The Cenozoic Magmatism of East Africa: Part V – Magma Sources and Processes in the East African Rift
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The Central Kenya Peralkaline Province: Insights Into the Evolution of Peralkaline Salic Magmas
The central Kenya peralkaline province: Insights into the evolution of peralkaline salic magmas. Ray Macdonald, Bruno Scaillet To cite this version: Ray Macdonald, Bruno Scaillet. The central Kenya peralkaline province: Insights into the evolution of peralkaline salic magmas.. Lithos, Elsevier, 2006, 91, pp.1-4, 59-73. 10.1016/j.lithos.2006.03.009. hal-00077416 HAL Id: hal-00077416 https://hal-insu.archives-ouvertes.fr/hal-00077416 Submitted on 10 Jul 2006 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. The central Kenya peralkaline province: Insights into the evolution of peralkaline salic magmas R. Macdonalda, and B. Scailletb aEnvironment Centre, Lancaster University, Lancaster LA1 4YQ, UK bISTO-CNRS, 1a rue de la Férollerie, 45071 Orléans cedex 2, France Abstract The central Kenya peralkaline province comprises five young (< 1 Ma) volcanic complexes dominated by peralkaline trachytes and rhyolites. The geological and geochemical evolution of each complex is described and issues related to the development of peralkalinity in salic magmas are highlighted. The peralkaline trachytes may have formed by fractionation of basaltic magma via metaluminous trachyte and in turn generated pantellerite by the same mechanism. Comenditic rhyolites are thought to have formed by volatile-induced crustal anatexis and may themselves have been parental to pantelleritic melts by crystal fractionation. -
And Post-Collision Calc-Alkaline Magmatism in the Qinling Orogenic Belt, Central China, As Documented by Zircon Ages on Granitoid Rocks
Journal of the Geological Societv. London, Vol. 153, 1996, pp. 409-417. Palaeozoic pre- and post-collision calc-alkaline magmatism in the Qinling orogenic belt, central China, as documented by zircon ages on granitoid rocks F. XUE'.*,',A. KRONER', T. REISCHMANN' & F. LERCH' 'Institut fiir Geowissenschaften, Universitat Mainz, 55099 Mainz, Germany 'Department of Geology, Northwest University, 710069 Xi'an, China .'Present address: Department of Geophysical Sciences, The University of Chicago, 5734 South Ellis Avenue, Chicago, IL 60637, USA Abstract: Basedon large-scale reconnaissance mapping, we identifiedtwo calc-alkaline plutonic assemblagesfrom the northern Qinling orogenic belt.central China. The older assemblage of intrusions. closely associated and deformed coevally with their host volcanic arc sequences, seems to represent the fractionation product of basaltic arc magma. It therefore predates the collision of the North China Block with the Central Qinling island-arc system that developed in a SW Pacific-type oceanic domain south of the North China Block. Single-zircon zo7Pb/2'"Pb evaporation dating yielded early to middle Ordovician ages for this assemblage. with a relatively small range from 487.2 f 1.1 to 470.2 f 1.3 Ma. Intrusions of the younger assemblage are largely undeformed and truncate structures shown in rocks of theolder assemblage. They are interpreted as post-collisional calc-alkaline granitoids.Single zircon dating provided an age of 401.8 f 0.8 Mafor the younger assemblage. consistentwith earlier work that defines an age range from c. 420 to 395Ma. Our datafavour a tectonicmodel involving formation and amalgamation of islandarc and microcontinent terranes between ca. 490 and 470 Ma ago to create the Central Qinling Zone which subsequently collided with theNorth China Block prior to c. -
Historical Volcanism and the State of Stress in the East African Rift System
Historical volcanism and the state of stress in the East African Rift System Article Accepted Version Open Access Wadge, G., Biggs, J., Lloyd, R. and Kendall, J.-M. (2016) Historical volcanism and the state of stress in the East African Rift System. Frontiers in Earth Science, 4. 86. ISSN 2296- 6463 doi: https://doi.org/10.3389/feart.2016.00086 Available at http://centaur.reading.ac.uk/66786/ It is advisable to refer to the publisher’s version if you intend to cite from the work. See Guidance on citing . To link to this article DOI: http://dx.doi.org/10.3389/feart.2016.00086 Publisher: Frontiers media All outputs in CentAUR are protected by Intellectual Property Rights law, including copyright law. Copyright and IPR is retained by the creators or other copyright holders. Terms and conditions for use of this material are defined in the End User Agreement . www.reading.ac.uk/centaur CentAUR Central Archive at the University of Reading Reading’s research outputs online 1 Historical volcanism and the state of stress in the East African 2 Rift System 3 4 5 G. Wadge1*, J. Biggs2, R. Lloyd2, J-M. Kendall2 6 7 8 1.COMET, Department of Meteorology, University of Reading, Reading, UK 9 2.COMET, School of Earth Sciences, University of Bristol, Bristol, UK 10 11 * [email protected] 12 13 14 Keywords: crustal stress, historical eruptions, East African Rift, oblique motion, 15 eruption dynamics 16 17 18 19 20 21 Abstract 22 23 Crustal extension at the East African Rift System (EARS) should, as a tectonic ideal, 24 involve a stress field in which the direction of minimum horizontal stress is 25 perpendicular to the rift. -
