Olivines, Their Pseudomorphs and Secondary Products
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Phyllosilicate Minerals in the Hydrothermal Mafic–Ultramafic-Hosted Massive-Sulfide Deposit of Ivanovka
Contrib Mineral Petrol (2004) 147: 363–383 DOI 10.1007/s00410-004-0565-3 ORIGINAL PAPER Paolo Nimis Æ Svetlana G. Tesalina Æ Paolo Omenetto Paola Tartarotti Æ Catherine Lerouge Phyllosilicate minerals in the hydrothermal mafic–ultramafic-hosted massive-sulfide deposit of Ivanovka (southern Urals): comparison with modern ocean seafloor analogues Received: 15 August 2003 / Accepted: 9 February 2004 / Published online: 17 March 2004 Ó Springer-Verlag 2004 Abstract We have studied textural relationships and required a high contribution of Mg-rich seawater to the compositions of phyllosilicate minerals in the mafic– hydrothermal fluid, which could be achieved in a highly ultramafic-hosted massive-sulfide deposit of Ivanovka permeable, breccia-dominated seafloor. More evolved (Main Uralian Fault Zone, southern Urals). The main hydrothermal fluids produced addition of silica, car- hydrothermal phyllosilicate minerals are Mg-rich chlo- bonates and further sulfides, and led to local develop- rite, variably ferroan talc, (Mg, Si)-rich and (Ca, Na, ment of saponite after chlorite and widespread K)-poor saponite (stevensite), and serpentine. These replacement of serpentine by talc. The Ivanovka deposit minerals occur both as alteration products after mafic shows many similarities with active and fossil hydro- volcanics and ultramafic protoliths and, except serpen- thermal sites on some modern oceanic spreading centers tine, as hydrothermal vein and seafloor mound-like characterized by highly permeable upflow zones. How- precipitates associated with variable amounts of (Ca, ever, given the arc signature of the ore host rocks, the Mg, Fe)-carbonates, quartz and Fe and Cu (Co, Ni) most probable setting for the observed alteration–min- sulfides. -
Washington State Minerals Checklist
Division of Geology and Earth Resources MS 47007; Olympia, WA 98504-7007 Washington State 360-902-1450; 360-902-1785 fax E-mail: [email protected] Website: http://www.dnr.wa.gov/geology Minerals Checklist Note: Mineral names in parentheses are the preferred species names. Compiled by Raymond Lasmanis o Acanthite o Arsenopalladinite o Bustamite o Clinohumite o Enstatite o Harmotome o Actinolite o Arsenopyrite o Bytownite o Clinoptilolite o Epidesmine (Stilbite) o Hastingsite o Adularia o Arsenosulvanite (Plagioclase) o Clinozoisite o Epidote o Hausmannite (Orthoclase) o Arsenpolybasite o Cairngorm (Quartz) o Cobaltite o Epistilbite o Hedenbergite o Aegirine o Astrophyllite o Calamine o Cochromite o Epsomite o Hedleyite o Aenigmatite o Atacamite (Hemimorphite) o Coffinite o Erionite o Hematite o Aeschynite o Atokite o Calaverite o Columbite o Erythrite o Hemimorphite o Agardite-Y o Augite o Calciohilairite (Ferrocolumbite) o Euchroite o Hercynite o Agate (Quartz) o Aurostibite o Calcite, see also o Conichalcite o Euxenite o Hessite o Aguilarite o Austinite Manganocalcite o Connellite o Euxenite-Y o Heulandite o Aktashite o Onyx o Copiapite o o Autunite o Fairchildite Hexahydrite o Alabandite o Caledonite o Copper o o Awaruite o Famatinite Hibschite o Albite o Cancrinite o Copper-zinc o o Axinite group o Fayalite Hillebrandite o Algodonite o Carnelian (Quartz) o Coquandite o o Azurite o Feldspar group Hisingerite o Allanite o Cassiterite o Cordierite o o Barite o Ferberite Hongshiite o Allanite-Ce o Catapleiite o Corrensite o o Bastnäsite -
The Geological Newsletter
