Geochemistry of Mid-Ocean Ridge Basalt Within and Surrounding The
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51. Breakup and Seafloor Spreading Between the Kerguelen Plateau-Labuan Basin and the Broken Ridge-Diamantina Zone1
Wise, S. W., Jr., Schlich, R., et al., 1992 Proceedings of the Ocean Drilling Program, Scientific Results, Vol. 120 51. BREAKUP AND SEAFLOOR SPREADING BETWEEN THE KERGUELEN PLATEAU-LABUAN BASIN AND THE BROKEN RIDGE-DIAMANTINA ZONE1 Marc Munschy,2 Jerome Dyment,2 Marie Odile Boulanger,2 Daniel Boulanger,2 Jean Daniel Tissot,2 Roland Schlich,2 Yair Rotstein,2,3 and Millard F. Coffin4 ABSTRACT Using all available geophysical data and an interactive graphic software, we determined the structural scheme of the Australian-Antarctic and South Australian basins between the Kerguelen Plateau and Broken Ridge. Four JOIDES Resolution transit lines between Australia and the Kerguelen Plateau were used to study the detailed pattern of seafloor spreading at the Southeast Indian Ridge and the breakup history between the Kerguelen Plateau and Broken Ridge. The development of rifting between the Kerguelen Plateau-Labuan Basin and the Broken Ridge-Diamantina Zone, and the evolution of the Southeast Indian Ridge can be summarized as follows: 1. From 96 to 46 Ma, slow spreading occurred between Antarctica and Australia; the Kerguelen Plateau, Labuan Basin, and Diamantina Zone stretched at 88-87 Ma and 69-66 Ma. 2. From 46 to 43 Ma, the breakup between the Southern Kerguelen Plateau and the Diamantina Zone propagated westward at a velocity of about 300 km/m.y. The breakup between the Northern Kerguelen Plateau and Broken Ridge occurred between 43.8 and 42.9 Ma. 3. After 43 Ma, volcanic activity developed on the Northern Kerguelen Plateau and at the southern end of the Ninetyeast Ridge. Lava flows obscured the boundaries of the Northern Kerguelen Plateau north of 48°S and of the Ninetyeast Ridge south of 32°S, covering part of the newly created oceanic crust. -
Geological Timeline - Tasmania
GEODIVERSITY Geological Timeline - Tasmania Tasmania’s spectacular geodiversity has contributed Chains of volcanoes form across Tasmania, including Mt directly to the islands’ biodiversity. The State’s Read Volcanic Belt, a highly significant mineralised belt. geodiversity is a result of continental drift, ice ages, humid, hot conditions and earthquakes occurring over 443 - 408 Million Years Ago more than a billion years. Extensive erosion and subsequent deposition form the sandstones and conglomerates of West Coast Range and A very brief and summarised account of Tasmania’s Denison Range. geological history is outlined below. Although Tasmania is referred to frequently, it was not until about 45 Tasmania partly covered by a warm tropical sea and part million years ago that Tasmania began to look anything of a much larger land mass of Gondwana situated near like it does today. the equator. Gordon Limestone formed from the debris of marine life. Today this limestone outcrops in parts of 4600 - 635 Million Years Ago the Franklin and Gordon River valleys and around Mole The Earth formed about 4600 million years ago. Creek, where subsequent disolving by water has formed many karst and cave systems. Little is known about the Precambrian, despite it making up roughly seven-eighths of the Earth’s history. This is 408 - 360 Million Years Ago because traces of the geological heritage of Precambrian Warm shallow continental seas provide a hospitable times have been erased by relentless subsequent erosion. environment for marine life of all kinds. Coral reefs made First evidence of simple life forms, cyanobacteria, the their first appearance during this time, and first bony fish building blocks for stromatolites, are among the oldest appear. -
South-East Marine Region Profile
