Exploring and Modeling the Magma–Hydrothermal Regime
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Age Progressive Volcanism in the New England Seamounts and the Opening of the Central Atlantic Ocean
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 89, NO. B12, PAGES 9980-9990, NOVEMBER 10, 1984 AGEPROGRESSIVE VOLCANISM IN THENEW ENGLAND SEAMOUNTS AND THE OPENING OF THE CENTRAL ATLANTIC OCEAN R. A. Duncan College of Oceanography, Oregon State University, Corvallis Abstract. Radiometric ages (K-Ar and •øAr- transient featur e•s that allow calculations of 39Ar methods) have been determined on dredged relative motions only. volcanic rocks from seven of the New England The possibility that plate motions may be Seamounts, a prominent northwest-southeast trend- recorded by lines of islands and seamounts in the ing volcanic lineament in the northwestern ocean basins is attractive in this regard. If, Atlantic Ocean. The •øAr-39Ar total fusion and as the Carey-Wilson-Morgan model [Carey, 1958; incren•ental heating ages show an increase in Wilson, 1963; Morgan, 19•1] proposes, sublitho- seamount construction age from southeast to spheric, thermal anomalies called hot spots are northwest that is consistent with northwestward active and fixed with respect to one another in motion of the North American plate over a New the earth's upper mantle, they would then consti- England hot spot between 103 and 82 Ma. A linear tute a reference frame for directly and precisely volcano migration rate of 4.7 cm/yr fits the measuring plate motions. Ancient longitudes as seamount age distribution. These ages fall well as latitudes would be determined from vol- Within a longer age progression from the Corner cano construction ages along the tracks left by Seamounts (70 to 75 Ma), at the eastern end of hot spots and, providing relative plate motions the New England Seamounts, to the youngest phase are also known, quantitative estimates of conver- of volcanism in the White Mountain Igneous gent plate motions can be calculated [Engebretson Province, New England (100 to 124 Ma). -
Hydrothermal Circulation Within the Endeavour Segment; Juan De Fuca Ridge
Hydrothermal Circulation within the Endeavour Segment; Juan de Fuca Ridge H. Paul Johnson1, Maurice A. Tivey2, Tor A. Bjorklund1, and Marie S. Salmi1 1School of Oceanography, University of Washington, Seattle, WA 98195-7940 2Department of Geology and Geophysics Woods Hole Oceanographic Institution Woods Hole, MA 02543 Correspondence should be addressed to HPJ, [email protected] 206-543-8474 Hydrothermal Circulation within the Endeavour Segment; Juan de Fuca Ridge Abstract Areas of the seafloor at mid-ocean ridges where hydrothermal vents discharge are easily recognized by the dramatic biological, physical and chemical processes that characterize such sites. Locations where seawater flows into the seafloor to recharge hydrothermal cells within the crustal reservoir are by contrast almost invisible, but can be indirectly identified by a systematic grid of conductive heat flow measurements. An array of conductive heat flow stations in the Endeavour axial valley of the Juan de Fuca Ridge has identified recharge zones that appear to represent a nested system of fluid circulation paths. At the scale of an axial rift valley, conductive heat flow data indicate a general cross-valley fluid flow, where seawater enters the shallow sub-surface crustal reservoir at the eastern wall of the Endeavour axial valley and undergoes a kilometer of horizontal transit beneath the valley floor, finally exiting as warm hydrothermal fluid discharge on the western valley bounding wall. Recharge zones also have been identified as located within an annular ring of very cold seafloor around the large Main Endeavour Hydrothermal Field, with seawater inflow occurring within faults that surround the fluid discharge sites. -
Three-Dimensional Models of Hydrothermal Circulation Through a Seamount Network on Fast-Spreading Crust ∗ Rachel M
