Physics and Chemistry of Mantle Plumes
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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. -
Chemical Composition of Earth's Primitive Mantle and Its Variance: 2
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 112, B03212, doi:10.1029/2005JB004224, 2007 Click Here for Full Article Chemical composition of Earth’s primitive mantle and its variance: 2. Implications for global geodynamics Tanya Lyubetskaya1 and Jun Korenaga1 Received 16 December 2005; revised 17 June 2006; accepted 20 November 2006; published 29 March 2007. [1] The global budgets of argon and heat-producing elements have traditionally been used to argue for layered-mantle convection because they require a large fraction of Earth’s mantle to remain isolated from mantle convection. We revise these mass balance arguments using our new composition model of the primitive mantle and show that the global budgets of argon, heat-producing elements, and rare earth elements are consistent with Earth’s mantle almost entirely composed of the mid-ocean ridge basalt source mantle, supporting the notion of whole mantle convection. Combined with a recent theory on the thermal evolution of Earth, our revised thermal budget implies inefficient mixing and processing in the past, explaining the survival of long-lived geochemical heterogeneities in convecting mantle. Citation: Lyubetskaya, T., and J. Korenaga (2007), Chemical composition of Earth’s primitive mantle and its variance: 2. Implications for global geodynamics, J. Geophys. Res., 112, B03212, doi:10.1029/2005JB004224. 1. Introduction arguments do not provide a robust constraint on the size of such a hidden reservoir, because the interpretation of [2] The structure of mantle convection has been one of geochemical data is often model-dependent. For example, the most controversial subjects in modern geodynamics and observed geochemical differences between mantle-derived geochemistry. -
Mantle Plumes
Geol. 655 Isotope Geochemistry Lecture 21 Spring 2007 ISOTOPIC EVOLUTION OF THE MANTLE IV THE ORIGIN OF MANTLE PLUMES AND THE COMMON COMPONENT IN PLUMES Determining how the various geochemical reservoirs of the mantle have evolved is among the most vexing problems in geochemistry. The principal observation to be explained is that mantle plumes in- variably have less depleted isotopic signatures than MORB, and the isotopic compositions of some in- dicate net enrichment in incompatible elements. As we saw in the previous lecture, mantle plumes were initially thought to consist of primitive mantle (e.g., Schilling, 1973). As we found, mixing be- tween primitive and depleted mantle can explain the Sr and Nd isotopic compositions of some plumes, but virtually none of the Pb isotope data can be explained this way, nor are the trace element composi- tions of OIB consistent with plumes being composed of primitive mantle. Indeed, although ‘primitive mantle’ has proved to be a useful hypothetical concept, no mantle-derived basalts or xenoliths have appropriate compositions to be ‘primitive mantle’ or derived from it. It is possible that no part of the mantle retains its original, primitive, composition (on the other hand, to have survived, primitive man- tle must not participate in volcanism and other such processes, so the absence of evidence for a primi- tive mantle reservoir is not evidence of its absence). Hofmann and White (1982) suggested mantle plumes obtain their unique geochemical signature through deep recycling of oceanic crust (Figure 21.1). Partial melting at mid-ocean ridges creates oce- anic crust that is less depleted in incompatible elements than the depleted upper mantle. -
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. -
Chemical Composition of Earth's Primitive Mantle and Its Variance
