Appendix D Volcanic Materials: Science Language for Their Naming and Characterization in Digital Geologic- Map Databases
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UC Berkeley Archaeological X-Ray Fluorescence Reports
UC Berkeley Archaeological X-ray Fluorescence Reports Title X-Ray Fluorescence (XRF) Analysis Major Oxide and Trace Element Concentrations of Mainly Volcanic Rock Artifacts from a Number of Sites in Central Arizona Permalink https://escholarship.org/uc/item/7pt4r7vt Author Shackley, M. Steven Publication Date 2013-07-10 Supplemental Material https://escholarship.org/uc/item/7pt4r7vt#supplemental License https://creativecommons.org/licenses/by-nc/4.0/ 4.0 eScholarship.org Powered by the California Digital Library University of California www.escholarship.org/uc/item/7pt4r7vt GEOARCHAEOLOGICAL X-RAY FLUORESCENCE SPECTROMETRY LABORATORY 8100 WYOMING BLVD., SUITE M4-158 ALBUQUERQUE, NM 87113 USA X-RAY FLUORESCENCE (XRF) ANALYSIS MAJOR OXIDE AND TRACE ELEMENT CONCENTRATIONS OF MAINLY VOLCANIC ROCK ARTIFACTS FROM A NUMBER OF SITES IN CENTRAL ARIZONA Probable Cienega Large and San Pedro points from the collection by M. Steven Shackley Ph.D., Director Geoarchaeological XRF Laboratory Albuquerque, New Mexico Report Prepared for Dr. Anna Neuzil EcoPlan Associates, Inc. Tucson, Arizona 10 July 2013 www.escholarship.org/uc/item/7pt4r7vt INTRODUCTION The analysis here of artifacts mainly produced from high silica rhyolite is an attempt to provide a beginning data base for further artifact provenance studies in central Arizona. An intensive oxide and trace element analysis of the artifacts indicates a strong preference for high silica volcanics for the production of stone tools including dart points such as the ones figured on the cover page. None of the artifacts can be assigned to source at this time. The assemblage appears to be a Late Archaic/Cienega Phase assemblage rather typical of the region (Sliva 2...). -
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. -
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. -
Derivation of Intermediate to Silicic Magma from the Basalt Analyzed at the Vega 2 Landing Site, Venus
RESEARCH ARTICLE Derivation of intermediate to silicic magma from the basalt analyzed at the Vega 2 landing site, Venus J. Gregory Shellnutt* National Taiwan Normal University, Department of Earth Sciences, Taipei, Taiwan * [email protected] Abstract a1111111111 a1111111111 Geochemical modeling using the basalt composition analyzed at the Vega 2 landing site a1111111111 indicates that intermediate to silicic liquids can be generated by fractional crystallization and a1111111111 equilibrium partial melting. Fractional crystallization modeling using variable pressures (0.01 a1111111111 GPa to 0.5 GPa) and relative oxidation states (FMQ 0 and FMQ -1) of either a wet (H2O = 0.5 wt%) or dry (H2O = 0 wt%) parental magma can yield silicic (SiO2 > 60 wt%) composi- tions that are similar to terrestrial ferroan rhyolite. Hydrous (H2O = 0.5 wt%) partial melting can yield intermediate (trachyandesite to andesite) to silicic (trachydacite) compositions at OPEN ACCESS all pressures but requires relatively high temperatures ( 950ÊC) to generate the initial melt Citation: Shellnutt JG (2018) Derivation of at intermediate to low pressure whereas at high pressure (0.5 GPa) the first melts will be intermediate to silicic magma from the basalt generated at much lower temperatures (< 800ÊC). Anhydrous partial melt modeling yielded analyzed at the Vega 2 landing site, Venus. PLoS mafic (basaltic andesite) and alkaline compositions (trachybasalt) but the temperature ONE 13(3): e0194155. https://doi.org/10.1371/ journal.pone.0194155 required to produce the first liquid is very high ( 1130ÊC). Consequently, anhydrous partial melting is an unlikely process to generate derivative liquids. The modeling results indicate Editor: Axel K Schmitt, Heidelberg University, GERMANY that, under certain conditions, the Vega 2 composition can generate silicic liquids that pro- duce granitic and rhyolitic rocks. -
