A Record of Plume-Induced Plate Rotation Triggering Seafloor Spreading And
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The Western Branch of the East African Rift: a Review of Tectonics, Volcanology and Geothermal Activity
Presented at SDG Short Course IV on Exploration and Development of Geothermal Resources, organized by UNU-GTP and KenGen, at Lake Bogoria and Lake Naivasha, Kenya, Nov. 13 – Dec. 3, 2019. THE WESTERN BRANCH OF THE EAST AFRICAN RIFT: A REVIEW OF TECTONICS, VOLCANOLOGY AND GEOTHERMAL ACTIVITY Björn S. Hardarson Iceland GeoSurvey (ÍSOR) Grensásvegur 9, 108 Reykjavik ICELAND [email protected] ABSTRACT The East African Rift System (EARS) is a classic example of continental rifting and provides an excellent framework to study extensional magmatism and the evolution of several central volcanic systems that have formed along the rift from the Tertiary to Recent. Many of the volcanic structures have developed substantial high-temperature geothermal systems where the heat source is magmatic and related to central volcanoes. Detailed studies indicate that the geothermal potential in Eastern Africa is in the excess of 15,000 MWe. However, despite the high geothermal potential of EARS only Kenya has installed significant capacity of about 570 MW. Magmatism along the EARS is generally believed to be associated with mantle plume activities but the number and nature of mantle plumes is still, however, controversial. EARS is divided into two main branches, the Eastern- and Western rifts, and it is well documented that significantly greater volcanism is observed in the older Eastern rift (i.e. Ethiopia and Kenya) compared to that in the younger Western rift, where eruptive activity is, in general, restricted to four spatially distinct provinces along the rift axis. These are the Toro-Ankole in western Uganda, the Virunga and Kivu provinces along the border of the DRC with Uganda, Rwanda and Burundi, and the Rungwe volcanic field in SW Tanzania. -
Kinematic Reconstruction of the Caribbean Region Since the Early Jurassic
Earth-Science Reviews 138 (2014) 102–136 Contents lists available at ScienceDirect Earth-Science Reviews journal homepage: www.elsevier.com/locate/earscirev Kinematic reconstruction of the Caribbean region since the Early Jurassic Lydian M. Boschman a,⁎, Douwe J.J. van Hinsbergen a, Trond H. Torsvik b,c,d, Wim Spakman a,b, James L. Pindell e,f a Department of Earth Sciences, Utrecht University, Budapestlaan 4, 3584 CD Utrecht, The Netherlands b Center for Earth Evolution and Dynamics (CEED), University of Oslo, Sem Sælands vei 24, NO-0316 Oslo, Norway c Center for Geodynamics, Geological Survey of Norway (NGU), Leiv Eirikssons vei 39, 7491 Trondheim, Norway d School of Geosciences, University of the Witwatersrand, WITS 2050 Johannesburg, South Africa e Tectonic Analysis Ltd., Chestnut House, Duncton, West Sussex, GU28 OLH, England, UK f School of Earth and Ocean Sciences, Cardiff University, Park Place, Cardiff CF10 3YE, UK article info abstract Article history: The Caribbean oceanic crust was formed west of the North and South American continents, probably from Late Received 4 December 2013 Jurassic through Early Cretaceous time. Its subsequent evolution has resulted from a complex tectonic history Accepted 9 August 2014 governed by the interplay of the North American, South American and (Paleo-)Pacific plates. During its entire Available online 23 August 2014 tectonic evolution, the Caribbean plate was largely surrounded by subduction and transform boundaries, and the oceanic crust has been overlain by the Caribbean Large Igneous Province (CLIP) since ~90 Ma. The consequent Keywords: absence of passive margins and measurable marine magnetic anomalies hampers a quantitative integration into GPlates Apparent Polar Wander Path the global circuit of plate motions. -
Playing Jigsaw with Large Igneous Provinces a Plate Tectonic