JAN 90 THE GEOLOGICAL NEWSLETTER ·• GEOLOGICAL SOCIETY OF THE OREGON COUNTRY GEOLOGICAL SOCIETY Non-Profit Org. U.S. POSTAGE OF THE OREGON COUNTRY PAID P.O. BOX ?a 7- Portland, Oregon PORTLAND, OR 97207- -:· ·--~··, Permit No. 999 - -- '~ Dr. Frank Boersma 120 W. 33~d Street Vancouver, WA 98660 GEOLOGICAL SOCIETY OF THE OREGOt\ COllNTRY 1989-1990 ADMINISTRATION BOARD OF DIRECTORS President Directors Rosemary Kenney 221-0757 Peter E. Baer (3 years) 661-7995 4211 S\-1 Condor Charlene Holzwarth (2 years) 284-3444 Portland, OR 97201 Esther Kennedy (1 year) 287-3091 Vice President Margaret L. Steere 246-1670 Immediate Past Presidents Joline Robustelli 223-2852 6929 SW 34 Ave. ~ Portland, OR 97219 R.E. (Andy) Corcoran 244-5605 Secretary Alta B. Fosback 641-6323 THE GEOLOGICAL NEWSLETTER 8942 SW Fairview Place Tigard, OR 97223 Editor: Sandra Anderson 775-5538 Treasurer Calendar: Margaret Steere 246-1670 Braden Pillow 659-6318 Business Manager: Carol Cole 220-0078 19562 SE Cottonwood St. Assist: Cecelia Crater 235-5158 Milwaukie, OR 97267 ACTIVITIES CHAIRS Calligrapher Properties and PA System Wallace R.· McClung 637-3834 (Luncheon) Donald Botteron 245-6251 Field Trips (Evening) Walter A. Sunderland 625-6840 Charlene Holzwarth 284-3444 Publications Alta B. Fosback 641-6323 Geneva E. Reddekopp 654-9818 Geology Seminars Publicity Donald D. Barr 246-2785 Roberta L. Walter 235-3579 Historian Refreshments Phyllis G. Bonebrake 289-8597 (Friday Evening) Hospitality David and Marvel Gillespie 246-2368 254-0135 (Luncheon) Margaret Fink 289-0188 Harold and Patricia Gay Moore (Evening) Maxine Harrington 297-ll86 (Geology Seminars) Catherine Evenson 654-2636 Library: Esther Kennedy 287-3091 ' ' Betty Turner 246-3192 Telephone n Past Presidents Panel Jean L. -
Lafayette - 800 Grams Nakhlite
Lafayette - 800 grams Nakhlite Figure 1. Photograph showing fine ablation features Figure 2. Photograph of bottom surface of Lafayette of fusion crust on Lafayette meteorite. Sample is meteorite. Photograph from Field Museum Natural shaped like a truncated cone. This is a view of the top History, Chicago, number 62918. of the cone. Sample is 4-5 centimeters across. Photo- graph from Field Museum Natural History, Chicago, number 62913. Introduction According to Graham et al. (1985), “a mass of about 800 grams was noticed by Farrington in 1931 in the geological collections in Purdue University in Lafayette Indiana.” It was first described by Nininger (1935) and Mason (1962). Lafayette is very similar to the Nakhla and Governador Valadares meteorites, but apparently distinct from them (Berkley et al. 1980). Lafayette is a single stone with a fusion crust showing Figure 3. Side view of Lafayette. Photograph from well-developed flow features from ablation in the Field Museum Natural History, Chicago, number Earth’s atmosphere (figures 1,2,3). The specimen is 62917. shaped like a rounded cone with a blunt bottom end. It was apparently oriented during entry into the Earth’s that the water released during stepwise heating of atmosphere. Note that the fine ablation features seen Lafayette was enriched in deuterium. The alteration on Lafayette have not been reported on any of the assemblages in Lafayette continue to be an active field Nakhla specimens. of research, because it has been shown that the alteration in Lafayette occurred on Mars. Karlsson et al. (1992) found that Lafayette contained the most extra-terrestrial water of any Martian Lafayette is 1.32 b.y. -
The New IMA List of Gem Materials – a Work in Progress – Updated: July 2018
The New IMA List of Gem Materials – A Work in Progress – Updated: July 2018 In the following pages of this document a comprehensive list of gem materials is presented. The list is distributed (for terms and conditions see below) via the web site of the Commission on Gem Materials of the International Mineralogical Association. The list will be updated on a regular basis. Mineral names and formulae are from the IMA List of Minerals: http://nrmima.nrm.se//IMA_Master_List_%282016-07%29.pdf. Where there is a discrepancy the IMA List of Minerals will take precedence. Explanation of column headings: IMA status: A = approved (it applies to minerals approved after the establishment of the IMA in 1958); G = grandfathered (it applies to minerals discovered before the birth of IMA, and generally considered as valid species); Rd = redefined (it applies to existing minerals which were redefined during the IMA era); Rn = renamed (it applies to existing minerals which were renamed during the IMA era); Q = questionable (it applies to poorly characterized minerals, whose validity could be doubtful). Gem material name: minerals are normal text; non-minerals are bold; rocks are all caps; organics and glasses are italicized. Caveat (IMPORTANT): inevitably there will be mistakes in a list of this type. We will be grateful to all those who will point out errors of any kind, including typos. Please email your corrections to [email protected]. Acknowledgments: The following persons, listed in alphabetic order, gave their contribution to the building and the update of the IMA List of Minerals: Vladimir Bermanec, Emmanuel Fritsch, Lee A. -
