Drilling the Crust at Mid-Ocean Ridges
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Seamount Abundances and Abyssal Hill Morphology on the Eastern
GEOPHYSICALRESEARCH LETTERS, VOL. 24, NO. 15,PAGES 1955-1958, AUGUST 1, 1997 Seamountabundances and abyssalhill morphology on the eastern flank of the East Pacific Rise at 14øS IngoGrevemeyer, 12Vincent Renard, 3Claudia Jennrich, • and Wilfried Weigel I Abstract. Bathymetricdata from a Hydrosweepmultibeam hills. Abyssalhills in the PacificOcean form. primarily sonarsurvey of a 720 km longtectonic corridor on theeast througha complexcombination of volcanicconstructional flank of the southernEPR at 14ø14'S coveredabout 25,000 processesand faulting that occur at or nearthe ridgeaxis km2 of zero-ageto 8.5 m.y. old crust(magnetic anomaly [e.g., Golf, 1991; MacdonaMet al., 1996]. Stochastic 4A). In this corridorwe documenta strongcorrelation of analysisof abyssalhills have shownthat ridge flank robustalong flowline changes in abyssalhill morphologyroughness increases with decreasing spreading rate [Menard, and seamountsize distributionwith spreadingrate changes 1967;Malinverno, 199l; Goff, 199l]. Nevertheless,seafloor deducedfrom our magneticdata. Indeed, we find thatboth roughnessvalues show a largevariation along a single rmsheight of abyssalhills andabundance and height of spreadingsegment [Golf, 1991; Goffet al., 1993],suggesting seamountsincrease significantly as spreadingrate changes that spreadingrate cannotbe the solefactor governing from ~ 75 mm/yrto over 85 mm/yr(half rate). Moreover, variationsin abyssalhill morphology. we identified 46 seamountstaller than !.00 m. Previous From November 8 to December 30, 1995 the R/V Sonne studieson the southernEPR reporteda larger densityof carriedout the EXCO-cruise,a geophysicalsurvey on zero- seamounts,organized primarily in chains.Our investigation, age to about8.5 m.y. old seafloor created at the"superfast" however, revealed seamountsnot associatedwith major spreading(full rate >140 mm/yr) East Pacific Rise south of chains,leading us to theconclusion that different forms of the Garrettfracture zone [Weigelet al., 1996]. -
Transform Faults Represent One of the Three
8 Transform faults ransform faults represent one of the three Because of the drift of the newly formed oceanic types of plate boundaries. A peculiar aspect crust away from ridge segments, a relative move- T of their nature is that they are abruptly trans- ment along the faults is induced that corresponds formed into another kind of plate boundary at their to the spreading velocity on both sides of the termination (Wilson, 1965). Plates glide along the ridge. Th e sense of displacement is contrary to fault and move past each other without destruc- the apparent displacement of the ridge segments tion of or creation of new crust. Although crust is (Fig. 8.1b). In the example shown, the transform neither created or destroyed, the transform margin fault is a right-lateral strike-slip fault; if an observer is commonly marked by topographic features like straddles the fault, the right-hand side of the fault scarps, trenches or ridges. moves towards the observer, regardless of which Transform faults occur as several diff erent geo- way is faced. Transform faults end abruptly in a metries; they can connect two segments of growing point, the transformation point, where the strike- plate boundaries (R-R transform fault), one growing slip movement is transformed into a diverging or and one subducting plate boundary (R-T transform converging movement. Th is property gives this fault) or two subducting plate boundaries (T-T fault its name. In the example of the R-R transform transform fault); R stands for mid-ocean ridge, T for fault, the movement at both ends of the fault is deep sea trench ( subduction zone). -