PUBLICATIONS Geochemistry, Geophysics, Geosystems RESEARCH ARTICLE Playing jigsaw with Large Igneous Provinces—A plate tectonic 10.1002/2015GC006036 reconstruction of Ontong Java Nui, West Pacific Key Points: Katharina Hochmuth1, Karsten Gohl1, and Gabriele Uenzelmann-Neben1 New plate kinematic reconstruction of the western Pacific during the 1Alfred-Wegener-Institut Helmholtz-Zentrum fur€ Polar- und Meeresforschung, Bremerhaven, Germany Cretaceous Detailed breakup scenario of the ‘‘Super’’-Large Igneous Province Abstract The three largest Large Igneous Provinces (LIP) of the western Pacific—Ontong Java, Manihiki, Ontong Java Nui Ontong Java Nui ‘‘Super’’-Large and Hikurangi Plateaus—were emplaced during the Cretaceous Normal Superchron and show strong simi- Igneous Province as result of larities in their geochemistry and petrology. The plate tectonic relationship between those LIPs, herein plume-ridge interaction referred to as Ontong Java Nui, is uncertain, but a joined emplacement was proposed by Taylor (2006). Since this hypothesis is still highly debated and struggles to explain features such as the strong differences Correspondence to: in crustal thickness between the different plateaus, we revisited the joined emplacement of Ontong Java K. Hochmuth, [email protected] Nui in light of new data from the Manihiki Plateau. By evaluating seismic refraction/wide-angle reflection data along with seismic reflection records of the margins of the proposed ‘‘Super’’-LIP, a detailed scenario Citation: for the emplacement and the initial phase of breakup has been developed. The LIP is a result of an interac- Hochmuth, K., K. Gohl, and tion of the arriving plume head with the Phoenix-Pacific spreading ridge in the Early Cretaceous. The G. -
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. -
Africa-Arabia-Eurasia Plate Interactions and Implications for the Dynamics of Mediterranean Subduction and Red Sea Rifting
This page added by the GeoPRISMS office. Africa-Arabia-Eurasia plate interactions and implications for the dynamics of Mediterranean subduction and Red Sea rifting Authors: R. Reilinger, B. Hager, L. Royden, C. Burchfiel, R. Van der Hilst Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA USA, [email protected], Tel: (617)253 -7860 This page added by the GeoPRISMS office. Our proposed GeoPRISMS Initiative is based on the premise that understanding the mechanics of plate motions (i.e., the force balance on the plates) is necessary to develop realistic models for plate interactions, including processes at subduction and extensional (rifting) plate boundaries. Important advances are being made with new geologic and geophysical techniques and observations that are providing fundamental insights into the dynamics of these plate tectonic processes. Our proposed research addresses directly the following questions identified in the GeoPRISMS SCD Draft Science Plan: 4.2 (How does deformation across the subduction plate boundary evolve in space and time, through the seismic cycle and beyond?), 4.6 (What are the physical and chemical conditions that control subduction zone initiation and the development of mature arc systems?), and 4.7 (What are the critical feedbacks between surface processes and subduction zone mechanics and dynamics?). It has long been recognized that the Greater Mediterranean region provides a natural laboratory to study a wide range of geodynamic processes (Figure 1) including ocean subduction and continent- continent collision (Hellenic arc, Arabia-Eurasia collision), lithospheric delamination (E Turkey High Plateau, Alboran Sea/High Atlas), back-arc extension (Mediterranean basins, including Alboran, Central Mediterranean, Aegean), “escape” tectonics and associated continental transform faulting (Anatolia, North and East Anatolian faults), and active continental and ocean rifting (East African and northern Red Sea rifting, central Red Sea and Gulf of Aden young ocean rifting). -
Plate Tectonic Regulation of Global Marine Animal Diversity
