Characterization of Rock Samples Using Swir-Lwir
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Zunyite Al13si5o20cl(OH,F)18
Zunyite Al13Si5O20Cl(OH; F)18 c 2001 Mineral Data Publishing, version 1.2 ° Crystal Data: Cubic. Point Group: 43m: As excellent tetrahedral or pseudo-octahedral crystals, may be modi¯ed by the cube, up to 2 cm. Twinning: On 111 , contact and penetration. f g Physical Properties: Cleavage: Good on 111 . Tenacity: Brittle. Hardness = 7 f g D(meas.) = 2.874(5) D(calc.) = 2.87{2.90 May °uoresce red under UV. Optical Properties: Transparent; may be more or less opaque from inclusions. Color: Grayish white, °esh-red; colorless in thin section. Luster: Vitreous. Optical Class: Isotropic. n = 1.592{1.600 Cell Data: Space Group: F 43m: a = 13.8654{13.8882 Z = 4 X-ray Powder Pattern: Beni-Embarek, Algeria. 8.07 (100), 4.21 (100), 2.679 (90), 1.639 (90), 4.02 (60), 2.840 (50), 2.008 (50) Chemistry: (1) SiO2 24.33 Al2O3 57.88 Fe2O3 0.20 Li2O trace Na2O 0.24 K2O 0.10 F 5.61 Cl 2.91 H2O 10.89 P2O5 0.60 O = (F; Cl) 3.02 ¡ 2 Total 99.74 3+ (1) Zu~ni mine, Colorado, USA; corresponds to Al13:21Fe0:03P0:10Si4:66O20 Cl0:96[(OH)14:04F3:44]§=17:48: Occurrence: In highly aluminous shales and hydrothermally altered volcanic rocks. Association: Pyrophyllite, kaolinite, alunite, diaspore, rutile, pyrite, hematite, quartz. Distribution: In the USA, in the Zun~i mine, near Silverton, San Juan Co., and in the Charter Oak mine, Ouray Co., Colorado; near Silver City, Tintic district, Juab Co., Utah; in the Dome Rock Mountains, near Quartzsite, La Paz Co., Arizona, large crystals. -
Mineralogical Study of the Advanced Argillic Alteration Zone at the Konos Hill Mo–Cu–Re–Au Porphyry Prospect, NE Greece †
Article Mineralogical Study of the Advanced Argillic Alteration Zone at the Konos Hill Mo–Cu–Re–Au Porphyry Prospect, NE Greece † Constantinos Mavrogonatos 1,*, Panagiotis Voudouris 1, Paul G. Spry 2, Vasilios Melfos 3, Stephan Klemme 4, Jasper Berndt 4, Tim Baker 5, Robert Moritz 6, Thomas Bissig 7, Thomas Monecke 8 and Federica Zaccarini 9 1 Faculty of Geology & Geoenvironment, National and Kapodistrian University of Athens, 15784 Athens, Greece; [email protected] 2 Department of Geological and Atmospheric Sciences, Iowa State University, Ames, IA 50011, USA; [email protected] 3 Faculty of Geology, Aristotle University of Thessaloniki, 54124 Thessaloniki, Greece; [email protected] 4 Institut für Mineralogie, Westfälische Wilhelms-Universität Münster, 48149 Münster, Germany; [email protected] (S.K.); [email protected] (J.B.) 5 Eldorado Gold Corporation, 1188 Bentall 5 Burrard St., Vancouver, BC V6C 2B5, Canada; [email protected] 6 Department of Mineralogy, University of Geneva, CH-1205 Geneva, Switzerland; [email protected] 7 Goldcorp Inc., Park Place, Suite 3400-666, Burrard St., Vancouver, BC V6C 2X8, Canada; [email protected] 8 Center for Mineral Resources Science, Department of Geology and Geological Engineering, Colorado School of Mines, 1516 Illinois Street, Golden, CO 80401, USA; [email protected] 9 Department of Applied Geosciences and Geophysics, University of Leoben, Leoben 8700, Austria; [email protected] * Correspondence: [email protected]; Tel.: +30-698-860-8161 † The paper is an extended version of our paper published in 1st International Electronic Conference on Mineral Science, 16–21 July 2018. Received: 8 October 2018; Accepted: 22 October 2018; Published: 24 October 2018 Abstract: The Konos Hill prospect in NE Greece represents a telescoped Mo–Cu–Re–Au porphyry occurrence overprinted by deep-level high-sulfidation mineralization. -
Minerals of the San Luis Valley and Adjacent Areas of Colorado Charles F
New Mexico Geological Society Downloaded from: http://nmgs.nmt.edu/publications/guidebooks/22 Minerals of the San Luis Valley and adjacent areas of Colorado Charles F. Bauer, 1971, pp. 231-234 in: San Luis Basin (Colorado), James, H. L.; [ed.], New Mexico Geological Society 22nd Annual Fall Field Conference Guidebook, 340 p. This is one of many related papers that were included in the 1971 NMGS Fall Field Conference Guidebook. Annual NMGS Fall Field Conference Guidebooks Every fall since 1950, the New Mexico Geological Society (NMGS) has held an annual Fall Field Conference that explores some region of New Mexico (or surrounding states). Always well attended, these conferences provide a guidebook to