And Post-Collision Calc-Alkaline Magmatism in the Qinling Orogenic Belt, Central China, As Documented by Zircon Ages on Granitoid Rocks
Journal of the Geological Societv. London, Vol. 153, 1996, pp. 409-417. Palaeozoic pre- and post-collision calc-alkaline magmatism in the Qinling orogenic belt, central China, as documented by zircon ages on granitoid rocks F. XUE'.*,',A. KRONER', T. REISCHMANN' & F. LERCH' 'Institut fiir Geowissenschaften, Universitat Mainz, 55099 Mainz, Germany 'Department of Geology, Northwest University, 710069 Xi'an, China .'Present address: Department of Geophysical Sciences, The University of Chicago, 5734 South Ellis Avenue, Chicago, IL 60637, USA Abstract: Basedon large-scale reconnaissance mapping, we identifiedtwo calc-alkaline plutonic assemblagesfrom the northern Qinling orogenic belt.central China. The older assemblage of intrusions. closely associated and deformed coevally with their host volcanic arc sequences, seems to represent the fractionation product of basaltic arc magma. It therefore predates the collision of the North China Block with the Central Qinling island-arc system that developed in a SW Pacific-type oceanic domain south of the North China Block. Single-zircon zo7Pb/2'"Pb evaporation dating yielded early to middle Ordovician ages for this assemblage. with a relatively small range from 487.2 f 1.1 to 470.2 f 1.3 Ma. Intrusions of the younger assemblage are largely undeformed and truncate structures shown in rocks of theolder assemblage. They are interpreted as post-collisional calc-alkaline granitoids.Single zircon dating provided an age of 401.8 f 0.8 Mafor the younger assemblage. consistentwith earlier work that defines an age range from c. 420 to 395Ma. Our datafavour a tectonicmodel involving formation and amalgamation of islandarc and microcontinent terranes between ca. 490 and 470 Ma ago to create the Central Qinling Zone which subsequently collided with theNorth China Block prior to c. -
Sixteenth Meeting of the GEBCO Sub-Committee on Undersea Feature Names (SCUFN) Met at the International Hydrographic Bureau, Monaco, Under the Chairmanship of Dr
Distribution : limited IOC-IHO/GEBCO SCUFN-XV1/3 English only INTERGOVERNMENTAL INTERNATIONAL OCEANOGRAPHIC HYDROGRAPHIC COMMISSION (of UNESCO) ORGANIZATION International Hydrographic Bureau Monaco, 10-12 April 2003 SUMMARY REPORT IOC-IHO/GEBCO SCUFN-XVI/3 Page 2 Page intentionally left blank IOC-IHO/GEBCO SCUFN-XVI/3 Page 1 Notes: A list of acronyms, used in this report, is in Annex 3. An alphabetical index of all undersea feature names appearing in this report is in Annex 6. 1. INTRODUCTION – APPROVAL OF AGENDA The sixteenth meeting of the GEBCO Sub-Committee on Undersea Feature Names (SCUFN) met at the International Hydrographic Bureau, Monaco, under the Chairmanship of Dr. Robert L. FISHER, Scripps Institution of Oceanography (SIO), USA. Attendees were welcomed by Capt. Hugo GORZIGLIA, IHB Director. He mentioned that the IHB had invited IHO Member States to make experts available to SCUFN and was pleased to see new faces at this meeting. The meeting welcomed Dr. Hans-Werner SCHENKE (AWI, Germany), Mr. Kunikazu NISHIZAWA (Japan Hydrographic Department), Mrs. Lisa A. TAYLOR (NGDC, USA), Captain Vadim SOBOLEV (HDNO, Russian Federation) and Mr Norman CHERKIS (USA) as new members of SCUFN. The list of participants is in Annex 1. The draft agenda was approved without changes (see Annex 2). Mr. Desmond P.D. SCOTT kindly accepted to serve as Rapporteur for the meeting. 2. MATTERS REMAINING FROM PREVIOUS MEETINGS 2.1 From SCUFN-XIII (Dartmouth, Nova Scotia, Canada, June 1999) Ref: Doc. IOC-IHO/GEBCO SCUFN-XIII/3 2.1.1 Southwest Pacific region The following four features and names in this area, still pending, were reviewed: • Paragraph 3.1.5 - Proposed names for two seamounts located at (18°56’S – 169°27’W) and (19°31’S – 167°36’W) were still awaited from Dr Robin FALCONER, NIWA, New Zealand. -
