Solo Sub Dive Is Deepest Ever
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Ocean Trench
R E S O U R C E L I B R A R Y E N C Y C L O P E D I C E N T RY Ocean trench Ocean trenches are long, narrow depressions on the seafloor. These chasms are the deepest parts of the ocean—and some of the deepest natural spots on Earth. G R A D E S 5 - 12+ S U B J E C T S Earth Science, Geology, Geography, Physical Geography C O N T E N T S 11 Images, 1 Video, 2 Links For the complete encyclopedic entry with media resources, visit: http://www.nationalgeographic.org/encyclopedia/ocean-trench/ Ocean trenches are long, narrow depressions on the seafloor. These chasms are the deepest parts of the ocean—and some of the deepest natural spots on Earth. Ocean trenches are found in every ocean basin on the planet, although the deepest ocean trenches ring the Pacific as part of the so-called “Ring of Fire” that also includes active volcanoes and earthquake zones. Ocean trenches are a result of tectonic activity, which describes the movement of the Earth’s lithosphere. In particular, ocean trenches are a feature of convergent plate boundaries, where two or more tectonic plates meet. At many convergent plate boundaries, dense lithosphere melts or slides beneath less-dense lithosphere in a process called subduction, creating a trench. Ocean trenches occupy the deepest layer of the ocean, the hadalpelagic zone. The intense pressure, lack of sunlight, and frigid temperatures of the hadalpelagic zone make ocean trenches some of the most unique habitats on Earth. -
Mapping the Ocean Floor Using the Hess Model Background Information Before World War II, Not Much Was Known About the Ocean Floor
WLHS/Marine Biology/Oppelt Name ________________________ Mapping the Ocean Floor Using the Hess Model Background Information Before World War II, not much was known about the ocean floor. The development of sonar during the war made more detailed maps of the ocean floor possible. Harry Hammond Hess, a geologist from Princeton University, was the captain of the assault transport vessel Cape Johnson. While stationed in the Pacific Ocean during World War II, Hess used the echo location (sonar) capabilities of this ship to collect data about the ocean floor. He later used this data to construct map of the ocean floor. He later used this information to construct a map of the ocean floor that led him to develop the hypothesis of the sea floor spreading. Echo location works by sending a signal out, called a ping, from a ship. That sound bounces off the ocean floor and is reflected back to the ship. By timing how long it takes to hear the echo of the sound, scientists can determine how far it is to the bottom. To determine the distance to the ocean floor, the time of the echo and the speed of sound in ocean water (1500 meters per second) must be determined. For example, if a ship sends out a ping that is reflected back in 1.34 seconds, the ping took 0.67 seconds to go down and 0.67 seconds to reflect back (1.34 sec ÷ 2 = 0.67 sec). To find the distance from the ship to the ocean floor, multiply 0.67 by the speed of sound in ocean water (1500 m/s). -
The Piccards and Their Submarines. Title
The Piccards and their Submarines Title 185 I first met Professor Auguste Piccard in the summer of 1936 in Santander, where the University of Madrid had organised a summer course for non-Spanish students. We were housed in an old royal castle on the rocky shore of the North Spanish coast with a delightful private bay for our daily swim. There I saw a very tall professor in a minute swimming trunk with astonishing spectacles, one of his unsung inventions. They are now commonplace, small attachable sun filters, to be turned up when not needed. I had never seen these before, although others may have used them earlier. Professor Piccard was already world famous for his balloon ascents into the strato- sphere, 15781 m in 1931, and in the following year to a height of 16940 m. I never saw him again, he died in 1962, aged 78 years. Many years later in Switzerland, I met his son Jacques Piccard. [See Title 1041 The record balloon ascents were successful because Piccard had constructed an air-tight spherical gondola of aluminium and an over-sized balloon, only slightly filled on the ground, but fully inflated at high altitudes. Based on the same principle, he invented later a submarine, consisting of a pressure resistant steel sphere, at- tached to a lighter-than-water gasoline filled ‘buoyant balloon’. This ‘allowed him, with heavy weights magnetically attached to his gondola, to descend to record depths of water. He called it a ‘bathyscaphe’ and named it The Trieste. His son Jacques, like his father a physicist-engineer, helped him in the design and construction of the bathyscaphe, and together they descended in The Trieste to a depth of 3099 m near the Island of Ponza in Italy. -