South-east marine region profile A description of the ecosystems, conservation values and uses of the South-east Marine Region June 2015 © Commonwealth of Australia 2015 South-east marine region profile: A description of the ecosystems, conservation values and uses of the South-east Marine Region is licensed by the Commonwealth of Australia for use under a Creative Commons Attribution 3.0 Australia licence with the exception of the Coat of Arms of the Commonwealth of Australia, the logo of the agency responsible for publishing the report, content supplied by third parties, and any images depicting people. For licence conditions see: http://creativecommons.org/licenses/by/3.0/au/ This report should be attributed as ‘South-east marine region profile: A description of the ecosystems, conservation values and uses of the South-east Marine Region, Commonwealth of Australia 2015’. The Commonwealth of Australia has made all reasonable efforts to identify content supplied by third parties using the following format ‘© Copyright, [name of third party] ’. Front cover: Seamount (CSIRO) Back cover: Royal penguin colony at Finch Creek, Macquarie Island (Melinda Brouwer) B / South-east marine region profile South-east marine region profile A description of the ecosystems, conservation values and uses of the South-east Marine Region Contents Figures iv Tables iv Executive Summary 1 The marine environment of the South-east Marine Region 1 Provincial bioregions of the South-east Marine Region 2 Conservation values of the South-east Marine Region 2 Key ecological features 2 Protected species 2 Protected places 2 Human activities and the marine environment 3 1. -
Insights on the Indian Ocean Tectonics and Geophysics Supported by GMT Polina Lemenkova
Insights on the Indian Ocean tectonics and geophysics supported by GMT Polina Lemenkova To cite this version: Polina Lemenkova. Insights on the Indian Ocean tectonics and geophysics supported by GMT. Riscuri si Catastrofe, ”Babes-Bolyai” University from Cluj-Napoca, Faculty of Geography, 2020, 27 (2), pp.67- 83. 10.24193/RCJ2020_12. hal-03033533 HAL Id: hal-03033533 https://hal.archives-ouvertes.fr/hal-03033533 Submitted on 1 Dec 2020 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 Riscuri și catastrofe, an XX, vol, 27 nr. 2/2020 INSIGHTS ON THE INDIAN OCEAN TECTONICS AND GEOPHYSICS SUPPORTED BY GMT POLINA LEMENKOVA1 Abstract. Insights on the Indian Ocean Tectonics and Geophysics Supported by GMT. This paper presented analyzed and summarized data on geological and geophysical settings about the tectonics and geological structure of the seafloor of the Indian Ocean by thematic visualization of the topographic, geophysical and geo- logical data. The seafloor topography of the Indian Ocean is very complex which includes underwater hills, isolated mountains, underwater canyons, abyssal and ac- cumulative plains, trenches. Complex geological settings explain seismic activity, repetitive earthquakes, and tsunami. -
Assessment of Australia's High Seas Permits
Assessment of Australia’s High Seas Permits May, 2013 © Commonwealth of Australia 2013 This work is copyright. Apart from any use as permitted under the Copyright Act 1968, no part may be reproduced by any process without prior written permission from the Commonwealth, available from the Department of Sustainability, Environment, Water, Population and Communities. Requests and inquiries concerning reproduction and rights should be addressed to: Assistant Secretary Marine Biodiversity and Biosecurity Branch Department of Sustainability, Environment, Water, Population and Communities GPO Box 787 Canberra ACT 2601 Disclaimer This document is an assessment carried out by the Department of Sustainability, Environment, Water, Population and Communities of a commercial fishery against the Australian Government ‘Guidelines for the Ecologically Sustainable Management of Fisheries – 2nd Edition’. It forms part of the advice provided to the Minister for Sustainability, Environment, Water, Population and Communities on the fishery in relation to decisions under Part 13A of the Environment Protection and Biodiversity Conservation Act 1999. The views expressed do not necessarily reflect those of the Minister for Sustainability, Environment, Water, Population and Communities or the Australian Government. While reasonable efforts have been made to ensure that the contents of this report are factually correct, the Australian Government does not accept responsibility for the accuracy or completeness of the contents, and shall not be liable for any loss or damage that may be occasioned directly or indirectly through the use of, or reliance on, the contents of this report. You should not rely solely on the information presented in the report when making a commercial or other decision. -
