Earth Science Chapter 10
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Timeline of Natural History
Timeline of natural history This timeline of natural history summarizes significant geological and Life timeline Ice Ages biological events from the formation of the 0 — Primates Quater nary Flowers ←Earliest apes Earth to the arrival of modern humans. P Birds h Mammals – Plants Dinosaurs Times are listed in millions of years, or Karo o a n ← Andean Tetrapoda megaanni (Ma). -50 0 — e Arthropods Molluscs r ←Cambrian explosion o ← Cryoge nian Ediacara biota – z ←Earliest animals o ←Earliest plants i Multicellular -1000 — c Contents life ←Sexual reproduction Dating of the Geologic record – P r The earliest Solar System -1500 — o t Precambrian Supereon – e r Eukaryotes Hadean Eon o -2000 — z o Archean Eon i Huron ian – c Eoarchean Era ←Oxygen crisis Paleoarchean Era -2500 — ←Atmospheric oxygen Mesoarchean Era – Photosynthesis Neoarchean Era Pong ola Proterozoic Eon -3000 — A r Paleoproterozoic Era c – h Siderian Period e a Rhyacian Period -3500 — n ←Earliest oxygen Orosirian Period Single-celled – life Statherian Period -4000 — ←Earliest life Mesoproterozoic Era H Calymmian Period a water – d e Ectasian Period a ←Earliest water Stenian Period -4500 — n ←Earth (−4540) (million years ago) Clickable Neoproterozoic Era ( Tonian Period Cryogenian Period Ediacaran Period Phanerozoic Eon Paleozoic Era Cambrian Period Ordovician Period Silurian Period Devonian Period Carboniferous Period Permian Period Mesozoic Era Triassic Period Jurassic Period Cretaceous Period Cenozoic Era Paleogene Period Neogene Period Quaternary Period Etymology of period names References See also External links Dating of the Geologic record The Geologic record is the strata (layers) of rock in the planet's crust and the science of geology is much concerned with the age and origin of all rocks to determine the history and formation of Earth and to understand the forces that have acted upon it. -
Playing Jigsaw with Large Igneous Provinces a Plate Tectonic
PUBLICATIONS Geochemistry, Geophysics, Geosystems RESEARCH ARTICLE Playing jigsaw with Large Igneous Provinces—A plate tectonic 10.1002/2015GC006036 reconstruction of Ontong Java Nui, West Pacific Key Points: Katharina Hochmuth1, Karsten Gohl1, and Gabriele Uenzelmann-Neben1 New plate kinematic reconstruction of the western Pacific during the 1Alfred-Wegener-Institut Helmholtz-Zentrum fur€ Polar- und Meeresforschung, Bremerhaven, Germany Cretaceous Detailed breakup scenario of the ‘‘Super’’-Large Igneous Province Abstract The three largest Large Igneous Provinces (LIP) of the western Pacific—Ontong Java, Manihiki, Ontong Java Nui Ontong Java Nui ‘‘Super’’-Large and Hikurangi Plateaus—were emplaced during the Cretaceous Normal Superchron and show strong simi- Igneous Province as result of larities in their geochemistry and petrology. The plate tectonic relationship between those LIPs, herein plume-ridge interaction referred to as Ontong Java Nui, is uncertain, but a joined emplacement was proposed by Taylor (2006). Since this hypothesis is still highly debated and struggles to explain features such as the strong differences Correspondence to: in crustal thickness between the different plateaus, we revisited the joined emplacement of Ontong Java K. Hochmuth, [email protected] Nui in light of new data from the Manihiki Plateau. By evaluating seismic refraction/wide-angle reflection data along with seismic reflection records of the margins of the proposed ‘‘Super’’-LIP, a detailed scenario Citation: for the emplacement and the initial phase of breakup has been developed. The LIP is a result of an interac- Hochmuth, K., K. Gohl, and tion of the arriving plume head with the Phoenix-Pacific spreading ridge in the Early Cretaceous. The G. -
Assembly, Configuration, and Break-Up History of Rodinia