Plate tectonic regulation of global marine animal diversity Andrew Zaffosa,1, Seth Finneganb, and Shanan E. Petersa aDepartment of Geoscience, University of Wisconsin–Madison, Madison, WI 53706; and bDepartment of Integrative Biology, University of California, Berkeley, CA 94720 Edited by Neil H. Shubin, The University of Chicago, Chicago, IL, and approved April 13, 2017 (received for review February 13, 2017) Valentine and Moores [Valentine JW, Moores EM (1970) Nature which may be complicated by spatial and temporal inequities in 228:657–659] hypothesized that plate tectonics regulates global the quantity or quality of samples (11–18). Nevertheless, many biodiversity by changing the geographic arrangement of conti- major features in the fossil record of biodiversity are consis- nental crust, but the data required to fully test the hypothesis tently reproducible, although not all have universally accepted were not available. Here, we use a global database of marine explanations. In particular, the reasons for a long Paleozoic animal fossil occurrences and a paleogeographic reconstruction plateau in marine richness and a steady rise in biodiversity dur- model to test the hypothesis that temporal patterns of continen- ing the Late Mesozoic–Cenozoic remain contentious (11, 12, tal fragmentation have impacted global Phanerozoic biodiversity. 14, 19–22). We find a positive correlation between global marine inverte- Here, we explicitly test the plate tectonic regulation hypothesis brate genus richness and an independently derived quantitative articulated by Valentine and Moores (1) by measuring the extent index describing the fragmentation of continental crust during to which the fragmentation of continental crust covaries with supercontinental coalescence–breakup cycles. The observed posi- global genus-level richness among skeletonized marine inverte- tive correlation between global biodiversity and continental frag- brates. -
Paleomagnetism and U-Pb Geochronology of the Late Cretaceous Chisulryoung Volcanic Formation, Korea
Jeong et al. Earth, Planets and Space (2015) 67:66 DOI 10.1186/s40623-015-0242-y FULL PAPER Open Access Paleomagnetism and U-Pb geochronology of the late Cretaceous Chisulryoung Volcanic Formation, Korea: tectonic evolution of the Korean Peninsula Doohee Jeong1, Yongjae Yu1*, Seong-Jae Doh2, Dongwoo Suk3 and Jeongmin Kim4 Abstract Late Cretaceous Chisulryoung Volcanic Formation (CVF) in southeastern Korea contains four ash-flow ignimbrite units (A1, A2, A3, and A4) and three intervening volcano-sedimentary layers (S1, S2, and S3). Reliable U-Pb ages obtained for zircons from the base and top of the CVF were 72.8 ± 1.7 Ma and 67.7 ± 2.1 Ma, respectively. Paleomagnetic analysis on pyroclastic units yielded mean magnetic directions and virtual geomagnetic poles (VGPs) as D/I = 19.1°/49.2° (α95 =4.2°,k = 76.5) and VGP = 73.1°N/232.1°E (A95 =3.7°,N =3)forA1,D/I = 24.9°/52.9° (α95 =5.9°,k =61.7)and VGP = 69.4°N/217.3°E (A95 =5.6°,N=11) for A3, and D/I = 10.9°/50.1° (α95 =5.6°,k = 38.6) and VGP = 79.8°N/ 242.4°E (A95 =5.0°,N = 18) for A4. Our best estimates of the paleopoles for A1, A3, and A4 are in remarkable agreement with the reference apparent polar wander path of China in late Cretaceous to early Paleogene, confirming that Korea has been rigidly attached to China (by implication to Eurasia) at least since the Cretaceous. The compiled paleomagnetic data of the Korean Peninsula suggest that the mode of clockwise rotations weakened since the mid-Jurassic. -
1 Introduction Gondwana
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Sydney eScholarship Regional plate tectonic reconstructions of the Indian Ocean Thesis Submitted in fulfilment of the requirements for the degree of Doctor of Philosophy Ana Gibbons School of Geosciences 2012 Supervised by Professor R. Dietmar Müller and Dr Joanne Whittaker The University of Sydney, PhD Thesis, Ana Gibbons, 2012 - Introduction DECLARATION I declare that this thesis contains less than 100,000 words and contains no work that has been submitted for a higher degree at any other university or institution. No animal or ethical approvals were applicable to this study. The use of any published written material or data has been duly acknowledged. Ana Gibbons ii The University of Sydney, PhD Thesis, Ana Gibbons, 2012 - Introduction ACKNOWLEDGEMENTS I would like to thank my supervisors for their endless encouragement, generosity, patience, and not least of all their expertise and ingenuity. I have thoroughly benefitted from working with them and cannot imagine a better supervisory team. I also thank Maria Seton, Carmen Gaina and Sabin Zahirovic for their help and encouragement. I thank Statoil (Norway), the Petroleum Exploration Society of Australia (PESA) and the School of Geosciences, University of Sydney for support. I am extremely grateful to Udo Barckhausen, Kaj Hoernle, Reinhard Werner, Paul Van Den Bogaard and all staff and crew of the CHRISP research cruise for a very informative and fun collaboration, which greatly refined this first chapter of this thesis. I also wish to thank Dr Yatheesh Vadakkeyakath from the National Institute of Oceanography, Goa, India, for his thorough review, which considerably improved the overall model and quality of the second chapter. -
