Handbook of Iron Meteorites, Volume 3 (Okano – Paloduro)
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Handbook of Iron Meteorites, Volume 3
Sierra Blanca - Sierra Gorda 1119 ing that created an incipient recrystallization and a few COLLECTIONS other anomalous features in Sierra Blanca. Washington (17 .3 kg), Ferry Building, San Francisco (about 7 kg), Chicago (550 g), New York (315 g), Ann Arbor (165 g). The original mass evidently weighed at least Sierra Gorda, Antofagasta, Chile 26 kg. 22°54's, 69°21 'w Hexahedrite, H. Single crystal larger than 14 em. Decorated Neu DESCRIPTION mann bands. HV 205± 15. According to Roy S. Clarke (personal communication) Group IIA . 5.48% Ni, 0.5 3% Co, 0.23% P, 61 ppm Ga, 170 ppm Ge, the main mass now weighs 16.3 kg and measures 22 x 15 x 43 ppm Ir. 13 em. A large end piece of 7 kg and several slices have been removed, leaving a cut surface of 17 x 10 em. The mass has HISTORY a relatively smooth domed surface (22 x 15 em) overlying a A mass was found at the coordinates given above, on concave surface with irregular depressions, from a few em the railway between Calama and Antofagasta, close to to 8 em in length. There is a series of what appears to be Sierra Gorda, the location of a silver mine (E.P. Henderson chisel marks around the center of the domed surface over 1939; as quoted by Hey 1966: 448). Henderson (1941a) an area of 6 x 7 em. Other small areas on the edges of the gave slightly different coordinates and an analysis; but since specimen could also be the result of hammering; but the he assumed Sierra Gorda to be just another of the North damage is only superficial, and artificial reheating has not Chilean hexahedrites, no further description was given. -
Open Research Online Oro.Open.Ac.Uk
Open Research Online The Open University’s repository of research publications and other research outputs The Moss (CO3) meteorite: an integrated isotopic, organic and mineralogical study Conference or Workshop Item How to cite: Greenwood, R. C.; Pearson, V. K.; Verchovsky, A. B.; Johnson, D.; Franchi, I. A.; Roaldset, E.; Raade, G. and Bartoschewitz, R. (2007). The Moss (CO3) meteorite: an integrated isotopic, organic and mineralogical study. In: 38th Lunar and Planetary Science Conference (Lunar and Planetary Science XXXVIII), 12-16 Mar 2007, Houston, Texas. For guidance on citations see FAQs. c [not recorded] Version: [not recorded] Link(s) to article on publisher’s website: http://www.lpi.usra.edu/meetings/lpsc2007/pdf/2267.pdf Copyright and Moral Rights for the articles on this site are retained by the individual authors and/or other copyright owners. For more information on Open Research Online’s data policy on reuse of materials please consult the policies page. oro.open.ac.uk Lunar and Planetary Science XXXVIII (2007) 2267.pdf THE MOSS (CO3) METEORITE: AN INTEGRATED ISOTOPIC, ORGANIC AND MINERALOGICAL STUDY. R. C. Greenwood1, V. K. Pearson1, A. B. Verchovsky1, D. Johnson1, I. A. Franchi1, E. Roaldset2, G. Raade2 and R. Bartoschewitz3, 1Planetary and Space Sciences Research Institute, Open University, Milton Keynes, MK7 6AA, UK. E-mail: [email protected]; 2Naturhistorisk museum, Universitetet i Oslo, Postboks 1172 Blindern, 0318 Oslo, Norway; 3Meteorite Laboratory, Lehmweg 53, D-38518 Gifhorn, Germany. Introduction: Following a bright fireball and a oxygen three-isotope diagram (Fig.1) previously ana- loud explosion the Moss meteorite fell on 14 July 2006 lyzed CO3 falls plot as a tight central cluster with CO3 at approximately 10:20am in the Moss-Rygge area on finds on either side [7]. -
March 21–25, 2016
FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk, -
Geological Survey Canada
