IODP Expedition 305 Preliminary Report
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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. -
Enhanced Mantle Upwelling/Melting Caused Segment Propagation, Oceanic Across the Ridge Crest of the TAMMAR Segment
PUBLICATIONS Journal of Geophysical Research: Solid Earth RESEARCH ARTICLE Enhanced Mantle Upwelling/Melting Caused Segment 10.1002/2017JB014273 Propagation, Oceanic Core Complex Die Off, Key Points: and the Death of a Transform Fault: • Seismic data confirm ridge propagation induced by increased The Mid-Atlantic Ridge at 21.5°N melt supply due to increased fertility or upwelling of the asthenosphere A. Dannowski1 , J. P. Morgan2, I. Grevemeyer1 , and C. R. Ranero3,4 • Source of melt supply is migrating, ended a transform fault, and possibly 1GEOMAR/Helmholtz-Centre for Ocean Research Kiel, Kiel, Germany, 2Earth Sciences Department, Royal Holloway stopped OCC formation 3 • The growth direction of the enhanced University of London, London, UK, Barcelona Centre for Subsurface Imaging, Institut de Ciencias del Mar, Barcelona, Spain, 4 melt supply region is influenced by ICREA, Barcelona, Spain the distance to “colder” mantle zones Abstract Crustal structure provides the key to understand the interplay of magmatism and tectonism, while oceanic crust is constructed at Mid-Ocean Ridges (MORs). At slow spreading rates, magmatic Correspondence to: A. Dannowski, processes dominate central areas of MOR segments, whereas segment ends are highly tectonized. The [email protected] TAMMAR segment at the Mid-Atlantic Ridge (MAR) between 21°250N and 22°N is a magmatically active segment. At ~4.5 Ma this segment started to propagate south, causing the termination of the transform fault Citation: at 21°400N. This stopped long-lived detachment faulting and caused the migration of the ridge offset to the Dannowski, A., Morgan, J. P., south. Here a segment center with a high magmatic budget has replaced a transform fault region with Grevemeyer, I., & Ranero, C. -
Geomorphology of the Bushveld Complex
Cademo Lab. Xeo16xico de Laxe Coruña. 1997. Vol. 22, pp. 209-227 Geomorphology of the Bushveld Complex Geomorfología del Complejo de Bushveld LAGEAT,Y. This paper deals wich che differenc relacion becween scruccure and lichology in che geomorphology of che Bushveld Complexo The final resules demonscrace chac, even so differenc scale ofsize, widerfor che epirogenic-cecconic movements and smaller for che lichology, che cwo faccors need co be considered for a beccer underscanding ofche landscape evolucion ofche area. Key words: ulerabasic and basic rocks, Bushveld Complex, scruccural geomorphology, lichological differences. LAGEAT, Y. (Universicé Blaise Pascaland UPRES-A 6042 (CNRS). Clermont-Ferrand (France) 210 Lageat, Y. CAD. LAB. XEOL. LAXE 22 (997) INTRODUCTION subdued topography. So, being concerned with the relationships between scenery and In spiteofthestrong emphasisonclimatic structure, the study wil1 consider two topics in French geomorphology since the different but complementary topics: fifties, research dealing with structural differential erosion and regional evolution landforms developed in crystalline shields ofa shield area (Y. LAGEAT, 1989). pioneered by the late Professor P. Birot has been upheld. In numerous regional monographs, widely distributed between GEOLOGICAL POTENTIAL theArcticCircleand theTropicofCapricorn, special attention has been devoted to the A presentation of the geology of the relationships between landforms and Bushveld Complex is essential to any geological structure, with the purpose to understanding of its surface morphology. distinguish between the direct control of Ranging in composition from ultrabasic ro recent faulting and the response of acid, it outcrops largely within a region contrasting rock units todifferential erosiono covered bya characteristicvegetation termed This ambiguity may be easily overcome in «Bushveld». -
The Nain Anorthosite Project, Labrador: Field
