Geochemical Behavior of Chromium Tion in Ultramafic Rocks, Then Discuss
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The Evolution of a Heterogeneous Martian Mantle: Clues from K, P, Ti, Cr, and Ni Variations in Gusev Basalts and Shergottite Meteorites
Earth and Planetary Science Letters 296 (2010) 67–77 Contents lists available at ScienceDirect Earth and Planetary Science Letters journal homepage: www.elsevier.com/locate/epsl The evolution of a heterogeneous Martian mantle: Clues from K, P, Ti, Cr, and Ni variations in Gusev basalts and shergottite meteorites Mariek E. Schmidt a,⁎, Timothy J. McCoy b a Dept. of Earth Sciences, Brock University, St. Catharines, ON, Canada L2S 3A1 b Dept. of Mineral Sciences, National Museum of Natural History, Smithsonian Institution, Washington, DC 20560-0119, USA article info abstract Article history: Martian basalts represent samples of the interior of the planet, and their composition reflects their source at Received 10 December 2009 the time of extraction as well as later igneous processes that affected them. To better understand the Received in revised form 16 April 2010 composition and evolution of Mars, we compare whole rock compositions of basaltic shergottitic meteorites Accepted 21 April 2010 and basaltic lavas examined by the Spirit Mars Exploration Rover in Gusev Crater. Concentrations range from Available online 2 June 2010 K-poor (as low as 0.02 wt.% K2O) in the shergottites to K-rich (up to 1.2 wt.% K2O) in basalts from the Editor: R.W. Carlson Columbia Hills (CH) of Gusev Crater; the Adirondack basalts from the Gusev Plains have more intermediate concentrations of K2O (0.16 wt.% to below detection limit). The compositional dataset for the Gusev basalts is Keywords: more limited than for the shergottites, but it includes the minor elements K, P, Ti, Cr, and Ni, whose behavior Mars igneous processes during mantle melting varies from very incompatible (prefers melt) to very compatible (remains in the shergottites residuum). -
Uhm Phd 9230509 R.Pdf
INFORMATION TO USERS This manuscript has been reproduced from the microfilm master. UMI films the text directly from the original or copy submitted. Thus, some thesis and dissertation copies are in typewriter face, while others may be from any type of computer printer. The quality of this reproduction is dependent upon the quality of the copy submitted. Broken or indistinct print, colored or poor quality illustrations and photographs, print bleedthrough, substandard margins, and improper alignment can adversely affect reproduction. In the unlikely event that the author did not send UMI a complete manuscript and there are missing pages, these will be noted. Also, if unauthorized copyright material had to be removed, a note will indicate the deletion. Oversize materials (e.g., maps, drawings, charts) are reproduced by sectioning the original, beginning at the upper left-hand corner and continuing from left to right in equal sections with small overlaps. Each original is also photographed in one exposure and is included in reduced form at the back of the book. Photographs included in the original manuscript have been reproduced xerographically in this copy. Higher quality 6" x 9" black and white photographic prints are available for any photographs or illustrations appearing in this copy for an additional charge. Contact UMI directly to order. U·M·I University Microfilms International A Bell & Howetl truorrnanoo Company 300 North Zeeb Road. Ann Arbor. M148106-1346 USA 313,761-4700 800 521-0600 Order Number 9230509 Mid-ocean ridge magmatism: Style of mantle upwelling, partial melting, crustal level processes, and spreading rate dependence. A petrologic approach Niu, Yaoling, Ph.D. -
