Chapter 5: Lunar Minerals
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Baddeleyite Microstructures in Variably Shocked Martian Meteorites: an Opportunity to Link Shock Barometry and Robust Geochronology
51st Lunar and Planetary Science Conference (2020) 2302.pdf BADDELEYITE MICROSTRUCTURES IN VARIABLY SHOCKED MARTIAN METEORITES: AN OPPORTUNITY TO LINK SHOCK BAROMETRY AND ROBUST GEOCHRONOLOGY. L. G. Staddon1*, J. R. Darling1, N. R. Stephen2, J. Dunlop1, and K. T. Tait3,4. 1School of Environment, Geography and Geoscience, University of Portsmouth, UK; *[email protected], 2Plymouth Electron Microscopy Centre, Plymouth University, UK, 3Department of Earth Sciences, University of Toronto, Canada, 4Royal Ontario Museum, Toronto, Canada. Introduction: Baddeleyite (monoclinic ZrO2; m- [6]. Shergottites in which plagioclase has undergone ZrO2) has recently been shown to be capable of provid- complete transformation to maskelynite (S4), suggest- ing robust crystallisation ages for shergottites via in- ing shock pressures of at least ~29 GPa [6], are repre- situ U-Pb isotopic analyses [1,2]. However, in contrast sented by enriched shergottites NWA 8679 and NWA to experimental work [3], these studies also highlight 7257. Both samples are similarly evolved lithologies, that U-Pb isotope systematics of baddeleyite can be abundant in late stage phases such as Fe-Ti oxides, Cl- strongly modified by shock metamorphism. Up to apatite and Si- and K- rich mesostasis, though NWA ~80% radiogenic Pb loss was recorded within North- 7257 is doleritic [9,10]. Enriched basaltic shergottite west Africa (NWA) 5298 [1], with close correspond- NWA 5298 represents the most heavily shocked mar- ence of U-Pb isotopic ratios and baddeleyite micro- tian meteorite studied here (S6), containing both structures [4]. Combined microstructural analysis and maskelynite and vesicular plagioclase melt [4]. U-Pb geochronology of baddeleyite therefore offers Baddeleyite grains >2 µm in length were located tremendous potential to provide robust constraints on via a combination of automated backscattered electron crystallisation and impact ages for martian meteorites. -
Mount Apatite Park, Auburn, Maine
Mount Apatite Park is a 325-acre wooded park located in the western portion of the city. The park offers a wide variety of recreational opportunities not often found in municipal park settings. Rock hounds have known about this area for over 150 years, when the first discoveries of gem-quality tourmaline were found there. Since then, the area has experienced a great deal of mineral exploration, both commercial and amateur. Today amateurs may still search the mine tailings for apatite, tourmaline, and quartz specimens (special rules apply). The park features approximately four miles of trails for non-motorized uses such as hiking, mountain biking, cross-country skiing, and snowshoeing. The Andy Valley Sno Gypsies also maintain a snowmobile trailhead within the park, which links to miles of regional snowmobile trails.The park is open from dawn until dusk year-round. As with all municipal parks, hunting is not allowed within park boundaries. Park brochures, which include a trail map, park rules, and other park information, are available at the Auburn Parks & Recreation Department office, Monday through Friday, 8a.m.-4:30p.m. Mount Apatite Park, Auburn, Maine Significance The Mt. Apatite quarries were important producers of commercial feldspar in the early 1900's. They played a prominent part in Maine's mining history. During the course of this mining activity, rare minerals and colorful crystals of green and pink tourmaline were found in both the Greenlaw and Maine Feldspar Quarries. These quarries also produced many large crystals of transparent smoky quartz. The complexity of the mineral assemblage at Mt. -
Download PDF About Minerals Sorted by Mineral Name
MINERALS SORTED BY NAME Here is an alphabetical list of minerals discussed on this site. More information on and photographs of these minerals in Kentucky is available in the book “Rocks and Minerals of Kentucky” (Anderson, 1994). APATITE Crystal system: hexagonal. Fracture: conchoidal. Color: red, brown, white. Hardness: 5.0. Luster: opaque or semitransparent. Specific gravity: 3.1. Apatite, also called cellophane, occurs in peridotites in eastern and western Kentucky. A microcrystalline variety of collophane found in northern Woodford County is dark reddish brown, porous, and occurs in phosphatic beds, lenses, and nodules in the Tanglewood Member of the Lexington Limestone. Some fossils in the Tanglewood Member are coated with phosphate. Beds are generally very thin, but occasionally several feet thick. The Woodford County phosphate beds were mined during the early 1900s near Wallace, Ky. BARITE Crystal system: orthorhombic. Cleavage: often in groups of platy or tabular crystals. Color: usually white, but