Glacial-Interglacial Sea Surface Temperture And
PLANKTIC FORAMINIFERA-BASED SEA SURFACE TEMPERATURE ESTIMATES AND LATE QUATERNARY OCEANOGRAPHY OFF NEW ZEALAND’S WEST COAST Andrew Peter Kolodziej A thesis submitted in partial fulfillment for the degree of Masters of Science in Geology School of Geography, Environment and Earth Sciences Victoria University 2010 i ii Abstract Planktic foraminiferal assemblages were used to investigate the paleoceanography of the Eastern Tasman Sea over the last 480 kyrs (Marine Isotope Stages 12-1). One hundred and sixty-two faunas (96 picked and identified as part of this project (MIS 12-6) added to 66 census counts from Dr. M. Crundwell (MIS 6-1)) have been assembled from Marion Dufresne piston core MD06-2986 (~43˚ S. off New Zealand‟s west coast, 1477 m water depth). Faunal changes through the last five glacial-interglacial cycles are used to track surface water mass movement. Glacial periods are dominated by the eutrophic species Globigerina bulloides, with significant contributions from the temperate species Globoconella inflata. Temperate species Neogloboquadrina incompta and Gc. inflata dominate interglacials, with the former dominating the warmer parts and the latter dominating the cooler parts of the interglacials. Modern Analogue Technique (MAT) and an Artificial Neural Network (ANN) were used to estimate past sea surface temperatures (SST) based on the foraminiferal census counts data (23 species, ~46,000 specimens). SSTs show that MIS 12 was the longest, sustained cold period, while the coldest temperature was recorded in MIS 5d (~8º C). Interglacials MIS 11 and 5e are the two warmest stages of the record, with SSTs reaching ~18.5º C, about ~2º C warmer than present day. -
CHAPTER 2 Aseismic Ridges of the Northeastern Indian Ocean
CHAPTER 2 Aseismic ridges of the northeastern Indian Ocean 2.1 Evolution of the Indian Ocean 2.2 Major Aseismic Ridges 2.2.1 The Ninetyeast Ridge 2.2.2 The Chagos-Laccadive Ridge 2.2.3 The 85°E Ridge 2.2.4 The Comorin Ridge 2.2.5 The Broken Ridge 2.3 Other Major Structural Features 2.3.1 The Kerguelen Plateau 2.3.2 The Elan Bank 2.3.3 The Afanasy Nikitin seamount Chapter 2 Aseismic ridges of the northeastern Indian Ocean 2.1 Evolution of the Indian Ocean The initiation of the Indian Ocean commenced with the breakup of the Gondwanaland super-continent into two groups of continental masses during the Mesozoic period (Norton and Sclater, 1979). The first split of the Gondwanaland may possibly have associated with the Karoo mega-plume (Lawver and Gahagan, 1998). Followed by this rifting phase, during the late Jurassic, the Mozambique and Somali basins have formed by seafloor spreading activity of series of east-west trending ridge segments. Thus, the Gondwanaland super-continent divided into western and eastern continental blocks. The Western Gondwanaland consisted of Africa, Arabia and South America, whereas the East Gondwanaland consisted of Antarctica, Australia, New Zeeland, Seychelles, Madagascar and India-Sri Lanka (Figure 2.1). After initial break-up, the East Gondwanaland moved southwards from the West Gondwanaland and led to gradual enlargement of the intervening seaways between them (Bhattacharya and Chaubey, 2001). Both West and East Gondwanaland masses have further sub-divided during the Cretaceous period. Approximate reconstructions of continental masses of the Gondwanaland from Jurassic to Present illustrating the aforesaid rifting events are shown in Figure 2.1 (Royer et al., 1992). -
38. Tectonic Constraints on the Hot-Spot Formation of Ninetyeast Ridge1