Author's personal copy Available online at www.sciencedirect.com Precambrian Research 160 (2008) 179–210 Assembly, configuration, and break-up history of Rodinia: A synthesis Z.X. Li a,g,∗, S.V. Bogdanova b, A.S. Collins c, A. Davidson d, B. De Waele a, R.E. Ernst e,f, I.C.W. Fitzsimons g, R.A. Fuck h, D.P. Gladkochub i, J. Jacobs j, K.E. Karlstrom k, S. Lu l, L.M. Natapov m, V. Pease n, S.A. Pisarevsky a, K. Thrane o, V. Vernikovsky p a Tectonics Special Research Centre, School of Earth and Geographical Sciences, The University of Western Australia, Crawley, WA 6009, Australia b Department of Geology, Lund University, Solvegatan 12, 223 62 Lund, Sweden c Continental Evolution Research Group, School of Earth and Environmental Sciences, University of Adelaide, Adelaide, SA 5005, Australia d Geological Survey of Canada (retired), 601 Booth Street, Ottawa, Canada K1A 0E8 e Ernst Geosciences, 43 Margrave Avenue, Ottawa, Canada K1T 3Y2 f Department of Earth Sciences, Carleton U., Ottawa, Canada K1S 5B6 g Tectonics Special Research Centre, Department of Applied Geology, Curtin University of Technology, GPO Box U1987, Perth, WA 6845, Australia h Universidade de Bras´ılia, 70910-000 Bras´ılia, Brazil i Institute of the Earth’s Crust SB RAS, Lermontova Street, 128, 664033 Irkutsk, Russia j Department of Earth Science, University of Bergen, Allegaten 41, N-5007 Bergen, Norway k Department of Earth and Planetary Sciences, Northrop Hall University of New Mexico, Albuquerque, NM 87131, USA l Tianjin Institute of Geology and Mineral Resources, CGS, No. -
Subsidence and Growth of Pacific Cretaceous Plateaus
ELSEVIER Earth and Planetary Science Letters 161 (1998) 85±100 Subsidence and growth of Paci®c Cretaceous plateaus Garrett Ito a,Ł, Peter D. Clift b a School of Ocean and Earth Science and Technology, POST 713, University of Hawaii at Manoa, Honolulu, HI 96822, USA b Department of Geology and Geophysics, Woods Hole Oceanographic Institution, Woods Hole, MA 02543, USA Received 10 November 1997; revised version received 11 May 1998; accepted 4 June 1998 Abstract The Ontong Java, Manihiki, and Shatsky oceanic plateaus are among the Earth's largest igneous provinces and are commonly believed to have erupted rapidly during the surfacing of giant heads of initiating mantle plumes. We investigate this hypothesis by using sediment descriptions of Deep Sea Drilling Project (DSDP) and Ocean Drilling Program (ODP) drill cores to constrain plateau subsidence histories which re¯ect mantle thermal and crustal accretionary processes. We ®nd that total plateau subsidence is comparable to that expected of normal sea¯oor but less than predictions of thermal models of hotspot-affected lithosphere. If crustal emplacement was rapid, then uncertainties in paleo-water depths allow for the anomalous subsidence predicted for plumes with only moderate temperature anomalies and volumes, comparable to the sources of modern-day hotspots such as Hawaii and Iceland. Rapid emplacement over a plume head of high temperature and volume, however, is dif®cult to reconcile with the subsidence reconstructions. An alternative possibility that reconciles low subsidence over a high-temperature, high-volume plume source is a scenario in which plateau subsidence is the superposition of (1) subsidence due to the cooling of the plume source, and (2) uplift due to prolonged crustal growth in the form of magmatic underplating. -
Amplify Science Earth's Changing Climate
Lawrence Hall of Science has new instructional materials that address the Next Generation Science Standards! Check out these Middle School Units… As just one example, compare Middle School units from three different Hall programs. See for yourself how each program goes about addressing the Middle School NGSS Standards related to Human Impacts and Climate Change, and choose the approach that best meets the needs of your school district. MS NGSS Performance Expectations: Human Impacts and Climate Change • MS-ESS3-2. Analyze and interpret data on natural hazards to forecast future catastrophic events and inform the development of technologies to mitigate their effects. • MS-ESS3-3. Apply scientific principles to design a method for monitoring and minimizing a human impact on the Environment. • MS-ESS3-4. Construct an argument supported by evidence for how increases in human population and per-capita consumption of natural resources impact Earth’s systems. • MS-ESS3-5. Ask questions to clarify evidence of the factors that have caused the rise in global temperatures over the past century. Sample Units from Three Different Hall Programs • Amplify Science—Earth’s Changing Climate: Vanishing Ice Earth’s Changing Climate Engineering Internship • FOSS—Weather and Water • Ocean