may be light shades of blue, brown, yellow, or red. Hardness: 3.0 to 3.5. Streak: white. Luster: vitreous to pearly. Specific gravity: 4.5. Tenacity: brittle. Uses: in heavy muds in oil-well drilling, to increase brilliance in the glass-making industry, as filler for paper, cosmetics, textiles, linoleum, rubber goods, paints. Barite generally occurs in a white massive variety (often appearing earthy when weathered), although some clear to bluish, bladed barite crystals have been observed in several vein deposits in central Kentucky, and commonly occurs as a solid solution series with celestite where barium and strontium can substitute for each other. Various nodular zones have been observed in Silurian–Devonian rocks in east-central Kentucky. -
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. -
Alkali Pyroxenes and Amphiboles: a Window on Rare
Alkali pyroxenes and amphiboles: a window on rare earth elements and other high field strength elements behavior through the magmatic-hydrothermal transition of peralkaline granitic systems Cyrielle Bernard, Guillaume Estrade, Stefano Salvi, Didier Béziat, Martin Smith To cite this version: Cyrielle Bernard, Guillaume Estrade, Stefano Salvi, Didier Béziat, Martin Smith. Alkali pyroxenes and amphiboles: a window on rare earth elements and other high field strength elements behavior through the magmatic-hydrothermal transition of peralkaline granitic systems. Contributions to Mineralogy and Petrology, Springer Verlag, 2020, 10.1007/s00410-020-01723-y. hal-02989854 HAL Id: hal-02989854 https://hal.archives-ouvertes.fr/hal-02989854 Submitted on 5 Nov 2020 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. 1 Alkali pyroxenes and amphiboles: a window on Rare Earth Elements and other High Field Strength 2 Elements behavior through the magmatic-hydrothermal transition of peralkaline granitic systems 3 4 Cyrielle Bernarda, Guillaume Estradea⸸, Stefano Salvia, Didier Béziata , Martin Smithb 5 a GET, CNRS, UPS, Université de Toulouse III, Toulouse, France 6 b School of Environment and Technology, University of Brighton, Brighton, BN2 4GJ, UK 7 8 ⸸ Corresponding author: [email protected] 9 ORCID: 0000-0001-6907-7469 10 11 12 Acknowledgments 13 This work was supported by an INSU/TelluS grant from CNRS (French National Center for Scientific 14 Research). -
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. -
The Stability, Electronic Structure, and Optical Property of Tio2 Polymorphs
The stability, electronic structure, and optical property of TiO2 polymorphs Tong Zhu and Shang-Peng Gaoa) Department of Materials Science, Fudan University, Shanghai 200433, P. R. China Phonon density of states calculation shows that a new TiO2 polymorph with tridymite structure is mechanically stable. Enthalpies of 9 TiO2 polymorphs under different pressure are presented to study the relative stability of the TiO2 polymorphs. Band structures for the TiO2 polymorphs are calculated by density functional theory with generalized gradient approximation and the band energies at high symmetry k-points are corrected using the GW method to accurately determine the band gap. The differences between direct band gap energies and indirect band gap energies are very small for rutile, columbite and baddeleyite TiO2, indicating a quasi-direct band gap character. The band gap energies of baddeleyite (quasi-direct) and brookite (direct) TiO2 are close to that of anatase (indirect) TiO2. The band gap of the newly predicted tridymite-structured TiO2 is wider than the other 8 polymorphs. For optical response calculations, two-particle effects have been included by solving the Bethe-Salpeter equation for Coulomb correlated electron-hole pairs. TiO2 with cotunnite, pyrite, and fluorite structures have optical transitions in the visible light region. I. INTRODUCTION 1,2 Even after half a century of research, investigation of the fundamental properties of TiO2 crystal phases remains very important properly due to their important role to effectively utilize solar energy. For instance, 3 4 photocatalytic splitting of water into H2 and O2, photovoltaic generation of electricity, degradation of 5,6 7 environmentally hazard materials, and reduction of CO2 into hydrocarbon fuels. -
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. -
74275 Oriented Ilmenite Basalt 1493 Grams