Geochemistry of Sideromelane and Felsic Glass Shards in Pleistocene Ash Layers at Sites 953, 954, and 9561
Weaver, P.P.E., Schmincke, H.-U., Firth, J.V., and Duffield, W. (Eds.), 1998 Proceedings of the Ocean Drilling Program, Scientific Results, Vol. 157 25. GEOCHEMISTRY OF SIDEROMELANE AND FELSIC GLASS SHARDS IN PLEISTOCENE ASH LAYERS AT SITES 953, 954, AND 9561 Andrey A. Gurenko2 and Hans-Ulrich Schmincke2 ABSTRACT Sideromelane and felsic glass shards from unconsolidated Pleistocene volcaniclastic sediments drilled at Sites 953, 954, and 956 are thought to have derived from submarine and subaerial volcanic eruptions on Gran Canaria (Sites 953 and 954) and Tenerife (Sites 954 and 956). We analyzed these glasses by electron microprobe for major elements and sulfur, chlorine, and fluorine. Sideromelane glasses represent a spectrum from alkali basalt through basanite, hawaiite, mugearite, and tephrite to nephelinite. Felsic glasses have compositions similar to benmoreite, trachyte, and phonolite. Vesiculated mafic and felsic glass shards, which are characterized by low S and Cl concentrations (0.01−0.06 wt% S and 0.01–0.04 wt% Cl), are interpreted to have formed by pyroclastic activity on land or in shallow water and appeared to have been strongly degassed. Vesicle-free blocky glass shards having 0.05−0.13 wt% S are likely to have resulted from submarine eruptions at moderate water depths and represent undegassed or slightly degassed magmas. Cl concentrations range from 0.01 to 0.33 wt% and increase with increasing MgO, suggesting that Cl behaves as an incompatible element during magma crystallization. Concentrations of fluorine (0.04− 0.34 wt% F) are likely to represent undegassed values, and the variations in F/K ratios between 0.02 and 0.24 are believed to reflect those of parental magmas and of the mantle source. -
Tardi-Magmatic Precipitation of Martian Fe/Mg-Rich Clay Minerals Via Igneous Differentiation
©2020TheAuthors Published by the European Association of Geochemistry ▪ Tardi-magmatic precipitation of Martian Fe/Mg-rich clay minerals via igneous differentiation J.-C. Viennet1*, S. Bernard1, C. Le Guillou2, V. Sautter1, P. Schmitt-Kopplin3, O. Beyssac1, S. Pont1, B. Zanda1, R. Hewins1, L. Remusat1 Abstract doi: 10.7185/geochemlet.2023 Mars is seen as a basalt covered world that has been extensively altered through hydrothermal or near surface water-rock interactions. As a result, all the Fe/Mg-rich clay minerals detected from orbit so far have been interpreted as secondary, i.e. as products of aqueous alteration of pre-existing silicates by (sub)surface water. Based on the fine scale petrographic study of the evolved mesostasis of the Nakhla mete- orite, we report here the presence of primary Fe/Mg-rich clay minerals that directly precipitated from a water-rich fluid exsolved from the Cl-rich parental melt of nakhlites during igneous differentiation. Such a tardi-magmatic precipitation of clay minerals requires much lower amounts of water compared to production via aque- ous alteration. Although primary Fe/Mg-rich clay minerals are minor phases in Nakhla, the contribution of such a process to Martian clay formation may have been quite significant during the Noachian given that Noachian magmas were richer in H2O. In any case, the present discovery justifies a re-evaluation of the exact origin of the clay minerals detected on Mars so far, with potential consequences for our vision of the early magmatic and climatic histories of Mars. Received 26 January 2020 | Accepted 27 May 2020 | Published 8 July 2020 Letter mafic crustal materials (Smith and Bandfield, 2012; Ehlmann and Edwards, 2014). -