UNU/IOC/UNESCO Workshop on International Co-Operation in The
Intergovernmental Oceanographic Commission Workshop report No. 32 - supplement Papers submitted to the UNU/IOC/UNESCOWorkshop on International Co-operation in the Development of Marine Science and the Transfer of Techtïobgy in the context of the New Ocean Regime Paris, 27 September - 1 October 1982 The Summary Report of the UNU/IOC/Unesco Workshop on International Co-operation in the Development of Marine Science and the Transfer of Technology in the Context of the new Ocean Regime was issued as IOC Workshop Report No. 32. This Supplement contains the papers presented at the Workshop, J I CONTENTS page FOREWORD 1-2 PAPERS PRESENTED A General Eeview of the New Convention on the Law of 3 - 35 the Sea Having a Bearing on Marine Science and Its Application Alexander YANKOV International Cooperation in Marine Scientific Research 36 - 57 and in the Development and Transfer of Marine Science and Technology in the Convention of the Law of the Sea with Particular Reference to the Attention Paid to the knterests of Developing Countries Maria Eduarda GONÇALVES Convention of the Law of the Sea and the New International 58 - 72 Economic Order René Jean DUPUY' Creating Favourable Condit ions for the International 73 - 88 Cooperation for the Transfer of Marine Science and Technology in the Context of the New Ocean Regime Agustin AYALA-CASTANARES New Ocean Regime and Marine Scientific Research S9 - 113 Syed Zahoor QASIM Flow of Scientific Data and Information and the Transfer 114- 122 of Knowledge to Developing Countries Geoffrey KESTEVEN Developing the Marine Scientific and Technological 130- 149 Capacity of States Inocencio RONQUILLO Ulf LIE Promoting Marine Scientific Research Centres and Networks 150 159 Sidney HOLT The IO1 Training Programme on the Management and 160 - 173 Conservation of Marine Resources: A Case Study Elizabeth MANN BORGESE LIST OF PARTICIPANTS 174 -177 -1- FOREWORD The Convention adopted by the Third United Nations Conference on the Law of the Sea (UNCLOS) defines a new international regime inter alia for use of the ocean and its resources. -
Sterns Lebensdaten Und Chronologie Seines Wirkens
Sterns Lebensdaten und Chronologie seines Wirkens Diese Chronologie von Otto Sterns Wirken basiert auf folgenden Quellen: 1. Otto Sterns selbst verfassten Lebensläufen, 2. Sterns Briefen und Sterns Publikationen, 3. Sterns Reisepässen 4. Sterns Züricher Interview 1961 5. Dokumenten der Hochschularchive (17.2.1888 bis 17.8.1969) 1888 Geb. 17.2.1888 als Otto Stern in Sohrau/Oberschlesien In allen Lebensläufen und Dokumenten findet man immer nur den VornamenOt- to. Im polizeilichen Führungszeugnis ausgestellt am 12.7.1912 vom königlichen Polizeipräsidium Abt. IV in Breslau wird bei Stern ebenfalls nur der Vorname Otto erwähnt. Nur im Emeritierungsdokument des Carnegie Institutes of Tech- nology wird ein zweiter Vorname Otto M. Stern erwähnt. Vater: Mühlenbesitzer Oskar Stern (*1850–1919) und Mutter Eugenie Stern geb. Rosenthal (*1863–1907) Nach Angabe von Diana Templeton-Killan, der Enkeltochter von Berta Kamm und somit Großnichte von Otto Stern (E-Mail vom 3.12.2015 an Horst Schmidt- Böcking) war Ottos Großvater Abraham Stern. Abraham hatte 5 Kinder mit seiner ersten Frau Nanni Freund. Nanni starb kurz nach der Geburt des fünften Kindes. Bald danach heiratete Abraham Berta Ben- der, mit der er 6 weitere Kinder hatte. Ottos Vater Oskar war das dritte Kind von Berta. Abraham und Nannis erstes Kind war Heinrich Stern (1833–1908). Heinrich hatte 4 Kinder. Das erste Kind war Richard Stern (1865–1911), der Toni Asch © Springer-Verlag GmbH Deutschland 2018 325 H. Schmidt-Böcking, A. Templeton, W. Trageser (Hrsg.), Otto Sterns gesammelte Briefe – Band 1, https://doi.org/10.1007/978-3-662-55735-8 326 Sterns Lebensdaten und Chronologie seines Wirkens heiratete. -
