New Age of Fishes Initiated by the Cretaceous−Paleogene Mass Extinction
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Is Earth's Magnetic Field Reversing? ⁎ Catherine Constable A, , Monika Korte B
Earth and Planetary Science Letters 246 (2006) 1–16 www.elsevier.com/locate/epsl Frontiers Is Earth's magnetic field reversing? ⁎ Catherine Constable a, , Monika Korte b a Institute of Geophysics and Planetary Physics, Scripps Institution of Oceanography, University of California at San Diego, La Jolla, CA 92093-0225, USA b GeoForschungsZentrum Potsdam, Telegrafenberg, 14473 Potsdam, Germany Received 7 October 2005; received in revised form 21 March 2006; accepted 23 March 2006 Editor: A.N. Halliday Abstract Earth's dipole field has been diminishing in strength since the first systematic observations of field intensity were made in the mid nineteenth century. This has led to speculation that the geomagnetic field might now be in the early stages of a reversal. In the longer term context of paleomagnetic observations it is found that for the current reversal rate and expected statistical variability in polarity interval length an interval as long as the ongoing 0.78 Myr Brunhes polarity interval is to be expected with a probability of less than 0.15, and the preferred probability estimates range from 0.06 to 0.08. These rather low odds might be used to infer that the next reversal is overdue, but the assessment is limited by the statistical treatment of reversals as point processes. Recent paleofield observations combined with insights derived from field modeling and numerical geodynamo simulations suggest that a reversal is not imminent. The current value of the dipole moment remains high compared with the average throughout the ongoing 0.78 Myr Brunhes polarity interval; the present rate of change in Earth's dipole strength is not anomalous compared with rates of change for the past 7 kyr; furthermore there is evidence that the field has been stronger on average during the Brunhes than for the past 160 Ma, and that high average field values are associated with longer polarity chrons. -
The Relationship Between the Iridium Anomaly and Palynological Floral Events at Three Cretaceous-Tertiary Boundary Localities in Western Canada
The relationship between the iridium anomaly and palynological floral events at three Cretaceous-Tertiary boundary localities in western Canada JOHN F. LERBEKMO University of Alberta, Department of Geology, Edmonton, Alberta T6G 2E3, Canada ARTHUR R. SWEET Geological Survey of Canada, 3303 33 Street N. W., Calgary, Alberta T2L 2E7, Canada ROBERT M. ST. LOUIS* University of Alberta, Department of Geology, Edmonton, Alberta T6G 2E3, Canada ABSTRACT Snead, 1969; a series of papers by Srivastava, culminating in Srivastava, 1970; Leffingwell, 1971; Tschudy, 1971; Sweet, 1978) concerning the Profiles illustrating the abundance of iridium and the changes in region from Colorado through Montana and into Saskatchewan and the relative abundances of major groups within the palynoflora are Alberta substantiated Stanley's work. Collectively, these papers demon- given for three localities from western Canada. The peak abundance strate that the flora coexisting with the dinosaurian Triceratops fauna (of of iridium ranges from 1.35 to 5.60 ppb and corresponds to the base of late Maastrichtian age; Jeletzky, 1960) is characterized by a diverse suite a coal and to a floral-extinction event at the three localities. Imme- of angiosperm pollen that generally dominates the over-all assemblage. diately above the iridium-peak anomaly, angiosperm pollen is con- The most visually conspicuous taxa in this flora belong to Aquilapollenites, spicuous in the assemblage, in contrast to the fern-spore spike Wodehouseia, and allied angiosperm genera, although they rarely exceed a described for sections in the mid-continental United States and at the few percent in relative abundance. Above beds carrying the Triceratops Morgan Creek locality in south-central Saskatchewan. -
