Chapter 3 Intrusive Igneous Rocks
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Primordial Hydrogen-Helium Degassing, an Overlooked Major Energy Source for Internal Terrestrial Processes
HAIT Journal of Science and Engineering B, Volume 2, Issues 1-2, pp. 125-167 Copyright C 2005 Holon Academic Institute of Technology ° Primordial hydrogen-helium degassing, an overlooked major energy source for internal terrestrial processes 1, 2 Arie Gilat ∗ and Alexander Vol 1Geological Survey of Israel (ret.), 8 Yehoash St., Jerusalem 93152, Israel 2Enlightment Ltd. 33 David Pinsky St., Haifa 34454, Israel ∗Corresponding author: [email protected] Received 20 July 2004, revised 3 February 2005, accepted 16 February 2005 Abstract The currently accepted theories concerning terrestrial processes are lacking in accounting for a source of internal energy which: (a) are quickly focused, e.g. earthquakes and volcanic eruptions; (b) are of very high density; (c) provide very high velocities of energy re- lease; (d) have very high density of the energy transport and relatively small losses during transportation over long distances; (e) are quasi- constantly released and practically limitless. This energy release is always accompanied by H- and He-degassing. Solid solutions of H and He, and compounds of He with H, O, Si and metals were discovered in laboratory experiments of ultra-high PT-conditions; He-S, He-Cl, He- C, He-N structures can be deduced from their atomic structure and compositions of natural He-reach gases. Ultra-high PT-conditions ex- ist in the Earth’s interior; hence it seems most likely that some “exotic” compounds are present in the Earth’s core and mantle. During Earth’s accretion, primordial hydrogen and helium were trapped and stored in the planet interior as H- and He- solutions and compounds, stable only under ultrahigh PT-conditions that were dis- covered in recent experiments. -
Making Geoscience Fieldwork Inclusive and Accessible for Students with Disabilities GEOSPHERE, V
Research Paper THEMED ISSUE: Human Dimensions in Geoscience GEOSPHERE Making geoscience fieldwork inclusive and accessible for students with disabilities GEOSPHERE, v. 15, no. 6 Alison Stokes1, Anthony D. Feig2, Christopher L. Atchison3, and Brett Gilley4 1School of Geography, Earth and Environmental Sciences, University of Plymouth, PL4 8AA, UK https://doi.org/10.1130/GES02006.1 2Department of Geography and Environmental Studies, Central Michigan University, Mount Pleasant, Michigan 48858, USA 3School of Education and Department of Geology, University of Cincinnati, Cincinnati, Ohio 45221, USA 2 figures; 4 tables 4Department of Earth, Ocean and Atmospheric Sciences, University of British Columbia, Vancouver, British Columbia, Canada V6T 1Z4 CORRESPONDENCE: [email protected] ABSTRACT into the workplace (e.g., Levine et al., 2007; Gonzales and Keane, 2009; Houl- CITATION: Stokes, A., Feig, A.D., Atchison, C.L., and Gilley, B., 2019, Making geoscience fieldwork in- ton, 2010; LaDue and Pacheco, 2013). While a number of these projects have clusive and accessible for students with disabilities: Fieldwork is a fundamental characteristic of geoscience. However, the focused on specific aspects of diversity such as race and/or ethnicity (e.g., Geosphere, v. 15, no. 6, p. 1809–1825, https://doi .org requirement to participate in fieldwork can present significant barriers to stu- Gannet Hallar et al., 2010; Stokes et al., 2015; Carrick et al., 2016) and gender /10.1130 /GES02006.1. dents with disabilities engaging with geoscience as an academic discipline and (e.g., Canetto et al., 2012; Stokes et al., 2015), little attention has been paid to Science Editor: Shanaka de Silva subsequently progressing on to a career as a geoscience professional. -
The Forsterite-Anorthite-Albite System at 5 Kb Pressure Kristen Rahilly