74275 Oriented Ilmenite Basalt 1493 grams 74275 Figure 1: Location of basalt sample 74275 at Shorty Crater - also see 74220. (falce color) AS17-137-20990 Introduction 1981). This sample has proven useful to studies that 74275 is a fine-grained, high-Ti mare basalt with require known lunar orientation with extended significant armalcolite content (Hodges and Kushiro exposure history to the extra-lunar environment 1974; Neal and Taylor 1993). It contains vesicles, vugs (micrometeorites, cosmic rays, solar irradiation). The and unusual olivine megacrysts (Fo82) (Meyer and sample is relatively flat 17 by 12 cm and 4 cm thick. Wilshire 1974). The top (T1) surface is somewhat rounded and has many micrometeorite pits (figure 4), while the bottom 74275 was collected from the rim of Shorty Crater (B1) surface is flat and angular and without any (figure 1) and was photographed both on the lunar evidence of exposure to the micrometeorites (figure surface and in the laboratory (with similar lighting) to 5). Fink et al. (1998) have carefully considered the document the exact lunar orientation. (Wolfe et al. exact orientation (30 deg tilt), shielding (nearby Lunar Sample Compendium C Meyer 2011 boulder) and detailed exposure history (complex) of 74275 74275. Di Hd This basalt has been determined to be very old (> 3.8 b.y.). Based on trace element analysis it is a type C Apollo 17 basalt. Petrography Perhaps the best petrographic description of 74275 is En Fs given by Hodges and Kushiro (1974): “Rock 74275 is a fine-grained ilmenite basalt with microphenocrysts Fo Fa of olivine (Fo80-71), titanaugite (up to 6.8 wt. -
Coupled Substitution of H and Minor Elements in Rutile and The
American Mineralogist, Volume 78, pages I 181-1I9I, 1993 Coupled substitution of H and minor elementsin rutile and the implications of high OH contentsin Nb- and Cr-rich rutile from the upper mantle DrvrrrnrosVr-lssopour,os S. S. Papadopulosand Associates,Inc.,7944 Wisconsin Avenue, Bethesda,Maryland 20814-3620,U.S.A. Gponcn R. Rossnn.q,N Division of Geological and Planetary Sciences,California Institute of Technology,Pasadena, California 91125, U.S.A. SrnpHrN E. Hlccrnry Department of Geology, University of Massachusetts,Amherst, Massachusetts01003, U.S.A. Ansrucr Infrared absorption spectraof rutile crystals from a variety of geologicalenvironments (carbonatite,hydrothermal vein, kyanite * rutile + lazulite association,xenoliths that are kimberlite hosted and dominated by Nb- and Cr-rich rutile) exhibit strong absorption in the 3300-cm-' regtrondue to interstitial protons bonded to structure O. In general the proton is located at sites slightly displaced from t/zYz0of the unit cell, although some samplesshow evidenceofadditional protons at tetrahedral interstitial sites.H contents of rutile range up to 0.8 rvto/oHrO, the highest concentrations occurring in mantle-derived Nb- and Cr-rich rutile of metasomatic origin. The role of H in rutile was examined, particularly with respect to its relations to other impurities. Protons are present in the rutile structure to compensatefor trivalent substitutional cations (Cr, Fe, V, Al), which are only partly compensatedby pentavalent ions (Nb, Ta). The possibility of using the H content of rutile as a geohygrometeris illustrated for the caseof coexisting hematite and rutile. INrnonucrroN crystalsto an OH stretch mode. The study by von Hippel (1962) pro- Rutile is known to have a greal affinity for H, and et al. -
Occurrence, Alteration Patterns and Compositional Variation of Perovskite in Kimberlites
975 The Canadian Mineralogist Vol. 38, pp. 975-994 (2000) OCCURRENCE, ALTERATION PATTERNS AND COMPOSITIONAL VARIATION OF PEROVSKITE IN KIMBERLITES ANTON R. CHAKHMOURADIAN§ AND ROGER H. MITCHELL Department of Geology, Lakehead University, 955 Oliver Road, Thunder Bay, Ontario P7B 5E1, Canada ABSTRACT The present work summarizes a detailed investigation of perovskite from a representative collection of kimberlites, including samples from over forty localities worldwide. The most common modes of occurrence of perovskite in archetypal kimberlites are discrete crystals set in a serpentine–calcite mesostasis, and reaction-induced rims on earlier-crystallized oxide minerals (typically ferroan geikielite or magnesian ilmenite). Perovskite precipitates later than macrocrystal spinel (aluminous magnesian chromite), and nearly simultaneously with “reaction” Fe-rich spinel (sensu stricto), and groundmass spinels belonging to the magnesian ulvöspinel – magnetite series. In most cases, perovskite crystallization ceases prior to the resorption of groundmass spinels and formation of the atoll rim. During the final evolutionary stages, perovskite commonly becomes unstable and reacts with a CO2- rich fluid. Alteration of perovskite in kimberlites involves resorption, cation leaching and replacement by late-stage minerals, typically TiO2, ilmenite, titanite and calcite. Replacement reactions are believed to take place at temperatures below 350°C, 2+ P < 2 kbar, and over a wide range of a(Mg ) values. Perovskite from kimberlites approaches the ideal formula CaTiO3, and normally contains less than 7 mol.% of other end-members, primarily lueshite (NaNbO3), loparite (Na0.5Ce0.5TiO3), and CeFeO3. Evolutionary trends exhibited by perovskite from most localities are relatively insignificant and typically involve a decrease in REE and Th contents toward the rim (normal pattern of zonation).