Asteroid Impact, Not Volcanism, Caused the End-Cretaceous Dinosaur Extinction
Asteroid impact, not volcanism, caused the end-Cretaceous dinosaur extinction Alfio Alessandro Chiarenzaa,b,1,2, Alexander Farnsworthc,1, Philip D. Mannionb, Daniel J. Luntc, Paul J. Valdesc, Joanna V. Morgana, and Peter A. Allisona aDepartment of Earth Science and Engineering, Imperial College London, South Kensington, SW7 2AZ London, United Kingdom; bDepartment of Earth Sciences, University College London, WC1E 6BT London, United Kingdom; and cSchool of Geographical Sciences, University of Bristol, BS8 1TH Bristol, United Kingdom Edited by Nils Chr. Stenseth, University of Oslo, Oslo, Norway, and approved May 21, 2020 (received for review April 1, 2020) The Cretaceous/Paleogene mass extinction, 66 Ma, included the (17). However, the timing and size of each eruptive event are demise of non-avian dinosaurs. Intense debate has focused on the highly contentious in relation to the mass extinction event (8–10). relative roles of Deccan volcanism and the Chicxulub asteroid im- An asteroid, ∼10 km in diameter, impacted at Chicxulub, in pact as kill mechanisms for this event. Here, we combine fossil- the present-day Gulf of Mexico, 66 Ma (4, 18, 19), leaving a crater occurrence data with paleoclimate and habitat suitability models ∼180 to 200 km in diameter (Fig. 1A). This impactor struck car- to evaluate dinosaur habitability in the wake of various asteroid bonate and sulfate-rich sediments, leading to the ejection and impact and Deccan volcanism scenarios. Asteroid impact models global dispersal of large quantities of dust, ash, sulfur, and other generate a prolonged cold winter that suppresses potential global aerosols into the atmosphere (4, 18–20). These atmospheric dinosaur habitats. -
Paleogene and Neogene Time Scale of GTS 2012 Paleogene Neogene N
Paleogene and Neogene Time Scale of GTS 2012 Paleogene Neogene N. Vandenberghe 1, F.J. Hilgen 2 and R.P. Speijer 3 F.J. Hilgen 1, L.J. Lourens 2 and J.A. Van Dam 3 1. Department of Earth and Environmental Sciences, K. U. Leuven, Celestijnenlaan 200E, B - 3001 Leuven, Belgium, [email protected] 1. Department of Earth Sciences, Utrecht University, Budapestlaan 4, 3584 CD Utrecht, The Netherlands, [email protected] 2. Department of Earth Sciences, Utrecht University, Budapestlaan 4, 3584 CD Utrecht, The Netherlands, [email protected] 2. Department of Earth Sciences, Utrecht University, Budapestlaan 4, 3508 TA Utrecht, The Netherlands, [email protected] 3. Department of Earth and Environmental Sciences, K. U. Leuven, Celestijnenlaal 200E, B - 3001 Leuven, Belgium, [email protected] 3. Institut Català de Paleontologia Miquel Crusafont (ICP), Campus de la UAB, Mòdul ICP, E-08193 cerdanyola del Vallès, Spain, [email protected] Of the 9 Paleogene stages, only 3 remain to be formally defined: the Bartonian and Priabonian stages of upper Paleogene Time Scale Eocene and the Chattian (base of upper Oligocene). Larger 18 13 AGE Epoch/Age Polarity Mega- Dinoflagellate Cysts North American O C AGE -1.0 -0.5 -0.5 Of the 8 Neogene stages, only 2 remain to be formally defined: the Burdigalian and Langhian stages of lower and middle Mio- (Ma) Chron Cycles Planktonic Foraminifera Benthic Calcareous Nannofossils Radiolarians NALMA MP European Mammals ALMA SALMA 0.0 0.5 1.0 1.5 2.0 0.0 0.5 1.0 1.5 2.0 2.5 Age (Stage) (Ma) During the Paleogene, the global climate, being warm (Stage) Northwestern Europe Mammals other zones Foraminifera ELMA R T low latitude southern high latitude until the late Eocene, shows a significant cooling trend cene. -