Observational and Theoretical Studies of the Dynamics of Mantle Plume–Mid-Ocean Ridge Interaction
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MANTLE PLUMES and FLOOD BASALTS Scribedblob of Uniformtemperature, Rather Than Resultingfrom Startsat the Paranaflood Basalt Province,South America
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Memorial University Research Repository JOURNALOF GEOPHYSICAL RESEARCH, VOL. 106, NO. B2, PAGES 2047-2059, FEBRUARY 10, 2001 Mantleplumes and flood basalts: Enhanced melting fromplume ascent and an eclogitecomponent A.M. Leitch•, andG. F.Davies ResearchSchool of EarthSciences, Australian National University, Canberra, ACT Abstract.New numerical models of startingplumes reproduce the observed volumes and rates of floodbasalt eruptions, even for a plumeof moderatetemperature arriving under thick lithosphere. Thesemodels follow the growth of a newplume from a thermalboundary layer and its subsequent risethrough the mantle viscosity structure. They show that as a plumehead rises into the lower- viscosityupper mantle it narrows,and it isthus able to penetrate rapidly right to thebase of litho- sphere,where it spreadsas a thinlayer. This behavior also brings the hottest plume matehal to the shallowestdepths. Both factors enhance melt production compared with previous plume models. Themodel plumes are also assumed to containeclogite bodies, inferred from geochemistry to be recycledoceanic crust. Previous numerical models have shown that the presence of nonreacting eclogitebodies may greatly enhance melt production. it hasbeen argued that the eclogite-derived meltwould react with surroundingperidotite and refreeze; however, recent experimental studies indicatethat eclogite-derived melts may have reached the Earth's surface with onlymoderate or evenminor -
Mantle Plumes and Intraplate Volcanism Volcanism on the Earth
Mantle Plumes and Intraplate Volcanism Origin of Oceanic Island Volcanoes EAS 302 Lecture 20 Volcanism on the Earth • Mid-ocean ridges (>90% of the volcanism) – “constructive” plate margins • Subduction-related (much of the rest) – “destructive plate” margins • Volcanism in plate interiors (usually) – , e.g., Yellowstone, Hawaii not explained by the plate tectonic paradigm. Characteristics of Intra-plate Volcanoes • Not restricted to plate margins. • Occur at locations that are stationary relative to plate motions, “hot spots”(pointed out by J. T. Wilson, 1963). • Distinctive isotopic and trace element composition. Hot Spot Traces on the Pacific Ocean Floor The Mantle Plume Model • “ Hot spot” volcanoes are manifestations of mantle plumes: columns of hot rock rising buoyantly from the deep mantle – This idea proposed by W. J. Morgan in 1971. • Evidence – Maintain (almost) fixed positions relative to each other; i.e., they are not affected by plate motions – A number of “hot spots” are associated with “swells”, indicative of hot mantle below – Their magmas are compositionally distinct from mid-ocean ridge basalts and therefore must be derived from a different part of the mantle Current Mantle Plumes The Hawaiian Mantle Plume Age of Hawaiian Volcanism The Hawaiian “Swell” Plumes at the surface • In the last 100-200 km, the plume begins to melt. • Once it reaches the base of the lithosphere, it can no longer rise and spreads out. Isotopic Compositions of Oceanic Island Basalts • Nd and Sr isotope ratios 12 DMM distinct from MORB: 10 derived from separate MORB 8 reservoir which is less 6 depleted (and Society ε Nd 4 sometimes enriched) in HIMU incompatible elements. -
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. -
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. -
Mantle Dynamics and Characteristics of the Azores Plateau