Alkalic-Type Epithermal Gold Deposit Model
Alkalic-Type Epithermal Gold Deposit Model Chapter R of Mineral Deposit Models for Resource Assessment Scientific Investigations Report 2010–5070–R U.S. Department of the Interior U.S. Geological Survey Cover. Photographs of alkalic-type epithermal gold deposits and ores. Upper left: Cripple Creek, Colorado—One of the largest alkalic-type epithermal gold deposits in the world showing the Cresson open pit looking southwest. Note the green funnel-shaped area along the pit wall is lamprophyre of the Cresson Pipe, a common alkaline rock type in these deposits. The Cresson Pipe was mined by historic underground methods and produced some of the richest ores in the district. The holes that are visible along several benches in the pit (bottom portion of photograph) are historic underground mine levels. (Photograph by Karen Kelley, USGS, April, 2002). Upper right: High-grade gold ore from the Porgera deposit in Papua New Guinea showing native gold intergrown with gold-silver telluride minerals (silvery) and pyrite. (Photograph by Jeremy Richards, University of Alberta, Canada, 2013, used with permission). Lower left: Mayflower Mine, Montana—High-grade hessite, petzite, benleonardite, and coloradoite in limestone. (Photograph by Paul Spry, Iowa State University, 1995, used with permission). Lower right: View of north rim of Navilawa Caldera, which hosts the Banana Creek prospect, Fiji, from the portal of the Tuvatu prospect. (Photograph by Paul Spry, Iowa State University, 2007, used with permission). Alkalic-Type Epithermal Gold Deposit Model By Karen D. Kelley, Paul G. Spry, Virginia T. McLemore, David L. Fey, and Eric D. Anderson Chapter R of Mineral Deposit Models for Resource Assessment Scientific Investigations Report 2010–5070–R U.S. -
USGS Professional Paper 1692
USG S Eruptive History and Chemical Evolution of the Precaldera and Postcaldera Basalt-Dacite Sequences, Long Valley, California: Implications for Magma Sources, Current Seismic Unrest, and Future Volcanism Professional Paper 1692 U.S. Department of the Interior U.S. Geological Survey This page intentionally left blank Eruptive History and Chemical Evolution of the Precaldera and Postcaldera Basalt-Dacite Sequences, Long Valley, California: Implications for Magma Sources, Current Seismic Unrest, and Future Volcanism By Roy A. Bailey Professional Paper 1692 U.S. Department of the Interior U.S. Geological Survey ii U.S. Department of the Interior Gale A. Norton, Secretary U.S. Geological Survey Charles G. Groat, Director U.S. Geological Survey, Reston, Virginia: 2004 For sale by U.S. Geological Survey Information Services Box 25286, Denver Federal Center Denver, CO 80225 This report and any updates to it are available online at: http://pubs.usgs.gov//pp/p1692/ Additional USGS publications can be found at: http://geology.usgs.gov/products.html For more information about the USGS and its products: Telephone: 1–888–ASK–USGS (1–888–275–8747) World Wide Web: http://www.usgs.gov/ Any use of trade, product, or firm names in this publication is for descriptive purposes only and does not imply endorsement of the U.S. Government. Although this report is in the public domain, it contains copyrighted materials that are noted in the text. Permission to reproduce those items must be secured from the individual copyright owners. Cataloging-in-publication data are on file with the Library of Congress (URL http://www.loc.gov/). -