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 112, B03211, doi:10.1029/2005JB004223, 2007 Click Here for Full Article Chemical composition of Earth’s primitive mantle and its variance: 1. Method and results Tanya Lyubetskaya1 and Jun Korenaga1 Received 16 December 2005; revised 17 June 2006; accepted 20 November 2006; published 29 March 2007. [1] We present a new statistical method to construct a model for the chemical composition of Earth’s primitive mantle along with its variance. Earth’s primitive mantle is located on the melting trend exhibited by the global compilation of mantle peridotites, using cosmochemical constraints on the relative abundances of refractory lithophile elements (RLE). This so-called pyrolite approach involves the least amount of assumptions, thereby being probably most satisfactory compared to other approaches. Its previous implementations, however, suffer from questionable statistical treatment of noisy geochemical data, leaving the uncertainty of model composition poorly quantified. In order to properly take into account how scatters in peridotite data affect this geochemical inference, we combine the following statistical techniques: (1) modeling a nonlinear melting trend in the multidimensional compositional space through the principal component analysis, (2) determining the primitive mantle composition on the melting trend by simultaneously imposing all of cosmochemical constraints with least squares, and (3) mapping scatters in original data into the variance of the final model through the bootstrap resampling technique. Whereas our model is similar to previous models in terms of Mg, Si, and Fe abundances, the RLE contents are at 2.16 ± 0.37 times the CI chondrite concentration, which is lower than most of previous estimates. -
2.01 Cosmochemical Estimates of Mantle Composition H
2.01 Cosmochemical Estimates of Mantle Composition H. Palme Universita¨tzuKo¨ln, Germany and Hugh St. C. O’Neill Australian National University, Canberra, ACT, Australia 2.01.1 INTRODUCTION AND HISTORICAL REMARKS 1 2.01.2 THE COMPOSITION OF THE EARTH’S MANTLE AS DERIVED FROM THE COMPOSITION OF THE SUN 3 2.01.3 THE CHEMICAL COMPOSITION OF CHONDRITIC METEORITES AND THE COSMOCHEMICAL CLASSIFICATION OF ELEMENTS 4 2.01.4 THE COMPOSITION OF THE PRIMITIVE MANTLE BASED ON THE ANALYSIS OF UPPER MANTLE ROCKS 6 2.01.4.1 Rocks from the Mantle of the Earth 6 2.01.4.2 The Chemical Composition of Mantle Rocks 7 2.01.4.2.1 Major element composition of the Earth’s primitive mantle 11 2.01.4.2.2 Comparison with other estimates of PM compositions 13 2.01.4.2.3 Abundance table of the PM 13 2.01.4.3 Is the Upper Mantle Composition Representative of the Bulk Earth Mantle? 20 2.01.5 COMPARISON OF THE PM COMPOSITION WITH METEORITES 21 2.01.5.1 Refractory Lithophile Elements 21 2.01.5.2 Refractory Siderophile Elements 23 2.01.5.3 Magnesium and Silicon 24 2.01.5.4 The Iron Content of the Earth 25 2.01.5.5 Moderately Volatile Elements 26 2.01.5.5.1 Origin of depletion of moderately volatile elements 28 2.01.5.6 HSEs in the Earth’s Mantle 31 2.01.5.7 Late Veneer Hypothesis 32 2.01.6 THE ISOTOPIC COMPOSITION OF THE EARTH 33 2.01.7 SUMMARY 34 REFERENCES 35 2.01.1 INTRODUCTION AND HISTORICAL scientists begin to consider Chladni’s hypothesis REMARKS seriously. -
A New Insight Into the Hawaiian Plume
Earth and Planetary Science Letters 241 (2006) 438–453 www.elsevier.com/locate/epsl A new insight into the Hawaiian plume Jianshe Lei *, Dapeng Zhao Geodynamics Research Centre, Ehime University, Japan Received 19 June 2005; received in revised form 22 November 2005; accepted 27 November 2005 Available online 5 January 2006 Editor: S. King Abstract Although many geochemical, geophysical and seismological studies have suggested that the Hawaiian mantle plume originates from the core–mantle boundary (CMB), so far no tomographic model shows a continuous image of the Hawaiian plume in the entire mantle because of the few seismic stations on the narrow Hawaiian island chain. Here we present a new tomographic image beneath Hawaii determined by using simultaneously 10 kinds of seismic phases, P, pP, PP, PcP, Pdiff, PKPab, PKPbc, PKiKP, PKKPab and PKKPbc, extracted from the data set compiled by the International Seismological Center. Of these phases, PKiKP, PKKPab and PKKPbc are, for the first time, attempted to use in the global seismic tomography. Our results show a slow anomaly beneath