The Forsterite-Anorthite-Albite System at 5 kb Pressure Kristen Rahilly Submitted to the Department of Geosciences of Smith College in partial fulfillment of the requirements for the degree of Bachelor of Arts John B. Brady, Honors Project Advisor Acknowledgements First I would like to thank my advisor John Brady, who patiently taught me all of the experimental techniques for this project. His dedication to advising me through this thesis and throughout my years at Smith has made me strive to be a better geologist. I would like to thank Tony Morse at the University of Massachusetts at Amherst for providing all of the feldspar samples and for his advice on this project. Thank you also to Michael Jercinovic over at UMass for his help with last-minute carbon coating. This project had a number of facets and I got assistance from many different departments at Smith. A big thank you to Greg Young and Dale Renfrow in the Center for Design and Fabrication for patiently helping me prepare and repair the materials needed for experiments. I’m also grateful to Dick Briggs and Judith Wopereis in the Biology Department for all of their help with the SEM and carbon coater. Also, the Engineering Department kindly lent their copy of LabView software for this project. I appreciated the advice from Mike Vollinger within the Geosciences Department as well as his dedication to driving my last three samples over to UMass to be carbon coated. The Smith Tomlinson Fund provided financial support. Finally, I need to thank my family for their support and encouragement as well as my friends here at Smith for keeping this year fun and for keeping me balanced. -
Bedrock Geology Glossary from the Roadside Geology of Minnesota, Richard W
Minnesota Bedrock Geology Glossary From the Roadside Geology of Minnesota, Richard W. Ojakangas Sedimentary Rock Types in Minnesota Rocks that formed from the consolidation of loose sediment Conglomerate: A coarse-grained sedimentary rock composed of pebbles, cobbles, or boul- ders set in a fine-grained matrix of silt and sand. Dolostone: A sedimentary rock composed of the mineral dolomite, a calcium magnesium car- bonate. Graywacke: A sedimentary rock made primarily of mud and sand, often deposited by turbidi- ty currents. Iron-formation: A thinly bedded sedimentary rock containing more than 15 percent iron. Limestone: A sedimentary rock composed of calcium carbonate. Mudstone: A sedimentary rock composed of mud. Sandstone: A sedimentary rock made primarily of sand. Shale: A deposit of clay, silt, or mud solidified into more or less a solid rock. Siltstone: A sedimentary rock made primarily of sand. Igneous and Volcanic Rock Types in Minnesota Rocks that solidified from cooling of molten magma Basalt: A black or dark grey volcanic rock that consists mainly of microscopic crystals of pla- gioclase feldspar, pyroxene, and perhaps olivine. Diorite: A plutonic igneous rock intermediate in composition between granite and gabbro. Gabbro: A dark igneous rock consisting mainly of plagioclase and pyroxene in crystals large enough to see with a simple magnifier. Gabbro has the same composition as basalt but contains much larger mineral grains because it cooled at depth over a longer period of time. Granite: An igneous rock composed mostly of orthoclase feldspar and quartz in grains large enough to see without using a magnifier. Most granites also contain mica and amphibole Rhyolite: A felsic (light-colored) volcanic rock, the extrusive equivalent of granite. -
Neuro-Fuzzy Classification of Felsic Lava Geomorphology at Alarcon Rise, Mexico Christina Hefron Maschmeyer University of South Carolina
University of South Carolina Scholar Commons Theses and Dissertations 2016 Neuro-Fuzzy Classification of Felsic Lava Geomorphology at Alarcon Rise, Mexico Christina Hefron Maschmeyer University of South Carolina Follow this and additional works at: https://scholarcommons.sc.edu/etd Part of the Geology Commons Recommended Citation Maschmeyer, C. H.(2016). Neuro-Fuzzy Classification of Felsic Lava Geomorphology at Alarcon Rise, Mexico. (Master's thesis). Retrieved from https://scholarcommons.sc.edu/etd/3566 This Open Access Thesis is brought to you by Scholar Commons. It has been accepted for inclusion in Theses and Dissertations by an authorized administrator of Scholar Commons. For more information, please contact [email protected]. NEURO-FUZZY CLASSIFICATION OF FELSIC LAVA GEOMORPHOLOGY AT ALARCON RISE, MEXICO by Christina Hefron Maschmeyer Bachelor of Science College of Charleston, 2014 Bachelor of Arts College of Charleston, 2014 Submitted in Partial Fulfillment of the Requirements For the Degree of Master of Science in Geological Sciences College of Arts and Sciences University of South Carolina 2016 Accepted by: Scott White, Director of Thesis Michael Bizimis, Reader Brian Dreyer, Reader Lacy Ford, Senior Vice Provost and Dean of Graduate Studies © Copyright by Christina Hefron Maschmeyer, 2016 All Rights Reserved. ii DEDICATION This thesis is dedicated to Dr. Jim Carew for making me go to graduate school. iii ACKNOWLEDGEMENTS Data for this study were collected during cruises in 2012 aboard the R/V Zephyr and R/V Western Flyer and during 2015 on the R/V Rachel Carson and R/V Western Flyer from the Monterey Bay Aquarium Research Institute. I want to thank the captains, crews, ROV pilots and science parties for their work during these expeditions. -
