Genesis of the Western Samoa Seamount Province: Age, Geochemical Fingerprint and Tectonics
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Cenozoic Changes in Pacific Absolute Plate Motion A
CENOZOIC CHANGES IN PACIFIC ABSOLUTE PLATE MOTION A THESIS SUBMITTED TO THE GRADUATE DIVISION OF THE UNIVERSITY OF HAWAI`I IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF MASTER OF SCIENCE IN GEOLOGY AND GEOPHYSICS DECEMBER 2003 By Nile Akel Kevis Sterling Thesis Committee: Paul Wessel, Chairperson Loren Kroenke Fred Duennebier We certify that we have read this thesis and that, in our opinion, it is satisfactory in scope and quality as a thesis for the degree of Master of Science in Geology and Geophysics. THESIS COMMITTEE Chairperson ii Abstract Using the polygonal finite rotation method (PFRM) in conjunction with the hotspot- ting technique, a model of Pacific absolute plate motion (APM) from 65 Ma to the present has been created. This model is based primarily on the Hawaiian-Emperor and Louisville hotspot trails but also incorporates the Cobb, Bowie, Kodiak, Foundation, Caroline, Mar- quesas and Pitcairn hotspot trails. Using this model, distinct changes in Pacific APM have been identified at 48, 27, 23, 18, 12 and 6 Ma. These changes are reflected as kinks in the linear trends of Pacific hotspot trails. The sense of motion and timing of a number of circum-Pacific tectonic events appear to be correlated with these changes in Pacific APM. With the model and discussion presented here it is suggested that Pacific hotpots are fixed with respect to one another and with respect to the mantle. If they are moving as some paleomagnetic results suggest, they must be moving coherently in response to large-scale mantle flow. iii List of Tables 4.1 Initial hotspot locations . -
S41467-020-18361-4.Pdf
ARTICLE https://doi.org/10.1038/s41467-020-18361-4 OPEN Seafloor evidence for pre-shield volcanism above the Tristan da Cunha mantle plume ✉ Wolfram H. Geissler 1 , Paul Wintersteller 2,3, Marcia Maia4, Anne Strack3, Janina Kammann5, Graeme Eagles 1, Marion Jegen6, Antje Schloemer1,7 & Wilfried Jokat 1,2 Tristan da Cunha is assumed to be the youngest subaerial expression of the Walvis Ridge hot spot. Based on new hydroacoustic data, we propose that the most recent hot spot volcanic 1234567890():,; activity occurs west of the island. We surveyed relatively young intraplate volcanic fields and scattered, probably monogenetic, submarine volcanoes with multibeam echosounders and sub-bottom profilers. Structural and zonal GIS analysis of bathymetric and backscatter results, based on habitat mapping algorithms to discriminate seafloor features, revealed numerous previously-unknown volcanic structures. South of Tristan da Cunha, we discovered two large seamounts. One of them, Isolde Seamount, is most likely the source of a 2004 submarine eruption known from a pumice stranding event and seismological analysis. An oceanic core complex, identified at the intersection of the Tristan da Cunha Transform and Fracture Zone System with the Mid-Atlantic Ridge, might indicate reduced magma supply and, therefore, weak plume-ridge interaction at present times. 1 Alfred Wegener Institute, Helmholtz Centre for Polar and Marine Research, Am Alten Hafen 26, 27568 Bremerhaven, Germany. 2 Faculty of Geosciences, University of Bremen, Klagenfurter Str. 4, 28359 Bremen, Germany. 3 MARUM—Center of Marine Environmental Sciences, University of Bremen, Leobener Str. 8, 28359 Bremen, Germany. 4 CNRS-UBO Laboratoire Domaines Océaniques, Institut Universitaire Européen de la Mer, 29280 Plouzané, France. -
Ancient Helium and Tungsten Isotopic Signatures Preserved in Mantle Domains Least Modified by Crustal Recycling
