Pacific-Panthalassic Reconstructions
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Massive Basalt Flows on the Southern Flank of Tamu Massif, Shatsky Rise: a Reappraisal of ODP Site 1213 Basement Units1 A.A.P
Sager, W.W., Sano, T., Geldmacher, J., and the Expedition 324 Scientists Proceedings of the Integrated Ocean Drilling Program, Volume 324 Massive basalt flows on the southern flank of Tamu Massif, Shatsky Rise: a reappraisal of ODP Site 1213 basement units1 A.A.P. Koppers,2 T. Sano, 3 J.H. Natland,3 M. Widdowson,3 R. Almeev,3 A.R. Greene,3 D.T. Murphy,3 A. Delacour,3 M. Miyoshi,3 K. Shimizu,3 S. Li,3 N. Hirano,3 J. Geldmacher,3 and the Expedition 324 Scientists3 Chapter contents Abstract Abstract . 1 Drilling during Ocean Drilling Program Leg 198 at Site 1213 re- covered three massive basalt units (8–15 m thick) from the south- Introduction . 1 ern flank of Tamu Massif at Shatsky Rise. Originally, these igneous Volcanology and igneous petrology of Site 1213. 2 units were interpreted to represent three diabase sills. During In- Interpretation and conclusions. 5 tegrated Ocean Drilling Program Expedition 324, this core was re- Acknowledgments. 6 described leading to the new conclusion that these diabase units References . 6 represent three submarine massive basalt flows. These massive Figures . 8 submarine flows were probably emplaced as inflated compound Table . 20 sheet flows during eruptions similar to those in large oceanic pla- teaus and continental flood basalts. Introduction The main objective of Integrated Ocean Drilling Program (IODP) Expedition 324 was to test competing mantle plume and plate tectonic models for ocean plateau formation at Shatsky Rise (Fig. F1). In these tests, determining the timing, duration, and source of volcanism at Shatsky Rise is of pivotal importance to under- stand the origin of this oceanic plateau. -
Scientists Confirm Existence of Largest Single Volcano on Earth (Update) 5 September 2013
Scientists confirm existence of largest single volcano on Earth (Update) 5 September 2013 Tamu Massif did indeed erupt from a single source near the center. "Tamu Massif is the biggest single shield volcano ever discovered on Earth," Sager said. "There may be larger volcanoes, because there are bigger igneous features out there such as the Ontong Java Plateau, but we don't know if these features are one volcano or complexes of volcanoes." MCS re?ection Line A–B, across the axis of Tamu Massif. Credit: Nature A University of Houston (UH) professor led a team of scientists to uncover the largest single volcano yet documented on Earth. Covering an area roughly equivalent to the British Isles or the state of New Mexico, this volcano, dubbed the Tamu Massif, is nearly as big as the giant volcanoes of Mars, placing it among the largest in the Solar System. William Sager, a professor in the Department of Earth and Atmospheric Sciences at UH, first began studying the volcano about 20 years ago at Texas A&M's College of Geosciences. Sager and his team's findings appear in the Sept. 8 issue of Nature Geoscience, the monthly multi-disciplinary journal reflecting disciplines within the geosciences. Located about 1,000 miles east of Japan, Tamu Massif is the largest feature of Shatsky Rise, an underwater mountain range formed 130 to 145 million years ago by the eruption of several underwater volcanoes. Until now, it was unclear whether Tamu Massif was a single volcano, or a IODP technician Margaret Hastedt labels pieces of core composite of many eruption points. -
Marinegeology