THE NAIN ANORTHOSITE PROJECT, LABRADOR: FIELD REPORT 1971 S. A. MORSE I EDITOR R. V. PITS I ULAK CONTRIBUTION NO. 9 GEOLOGY DEPARTMENT UNIVERSITY OF MASSACHUSETTS AMHERST, MASSACHUSETTS L THE NAIN ANORTHOSITE PROJECT, LABRADOR: FIElD REPORT 1971 S. A. Morse, Editor Final Report under NSF Grants GA-21386 and GA-27134 to Franklin and Marshall College: "Evolution of Anorthosite and Related Crustal Rocks in Coastal Labrador", and "Facility for Crustal Studies in Coastal Labrador." S. A. Morse, Principal Investigator (now at U.Mass/Amherst) Dirk de Waard, Syracuse Associate Investigators E. P. Wheeler 2nd, Cornell Other contributors: Research Assistants: J. H. Berg, U. Mass/Amherst C. D. Brauer, Vassar G. A. Plananaky, Harvard F. Finley, Syracuse C. C. Rubins, Syracuse T. H. Folkomer, Franklin & Marshall B.G.J. Upton, Edinburgh D. Russell, Syracuse Charles Woodward, Syracuse J. A. Speer, Virginia Polytechnic Contribution No. 9 Amherst, Massachusetts Geology Department December, 1971 Uni~ersity of Massachusetts L I - CONTENTS INTRODUCTION •••••••••.•••••.•••••••••• ......................... 1 GEOLOGIC~ REPORT. • • • • • • • . • • . • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • 9 General Statement ••••••• 9 Collateral Studies •• 12 Eastern Con tact Zone . .....................................•.... 15 Country rocks of the anorthosite massif and anorthosite contacts in the Ford Harbour Region (de Waard) ••••••••••••••••••••• 15 Intrusive contact relations in the outer is lands (Wlleele r) .................................... -
62237 Troctolitic Anorthosite 62.4 Grams
62237 Troctolitic Anorthosite 62.4 grams Figure 1: Photo of 62237. NASA S72-41797 (B&W), NASA S72-38959 (color). Cube is 1 cm. Introduction 62237 and 62236 are chalky white rocks that were Warren and Wasson (1977) concluded that 62237 is collected together along with 62235 and incidental soil, “chemically pristine”, because it was lacking in from the rim of Buster Crater, station 2, Apollo 16 meteoritic siderophiles. (figure 2), where they were found half buried in the regolith (Sutton 1981). The mineral chemistry of these 62237 has been crushed to form a cataclastic texture, rocks is similar and indicates that they belong to the but, in places, the original coarse-grained igneous suite of lunar plutonic rocks termed ferroan anorthosite texture can be discerned by relic clasts (figure 3). (James 1980). Mineralogy Olivine: Olivine (Fo ) crystals up to 3 mm in size Petrography 59-61 Dymek et al. (1975) concluded that 62237 was a slowly are reported in 62237 by Dymek et al. (1975). Warren cooled plutonic lunar rock (figure 1). The mineralogy and Wasson (1977) and Bersch et al. (1991) also of 62237 is that of a ferroan anorthosite with fairly provided analyses of olivine in 62237. Dymek et al. abundant (~20%) mafic minerals (figure 5). noted that olivine in 62237 was extremely depleted in Ca. Lunar Sample Compendium C Meyer 2011 Figure 2: Location of 62237. Pyroxene: Dymek et al. (1975) and Bersch et al. (1991) determined the composition of pyroxene in 62237 (figure 4). Plagioclase: Plagioclase in 62237 is An95-99 and contains only small amount of minor elements (Dymek et al. -
Nickel Content of an Alaskan Basic Rock
If yon do not need this publication after it has served your purpose, please return it to the Geological Survey, using the official mailing label at the end UNITED STATES DEPARTMENT OF THE INTERIOR Harold L. Ickes, Secretary GEOLOGICAL SURVEY W. C. Mendenhall, Director Bulletin 897 D NICKEL CONTENT OF AN ALASKAN BASIC ROCK BY JOHN C. REED Mineral resources of Alaska, 1936 (Pages 263-268) UNITED STATES GOVERNMENT PRINTING OFFICE WASHINGTON : 1939 ?For sale by the Superintendent of Documents, Washington, D. C. ....... Price 5 cent! CONTENTS Page- Abstract__----------__...__-_--_--__--___-._--_._..__.____ 265 Location and general features.__--_--_------__-_-__---_-_--___-_-___ 263 Petrographic studies-______-_-__---_--_-----___---_--_-__-____-____ 265- Chemical analyses----___-_-__-_-_--__-_---_-____-_____-___________ 267 Conclusions_ _ ___-_________________-_____-_--_-____-___--___----__ 268- ILLUSTRATION Page FIGURE 11. Index map showing location of nickel-bearing sill on Admiralty Island.. ....... ______________--..