Extrusive and Intrusive Magmatism Greatly Influence the Tectonic Mode of Earth-Like Planets
EPSC Abstracts Vol. 11, EPSC2017-945, 2017 European Planetary Science Congress 2017 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2017 Extrusive and Intrusive Magmatism Greatly Influence the Tectonic Mode of Earth-Like Planets D. Lourenco, P. J. Tackley, A. Rozel and M. Ballmer Institute of Geophysics, Department of Earth Sciences, ETH Zurich, Switzerland ([email protected] / Fax: +41 44 633 1065) Abstract reported in [3], we use thermo-chemical global mantle convection numerical simulations to Plate tectonics on Earth-like planets is typically systematically investigate the effect of plutonism, in modelling using a strongly temperature-dependent conjugation with eruptive volcanism. Results visco-plastic rheology. Previous analyses have reproduce the three common tectonic/convective generally focussed on purely thermal convection. regimes usually obtained in simulations using a However, we have shown that the influence of visco-plastic rheology: stagnant-lid (a one-plate compositional heterogeneity in the form of planet), episodic (where the lithosphere is unstable continental [1] or oceanic [2] crust can greatly and frequently overturns into the mantle), and influence plate tectonics by making it easier (i.e. it mobile-lid (similar to plate tectonics). At high occurs at a lower yield stress or friction coefficient). intrusion efficiencies, we observe and characterise a Here we present detailed results on this topic, in new additional regime called “plutonic-squishy lid”. particular focussing on the influence of intrusive vs. This regime is characterised by a set of strong plates extrusive magmatism on the tectonic mode. separated by warm and weak regions generated by plutonism. Eclogitic drippings and lithospheric delaminations often occur around these weak regions. -
Atlas of the Mediterranean Seamounts and Seamount-Like Structures
Atlas of the Mediterranean Seamounts and Seamount-like Structures ULISSE 44 N JANUA S.LUCIA SPINOLA OCCHIALI ARAGÓ CALYPSO HILLS 42 CIALDI FELIBRES HILLS 42 TIBERINO ETRUSCHI LA RENAIXENÇA HILLS ALBANO MONTURIOL S.FELIÙ SMS DAUNO VERCELLI SALVÁ BRUTUS SPARTACUS CASSINIS EBRO BARONIE-K MARUSSI SECCHI-ADRIANO FARFALLE ALBATROS-CICERONE CRESQUES BERTRAN SELLI VENUS MORROT DE LA CIUTADELLA GORTANI SELE MONTE DELLA RONDINE TACITO SÓLLER ALABE DE MARCHI SIRENE SARDINIA D’ANCONA FLAVIO GIOIA AMENDOLARA 40 SALLUSTIO 40 MAGNAGHI POSEIDONE ROSSANO APHRODITI VAVILOV TIBULLO DIAMANTE MORROT CORNAGLIA V.EMANUELE CARIATI DE SA DRAGONERA MAJOR ISSEL PALINURO-STRABO OVIDIO VILADESTERS CATULLO GLAVKI ORAZIO MARSILI-PLINIO GLABRO ENOTRIO MANSEL JOHNSTON STONY SPONGE QUIRRA ENEA TITO LIVIO VIRGILIO ALCIONE AUGUSTO SES OLIVES GARIBALDI-GLAUCO LAMETINO 1 BROUKER JAUME 1 CORNACYA LAMETINO 2 COLOM TRAIANO LUCREZIO STOKES XABIA-IBIZA VESPASIANO LITERI SINAYA VALLSECA SISIFO EMILE BAUDOT GIULIO CESARE-CAESAR DREPANO ENARETE CASONI FONTSERÈ ICHNUSA IRA NAVTILOS CABO DE LA NAO AUSIÀS MARCH ANCHISE BELL GUYOT POMPEO PROMETEO MARTORELL ACESTE-TIBERIO EOLO FORMENTERA SOLUNTO ALKYONI FERRER SCUSO SAN VITO LOS MARTINES ALÍ BEI FINALE DON JUAN RESGUI RIBA SENTINELLE (SKERKI) BALIKÇI EL38 PLANAZO BIDDLECOMBE SILVIA 38 PLIS PLAS KEITH SECO DE PALOS ESTAFETTE HECATE ADVENTURE TALBOT TETIDE 170 km ÁGUILAS GALATEA PANTELLERIA ANFITRITE EMPEDOCLE PINNE ANTEO 2 KHAYR-AL-DIN CIMOTOE ANTEO 3 ABUBACER FOERSTNER NAMELESS PNT. E MADREPORE ANTEO 1 AVENZOAR PNT. CB CHELLA CABO DE GATA ANGELINA ALFEO SABINAR PNT. SW AVEMPACE-ALGARROBO MAIMONIDES RIDGE BANNOCK KOLUMBO DJIBOUTI-HERRADURA POLLUX BILIM ADRA-AVERROES MAIMONIDES BIRSA PNT. SE HERRADURA-DJIBOUTI LINOSA III AL-MANSOUR A EL SEGOVIANO DJIBOUTI VILLE ALBORÁN LINOSA I LINOSA II HÉSPERIDES HÉRCULES EL IDRISSI YUSUF KARPAS CATIFAS-W. -
