Seafloor Hydrothermal Activity Around a Large Non-Transform
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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. -
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 -
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. -
Geophysical Journal International
Geophysical Journal International Geophys. J. Int. (2013) doi: 10.1093/gji/ggt372 Geophysical Journal International Advance Access published October 11, 2013 Cretaceous to present kinematics of the Indian, African and Seychelles plates Graeme Eagles∗ and Ha H. Hoang Department of Earth Sciences, Royal Holloway University of London, Egham, Surrey, TW20 0EX, United Kingdom. E-mail: [email protected] Downloaded from Accepted 2013 September 16. Received 2013 September 13; in original form 2012 November 12 SUMMARY An iterative inverse model of seafloor spreading data from the Mascarene and Madagascar http://gji.oxfordjournals.org/ basins and the flanks of the Carlsberg Ridge describes a continuous history of Indian–African Plate divergence since 84 Ma. Visual-fit modelling of conjugate magnetic anomaly data from near the Seychelles platform and Laxmi Ridge documents rapid rotation of a Seychelles Plate about a nearby Euler pole in Palaeocene times. As the Euler pole migrated during this rotation, the Amirante Trench on the western side of the plate accommodated first convergence and later divergence with the African Plate. The unusual present-day morphology of the Amirante GJI Geodynamics and tectonics Trench and neighbouring Amirante Banks can be related to crustal thickening by thrusting and at Alfred Wegener Institut fuer Polar- und Meeresforschung Bibliothek on October 11, 2013 folding during the convergent phase and the subsequent development of a spreading centre with a median valley during the divergent phase. The model fits FZ trends in the north Arabian and east Somali basins, suggesting that they formed in India–Africa Plate divergence. Seafloor fabric in and between the basins shows that they initially hosted a segmented spreading ridge that accommodated slow plate divergence until 71–69 Ma, and that upon arrival of the Deccan–Reunion´ plume and an increase to faster plate divergence rates in the period 69–65 Ma, segments of the ridge lengthened and propagated. -
Complex Subsurface Hydrothermal Fluid Mixing at a Submarine Arc Volcano Supports Distinct and Highly Diverse Microbial Communities
Complex subsurface hydrothermal fluid mixing at a submarine arc volcano supports distinct and highly diverse microbial communities Anna-Louise Reysenbacha,1,2, Emily St. Johna,2, Jennifer Meneghina, Gilberto E. Floresb, Mircea Podarc, Nina Dombrowskid, Anja Spangd,e, Stephane L’Haridonf, Susan E. Humphrisg, Cornel E. J. de Rondeh, Fabio Caratori Tontinih, Maurice Tiveyg, Valerie K. Stuckeri, Lucy C. Stewarth,j, Alexander Diehlk,l, and Wolfgang Bachk,l aCenter for Life in Extreme Environments, Biology Department, Portland State University, Portland, OR 97201; bDepartment of Biology, California State University, Northridge, CA 91330; cBiosciences Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831; dRoyal Netherlands Institute for Sea Research, Department of Marine Microbiology and Biogeochemistry, NL-1790 AB Den Burg, The Netherlands; eDepartment of Cell and Molecular Biology, Science for Life Laboratory, Uppsala University, SE-75123 Uppsala, Sweden; fCNRS, Institut Français de Recherche pour l’Exploitation de la Mer, Laboratoire de Microbiologie des Environnements Extrêmes, Université de Bretagne Occidentale, F-29280 Plouzané, France; gDepartment of Geology and Geophysics, Woods Hole Oceanographic Institution, Woods Hole, MA 02543; hDepartment of Earth Systems and Resources, GNS Science, Avalon, Lower Hutt 5010, New Zealand; iLaboratories and Collections, GNS Science, Avalon, Lower Hutt 5010, New Zealand; jToha Science, Wellington 6011, New Zealand; kFaculty of Geosciences, University of Bremen, 28359 Bremen, Germany; and lMARUM - Center for Marine Environmental Sciences, University of Bremen, 28359 Bremen, Germany Edited by Edward F. DeLong, University of Hawaii at Manoa, Honolulu, HI, and approved November 3, 2020 (received for review September 10, 2020) Hydrothermally active submarine volcanoes are mineral-rich bio- seawater circulation through oceanic crust. -
21. Tectonic Evolution of the Atlantis Ii Fracture Zone1
Von Herzen, R.P., Robinson, P.T., et al., 1991 Proceedings of the Ocean Drilling Program, Scientific Results,Vol. 118 21. TECTONIC EVOLUTION OF THE ATLANTIS II FRACTURE ZONE1 Henry J.B. Dick,2 Hans Schouten,2 Peter S. Meyer,2 David G. Gallo,2 Hugh Bergh,3 Robert Tyce,4 Phillipe Patriat,5 Kevin T.M. Johnson,2 Jon Snow,2 and Andrew Fisher6 ABSTRACT SeaBeam echo sounding, seismic reflection, magnetics, and gravity profiles were run along closely spaced tracks (5 km) parallel to the Atlantis II Fracture Zone on the Southwest Indian Ridge, giving 80% bathymetric coverage of a 30- × 170-nmi strip centered over the fracture zone. The southern and northern rift valleys of the ridge were clearly defined and offset north-south by 199 km. The rift valleys are typical of those found elsewhere on the Southwest Indian Ridge, with relief of more than 2200 m and widths from 22 to 38 km. The ridge-transform intersections are marked by deep nodal basins lying on the transform side of the neovolcanic zone that defines the present-day spreading axis. The walls of the transform generally are steep (25°-40°), although locally, they can be more subdued. The deepest point in the transform is 6480 m in the southern nodal basin, and the shallowest is an uplifted wave-cut terrace that exposes plutonic rocks from the deepest layer of the ocean crust at 700 m. The transform valley is bisected by a 1.5-km-high median tectonic ridge that extends from the northern ridge-transform intersection to the midpoint of the active transform. -
