APPENDIX PHYSICAL PRINCIPLES MENTIONED in the TEXT Bernoulli's Theorem in a Stream Ofliquid, the Sum of the Elevation Head
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Identification of Erosional Terraces on Seamounts
ORIGINAL RESEARCH published: 03 July 2018 doi: 10.3389/feart.2018.00088 Identification of Erosional Terraces on Seamounts: Implications for Interisland Connectivity and Subsidence in the Galápagos Archipelago Darin M. Schwartz 1*, S. Adam Soule 2, V. Dorsey Wanless 1 and Meghan R. Jones 2 1 Department of Geosciences, Boise State University, Boise, ID, United States, 2 Geology and Geophysics Department, Woods Hole Oceanographic Institution, Woods Hole, MA, United States Shallow seamounts at ocean island hotspots and in other settings may record emergence histories in the form of submarine erosional terraces. Exposure histories are valuable for constraining paleo-elevations and sea levels in the absence of more traditional Edited by: markers, such as drowned coral reefs. However, similar features can also be produced Ricardo S. Ramalho, Universidade de Lisboa, Portugal through primary volcanic processes, which complicate the use of terraced seamounts Reviewed by: as an indicator of paleo-shorelines. In the western Galápagos Archipelago, we utilize Neil Mitchell, newly collected bathymetry along with seafloor observations from human-occupied University of Manchester, submersibles to document the location and depth of erosional terraces on seamounts United Kingdom Daneiele Casalbore, near the islands of Santiago, Santa Cruz, Floreana, Isabela, and Fernandina. We directly Sapienza Università di Roma, Italy observed erosional features on 22 seamounts with terraces. We use these observations Rui Quartau, Instituto Hidrográfico, Portugal and bathymetric analysis to develop a framework to identify terrace-like morphologic *Correspondence: features and classify them as either erosional or volcanic in origin. From this framework Darin M. Schwartz we identify 79 erosional terraces on 30 seamounts that are presently found at depths [email protected] of 30 to 300 m. -
The Depths of Magma Chambers Under the Galapagos Ridge Presented in Partial Fulfillment of the Requirements for Graduation With
The Depths of Magma Chambers under the Galapagos Ridge Presented in Partial Fulfillment of the Requirements for Graduation with a Bachelor of Science in Geological Sciences in the undergraduate colleges of The Ohio State University by Emily V. England The Ohio State University August 2008 Dr. Michael Barton Advisor Table of Contents Acknowledgements……………………………………………………………………..p.1 Abstract…………………………………………………………………………………p.2 Introduction…………………………………………………………………………….p.4 Background……………………………………………………………………………..p.6 Methods………………………………………………………………………………..p.9 Samples……………………………………………………………………………..…p.11 Results…………………………………………………………………………………p.13 Discussion……………………………………………………………………………..p.15 Conclusions……………………………………………………………………………p. 18 References…………………………………………………………………………….p.19 Appendix (Summary of P and T)……………………………………………………..p. 21 ACKNOWLEDGEMENTS I would like to give thanks to the following people for helping me with my research on the Galapagos ridge while at The Ohio State University: my research advisor Dr. Michael Barton who suggested this project and mentored me along the way, Dr. Wendy Panero for her time and conversation, graduate student Daniel Kelley, and classmate Jameson “Dino” Scott. I would also like to acknowledge the entire Geological Sciences Department at OSU. I have been thoroughly pleased with my education and believe that I have found a field that I will enjoy and pursue for the rest of my life. And of course I thank my parents and family for more than words can say. 1 ABSTRACT The Galapagos Ridge System is one of the -
South-East Asia Second Edition CHARLES S
Geological Evolution of South-East Asia Second Edition CHARLES S. HUTCHISON Geological Society of Malaysia 2007 Geological Evolution of South-east Asia Second edition CHARLES S. HUTCHISON Professor emeritus, Department of geology University of Malaya Geological Society of Malaysia 2007 Geological Society of Malaysia Department of Geology University of Malaya 50603 Kuala Lumpur Malaysia All rights reserved. No part of this publication may be reproduced, stored in a retrieval system, or transmitted, in any form or by any means, electronic, mechanical, photocopying, recording, or otherwise, without the prior permission of the Geological Society of Malaysia ©Charles S. Hutchison 1989 First published by Oxford University Press 1989 This edition published with the permission of Oxford University Press 1996 ISBN 978-983-99102-5-4 Printed in Malaysia by Art Printing Works Sdn. Bhd. This book is dedicated to the former professors at the University of Malaya. It is my privilege to have collabo rated with Professors C. S. Pichamuthu, T. H. F. Klompe, N. S. Haile, K. F. G. Hosking and P. H. Stauffer. Their teaching and publications laid the foundations for our present understanding of the geology of this complex region. I also salute D. ]. Gobbett for having the foresight to establish the Geological Society of Malaysia and Professor Robert Hall for his ongoing fascination with this region. Preface to this edition The original edition of this book was published by known throughout the region of South-east Asia. Oxford University Press in 1989 as number 13 of the Unfortunately the stock has become depleted in 2007. Oxford monographs on geology and geophysics. -