Earth and Planetary Science Letters 362 (2013) 258–271 Contents lists available at SciVerse ScienceDirect Earth and Planetary Science Letters journal homepage: www.elsevier.com/locate/epsl Mantle dynamics and characteristics of the Azores plateau C. Adam a,n, P. Madureira a,b, J.M. Miranda c, N. Lourenc-o c,d, M. Yoshida e, D. Fitzenz a,1 a Centro de Geofı´sica de E´vora/Univ. E´vora, 7002-554 E´vora, Portugal b Estrutura de Missao~ para a Extensao~ da Plataforma Continental (EMEPC), 2770-047, Pac-o d’ Arcos, Portugal c Instituto Portugues do Mar e da Atmosfera, Lisboa, Portugal d University of Algarve, IDL, Campus de Gambelas, 8000 Faro, Portugal e Institute for Research on Earth Evolution (IFREE), Japan Agency for Marine-Earth Science and Technology (JAMSTEC), Yokosuka, Kanagawa 237-0061, Japan article info abstract Article history: Situated in the middle of the Atlantic Ocean, the Azores plateau is a region of elevated topography Received 25 July 2012 encompassing the triple junction between the Eurasian, Nubian and North American plates. The plateau is Received in revised form crossed by the Mid-Atlantic Ridge, and the Terceira Rift is generally thought of as its northern boundary. 2 November 2012 The origin of the plateau and of the Terceira Rift is still under debate. This region is associated with active Accepted 5 November 2012 volcanism. Geophysical data describe complex tectonic and seismic patterns. The mantle under this region Editor: T. Spohn Available online 18 January 2013 is characterized by anomalously slow seismic velocities. However, this mantle structure has not yet been used to quantitatively assess the influence of the mantle dynamics on the surface tectonics. -
Large Igneous Provinces and the Mantle Plume Hypothesis
Large Igneous Provinces and the Mantle Plume Hypothesis Columnar jointing in a postglacial basalt flow at Aldeyarfoss, NE Iceland. PHOTO JOHN MACLENNAN Ian H. Campbell1 antle plumes are columns of hot, solid material that originate deep in the mantle, probably at the core–mantle boundary. Laboratory 1990) and aseismic ridges, like the Chagos–Lacadive Ridge, to the and numerical models replicating conditions appropriate to the M melting of a plume tail (Wilson mantle show that mantle plumes have a regular and predictable shape that 1963; Morgan 1971). allows a number of testable predictions to be made. New mantle plumes are predicted to consist of a large head, 1000 km in diameter, followed by a THE MANTLE PLUME HYPOTHESIS narrower tail. Initial eruption of basalt from a plume head should be preceded Convection in fluids is driven by by ~1000 m of domal uplift. High-temperature magmas are expected to buoyancy anomalies that originate dominate the first eruptive products of a new plume and should be concen- in thermal boundary layers. trated near the centre of the volcanic province. All of these predictions are Earth’s mantle has two boundary confirmed by observations. layers. The upper boundary layer is the lithosphere, which cools KEYWORDS: mantle plume, large igneous provinces, uplift, picrite through its upper surface. It even- tually becomes denser than the INTRODUCTION underlying mantle and sinks back into it, driving plate tectonics. The lower boundary layer is The plate tectonic hypothesis provides an elegant explana- the contact between the Earth’s molten iron–nickel outer tion for Earth’s two principal types of basaltic volcanism, core and the mantle. -
Origin of Indian Ocean Seamount Province by Shallow Recycling of Continental Lithosphere
LETTERS PUBLISHED ONLINE: 27 NOVEMBER 2011 | DOI: 10.1038/NGEO1331 Origin of Indian Ocean Seamount Province by shallow recycling of continental lithosphere K. Hoernle1*, F. Hauff1, R. Werner1, P. van den Bogaard1, A. D. Gibbons2, S. Conrad1 and R. D. Müller2 The origin of the Christmas Island Seamount Province in the 5° S Outsider Seamount Sumatra northeast Indian Ocean is enigmatic. The seamounts do not Java form the narrow, linear and continuous trail of volcanoes 53 Investigator Rise Bali that would be expected if they had formed above a mantle Vening-Meinesz 1,2 3 Cocos- plume . Volcanism above a fracture in the lithosphere is also Keeling Volcanic Province 10° S unlikely, because the fractures trend orthogonally with respect Islands 4¬44 Christmas Island 64 70 65 85 105 to the east–west trend of the Christmas Island chain. Here 56 71 94 40 39 we combine Ar= Ar age, Sr, Nd, Hf