Cr-Rich Spinels As Petrogenetic Indicators
American Mineralogist, Volume 73, pages 741-753, 1988 Cr-rich spinels as petrogeneticindicators: MORB-type lavas from the Lamont seamountchain, easternPacific J,trrns F. Ar.r-.c.N* Department of Geological Sciences,Northwestern University, Evanston, Illinois 60201, U.S.A. Rrcn.qno O. Sacr Department of Earth and Atmospheric Sciences,Purdue University, West Lafayette, Indiana 47907, U.S.A. Roonv Bxttzt Department of Geological Sciences,Northwestern University, Evanston, Illinois 60201, U.S.A. Ansrucr The composition and morphology of Cr-rich spinels in MORBs reflect and record pre- eruptive petrogeneticevents such as magma-chamberrecharge, fractionation, and magma mixing. In this paper we examine Cr-rich spinels in MORB-type lavas erupted from the near-ridge Lamont seamountsand from the adjacent East Pacific Rise crest at 10'N. The spinels studied are exclusively from quickly quenchedglassy to spherulitic flow margins. The host lavas are depleted [(LalSm)" < 0.57] and relatively primitive [Me/(Me + Fe2*) to 0.71, Cr to 460 ppml, with the most primitive samplesapproaching the composition of liquids in equilibrium with mantle peridotite. The spinelscover a wide range in Al and Cr contents,with spinel Cr/(Cr + Al) ranging from 0.20 to 0.54 for the entire suite. As in other depleted MORBs, TiO, and calculated FerO. contents in the spinels are low (0. 16- 0.85 and 5.5-9.2 wto/0,respectively). Contents of Al, Mg, and Fe of groundmassspinels strongly correlate with host-glasscomposition, but spinel Cr content shows little correla- tion with host-glassCr content. Castingof spinel compositions in terms of Mg-Fe'z*spinel- host liquid exchangeequilibria and in terms of the compositionally related crystallochem- ical effectson this exchangeshows that for a given lava suite derived from similar parental lavas, spinel Crl(Cr + Al) increasesand Mg/@g + Fe2+)decreases with the amount of Fe enrichment, Al depletion, and extent of fractionation [as representedby the normative ratio Diop/(Ol + Diop)l of the liquids in which they equilibrated. -
Nonexplosive and Explosive Magma/Wet-Sediment Interaction
Journal of Volcanology and Geothermal Research 181 (2009) 155–172 Contents lists available at ScienceDirect Journal of Volcanology and Geothermal Research journal homepage: www.elsevier.com/locate/jvolgeores Nonexplosive and explosive magma/wet-sediment interaction during emplacement of Eocene intrusions into Cretaceous to Eocene strata, Trans-Pecos igneous province, West Texas Kenneth S. Befus a,⁎, Richard E. Hanson a, Daniel P. Miggins b, John A. Breyer a, Arthur B. Busbey a a Department of Geology, Texas Christian University, Box 298830, Fort Worth, TX 76129, USA b U.S. Geological Survey, Denver Federal Center, Box 25046, Denver, CO 80225, USA article info abstract Article history: Eocene intrusion of alkaline basaltic to trachyandesitic magmas into unlithified, Upper Cretaceous Received 16 June 2008 (Maastrichtian) to Eocene fluvial strata in part of the Trans-Pecos igneous province in West Texas produced Accepted 22 December 2008 an array of features recording both nonexplosive and explosive magma/wet-sediment interaction. Intrusive Available online 13 January 2009 complexes with 40Ar/39Ar dates of ~47–46 Ma consist of coherent basalt, peperite, and disrupted sediment. Two of the complexes cutting Cretaceous strata contain masses of conglomerate derived from Eocene fluvial Keywords: deposits that, at the onset of intrusive activity, would have been N400–500 m above the present level of phreatomagmatism peperite exposure. These intrusive complexes are inferred to be remnants of diatremes that fed maar volcanoes during diatreme an early stage of magmatism in this part of the Trans-Pecos province. Disrupted Cretaceous strata along Trans-Pecos Texas diatreme margins record collapse of conduit walls during and after subsurface phreatomagmatic explosions. -