Hunting for Hydrothermal Vents Along the Galã¡Pagos Spreading Center
University of South Carolina Scholar Commons Faculty Publications Earth, Ocean and Environment, School of the 12-2007 Hunting for Hydrothermal Vents Along the Galápagos Spreading Center Rachel M. Haymon University of California - Santa Barbara Edward T. Baker Joseph A. Resing Scott M. White University of South Carolina - Columbia, [email protected] Ken C. Macdonald University of California - Santa Barbara Follow this and additional works at: https://scholarcommons.sc.edu/geol_facpub Part of the Earth Sciences Commons Publication Info Published in Oceanography, Volume 20, Issue 4, 2007, pages 100-107. Haymon, R. M., Baker, E. T., Resing, J. A., White, S. M., & Macdonald, K. C. (2007). Hunting for hydrothermal vents along the Galápagos Spreading Center. Oceanography, 20 (4), 100-107. © Oceanography 2007, Oceanography Society This Article is brought to you by the Earth, Ocean and Environment, School of the at Scholar Commons. It has been accepted for inclusion in Faculty Publications by an authorized administrator of Scholar Commons. For more information, please contact [email protected]. or collective redistirbution of any portion of this article by photocopy machine, reposting, or other means is permitted only with the approval of The Oceanography Society. Send all correspondence to: [email protected] ofor Th e The to: [email protected] Oceanography approval Oceanography correspondence all portionthe Send Society. ofwith any permitted articleonly photocopy by Society, is of machine, reposting, this means or collective or other redistirbution This article has This been published in S P E C I A L Iss U E O N O C E A N E XPL O RATI on B Y R AC H E L M . -
On the Emergence and Submergence of the Galapagos Islands
On the emergence and submergence of the Galápagos Islands Item Type article Authors Geist, Dennis Download date 23/09/2021 23:04:08 Link to Item http://hdl.handle.net/1834/23895 March7996 NOTICIAS DE GALAPAGOS ON THE EMERGENCE AND SUBMERCENCE OF THE GALÁPAGOS ISLANDS By: Dennis Geist INTRODUCTION emerge above the sea due to two principal effects. First, as the Nazca plate travels over the Galápagos hotspot, the The age of sustained emergence of the individual seafloor rises due to thermal expansion. The Galápagos Galápagos islands above the sea is an important issue in thermal swell is predicted to be only 400 m high (Epp, developing evolutionary models for their unique terres- 1984). The sea floor to the west of Fernandina is about trial biota. For one, the age of emergence of the oldest 3200 m deep, so 2800 m of lava needs to pile up on the island permits estimation of when terrestrial organisms swell for an island to form. In reality, much more magma may have originally colonized the archipelago. Second, is required, because as lava erupts from an oceanic volca- the ages of the individual islands and minor islets are no, the extra weight causes the earth's crust to sag into the required for quantitative assessments of rates of coloni- mantle, forming a deep root. Feighner and Richard s (799a) zation and diversification within the archipelago. estimate, for example, that the base of the crust is up to 7 Emergence is not a straightforward geologic problem, km deeper beneath Isabela than it is to the west; in other because the islands constitute an extremely dynamic en- words, for every 1 km of elevation growth of a volcano, vironment - the shorelines that we see today are transient about 4 km of "sinking" occurs. -
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). -
Observational Test of the Global Moving Hot Spot Reference Frame