70-66 GEOLOGICAL PAPER 70-66 ., SURVEY OF CANADA DEPARTMENT OF ENERGY, MINES AND RESOURCES REVISED CATALOGUE OF THE NATIONAL METEORITE COLLECTION OF CANADA LISTING ACQUISITIONS TO AUGUST 31, 1970 J. A. V. Douglas 1971 Price, 75 cents GEOLOGICAL SURVEY OF CANADA CANADA PAPER 70-66 REVISED CATALOGUE OF THE NATIONAL METEORITE COLLECTION OF CANADA LISTING ACQUISITIONS TO AUGUST 31, 1970 J. A. V. Douglas DEPARTMENT OF ENERGY, MINES AND RESOURCES @)Crown Copyrights reserved Available by mail from Information Canada, Ottawa from the Geological Survey of Canada 601 Booth St., Ottawa and Information Canada bookshops in HALIFAX - 1735 Barrington Street MONTREAL - 1182 St. Catherine Street West OTTAWA - 171 Slater Street TORONTO - 221 Yonge Street WINNIPEG - 499 Portage Avenue VANCOUVER - 657 Granville Street or through your bookseller Price: 75 cents Catalogue No. M44-70-66 Price subject to change without notice Information Canada Ottawa 1971 ABSTRACT A catalogue of the National Meteorite Collection of Canada, published in 1963 listed 242 different meteorite specimens. Since then specimens from 50 a dditional meteorites have been added to the collection and several more specimens have been added to the tektite collection. This report describes all specimens in the collection. REVISED CATALOGUE OF THE NATIONAL METEORITE COLLECTION OF CANADA LISTING ACQUISITIONS TO AUGUST 31, 1970 INTRODUCTION At the beginning of the nineteenth century meteorites were recog nized as unique objects worth preserving in collections. Increasingly they have become such valuable objects for investigation in many fields of scienti fic research that a strong international interest in their conservation and pre servation has developed (c. f. -
W Numerze: – Wywiad Z Kustoszem Watykańskiej Kolekcji C.D. – Cz¹stki
KWARTALNIK MI£OŒNIKÓW METEORYTÓW METEORYTMETEORYT Nr 3 (63) Wrzesieñ 2007 ISSN 1642-588X W numerze: – wywiad z kustoszem watykañskiej kolekcji c.d. – cz¹stki ze Stardusta a meteorytry – trawienie meteorytów – utwory sp³ywania na Sikhote-Alinach – pseudometeoryty – konferencja w Tucson METEORYT Od redaktora: kwartalnik dla mi³oœników OpóŸnieniami w wydawaniu kolejnych numerów zaczynamy meteorytów dorównywaæ „Meteorite”, którego sierpniowy numer otrzyma³em Wydawca: w paŸdzierniku. Tym razem g³ówn¹ przyczyn¹ by³y k³opoty z moim Olsztyñskie Planetarium komputerem, ale w koñcowej fazie redagowania okaza³o siê tak¿e, i Obserwatorium Astronomiczne ¿e brak materia³u. Musia³em wiêc poczekaæ na mocno opóŸniony Al. Pi³sudskiego 38 „Meteorite”, z którego dorzuci³em dwa teksty. 10-450 Olsztyn tel. (0-89) 533 4951 Przeskok o jeden numer niezupe³nie siê uda³, a zapowiedzi¹ [email protected] dalszych k³opotów jest mi³y sk¹din¹d fakt, ¿e przep³yw materia³ów zacz¹³ byæ dwukierunkowy. W najnowszym numerze „Meteorite” konto: ukaza³ siê artyku³ Marcina Cima³y o Moss z „Meteorytu” 3/2006, 88 1540 1072 2001 5000 3724 0002 a w kolejnym numerze zapowiedziany jest artyku³ o Morasku BOŒ SA O/Olsztyn z „Meteorytu” 4/2006. W rezultacie jednak bêdzie mniej materia³u do Kwartalnik jest dostêpny g³ównie t³umaczenia i trzeba postaraæ siê o dalsze w³asne teksty. Czy mo¿e ktoœ w prenumeracie. Roczna prenu- merata wynosi w 2007 roku 44 z³. chcia³by coœ napisaæ? Zainteresowanych prosimy o wp³a- Z przyjemnoœci¹ odnotowujê, ¿e nabieraj¹ tempa przygotowania cenie tej kwoty na konto wydawcy do kolejnej konferencji meteorytowej, która planowana jest na 18—20 nie zapominaj¹c o podaniu czytel- nego imienia, nazwiska i adresu do kwietnia 2008 r. -
Texture, Chemical Composition and Genesis of Schreibersite in Iron Meteorite
Title Texture, Chemical Composition and Genesis of Schreibersite in Iron Meteorite Author(s) Yoshikawa, Masahide; Matsueda, Hiroharu Citation 北海道大学理学部紀要, 23(2), 255-280 Issue Date 1992-08 Doc URL http://hdl.handle.net/2115/36782 Type bulletin (article) File Information 23-2_p255-280.pdf Instructions for use Hokkaido University Collection of Scholarly and Academic Papers : HUSCAP Jour. Fac. Sci ., Hokkaido Univ., Ser. IV, vol. 23, no. 2, Aug., 1992. pp. 255 -280 TEXTURE, CHEMICAL COMPOSITION AND GENESIS OF SCHREIBERSITE IN IRON METEORITE by Masahide Yoshikawa* and Hiroharu Matsueda (with 13 text-figures, 9 