participants. Besides detailed road logs, the guidebooks contain many well written, edited, and peer-reviewed geoscience papers. These books have set the national standard for geologic guidebooks and are an essential geologic reference for anyone working in or around New Mexico. Free Downloads NMGS has decided to make peer-reviewed papers from our Fall Field Conference guidebooks available for free download. Non-members will have access to guidebook papers two years after publication. Members have access to all papers. This is in keeping with our mission of promoting interest, research, and cooperation regarding geology in New Mexico. However, guidebook sales represent a significant proportion of our operating budget. Therefore, only research papers are available for download. Road logs, mini-papers, maps, stratigraphic charts, and other selected content are available only in the printed guidebooks. Copyright Information Publications of the New Mexico Geological Society, printed and electronic, are protected by the copyright laws of the United States. -
Nontronite Is a Smectire Group Clay Mineral Which. Ff,T'lffi'"Fff"#:J""
The American Mineralogist, Yolume60, pages 840448, 1975 Primary NontroniteFrom the VenezuelanGuayana W. C. ISpHoRpllrC Department of Geology and Geography, Uniuersity of South Alabama Mobile, Alabama 36688 Abstract Nontronite, the iron-rich end member of SmectiteGroup clays, has previouslybeen reported as a hydrothermalalteration product, as a constituentof soil clays formed by weatheringof a variety of rock types,and as an alterationproduct of volcanicrocks. This paper describesthe chemical,optical, and X-ray propertiesof a new occurrenceof the mineralwhere its origin is apparentlyrelated to directcrystallization from high temperature waters.The mineral is further unique in that it containsonly a very small percentageof aluminaand therebyclosely approaches the previouslyunreported wholly iron end-member. Significantdifferences were found in the optical propertiesof the Venezuelannontronit€ when comparedwith those of an earlier study, especiallywith regard to the variation in refractiveindex with Fe2Oscontent. It now appearsthat this variationhas been over-simpli- fied and may not be as orderlyas was previouslybelieved. The variouslines of evidencethat argue againstan origin by either hydrothermalalteration or chemicalweathering are dis- cussed,as well as thosesupporting an origin by direct crystallizationfrom high temperature watersof probablemagmatic or metamorphicorigin. lntroduction product in gneissesand slates.At the other sites,non- Nontroniteisa Smectire Group clay mineral which. ff,T'Lffi'"fff"#:j""1|# ,XXT::""."t1:j'# occurs as the iron-rich end-memberin the d.ioc- rr-;i",;-be an arterationproduct. At the type tahedral sub-group montmorillonite-beidellite- io.uri,v,Nontron, France, Berthier (1g27) descri6ed nontroniteseries' It haspreviously been *p":l:9^:t^1 ,tr" ri".r"r-: as occurringas "onion-like" massesas- constituentof sedimentaryrocks, as the productof -:-,--; -,,, alterationorvolcanic grasses andas a hydrother.mal alterationproduct. -
Bio-Preservation Potential of Sediment in Eberswalde Crater, Mars
Western Washington University Western CEDAR WWU Graduate School Collection WWU Graduate and Undergraduate Scholarship Fall 2020 Bio-preservation Potential of Sediment in Eberswalde crater, Mars Cory Hughes Western Washington University, [email protected] Follow this and additional works at: https://cedar.wwu.edu/wwuet Part of the Geology Commons Recommended Citation Hughes, Cory, "Bio-preservation Potential of Sediment in Eberswalde crater, Mars" (2020). WWU Graduate School Collection. 992. https://cedar.wwu.edu/wwuet/992 This Masters Thesis is brought to you for free and open access by the WWU Graduate and Undergraduate Scholarship at Western CEDAR. It has been accepted for inclusion in WWU Graduate School Collection by an authorized administrator of Western CEDAR. For more information, please contact [email protected]. Bio-preservation Potential of Sediment in Eberswalde crater, Mars By Cory M. Hughes Accepted in Partial Completion of the Requirements for the Degree Master of Science ADVISORY COMMITTEE Dr. Melissa Rice, Chair Dr. Charles Barnhart Dr. Brady Foreman Dr. Allison Pfeiffer GRADUATE SCHOOL David L. Patrick, Dean Master’s Thesis In presenting this thesis in partial fulfillment of the requirements for a master’s degree at Western Washington University, I grant to Western Washington University the non-exclusive royalty-free right to archive, reproduce, distribute, and display the thesis in any and all forms, including electronic format, via any digital library mechanisms maintained by WWU. I represent and warrant this is my original work, and does not infringe or violate any rights of others. I warrant that I have obtained written permissions from the owner of any third party copyrighted material included in these files. -