Weissel, J., Peirce, J., Taylor, E., Alt, J., et al. 1991 Proceedings of the Ocean Drilling Program, Scientific Results, Vol. 121 38. TECTONIC CONSTRAINTS ON THE HOT-SPOT FORMATION OF NINETYEAST RIDGE1 Jean-Yves Royer,2 John W. Peirce,3 and Jeffrey K. Weissel4 ABSTRACT This paper examines the constraints on the tectonic setting of Ninetyeast Ridge, based on a compilation of bathymetric and magnetic data from the basins surrounding Ninetyeast Ridge in the Indian Ocean that includes the magnetic profiles collected under way during ODP Leg 121. Magnetic data in the Central Indian Basin demonstrate that the spreading center immediately west of Ninetyeast Ridge jumped to the south by a total amount of 11° between 68 and 46 Ma, implying that parts of the mirror image of Ninetyeast Ridge on the Antarctic plate were transferred onto the Indian plate. The obliquity of Ninetyeast Ridge relative to the fracture zone pattern and the occurrence of an Eocene extinct spreading axis in the Wharton Basin suggest that the northern part of Ninetyeast Ridge was emplaced by intraplate volcanism on the Indian plate, whereas the middle and southern parts of the ridge were emplaced along transform plate boundaries. The northward drift of the Indian plate over a single hot spot is the most plausible origin for Ninetyeast Ridge. Based on a recent kinematic model for the relative motions of the Indian, Antarctic, and Australian plates, we present a simple model that reconciles most of the available observations for Ninetyeast Ridge: Paleomagnetism, distribution of basement ages, geochemistry, and geometry. In addition, the model predicts a slow westward migration of the Kerguelen/Ninetyeast hot spot with respect to the Antarctic and Australian plates between the Late Cretaceous and early Oligocene (84 to 36 Ma). -
7TH ANNUAL MEETING of the COMMISSION 23-27 January 2019, the Hague, the Netherlands
7TH ANNUAL MEETING OF THE COMMISSION 23-27 January 2019, The Hague, The Netherlands COMM7-Prop14.1 Explanatory Note: Exploratory fishing for Patagonian toothfish within the SPRFMO Convention Area European Union PO Box 3797, Wellington 6140, New Zealand P: +64 4 499 9889 – F: +64 4 473 9579 – E: [email protected] www.sprfmo.int COMM7-Prop14.1 Explanatory Note to Prop14 Background document: Exploratory fishing for Patagonian toothfish within the SPRFMO Convention Area European Union Table of Contents 1 Purpose .......................................................................................................................................... 3 2 Introduction ................................................................................................................................... 6 3 Vessel specific details as required under paragraphs 2 and 3 of Annex 1 of CMM 05-2016 (Record of Vessels) ................................................................................................................................................... 6 4 Fisheries Operation Plan .............................................................................................................. 11 4.1 Description of the exploratory fishery ................................................................................. 11 4.2 Fishing gear ......................................................................................................................... 11 4.3 Time period of the fisheries operation plan ....................................................................... -
A Global Review and Digital Database of Large-Scale Extinct Spreading Centers GEOSPHERE
Research Paper GEOSPHERE A global review and digital database of large-scale extinct GEOSPHERE; v. 13, no. 3 spreading centers doi:10.1130/GES01379.1 Sarah J. MacLeod, Simon E. Williams, Kara J. Matthews, R. Dietmar Müller, and Xiaodong Qin EarthByte Group, School of Geosciences, University of Sydney, Camperdown, New South Wales 2006, Australia 9 figures; 4 tables; 2 supplemental files CORRESPONDENCE: sarah.macleod@ sydney ABSTRACT into which proposed locations are more likely to have been former spreading .edu .au centers, and our analysis further leads to the discovery of several previously Extinct mid-ocean ridges record past plate boundary reorganizations, and unidentified structures in the south of the West Philippine Basin that likely CITATION: MacLeod, S.J., Williams, S.E., Matthews, K.J., Müller, R.D., and Qin, X.D., 2017, A global review identifying their locations is crucial to developing a better understanding of represent extinct ridges and a possible extinct ridge in the western South At- and digital database of large-scale extinct spread- the drivers of plate tectonics and oceanic crustal