Comparison of Hawaiian Basalts By: Alex Van Ningen and Adam Sagaser Geology 422: Petrology 5/2/2014 Introduction
COMPARISON OF HAWAIIAN BASALTS BY: ALEX VAN NINGEN AND ADAM SAGASER GEOLOGY 422: PETROLOGY 5/2/2014 INTRODUCTION • The Hawaiian Islands were formed as a result of the Pacific Plate moving Northwest over a hotspot in the Earth’s mantle. • The islands in the southeast are the youngest and most volcanically active. • Hawai’i (the Big Island) is composed of a group of five volcanoes, with Mauna Loa being the world’s largest volcano and Kilauea being the world’s most active volcano (Saini-eidukat and Schwert, 2013). Image Source: U.S.G.S. Kauai Niihau Oahu Molokai Lanai Maui Kahoolawe Hawai’i Photo coutesy of: NASA HAWAI’I (THE BIG ISLAND) • Two samples were obtained from the big island. Sample 130309 was obtained from Kohala and sample 130315 was obtained from Hualalai. • Our initial hypothesis was that the sample from Kohala is a benmorite, and the sample from Hualalai is a basalt. Image source: U.S.G.S. RESEARCH & METHODS Sample: 130315 • To begin, we took our samples and put them in a jaw crusher. • For sample number 130315, there was some olivine and calcite that may have formed as a xenolith. An attempt was made to remove as much of the secondary minerals as possible. Sample: 130309 • Both samples were taken to Dr. Lewis’s lab, where a ring pulverizer was used to grind the fragments into a powder. • Thin sections were also prepared for conceptual purposes. RESEARCH & METHODS • Both sets of powder underwent loss on ignition (LOI) in a muffle furnace. This was initially done at 105⁰C. -
Fingerprints of Kamafugite-Like Magmas in Mesozoic Lamproites of the Aldan Shield: Evidence from Olivine and Olivine-Hosted Inclusions
minerals Article Fingerprints of Kamafugite-Like Magmas in Mesozoic Lamproites of the Aldan Shield: Evidence from Olivine and Olivine-Hosted Inclusions Ivan F. Chayka 1,2,*, Alexander V. Sobolev 3,4, Andrey E. Izokh 1,5, Valentina G. Batanova 3, Stepan P. Krasheninnikov 4 , Maria V. Chervyakovskaya 6, Alkiviadis Kontonikas-Charos 7, Anton V. Kutyrev 8 , Boris M. Lobastov 9 and Vasiliy S. Chervyakovskiy 6 1 V. S. Sobolev Institute of Geology and Mineralogy Siberian Branch of the Russian Academy of Sciences, 630090 Novosibirsk, Russia; [email protected] 2 Institute of Experimental Mineralogy, Russian Academy of Sciences, 142432 Chernogolovka, Russia 3 Institut des Sciences de la Terre (ISTerre), Université de Grenoble Alpes, 38041 Grenoble, France; [email protected] (A.V.S.); [email protected] (V.G.B.) 4 Vernadsky Institute of Geochemistry and Analytical Chemistry, Russian Academy of Sciences, Moscow, Russia; [email protected] 5 Department of Geology and Geophysics, Novosibirsk State University, 630090 Novosibirsk, Russia 6 Institute of Geology and Geochemistry, Ural Branch of the Russian Academy of Sciences, 620016 Yekaterinburg, Russia; [email protected] (M.V.C.); [email protected] (V.S.C.) 7 School of Chemical Engineering and Advanced Materials, The University of Adelaide, Adelaide, SA 5005, Australia; [email protected] 8 Institute of Volcanology and Seismology, Far Eastern Branch of the Russian Academy of Sciences, 683000 Petropavlovsk-Kamchatsky, Russia; [email protected] 9 Institute of Mining, Geology and Geotechnology, Siberian Federal University, 660041 Krasnoyarsk, Russia; [email protected] * Correspondence: [email protected]; Tel.: +7-985-799-4936 Received: 17 February 2020; Accepted: 6 April 2020; Published: 9 April 2020 Abstract: Mesozoic (125–135 Ma) cratonic low-Ti lamproites from the northern part of the Aldan Shield do not conform to typical classification schemes of ultrapotassic anorogenic rocks. -