Earth and Planetary Science Letters 501 (2018) 138–151 Contents lists available at ScienceDirect Earth and Planetary Science Letters www.elsevier.com/locate/epsl Three-dimensional models of hydrothermal circulation through a seamount network on fast-spreading crust ∗ Rachel M. Lauer a,b,c, , Andrew T. Fisher b,c, Dustin M. Winslow b,c,d a Department of Geoscience, University of Calgary, Calgary, Alberta, Canada b Earth and Planetary Sciences Department, University of California, Santa Cruz, 95064, USA c Center for Dark Energy Biosphere Investigations, University of California, Santa Cruz, 95064, USA d GrowthIntel, 25-27 Horsell Road, London N5 1XL, UK a r t i c l e i n f o a b s t r a c t Article history: We present results from three-dimensional, transient, fully coupled simulations of fluid and heat Received 25 February 2018 transport on a ridge flank in fast-spread ocean crust. The simulations quantify relationships between rates Received in revised form 17 July 2018 of fluid flow, the extent of advective heat extraction, the geometry of crustal aquifers and outcrops, and Accepted 14 August 2018 crustal hydrologic parameters, with the goal of simulating conditions similar to those seen on 18–24 M.y. Available online xxxx old seafloor of the Cocos plate, offshore Costa Rica. Extensive surveys of this region documented a Editor: M. Bickle 2 ∼14,500 km area of the seafloor with heat flux values that are 10–35% of those predicted from Keywords: conductive cooling models, and identified basement outcrops that serve as pathways for hydrothermal hydrothermal circulation circulation via recharge of bottom water and discharge of cool hydrothermal fluid. -
Chapter 2 Alaska’S Igneous Rocks
Chapter 2 Alaska’s Igneous Rocks Resources • Alaska Department of Natural Resources, 2010, Division of Geological and Geophysical Surveys, Alaska Geologic Materials Center website, accessed May 27, 2010, at http://www.dggs.dnr.state.ak.us/?link=gmc_overview&menu_link=gmc. • Alaska Resource Education: Alaska Resource Education website, accessed February 22, 2011, at http://www.akresource.org/. • Barton, K.E., Howell, D.G., and Vigil, J.F., 2003, The North America tapestry of time and terrain: U.S. Geological Survey Geologic Investigations Series I-2781, 1 sheet. (Also available at http://pubs.usgs.gov/imap/i2781/.) • Danaher, Hugh, 2006, Mineral identification project website, accessed May 27, 2010, at http://www.fremontica.com/minerals/. • Digital Library for Earth System Education, [n.d.], Find a resource—Bowens reaction series: Digital Library for Earth System Education website, accessed June 10, 2010, at http://www.dlese.org/library/query.do?q=Bowens%20reaction%20series&s=0. • Edwards, L.E., and Pojeta, J., Jr., 1997, Fossils, rocks, and time: U.S. Geological Survey website. (Available at http://pubs.usgs.gov/gip/fossils/contents.html.) • Garden Buildings Direct, 2010, Rocks and minerals: Garden Buildings Direct website, accessed June 4, 2010, at http://www.gardenbuildingsdirect.co.uk/Article/rocks-and- minerals. • Illinois State Museum, 2003, Geology online–GeoGallery: Illinois State Museum Society database, accessed May 27, 2010 at http://geologyonline.museum.state.il.us/geogallery/. • Knecht, Elizebeth, designer, Pearson, R.W., and Hermans, Majorie, eds., 1998, Alaska in maps—A thematic atlas: Alaska Geographic Society, 100 p. Lillie, R.J., 2005, Parks and plates—The geology of our National parks, monuments, and seashores: New York, W.W. -
Volcanism in a Plate Tectonics Perspective
Appendix I Volcanism in a Plate Tectonics Perspective 1 APPENDIX I VOLCANISM IN A PLATE TECTONICS PERSPECTIVE Contributed by Tom Sisson Volcanoes and Earth’s Interior Structure (See Surrounded by Volcanoes and Magma Mash for relevant illustrations and activities.) To understand how volcanoes form, it is necessary to know something about the inner structure and dynamics of the Earth. The speed at which earthquake waves travel indicates that Earth contains a dense core composed chiefly of iron. The inner part of the core is solid metal, but the outer part is melted and can flow. Circulation (movement) of the liquid outer core probably creates Earth’s magnetic field that causes compass needles to point north and helps some animals migrate. The outer core is surrounded by hot, dense rock known as the mantle. Although the mantle is nearly everywhere completely solid, the rock is hot enough that it is soft and pliable. It flows very slowly, at speeds of inches-to-feet each year, in much the same way as solid ice flows in a glacier. Earth’s interior is hot both because of heat left over from its formation 4.56 billion years ago by meteorites crashing together (accreting due to gravity), and because of traces of natural radioactivity in rocks. As radioactive elements break down into other elements, they release heat, which warms the inside of the Earth. The outermost part of the solid Earth is the crust, which is colder and about ten percent less dense than the mantle, both because it has a different chemical composition and because of lower pressures that favor low-density minerals. -