tables and 3 plates) Abstract Thirteen iron meteorites composed of Hexahedrite, Octahedrite and Ataxite were investigated to estimate their cooling history and origin. They are mainly composed of Fe-Ni metals (kamacite and taenite) with smaller amounts of schreibersite (Fe, Ni)3P and sulfides (troilite and sphalerite) . Schreibersite occurs an idiomorphic and xenomorphic crystals and its mode of occurrence is variable in iron meteorites. Xenomorphic schreibersite is subdivided into 6 types on the basis of their textures and relationships with coexisting minerals. Chemical composition of schreibersite varies from 20 to 40 atom. % Ni with textural types among some iron meteorites with different bulk chemical compositions and even in the same meteorite (e. g. Canyon Diablo), while it does not vary so clear with textural types in ALH - 77263. Schreibersite seems to maintain a local equilibrium with coexisting metal phases. Based on the Fe- Ni- P phase diagram, it is estimated that xenomorphic and coarse-grained schreibersite in Y- 75031 and in DRPA 7S007 were crystallized from stability field of taenite and schreibersite at about SOO°C under rapid diffusion conditions. -
Siderophile Elements and Molybdenum, Tungsten, And
ABSTRACT Title of Dissertation: SIDEROPHILE ELEMENTS AND MOLYBDENUM, TUNGSTEN, AND OSMIUM ISOTOPES AS TRACERS OF PLANETARY GENETICS AND DIFFERENTIATION: IMPLICATIONS FOR THE IAB IRON METEORITE COMPLEX Emily Anne Worsham, Doctor of Philosophy, 2016 Dissertation directed by: Professor Richard Walker, Department of Geology Isotopic and trace element abundance data for iron meteorites and chondrites are presented in order to investigate the nature of genetic relations between and among meteorite groups. Nebular and planetary diversity and processes, such as differentiation, can be better understood through study of IAB complex iron meteorites. This is a large group of chemically and texturally similar meteorites that likely represent metals with a thermal history unlike most other iron meteorite groups, which sample the cores of differentiated planetesimals. The IAB complex contains a number of chemical subgroups. Trace element determination and modeling, Re/Os isotopic systematics, nucleosynthetic Mo isotopic data, and 182Hf-182W geochronology are used to determine the crystallization history, genetics, and relative metal-silicate segregation ages of the IAB iron meteorite complex. Highly siderophile element abundances in IAB complex meteorites demonstrate that diverse crystallization mechanisms are represented in the IAB complex. Relative abundances of volatile siderophile elements also suggest late condensation of some IAB precursor materials. Improvements in the procedures for the separation, purification, and high- precision analysis of Mo have led to a ~2 fold increase in the precision of 97Mo/96Mo isotope ratio measurements, compared to previously published methods. Cosmic ray exposure-corrected Mo isotopic compositions of IAB complex irons indicate that at least three parent bodies are represented in the complex. The Hf-W metal-silicate segregation model ages of IAB complex subgroups suggests that at least four metal segregation events occurred among the various IAB parent bodies. -
Handbook of Iron Meteorites, Volume 3 (Willow Creek – Wood's Mountian)
Willamette - Willow Creek 1321 Stage four would be the penetration of the atmos Williamstown. See Kenton County phere. However, no remnants of the associated sculpturing (Williamstown) are to be seen today. The fusion crust and heat-affected o:2 zones are all removed by weathering. Immediately after its landing, the external shape of Willamette may have re Willow Creek, Wyoming, U.S.A. sembled that of Morito rather closely. Stage five is the final long-term exposure in the humid 43°26'N, 106° 46'W; about 1,800 m Oregon valley forest during which the deep cavities, partially penetrating and generally perpendicular to the Coarse