Modeling Seafloor Spreading Adapted from a Lesson Developed by San Lorenzo USD Teachers: Julie Ramirez, Veenu Soni, Marilyn Stewart, and Lawrence Yano (2012)
Teacher Instruction Sheet Modeling Seafloor Spreading Adapted from a lesson developed by San Lorenzo USD Teachers: Julie Ramirez, Veenu Soni, Marilyn Stewart, and Lawrence Yano (2012) Teacher Background The process of seafloor spreading created the seafloor of the oceans. For example, in the Atlantic Ocean, North America and South America moved away from Europe and Africa and the resulting crack was filled by mantle material, which cooled and formed new lithosphere. The process continues today. Molten mantle materials continually rise to fill the cracks formed as the plates move slowly apart from each other. This process creates an underwater mountain chain, known as a mid-ocean ridge, along the zone of newly forming seafloor. Molten rock erupts along a mid-ocean ridge, then cools and freezes to become solid rock. The direction of the magnetic field of the Earth at the time the rock cools is "frozen" in place. This happens because magnetic minerals in the molten rock are free to rotate so that they are aligned with the Earth's magnetic field. After the molten rock cools to a solid rock, these minerals can no longer rotate freely. At irregular intervals, averaging about 200-thousand years, the Earth's magnetic field reverses. The end of a compass needle that today points to the north will instead point to the south after the next reversal. The oceanic plates act as a giant tape recorder, preserving in their magnetic minerals the orientation of the magnetic field present at the time of their creation. Geologists call the current orientation "normal" and the opposite orientation "reversed." USGS Teacher Instruction Sheet In the figure above, two plates are moving apart. -
Ocean-Climate.Org
ocean-climate.org THE INTERACTIONS BETWEEN OCEAN AND CLIMATE 8 fact sheets WITH THE HELP OF: Authors: Corinne Bussi-Copin, Xavier Capet, Bertrand Delorme, Didier Gascuel, Clara Grillet, Michel Hignette, Hélène Lecornu, Nadine Le Bris and Fabrice Messal Coordination: Nicole Aussedat, Xavier Bougeard, Corinne Bussi-Copin, Louise Ras and Julien Voyé Infographics: Xavier Bougeard and Elsa Godet Graphic design: Elsa Godet CITATION OCEAN AND CLIMATE, 2016 – Fact sheets, Second Edition. First tome here: www.ocean-climate.org With the support of: ocean-climate.org HOW DOES THE OCEAN WORK? OCEAN CIRCULATION..............................………….....………................................……………….P.4 THE OCEAN, AN INDICATOR OF CLIMATE CHANGE...............................................…………….P.6 SEA LEVEL: 300 YEARS OF OBSERVATION.....................……….................................…………….P.8 The definition of words starred with an asterisk can be found in the OCP little dictionnary section, on the last page of this document. 3 ocean-climate.org (1/2) OCEAN CIRCULATION Ocean circulation is a key regulator of climate by storing and transporting heat, carbon, nutrients and freshwater all around the world . Complex and diverse mechanisms interact with one another to produce this circulation and define its properties. Ocean circulation can be conceptually divided into two Oceanic circulation is very sensitive to the global freshwater main components: a fast and energetic wind-driven flux. This flux can be described as the difference between surface circulation, and a slow and large density-driven [Evaporation + Sea Ice Formation], which enhances circulation which dominates the deep sea. salinity, and [Precipitation + Runoff + Ice melt], which decreases salinity. Global warming will undoubtedly lead Wind-driven circulation is by far the most dynamic. to more ice melting in the poles and thus larger additions Blowing wind produces currents at the surface of the of freshwaters in the ocean at high latitudes. -