_ I\_AGcO--',/_::,5 207247 Reprinted from /,v --,-/S--c/?-. MARINEGEOLOGY INTERNATIONAL JOURNAL OF MARINE GEOLOGY, GEOCHEMISTRY AND GEOPHYSICS Marine Geology 138 (1997) 273 301 Characteristics of seamounts near Hawaii as viewed by GLORIA Nathan T. Bridges Department of Geoscienees, University of Massachusetts, Amherst, MA 01003, USA Received 8 March 1996; accepted 19 November 1996 ELSEVIER ..... rZ MARINE QEOLOQY Editors-in-Chief For Europe, Africa and the Near East: H. Chamley, Universit(_ des Sciences et Techniques de Lille-Artois, S(_dimentologie et G_ochimie, B.P. 36, 59655 Villeneuve d'Ascq, France Tel.: +33-03 20 43 41 30 For the Americas, Pacific and Far East: M.A. Arthur, Department of Geosciences, The Pennsylvania State University, 503 Deike Building, University Park, PA 16802-2714, U.S.A. Tel.: + 1-814-865-6711; Fax: + 1-814-865-3191; E-mail: [email protected] Editorial Board R. Batiza, Honolulu, Hawaii, USA D. Jongsma, O'Connor, A.C.T., D.A. Ross, Woods Hole, Mass., USA W. Berger, La Jolla, Calif., USA Australia W.F. Ruddiman, Charlottesville, Va., USA A.H. Bouma, Baton Rouge, La., USA A.E.S. Kemp, Southampton, UK A.D. Short, Sydney, NSW, Australia A.J. Bowen, Halifax, N.S., Canada N.H. Kenyon, Southampton, UK D.J. Stanley, Washington, D.C., USA L. Carter, Wellington, New Zealand E.M. Klein, Durham, N.C., USA P. Stoffers, Kiel, Germany J.R. Curray, La Jolla, Calif., USA H.J. Knebel, Woods Hole, Mass., USA A.H.B. Stride, Petersfield, UK P.J. Davies, Sydney, N.S.W., Australia S.A. -
32. Radiometric Ages of Basement Lavas Recovered at Loen, Wodejebato, Mit, and Takuyo-Daisan Guyots, Northwestern Pacific Ocean1
Haggerty, J.A., Premoli Silva, I., Rack, F., and McNutt, M.K. (Eds.), 1995 Proceedings of the Ocean Drilling Program, Scientific Results, Vol. 144 32. RADIOMETRIC AGES OF BASEMENT LAVAS RECOVERED AT LOEN, WODEJEBATO, MIT, AND TAKUYO-DAISAN GUYOTS, NORTHWESTERN PACIFIC OCEAN1 Malcolm S. Pringle2 and Robert A. Duncan3 ABSTRACT The best estimate for the age of the oldest volcanism recovered from the summits of Loen, Wodejebato, MIT, and Takuyo- Daisan guyots, northwestern Pacific Ocean, is 113, 83, 123, and 118 Ma, respectively. All of these sites originated in the central and western regions of the South Pacific Isotopic and Thermal Anomaly (SOPITA). The 113-Ma age for Loen Guyot is signifi- cantly different from the 76-Ma age of volcanism under the carbonate platform of its neighbor, the living Anewetak Atoll, and suggests that drowned guyot/living atoll seamount pairs may have no genetically significant relationship other than geographic proximity. Although all of the basalts recovered from the top of Wodejebato Guyot were erupted during polarity Chron 33R (ca. 79-85 Ma), both the occurrence of reworked Cenomanian calcareous nannofossils in one of the summit cores and the existence of a thick Cenomanian volcaniclastic sequence, including 94-Ma basaltic clasts, in the archipelagic apron indicate that there must have been a Cenomanian or older edifice beneath the drilled summit volcanics. AT MIT Guyot, two late-stage periods of volcanism can be recognized: late Aptian (ca. 115 Ma) phreatomagmatic eruptions through the existing volcanic and carbonate platform, and 120-Ma hawaiites seen both as exotic clasts in the 115-Ma tuffs and as lava flows at the top of the basement sequence. -
(2020) Pūhāhonu: Earth's Biggest and Hottest Shield Volcano. Earth And
Earth and Planetary Science Letters 542 (2020) 116296 Contents lists available at ScienceDirect Earth and Planetary Science Letters www.elsevier.com/locate/epsl Puh¯ ahonu:¯ Earth’s biggest and hottest shield volcano ∗ Michael O. Garcia a, , Jonathan P. Tree a, Paul Wessel a, John R. Smith b a Department of Earth Sciences, University of Hawai‘i at Manoa,¯ Honolulu, HI 96822, USA b Department of Oceanography, University of Hawai‘i at Manoa,¯ Honolulu, HI 96822, USA a r t i c l e i n f o a b s t r a c t Article history: New bathymetric and gravity mapping, refined volume calculations and petrologic analyses show that Received 22 November 2019 the Hawaiian volcano Puh¯ ahonu¯ is the largest and hottest shield volcano on Earth. This ∼12.5-14.1 Ma Received in revised form 5 April 2020 volcano in the northwest Hawaiian Ridge (NWHR) is twice the size of Mauna Loa volcano (148 ± 29 vs. Accepted 18 April 2020 3 3 74.0 × 10 km ), which was assumed to be not only the largest Hawaiian volcano but also the largest Available online xxxx known shield volcano. We considered four testable mechanisms to increase magma production, including Editor: R. Dasgupta 1) thinner lithosphere, 2) slower propagation rate, 3) more fertile source, and 4) hotter mantle. The first Keywords: three of these have been ruled out. The lithosphere was old (∼88 Myrs) when Puh¯ ahonu¯ was formed, Hawaii and thus, too thick and cold to allow for greater extents of partial melting. The propagation rate was volume relatively fast when it erupted (87 km/Myr), so this is another unlikely reason. -