accretion. Frequently, extinct lantic. We make available our global compilation of data and analyses of indi- ing centers: Geosphere, v. 13, no. 3, p. 911–949, ridges cannot be easily identified within existing geophysical data sets, and vidual ridges in a global extinct ridge data set at the GPlates Portal webpage1. doi:10.1130/GES01379.1. there are many controversial examples that are poorly constrained. We ana- lyze the axial morphology and gravity signal of 29 well-constrained, global, Received 17 June 2016 Revision received 29 November 2016 large-scale extinct ridges that are digitized from global data sets, to describe INTRODUCTION Accepted 15 March 2017 their key characteristics. -
Surface-Circulation Change in the Southern Ocean Across the Middle Eocene Climatic Optimum: Inferences from Dinoflagellate Cysts and Biomarker Paleothermometry 5
Clim. Past Discuss., https://doi.org/10.5194/cp-2019-35 Manuscript under review for journal Clim. Past Discussion started: 4 April 2019 c Author(s) 2019. CC BY 4.0 License. Surface-circulation change in the Southern Ocean across the Middle Eocene Climatic Optimum: inferences from dinoflagellate cysts and biomarker paleothermometry 5 Margot J. Cramwinckel1, Lineke Woelders1,*, Emiel P. Huurdeman2, Francien Peterse1, Stephen J. Gallagher3, Jörg Pross2, Catherine E. Burgess4,#, Gert-Jan Reichart1,5, Appy Sluijs1, Peter K. Bijl1 1Department of Earth Sciences, Faculty of Geoscience, Utrecht University, Utrecht, The Netherlands 10 2Paleoenvironmental Dynamics Group, Institute of Earth Sciences, Heidelberg University, Heidelberg, Germany 3School of Earth Sciences, The University of Melbourne, Melbourne, Australia 4School of Earth and Ocean Sciences, Cardiff University, Cardiff, United Kingdom 5NIOZ Royal Netherlands Institute for Sea Research and Utrecht University, Den Burg, Texel, The Netherlands *Now at Institute of Arctic and Alpine Research, University of Colorado, Boulder, US 15 #Now at Shell UK LTD, Aberdeen, UK Correspondence to: Margot J. Cramwinckel ([email protected]) Abstract Global climate cooled from the early Eocene hothouse (~52–50 Ma) to the latest Eocene (~34 Ma). At the same time, the tectonic evolution of the Southern Ocean was characterized by the opening and deepening of circum-Antarctic gateways, 20 which affected both surface- and deep-ocean circulation. The Tasman Gateway played a key role in regulating ocean throughflow between Australia and Antarctica. Southern Ocean surface currents through and around the Tasman Gateway have left recognizable tracers in the spatiotemporal distribution of plankton fossils, including organic-walled dinoflagellate cysts. -
Heat Flow from the Southeast Indian Ridge Flanks Between 80°E and 140°E: Data Review and Analysis L
Heat flow from the Southeast Indian Ridge flanks between 80E and 140E: Data review and analysis L. G´eli,T. C. Lee, J. R. Cochran, J. Francheteau, D. Abbott, C. Labails, D. Appriou To cite this version: L. G´eli,T. C. Lee, J. R. Cochran, J. Francheteau, D. Abbott, et al.. Heat flow from the Southeast Indian Ridge flanks between 80E and 140E: Data review and analysis. Journal of Geophysical Research : Solid Earth, American Geophysical Union, 2008, 113, pp.B01101. <10.1029/2007JB005001>. <insu-00267287> HAL Id: insu-00267287 https://hal-insu.archives-ouvertes.fr/insu-00267287 Submitted on 15 Feb 2011 HAL is a multi-disciplinary open access L'archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destin´eeau d´ep^otet `ala diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publi´esou non, lished or not. The documents may come from ´emanant des ´etablissements d'enseignement et de teaching and research institutions in France or recherche fran¸caisou ´etrangers,des laboratoires abroad, or from public or private research centers. publics ou priv´es. JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 113, B01101, doi:10.1029/2007JB005001, 2008 Click Here for Full Article Heat flow from the Southeast Indian Ridge flanks between 80°E and 140°E: Data review and analysis L. Ge´li,1 T. C. Lee,2 J. R. Cochran,3 J. Francheteau,4 D. Abbott,3 C. Labails,1 and D. Appriou1 Received 18 February 2007; revised 21 May 2007; accepted 20 September 2007; published 5 January 2008.