Sciences Sequence—The Ocean-Atmosphere Connection and Climate Change ©The Regents of the University of California ©The Regents of the University of California Description of two Middle School units from Amplify Science Earth’s Changing Climate: Vanishing Ice and Earth’s Changing Climate Engineering Internship Grade 6-8 Units — requiring at least 19 and 10 45-minute class sessions respectively (two of 27 Middle School Amplify Science units) The Problem: Why is the ice on Earth’s surface melting? Students’ Role: In the role of student climatologists, students investigate what is causing ice on Earth’s surface to melt in order to help the fictional World Climate Institute educate the public about the processes involved. -
Present-Day Crustal Motion in the Solomon Islands from GPS
GEOPHYSICAL RESEARCH LETTERS, VOL. 25, NO. 19, PAGES 3627-3630, OCTOBER 1, 1998 Present-day crustal motion in the Solomon Islands from GPS observations Paul Tregoning Research School of Earth Sciences, The Australian National University, Canberra, Australia Francis Tan, John Gilliland School of Geoinformatics, Planning and Building, The University of South Australia, Adelaide, Australia Herbert McQueen and Kurt Lambeck Research School of Earth Sciences, The Australian National University, Canberra, Australia Abstract. Site velocities in the Solomon Islands from Ontong Java Plateau (OJP) collided with the Solomon Arc, Global Positioning System measurements spanning two years probably ∼20 to 25 Ma [e.g. Coleman and Kroenke, 1981; provide direct evidence of active deformation between the Kroenke, 1984; Yan and Kroenke, 1993]. Since that time it Pacific Plate and the Solomon Arc block. Convergence is is thought that subduction of the Pacific Plate ceased dur- occurring at the San Cristobal Trench at a rate of ∼524 ing the Early Miocene but it may have recommenced in the mm/yr, with no apparent local deformation occurring in the Mid-Miocene. About 10 Ma polarity reversal occurred and Australian Plate at a distance of ∼100 km from the trench. the Australian Plate began subducting to the northeast at The islands of Guadalcanal and Makira are in a first ap- the New Britain and San Cristobal Trenches, thus creating proximation moving with the Pacific Plate although there is the southern islands of the New Georgia group, Bougainville evidence of small but significant decoupling from the Pacific and Buka Island [Vedder and Bruns, 1989]. Active shallow Plate of 14-23 mm/yr in a direction of 75-85◦. -
Proto-Adamastor Ocean Crust (920 Ma) Described in Brasiliano Orogen from Coetaneous Zircon and Tourmaline
Geoscience Frontiers xxx (xxxx) xxx HOSTED BY Contents lists available at ScienceDirect China University of Geosciences (Beijing) Geoscience Frontiers journal homepage: www.elsevier.com/locate/gsf Research Paper Proto-Adamastor ocean crust (920 Ma) described in Brasiliano Orogen from coetaneous zircon and tourmaline Léo A. Hartmann a,*, Mariana Werle a, Cassiana R.L. Michelin a, Cristiano Lana b, Gláucia N. Queiroga b, Marco P. Castro b, Karine R. Arena a a Instituto de Geociências, Universidade Federal do Rio Grande do Sul, Avenida Bento Gonçalves, 9500, 91501-970, Porto Alegre, Rio Grande do Sul, Brazil b Departamento de Geologia, Escola de Minas, Universidade Federal de Ouro Preto, Morro do Cruzeiro, 35400-000, Ouro Preto, Minas Gerais, Brazil article info abstract Article history: Proto-Adamastor ocean bathed Rodinia and successor continental fragments from 1.0e0.9 Ga up to Received 25 March 2018 0.75 Ga, and evolved into world Adamastor Ocean at 0.75e0.60 Ga. Mesoproterozoic oceanic crust is Received in revised form poorly preserved on continents, only indirect evidence registered in Brasiliano Orogen. We report first 27 June 2018 evidence of ophiolite originated in proto-Adamastor. We use multi-technique U-Pb-Hf zircon and d11B Accepted 18 September 2018 tourmaline isotopic and elemental compositions. The host tourmalinite is enclosed in metaserpentinite, Available online xxx ¼þ ¼ Handling Editor: R. Damian Nance both belonging to the Bossoroca ophiolite. Zircon is 920 Ma-old, 3 Hf(920 Ma) 12, HfTDM 1.0 Ga and has ‘oceanic’ composition (e.g., U/Yb < 0.1). Tourmaline is dravite with d11B ¼þ1.8& (Tur 1), 0& (Tur 2), À & Keywords: 8.5 (Tur 3). -
Planets of the Solar System