RESEARCH LETTER Observational Test of the Global Moving Hot Spot 10.1029/2019GL083663 Reference Frame Key Points: Chengzu Wang1 , Richard G. Gordon1 , Tuo Zhang1 , and Lin Zheng1 • The fit of the Global Moving Hotspot Reference Frame (GMHRF) to 1Department of Earth, Environmental, and Planetary Sciences, William Marsh Rice University, Houston, TX, USA observed geologically young trends of hot spot tracks is evaluated • The data are fit significantly worse (p = 0.005) by the GMHRF than by Abstract The Global Moving Hotspot Reference Frame (GMHRF) has been claimed to fit hot spot tracks fixed hot spots better than the fixed hot spot approximation mainly because the GMHRF predicts ≈1,000 km southward • Either plume conduits do not advect motion through the mantle of the Hawaiian mantle plume over the past 80 Ma. As the GMHRF is passively with mantle flow or the GMHRF mantle velocity field is determined by starting at present and calculating backward in time, it should be most accurate and incorrect reliable for the recent geologic past. Here we compare the fit of the GMHRF and of fixed hot spots to the observed trends of young tracks of hot spots. Surprisingly, we find that the GMHRF fits the data significantly Supporting Information: worse (p = 0.005) than does the fixed hot spot approximation. Thus, either plume conduits are not passively • Supporting Information S1 advected with the mantle flow calculated for the GMHRF or Earth's actual mantle velocity field differs substantially from that calculated for the GMHRF. Correspondence to: Hot spots are the surface manifestations of plumes of hot rock that R. -
Pleistocene Volcanism in the Anahim Volcanic Belt, West-Central British Columbia
University of Calgary PRISM: University of Calgary's Digital Repository Graduate Studies The Vault: Electronic Theses and Dissertations 2014-10-24 A Second North American Hot-spot: Pleistocene Volcanism in the Anahim Volcanic Belt, west-central British Columbia Kuehn, Christian Kuehn, C. (2014). A Second North American Hot-spot: Pleistocene Volcanism in the Anahim Volcanic Belt, west-central British Columbia (Unpublished doctoral thesis). University of Calgary, Calgary, AB. doi:10.11575/PRISM/25002 http://hdl.handle.net/11023/1936 doctoral thesis University of Calgary graduate students retain copyright ownership and moral rights for their thesis. You may use this material in any way that is permitted by the Copyright Act or through licensing that has been assigned to the document. For uses that are not allowable under copyright legislation or licensing, you are required to seek permission. Downloaded from PRISM: https://prism.ucalgary.ca UNIVERSITY OF CALGARY A Second North American Hot-spot: Pleistocene Volcanism in the Anahim Volcanic Belt, west-central British Columbia by Christian Kuehn A THESIS SUBMITTED TO THE FACULTY OF GRADUATE STUDIES IN PARTIAL FULFILMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY GRADUATE PROGRAM IN GEOLOGY AND GEOPHYSICS CALGARY, ALBERTA OCTOBER, 2014 © Christian Kuehn 2014 Abstract Alkaline and peralkaline magmatism occurred along the Anahim Volcanic Belt (AVB), a 330 km long linear feature in west-central British Columbia. The belt includes three felsic shield volcanoes, the Rainbow, Ilgachuz and Itcha ranges as its most notable features, as well as regionally extensive cone fields, lava flows, dyke swarms and a pluton. Volcanic activity took place periodically from the Late Miocene to the Holocene. -
Tectonic Patterns and Cenozoic Basalts in the Western Margin of the South China Sea
AAPG International Conference d EtbihiJion '94 Augwt21-24, 1994, KualaLumpur,Malay.till Tectonic patterns and Cenozoic basalts in the western margin of the South China Sea POW-FOONG FAN School of Ocean and Earth Science and Technology Department of Geology and Geophysics, University of Hawaii Honolulu, Hawaii 96822 U_S.A. Abstract: The allochthonous fragments - Indosinia, Sibumasu, East Malaya, and Southwest Kalimantan - rifted from Gondwanaland and drifted northward. Indosinia collided with the Yangzi-Huanan terranes in Devonian or Early Carboniferous period and became part of the East Asia continent. Sibumasu collided· with East Asia continent and East Malaya during the Indosinian Orogeny (220-200 Ma). The Southwest Kalimantan terrane probably rifted from the northeast margin of Indosinia in the Cretaceous. ·At about 50 Ma the collision of the Indian continent into the Eurasian continent led to the fragmentation of Asia and was followed by the opening of the Andaman Sea, the clockwise rotation of the Indochina plate, and the rifting and the opening of the South China Sea. The Late Cretaceous alkaline intrusions in the Red River area of northern Vietnam formed during initial stage of rifting of the South China Sea. The Indian-Eurasian collision has successively pushed the Indochina Peninsula in the east southeast direction. Most of the Middle Tertiary movements probably occurred along the left-lateral Red River, Tonle Sap-Mekong faults concurrent with the opening of most of the eastern South China Sea. The extensional tectonics along these predominantly strike-slip faults may be responsible for the Pliocene Pleistocene alkaline basalts, which extend from the Mekong Delta northwestward into Thailand. -
Synoptic Taxonomy of Major Fossil Groups