The Next Generation of Ocean Exploration. Kelly Walsh Repeats Father’S Historic Dive, 60 Years Later, on Father’S Day Weekend
From father to son; the next generation of ocean exploration. Kelly Walsh repeats father’s historic dive, 60 years later, on Father’s Day weekend DSSV Pressure Drop. Challenger Deep, Mariana Trench 200miles SW of Guam. June 20th, 2020 – Kelly Walsh, 52, today completed a historic dive to approximately 10,925m in the Challenger Deep. The dive location was the Western Pool, the same area that was visited by Kelly’s father, Captain Don Walsh, USN (Ret), PhD, who was the pilot of the bathyscaph ‘Trieste’ during the first dive to the Challenger Deep in 1960. Mr. Walsh’s 12- hour dive, coordinated by EYOS Expeditions, was undertaken aboard the deep-sea vehicle Triton 36000/2 ‘Limiting Factor” piloted by the owner of the vehicle Victor Vescovo, a Dallas, Texas based businessman and explorer. The expedition to the Challenger Deep is a joint venture by Caladan Oceanic, Triton Submarines and EYOS Expeditions. Mr. Vescovo and his team made headlines last year by completing a circumnavigation of the globe that enabled Mr. Vescovo to become the first person to dive to the deepest point of each of the worlds five oceans. The dives by father and son connect a circle of exploration history that spans 60 years. “It was a hugely emotional journey for me,” said Kelly Walsh aboard DSSV Pressure Drop, the expedition’s mothership. “I have been immersed in the story of Dad’s dive since I was born-- people find it fascinating. It has taken 60 years but thanks to EYOS Expeditions and Victor Vescovo we have now taken this quantum leap forward in our ability to explore the deep ocean. -
Philippine Sea Plate Inception, Evolution, and Consumption with Special Emphasis on the Early Stages of Izu-Bonin-Mariana Subduction Lallemand
Progress in Earth and Planetary Science Philippine Sea Plate inception, evolution, and consumption with special emphasis on the early stages of Izu-Bonin-Mariana subduction Lallemand Lallemand Progress in Earth and Planetary Science (2016) 3:15 DOI 10.1186/s40645-016-0085-6 Lallemand Progress in Earth and Planetary Science (2016) 3:15 Progress in Earth and DOI 10.1186/s40645-016-0085-6 Planetary Science REVIEW Open Access Philippine Sea Plate inception, evolution, and consumption with special emphasis on the early stages of Izu-Bonin-Mariana subduction Serge Lallemand1,2 Abstract We compiled the most relevant data acquired throughout the Philippine Sea Plate (PSP) from the early expeditions to the most recent. We also analyzed the various explanatory models in light of this updated dataset. The following main conclusions are discussed in this study. (1) The Izanagi slab detachment beneath the East Asia margin around 60–55 Ma likely triggered the Oki-Daito plume occurrence, Mesozoic proto-PSP splitting, shortening and then failure across the paleo-transform boundary between the proto-PSP and the Pacific Plate, Izu-Bonin-Mariana subduction initiation and ultimately PSP inception. (2) The initial splitting phase of the composite proto-PSP under the plume influence at ∼54–48 Ma led to the formation of the long-lived West Philippine Basin and short-lived oceanic basins, part of whose crust has been ambiguously called “fore-arc basalts” (FABs). (3) Shortening across the paleo-transform boundary evolved into thrusting within the Pacific Plate at ∼52–50 Ma, allowing it to subduct beneath the newly formed PSP, which was composed of an alternance of thick Mesozoic terranes and thin oceanic lithosphere. -
Microbiology of Seamounts Is Still in Its Infancy