THE PETROCHEMISTRY of JAKE M: a MARTIAN MUGEARITE. Stolper
44th Lunar and Planetary Science Conference (2013) 1685.pdf THE PETROCHEMISTRY OF JAKE_M: A MARTIAN MUGEARITE. Stolper, E.M.1, Baker, M.B.1, Fisk, M.2, Gellert, R.3, King, P.L.4, McLennan, S.M.5, Minitti, M.6, Newcombe, M.1, Schmidt, M.E. 7, Treiman, A.H.8, and the MSL Science Team. 1Caltech, Pasadena, CA 91125, 2Oregon State Univ., 3Univ. Guelph, 4Res. School Earth Sci., ANU, 5SUNY, Stony Brook, 6Applied Phys. Lab., Johns Hopkins Univ., 7Brock Univ., 8Lunar & Planet. Inst. Introduction: Rock “Jake_M” (JM; named for JPL The surface of JM was not brushed or abraded prior engineer Jake Matijevic) was the first sample analyzed to analysis, so the APXS analyses probably include by the Alpha Particle X-ray Spectrometer (APXS) in- contributions from surface coatings, including adhering strument on MSL [1]. Although it is an isolated frag- dust, and these are the probable source of the S and Cl ment lacking field context, its dark color and apparently in JM. Experience with MER, however, indicates that fine-grained texture suggested it was a relatively homo- the characteristics of rock compositions are typically geneous igneous rock and thus an appropriate sample to not obscured by surface components, and the levels of S initiate the APXS analytical program. We report here and Cl in JM are lower than virtually all unbrushed the preliminary APXS analyses of JM and a plausible analyses from the Spirit rover and lower than many of interpretation of their significance for petrogenesis. the brushed analyses, so the level of surface contamina- Results: Three spots on JM were analyzed with the tion and alteration are likely relatively minor [5]. -
Lunar Crater Volcanic Field (Reveille and Pancake Ranges, Basin and Range Province, Nevada, USA)
Research Paper GEOSPHERE Lunar Crater volcanic field (Reveille and Pancake Ranges, Basin and Range Province, Nevada, USA) 1 2,3 4 5 4 5 1 GEOSPHERE; v. 13, no. 2 Greg A. Valentine , Joaquín A. Cortés , Elisabeth Widom , Eugene I. Smith , Christine Rasoazanamparany , Racheal Johnsen , Jason P. Briner , Andrew G. Harp1, and Brent Turrin6 doi:10.1130/GES01428.1 1Department of Geology, 126 Cooke Hall, University at Buffalo, Buffalo, New York 14260, USA 2School of Geosciences, The Grant Institute, The Kings Buildings, James Hutton Road, University of Edinburgh, Edinburgh, EH 3FE, UK 3School of Civil Engineering and Geosciences, Newcastle University, Newcastle, NE1 7RU, UK 31 figures; 3 tables; 3 supplemental files 4Department of Geology and Environmental Earth Science, Shideler Hall, Miami University, Oxford, Ohio 45056, USA 5Department of Geoscience, 4505 S. Maryland Parkway, University of Nevada Las Vegas, Las Vegas, Nevada 89154, USA CORRESPONDENCE: gav4@ buffalo .edu 6Department of Earth and Planetary Sciences, 610 Taylor Road, Rutgers University, Piscataway, New Jersey 08854-8066, USA CITATION: Valentine, G.A., Cortés, J.A., Widom, ABSTRACT some of the erupted magmas. The LCVF exhibits clustering in the form of E., Smith, E.I., Rasoazanamparany, C., Johnsen, R., Briner, J.P., Harp, A.G., and Turrin, B., 2017, overlapping and colocated monogenetic volcanoes that were separated by Lunar Crater volcanic field (Reveille and Pancake The Lunar Crater volcanic field (LCVF) in central Nevada (USA) is domi variable amounts of time to as much as several hundred thousand years, but Ranges, Basin and Range Province, Nevada, USA): nated by monogenetic mafic volcanoes spanning the late Miocene to Pleisto without sustained crustal reservoirs between the episodes. -
NEW STUDY of the CERRO SECO RHYOLITE, VALLES CALDERA, NEW MEXICO a Thesis Presented to the Faculty of the Department of Geology