________ 264 NICKEL CONTENT OF AN ALASKAN BASIC ROCK By JOHN C. REED ABSTRACT A nickel-bearing sill, about 126 feet thick, lies in a thick sequence of greenstone schists, graphitic phyllites, and quartzites near the north end of Admiralty Island not far from Juneau, Alaska. Petrographic measurements show that volumetrically the rock is made up of about 62.07 percent labradprite, 34.22 percent olivine, 2.42 percent pyroxene, 0.79 percent pyrrhotite, 0.21 percent magnetite, 0.14 percent chalcopyrite, and 0.06 percent pentlandite. -
Role of Late Jurassic Intra-Oceanic Structural Inheritance in the Alpine Tectonic Evolution of the Monviso Meta-Ophiolite Complex (Western Alps)
Geol. Mag. 155 (2), 2018, pp. 233–249. c Cambridge University Press 2017 233 doi:10.1017/S0016756817000553 Role of Late Jurassic intra-oceanic structural inheritance in the Alpine tectonic evolution of the Monviso meta-ophiolite Complex (Western Alps) ∗ ∗ ∗ GIANNI BALESTRO , ANDREA FESTA †, ALESSANDRO BORGHI , ∗ ∗ DANIELE CASTELLI , MARCO GATTIGLIO & PAOLA TARTAROTTI‡ ∗ Dipartimento di Scienze della Terra, Università di Torino, Via Valperga Caluso, 35, 10125 – Torino, Italy ‡Dipartimento di Scienze della Terra, Università di Milano, Via Mangiagalli, 34, 20133 – Milano, Italy (Received 31 October 2016; accepted 2 June 2017; first published online 17 July 2017) Abstract – The eclogite-facies Monviso meta-ophiolite Complex in the Western Alps represents a well-preserved fragment of oceanic lithosphere and related Upper Jurassic – Lower Cretaceous sed- imentary covers. This meta-ophiolite sequence records the evolution of an oceanic core complex formed by mantle exhumation along an intra-oceanic detachment fault (the Baracun Shear Zone), re- lated to the opening of the Ligurian–Piedmont oceanic basin (Alpine Tethys). On the basis of detailed geological mapping, and structural, stratigraphic and petrological observations, we propose a new interpretation for the tectonostratigraphic architecture of the Monviso meta-ophiolite Complex, and discuss the role played by structural inheritance in its formation. We document that subduction- and exhumation-related Alpine tectonics were strongly influenced by the inherited Jurassic intra-oceanic tectonosedimentary physiography. The latter, although strongly deformed during a major Alpine stage of non-cylindrical W-verging folding and faulting along exhumation-related Alpine shear zones (i.e. the Granero–Casteldelfino and Villanova–Armoine shear zones), was not completely dismembered into different tectonic units or subduction-related mélanges as suggested in previous interpretations. -
Fluid Evolution in an Oceanic Core Complex: a Fluid Inclusion Study from IODP Hole U1309 D - Atlantis Massif, 30°N, Mid-Atlantic Ridge
This is a repository copy of Fluid evolution in an Oceanic Core Complex: a fluid inclusion study from IODP hole U1309 D - Atlantis Massif, 30°N, Mid-Atlantic Ridge. White Rose Research Online URL for this paper: http://eprints.whiterose.ac.uk/80181/ Version: Published Version Article: Castelain, T, McCaig, AM and Cliff, RA (2014) Fluid evolution in an Oceanic Core Complex: a fluid inclusion study from IODP hole U1309 D - Atlantis Massif, 30°N, Mid-Atlantic Ridge. Geochemistry, Geophysics, Geosystems, 15 (4). 