Ancient helium and tungsten isotopic signatures preserved in mantle domains least modified by crustal recycling Matthew G. Jacksona,1, Janne Blichert-Toftb,2, Saemundur A. Halldórssonc,2, Andrea Mundl-Petermeierd, Michael Bizimise, Mark D. Kurzf, Allison A. Pricea, Sunna Harðardóttirc, Lori N. Willhitea,g, Kresten Breddamh, Thorsten W. Beckeri,j, and Rebecca A. Fischerk aDepartment of Earth Science, University of California, Santa Barbara, CA 93106-9630; bLaboratoire de Géologie de Lyon, Ecole Normale Supérieure de Lyon, CNRS, and Université de Lyon, 69007 Lyon, France; cNordVulk, Institute of Earth Sciences, University of Iceland, 102 Reykjavík, Iceland; dDepartment of Lithospheric Research, University of Vienna, 1090 Vienna, Austria; eSchool of the Earth, Ocean and Environment, University of South Carolina, Columbia, SC 29208; fDepartment of Marine Chemistry, Woods Hole Oceanographic Institution, Woods Hole, MA 02543; gDepartment of Geology, University of Maryland, College Park, MD 20742; hRadiation Protection, Danish Health Authority, 2300 Copenhagen, Denmark; iInstitute for Geophysics, The Jackson School of Geosciences, The University of Texas at Austin, Austin, TX 78713; jDepartment of Geological Sciences, The Jackson School of Geosciences, The University of Texas at Austin, Austin, TX 78713; and kDepartment of Earth & Planetary Sciences, Harvard University, Cambridge, MA 02138 Edited by Albrecht W. Hofmann, Max Planck Institute for Chemistry, Mainz, Germany, and approved October 22, 2020 (received for review May 14, 2020) Rare high-3He/4He signatures in ocean island basalts (OIB) erupted Sr-Nd-Pb isotopic space, these four geochemical endmembers can at volcanic hotspots derive from deep-seated domains preserved in be used to define the apices of a tetrahedron (8) (Fig. -
C"""- Signature of Author, Joint Program in Oceanography Massachusetts Institute of Technology/ Woods Hole Oceanographic Institution
GLOBAL ISOTOPIC SIGNATURES OF OCEANIC ISLAND BASALTS by LYNN A. OSCHMANN A.B. BRYN MAWR COLLEGE (1989) SUBMITTED IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF MASTER OF SCIENCE IN OCEANOGRAPHY at the MASSACHUSETTS INSTITUTE OF TECHNOLOGY and the WOODS HOLE OCEANOGRAPHIC INSTITUTION August 1991 @Lynn A. Oschmann 1991 The author hereby grants to MIT, WHOI, and the U.S. Government permission to reproduce and distribute copies of this thesis in whole or in part. %/7_ ) C"""- Signature of Author, Joint Program in Oceanography Massachusetts Institute of Technology/ Woods Hole Oceanographic Institution Certified by - 1% Dr. Stanley R. Hart Senior Scientist, Woods Hole Oceanographic Institution Thesis Supervisor Accepted by Dr. G. Pat Lohman Chairman, Joint Committee for Geology and Geophysics, Massachusetts Institute of Technology/ Woods Hole Oceanographic Institution MVIr 2 GLOBAL ISOTOPIC SIGNATURES OF OCEANIC ISLAND BASALTS by LYNN A. OSCHMANN Submitted to the Department of Earth, Atmospheric and Planetary Sciences Massachusetts Institute of Technology and the Department of Geology and Geophysics Woods Hole Oceanographic Institution August 9, 1991 in partial fulfillment of the requirements for the degree of MASTER OF SCIENCE IN OCEANOGRAPHY ABSTRACT Sr, Nd and Pb isotopic analyses of 477 samples representing 30 islands or island groups, 3 seamounts or seamount chains, 2 oceanic ridges and 1 oceanic plateau [for a total of 36 geographic features] are compiled to form a comprehensive oceanic island basalt [OIB] data set. These samples are supplemented by 90 selected mid-ocean ridge basalt [MORB] samples to give adequate representation to MORB as an oceanic basalt end-member. This comprehensive data set is used to infer information about the Earth's mantle. -
Recycled Ancient Ghost Carbonate in the Pitcairn Mantle Plume
Recycled ancient ghost carbonate in the Pitcairn mantle plume Xiao-Jun Wanga, Li-Hui Chena,1, Albrecht W. Hofmannb,1, Takeshi Hanyuc, Hiroshi Kawabatad, Yuan Zhonga, Lie-Wen Xiee, Jin-Hua Shia, Takashi Miyazakic, Yuka Hiraharac,2, Toshiro Takahashic,3, Ryoko Sendac,4, Qing Changc, Bogdan S. Vaglarovc, and Jun-Ichi Kimurac aState Key Laboratory for Mineral Deposits Research, School of Earth Sciences and Engineering, Nanjing University, 210023 Nanjing, China; bAbteilung Klimageochemie, Max-Planck-Institut für Chemie, D-55128 Mainz, Germany; cDepartment of Solid Earth Geochemistry, Japan Agency for Marine-Earth Science and Technology, 237-0061 Yokosuka, Japan; dFaculty of Science and Technology, Kochi University, 780-8520 Kochi, Japan; and eState Key Laboratory of Lithospheric Evolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, 100029 Beijing, China Edited by Richard W. Carlson, Carnegie Institution for Science, Washington, DC, and approved July 17, 2018 (received for review November 9, 2017) The extreme Sr, Nd, Hf, and