Extrusive and Intrusive Magmatism Greatly Influence the Tectonic Mode of Earth-Like Planets
EPSC Abstracts Vol. 11, EPSC2017-945, 2017 European Planetary Science Congress 2017 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2017 Extrusive and Intrusive Magmatism Greatly Influence the Tectonic Mode of Earth-Like Planets D. Lourenco, P. J. Tackley, A. Rozel and M. Ballmer Institute of Geophysics, Department of Earth Sciences, ETH Zurich, Switzerland ([email protected] / Fax: +41 44 633 1065) Abstract reported in [3], we use thermo-chemical global mantle convection numerical simulations to Plate tectonics on Earth-like planets is typically systematically investigate the effect of plutonism, in modelling using a strongly temperature-dependent conjugation with eruptive volcanism. Results visco-plastic rheology. Previous analyses have reproduce the three common tectonic/convective generally focussed on purely thermal convection. regimes usually obtained in simulations using a However, we have shown that the influence of visco-plastic rheology: stagnant-lid (a one-plate compositional heterogeneity in the form of planet), episodic (where the lithosphere is unstable continental [1] or oceanic [2] crust can greatly and frequently overturns into the mantle), and influence plate tectonics by making it easier (i.e. it mobile-lid (similar to plate tectonics). At high occurs at a lower yield stress or friction coefficient). intrusion efficiencies, we observe and characterise a Here we present detailed results on this topic, in new additional regime called “plutonic-squishy lid”. particular focussing on the influence of intrusive vs. This regime is characterised by a set of strong plates extrusive magmatism on the tectonic mode. separated by warm and weak regions generated by plutonism. Eclogitic drippings and lithospheric delaminations often occur around these weak regions. -
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. -
Environmental Effects of Large Igneous Province Magmatism: a Siberian Perspective Benjamin A
20 Environmental effects of large igneous province magmatism: a Siberian perspective benjamin a. black, jean-franc¸ois lamarque, christine shields, linda t. elkins-tanton and jeffrey t. kiehl 20.1 Introduction Even relatively small volcanic eruptions can have significant impacts on global climate. The eruption of El Chichón in 1982 involved only 0.38 km3 of magma (Varekamp et al., 1984); the eruption of Mount Pinatubo in 1993 involved 3–5km3 of magma (Westrich and Gerlach, 1992). Both these eruptions produced statistically significant climate signals lasting months to years. Over Earth’s his- tory, magmatism has occurred on vastly larger scales than those of the Pinatubo and El Chichón eruptions. Super-eruptions often expel thousands of cubic kilo- metres of material; large igneous provinces (LIPs) can encompass millions of cubic kilometres of magma. The environmental impact of such extraordinarily large volcanic events is controversial. In this work, we explore the unique aspects of LIP eruptions (with particular attention to the Siberian Traps), and the significance of these traits for climate and atmospheric chemistry during eruptive episodes. As defined by Bryan and Ernst (2008), LIPs host voluminous (> 100,000 km3) intraplate magmatism where the majority of the magmas are emplaced during short igneous pulses. The close temporal correlation between some LIP eruptions and mass extinction events has been taken as evidence supporting a causal relationship (Courtillot, 1994; Rampino and Stothers, 1988; Wignall, 2001); as geochronological data become increasingly precise, they have continued to indicate that this temporal association may rise above the level of coincidence (Blackburn et al., 2013). Several obstacles obscure the mechanisms that might link LIP magmatism with the degree of global environmental change sufficient to trigger mass extinction. -
Alcolapia Grahami ERSS