The History of Water on Mars: Hydrated Minerals As a Water Sink in the Martian Crust
Ninth International Conference on Mars 2019 (LPI Contrib. No. 2089) 6065.pdf THE HISTORY OF WATER ON MARS: HYDRATED MINERALS AS A WATER SINK IN THE MARTIAN CRUST. L. J. Wernicke1,2 and B. M. Jakosky1,3, 1Laboratory for Atmospheric and Space Physics, University of Colorado Boulder. [email protected]. [email protected]. Introduction: The ancient landscape of Mars pro- example calculation. Nontronite’s empirical formula vides morphological and mineralogical evidence that and all other values used in the example calculation can significant amounts of liquid water once flowed on its be found in Table 1. Nontronite has 6 oxygen atoms surface. Previous research has identified the amount of from water and hydroxyl, which comprises 19.36% of water stored in the polar caps and in high latitude sub- its molecular mass. The oxygen mass/thickness of surface ice [1]. The amount of water lost to space has nontronite is: also been constrained [2]. But how much water is stored (0.1936)*(2300 kg/m3)*(1.449×1014 m2) in Martian rocks? 16 =6.45×10 kg/m Chemical alteration hydrates Martian minerals, stor- 3+ ing water within Martian rocks. A large variety of hy- Nontronite - Na0.3Fe 2Si3AlO10(OH)2•4(H2O) drated minerals have been detected on the surface of Molecular mass (kg) 0.4959 Mars [3,4], and a significant abundance of hydrated minerals has been detected inside Martian craters [5,6]. Oxygen from water 19.36% We use published surveys of the global distribution and Density (kg/m3) 2300 abundance of hydrated minerals to calculate the total Surface area of Mars (m2) 1.449×1014 volume of water stored in hydrated minerals within the Oxygen Mass/thick (kg/m) 6.45×1016 Martian crust. -
An Investigation Into Transitions in Clay Mineral Chemistry on Mars
UNLV Theses, Dissertations, Professional Papers, and Capstones 8-31-2015 An Investigation into Transitions in Clay Mineral Chemistry on Mars Seth Gainey University of Nevada, Las Vegas Follow this and additional works at: https://digitalscholarship.unlv.edu/thesesdissertations Part of the Geochemistry Commons, Geology Commons, and the Mineral Physics Commons Repository Citation Gainey, Seth, "An Investigation into Transitions in Clay Mineral Chemistry on Mars" (2015). UNLV Theses, Dissertations, Professional Papers, and Capstones. 2475. http://dx.doi.org/10.34917/7777303 This Dissertation is protected by copyright and/or related rights. It has been brought to you by Digital Scholarship@UNLV with permission from the rights-holder(s). You are free to use this Dissertation in any way that is permitted by the copyright and related rights legislation that applies to your use. For other uses you need to obtain permission from the rights-holder(s) directly, unless additional rights are indicated by a Creative Commons license in the record and/or on the work itself. This Dissertation has been accepted for inclusion in UNLV Theses, Dissertations, Professional Papers, and Capstones by an authorized administrator of Digital Scholarship@UNLV. For more information, please contact [email protected]. AN INVESTIGATION INTO TRANSITIONS IN CLAY MINERAL CHEMISTRY ON MARS By Seth R. Gainey Bachelor of Science in Geology St. Cloud State University 2009 Master of Science in Geology University of Oklahoma 2011 A dissertation submitted in partial fulfillment of the requirements for the Doctor of Philosophy – Geoscience Department of Geoscience College of Sciences The Graduate College University of Nevada, Las Vegas August 2015 Copyright by Seth R. -
Subsurface Water and Clay Mineral Formation During the Early History of Mars Bethany L