Lunar Volcanism Notes (Adapted From
Lunar Volcanism Notes (adapted from http://www.asi.org/adb/m/04/02/volcanic-activity.html) The volcanic rocks produced on the moon are basalts. Basalts are common products of mantle partial melting on the terrestrial planets. This is mainly due to broad similarity of their mantle compositions. For partial melting to occur on the moon, temperatures greater than 1100°C at depths of about 200 km are required. The bulk eruption styles appear to be in the form of lava flows. There is also widespread evidence of fire-fountaining forming pyroclastic deposits (typically glass beads). Sinuous Rilles These are meandering channels which commonly begin at craters. They end by fading into the mare surface, or into chains of elongated pits. Sizes range from a few tens of meters to 3km in width. Lengths range up to 300km in length. Channels are U-shaped or V-shaped, but fallen debris (from the walls, or crater ejecta) have generally modified their cross-sections. Most sinuous rilles are near the mare basin edges, although they are found in most mare deposits. Apollo 15 confirmed the theory that sinuous rilles were analogous to lava channels and collapsed lava tubes. Lunar rilles are much larger than their terrestrial equivalents. This is thought to be due to a combination of reduced gravity, high melt temperature, low viscosity, and high extrusion rates. Domes (Shield Volcanoes) Domes are defined as broad, shallow landforms. These are convex, circular to oval in shape, and occur on the mare basins. Eighty low domes (2-3 degree slopes) have been mapped (Guest & Murray, 1976). -
Hawaiian Volcanoes: from Source to Surface Site Waikolao, Hawaii 20 - 24 August 2012
AGU Chapman Conference on Hawaiian Volcanoes: From Source to Surface Site Waikolao, Hawaii 20 - 24 August 2012 Conveners Michael Poland, USGS – Hawaiian Volcano Observatory, USA Paul Okubo, USGS – Hawaiian Volcano Observatory, USA Ken Hon, University of Hawai'i at Hilo, USA Program Committee Rebecca Carey, University of California, Berkeley, USA Simon Carn, Michigan Technological University, USA Valerie Cayol, Obs. de Physique du Globe de Clermont-Ferrand Helge Gonnermann, Rice University, USA Scott Rowland, SOEST, University of Hawai'i at M noa, USA Financial Support 2 AGU Chapman Conference on Hawaiian Volcanoes: From Source to Surface Site Meeting At A Glance Sunday, 19 August 2012 1600h – 1700h Welcome Reception 1700h – 1800h Introduction and Highlights of Kilauea’s Recent Eruption Activity Monday, 20 August 2012 0830h – 0900h Welcome and Logistics 0900h – 0945h Introduction – Hawaiian Volcano Observatory: Its First 100 Years of Advancing Volcanism 0945h – 1215h Magma Origin and Ascent I 1030h – 1045h Coffee Break 1215h – 1330h Lunch on Your Own 1330h – 1430h Magma Origin and Ascent II 1430h – 1445h Coffee Break 1445h – 1600h Magma Origin and Ascent Breakout Sessions I, II, III, IV, and V 1600h – 1645h Magma Origin and Ascent III 1645h – 1900h Poster Session Tuesday, 21 August 2012 0900h – 1215h Magma Storage and Island Evolution I 1215h – 1330h Lunch on Your Own 1330h – 1445h Magma Storage and Island Evolution II 1445h – 1600h Magma Storage and Island Evolution Breakout Sessions I, II, III, IV, and V 1600h – 1645h Magma Storage -
Magma Emplacement and Deformation in Rhyolitic Dykes: Insight Into Magmatic Outgassing