Milford Sound, Airport Wall, Mile High Club New Zealand, Southern Alps
AAC Publications Milford Sound, Airport Wall, Mile High Club New Zealand, Southern Alps In recent years I have been living between France and the USA, not really spending much time in my native New Zealand. My wife, Julie, is French, and our loose plan was to settle in France when our young son, Sam, started school. At the end of 2019, we had just finished a three-month road trip in California and headed back to NZ for Christmas—for what we intended to be a 10-week visit. But that was before COVID-19. In February, France began its first lockdown, and India, where I was meant to go in April to attempt Changabang, canceled all tourist visas. Since we were already in New Zealand, which at the time had no COVID- related restrictions, we took the easy option of staying there. A few months passed. New Zealand went through its own lockdown, which ended on May 13. We emerged with few restrictions, but we certainly weren’t leaving the country anytime soon. For two years, I had thought of Changabang daily, and for four months I’d been training cardio almost exclusively. Now I began looking for an outlet for all of the energy I had been saving for Changabang. There were no standout alpine objectives calling my name in New Zealand, but my friend Merry Schimanski, who was taking a year off work, was keen to help me develop a long rock route. Like me, he has a love of ground-up adventure climbing, and he is also well versed in establishing big granite lines. -
Crystallization History of Gabbroic Shergottite Nwa 6963 As Revealed by Pyroxene Zoning
Lunar and Planetary Science XLVIII (2017) 1504.pdf CRYSTALLIZATION HISTORY OF GABBROIC SHERGOTTITE NWA 6963 AS REVEALED BY PYROXENE ZONING. A. L. Meado1, S. P. Schwenzer2, S. J. Hammond2, and J. Filiberto1,2, 1Southern Illinois University, Department of Geology, Carbondale IL 62901, USA. [email protected], 2School of Enviroment, Earth, and Ecosystem Sciences, The Open University, Walton Hall, Milton Keynes, MK7 6AA, UK. Introduction: NorthWest Africa (NWA) 6963 is an comprised of 40 to 120 measured points depending on intriguing new coarse grained Martian meteorite that grain size. This method produced precise zoing profiles further extends our sample collection both composition- used to interpret NWA 6963 petrogenetic history. Meas- ally and texturally [1]. It was originally documented as urements too close to the edge of grains, melt inclusions, a basaltic shergottite because the pyroxene composi- sulfides, fractures, or alteration were removed from zon- tions [2, 3] and modal abundances are similar to Sher- ing profiles. Outliers were identified by obvious gotty. However, recent work reclassified NWA 6963 as changes in bulk chemisty, poor oxide weight totals, and an intrusive, gabbroic Martian meteorite because of the visual inspection of back scatter electron (BSE) images. large oriented pyroxene crystals [1]. This investigation Element maps of three pyroxene grains were produced will focus on NWA 6963 pyroxene zoning profiles and to better interpret zoning profiles. interpreting igneous processes related to its crystalliza- Trace elements have recently been analyzed by laser tion history. ablation-ICPMS at the Open University, UK. The data Compositional zoning of pyroxene crystals in basal- is currently being reduced to further interpret pyroxene tic shergottites have previously been interpreted for pe- zoning profiles in NWA 6963. -
The Surface Reactions of Silicate Minerals
