scholarly journals Large Igneous Province Record Through Time and Implications for Secular Environmental Changes and Geological Time‐Scale Boundaries

Author(s):  
Richard E. Ernst ◽  
David P. G. Bond ◽  
Shuan‐Hong Zhang ◽  
Kenneth L. Buchan ◽  
Stephen E. Grasby ◽  
...  
2021 ◽  
Author(s):  
Michael Way ◽  
Richard Ernst ◽  
Jeffrey Scargle

<p class="p1"><span class="s1">Large scale volcanism has played a critical role in the long-term habitability </span><span class="s1">of Earth and possibly Venus.<span class="Apple-converted-space">  </span>We examine the timing of Large Igneous Provinces </span><span class="s1">(LIPs) through Earth’s history [1] to estimate the likelihood of nearly simultaneous </span><span class="s1">events that could drive a planet into an extreme moist or runaway greenhouse, </span><span class="s1">quenching subductive plate tectonics. Such events would end volatile cycling </span>and may have caused the heat-death of Venus. Using the Earth's LIP record <span class="s1">a conservative estimate of the rate of LIPs in a random history statistically </span>the same as Earth’s, pairs and triplets of LIPs closer in time <span class="s1">than 0.1-1 Myrs are likely. This simultaneity threshold is significant to the </span><span class="s1">extent that it is less than the time over which environmental effects </span><span class="s1">have been shown to persist, for example in the Siberian Traps record [2,3].</span></p> <p class="p1"><span class="s1">[1] Ernst, R.E. et al. (2021). Large Igneous Province Record Through Time and </span><span class="s1">Implications for Secular Environmental Changes and Geological Time-Scale </span>Boundaries. In: Ernst, R.E., Dickson, A.J., Bekker, A. (eds.) Large Igneous <span class="s1">Provinces: A Driver of Global Environmental and Biotic Changes. AGU Geophysical </span><span class="s1">Monograph 255 (pp. 3-26).</span></p> <p class="p1"><span class="s1">[2] Burgess, S.D. et al. (2014). High-precision timeline for Earth’s most </span><span class="s1">severe extinction. Proceedings of the National Academy of Sciences, 111:</span></p> <p class="p1"><span class="s1">3316–3321 [correction 2014, 111: 5050]. </span></p> <p class="p1"><span class="s1">[3] Burgess, S.D. & Bowring, S.A. (2015). High-precision geochronology confirms </span><span class="s1">voluminous magmatism before, during and after Earth's most severe extinction. </span><span class="s1">Sci. Adv. 1 (7), e1500470. http://dx.doi.org/10.1126/sciadv.1500470. </span></p>


2021 ◽  
Author(s):  
Mathieu Martinez ◽  
Beatriz Aguirre-Urreta ◽  
Marina Lescano ◽  
Guillaume Dera ◽  
Julieta Omarini ◽  
...  