Pb isotopic compositions found in Pitcairn stable isotope tracer, magnesium, which undergoes strong iso- Island basalts have been labeled enriched mantle 1 (EM1), character- topic fractionation during precipitation of carbonate from izing them as one of the isotopic mantle end members. The EM1 seawater/pore fluids (12), producing distinctively low δ26Mg origin has been vigorously debated for over 25 years, with interpre- values in marine carbonates. Because of this, it appears to be an tations ranging from delaminated subcontinental lithosphere, to excellent tracer of a more specific recycled component than, for recycled lower continental crust, to recycled oceanic crust carrying example, oxygen isotopes. ancient pelagic sediments, all of which may potentially generate the There are many models for the creation of chemical hetero- requisite radiogenic isotopic composition. -
The Pitcairn Hotspot in the South Paci¢C: Distribution and Composition of Submarine Volcanic Sequences
Available online at www.sciencedirect.com R Journal of Volcanology and Geothermal Research 121 (2003) 219^245 www.elsevier.com/locate/jvolgeores The Pitcairn hotspot in the South Paci¢c: distribution and composition of submarine volcanic sequences R. Hekinian a;Ã, J.L. Chemine¤e b, J. Dubois b, P. Sto¡ers a, S. Scott c, C. Guivel d, D. Garbe-Scho«nberg a, C. Devey e, B. Bourdon b, K. Lackschewitz e, G. McMurtry f , E. Le Drezen g a Universita«t Kiel, Institut fu«r Geowissenschaften, OlshausentraMe 40, 24098 Kiel, Germany b Institut de Physique du Globe de Paris, 4 Place Jussieu, 75252 Paris, France c Geology Department, University of Toronto, Toronto, ON, Canada M5S 3B1 d Universite¤ de Nantes, Faculte¤ des Sciences, 2 Rue de la Houssinie're, 92208 Nantes, France e University of Bremen, Geowissenschaften, Postfach 340440, 28334 Bremen, Germany f University of Hawaii, Department of Oceanography, 1000 Pope Road, Honolulu, HI 96822, USA g IFREMER Centre de Brest, Ge¤oscience Marine, 29280 Plouzane¤, France Received 19 March 2002; accepted 30 August 2002 Abstract Multibeam bathymetry and bottom imaging (Simrad EM12D) studies on an area of about 9500 km2 were conducted over the Pitcairn hotspot near 25‡10PS, 129‡ 20PW. In addition, 15 dives with the Nautile submersible enabled us to obtain ground-true observations and to sample volcanic structures on the ancient ocean crust of the Farallon Plate at 3500^4300 m depths. More than 100 submarine volcanoes overprint the ancient crust and are divided according to their size into large ( s 2000 m in height), intermediate (500^2000 m high) and small ( 6 500 m high) edifices. -
Aula 4 – Tipos Crustais Tipos Crustais Continentais E Oceânicos
14/09/2020 Aula 4 – Tipos Crustais Introdução Crosta e Litosfera, Astenosfera Crosta Oceânica e Tipos crustais oceânicos Crosta Continental e Tipos crustais continentais Tipos crustais Continentais e Oceânicos A interação divergente é o berço fundamental da litosfera oceânica: não forma cadeias de montanhas, mas forma a cadeia desenhada pela crista meso- oceânica por mais de 60.000km lineares do interior dos oceanos. A interação convergente leva inicialmente à formação dos arcos vulcânicos e magmáticos (que é praticamente o berço da litosfera continental) e posteriormente à colisão (que é praticamente o fechamento do Ciclo de Wilson, o desparecimento da litosfera oceânica). 1 14/09/2020 Curva hipsométrica da terra A área de superfície total da terra (A) é de 510 × 106 km2. Mostra a elevação em função da área cumulativa: 29% da superfície terrestre encontra-se acima do nível do mar; os mais profundos oceanos e montanhas mais altas uma pequena fração da A. A > parte das regiões de plataforma continental coincide com margens passivas, constituídas por crosta continental estirada. Brito Neves, 1995. Tipos crustais circunstâncias geométrico-estruturais da face da Terra (continentais ou oceânicos); Característica: transitoriedade passar do Tempo Geológico e como forma de dissipar o calor do interior da Terra. Todo tipo crustal adveio de um outro ou de dois outros, e será transformado em outro ou outros com o tempo, toda esta dança expressando a perda de calor do interior para o exterior da Terra. Nenhum tipo crustal é eterno; mais "duráveis" (e.g. velhos Crátons de de "ultra-longa duração"); tipos de curta duração, muitas modificações e rápida evolução potencial (como as bacias de antearco). -