Geochemistry and Age of Shatsky, Hess, and Ojin Rise Seamounts: Implications for a Connection Between the Shatsky and Hess Rises
Accepted Manuscript Geochemistry and Age of Shatsky, Hess, and Ojin Rise seamounts: Implications for a connection between the Shatsky and Hess Rises Maria Luisa G. Tejada, Jörg Geldmacher, Folkmar Hauff, Daniel Heaton, Anthony A.P. Koppers, Dieter Garbe-Schönberg, Kaj Hoernle, Ken Heydolph, William W. Sager PII: S0016-7037(16)30165-X DOI: http://dx.doi.org/10.1016/j.gca.2016.04.006 Reference: GCA 9701 To appear in: Geochimica et Cosmochimica Acta Received Date: 4 September 2015 Accepted Date: 1 April 2016 Please cite this article as: Tejada, M.L.G., Geldmacher, J., Hauff, F., Heaton, D., Koppers, A.A.P., Garbe- Schönberg, D., Hoernle, K., Heydolph, K., Sager, W.W., Geochemistry and Age of Shatsky, Hess, and Ojin Rise seamounts: Implications for a connection between the Shatsky and Hess Rises, Geochimica et Cosmochimica Acta (2016), doi: http://dx.doi.org/10.1016/j.gca.2016.04.006 This is a PDF file of an unedited manuscript that has been accepted for publication. As a service to our customers we are providing this early version of the manuscript. The manuscript will undergo copyediting, typesetting, and review of the resulting proof before it is published in its final form. Please note that during the production process errors may be discovered which could affect the content, and all legal disclaimers that apply to the journal pertain. 1 Geochemistry and Age of Shatsky, Hess, and Ojin Rise seamounts: Implications 2 for a connection between the Shatsky and Hess Rises 3 Maria Luisa G. Tejada a,b*, Jörg Geldmacher c, Folkmar Hauff c, Daniel Heaton d, Anthony A. -
Geomorphometric Descriptions of Archipelagic Aprons Off the Southern Flanks of French Frigate Shoals and Necker Island Edifices, Northwest Hawaiian Ridge
Geomorphometric descriptions of archipelagic aprons off the southern flanks of French Frigate Shoals and Necker Island edifices, Northwest Hawaiian Ridge James V. Gardner†, Brian R. Calder†, and Andrew A. Armstrong† Center for Coastal and Ocean Mapping–Joint Hydrographic Center, 24 Colovos Road, University of New Hampshire, Durham, New Hampshire 03824, USA ABSTRACT landslides are more recent, perhaps even Vogt and Smoot, 1984; Smoot, 1985), or mesh Quaternary in age. The presence of a chute- grids (e.g., Taylor et al., 1975, 1980; Smoot, This study describes the geomorphometries like feature on the mid-flank of the French 1982, 1983a, 1983b, 1985). Recently, studies of archipelagic aprons on the southern flanks Frigate Shoals edifice appears to be the result have utilized modern multibeam data (e.g., De- of the French Frigate Shoals and Necker Is- of rejuvenated volcanism that occurred long plus et al., 2001; Masson et al., 2002; Mitchell land edifices on the central Northwest Hawai- after the initial volcanism ceased to build the et al., 2002; Bohannon and Gardner, 2004; Silver ian Ridge that are hotspot volcanoes that have edifice. et al., 2009; Casalbore et al., 2010; Montanaro been dormant for 10–11 m.y. The archipe- and Beget, 2011; Watt et al., 2012b, 2014; Saint- lagic aprons are related to erosional headwall INTRODUCTION Ange et al., 2013; Ramalho et al., 2015; Watson scarps and gullies on landslide surfaces but et al., 2017; Clare et al., 2018; Counts et al., also include downslope gravitational features Archipelagic aprons are submarine landslide 2018; Pope et al., 2018; Quartau et al., 2018; that include slides, debris avalanches, bed- complexes composed of erosion and deposition- Santos et al., 2019; Casalbore et al., 2020) to form fields, and outrunners. -
Ages of Seamounts, Islands and Plateaus on the Pacific Plate Version 2.1 - 15 May 2004