Chapter Planets of the 27 Solar System Chapter OutlineOutline 1 ● Formation of the Solar System The Nebular Hypothesis Formation of the Planets Formation of Solid Earth Formation of Earth’s Atmosphere Formation of Earth’s Oceans 2 ● Models of the Solar System Early Models Kepler’s Laws Newton’s Explanation of Kepler’s Laws 3 ● The Inner Planets Mercury Venus Earth Mars 4 ● The Outer Planets Gas Giants Jupiter Saturn Uranus Neptune Objects Beyond Neptune Why It Matters Exoplanets UnderstandingU d t di theth formationf ti and the characteristics of our solar system and its planets can help scientists plan missions to study planets and solar systems around other stars in the universe. 746 Chapter 27 hhq10sena_psscho.inddq10sena_psscho.indd 774646 PDF 88/15/08/15/08 88:43:46:43:46 AAMM Inquiry Lab Planetary Distances 20 min Turn to Appendix E and find the table entitled Question to Get You Started “Solar System Data.” Use the data from the How would the distance of a planet from the sun “semimajor axis” row of planetary distances to affect the time it takes for the planet to complete devise an appropriate scale to model the distances one orbit? between planets. Then find an indoor or outdoor space that will accommodate the farthest distance. Mark some index cards with the name of each planet, use a measuring tape to measure the distances according to your scale, and place each index card at its correct location. 747 hhq10sena_psscho.inddq10sena_psscho.indd 774747 22/26/09/26/09 111:42:301:42:30 AAMM These reading tools will help you learn the material in this chapter. -
I. Convergent Plate Boundaries (Destructive Margins) (Colliding Plates)
I. Convergent plate boundaries (destructive margins) (colliding plates) 1. Plates collide, an ocean trench forms, lithosphere is subducted into the mantle 2. Types of convergence—three general classes, created by two types of plates —denser oceanic plate subsides into mantle SUBDUCTION --oceanic trench present where this occurs -- Plate descends angle average 45o a. Oceanic-continental convergence 1. Denser oceanic slab sinks into the asthenosphere—continental plate floats 2. Pockets of magma develop and rise—due to water added to lower part of overriding crust—100-150 km depth 3. Continental volcanic arcs form a. e.g., Andes Low angle, strong coupling, strong earthquakes i. Nazca plate ii. Seaward migration of Peru-Chile trench b. e.g., Cascades c. e.g., Sierra Nevada system example of previous subduction b. Oceanic-oceanic convergence 1. Two oceanic slabs converge HDEW animation Motion at Plate Boundaries a. one descends beneath the other b. the older, colder one 2. Often forms volcanoes on the ocean floor 3. Volcanic island arcs forms as volcanoes emerge from the sea 200-300 km from subduction trench TimeLife page 117 Philippine Arc a. e.g., Aleutian islands b. e.g., Mariana islands c. e.g., Tonga islands all three are young volcanic arcs, 20 km thick crust Japan more complex and thicker crust 20-35 km thick c. Continental-continental convergence— all oceaninc crust is destroyed at convergence, and continental crust remains 1. continental crust does not subside—too buoyant 2. two continents collide—become ‘sutured’ together 3. Can produce new mountain ranges such as the Himalayas II. Transform fault boundaries 1. -
Plate Tectonics Says That Earth’S Plates Move Because of Convection Currents in the Mantle
Bellringer Which ocean is getting smaller and which ocean is getting bigger due to subduction and sea floor spreading? Plate Tectonic Theory Notes How Plates Move • Earth’s crust is broken into many jagged pieces. The surface is like the shell of a hard-boiled egg that has been rolled. The pieces of Earth’s crust are called plates. Plates carry continents, oceans floors, or both. How Plates Move • The theory of plate tectonics says that Earth’s plates move because of convection currents in the mantle. Currents in the mantle carry plates on Earth’s surface, like currents in water carry boats on a river, or Cheerios in milk. How Plates Move • Plates can meet in three different ways. Plates may pull apart, push together, or slide past each other. Wherever plates meet, you usually get volcanoes, mountain ranges, or ocean trenches. Plate Boundaries • A plate boundary is where two plates meet. Faults form