Hawaii ascending continuously from the CMB to the surface, implying that the Hawaiian plume indeed originates from the CMB. This image is improved notably over the previous results in the whole mantle, particularly in and below the middle mantle, suggesting that later phases, PP, Pdiff, PKP and particularly PKiKP, are of great importance for better imaging the Hawaiian plume. This slow anomaly is considered to be a plume conduit being tilted, which is likely caused by the mantle flow. This indicates that the position of the Hawaiian hotspot on the surface is not stationary, as evidenced by the recent paleomagnetic and numerical modeling studies. -
Mantle Plumes
CORE CONCEPTS CORE CONCEPTS Mantle plumes Charles Choi The potential importance of mantle plumes Science Writer may go well beyond explaining volcanism within plates. For example, the mantle plume that may lie under Réunion Island in the Indian Ocean has apparently burned Volcanoes are usually found near the borders volcanoes, which dwell more than 2,000 a track of volcanic activity that reaches of tectonic plates that are violently either miles (3,200 km) from the nearest plate about 3,400 miles (5,500 km) northward pushing or pulling at each other. Mysteri- boundary. Scientists think that as the Pacific to the Deccan Plateau region of what is ously, however, volcanoes sometimes erupt plate slid over a “hot spot,” a line of volca- now India. Catastrophic volcanism there in the middle of these plates instead. The 65 million years ago gushed lava across noes blossomed. 2 culprits behind these outbursts might be In 1971, geophysicist W. Jason Morgan 580,000 square miles (1.5 million km ), giant pillars of hot molten rock known as proposed that hot spots resulted from plumes more than twice the area of Texas, po- mantle plumes, jets of magma rising up of magma originating in the lower mantle tentially hastening the end of the age of from near the Earth’s core to penetrate over- dinosaurs. near the Earth’scoreatdepthsofmorethan lying material like a blowtorch. Still, decades However, it remains hotly debated whether after mantle plumes were first proposed, 1,550 miles (2,500 km). Researchers think mantle plumes exist. For example, Massa- controversy remains as to whether or not these mantle plumes are shaped like mush- chusetts Institute of Technology seismologist they exist. -
Mantle Plumes and Their Role in Earth Processes
REVIEWS Mantle plumes and their role in Earth processes Anthony A. P. Koppers 1 ✉ , Thorsten W. Becker 2, Matthew G. Jackson 3, Kevin Konrad 1,4, R. Dietmar Müller 5, Barbara Romanowicz6,7,8, Bernhard Steinberger 9,10 and Joanne M. Whittaker 11 Abstract | The existence of mantle plumes was first proposed in the 1970s to explain intra-plate, hotspot volcanism, yet owing to difficulties in resolving mantle upwellings with geophysical images and discrepancies in interpretations of geochemical and geochronological data, the origin, dynamics and composition of plumes and their links to plate tectonics are still contested. In this Review, we discuss progress in seismic imaging, mantle flow modelling, plate tectonic reconstructions and geochemical analyses that have led to a more detailed understanding of mantle plumes. Observations suggest plumes could be both thermal and chemical in nature, can attain complex and broad shapes, and that more than 18 plumes might be rooted in regions of the lowermost mantle. The case for a deep mantle origin is strengthened by the geochemistry of hotspot volcanoes that provide evidence for entrainment of deeply recycled subducted components, primordial m an tle domains and, potentially, materials from Earth’s core. Deep mantle plumes often appear deflected by large-scale mantle flow, resulting in hotspot motions required to resolve past tectonic plate motions. Future research requires improvements in resolution of seismic tomography to better visualize deep mantle plume structures at smaller than 100-km scales. Concerted multi-proxy geochemical and dating efforts are also needed to better resolve spatiotemporal and chemical evolutions of long-lived mantle plumes.