1193 - 1214. ISSN 1525-2027 https://doi.org/10.1002/2013GC004975 Reuse Unless indicated otherwise, fulltext items are protected by copyright with all rights reserved. The copyright exception in section 29 of the Copyright, Designs and Patents Act 1988 allows the making of a single copy solely for the purpose of non-commercial research or private study within the limits of fair dealing. The publisher or other rights-holder may allow further reproduction and re-use of this version - refer to the White Rose Research Online record for this item. Where records identify the publisher as the copyright holder, users can verify any specific terms of use on the publisher’s website. Takedown If you consider content in White Rose Research Online to be in breach of UK law, please notify us by emailing [email protected] including the URL of the record and the reason for the withdrawal request. [email protected] https://eprints.whiterose.ac.uk/ PUBLICATIONS Geochemistry, Geophysics, Geosystems RESEARCH ARTICLE Fluid evolution in an Oceanic Core Complex: A fluid inclusion 10.1002/2013GC004975 study from IODP hole U1309 D—Atlantis Massif, 30N, Key Points: Mid-Atlantic Ridge The TAG model is a good analog for fluid evolution at Atlantis Massif Teddy Castelain1, Andrew M. -
Fossil Oceanic Core Complexes in the Alps. New Field, Geochemical And
Decrausaz et al. Swiss J Geosci (2021) 114:3 https://doi.org/10.1186/s00015-020-00380-4 Swiss Journal of Geosciences ORIGINAL PAPER Open Access Fossil oceanic core complexes in the Alps. New feld, geochemical and isotopic constraints from the Tethyan Aiguilles Rouges Ophiolite (Val d’Hérens, Western Alps, Switzerland) Thierry Decrausaz1,2* , Othmar Müntener1, Paola Manzotti3, Romain Lafay2 and Carl Spandler4 Abstract Exhumation of basement rocks on the seafoor is a worldwide feature along passive continental margins and (ultra-) slow-spreading environments, documented by dredging, drilling or direct observations by diving expeditions. Com- plementary observations from exhumed ophiolites in the Alps allow for a better understanding of the underlying processes. The Aiguilles Rouges ophiolitic units (Val d’Hérens, Switzerland) are composed of kilometre-scale remnants of laterally segmented oceanic lithosphere only weakly afected by Alpine metamorphism (greenschist facies, Raman thermometry on graphite: 370–380 °C) and deformation. Geometries and basement-cover sequences comparable to the ones recognized in actual (ultra-) slow-spreading environments were observed, involving exhumed serpentinized and carbonatized peridotites, gabbros, pillow basalts and tectono-sedimentary cover rocks. One remarkable feature is the presence of a kilometric gabbroic complex displaying preserved magmatic minerals, textures and crosscutting relationships between the host gabbro and intruding diabase, hornblende-bearing dikelets or plagiogranite. The bulk major and trace element chemistry of mafc rocks is typical of N-MORB magmatism (Ce N/YbN: 0.42–1.15). This is supported by in-situ isotopic signatures of magmatic zircons (εHf 13 0.6) and apatites (εNd 8.5 0.8), determined for gabbros and plagiogranites. -
Integrated Ocean Drilling Program Expedition 312 Preliminary Report (Including Expedition 309 Accomplishments)
Integrated Ocean Drilling Program Expedition 312 Preliminary Report (including Expedition 309 accomplishments) Superfast Spreading Rate Crust 3 A complete in situ section of upper oceanic crust formed at a superfast spreading rate 28 October–28 December 2005 Expedition 309 and 312 Scientists PUBLISHER’S NOTES Material in this publication may be copied without restraint for library, abstract service, educational, or personal research purposes; however, this source should be appropriately acknowledged. Citation: Expedition 309 and 312 Scientists, 2006. Superfast spreading rate crust 3: a complete in situ section of upper oceanic crust formed at a superfast spreading rate. IODP Prel. Rept., 312. doi:10:2204/ iodp.pr.312.2006 Distribution: Electronic copies of this series may be obtained from the Integrated Ocean Drilling Program (IODP) Publication Services homepage on the World Wide Web at iodp.tamu.edu/publications. This publication was prepared by the Integrated Ocean Drilling Program U.S. Implementing Organization (IODP-USIO): Joint Oceanographic Institutions, Inc., Lamont-Doherty Earth Observatory of Columbia University, and Texas A&M University, as an account of work performed under the international Integrated Ocean Drilling Program, which is managed by IODP Management International (IODP-MI), Inc. Funding for the program is provided by