GMT Based Comparative Analysis and Geomorphological Mapping of the Kermadec and Tonga Trenches, Southwest Pacific Ocean Polina Lemenkova
GMT Based Comparative Analysis and Geomorphological Mapping of the Kermadec and Tonga Trenches, Southwest Pacific Ocean Polina Lemenkova To cite this version: Polina Lemenkova. GMT Based Comparative Analysis and Geomorphological Mapping of the Ker- madec and Tonga Trenches, Southwest Pacific Ocean. Geographia Technica, Cluj University Press, 2019, 14 (2), pp.39-48. 10.21163/GT_2019.142.04. hal-02333464 HAL Id: hal-02333464 https://hal.archives-ouvertes.fr/hal-02333464 Submitted on 16 Dec 2019 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Distributed under a Creative Commons Attribution| 4.0 International License Geographia Technica, Vol. 14, Issue 2, 2019, pp 39 to 48 GMT BASED COMPARATIVE ANALYSIS AND GEOMORPHOLOGICAL MAPPING OF THE KERMADEC AND TONGA TRENCHES, SOUTHWEST PACIFIC OCEAN Polina LEMENKOVA1 DOI: 10.21163/GT_2019.142.04 ABSTRACT: Current study is focused on the GMT based modelling of the two hadal trenches located in southwest Pacific Ocean, eastwards from Australia: Tonga and Kermadec. Due to its inaccessible location, the seafloor of the deep-sea trench can only be visualized using remote sensing tools and advanced algorithms of data analysis. The importance of the developing and technical improving of the innovative methods in cartographic data processing is indisputable. -
Petit Spot Rejuvenated Volcanism Superimposed on Plume-Derived
RESEARCH ARTICLE “Petit Spot” Rejuvenated Volcanism Superimposed 10.1029/2018GC007985 on Plume‐Derived Samoan Shield Volcanoes: Key Points: ‐ • Within the 645‐m Tutuila drill core Evidence From a 645 m Drill Core From we find isotopically heterogeneous lavas as well as several abrupt Tutuila Island, American Samoa temporal and geochemical Andrew A. Reinhard1 , Matthew G. Jackson1 , Jerzy Blusztajn2 , Anthony A. P. Koppers3 , boundaries 1 4 • The proximity of Samoan volcanoes Alexander R. Simms , and Jasper G. Konter to the Tonga Trench and 1 2 geochronology are consistent with a Department of Earth Science, University of California, Santa Barbara, CA, USA, Woods Hole Oceanographic Institution, tectonic influence on rejuvenated Woods Hole, MA, USA, 3College of Earth, Ocean, and Atmospheric Sciences, Oregon State University, Corvallis, OR, USA, volcanism 4Department of Earth Sciences, University of Hawai'i at Mānoa, Honolulu, HI, USA • The tectonic setting and isotopic signatures of the Samoan rejuvenated lavas link them to “petit spots” outboard of the Japan Trench Abstract In 2015 a geothermal exploration well was drilled on the island of Tutuila, American Samoa. The sample suite from the drill core provides 645 m of volcanic stratigraphy from a Samoan volcano, Supporting Information: spanning 1.45 million years of volcanic history. In the Tutuila drill core, shield lavas with an EM2 (enriched • Supporting Information S1 mantle 2) signature are observed at depth, spanning 1.46 to 1.44 Ma. These are overlain by younger (1.35 to • Table S1 “ ” • Table S2 1.17 Ma) shield lavas with a primordial common (focus zone) component interlayered with lavas that • Table S3 sample a depleted mantle component. -
2. the D'entrecasteaux Zone—New Hebrides
Collot, J.-Y., Greene, H. G., Stokking, L. B., et al., 1992 Proceedings of the Ocean Drilling Program, Initial Reports, Vol. 134 2. THE D'ENTRECASTEAUX ZONE-NEW HEBRIDES ISLAND ARC COLLISION ZONE: AN OVERVIEW1 J.-Y. Collot2 and M. A. Fisher3 ABSTRACT The <TEntrecasteaux Zone, encompassing the North d'Entrecasteaux Ridge and the Bougainville Guyot, collide with the central New Hebrides Island Arc. The d'Entrecasteaux Zone trends slightly oblique to the 10-cm/yr relative direction of plate motion so that the ridge and the guyot scrape slowly (2.5 cm/yr) north, parallel to the trench. The North d'Entrecasteaux Ridge consists of Paleogene mid-ocean ridge basalt basement and Pliocene to Pleistocene sediment. The Bougainville Guyot is an andesitic, middle Eocene volcano capped with upper Oligocene to lower Miocene and Miocene to Pliocene lagoonal