Lake Magadi Tilapia (Alcolapia grahami) Ecological Risk Screening Summary U.S. Fish & Wildlife Service, March 2015 Revised, August 2017, October 2017 Web Version, 8/21/2018 1 Native Range and Status in the United States Native Range From Bayona and Akinyi (2006): “The natural range of this species is restricted to a single location: Lake Magadi [Kenya].” Status in the United States No records of Alcolapia grahami in the wild or in trade in the United States were found. The Florida Fish and Wildlife Conservation Commission has listed the tilapia Alcolapia grahami as a prohibited species. Prohibited nonnative species (FFWCC 2018), “are considered to be dangerous to the ecology and/or the health and welfare of the people of Florida. These species are not allowed to be personally possessed or used for commercial activities.” Means of Introductions in the United States No records of Alcolapia grahami in the United States were found. 1 Remarks From Bayona and Akinyi (2006): “Vulnerable D2 ver 3.1” Various sources use Alcolapia grahami (Eschmeyer et al. 2017) or Oreochromis grahami (ITIS 2017) as the accepted name for this species. Information searches were conducted under both names to ensure completeness of the data gathered. 2 Biology and Ecology Taxonomic Hierarchy and Taxonomic Standing According to Eschmeyer et al. (2017), Alcolapia grahami (Boulenger 1912) is the current valid name for this species. It was originally described as Tilapia grahami; it has also been known as Oreoghromis grahami, and as a synonym, but valid subspecies, of -
PROF. GEORGE OKOYE KRHODA, CBS Department of Geography and Environmental Studies University of Nairobi P.O
PROF. GEORGE OKOYE KRHODA, CBS Department of Geography and Environmental Studies University of Nairobi P.O. Box 30197, 00100 Nairobi, KENYA Tel: +254 720 204 305; +254 733 454 216; +254 20-2017213 Fax: +254 020-2017213 Email: [email protected] PROFILE Prof. George Okoye Krhoda, CBS, is Associate Professor of Geography and Environmental Studies and Vice Chairman of the Daystar University Council. He is a Hydrologist/Water Resources Management specialist and has B.Ed.(Hons), M.A and Ph.D on River Hydraulics And Water Resources Planning. Krhoda is also the Managing Director of Research on Environment and Development Planning (REDPLAN) Consultants Ltd. Until December 2006, he was the Permanent Secretary, Ministry of Environment and Natural Resources and Chairman of the Negotiation Committee on the Nile Basin Cooperative Framework, and earlier Permanent Secretary in the Ministry of Water and Irrigation where most of the water sector reforms were carried under his watch. Currently finalizing “Environmental and social impact assessment (ESIA) for Akiira One Geothermal Power Energy in Rift Valley, having completed ESIA for Mount Suswa Geothermal Energy, Formulation of Kenya’s national Groundwater Policy; National Transboundary Water Resources Policy, and Outcome Evaluation of UNDP Rwanda Environment Programme”. Recently, Prof. Krhoda has been involved in “Development of the Mau Forest Complex Investment Programme”, “Lake Naivasha Conservation and Integrated Water Resources Management (IWRM) Programme” in developing, managing and evaluating -
Provenance and Implication of Carboniferous–Permian Detrital
minerals Article Provenance and Implication of Carboniferous–Permian Detrital Zircons from the Upper Paleozoic, Southern Ordos Basin, China: Evidence from U-Pb Geochronology and Hf Isotopes Ziwen Jiang 1, Jinglan Luo 1,*, Xinshe Liu 2,3, Xinyou Hu 2,3, Shangwei Ma 4, Yundong Hou 2,3, Liyong Fan 2,3 and Yuhua Hu 1 1 State Key Laboratory of Continental Dynamics, Department of Geology, Northwest University, Xi’an 710069, China; [email protected] (Z.J.); [email protected] (Y.H.) 2 State Engineering Laboratory of Exploration and Development for Low Permeability Oil and Gas Fields, Xi’an 710018, China; [email protected] (X.L.); [email protected] (X.H.); [email protected] (Y.H.); [email protected] (L.F.) 3 Research Institute of Petroleum Exploration and Development, PetroChina Changqing Oilfield Company, Xi’an 710018, China 4 Shaanxi Mineral Resources and Geological Survey, Xi’an 710068, China; [email protected] * Correspondence: [email protected] Received: 9 February 2020; Accepted: 13 March 2020; Published: 15 March 2020 Abstract: Carboniferous–Permian detrital zircons are recognized in the Upper Paleozoic of the whole Ordos Basin. Previous studies revealed that these Carboniferous–Permian zircons occurred in the Northern Ordos Basin mainly originated from the Yinshan Block. What has not been well documented until now is where this period’s zircons in the Southern Ordos Basin came from, and very little discussion about their provenance. To identify the provenance of the detrital zircons dating from ~350 to 260 Ma, five sandstone samples from the Shan 1 Member of Shanxi Formation and eight sandstone samples from the He 8 Member of Shihezi Formation were analyzed for detrital zircon U-Pb age dating and in situ Lu-Hf isotopic compositions. -
In Water Composition Due to Abstraction of Soda Ash. Impact