Ages of seamounts, islands and plateaus on the Pacific plate version 2.1 - 15 May 2004 Valérie Clouard(1) and Alain Bonneville(2) [email protected] [email protected] (1) Departamento de Geofisica - U. de Chile Blanco Encalada 2002 / Casilla 2777 / Santiago / Chile Tel. : +56 2 678 42 96 / Fax: +56 2 696 86 86 (2) Lab. Géosciences Marines / Institut de Physique du Globe / CNRS 4, Place Jussieu/ 75252 Paris Cedex 05 / France Tel.:+33 1 44 27 68 94 / Fax: +33 1 44 27 99 69 This report presents a compilation of reliable dating of seamounts and islands of the Pacific plate (1300 samples). Paleomagnetic ages obtained from seamount magnetism have not been considered. We also do not consider foraminifers ages which only give minimum ages of seamounts. Only radiometric ages are thus considered, and Ar/Ar ages are preferred over K/Ar, when both exist at the same place. The following table presents the results of this compilation with the references of the selected data. An average age (as used in [1] and [2]) is proposed when several ages have been determined for the same volcanic stage, in this case the geographical coordinates are given only once on the line of the average age. When several volcanic stages exist for a same seamount or island, their ages are also presented with the same rule as above. NB: an ASCII file (ages_pacific_v2.1.dat) with only average ages and geographical coordinates is also available for plotting purposes. Averag Average Name (island, Long. E Latitude Age Error Island or seamount e age error seamount, plateau or Method Ref. -
Okeanos Explorer ROV Dive Summary
Okeanos Explorer ROV Dive Summary Dive Information General Location General Area Descriptor US EEZ around Hawaii, South of Musicians / North of Hawaiian Islands Site Name Mendelsohn Seamount Science Team Leads John R. Smith/Meagan Putts Expedition Coordinator Kasey Cantwell ROV Dive Supervisor Karl McLetchie Mapping Lead Mike White ROV Dive Name Cruise EX1708 Leg - Dive Number DIVE19 Equipment Deployed ROV Deep Discoverer Camera Platform Seirios ROV Measurements CTD Depth Altitude Scanning Sonar USBL Position Heading Pitch Roll HD Camera 1 HD Camera 2 Low Res Cam 1 Low Res Cam 2 Low Res Cam 3 Low Res Cam 4 Low Res Cam 5 Equipment Malfunctions DO sensor?? Dive Summary: EX1708_DIVE19 ^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^ In Water: 2017-09-25T18:34:52.519000 25°, 09.569' N ; 161°, 38.672' W Out Water: 2017-09-26T01:05:33.440000 25°, 09.614' N ; 161°, 38.670' W ROV Dive Summary Off Bottom: 2017-09-26T00:06:57.047000 (from processed ROV 25°, 09.651' N ; 161°, 38.877' W data) On Bottom: 2017-09-25T19:37:17.885000 25°, 09.632' N ; 161°, 38.635' W Dive duration: 6:30:40 Bottom Time: 4:29:39 Max. depth: 1795.8 m Special Notes Name Email Affiliation Asako Planetary Exploration Research Matsumoto [email protected] Center, Chiba Institute of Technology Bruce NOAA NMFS Pacific Islands Fisheries Mundy [email protected] Science Center Christopher Scientists Involved Kelley [email protected] University of Hawaii (please provide name, Christopher Dept. Invertebrate Zoology, NMNH location, affiliation, Mah [email protected] Smithsonian -
Okeanos Explorer ROV Dive Summary
Okeanos Explorer ROV Dive Summary Dive Information General Location General Area Musicians Seamounts Descriptor Site Name Liszt Seamount Science Team Leads John R. Smith/Meagan Putts Expedition Kasey Cantwell Coordinator ROV Dive Supervisor Karl McLetchie Mapping Lead Mike White ROV Dive Name Cruise EX1708 Leg - Dive Number DIVE14 Equipment Deployed ROV Deep Discoverer Camera Platform Seirios CTD Depth Altitude ROV Measurements Scanning Sonar USBL Position Heading Pitch Roll HD Camera 1 HD Camera 2 Low Res Cam 1 Low Res Cam 2 Low Res Cam 3 Low Res Cam 4 Low Res Cam 5 Equipment DO sensor?? Malfunctions Dive Summary: EX1708_DIVE14 ^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^ In Water: 2017-09-20T18:27:30.486000 28°, 57.610' N ; 162°, 04.405' W Out Water: 2017-09-21T02:32:27.343000 28°, 57.455' N ; 162°, 03.691' W ROV Dive Summary Off Bottom: 2017-09-21T01:16:51.240000 (from processed ROV 28°, 57.767' N ; 162°, 04.319' W data) On Bottom: 2017-09-20T19:57:03.855000 28°, 57.523' N ; 162°, 04.279' W Dive duration: 8:4:56 Bottom Time: 5:19:47 Max. depth: 2564.5 m Special Notes Name Email Affiliation Amanda Netburn [email protected] NOAA OER Planetary Exploration Research Center, Chiba Asako Matsumoto [email protected] Institute of Technology NOAA NMFS Pacific Islands Fisheries Science Bruce Mundy [email protected] Center Scientists Involved (please provide name, Christopher Kelley [email protected] University of Hawaii location, affiliation, Dept. Invertebrate email) Zoology, NMNH Christopher Mah [email protected] Smithsonian -