Analogues for Radioactive Waste For~1S •
PNL-2776 UC-70 3 3679 00049 3611 ,. NATURALLY OCCURRING GLASSES: ANALOGUES FOR RADIOACTIVE WASTE FOR~1S • Rodney C. Ewing Richard F. Haaker Department of Geology University of New Mexico Albuquerque, ~ew Mexico 87131 April 1979 Prepared for the U.S. Department of Energy under Contract EY-76-C-06-1830 Pacifi c i'lorthwest Laboratory Richland, Washington 99352 TABLE OF CONTENTS List of Tables. i i List of Figures iii Acknowledgements. Introduction. 3 Natural Glasses 5 Volcanic Glasses 9 Physical Properties 10 Compos i ti on . 10 Age Distributions 10 Alteration. 27 Devitrification 29 Hydration 32 Tekti tes. 37 Physical Properties 38 Composition . 38 Age Distributions . 38 Alteration, Hydration 44 and Devitrification Lunar Glasses 44 Summary . 49 Applications to Radioactive Waste Disposal. 51 Recommenda ti ons 59 References 61 Glossary 65 i LIST OF TABLES 1. Petrographic Properties of Natural Glasses 6 2. Average Densities of Natural Glasses 11 3. Density of Crystalline Rock and Corresponding Glass 11 4. Glass and Glassy Rocks: Compressibility 12 5. Glass and Glassy Rocks: Elastic Constants 13 6. Glass: Effect of Temperature on Elastic Constants 13 7. Strength of Hollow Cylinders of Glass Under External 14 Hydrostatic Pressure 8. Shearing Strength Under High Confining Pressure 14 9. Conductivity of Glass 15 10. Viscosity of Miscellaneous Glasses 16 11. Typical Compositions for Volcanic Glasses 18 12. Selected Physical Properties of Tektites 39 13. Elastic Constants 40 14. Average Composition of Tektites 41 15. K-Ar and Fission-Track Ages of Tektite Strewn Fields 42 16. Microprobe Analyses of Various Apollo 11 Glasses 46 17. -
Icelandic Hyaloclastite Tuffs Petrophysical Properties, Alteration and Geochemical Mobility
Icelandic Hyaloclastite Tuffs Petrophysical Properties, Alteration and Geochemical Mobility Hjalti Franzson Gudmundur H. Gudfinnsson Julia Frolova Helga M. Helgadóttir Bruce Pauly Anette K. Mortensen Sveinn P. Jakobsson Prepared for National Energy Authority and Reykjavík Energy ÍSOR-2011/064 ICELAND GEOSURVEY Reykjavík: Orkugardur, Grensásvegur 9, 108 Reykjavík, Iceland - Tel.: 528 1500 - Fax: 528 1699 Akureyri: Rangárvellir, P.O. Box 30, 602 Akureyri, Iceland - Tel.: 528 1500 - Fax: 528 1599 [email protected] - www.isor.is Report Project no.: 540105 Icelandic Hyaloclastite Tuffs Petrophysical Properties, Alteration and Geochemical Mobility Hjalti Franzson Gudmundur H. Gudfinnsson Julia Frolova Helga M. Helgadóttir Bruce Pauly Anette K. Mortensen Sveinn P. Jakobsson Prepared for National Energy Authority and Reykjavík Energy ÍSOR-2011/064 December 2011 Key page Report no. Date Distribution ÍSOR-2011/064 December 2011 Open Closed Report name / Main and subheadings Number of copies Icelandic Hyaloclastite Tuffs. Petrophysical Properties, Alteration 7 and Geochemical Mobility Number of pages 103 Authors Project manager Hjalti Franzson, Gudmundur H. Gudfinnsson, Julia Frolova, Hjalti Franzson Helga M. Helgadóttir, Bruce Pauly, Anette K. Mortensen and Sveinn P. Jakobsson Classification of report Project no. 540105 Prepared for National Energy Authority and Reykjavík Energy Cooperators Moscow University, University of California in Davis, Natural History Museum in Iceland Abstract This study attempts to define the properties of hyaloclastite formations which control their petrophysical characteristics during their progressive alteration. It is based on 140 tuffaceous cores from last glaciation to 2–3 m y. The water content shows a progressive increase with alteration to about 12%, which mainly is bound in the smectite and zeolite alteration minerals. -