Chapter 6 - Lake Natron Soda Ash ESIA 6 - 8 in water composition due to abstraction of soda ash. Impact: Introduction of animal pests and pathogens to the Lake system Impact No. B/E 3 Changes in disease vector populations Ranking: Negative slight Characteristics: Domestic waste attracting pests. Abandoned borrow pits providing mosquito breeding sites. Increase in introduction of vectors through increased human and vehicle movement. Impact: Loss of fresh water habitats in the Lake due to dry season abstraction Impact No. B/E 4 Changes in aquatic biota Ranking: Negative slight Characteristics: Abstraction of surface water from the Wosi Wosi River Impact: The Cyperus laevigatus sedgelands surrounding the semi sodic springs in the southern and eastern sides of the Lake form critical late dry season grazing for domestic stock and wildlife. Increased pressure or disturbance could deplete the remaining wildlife populations Impact No. B/E 5 Changes in terrestrial plant populations Ranking: Negative moderate Characteristics: Access road along east side of the Lake would threaten the use of 400 ha of dry season grazing. This area has a stocking rate of at least 2.5 LSU/ha during he dry season Impact: Introduction of alien invasive plant and animal species Impact No. B/E 5 Changes in terrestrial plant (and animal) populations Ranking: Negative slight Characteristics: Concerns relating to construction activities, the development of domestic gardens, the introduction of brine shrimp into the process Impact: Illegal hunting activities will increase with human immigration into the area Impact No. B/E 6 Changes in terrestrial wildlife populations Ranking: Negative slight Characteristics: There is a present decline in rare wildlife species such as gerenuk and Coir bustard and local extinction of rhino and Oryx due to increased pressure on grazing resources and increased poaching. -
Geology Area South of Magadi
_£I Report No. 61 GOVERNMENT OF KENYA MINISTRY OF COMMERCE AND INDUSTRY GEOLOGICAL SURVEY OF KENYA GEOLOGY OF THE AREA SOUTH OF MAGADI DEGREE SHEET 58, N.W. QUARTER (with coloured geological map) by B. H. BAKER, B.Sc, F.G.S. Geologist Eight Shillings - 1963 "ISfiICrLIBSARY ïIE-- :i963l4 j». ^itfageningen _ .The'Netherlands Li / J Scanned from original by ISRIC - World Soil Information, as ICSU World Data Centre for Soils. The purpose is to make a safe depository for endangered documents and to make the accrued information available for consultation, following Fair Use Guidelines. Every effort is taken to respect Copyright of the materials within the archives where the identification of the Copyright holder is clear and, where feasible, to contact the originators. For questions please contact soil.isricPwur.nl indicating the item reference number concerned. GEOLOGY OF THE AREA SOUTH OF MAGADI DEGREE SHEET 58, N.W. QUARTER (with coloured geological map) by B. H. BAKER, B.Sc, F.G.S. Geologist 165^G FOREWORD The publication of the report on the geology of the area south of Magadi completes the account of the southern end of the Rift Valley as it occurs in Kenya. The Magadi area itself was described by Mr. Baker in Report No. 42 (1958). During the mapping of the continua tion of the Magadi area the discovery of some critical exposures enabled the correction of an error of succession in the lower Pleistocene rocks that had been made during the survey of the Magadi area. The area is wild and desolate, but of considerable interest scenically, with the western Rift wall a little beyond its west boundary, rugged hills of ancient rocks in the south-east and two prominent volcanoes, Lenderut and Shombole, rising from the Rift floor. -
Magma Genesis, Plate Tectonics, and Chemical Differentiation of the Earth
REVIEWS OF GEOPHYSICS, VOL. 26, NO. 3, PAGES 370-404, AUGUST 1988 Magma Genesis, Plate Tectonics, and Chemical Differentiation of the Earth PETER J. WYLLIE Division of Geolo•7icaland Planetary Sciences,California Institute of Technolo•Ty,Pasadena Magma genesis,migration, and eruption have played prominent roles in the chemical differentiation of the Earth. Plate tectonics has provided the framework of tectonic environments for different suites of igneousrocks and the dynamic mechanismsfor moving massesof rock into melting regions.Petrology is rooted in geophysics.Petrological and geophysicalprocesses are calibrated by the phase equilibria of the materials. The geochemistry of basalts and mantle xenoliths demonstrates that the mantle is hetero- geneous.The geochemical reservoirs are related to mantle convection, with interpretation of a mantle layered or stratified or peppered with blobs. Seismic tomography is beginning to reveal the density distribution of the mantle in three dimensions,and together with fluid mechanical models and interpreta- tion of the geoid, closer limits are being placed on mantle convection. Petrological cross sectionscon- structed for various tectonic environments by transferring phase boundaries for source rocks onto assumedthermal structuresprovide physical frameworks for consideration of magmatic and metasoma- tic events,with examplesbeing given for basalts,andesites, and granites at ocean-continentconvergent plate boundaries, basalts and nephelinitesfrom a thermal plume beneath Hawaii, kimberlites in cratons,