RESEARCH BULLETIN 614 SEPTEMBER, 1956 UNIVERSITY OF MISSOURI COLLEGE OF AGRICULTURE AGRICULTURAL EXPERIMENT STATION J. H. Longwell, Director The Surface Reactions Of Silicate Minerals PART II. REACTIONS OF FELDSPAR SURFACES WITH SALT SOLUTIONS. V. E. NASH AND C. E. MARSHALL (Publication authorized September 5, 1956) COLUMBIA, MISSOURI TABLE OF CONTENTS Introduction .......... .. 3 The Interaction of Albite with Salt Solutions . .. 4 The Interaction of Anorthite with Salt Solutions ........ .. 7 Relative Effectiveness of Ammonium Chloride and Magnesium Chloride on the Release of Sodium from Albite . .. 9 Surface Interaction of Albite with Salt Solutions in Methanol . .. 13 Experiments on Cationic Fixation ............................... 16 Detailed Exchange and Activity Studies with Individual Feldspars .......... .. 19 Procedure .. .. 20 Microcline . .. 21 Albite .................................................... 22 Oligoclase . .. 23 Andesine . .. 24 Labradori te . .. 25 Bytownite ................................................. 25 Anorthite . .. 27 Discussion ........ .. 28 Summary ..................................................... 35 References .. .. 36 Most of the experimental material of this and the preceding Research Bulletin is taken from the Ph.D. Thesis of Victor Nash, University of Missouri, June 1955. The experiments on cation fixation were carried our with the aid of a research grant from the Potash Rock Company of America, Lithonia, Georgia, for which the authors wish to record their appreciation. The work was part of Department of Soils Research Project No.6, entitled, "Heavy Clays." The Surface Reactions of Silicate Minerals PART II. REACTIONS OF FELDSPAR SURFACES WITH SALT SOLUTIONS. v. E. NASH AND C. E. MARSHALL INTRODUCTION The review of literature cited in Part I of this series indicates that little is known of the interaction of feldspar surfaces with salt solutions. The work of Breazeale and Magistad (1) clearly demonstrated that ex change reactions between potassium and calcium occur in the case of or thoclase surfaces. -
A POST IMPACT VOLCANISM SCENARIO for the FORMATION of the OLIVINE-RICH UNIT in the REGION of NILI FOSSAE, MARS. L. Mandon1, C. Q
49th Lunar and Planetary Science Conference 2018 (LPI Contrib. No. 2083) 1473.pdf A POST IMPACT VOLCANISM SCENARIO FOR THE FORMATION OF THE OLIVINE - RICH UNIT IN THE REGION OF NILI FOSSAE, MARS. L. Mandon 1 , C. Quantin 1 , P. Thollot 1 , L. Lozac’h 1 , N. Mangold 2 , G. Dromart 1 , P. Beck 3 , E. Dehouck 1 , S. Breton 1 , C. Millot 1 . 1 Laboratoire de Géologie de Lyon Terre, Planètes, Environnement , Université de Lyon, France. 2 Laboratoire de Planétologie et Géodynamique , Université de Nantes, France. 3 Institut de Planétologie et d'Astrophysique de Gre- noble , Université Grenoble Alpes, France. lucia.ma ndon@univ - lyon1.fr. Introduction: The Nili Fossae region exhibits the gets using MarsSI. We used HRSC DTMs computed largest Martian exposures of olivine - rich materials, as by the Fr eie Universitaet Berlin and DLR Berlin . deduced from orbital near - infrared and thermal spec- Strikes and dips measurements were performed using troscopy [1, 2] . Several hypotheses have been pro- the ArcGIS extension LayerTools [7]. Finally, we posed to explain the origin of a widespread olivine - rich performed crater size analyses on both small (~1 km²) formati on in the region: (1) these materials might be and wide (~900 km²) olivine - rich areas. Using the crustal rocks excavated by the giant impact leading to Craterstats software [8], we compared size distribu- the formation of Isidis Planitia [2], a 1200 km wide tions to isochrons generated by the Ivanov production impact basin east of Nili Fossae. (2) They could result function to estimate a surface age [9]. from mafic effusive lava flows occurring befo re [3] or Results: At HiRISE resolution, the unit appears after [4] the giant impact. -
Module 7 Igneous Rocks IGNEOUS ROCKS
Module 7 Igneous Rocks IGNEOUS ROCKS ▪ Igneous Rocks form by crystallization of molten rock material IGNEOUS ROCKS ▪ Igneous Rocks form by crystallization of molten rock material ▪ Molten rock material below Earth’s surface is called magma ▪ Molten rock material erupted above Earth’s surface is called lava ▪ The name changes because the composition of the molten material changes as it is erupted due to escape of volatile gases Rocks Cycle Consolidation Crystallization Rock Forming Minerals 1200ºC Olivine High Ca-rich Pyroxene Ca-Na-rich Amphibole Intermediate Na-Ca-rich Continuous branch Continuous Discontinuous branch Discontinuous Biotite Na-rich Plagioclase feldspar of liquid increases liquid of 2 Temperature decreases Temperature SiO Low K-feldspar Muscovite Quartz 700ºC BOWEN’S REACTION SERIES Rock Forming Minerals Olivine Ca-rich Pyroxene Ca-Na-rich Amphibole Na-Ca-rich Continuous branch Continuous Discontinuous branch Discontinuous Biotite Na-rich Plagioclase feldspar K-feldspar Muscovite Quartz BOWEN’S REACTION SERIES Rock Forming Minerals High Temperature Mineral Suite Olivine • Isolated Tetrahedra Structure • Iron, magnesium, silicon, oxygen • Bowen’s Discontinuous Series Augite • Single Chain Structure (Pyroxene) • Iron, magnesium, calcium, silicon, aluminium, oxygen • Bowen’s Discontinuos Series Calcium Feldspar • Framework Silicate Structure (Plagioclase) • Calcium, silicon, aluminium, oxygen • Bowen’s Continuous Series Rock Forming Minerals Intermediate Temperature Mineral Suite Hornblende • Double Chain Structure (Amphibole) -