Ferric Saponite and Serpentine in the Nakhlite Martian Meteorites
Available online at www.sciencedirect.com ScienceDirect Geochimica et Cosmochimica Acta 136 (2014) 194–210 www.elsevier.com/locate/gca Ferric saponite and serpentine in the nakhlite martian meteorites L.J. Hicks a, J.C. Bridges a,⇑, S.J. Gurman b a Space Research Centre, Dept. of Physics & Astronomy, University of Leicester, Leicester LE1 7RH, UK b Dept. of Physics & Astronomy, University of Leicester, Leicester LE1 7RH, UK Received 29 October 2013; accepted in revised form 7 April 2014; available online 18 April 2014 Abstract Transmission electron microscopy and Fe-K X-ray absorption spectroscopy have been used to determine structure and ferric content of the secondary phase mineral assemblages in the nakhlite martian meteorites, NWA 998, Lafayette, Nakhla, GV, Y 000593, Y 000749, MIL 03346, NWA 817, and NWA 5790. The secondary phases are a rapidly cooled, metastable assemblage that has preserved Mg# and Ca fractionation related to distance from the fluid source, for most of the nakhlites, though one, NWA 5790, appears not to have experienced a fluid pathway. All nine nakhlite samples have also been analysed with scanning electron microscopy, electron probe micro analysis, Bright Field high-resolution transmission electron microscopy (HRTEM) and selected area electron diffraction. By measuring the energy position of the Fe-K XANES 1s ! 3d pre-edge transition centroid we calculate the ferric content of the minerals within the nakhlite meteorites. The crystalline phyllosilicates and amorphous silicate of the hydrothermal deposits filling the olivine fractures are found to have variable Fe3+/RFe values ranging from 0.4 to 0.9. In Lafayette, the central silicate gel parts of the veins are more ferric than the phyllosilicates around it, showing that the fluid became increasingly oxidised. -
HIGH TEMPERATURE PHASES in SEPIOLITB, ATTAPULGITE and SAPONITE Gnoncrs Kulnrcrr,* Departmentof Geology, Uniters'ityof Lllinois, Urbana,Illinois
THE AMERICAN MINERALOGIST, VOL 44, JULY_AUGUST, 1959 HIGH TEMPERATURE PHASES IN SEPIOLITB, ATTAPULGITE AND SAPONITE Gnoncrs Kulnrcrr,* Departmentof Geology, Uniters'ityof lllinois, Urbana,Illinois. AssrnA.cr The high temperature reactions of sepiolite, attapulgite and saponite were studied by continuous high temperatute rc-ray diffraction techniques. The easy formation of enstatite from the fibrous minerals is explained by structural analogy. The reactions of the well crystallized specimens of sepiolite and attapulgite difier somewhat from those of their massive sedimentary varieties. The difierences cannot be ex- plained with the chemical and structural data, suggesting possible variations in some inti- mate details of the framework of these two varieties. INrnooucuox The nature of the crystalline phases formed by firing the magnesian clay mineralshas beendescribed (2,3,7, I0, 12,15, 16),but only for the well crystallized chlorites (3) have the precise conditions of formation of these phases as well as their structural relationships with the starting material been clearly determined. The three minerals chosenfor this investigation provide difierent struc- tural arrangementsof the same type of lattice in a series of Al-Mg hydrous silicates.Saponite and sepiolite have the same bulk composi- tion but they difier in the mode of assemblage,i.e. layers or ribbons, of their structural units. Attapulgite has the same kind of framework as sepiolite, but a large proportion of magnesium has been replaced by aluminum or iron. It was thought that, by taking advantage of these features and by using a method of continuous high-tempetature x-ray diffraction analysis,a new contribution to the problem would be possible. -
The Telephone City Crystal Brantford Lapidary & Mineral Society