EGU2018-5700, 2018 EGU General Assembly 2018 © Author(S) 2018
Geophysical Research Abstracts Vol. 20, EGU2018-5700, 2018 EGU General Assembly 2018 © Author(s) 2018. CC Attribution 4.0 license. Numerical modeling for the geodynamic formation of the Tamu Massif, the largest single volcano on Earth Jinchang Zhang (1), Min Ding (2), and Zhiyuan Zhou (1) (1) CAS Key Laboratory of Ocean and Marginal Sea Geology, South China Sea Institute of Oceanology, Chinese Academy of Sciences, Guangzhou, China ([email protected]), (2) School of Earth and Space Sciences, Peking University, Beijing, China The Western Pacific Ocean has most of the underwater volcanoes on Earth, and among them the Tamu Massif within the Shatsky Rise is proved to be the largest single volcano. By comparing thermo-mechanical models with gravity, topography, and seismic observations, we seek to address an important question: “How did this Earth’s largest volcano form by the interaction between a ridge-ridge-ridge triple junction and a mantle plume?” We focus on the following tasks: 1.set up three-dimensional thermo-mechanical models to simulate the ridge-plume interac- tion; 2.calculate the coupled mantle flow and temperature structure, and constrain the model parameters (spreading rates, plume size and depth, loading time, magma types, melting conditions, source temperature) using magnetic anomalies and magmatic geochemistry characteristics; 3.compute model-based magma supply and compare with crustal thickness and crustal volume estimates from seismic sounding and gravity observations; 4.invert for model parameters and find the control parameters on the volcano’s formation. It is creative to conduct a quantitative anal- ysis of the volcano’s formation, which can provide insights to the geodynamic evolution of thick oceanic crust. -
Structural and Morphologic Study of Shatsky Rise Oceanic
STRUCTURAL AND MORPHOLOGIC STUDY OF SHATSKY RISE OCEANIC PLATEAU IN THE NORTHWEST PACIFIC OCEAN FROM 2D MULTICHANNEL SEISMIC REFLECTION AND BATHYMETRY DATA AND IMPLICATIONS FOR OCEANIC PLATEAU EVOLUTION A Dissertation by JINCHANG ZHANG Submitted to the Office of Graduate and Professional Studies of Texas A&M University in partial fulfillment of the requirements for the degree of DOCTOR OF PHILOSOPHY Chair of Committee, William W. Sager Co-Chair of Committee, Zuosheng Yang Committee Members, Mitch W. Lyle Richard L. Gibson Head of Department, Debbie J. Thomas May 2014 Major Subject: Oceanography Copyright 2014 Jinchang Zhang ABSTRACT Shatsky Rise is one of the largest oceanic plateaus, a class of volcanic features whose formation is poorly understood. It is also a plateau that was formed near spreading ridges, but the connection is unclear. The geologic structure and morphology of Shatsky Rise oceanic plateau provides key observations that can help understand its formation. Deep penetrating 2D multichannel seismic (MCS) reflection profiles and high-resolution multi-beam sonar data were acquired over the southern half of Shatsky Rise on R/V Marcus G. Langseth during two cruises. The MCS profiles allow us to image Shatsky Rise's upper crustal structure and Moho structure with unprecedented detail, and the multi-beam bathymetry data allow us to produce an improved bathymetric map of the plateau. MCS profiles and bathymetry data show that two of the volcanic massifs within Shatsky Rise are immense central volcanoes. Tamu Massif, the largest (~450 × 650 km) and oldest (~145 Ma) volcano, is a single central volcano with rounded shape and shallow flank slopes (<0.5o-1.5o), characterized by lava flows emanating from the volcano center and extending hundreds of kilometers down smooth, shallow flanks to the surrounding seafloor.