<p>The interval from the Valanginian to the Barremian stages (137–121 Ma; Early Cretaceous) is punctuated by several episodes of environmental changes, accompanied by shifts in weathering intensity on the continents and changes in the Tethyan neritic carbonate production. We synthetize here the astrochronology of two recent studies performed in the Neuquén basin, Vocontian Basin and Subbetic Domain (Aguirre-Urreta et al., 2019; Martinez et al., 2020), anchored to CA-ID-TIMS U-Pb ages, which conclusions have been included in the Geologic Time Scale 2020 (Gale et al, in press). We applied this time scale to a compilation of carbon-isotope ratio from belemnites and proxies of detrital supply in the Tethyan area (Vocontian Basin and Subbetic Domain). From this compilation, we show that the episodes of environmental changes are paced by a 2.4-Myr cycle and, with a lower amplitude, a 1.2-Myr cycle. In addition, the new time scale shows the synchronicity between the Weissert Event and the Parana-Etendeka Large Igneous Province. In the series of carbon-isotope ratios measured on belemnite rostra, the amplitude of the 2.4-Myr cycle is twice higher during the Valanginian than in the Late Barremian and three times higher than in the Hauterivian and Early Barremian, suggesting that the activity of the Parana-Etendeka Large Igneous Province amplified the initial orbital forcing to trigger the environmental changes observed during the Mid-Valanginian.</p><p>Reference:</p><p>Aguirre-Urreta, B., Martinez, M., Schmitz, M., Lescano, M., Omarini, J., Tunik, M., Kuhnert, H., Concheyro, A., Rawson, P.F., Ramos, V.A., Reboulet, S., Noclin, N., Frederichs, T., Nickl, A.-L., Pälike, H., 2019. Interhemispheric radio-astrochronological calibration of the time scales from the Andean and the Tethyan areas in the Valanginian–Hauterivian (Early Cretaceous). Gondwana Research 70, 104-132. https://doi.org/10.1016/j.gr.2019.01.006.</p><p>Gale, A.S., Mutterlose, J., Batenburg, S., in press. Chapter 27: The Cretaceous Period, in: Gradstein, F.M., Ogg, J.G., Schmitz, M.D., Ogg, G.M. (Eds.) Geologic Time Scale 2020. Elsevier BV, Amsterdam, The Netherlands, pp. 1023–1086.</p><p>Martinez, M., Aguado, R., Company, M., Sandoval, J., O’Dogherty, L., 2020. Integrated astrochronology of the Barremian Stage (Early Cretaceous) and its biostratigraphic subdivisions. Global and Planetary Change 195, 103368. https://doi.org/10.1016/j.gloplacha.2020.103368.</p>


2009 ◽  
Vol 96 (4) ◽  
pp. 249-262 ◽  
Author(s):  
Brian McGowran ◽  
Bill Berggren ◽  
Frits Hilgen ◽  
Fritz Steininger ◽  
Marie-Pierre Aubry ◽  
...  

2021 ◽  
Vol 3-4 (185-186) ◽  
pp. 56-64
Author(s):  
Svitlana Hnylko

Paleogene deposits are the main reservoir of hydrocarbon resources in the Carpathians and creation of the modern stratigraphic scheme of these deposits is the basis for improving the efficiency of geological search works. The reliable stratification is a necessary precondition for the preparation of geological maps. Stratification of the Paleocene–Eocene sediments is provided by foraminifera, nannoplankton, dinocysts, radiolarians, sponge spicules, palynoflora. Planktonic foraminifera is the main stratigraphic group of the Paleogene fauna. In the predominantly non-calcareous flysch of the Paleocene–Eocene of the Carpathians, mainly agglutinated benthic foraminifera of siliceous composition are developed. Planktonic foraminifera are distributed locally – in calcareous facies. The most complete sequence of Paleocene–Eocene planktonic foraminifera is represented in the Metova Formation (the Vezhany nappe of the Inner Carpathians). The results of own researches of natural sections of sediments distributed within the Magursky, Monastyretsky and Vezhany nappes of the Ukrainian Carpathians together with the analysis of literature sources are used. The article presents a generalized biozonal division of the Paleocene–Eocene of the Ukrainian Carpathians by planktonic foraminifera. On the basis of certain correlation levels, a comparison with the Geological Time Scale was made. The Parvularugoglobigerina eugubina Zone (lowermost Danian), Globoconusa daubjergensis Zone (middle Danian), Praemurica inconstans Zone (upper Danian); Morozovella angulata Zone (lower Selandian); Globanomalina pseudomenardii Zone fnd Acarinina acarinata Zone (upper Selandian–Thanetian); Morozovella subbotinae Zone (lower Ypresian), Morozovella aragonensis Zone (upper Ypresian); Acarinina bullbrooki Zone (lower Lutetian), Acarinina rotundimarginata Zone (upper Lutetian); Hantkenina alabamensis Zone (Bartonian); Globigerinatheka tropicalis Zone (lower Priabonian) and Subbotina corpulenta Zone (upper Priabonian) based on planktonic foraminifera are characterized in studied deposits.


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