic nonmarine biotic events are relatively low on the global scale. Biotic turnover at the end of the Triassic was likely driven by the CAMP (Central Atlantic Magmatic Province) eruptions, which caused significant environmental perturbations (cooling, warming, acidification) through outgassing, but the effects on the nonmarine biota appear to have been localized, transient and not catastrophic. Long-term changes in the terrestrial biota across the TJB are complex, dia-chronous and likely climate driven evolutionary changes in the context of fluctuating background extinction rates, not a single, sudden or mass extinction. ScienceDirect j ou rna l h ome pag e: http://www.journals.elsevier.com/journal-of-pal ae og eog raph y/ j o u r n a l o f p a l a e o g e o g r a p h y 4 (2 0 1 5) 3 3 1 e3 4 8
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A palaeomagnetic study has been carried out in five Lower Jurassic sections from the Neuquén basin, made up mainly of ammonitebearing sedimentary and, subordinately, volcanic rocks. Sampled sections are located to the north of the basin, along the Atuel river (Hettangian to Toarcian) and to the centre (Pliensbachian to Toarcian) of the basin. The palaeomagnetic study shows two magnetic components carried by titanomagnetites, one soft with a direction in coincidence with the local dipolar field, and another harder that is interpreted as the original Jurassic based on the field tests for palaeomagnetic stability. From the polarity successions obtained in each locality, a composite magnetostratigraphic scale for the Southern Hemisphere has been constructed. The resultant scale bears 11 zones of dominant reverse polarity (JR 1 to JR 11), and 12 zones of dominant normal polarity (JN 1 to JN 12), which have been tied to 19 ammonite zones of the Andean Region. The regional scale has, in turn, been correlated to the international geomagnetic time scale. A good fit between the two scales is observed, allowing to date intervals with no diagnostic fossils. On the other hand, two palaeomagnetic poles have been calculated, one for the Hettangian-Sinemurian interval (223°E, 51°S, A 95= 6°, N = 25) and the other for the Pliensbachian- Toarcian (67°E, 74°S, A 95= 5°, N = 52). Such poles were combined with others from the literature to obtain the apparent polar wander (APW) path for South America, which turns out to be remarkably dissimilar from the classical ones that show the continent in a stationary position throughout the Mesozoic. From the new APW path, it has been interpreted that South America may have rotated clockwise while it moved to the north. Eurasia's path is also presented in this study, revealing the same shape and chronology of tracks. These latitudinal changes that we observed from the palaeomagnetic data are supported by palaeoecological data.
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The Late Jurassic evolution of Boreal and Arctic basins is reflected in the widespread deposition of organic-rich black shales (source rocks). In this connection, the priority should be placed on the development and refinement of zonal schemes for the Upper Jurassic of the Laptev Sea coast based on ammonites, foraminifers, ostracods, dinocysts, and spores and pollen from reference sections as the basis for stratigraphic, paleogeographic, and facies studies. The Upper Jurassic and Lower Cretaceous reference section of interest is located on the left side of the Anabar Bay of the Laptev Sea (Nordvik Peninsula, Urdyuk-Khaya Cape). An uninterrupted and continuous section from Upper Oxfordian to Lower Valanginian is exposed in coastal cliffs and consists mainly of silty clay deposits with abundant macro- and microfossils. A reliable biostratigraphic subdivision of the Upper Jurassic interval of this section was taken as the basis for the assessment of the correlation potential of different fossil groups and subsequent interregional correlations, facies analysis, and detailed paleogeographic reconstructions of the study area. The analysis of variations in the composition of macrobenthic communities and microphytoplankton and terrestrial palynomorph assemblages and the biofacies analysis allowed the reconstruction of the evolution of marine paleoenvironmental settings in the western part of the Anabar-Lena sea and in the terrestrial settings in the adjacent land area of Siberia.
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One of the main controversial items in palaeoclimatology is to elucidate if climate during the Jurassic was warmer than present day, with no ice caps, or if ice caps were present in some specific intervals. The Pliensbachian Cooling event (Lower Jurassic) has been pointed out as one of the main candidates to have developed ice caps on the poles. To constrain the timing of this cooling event, including the palaeoclimatic evolution before and after cooling, as well as the calculation of the seawater palaeotemperatures are of primary importance to find arguments on this subject. For this purpose, the Rodiles section of the Asturian Basin (Northern Spain), a well exposed succession of the uppermost Sinemurian, Pliensbachian and Lower Toarcian deposits, has been studied. A total of 562 beds were measured and sampled for ammonites, for biostratigraphical purposes and for belemnites, to determine the palaeoclimatic evolution through stable isotope studies. Comparison of the recorded uppermost Sinemurian, Pliensbachian and Lower Toarcian changes in seawater palaeotemperature with other European sections allows characterization of several climatic changes of probable global extent. A warming interval which partly coincides with a negative δ13Cbel excursion was recorded at the Upper Sinemurian. After a "normal" temperature interval, a new warming interval that contains a short lived positive δ13Cbel peak, was developed at the Lower-Upper Pliensbachian transition. The Upper Pliensbachian represents an outstanding cooling interval containing a positive δ13Cbel excursion interrupted by a small negative δ13Cbel peak. Finally, the Lower Toarcian represented an exceptional warming period pointed as the main responsible for the prominent Lower Toarcian mass extinction.