Geologic History of Siletzia, a Large Igneous Province in the Oregon And
Geologic history of Siletzia, a large igneous province in the Oregon and Washington Coast Range: Correlation to the geomagnetic polarity time scale and implications for a long-lived Yellowstone hotspot Wells, R., Bukry, D., Friedman, R., Pyle, D., Duncan, R., Haeussler, P., & Wooden, J. (2014). Geologic history of Siletzia, a large igneous province in the Oregon and Washington Coast Range: Correlation to the geomagnetic polarity time scale and implications for a long-lived Yellowstone hotspot. Geosphere, 10 (4), 692-719. doi:10.1130/GES01018.1 10.1130/GES01018.1 Geological Society of America Version of Record http://cdss.library.oregonstate.edu/sa-termsofuse Downloaded from geosphere.gsapubs.org on September 10, 2014 Geologic history of Siletzia, a large igneous province in the Oregon and Washington Coast Range: Correlation to the geomagnetic polarity time scale and implications for a long-lived Yellowstone hotspot Ray Wells1, David Bukry1, Richard Friedman2, Doug Pyle3, Robert Duncan4, Peter Haeussler5, and Joe Wooden6 1U.S. Geological Survey, 345 Middlefi eld Road, Menlo Park, California 94025-3561, USA 2Pacifi c Centre for Isotopic and Geochemical Research, Department of Earth, Ocean and Atmospheric Sciences, 6339 Stores Road, University of British Columbia, Vancouver, BC V6T 1Z4, Canada 3Department of Geology and Geophysics, University of Hawaii at Manoa, 1680 East West Road, Honolulu, Hawaii 96822, USA 4College of Earth, Ocean, and Atmospheric Sciences, Oregon State University, 104 CEOAS Administration Building, Corvallis, Oregon 97331-5503, USA 5U.S. Geological Survey, 4210 University Drive, Anchorage, Alaska 99508-4626, USA 6School of Earth Sciences, Stanford University, 397 Panama Mall Mitchell Building 101, Stanford, California 94305-2210, USA ABSTRACT frames, the Yellowstone hotspot (YHS) is on southern Vancouver Island (Canada) to Rose- or near an inferred northeast-striking Kula- burg, Oregon (Fig. -
Geological Evolution of the Red Sea: Historical Background, Review and Synthesis
See discussions, stats, and author profiles for this publication at: https://www.researchgate.net/publication/277310102 Geological Evolution of the Red Sea: Historical Background, Review and Synthesis Chapter · January 2015 DOI: 10.1007/978-3-662-45201-1_3 CITATIONS READS 6 911 1 author: William Bosworth Apache Egypt Companies 70 PUBLICATIONS 2,954 CITATIONS SEE PROFILE Some of the authors of this publication are also working on these related projects: Near and Middle East and Eastern Africa: Tectonics, geodynamics, satellite gravimetry, magnetic (airborne and satellite), paleomagnetic reconstructions, thermics, seismics, seismology, 3D gravity- magnetic field modeling, GPS, different transformations and filtering, advanced integrated examination. View project Neotectonics of the Red Sea rift system View project All content following this page was uploaded by William Bosworth on 28 May 2015. The user has requested enhancement of the downloaded file. All in-text references underlined in blue are added to the original document and are linked to publications on ResearchGate, letting you access and read them immediately. Geological Evolution of the Red Sea: Historical Background, Review, and Synthesis William Bosworth Abstract The Red Sea is part of an extensive rift system that includes from south to north the oceanic Sheba Ridge, the Gulf of Aden, the Afar region, the Red Sea, the Gulf of Aqaba, the Gulf of Suez, and the Cairo basalt province. Historical interest in this area has stemmed from many causes with diverse objectives, but it is best known as a potential model for how continental lithosphere first ruptures and then evolves to oceanic spreading, a key segment of the Wilson cycle and plate tectonics.