Description of Map Units Northeast Asia Geodynamics Map
DESCRIPTION OF MAP UNITS NORTHEAST ASIA GEODYNAMICS MAP OVERLAP ASSEMBLAGES (Arranged alphabetically by map symbol) ad Adycha intermountain sedimentary basin (Miocene and Pliocene) (Yakutia) Basin forms a discontinuous chain along the foot of southwestern slope of Chersky Range in the Yana and Adycha Rivers basins. Contain Miocene and Pliocene sandstone, pebble gravel conglomerate, claystone, and minor boulder gravel conglomerate that range up to 400 m thick. REFERENCES: Grinenko and others, 1998. ag Agul (Rybinsk) molasse basin (Middle Devonian to Early Carboniferous) (Eastern Sayan) Consists of Middle Devonian through Early Carboniferous aerial and lacustrine sand-silt-mudstone, conglomerate, marl, and limestone with fauna and flora. Tuff, tuffite, and tuffaceous rock occur in Early Carboniferous sedimentary rocks. Ranges up to 2,000 m thick in southwestern margin of basin. Unconformably overlaps Early Devonian rocks of South Siberian volcanic-plutonic belt and Precambrian and early Paleozoic rocks of the Siberian Platform and surrounding fold belts. REFERENCES: Yanov, 1956; Graizer, Borovskaya, 1964. ags Argun sedimentary basin (Early Paleozoic) (Northeastern China) Occurs east of the Argun River in a discontinuously exposed, northeast-trending belt and consists of Cambrian and Ordovician marine, terrigenous detrital, and carbonate rocks. Cambrian units are composed of of feldspar- quartz sandstone, siltstone, shale and limestone and contain abundant Afaciacyathus sp., Bensocyathus sp., Robustocyathus yavorskii, Archaeocyathus yavorskii(Vologalin), Ethomophyllum hinganense Gu,o and other fossils. Ordovicain units consist of feldspar-quartz sandstone, siltstone, fine-grained sandstone and phylitic siltstone, and interlayered metamorphosed muddy siltstone and fine-grained sandstone with brachiopods, corals, and trilobites. Total thickness ranges up to 4,370 m. Basin unconformably overlies the Argunsky metamorphic terrane. -
Chapter 51. Biological Communities on Seamounts and Other Submarine Features Potentially Threatened by Disturbance
Chapter 51. Biological Communities on Seamounts and Other Submarine Features Potentially Threatened by Disturbance Contributors: J. Anthony Koslow, Peter Auster, Odd Aksel Bergstad, J. Murray Roberts, Alex Rogers, Michael Vecchione, Peter Harris, Jake Rice, Patricio Bernal (Co-Lead members) 1. Physical, chemical, and ecological characteristics 1.1 Seamounts Seamounts are predominantly submerged volcanoes, mostly extinct, rising hundreds to thousands of metres above the surrounding seafloor. Some also arise through tectonic uplift. The conventional geological definition includes only features greater than 1000 m in height, with the term “knoll” often used to refer to features 100 – 1000 m in height (Yesson et al., 2011). However, seamounts and knolls do not appear to differ much ecologically, and human activity, such as fishing, focuses on both. We therefore include here all such features with heights > 100 m. Only 6.5 per cent of the deep seafloor has been mapped, so the global number of seamounts must be estimated, usually from a combination of satellite