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The paper describes Late Jurassic–Early Cretaceous seep carbonate boulders from the Russian Arctic island of Novaya Zemlya, collected in 1875 by A.E. Nordenskiöld during his expedition to Siberia. The carbonates are significantly depleted in heavy carbon isotopes (δ13C values as low as ca. − 40‰) and show textures typical for carbonates formed under the influence of hydrocarbons, such as fibrous carbonate cements and corrosion cavities. The rocks contain index fossils of Late Oxfordian–Early Kimmeridgian, Late Tithonian (Jurassic) and latest Berriasian–Early Valanginian (Cretaceous) age. The fossil fauna is species rich and dominated by molluscs, with subordinate brachiopods, echinoderms, foraminifera, serpulids and ostracods. Most of the species, including two chemosymbiotic bivalve species, likely belong to the ‘background’ fauna. Only a species of a hokkaidoconchid gastropod, and a possible abyssochrysoid gastropod, can be interpreted as restricted to the seep environment. Other seep faunas with similar taxonomic structure are suggestive of rather shallow water settings, but in case of Novaya Zemlya seep faunas such structure might result also from high northern latitude.
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Manganese (Mn) carbonate nodules, which differ from seafloor Mn nodules mainly composed of MnO2, are occasionally embedded in the form of a lens shape in the Jurassic accretionary complexes, such as the Mino Belt in Japan. The interpretation of the formation process of Mn carbonate is still controversial, particularly concerning whether the Mn carbonate was formed primarily or secondarily. In this study, a fresh Mn carbonate nodule incorporated into the red siliceous mudstone was collected for geochemical and sedimentological analysis. The optical observation of thin sections indicates that the Mn carbonate nodules are composed of abraded grains of rhodochrosite spherule with radiolarians and are sedimentary embedded in siliceous mudstone. Microfossil radiolarians from the Mn carbonate nodules and the host red siliceous mudstone are dated as the Bajocian, but the radiolarians in the nodules are somewhat older than those in the host red siliceous mudstone.
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One of the most profound environmental changes in the Mesozoic took place during Pliensbachian-Toarcian (Early Jurassic), including oceanic anoxia (Toarcian Oceanic Anoxic Event; T-OAE). The T-OAE is thought to have been caused by increased atmospheric CO2 triggered by Karoo–Ferrar volcanism. This idea, however, remains debated, primarily due to uncertainties in their age constraints of the relevant sedimentary sequences. To examine their temporal relationships, herein, we provide the astronomical time scale of the Lower Jurassic deep-sea bedded chert sequences from the pelagic Panthalassa superocean, which are exposed in the Inuyama area, central Japan. A 405-kyr tuned astrochronology, anchored to the end-Triassic extinction as 201.4 ± 0.2 Ma (Ikeda and Tada, 2013), allows us to constrain the ages of two black bedded cherts (T-OAE1 and T-OAE2). The ages of these T-OAEs overlap U–Pb ages of Karoo volcanic rocks. T-OAE in the European region is also synchronous with the Karoo–Ferrar volcanism, based on radiolarian and ammonite biostratigraphic correlation. These temporal relationships support the potential impact of Karoo–Ferrar volcanism on T-OAEs on a global scale. On the other hand, the onset of T-OAEs occur at the maxima of ~ 40 kyr, ~ 100 kyr, and 405 kyr cycles of chert thickness variation. The termination of T-OAEs and the recovery to oxic conditions in pelagic ocean coincide with the minima of ~ 40 kyr, ~ 100 kyr, and 405 kyr cycles of chert thickness. Moreove, the termination of final black chert and grey chert deposition coincide with the minima of ~ 1800 kyr cycles of chert thickness. These temporal relationships imply that orbital-scale productivity cycles were important in controlling the onset and termination of T-OAEs through the carbon cycle dynamics, which have been already amplified by Karoo–Ferrar volcanism.
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