limestones. Geophysical and geologic data collected prior to Leg 134 indicate that the two collision zones differ in morphology and structure. The North d'Entrecasteaux Ridge extends, with a gentle dip, for at least 15 km eastward beneath the arc slope and has produced a broad (20-30 km), strongly uplifted area (possibly by 1500-2500 m) that culminates at the Wousi Bank. This tectonic pattern is further complicated by the sweeping of the ridge along the trench, which has produced a lobate structure formed by strike-slip and thrust faults as well as massive slumps north of the ridge. South of the ridge, the sweeping has formed large normal faults and slump scars that suggest collapse of arc-slope rocks left in the wake of the ridge. -
SUBDUCTION ZONES • Most Subduction Zones Are Found in the Pacific Ocean
ANOTHER MEXICAN EARTHQUAKE! Magnitude 7.1, Tuesday Sept. 19, 2017 Why is there no oceanic crust older than 200 million years? SUBDUCTION • If new oceanic crust is being continuously created along the earth’s spreading ridge system, then we must find some way to re-cycle it back into the mantle. [WHY? –otherwise the earth would be expanding!!!!] • Old oceanic crust (>200 million years) is returned to the mantle at the deep ocean trenches. • These are known as SUBDUCTION ZONES • Most subduction zones are found in the Pacific Ocean. This means that the Pacific Ocean is shrinking and the Atlantic Ocean is expanding. Convection in the mantle Lithosphere Recap Lithosphere (or plate) – is rigid and is composed of crust and upper mantle. Thickness varies from 10-150 km. Asthenosphere – is soft, plastic and convecting. Melting of the asthenosphere produces volcanic rocks at ocean ridges. SUBDUCTION Cross-section through the southern Pacific Ocean New oceanic crust and lithosphere are created at the East Pacific Rise Old oceanic crust and lithosphere are subducted at deep ocean trenches (Tonga trench and Chile trench). Kamchatka Pacific Ocean trench Aleutian trench Japan trench Costa Rica trench Marianas trench Tonga trench Chile trench East Pacific Rise Notice that the trenches are often curved with the convex side facing the direction of subduction. This is because the earth is spherical Consequently by observing the curvature of the trench we can easily determine which side is being subducted Details of a subduction zone • Slab of lithosphere descends back into the mantle at a deep ocean trench. • Earthquakes trace the descent of the slab into the mantle (Benioff Zone). -
Absolute Plate Motions Constrained By
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 114, B10405, doi:10.1029/2009JB006416, 2009 Click Here for Full Article Absolute plate motions constrained by shear wave splitting orientations with implications for hot spot motions and mantle flow Corne´ Kreemer1 Received 27 February 2009; revised 11 June 2009; accepted 14 July 2009; published 22 October 2009. [1] Here, I present a new absolute plate motion model of the Earth’s surface, determined from the alignment of present-day surface motions with 474 published shear wave (i.e., SKS) splitting orientations. When limited to oceanic islands and cratons, splitting orientations are assumed to reflect anisotropy in the asthenosphere caused by the differential motion between lithosphere and mesosphere. The best fit model predicts a 0.2065°/Ma counterclockwise net rotation of the lithosphere as a whole, which revolves around a pole at 57.6°S and 63.2°E. This net rotation is particularly well constrained by data on cratons and/or in the Indo-Atlantic region. The average data misfit is 19° and 24° for oceanic and cratonic areas, respectively, but the normalized root-mean-square misfits are about equal at 5.4 and 5.2. Predicted plate motions are very consistent with recent hot spot track azimuths (<8° on many plates), except for the slowest moving plates (Antarctica, Africa, and Eurasia). The difference in hot spot propagation vectors and plate velocities describes the motion of hot spots (i.e., their underlying plumes). For most hot spots that move significantly, the motions are considerably smaller than and antiparallel to the absolute plate velocity. Only when the origin depth of the plume is considered can the hot spot motions be explained in terms of mantle flow.