Lunar Silica-Bearing Diorite: a Lithology from the Moon with Implications for Igneous Differentiation
50th Lunar and Planetary Science Conference 2019 (LPI Contrib. No. 2132) 2008.pdf LUNAR SILICA-BEARING DIORITE: A LITHOLOGY FROM THE MOON WITH IMPLICATIONS FOR IGNEOUS DIFFERENTIATION. T. J. Fagan1* and S. Ohkawa1, 1Dept. Earth Sci., Waseda Univ., 1-6-1 Nishi- waseda, Shinjuku, Tokyo, 169-8050, Japan (*[email protected]). Introduction: Silica-rich igneous (“granitic”) ratios and relatively high F concentrations indicate that rocks are rare on the Moon, but have been detected by the analyzed grains are apatite (not merrillite). remote sensing on the lunar surface [e.g., 1], and in Results: The silica-bearing diorite (Sil-Di) is dom- Apollo samples and lunar meteorites [e.g., 2-5]. To date, inated by pyroxene (55 mode%), plagioclase feldspar lunar granitic samples have been characterized by high (36%), silica (4.4%), ilmenite (3.9%) and K-feldspar concentrations of incompatible elements and/or mafic (0.3%) (Fig. 2). Apatite and troilite also occur. The Sil- silicates with high Fe# (atomic Fe/[Fe+Mg]x100) [2-5], Di exhibits interlocking, igneous textures with elongate both features consistent with origin from late-stage re- plagioclase feldspar (Fig. 2). Plagioclase feldspar has sidual liquids or very low degree partial melting. Fur- nearly constant composition of An88Ab11, but pyroxene thermore, silica-rich rocks detected by remote sensing has a wide range of zoning (Fig. 3). often combine the Christiansen feature in infra-red spec- The modal composition of the Sil-Di is plagioclase- tra with high incompatible element concentrations (e.g., rich compared to many silica-bearing igneous rocks Th detected by gamma-ray spectroscopy [1]), again re- from the Moon (Fig. -
3.18 Oneviewofthegeochemistryof Subduction-Related Magmatic Arcs
3.18 OneView of the Geochemistry of Subduction-Related Magmatic Arcs, with an Emphasis on Primitive Andesite and Lower Crust P. B. Ke l e m e n Columbia University, Palisades, NY, USA K. HanghÖj Lamont-Doherty Earth Observatory of Columbia University, Palisades, NY,USA and A. R. Greene University of British Columbia,Vancouver, BC, Canada 3.18.1 INTRODUCTION 2 3.18.1.1 Definition of Terms Used in This Chapter 2 3.18.2 ARC LAVA COMPILATION 3 3.18.3 CHARACTERISTICS OF ARC MAGMAS 7 3.18.3.1 Comparison with MORBs 7 3.18.3.1.1 Major elements 7 3.18.3.1.2 We are cautious about fractionation correction of major elements 9 3.18.3.1.3 Distinctive, primitive andesites 11 3.18.3.1.4 Major elements in calc-alkaline batholiths 11 3.18.3.2 Major and Trace-Element Characteristics of Primitive Arc Magmas 18 3.18.3.2.1 Primitive basalts predominate 18 3.18.3.2.2 Are some low Mgx basalts primary melts? Perhaps not 22 3.18.3.2.3 Boninites, briefly 22 3.18.3.2.4 Primitive andesites: a select group 23 3.18.3.2.5 Three recipes for primitive andesite 23 3.18.3.3 Trace Elements, Isotopes, and Source Components in Primitive Magmas 29 3.18.3.3.1 Incompatible trace-element enrichment 29 3.18.3.3.2 Tantalum and niobium depletion 36 3.18.3.3.3 U-series isotopes 37 3.18.3.3.4 Geodynamic considerations 40 3.18.4 ARC LOWER CRUST 43 3.18.4.1 Talkeetna Arc Section 43 3.18.4.1.1 Geochemical data from the Talkeetna section 45 3.18.4.1.2 Composition, fractionation, and primary melts in the Talkeetna section 49 3.18.4.2 Missing Primitive Cumulates: Due to Delamination 52 3.18.4.3 -