and high-precision Pb 47 64 81 107 97 112 104 136 Argo isotope analyses of volcanic rocks from the province with plate 90 95 115 Basin tectonic reconstructions. We find that the seamounts are 47– 47 102 115 Volc. 15° S Prov. 136 million years old, decrease in age from east to west and are Cocos-Keeling Eastern Wharton Basin consistently 0–25 million years younger than the underlying Volc. Prov. Volcanic Province oceanic crust, consistent with formation near a mid-ocean 7 cm yr¬1 ridge. The seamounts also exhibit an enriched geochemical 95° E 100° E 105° E 110° E 115° E signal, indicating that recycled continental lithosphere was present in their source. -
S41598-020-76691-1 1 Vol.:(0123456789)
www.nature.com/scientificreports OPEN Rifting of the oceanic Azores Plateau with episodic volcanic activity B. Storch1*, K. M. Haase1, R. H. W. Romer1, C. Beier1,2 & A. A. P. Koppers3 Extension of the Azores Plateau along the Terceira Rift exposes a lava sequence on the steep northern fank of the Hirondelle Basin. Unlike typical tholeiitic basalts of oceanic plateaus, the 1.2 km vertical submarine stratigraphic profle reveals two successive compositionally distinct basanitic to alkali basaltic eruptive units. The lower unit is volumetrically more extensive with ~ 1060 m of the crustal profle forming between ~ 2.02 and ~ 1.66 Ma, followed by a second unit erupting the uppermost ~ 30 m of lavas in ~ 100 kyrs. The age of ~ 1.56 Ma of the youngest in-situ sample at the top of the profle implies that the 35 km-wide Hirondelle Basin opened after this time along normal faults. This rifting phase was followed by alkaline volcanism at D. João de Castro seamount in the basin center indicating episodic volcanic activity along the Terceira Rift. The mantle source compositions of the two lava units change towards less radiogenic Nd, Hf, and Pb isotope ratios. A change to less SiO2-undersaturated magmas may indicate increasing degrees of partial melting beneath D. João de Castro seamount, possibly caused by lithospheric thinning within the past 1.5 million years. Our results suggest that rifting of oceanic lithosphere alternates between magmatically and tectonically dominated phases. Oceanic plateaus with a crustal thickness to 30 km cover large areas in the oceans and these bathymetric swells afect oceanic currents and marine life 1,2. -
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 -
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. -
Study Plan for the International Masters Programme in Geophysics
Study Plan for the International Masters Programme in Geophysics Credits 6 12 18 24 30 P1 Mathematical Geophysics P2 Statistical Geophysics P 3 Earth System Science P 4 Geocontinua r e t s e P3.1 Introduction to Earth System Science 1 [2 SWS, 3 ECTS] P2.1 Statistics for Geosciences (Lecture) P4.1 Methods of Geocontinua (Lecture) m e S P1.1 Mathematical Geophysics (Lecture) [4 SWS, 6 ECTS] [2 SWS, 3 ECTS] [2 SWS, 3 ECTS] t P3.2 Introduction to Earth System Science 2 [2 SWS, 3 ECTS] s 1 P1.2 Mathematical Geophysics (Exercise) [2 SWS, 3 ECTS] P2.2 Statistics for Geosciences (Exercise) P4.2 Methods of Geocontinua (Exercise) P3.3 Geophysics Research: Overview on Methods and Open [2 SWS, 3 ECTS] [2 SWS, 3 ECTS] Questions [2 SWS, 3 ECTS] P8 Geophyiscal Data P 5 Computational Geophysics P6 Scientific Programming P7 Advanced Geophysics Acquisition and WP: Specialisation I r Analysis e t s e P7.1 Geodynamics [2 SWS, 3 ECTS] P5.1 Computational Geophysics (Lecture) P6.1 Scientific Programming (Lecture) m e P8.1 Geophysical S [2SWS, 3ECTS] [2SWS, 3 ECTS] d P7.2 Seismology [2 SWS, 3 ECTS] Data Analysis: Elective Module, 6 ECTS n 2 Practical Introduction Choose one of WP1, WP2, WP3 P5.2 Computational Geophysics (Exercise) P6.2 Scientific Programming (Exercise) P7.3 Geo- and Paleomagnetism [2 SWS, 3 ECTS] [2 SWS, 3 ECTS] [2SWS, 3ECTS] [2SWS, 3 ECTS] P9 Research Training P10 Advanced Topics in Geophysics Elective Modules: Interdisciplinarity WP: Specialisation II r e t s P10.1 Tools, Techniques and current Trends e P9.1 Presentation, Communication, in