or collective redistirbution of any portion of this article by photocopy machine, reposting, or other means is permitted only with the approval of The approval portionthe ofwith any articlepermitted only photocopy by is of machine, reposting, this means or collective or other redistirbution This article has This been published in MOUNTAINS IN THE SEA Oceanography MICROBIOLOGY journal of The 23, Number 1, a quarterly , Volume OF SEAMOUNTS Common Patterns Observed in Community Structure O ceanography ceanography S BY DAVID EmERSON AND CRAIG L. MOYER ociety. © 2010 by The 2010 by O ceanography ceanography O ceanography ceanography ABSTRACT. Much interest has been generated by the discoveries of biodiversity InTRODUCTION S ociety. ociety. associated with seamounts. The volcanically active portion of these undersea Microbial life is remarkable for its resil- A mountains hosts a remarkably diverse range of unusual microbial habitats, from ience to extremes of temperature, pH, article for use and research. this copy in teaching to granted ll rights reserved. is Permission S ociety. ociety. black smokers rich in sulfur to cooler, diffuse, iron-rich hydrothermal vents. As and pressure, as well its ability to persist S such, seamounts potentially represent hotspots of microbial diversity, yet our and thrive using an amazing number or Th e [email protected] to: correspondence all end understanding of the microbiology of seamounts is still in its infancy. Here, we of organic or inorganic food sources. discuss recent work on the detection of seamount microbial communities and the Nowhere are these traits more evident observation that specific community groups may be indicative of specific geochemical than in the deep ocean. -
Dives of the Bathyscaph Trieste, 1958-1963: Transcriptions of Sixty-One Dictabelt Recordings in the Robert Sinclair Dietz Papers, 1905-1994
Dives of the Bathyscaph Trieste, 1958-1963: Transcriptions of sixty-one dictabelt recordings in the Robert Sinclair Dietz Papers, 1905-1994 from Manuscript Collection MC28 Archives of the Scripps Institution of Oceanography University of California, San Diego La Jolla, California 92093-0219: September 2000 This transcription was made possible with support from the U.S. Naval Undersea Museum 2 TABLE OF CONTENTS INTRODUCTION ...........................................................................................................................4 CASSETTE TAPE 1 (Dietz Dictabelts #1-5) .................................................................................6 #1-5: The Big Dive to 37,800. Piccard dictating, n.d. CASSETTE TAPE 2 (Dietz Dictabelts #6-10) ..............................................................................21 #6: Comments on the Big Dive by Dr. R. Dietz to complete Piccard's description, n.d. #7: On Big Dive, J.P. #2, 4 Mar., n.d. #8: Dive to 37,000 ft., #1, 14 Jan 60 #9-10: Tape just before Big Dive from NGD first part has pieces from Rex and Drew, Jan. 1960 CASSETTE TAPE 3 (Dietz Dictabelts #11-14) ............................................................................30 #11-14: Dietz, n.d. CASSETTE TAPE 4 (Dietz Dictabelts #15-18) ............................................................................39 #15-16: Dive #61 J. Piccard and Dr. A. Rechnitzer, depth of 18,000 ft., Piccard dictating, n.d. #17-18: Dive #64, 24,000 ft., Piccard, n.d. CASSETTE TAPE 5 (Dietz Dictabelts #19-22) ............................................................................48 #19-20: Dive Log, n.d. #21: Dr. Dietz on the bathysonde, n.d. #22: from J. Piccard, 14 July 1960 CASSETTE TAPE 6 (Dietz Dictabelts #23-25) ............................................................................57 #23-25: Italian Dive, Dietz, Mar 8, n.d. CASSETTE TAPE 7 (Dietz Dictabelts #26-29) ............................................................................64 #26-28: Italian Dive, Dietz, n.d. -
Serpentine Volcanoes
2016 Deepwater Exploration of the Marianas Serpentine Volcanoes Focus Serpentine mud volcanoes Grade Level 9-12 (Earth Science) Focus Question What are serpentine mud volcanoes and what geological and chemical processes are involved with their formation? Learning Objectives • Students will describe serpentinization and explain its significance to deep-sea ecosystems. Materials q Copies of Mud Volcano Inquiry Guide, one copy for each student group Audio-Visual Materials q (Optional) Interactive whiteboard Teaching Time One or two 45-minute class periods Seating Arrangement Groups of two to four students Maximum Number of Students 30 Key Words Mariana Arc Serpentine Mud volcano Mariana Trench Serpentinization Peridotite Image captions/credits on Page 2. Tectonic plate 1 www.oceanexplorer.noaa.gov Serpentine Volcanoes - 2016 Grades 9-12 (Earth Science) Background Information NOTE: Explanations and procedures in this lesson are written at a level appropriate to professional educators. In presenting