THE TELEPHONE CITY CRYSTAL BRANTFORD LAPIDARY & MINERAL SOCIETY JANUARY 2017 Volume 71 Issue 1 INSIDE THIS ISSUE: JANUARY MEETING— 2 EARTH ON THE MOVE& ARAGONITE UPCOMING EVENTS & 3 CLUB INFO PIECE OF DINOSAUR 4 TAIL IN AMBER RARE GEM MINE 5 & TUMBLER GRIT ROCK TUMBLING 6 MONTHLY MINERAL - 7 APATITE 2016 EXECUTIVE & 8 MISC. December Meeting Highlight Photo- listing on page 2 1 THE TELEPHONE CITY CRYSTAL DATE: FRIDAY JANUARY 20, 2017 TIME: 7:30 PM WHERE: TB COSTAIN/S.C. JOHNSON COMMUNITY CENTER, 16 MORRELL ST. BRANTFORD, ONT. PROGRAM: RENE PERRIN: “EARTH ON THE MOVE” “The title is "Earth on the Move" featuring how the earth has moved and is mov- ing now at both the large scale as in India moving North with various other big and much smaller ex- amples with a beautiful graphic showing all of the global movements as tracked by stations all over the world. This is a great image showing the movement directions with arrows.” THE MINERAL ARAGONITE Calcium carbonate forms as both Aragonite and Calcite, and these two minerals only differ in theircrystallization. Cal- cite, the more common mineral, forms in trigonal crystals, whereas Aragonite forms orthorhombic crystals. On occasion, crystals of Aragonite and Calcite are too small to be individually determined, and it is only possible to distinguish these two minerals with optical or x-ray testing. The true identity of microcrystalline forms of Aragonite or Calcite may also not be known without complex testing, and this can also cause a confusion between these species. Most large Aragonite crystals are twinned growths of three individual crystals that form pseudohexagonal trillings. -
Expedition 330 Core Descriptions, Site U1374 Thin Sections
Site U1374 thin sections U1374A-3R-1-W 114_116 Proc. IODP THIN SECTION: 330-U1374A-3R-1-W 114_116-BILLET 114-SLIDE 114 Piece No: Unit:I OBSERVER:THIN SECTION:SLIDE 114 Site U1374 core descriptions ROCK NAME: moderately olivine-phyric basalt clast WHERE SAMPLED: clast type 2 GRAINSIZE: fine grained TEXTURE: moderately phyric | Volume 330 PRIMARY PERCENT REL. VOL. SIZE(mm) VESICLE VESICLE MINERALOGY ORIGINAL REPLACED min. max. mode. MORPHOLOGY SPHERICITY Infilling [%] COMMENTS PHENOCRYSTS 10 olivine 5 20 8 1.2 skeletal incomplete dome face (iddingsite); "skeletal olivine" & "euhedral to subhedral" MICROPHENOCRYST plagioclase 0.01 0.3 0.4 laths[330] just 2 grains olivine 4 40 0.9 0.4 skeletal incomplete dome face (iddingsite); "skeletal olivine" & "euhedral to subhedral" augite 1 0.3 0.3 subhedral sector-zoning titanaugite VESICLES 3 0.1 1.8 0.6 low[330] 100 filled by calcite GROUNDMASS 87 opaque mineral 5 olivine 4 95 0.09 0.06 subhedral to replaced by iddingsite (hematite?) anhedral[330] glass 68 100 palagonite augite 1 anhedral plagioclase 9 0.2 0.01 microlite[330] SECONDARY SIZE(mm) MINERALOGY min. max. mode. REPLACING/FILLING COMMENTS calcite vesicle STRUCTURE no structure in groundmass COMMENTS SUMMARY DESCRIPTION Thin sections 1 U1374A-3R-2-W 7_9 Proc. IODP THIN SECTION: 330-U1374A-3R-2-W 7_9-BILLET 115-SLIDE 115 Piece No: Unit:I OBSERVER:THIN SECTION:SLIDE 115 Site U1374 core descriptions ROCK NAME: highly olivine-phyric basalt clast WHERE SAMPLED: CLAST TYPE 1 GRAINSIZE: fine grained TEXTURE: highly phyric & glomeroporphyritic | Volume 330 PRIMARY PERCENT REL. -
Aqueous Alteration of Yamato 000749 Based on Multi-Probe Microscopic Observation
Aqueous alteration of Yamato 000749 based on multi-probe microscopic observation Naoki Shiraishi1, Hiroki Suga1,2, Masaaki Miyahara1, Takuji Ohigashi3, Yuichi Inagaki3, Akira Yamaguchi4, Naotaka Tomioka 5, Yu Kodama6, and Eiji Ohtani7 1Hiroshima University, 2The University of Tokyo, 3UVSOR synchrotron facility, 4NIPR, 5Kochi Institute for Core Sample 6 7 Research, JAMSTEC, Marine Works Japan, Tohoku University Motivation Based on the results of Mars explorations and researches of Martian meteorites for many years, there is a high possibility that liquid water had existed extensively on Mars for a long time (Sekine, 2012). Martian meteorite is one of the important clues for restoring the past Martian surface environment that cannot be unveiled by Mars surface survey alone. It is expected that a member of Martian meteorites, nakhlites have evidences for a rock-fluid