octahedrite, Og. Bandwidth 1.40±0.25 mm. Partly recrystal topside of the mass, were formed. While no large-scale lized . HV 152±6. texture, such as silicate inclusions, can be considered Group IIIE. 8.76% Ni, about 0.35% P, 16.9 ppm Ga, 36.4 ppm Ge, responsible for the curious corrosion progress, it is possible 0 .05 ppm lr. that the very distinct troilite filaments have aided in the weathering. These lanes of fine-grained troilite, kamacite HISTORY and taenite would probably provide easy diffusion paths A mass of 112.5 pounds (51 kg) was found by John studded with electrochemical cells and with dilute sulfuric Forbes of Arminto, Wyoming, near Willow Creek, Natrona acid from decomposed troilite, where the kamacite phase County, about 1914. For a long time it was in the would provide the anodic areas and dissolve first. The final possession of the Forbes family, but in 1934 the meteorite product, the deeply carved Willamette mass, must, however, be seen to be believed. -
Pn S0016.7O37(O2 -7 the Lab Iron-Meteorite Complex: a Group
• / ] _caJ21_gcW211702/2_/9/02 14:24 Art: At'dole Input-lst disk, 2nd CW-trm] i i Oeoc/aumica ¢t Colimo¢/= 'mi¢l _ Vol. 66. No. I 7, pp. 000, _0012 Copynpt O 2002Br,ev_¢ Sclmm Lid ..,y Pergamon _16-7o37_o_$22.00 ÷ .o0 Primed|n_ USA. All ngh_ Pn s0016.7o37(o2_-7 The lAB iron-meteorite complex: A group, five subgroups, numerous grouplets, closely related, mainly formed by crystal segregation in rapidly cooling melts J T. W^_ _*_ and G. W. K_a_.M_VN Institute of Gee,physics mid planetary I'hy_lcr_.Univcl"slty of CalU'OITItlLLos Angeles. CA 90095-1567. USA _Ot,_ _ (Recetve,I A,_as_ 7. 2001; a_cepted mrev, sed form January 21. 2002) A__A_WL present new data tt_r mm meteorites that are members of group lAB or are closely related to this lar'[lxe g'r_up._and we have aiNt_ reevaluated some ot our earlier data for these irons. At.'_c':=_ LS_..c,-'.,.z _. __a_t_o d_stln_u_:,n lAB and IIICD irons on the basts of their positions on element-Ni diagrams._we tiadhthat plotting the new and rcvl_d data yields six sets of compact fields on element-Au diagrams, each set corresponding t,_ a _.omposmonal group. The largest set includes the majority (,,.,70) of irons previously designated IA: v,c christened this _t the lAB maan group. The _maining live sets we designate "subgroups" w_thtn the iAB complex Three of these subgroups have Au contents similar to the main group, and form parallel trcntl_ on most elcment-Ni diagrams. -
Elements M Meteoritic Minerals
SMITHSONIAN CONTRIBUTIONS TO THE EARTH SCIENCES NUMBER 3 Brian Mason Minor and Trace and A. L. Graham pi t Elements m Meteoritic Minerals SMITHSONIAN INSTITUTION PRESS CITY OF WASHINGTON 1970 ABSTRACT Mason, Brian and A. L. Graham. Minor and Trace Elements in Meteoritic Minerals. Smithsonian Contributions to the Earth Sciences, 3:1—17. 1970.—Nickel-iron, troilite, olivine, pyroxenes, plagioclase, chromite, and phosphate minerals (chlor- apatite and/or merrillite) have been separated from a number of meteorites (Modoc, St. Severin, Winona, Haraiya, Marjalahti, Springwater, Johnstown, Mt. Egerton, Soroti) and analyzed for minor and trace elements with the spark-source mass spectrometer. The elements Ni, Go, Ge, As, Ru, Rh, Pd, Sn, Sb, W, Re, Os, Ir, Pt, and Au are concentrated in nickel-iron: Se and Ag in troilite; Th, U, and the lanthanides in the phosphate minerals and in diopside; Eu, Sr, Ba, Rb, and Gs in plagioclase. Molybdenum and tellurium are concentrated in nickel-iron and troilite. The elements Ti, Sc, V, Cu, Zn, Mn, and Ga are distributed over several coexisting minerals. Official publication date is handstamped in a limited number of initial copies and is recorded in the Institution's annual report, Smithsonian Year. UNITED STATES GOVERNMENT PRINTING OFFICE WASHINGTON : 1970 For sale by the Superintendent of Documents, U.S. Government Printing Office Washington, D.C. 20402 - Price 30 cents (paper cover) Brian Mason Minor and Trace and A. L. Graham Elements in Meteoritic Minerals Introduction Vilcsek and Wanke (1965) and Honda and Shima (1967) ; however, study of their results indicates that During the past decade a very large amount of data this selective solution is seldom completely quantitative. -