and discussing this material with students, educators may need to adapt the language and instructional approach to styles that are best suited to specific student groups. The Marina Trench is an oceanic trench in the western Pacific Ocean that is formed by the collision of two large pieces of the Earth’s crust known as tectonic plates. These plates are portions of the Earth’s outer crust (the lithosphere) about 5 km thick, as well as the upper 60 - 75 km of the underlying mantle. The plates move on a hot, flexible mantle layer called the asthenosphere, which is several hundred kilometers thick. The Pacific Ocean Basin lies on top of the Pacific Plate. To the east, new crust is formed by magma rising from deep within Images from Page 1 top to bottom: the Earth. -
History of the Harte Research Institute for Gulf of Mexico Studies at Texas A&M University–Corpus Christi John W
Gulf of Mexico Science Volume 28 Article 8 Number 1 Number 1/2 (Combined Issue) 2010 History of the Harte Research Institute for Gulf of Mexico Studies at Texas A&M University–Corpus Christi John W. Tunnell Jr. Texas A&M University, Corpus Christi DOI: 10.18785/goms.2801.08 Follow this and additional works at: https://aquila.usm.edu/goms Recommended Citation Tunnell, J. W. Jr. 2010. History of the Harte Research Institute for Gulf of Mexico Studies at Texas A&M University–Corpus Christi. Gulf of Mexico Science 28 (1). Retrieved from https://aquila.usm.edu/goms/vol28/iss1/8 This Article is brought to you for free and open access by The Aquila Digital Community. It has been accepted for inclusion in Gulf of Mexico Science by an authorized editor of The Aquila Digital Community. For more information, please contact [email protected]. Tunnell: History of the Harte Research Institute for Gulf of Mexico Studie Gulf of Mexico Science, 2010(1–2), pp. 56–70 History of the Harte Research Institute for Gulf of Mexico Studies at Texas A&M University–Corpus Christi JOHN W. TUNNELL,JR. n 19 Sep. 2000, Mr. Edward H. Harte try, and conservation, as well as all three countries O donated $46 million to establish a new surrounding the Gulf of Mexico: the United research institute at Texas A&M University– States, Mexico, and Cuba (Table 1). I was Corpus Christi (TAMU-CC) to focus on the Gulf appointed Associate Director in September of Mexico. Mr. Harte, philanthropist and former 2001, and that fall the new institute was officially owner of Harte-Hanks, Inc., and the Corpus named the Harte Research Institute for Gulf of Christi Caller-Times newspaper, worked with Dr. -
So, How Deep Is the Mariana Trench?
Marine Geodesy, 37:1–13, 2014 Copyright © Taylor & Francis Group, LLC ISSN: 0149-0419 print / 1521-060X online DOI: 10.1080/01490419.2013.837849 So, How Deep Is the Mariana Trench? JAMES V. GARDNER, ANDREW A. ARMSTRONG, BRIAN R. CALDER, AND JONATHAN BEAUDOIN Center for Coastal & Ocean Mapping-Joint Hydrographic Center, Chase Ocean Engineering Laboratory, University of New Hampshire, Durham, New Hampshire, USA HMS Challenger made the first sounding of Challenger Deep in 1875 of 8184 m. Many have since claimed depths deeper than Challenger’s 8184 m, but few have provided details of how the determination was made. In 2010, the Mariana Trench was mapped with a Kongsberg Maritime EM122 multibeam echosounder and recorded the deepest sounding of 10,984 ± 25 m (95%) at 11.329903◦N/142.199305◦E. The depth was determined with an update of the HGM uncertainty model combined with the Lomb- Scargle periodogram technique and a modal estimate of depth. Position uncertainty was determined from multiple DGPS receivers and a POS/MV motion sensor. Keywords multibeam bathymetry, Challenger Deep, Mariana Trench Introduction The quest to determine the deepest depth of Earth’s oceans has been ongoing since 1521 when Ferdinand Magellan made the first attempt with a few hundred meters of sounding line (Theberge 2008). Although the area Magellan measured is much deeper than a few hundred meters, Magellan concluded that the lack of feeling the bottom with the sounding line was evidence that he had located the deepest depth of the ocean. Three and a half centuries later, HMS Challenger sounded the Mariana Trench in an area that they initially called Swire Deep and determined on March 23, 1875, that the deepest depth was 8184 m (Murray 1895).