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Isotope geochemistry of basaltic glasses from the Vance Seamounts, a near-ridge seamount chain adjacent to the Juan de Fuca Ridge Elizabeth Anne Cornejo B.Sc.H. Geology A thesis submitted to the School of Graduate Studies in partial fulfillment of the degree of Master of Science Department of Earth Sciences Carleton University April 2008 Ottawa, Ontario © Elizabeth Cornejo, 2008 Library and Bibliotheque et 1*1 Archives Canada Archives Canada Published Heritage Direction du Branch Patrimoine de I'edition 395 Wellington Street 395, rue Wellington Ottawa ON K1A0N4 Ottawa ON K1A0N4 Canada Canada Your file Votre reference ISBN: 978-0-494-44120-6 Our file Notre reference ISBN: 978-0-494-44120-6 NOTICE: AVIS: The author has granted a non L'auteur a accorde une licence non exclusive exclusive license allowing Library permettant a la Bibliotheque et Archives and Archives Canada to reproduce, Canada de reproduire, publier, archiver, publish, archive, preserve, conserve, sauvegarder, conserver, transmettre au public communicate to the public by par telecommunication ou par Plntemet, prefer, telecommunication or on the Internet, distribuer et vendre des theses partout dans loan, distribute and sell theses le monde, a des fins commerciales ou autres, worldwide, for commercial or non sur support microforme, papier, electronique commercial purposes, in microform, et/ou autres formats. paper, electronic and/or any other formats. The author retains copyright L'auteur conserve la propriete du droit d'auteur ownership and moral rights in et des droits moraux qui protege cette these. this thesis. Neither the thesis Ni la these ni des extraits substantiels de nor substantial extracts from it celle-ci ne doivent etre imprimes ou autrement may be printed or otherwise reproduits sans son autorisation. -
29. Sulfur Isotope Ratios of Leg 126 Igneous Rocks1
Taylor, B., Fujioka, K., et al., 1992 Proceedings of the Ocean Drilling Program, Scientific Results, Vol. 126 29. SULFUR ISOTOPE RATIOS OF LEG 126 IGNEOUS ROCKS1 Peter Torssander2 ABSTRACT Sulfur isotope ratios have been determined in 19 selected igneous rocks from Leg 126. The δ34S of the analyzed rocks ranges from -0.1 o/00 to +19.60 o/oo. The overall variation in sulfur isotope composition of the rocks is caused by varying degrees of seawater alteration. Most of the samples are altered by seawater and only five of them are considered to have maintained their magmatic sulfur isotope composition. These samples are all from the backarc sites and have δ34S values varying from +0.2 o/oo to +1.6 o/oo , of which the high δ34S values suggest that the earliest magmas in the rift are more arc-like in their sulfur isotope composition than the later magmas. The δ34S values from the forearc sites are similar to or heavier than the sulfur isotope composition of the present arc. INTRODUCTION from 0 o/oo to +9 o/00 (Ueda and Sakai, 1984), which could arise from inhomogeneities in the mantle but are more likely a result of contami- Sulfur is a volatile element that can be degassed during the ascent nation from the subducting slab (A. Ueda, pers. comm., 1988). of basaltic magma. Degassing causes sulfur isotope fractionation; the Leg 126 of the Ocean Drilling Program (ODP) drilled seven sites isotopic composition of sulfur in rocks can vary with the concentra- in the backarc and forearc of the Izu-Bonin Arc (Fig.