MAGMA EMPLACEMENT AND DEFORMATION IN RHYOLITIC DYKES: INSIGHT INTO MAGMATIC OUTGASSING Presented for the degree of Ph.D. by Ellen Marie McGowan MGeol (The University of Leicester, 2011) Initial submission January 2016 Final submission September 2016 Lancaster Environment Centre, Lancaster University Declaration I, Ellen Marie McGowan, hereby declare that the content of this thesis is the result of my own work, and that no part of the work has been submitted in substantially the same form for the award of a higher degree elsewhere. This thesis is dedicated to Nan-Nar, who sadly passed away in 2015. Nan, you taught our family the importance and meaning of love, we love you. Abstract Exposed rhyolitic dykes at eroded volcanoes arguably provide in situ records of conduit processes during rhyolitic eruptions, thus bridging the gap between surface and sub-surface processes. This study involved micro- to macro-scale analysis of the textures and water content within shallow (emplacement depths <500 m) rhyolitic dykes at two Icelandic central volcanoes. It is demonstrated that dyke propagation commenced with the intrusion of gas- charged currents that were laden with particles, and that the distribution of intruded particles and degree of magmatic overpressure required for dyke propagation were governed by the country rock permeability and strength, with pre-existing fractures playing a pivotal governing role. During this stage of dyke evolution significant amounts of exsolved gas may have escaped. Furthermore, during later magma emplacement within the dyke interiors, particles that were intruded and deposited during the initial phase were sometimes preserved at the dyke margins, forming dyke- marginal external tuffisite veins, which would have been capable of facilitating persistent outgassing during dyke growth. -
Multi-Stage Arc Magma Evolution Recorded by Apatite in Volcanic Rocks Chetan L
https://doi.org/10.1130/G46998.1 Manuscript received 6 February 2019 Revised manuscript received 11 November 2019 Manuscript accepted 5 December 2019 © 2020 The Authors. Gold Open Access: This paper is published under the terms of the CC-BY license. Published online 17 January 2020 Multi-stage arc magma evolution recorded by apatite in volcanic rocks Chetan L. Nathwani1,2, Matthew A. Loader2, Jamie J. Wilkinson2,1, Yannick Buret2, Robert H. Sievwright2 and Pete Hollings3 1 Department of Earth Science and Engineering, Imperial College London, Exhibition Road, South Kensington Campus, London SW7 2AZ, UK 2 London Centre for Ore Deposits and Exploration (LODE), Department of Earth Sciences, Natural History Museum, Cromwell Road, South Kensington, London SW7 5BD, UK 3 Department of Geology, Lakehead University, 955 Oliver Road, Thunder Bay, Ontario P7B 5E1, Canada ABSTRACT However, accessory minerals such as apatite are Protracted magma storage in the deep crust is a key stage in the formation of evolved, capable of capturing discrete periods of melt hydrous arc magmas that can result in explosive volcanism and the formation of economi- evolution during differentiation. For example, cally valuable magmatic-hydrothermal ore deposits. High magmatic water content in the apatite has been shown to record the Sr con- deep crust results in extensive amphibole ± garnet fractionation and the suppression of pla- tent of the melt at the time of its crystallization, gioclase crystallization as recorded by elevated Sr/Y ratios and high Eu (high Eu/Eu*) in the which has been used to reconstruct host-rock melt. Here, we use a novel approach to track the petrogenesis of arc magmas using apatite compositions in provenance studies (Jennings trace element chemistry in volcanic formations from the Cenozoic arc of central Chile. -
27. Chinook Trough Rifting and Hydrothermal Deposition at Sites 885 and 8861
Rea, D.K., Basov, I.A., Scholl, D.W., and Allan, J.F. (Eds.), 1995 Proceedings of the Ocean Drilling Program, Scientific Results, Vol. 145 27. CHINOOK TROUGH RIFTING AND HYDROTHERMAL DEPOSITION AT SITES 885 AND 8861 Gerald R. Dickens2 and Robert M. Owen2 ABSTRACT The Chinook Trough is a pronounced deep located in the central North Pacific Ocean that spans approximately 1500 km in a northeast-southwest direction. Geophysical and geomorphological considerations suggest that this feature is the southern litho- spheric scar marking initiation of Late Cretaceous north-south rifting within the ancient Farallon Plate. If this hypothesis is correct, then, by analogy to other active and passive mid-ocean rift zones, Late Cretaceous sediment deposited immediately south of the Chinook Trough should contain significant amounts of hydrothermal material deposited in association with the intraplate rifting event. Because the proposed tectonic origin for the Chinook Trough places seafloor south of the eastern end of the trough beneath the Cretaceous calcite compensation depth (CCD), expected hydrothermal components deposited during the Late Cretaceous at these locations also should lack carbonate dilution. Ocean Drilling Program Sites 885 and 886 were drilled approximately 60 km south of the northeast section of the Chinook Trough. High-resolution chemical and mineralogical analyses demonstrate that sediment deposited after 75-81 Ma at these sites contains an extensive record of hydrothermal deposition without associated carbonate. Various proxy indicators -