REVIEW doi:10.1038/nature10582 Subsurface water and clay mineral formation during the early history of Mars Bethany L. Ehlmann1{, John F. Mustard2, Scott L. Murchie3, Jean-Pierre Bibring1, Alain Meunier4, Abigail A. Fraeman5 & Yves Langevin1 Clay minerals, recently discovered to be widespread in Mars’s Noachian terrains, indicate long-duration interaction between water and rock over 3.7 billion years ago. Analysis of how they formed should indicate what environmental conditions prevailed on early Mars. If clays formed near the surface by weathering, as is common on Earth, their presence would indicate past surface conditions warmer and wetter than at present. However, available data instead indicate substantial Martian clay formation by hydrothermal groundwater circulation and a Noachian rock record dominated by evidence of subsurface waters. Cold, arid conditions with only transient surface water may have characterized Mars’s surface for over 4 billion years, since the early-Noachian period, and the longest-duration aqueous, potentially habitable environments may have been in the subsurface. hemical interactions between water and rock transform nominally salts from evaporating, sometimes acidic, groundwater discharge13. anhydrous materials formed by volcanic and igneous processes However, earlier Noachian environmental conditions resulting in clay C into hydrous phases, including clay minerals1 (phyllosilicates), formation are less well understood. In particular, it is not known whether 7 which incorporate OH or H2O in their structures (Table 1). On Earth, clay formation occurred mainly at the surface or in the subsurface . clay minerals form from near-surface weathering to produce soils, in This issue has a substantial bearing on understanding Mars’s early hydrothermal systems located mostly at sea-floor spreading centres, or evolution. -
Comprehensive Physicochemical Study of Dioctahedral Palygorskite
Comprehensive physicochemical study of dioctahedral palygorskite-rich clay from Marrakech High Atlas (Morocco) Benaissa Rhouta, Ezzouhra Zatile, Lahcen Bouna, Omar Lakbita, Francis Maury, Lahcen Daoudi, Marie Christine Lafont, M’barek Amjoud, François Senocq, Amane Jada, et al. To cite this version: Benaissa Rhouta, Ezzouhra Zatile, Lahcen Bouna, Omar Lakbita, Francis Maury, et al.. Compre- hensive physicochemical study of dioctahedral palygorskite-rich clay from Marrakech High Atlas (Mo- rocco). Physics and Chemistry of Minerals, Springer Verlag, 2013, vol. 40 (n° 5), pp. 411-424. 10.1007/s00269-013-0579-3. hal-01172017 HAL Id: hal-01172017 https://hal.archives-ouvertes.fr/hal-01172017 Submitted on 6 Jul 2015 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. Open Archive TOULOUSE Archive Ouverte (OATAO) OATAO is an open access repository that collects the work of Toulouse researchers and makes it freely available over the web where possible. This is an author-deposited version published in : http://oatao.univ-toulouse.fr/ Eprints ID : 14095 To link to this article : DOI:10.1007/s00269-013-0579-3 URL : http://dx.doi.org/10.1007/s00269-013-0579-3 To cite this version : Rhouta, Benaissa and Zatile, Ezzouhra and Bouna, Lahcen and Lakbita, Omar and Maury, Francis and Daoudi, Lahcen and Lafont, Marie Christine and Amjoud, M’Barek and Senocq, François and Jada, Amane and Aït Aghzzaf, Ahmed Comprehensive physicochemical study of dioctahedral palygorskite- rich clay from Marrakech High Atlas (Morocco). -
Sulfur-Poor Intense Acid Hydrothermal Alteration: a Distinctive Hydrothermal Environment ⇑ Douglas C
Ore Geology Reviews 88 (2017) 174–187 Contents lists available at ScienceDirect Ore Geology Reviews journal homepage: www.elsevier.com/locate/oregeo Sulfur-poor intense acid hydrothermal alteration: A distinctive hydrothermal environment ⇑ Douglas C. Kreiner , Mark D. Barton Department of Geosciences and Lowell Institute for Mineral Resources, University of Arizona, Tucson, AZ 85721, United States article info abstract Article history: A fundamentally distinct, sulfide-poor variant of intense acid (advanced argillic) alteration occurs at the Received 8 June 2016 highest structural levels in iron oxide-rich hydrothermal systems. Understanding the mineralogy, and Received in revised form 16 February 2017 geochemical conditions of formation in these sulfide-poor mineral assemblages have both genetic and Accepted 20 April 2017 environmental implications. New field observations and compilation of global occurrences of low- Available online 23 April 2017 sulfur advanced argillic alteration demonstrates