reaction occurred on Mars. One of the representative evidence for the rock-fluid reaction is “iddingsite”, which is an alteration texture formed in and around olivine grains in nakhlites. Many kinds of secondary minerals occur in the iddingsite through the rock-fluid reaction. The mineral assemblages, chemical compositions and chemical species of the secondary minerals depend on the varied parameters such as temperature and pH of the fluid. Suga et al. (2017) described the secondary minerals in the iddingsite of nakhlites Yamato (Y) 000593. Another Martian meteorites, Yamato (Y) 000749 is also a member of Yamato 00 nakhlites like Y 000593, containing abundant iddingsite. Based on Cohen et al. (2017), Y 000749 was located at the lower portion of the same nakhlites source compared to Y 000593. It is likely that these nakhlites have different mode of alteration even in the same source. -
Alkalic Rocks of Iron Hill Gunnison County, Colorado
If yon do not need this publication after it has served your purpose, please return it to the Geological Survey, using the official mailing label at the end UNITED STATES DEPARTMENT OF THE INTERIOR ALKALIC ROCKS OF IRON HILL GUNNISON COUNTY, COLORADO GEOLOGICAL SURVEY PROFESSIONAL PAPER 197-A UNITED STATES DEPARTMENT OF THE INTERIOR Harold L. Ickes, Secretary GEOLOGICAL SURVEY W. C. Mendenhall, Director Professional Paper 197-A ALKALIC ROCKS OF IRON HILL GUNNISON COUNTY, COLORADO BY ESPER S. LARSEN Shorter contributions to general geology, 1941 (Pages 1-64) UNITED STATES GOVERNMENT PRINTING OFFICE WASHINGTON : 1942 For sale by the Superintendent of Documents, Washington, D. C. ......... Price 40 cents CONTENTS Page Preface, by G. F. Loughlin_________________________ v Other dike rocks_______________-____________________ 29 Abstract____"_--__-___--__________________________ 1 Augite syenite and shonkinite ____.__--___--__--__ 29 Introduction. ______________________________________ 1 Olivine gabbro. ________________________________ 30 Location and topography. _______________________ 1 Carbonate veins_________----__---------__--_---___- 31 Field work and acknowledgments.________________ 2 Character __ __________________________________ 31 Geology of the surrounding area__________________ 2 Origin _______ _ ____ _ __ _.. __ __. ___ .__. 31 Age of the Iron Hill stock_____________________ 2 Hydrothermal processes- ______--_-___-_---_--__-___- 31 General geology of the Iron Hill stock _____________ 3 The hydrothermal products. _____________________ -
Turquoise in the Burro Mountains, New Mexico
TURQUOISE IN THE BURRO MOUNTAINS, NEW MEXICO. EDWARD R. ZALINSKI. [The following notes are from data collected during the year •9o5 while the writer was superintendent of the Azure Mining Company's property near Silver City. It was his intention to make a detailed study of the sub- ject, but this professional duties have hitherto prevented and in the following pages are presented the tentative conclusionsof an unfinished investigation.] HISTORY AND LOCALITIES. Turquoiseoriginally came fr4m' Persia by wayof Turkeyand was importedby the Venetians,who called it Turchesa,of which its presentname is the French variation. In America it has long been known to the southwesternIndians and was used by them for ornaments and mosaic work. Professor W. P. Blake, in •858 and '59, called attention to its occurrence at Cerrillos, New Mexico, where it had been mined by the aboriginesand early Spaniards. This locality has producedsome valuable gems, but the mines are not at present worked. Turquoise has been found also at Turquoise Moun- tain, CochiseCounty, and Mineral Park, Mohave County, Ari- zona; near Columbus and near Crescent, in southern Nevada; in Fresno County, California; and in Colorado. In New Mexico, besides Cerrillos mentioned above, it is known at Hachiti; in the Burro Mountains, Grant County; and in the Jarrilla Moun- tains, Otero County. The modern discovery of turquoise in the Burro Mountains dates from •875, but these depositswere known to the Indians and were worked by them. Remains of ancient operationsare still to be seen, while stone hammers, implements and fragments of pottery have been found near the old excavations.