Mafic-Felsic Magma Interaction at Satsuma-Iwojima Volcano, Japan
Earth Planets Space, 54, 303–325, 2002 Mafic-felsic magma interaction at Satsuma-Iwojima volcano, Japan: Evidence from mafic inclusions in rhyolites Genji Saito1, James A. Stimac2, Yoshihisa Kawanabe1, and Fraser Goff3 1Geological Survey of Japan, AIST, Central 7, Higashi 1-1-1, Tsukuba, Ibaraki 305-8567, Japan 2Philippine Geothermal, Inc., 12th Fl. Citibank Tower, 8741 Paseo de Roxas, Makati, Philippines 3EES-6, MS-D462, Los Alamos National Laboratory, Los Alamos, NM 87545, U.S.A. (Received January 9, 2001; Revised January 25, 2002; Accepted February 4, 2002) Geochemical and petrographic studies of the rhyolites and mafic inclusions from Satsuma-Iwojima volcano were carried out in order to investigate evolution of a silicic, bimodal magma system during the post-caldera stage. Abundant mafic inclusions, which are fine-grained with vesicles in their cores, are present in the Showa- Iwojima rhyolitic lava. Inclusions with similar textures are found in Iwodake volcanic bombs but are less common than in the Showa-Iwojima lava. The major and trace element compositions of the inclusions plot along mixing lines connecting the host rhyolites with spatially and temporally associated basaltic to basaltic andesite magmas. Plagioclase phenocrysts in the inclusions have a large variation in core compositions (An42 to An96), and exhibit various zoning profiles and reaction textures, indicating they coexisted with melts ranging from basaltic to rhyolitic composition. Pyroxenes also exhibit a wide range in composition and a variety of zoning patterns consistent with multiple sources. These results suggest that a stratified magma chamber exists beneath the volcano, consisting of a lower basaltic layer, an upper rhyolitic layer and an episodically-present, thin middle layer of andesite. -
Seafloor Hydrothermal Activity Around a Large Non-Transform
Journal of Marine Science and Engineering Article Seafloor Hydrothermal Activity around a Large Non-Transform Discontinuity along Ultraslow-Spreading Southwest Indian Ridge (48.1–48.7◦ E) Dong Chen 1,2, Chunhui Tao 2,3,*, Yuan Wang 2, Sheng Chen 4, Jin Liang 2, Shili Liao 2 and Teng Ding 1 1 Institute of Marine Geology, College of Oceanography, Hohai University, Nanjing 210098, China; [email protected] (D.C.); [email protected] (T.D.) 2 Key Laboratory of Submarine Geosciences, SOA & Second Institute of Oceanography, MNR, Hangzhou 310012, China; [email protected] (Y.W.); [email protected] (J.L.); [email protected] (S.L.) 3 School of Oceanography, Shanghai Jiao Tong University, Shanghai 200240, China 4 Ocean Technology and Equipment Research Center, School of Mechanical Engineering, Hangzhou Dianzi University, Hangzhou 310018, China; [email protected] * Correspondence: [email protected] Abstract: Non-transform discontinuity (NTD) is one category of tectonic units along slow- and ultraslow-spreading ridges. Some NTD-related hydrothermal fields that may reflect different driving mechanisms have been documented along slow-spreading ridges, but the discrete survey strategy makes it hard to evaluate the incidence of hydrothermal activity. On ultraslow-spreading ridges, fewer NTD-related hydrothermal activities were reported. Factors contributing to the occurrence of hydrothermal activities at NTDs and whether they could be potential targets for hydrothermal explo- Citation: Chen, D.; Tao, C.; Wang, Y.; Chen, S.; Liang, J.; Liao, S.; Ding, T. ration are poorly known. Combining turbidity and oxidation reduction potential (ORP) sensors with Seafloor Hydrothermal Activity a near-bottom camera, Chinese Dayang cruises from 2014 to 2018 have conducted systematic towed around a Large Non-Transform surveys for hydrothermal activity around a large NTD along the ultraslow-spreading Southwest ◦ Discontinuity along Indian Ridge (SWIR, 48.1–48.7 E).