that in common with the sulfide-rich variants of advanced argillic alteration, sulfide-poor examples exhibit nearly complete removal of alkalis, leaving Keywords: a residuum of aluminum-silicate + quartz. In contrast, the sulfur-poor variants lack the abundant pyri- Iron-oxide copper gold te ± other sulfides, hypogene alunite, Al-leached rocks (residual ‘‘vuggy” quartz) as well as the Au-Cu- IOCG Advanced argillic Ag ± As-rich mineralization of some sulfur-rich occurrences. Associated mineralization is dominated by Low-sulfur advanced argillic magnetite and/or hematite with accessory elements such as Cu, Au, REE, and P. These observations pre- sented here indicate there must be distinct geologic processes that result in the formation of low-sulfur advanced argillic styles of alteration. Hydrolysis of magmatic SO2 to sulfuric acid is the most commonly recognized mechanism for generat- ing hypogene advanced argillic alteration, but is not requisite for its formation. -
Minerals Found in Michigan Listed by County
Michigan Minerals Listed by Mineral Name Based on MI DEQ GSD Bulletin 6 “Mineralogy of Michigan” Actinolite, Dickinson, Gogebic, Gratiot, and Anthonyite, Houghton County Marquette counties Anthophyllite, Dickinson, and Marquette counties Aegirinaugite, Marquette County Antigorite, Dickinson, and Marquette counties Aegirine, Marquette County Apatite, Baraga, Dickinson, Houghton, Iron, Albite, Dickinson, Gratiot, Houghton, Keweenaw, Kalkaska, Keweenaw, Marquette, and Monroe and Marquette counties counties Algodonite, Baraga, Houghton, Keweenaw, and Aphrosiderite, Gogebic, Iron, and Marquette Ontonagon counties counties Allanite, Gogebic, Iron, and Marquette counties Apophyllite, Houghton, and Keweenaw counties Almandite, Dickinson, Keweenaw, and Marquette Aragonite, Gogebic, Iron, Jackson, Marquette, and counties Monroe counties Alunite, Iron County Arsenopyrite, Marquette, and Menominee counties Analcite, Houghton, Keweenaw, and Ontonagon counties Atacamite, Houghton, Keweenaw, and Ontonagon counties Anatase, Gratiot, Houghton, Keweenaw, Marquette, and Ontonagon counties Augite, Dickinson, Genesee, Gratiot, Houghton, Iron, Keweenaw, Marquette, and Ontonagon counties Andalusite, Iron, and Marquette counties Awarurite, Marquette County Andesine, Keweenaw County Axinite, Gogebic, and Marquette counties Andradite, Dickinson County Azurite, Dickinson, Keweenaw, Marquette, and Anglesite, Marquette County Ontonagon counties Anhydrite, Bay, Berrien, Gratiot, Houghton, Babingtonite, Keweenaw County Isabella, Kalamazoo, Kent, Keweenaw, Macomb, Manistee, -
A Specific Gravity Index for Minerats
A SPECIFICGRAVITY INDEX FOR MINERATS c. A. MURSKyI ern R. M. THOMPSON, Un'fuersityof Bri.ti,sh Col,umb,in,Voncouver, Canad,a This work was undertaken in order to provide a practical, and as far as possible,a complete list of specific gravities of minerals. An accurate speciflc cravity determination can usually be made quickly and this information when combined with other physical properties commonly leads to rapid mineral identification. Early complete but now outdated specific gravity lists are those of Miers given in his mineralogy textbook (1902),and Spencer(M,i,n. Mag.,2!, pp. 382-865,I}ZZ). A more recent list by Hurlbut (Dana's Manuatr of M,i,neral,ogy,LgE2) is incomplete and others are limited to rock forming minerals,Trdger (Tabel,l,enntr-optischen Best'i,mmungd,er geste,i,nsb.ildend,en M,ineral,e, 1952) and Morey (Encycto- ped,iaof Cherni,cal,Technol,ogy, Vol. 12, 19b4). In his mineral identification tables, smith (rd,entifi,cati,onand. qual,itatioe cherai,cal,anal,ys'i,s of mineral,s,second edition, New york, 19bB) groups minerals on the basis of specificgravity but in each of the twelve groups the minerals are listed in order of decreasinghardness. The present work should not be regarded as an index of all known minerals as the specificgravities of many minerals are unknown or known only approximately and are omitted from the current list. The list, in order of increasing specific gravity, includes all minerals without regard to other physical properties or to chemical composition. The designation I or II after the name indicates that the mineral falls in the classesof minerals describedin Dana Systemof M'ineralogyEdition 7, volume I (Native elements, sulphides, oxides, etc.) or II (Halides, carbonates, etc.) (L944 and 1951).