APPENDIX Synoptic Taxonomy of Major Fossil Groups Important fossil taxa are listed down to the lowest practical taxonomic level; in most cases, this will be the ordinal or subordinallevel. Abbreviated stratigraphic units in parentheses (e.g., UCamb-Ree) indicate maximum range known for the group; units followed by question marks are isolated occurrences followed generally by an interval with no known representatives. Taxa with ranges to "Ree" are extant. Data are extracted principally from Harland et al. (1967), Moore et al. (1956 et seq.), Sepkoski (1982), Romer (1966), Colbert (1980), Moy-Thomas and Miles (1971), Taylor (1981), and Brasier (1980). KINGDOM MONERA Class Ciliata (cont.) Order Spirotrichia (Tintinnida) (UOrd-Rec) DIVISION CYANOPHYTA ?Class [mertae sedis Order Chitinozoa (Proterozoic?, LOrd-UDev) Class Cyanophyceae Class Actinopoda Order Chroococcales (Archean-Rec) Subclass Radiolaria Order Nostocales (Archean-Ree) Order Polycystina Order Spongiostromales (Archean-Ree) Suborder Spumellaria (MCamb-Rec) Order Stigonematales (LDev-Rec) Suborder Nasselaria (Dev-Ree) Three minor orders KINGDOM ANIMALIA KINGDOM PROTISTA PHYLUM PORIFERA PHYLUM PROTOZOA Class Hexactinellida Order Amphidiscophora (Miss-Ree) Class Rhizopodea Order Hexactinosida (MTrias-Rec) Order Foraminiferida* Order Lyssacinosida (LCamb-Rec) Suborder Allogromiina (UCamb-Ree) Order Lychniscosida (UTrias-Rec) Suborder Textulariina (LCamb-Ree) Class Demospongia Suborder Fusulinina (Ord-Perm) Order Monaxonida (MCamb-Ree) Suborder Miliolina (Sil-Ree) Order Lithistida -
Geological Setting, Geochemistry and Genesis of the Sepon Gold and Copper Deposits, Laos
Geological setting, geochemistry and genesis of the Sepon gold and copper deposits, Laos by Paul W. Cromie B.Sc. (Hons.), M.Sc. (Econ. Geol.) A thesis submitted in fulfilment of the requirements for the degree of Doctor of Philosophy CODES ARC Centre of Excellence in Ore Deposits University of Tasmania (UTAS), Australia June 2010 ABSTRACT This study documents the geology, mineralogy, geochronology and geochemistry of the Sepon Mineral District (SMD) gold and copper deposits. The SMD is located in the Sepon Basin along the Truong Son Fold Belt on the NE margins of the Indochina Terrane in south-eastern Laos. The geology of the SMD is dominated by Ordovician, Silurian and Devonian-aged continental fluvial and shallow to deep marine sedimentary rocks that were deposited in a half graben basin. Intrusion of rhyodacite porphyry (RDP) mainly occurred along pre-existing faults during the Early Permian, constrained by U-Pb dating of zircons to between 2806 and 2977 Ma. Three main hypogene mineralisation styles are recognised in the SMD, comprising distal sedimentary-rock hosted gold (SHGD), proximal skarn (Cu+Au) and central porphyry (Cu-Mo). Exploration programs in the SMD conducted by CRA/RioTinto (1993-1999), Oxiana Limited/OZ Minerals Limited (2000-2008) resulted in the discovery of a mineral district containing resources of 83 Mt @ 1.8 g/t Au for 4.75 million ounces of gold in seven separate but adjacent SHGD, and supergene copper at three deposits, namely the Khanong (27 Mt @ 4.3 % Cu), Thengkham North (11.4 Mt @ 2.7 % Cu) and Thengkham South (9.8 Mt @ 2.3 % Cu) deposits. -
NI 43-101 TECHNICAL REPORT on the Saksrithai Property in Nakhon
1 NI 43-101 TECHNICAL REPORT On the Saksrithai Property in Nakhon Ratchasima Provence Kingdom of Thailand Latitude 15°18'41" Longitude 101°54'5” For Vatic Ventures Corp. 1008 Homer St Vancouver, British Columbia V6B 2X1 Canada Prepared By Derrick Strickland, P. Geo. December 21, 2017 Saksrithai Property NI-43-101 2 Table of Contents 1 Summary .................................................................................................................................... 3 2 INTRODUCTION .......................................................................................................................... 4 2.1 Units and Measurements ........................................................................................................ 5 3 RELIANCE ON OTHER EXPERTS .................................................................................................... 6 4 PROPERTY DESCRIPTION AND LOCATION .................................................................................... 6 5 ACCESSIBILITY, CLIMATE, PHYSIOGRAPHY, LOCAL RESOURCES, AND INFRASTRUCTURE............... 9 6 HISTORY.................................................................................................................................... 10 7 GEOLOGICAL SETTING AND MINERALIZATION ........................................................................... 13 7.1 Geology ................................................................................................................................ 13 7.2 Subsurface Geology .............................................................................................................