the following agencies: European Consortium for Ocean Research Drilling (ECORD) Ministry of Education, Culture, Sports, Science and Technology (MEXT) of Japan Ministry of Science and Technology (MOST), People’s Republic of China U.S. National Science Foundation (NSF) DISCLAIMER Any opinions, findings, and conclusions or recommendations expressed in this publication are those of the author(s) and do not necessarily reflect the views of the participating agencies, IODP Management International, Inc., Joint Oceanographic Institutions, Inc., Lamont-Doherty Earth Observatory of Columbia University, Texas A&M University, or Texas A&M Research Foundation. -
Babbitt Se.Indd
Prepared and Published with the Support of MISCELLANEOUS MAP SERIES THE U.S. GEOLOGICAL SURVEY AS PART OF THE 2004 STATE GEOLOGIC MAPPING PROGRAM ELEMENT (STATEMAP) MAP M-162 MINNESOTA GEOLOGICAL SURVEY OF THE NATIONAL GEOLOGIC MAPPING PROGRAM Bedrock Geology, Babbitt SE Quadrangle Harvey Thorleifson, Director �� ��� BEDROCK GEOLOGY OF THE BABBITT SOUTHEAST QUADRANGLE, ��� �� ��� ��� �� �� �� �� ST. LOUIS AND LAKE COUNTIES, MINNESOTA �� �� �� ��� �� By �� ��� �� ��� ��� �� �� James D. Miller, Jr. �� �� �� �� ��� 2005 �� �� ��� �� ��� �� �� ��� ������������������������ MAP SYMBOLS ����������� Geologic contact—Approximately located by outcrop control. ��� ��������� �� ��� ��������� Geologic contact—Poorly located by rare outcrop, topography, and/or ����������� �� ��� ����� geophysical data. ��������� �� ��� Fault—Inferred, based on geologic offset, topography, local structures, ��� �� ������� ��� ��� ����� and/or geophysical data. ��� ��� ������ ��� ��� ���������� Fault—Speculative, based on geophysical data and/or topography. ��� ��������� ������ Attitude of inclined sedimentary or volcanic bedding ��� ������� � ���������� �� �� Attitude of inclined igneous layering ��� ��� ��� ������ ��������� ��������������� Attitude of igneous foliation (inclined, horizontal) �� ��� Trend of igneous fabric ��� ��� ��� ��� ������������� Attitude of inclined bedding-parallel joint set ��� ��� ������ Attitude of vertical mineralized joint ��� �� �� �� Attitude of inclined felsic dike ��� ��� ��� Area of bedrock outcrop �� �� ��� ��� ����������� Drill hole -
Implications for the Rheological Behavior of Oceanic Detachment Faults
Article Volume 14, Number 8 28 August 2013 doi: 10.1002/ggge.20184 ISSN: 1525-2027 Mylonitic deformation at the Kane oceanic core complex: Implications for the rheological behavior of oceanic detachment faults Lars N. Hansen Department of Geological and Environmental Sciences, Stanford University, 450 Serra Mall, Building 320, Stanford, California, 94305, USA ([email protected]) Michael J. Cheadle, Barbara E. John, and Susan M. Swapp Department of Geology and Geophysics, University of Wyoming, Wyoming, USA Henry J. B. Dick, Brian E. Tucholke, and Maurice A. Tivey Department of Geology and Geophysics, Woods Hole Oceanographic Institution, Woods Hole, Massachusetts, USA [1] The depth extent, strength, and composition of oceanic detachment faults remain poorly understood because the grade of deformation-related fabrics varies widely among sampled oceanic core complexes (OCCs). We address this issue by analyzing fault rocks collected from the Kane oceanic core complex at 23300N on the Mid-Atlantic Ridge. A portion of the sample suite was collected from a younger fault scarp that cuts the detachment surface and exposes the interior of the most prominent dome. The style of deformation was assessed as a function of proximity to the detachment surface, revealing a 450 m thick zone of high-temperature mylonitization overprinted by a 200 m thick zone of brittle deformation. Geothermometry of deformed gabbros demonstrates that crystal-plastic deformation occurred at temperatures >700C. Analysis of the morphology of the complex in conjunction with recent thermochronology suggests that deformation initiated at depths of 7 km. Thus we suggest the detachment system extended into or below the brittle-plastic transition (BPT).