NEW STUDY OF THE CERRO SECO RHYOLITE, VALLES CALDERA, NEW MEXICO A Thesis Presented to the faculty of the Department of Geology California State University, Sacramento Submitted in partial satisfaction of the requirements for the degree of MASTER OF SCIENCE in Geology by Robin L. Wham SPRING 2018 NEW STUDY OF THE CERRO SECO RHYOLITE, VALLES CALDERA, NEW MEXICO A Thesis by Robin L. Wham Approved by: __________________________________, Committee Chair Lisa Hammersley __________________________________, Second Reader Amy Wagner __________________________________, Third Reader Fraser Goff ____________________________ Date ii Student: Robin L. Wham I certify that this student has met the requirements for format contained in the University format manual, and that this thesis is suitable for shelving in the Library and credit is to be awarded for the thesis. __________________________, Department Chair ___________________ Tim Horner Date Department of Geology iii Abstract of NEW STUDY OF THE CERRO SECO RHYOLITE, VALLES CALDERA, NEW MEXICO by Robin L. Wham Cerro Seco is one of six post-caldera rhyolite domes in the northern moat of the Valles Caldera, New Mexico. This study presents detailed mapping as well as petrographic and geochemical analysis of Cerro Seco’s eruptive units and surrounding lacustrine deposits. Cerro Seco’s eruptive members were previously mapped as three separate units: two flow units (lavas Qvse1 and Qvse2), and a pyroclastic unit Qvset. This study has revealed that the pyroclastic unit should be classified as two units: one ignimbrite and one hydromagmatic tuff. Outcrop morphology and pumice clast morphology support a hydromagmatic eruption for the newly classified unit; geochemical analysis illustrates that significant post-emplacement alteration involving water also occurred. -
Geochronology and Geochemistry of the Essimingor Volcano: Melting of Metasomatized Lithospheric Mantle Beneath the North Tanzanian Divergence Zone (East African Rift)
LITHOS-02833; No of Pages 16 Lithos xxx (2012) xxx–xxx Contents lists available at SciVerse ScienceDirect Lithos journal homepage: www.elsevier.com/locate/lithos Geochronology and geochemistry of the Essimingor volcano: Melting of metasomatized lithospheric mantle beneath the North Tanzanian Divergence zone (East African Rift) S. Mana a,⁎, T. Furman b, M.J. Carr a, G.F. Mollel c, R.A. Mortlock a, M.D. Feigenson a, B.D. Turrin a, C.C. Swisher III a a Department of Earth and Planetary Sciences, Rutgers University, NJ 08854, USA b Department of Geosciences, Pennsylvania State University, University Park, PA 16802, USA c Department of Earth and Atmospheric Sciences, University of Alberta, Edmonton, Canada T6G 2N8 article info abstract Article history: The North Tanzanian Divergence zone (NTD), at the southern end of the eastern branch of the East African Received 9 May 2012 Rift, is part of one of Earth's few currently active intra-continental rift systems. The NTD preserves a complex Accepted 23 September 2012 tectono-magmatic evolution of a rift in its early stage of activity. The oldest magmatism reported in the NTD Available online xxxx is associated with the centrally located Essimingor volcano. Although major element oxides show narrow compositional variations suggesting fractional crystallization, trace element abundances and Sr–Nd–Pb iso- Keywords: North Tanzanian Divergence topic data have complex distributions that require open-system processes. The more primitive samples fl 40Ar/39Ar dating (MgO>9 wt.%) likely re ect partial melting of a metasomatized lithospheric mantle characterized by residual Lead isotope garnet, phlogopite and minor amphibole.