along plate boundaries. A fault is a break in Earth’s crust where blocks of rock have slipped past each other. Plate Boundaries • Where two plates move apart, the boundary is called a divergent boundary. • A divergent boundary between two oceanic plates will result in a mid-ocean ridge AND rift valley. (SEE: Sea-Floor Spreading) • A divergent boundary between two continental plates will result in only a rift valley. This is currently happening at the Great Rift Valley in east Africa. Eventually, the Indian Ocean will pour into the lowered valley and a new ocean will form. Plate Boundaries • Where two plates push together, the boundary is called a convergent boundary. -
Dolerites of Svalbard, North-West Barents Sea Shelf: Age, Tectonic Setting and Significance for Geotectonic Interpretation of Th
RESEARCH/REVIEW ARTICLE Dolerites of Svalbard, north-west Barents Sea Shelf: age, tectonic setting and significance for geotectonic interpretation of the High-Arctic Large Igneous Province Krzysztof Nejbert1, Krzysztof P. Krajewski2, Elz˙bieta Dubin´ ska1 & Zolta´ nPe´ cskay3 1 Institute of Geochemistry, Mineralogy and Petrology, University of Warsaw, Al. Z˙ wirki i Wigury 93, PL-02089 Warsaw, Poland 2 Institute of Geological Sciences, Polish Academy of Sciences, Research Centre in Warsaw, ul. Twarda 51/55, PL-00818 Warsaw, Poland 3 Institute of Nuclear Research, Hungarian Academy of Sciences, Bem te´ r 18/c, HU-4026 Debrecen, Hungary Keywords Abstract Dolerite; geochemistry; petrogenesis; KÁAr whole rock ages; Svalbard; Cretaceous. The dolerites of Svalbard are mineralogically and geochemically homogeneous with geochemical features typical of continental within-plate tholeiites. Their Correspondence geochemistry is similar to tholeiites belonging to a bimodal suite defined as the Krzysztof P. Krajewski, Institute of Geologi- High-Arctic Large Igneous Province (HALIP). KÁAr dating of numerous cal Sciences, Polish Academy of Sciences, dolerites sampled from many locations across Svalbard define a narrow time Research Centre in Warsaw, ul. Twarda 51/ span of this magmatism from 125.593.6 to 78.392.6 Mya. Discrete peaks of 55, PL-00818 Warsaw, Poland. E-mail: [email protected] intensive activity occurred at 115.3, 100.8, 91.3 and 78.5 Mya corresponding to (1) breakup of the continental crust and formation of an initial rift as a result of mantle plume activity, located in the southern part of the Alpha Ridge; (2) magmatic activity related to spreading along the Alpha Ridge that led to the development of the initial oceanic crust and (3) continuation of spreading along the Alpha Ridge and termination of magmatic activity related to HALIP (last two peaks at 91.3 and 78.5 Mya). -
General Guide to the Science and Cosmos Museum
General guide to the Science and Cosmos Museum 1 Background: “Tenerife monts” and “Pico” near of Plato crater in the Moon PLANTA TERRAZA Terrace Floor 5 i 2 1 4 6 3 ASCENSOR 4 RELOJ DE SOL ECUATORIAL Elevator Analemmatic sundial i INFORMACIÓN 5 BUSTO PARLANTE Information “AGUSTÍN DE BETANCOURT” Agustín de Betancourt 1 PLAZA “AGUSTÍN DE talking bust BETANCOURT” Agustín de Betancourt 6 ZONA WI-FI Square Wi-Fi zone 2 ANTENA DE RADIOASTRONOMÍA Radioastronomy antenna 3 TELESCOPIO Telescope PLANTA BAJA Ground Floor WC 10 9 8 11 7 1 6 5 4 12 2 3 ASCENSOR Cosmos Lab - Creative Elevator Laboratory 1 EXPOSICIÓN 7 PLANETARIO Exhibition Planetarium 2 TALLER DE DIDÁCTICA 8 SALIDA DE EMERGENCIA Didactic Workshop Emergency exit 3 EFECTOS ÓPTICOS 9 MICROCOSMOS Optical illusions 10 SALÓN DE ACTOS 4 SALA CROMA KEY Assembly hall Chroma Key room 11 EXPOSICIONES TEMPORALES 5 LABERINTO DE ESPEJOS Temporary exhibitions Mirror Labyrinth 12 ZONA DE DESCANSO 6 COSMOS LAB - LABORATORIO Rest zone CREATIVO CONTENIDOS Contents 7 LA TIERRA The Earth 23 EL SOL The Sun 33 EL UNIVERSO The Universe 45 CÓMO FUNCIONA How does it work 72 EL CUERPO HUMANO The human body 5 ¿POR QUÉ PIRÁMIDES? Why pyramids? 1 Sacred places have often been con- ceived of as elevated spaces that draw the believer closer to the divi- nity. For this reason, once architec- tural techniques became sufficiently refined, mosques or cathedrals rai- sed their vaults, minarets, towers and spires to the sky. However, for thousands of years, the formula fa- voured by almost every culture was the pyramid.