Constraining the Source Regions of Lunar Meteorites Using Orbital Geochemical Data
Meteoritics & Planetary Science 50, Nr 2, 214–228 (2015) doi: 10.1111/maps.12412 Constraining the source regions of lunar meteorites using orbital geochemical data A. CALZADA-DIAZ1,2*, K. H. JOY3, I. A. CRAWFORD1,2, and T. A. NORDHEIM2,4 1Department of Earth and Planetary Sciences, Birkbeck College, London WC1E 7HX, UK 2Centre for Planetary Sciences UCL/Birkbeck, London WC1E 6BT, UK 3School of Earth, Atmospheric and Environmental Sciences, University of Manchester, Manchester M13 9PL, UK 4Mullard Space Science Laboratory, University College London, Dorking RH5 6NT, UK *Corresponding author. E-mail: [email protected] (Received 30 July 2014; revision accepted 06 November 2014) Abstract–Lunar meteorites provide important new samples of the Moon remote from regions visited by the Apollo and Luna sample return missions. Petrologic and geochemical analysis of these meteorites, combined with orbital remote sensing measurements, have enabled additional discoveries about the composition and age of the lunar surface on a global scale. However, the interpretation of these samples is limited by the fact that we do not know the source region of any individual lunar meteorite. Here, we investigate the link between meteorite and source region on the Moon using the Lunar Prospector gamma ray spectrometer remote sensing data set for the elements Fe, Ti, and Th. The approach has been validated using Apollo and Luna bulk regolith samples, and we have applied it to 48 meteorites excluding paired stones. Our approach is able broadly to differentiate the best compositional matches as potential regions of origin for the various classes of lunar meteorites. Basaltic and intermediate Fe regolith breccia meteorites are found to have the best constrained potential launch sites, with some impact breccias and pristine mare basalts also having reasonably well-defined potential source regions. -
Arxiv:1906.03473V2 [Physics.Geo-Ph] 30 Dec 2019 Double the Carbon Solubility in fluids Co-Existing with Sediments Subducted Along Cool Geotherms
Devolatilization of Subducting Slabs, Part II: Volatile Fluxes and Storage Meng Tian,1, ∗ Richard F. Katz,1 David W. Rees Jones,1, 2, 3 and Dave A. May1 1Department of Earth Sciences, University of Oxford, South Parks Road, Oxford, OX1 3AN, UK. 2Department of Earth Sciences, Bullard Laboratories, University of Cambridge, Madingley Road, Cambridge, CB3 0EZ, UK. 3School of Mathematics and Statistics, University of St Andrews, North Haugh, St Andrews, KY16 9SS, UK Subduction is a crucial part of the long-term water and carbon cycling between Earth's exo- sphere and interior. However, there is broad disagreement over how much water and carbon is liberated from subducting slabs to the mantle wedge and transported to island-arc volcanoes. In the companion paper Part I, we parameterize the metamorphic reactions involving H2O and CO2 for representative subducting lithologies. On this basis, a two-dimensional reactive transport model is constructed in this Part II. We assess the various controlling factors of CO2 and H2O release from subducting slabs. Model results show that up-slab fluid flow directions produce a flux peak of CO2 and H2O at subarc depths. Moreover, infiltration of H2O-rich fluids sourced from hydrated slab mantle enhances decarbonation or carbonation at lithological interfaces, increases slab surface fluxes, and redistributes CO2 from basalt and gabbro layers to the overlying sedimentary layer. As a result, removal of the cap sediments (by diapirism or off-scraping) leads to elevated slab surface CO2 and H2O fluxes. The modelled subduction efficiency (the percentage of initially subducted volatiles retained until ∼200 km deep) of H2O and CO2 is increased by open-system effects due to fractionation within the interior of lithological layers.