altimetry and multibeam data as well as extrapolation based on size-frequency relationships of seamounts for smaller features. Estimates have varied widely as a result of differences in methodologies as well as changes in the resolution of data. Yesson et al. (2011) identified 33,452 seamount and guyot features > 1000 m in height and 138,412 knolls (100 – 1000 m), whereas Harris et al. (2014) identified 10,234 seamount and guyot features, based on a stricter definition that restricted seamounts to conical forms. Estimates of total abundance range to >100,000 seamounts and to 25 million for features > 100 m in height (Smith 1991; Wessel et al., 2010). -
Did the 1999 Earthquake Swarm on Gakkel Ridge Open a Volcanic Conduit? a Detailed Teleseismic Data Analysis Carsten Riedel, Vera Schlindwein
Did the 1999 earthquake swarm on Gakkel Ridge open a volcanic conduit? A detailed teleseismic data analysis Carsten Riedel, Vera Schlindwein To cite this version: Carsten Riedel, Vera Schlindwein. Did the 1999 earthquake swarm on Gakkel Ridge open a volcanic conduit? A detailed teleseismic data analysis. Journal of Seismology, Springer Verlag, 2009, 14 (3), pp.505-522. 10.1007/s10950-009-9179-6. hal-00537995 HAL Id: hal-00537995 https://hal.archives-ouvertes.fr/hal-00537995 Submitted on 20 Nov 2010 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. J Seismol (2010) 14:505–522 DOI 10.1007/s10950-009-9179-6 ORIGINAL ARTICLE Did the 1999 earthquake swarm on Gakkel Ridge open a volcanic conduit? A detailed teleseismic data analysis Carsten Riedel · Vera Schlindwein Received: 19 February 2009 / Accepted: 2 November 2009 / Published online: 20 November 2009 © Springer Science + Business Media B.V. 2009 Abstract In 1999, a seismic swarm of 237 tele- ascending toward the potential conduit during the seismically recorded events marked a submarine beginning of April 1999, indicating an opening of eruption along the Arctic Gakkel Ridge, later on the vent. -
Geophysical Signatures of Oceanic Core Complexes
Geophys. J. Int. (2009) 178, 593–613 doi: 10.1111/j.1365-246X.2009.04184.x REVIEW ARTICLE Geophysical signatures of oceanic core complexes Donna K. Blackman,1 J. Pablo Canales2 and Alistair Harding1 1Scripps Institution of Oceanography, UCSD La Jolla, CA, USA. E-mail: [email protected] 2Woods Hole Oceanographic Institution, Woods Hole, MA, USA Accepted 2009 March 16. Received 2009 February 15; in original form 2008 July 25 SUMMARY Oceanic core complexes (OCCs) provide access to intrusive and ultramafic sections of young lithosphere and their structure and evolution contain clues about how the balance between mag- matism and faulting controls the style of rifting that may dominate in a portion of a spreading centre for Myr timescales. Initial models of the development of OCCs depended strongly on insights available from continental core complexes and from seafloor mapping. While these frameworks have been useful in guiding a broader scope of studies and determining the extent GJI Geodesy, potential field and applied geophysics of OCC formation along slow spreading ridges, as we summarize herein, results from the past decade highlight the need to reassess the hypothesis that reduced magma supply is a driver of long-lived detachment faulting. The aim of this paper is to review the available geophysical constraints on OCC structure and to look at what aspects of current models are constrained or required by the data. We consider sonar data (morphology and backscatter), gravity, magnetics, borehole geophysics and seismic reflection. Additional emphasis is placed on seismic velocity results (refraction) since this is where deviations from normal crustal accretion should be most readily quantified.