(Co3) Meteorite: an Integrated Isotopic, Organic and Mineralogical Study
Lunar and Planetary Science XXXVIII (2007) 2267.pdf THE MOSS (CO3) METEORITE: AN INTEGRATED ISOTOPIC, ORGANIC AND MINERALOGICAL STUDY. R. C. Greenwood1, V. K. Pearson1, A. B. Verchovsky1, D. Johnson1, I. A. Franchi1, E. Roaldset2, G. Raade2 and R. Bartoschewitz3, 1Planetary and Space Sciences Research Institute, Open University, Milton Keynes, MK7 6AA, UK. E-mail: [email protected]; 2Naturhistorisk museum, Universitetet i Oslo, Postboks 1172 Blindern, 0318 Oslo, Norway; 3Meteorite Laboratory, Lehmweg 53, D-38518 Gifhorn, Germany. Introduction: Following a bright fireball and a oxygen three-isotope diagram (Fig.1) previously ana- loud explosion the Moss meteorite fell on 14 July 2006 lyzed CO3 falls plot as a tight central cluster with CO3 at approximately 10:20am in the Moss-Rygge area on finds on either side [7]. The oxygen isotope analysis the east side of Oslofjord [1]. 5 stones were subse- for Moss plots within this central cluster and hence quently recovered with a total mass of nearly 4 kg [1]. confirms it as being a CO3 chondrite. Petrography, mineralogy and oxygen isotope analysis confirm that Moss is a carbonaceous chondrite of the Ornans group (CO3) [1]. Ornans-type chondrites are a distinct group with a characteristic texture consisting of a high density of small (0.2 – 0.5 mm) chondrules, inclusions and lithic fragments enclosed by a dark matrix. They also have a significantly lower matrix to chondrule ratio than other carbonaceous chondrites [2, 3]. As a consequence of this textural coherence, CO3 chondrites are thought to represent samples from a single asteroid. Unique among the carbonaceous chondites, the Ornans group show textural, mineralogical and isotopic evidence for a metamorphic series analogous to that seen in the or- dinary chondrites [4, 5, 6, 7]. -
Download Article (PDF)
Seven Shock-transformed Hexahedrites, Sensitive to Grainboundary Corrosion V. F. Buchwald Department of Metallurgy, Technical University, Lyngby, Denmark Z. Naturforsch. 35a, 361-369 (1980); received January 21, 1980* Dedicated to Professor II. Hintenberger on the occasion of his 70th birthday. Seven polycrystalline iron meteorites (Forsyth County, Holland's Store, Wathena, Pima Co., Chico Mountains, Kopjes Vlei and Mejillones), of bulk composition as normal hexahedrites of group 11 A, are shown to be severely altered hexahedrites. Mic-roprobe examination and various heat treatments of synthetic alloys support the conclusion that the meteorites after a primary slow cooling were subjected to shock-reheating above 800°C. Thereby the following transforma- tions took place a-^-y—>a2—>a, and an unequilibrated structure, very sensitive to grain-boundary corrosion was formed. Introduction Table 1. Weight and bulk composition of the seven polv- crystalline iron meteorites. Other important elements are The last ten years have seen a very significant iron (about 93%), cobalt (0.5%) and sulfur (0.1%). progress with respect to understanding the structure Weight percent PPm and composition of iron meteorites. The efforts in analysing for main and trace elements have resulted kg Ni P Ga Ge Ir in a classification system [1, 2] that may form the Forsyth basis for all further discussions. Mass-spectrometric County 23 5.54 0.21 60 176 31 work [3, 4] has provided valuable insight in the Holland's Store 12.5 5.35 0.25 61 184 20 isotopic composition and the content of noble gases, Wathena 0.57 5.54 0.27 60 184 7.0 data which allow us among other things to deduce Pima the age of meteorites, and the intensity of the cosmic County 0.21 5.60 0.25 60 181 8.9 Chico' radiation.