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). -
The Indian Ocean Diverse Ecosystems Harbor Distinctive Deep-Sea Life and Sought-After Minerals
A fact sheet from April 2018 IFM-GEOMAR The Indian Ocean Diverse ecosystems harbor distinctive deep-sea life and sought-after minerals Overview Vast abyssal plains, mountain chains, and seamounts cover the bottom of the Indian Ocean. Each area is home to life forms suited to its particularities—and each also holds valuable minerals that could be removed through seabed mining. Hydrothermal vents spew superheated, mineral-laden water into their surroundings that, when cooled, forms towers containing copper, cobalt, nickel, zinc, gold, and rare earth elements. These minerals are essential to modern economies. The vent zones are biologically rich as well, supporting mussels, stalked barnacles, scaly-foot snails, and a variety of microbes with potential biomedical and industrial applications. Atop the Indian Ocean’s abyssal plains are more than a billion potato-size nodules with rich concentrations of manganese, copper, cobalt, and nickel. On and near the nodules, wildlife—such as sponges, sea cucumbers, and fish—has evolved to flourish in the deep cold and darkness. Seabed mining is expected to have a significant and long-lasting impact on these deep-sea ecosystems. Mining equipment would remove or degrade habitats, sediment plumes could smother nearby life, and noise and light could harm the unique species that have evolved in order to live here. The International Seabed Authority (ISA) was established by the Law of the Sea treaty to manage seabed mining in areas beyond national jurisdiction while protecting the marine environment. The ISA is drafting regulations to accomplish these objectives with rules on where and how seabed mining could occur. -
Dick IIOE-2 Talks
Theme 4:Geological and deep-ocean biogeochemical processes Part 1 Marine geology & Geophysics Henry Dick WHOI The SW Indian Ridge – 7,700 km long, ultraslow spreading @ 14 mm/yr full rate 90 Ma Reunion Is. 94-100 Ma Reunion Is Rodriguez Gough Is. Nubia-Somalia Triple Junction Plate Boundary Marion Is. No Crozet Is. obvious track Speiss Smt. Bouvet Conrad Rise Triple Junction (inactive) The general hypothesis for ocean rises is plume mantle emplaced beneath the ridge creates uplift due to thick buoyant crust and excess mantle temperature Cold? Hot? Marion Rise has the highest Na8.0 of all ocean rises, which indicates that the degree of mantle melting must be small & the temperature anomaly associated with it must also be small. Depleted? Fertile? The Southwest Indian Ridge Largest abundance of exposed mantle rock anywhere on Earth Ultraslow spreading with unique tectonics Largest axial volcanoes on any ocean ridge Extreme ridge obliquity creates unusual thermal environments Densest array of transforms of any ocean ridge. Has one of the oldest continuously active geologic structures on Earth (~650 Myr) 24% Peridotite 62% Basalt 4% Gabbro 10% Greenstone & Diabase Systematic sampling of the SW Indian Ridge shows a lack of gabbroic crust and an exceptional % of exposed mantle Extreme variations in crustal thickness are matched by extreme variations in geochemistry ! Amagmatic Accretionary Segments Negligible Volcanic Crust Takes any Orientation to Spreading Direction ~24% of the lithosphere generated along the Southwest Indian Ridge has no crust with the mantle exposed directly to the seafloor. ! ! The crust over the Marion Rise and elsewhere along the is generally thin, but with abrupt rapid changes in local thickness. -
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. -
Slow Spreading Ridges of the Indian Ocean: an Overview of Marine Geophysical Investigations K
J. Ind. Geophys.Slow Union Spreading ( April Ridges 2015 of the ) Indian Ocean: An Overview of Marine Geophysical Investigations v.19, no.2, pp:137-159 Slow Spreading Ridges of the Indian Ocean: An Overview of Marine Geophysical Investigations K. A. Kamesh Raju*, Abhay V. Mudholkar, Kiranmai Samudrala CSIR-National Institute of Oceanography, Dona Paula, Goa – 403004, India *Corresponding author: [email protected] ABSTRACT Sparse and non-availability of high resolution geophysical data hindered the delineation of accurate morphology, structural configuration, tectonism and spreading history of Carlsberg Ridge (CR) and Central Indian Ridges (CIR) in the Indian Ocean between Owen fracture zone at about 10oN, and the Rodriguez Triple Junction at ~25oS. Analysis of available multibeam bathymetry, magnetic, gravity, seabed sampling on the ridge crest, and selected water column data suggest that even with similar slow spreading history the segmentation significantly differ over the CR and CIR ridge systems. Topography, magnetic and gravity signatures indicate non-transform discontinuity over CR and suggest that it has relatively slower spreading history than CIR. Magmatic and less magmatic events characterize CR and CIR respectively and well defined oceanic core complex (OCC) are confined only to segments of the CIR. The mantle Bouguer anomaly signatures over the ridges suggest crustal accretion and pattern of localized magnetic anomalies indicate zones of high magnetization coinciding with the axial volcanic ridges. Geophysical investigations /