 | | Book | | in your own back yard Author: HUGH CARMAN Hill of Content Editor: TOM KAPITANY To my wife Ann, for...by Marvin Killgore of Arizona, in his demonstration of preparing the meteorite for presentation and...acknowledge the assistance given by the Museum of Victoria, Melbourne in providing meteorites and photographic...presentable manner. First published in Australia in 1995 by Hill of Content Publishing Company Pty Ltd 86...86 Bourke Street Melbourne 3000 Australia © Copyright Hugh Carman 1995 Cover photograph: Rachael Kapitany |  | Liu, Chao, Hystad, Grethe, Golden, Joshua J., Hummer, Daniel R., Downs, Robert T., Morrison, Shaunna M., Ralph, Jolyon P., Hazen, Robert M. (2017) Chromium mineral ecology. American Mineralogist, 102 (3) 612-619 doi:10.2138/am-2017-5900 | Journal (article/letter/editorial) | | Road NW, Washington, D.C. 20015, U.S.A. Department of Mathematics, Computer Science, and Statistics, Purdue...Indiana 46323, U.S.A. 3 Department of Geosciences, University of Arizona, 1040 East 4th Street, Tucson...Tucson, Arizona 85721-0077, U.S.A. 4 Department of Geology, Southern Illinois University, Carbondale, Illinois...terrestrial Cr mineral species (http://rruff.info/ima, as of 15 April 2016), representing 4089 mineral species-locality...species-locality pairs (http://mindat.org and other sources, as of 15 April 2016). We find that Cr-containing mineral |  | | Journal (article/letter/editorial) | | mineral from the Murchison meteorite Chi Ma,* John r. BeCkett, and GeorGe r. rossMan Division of Geological...Geological and Planetary Sciences, California Institute of Technology, Pasadena, California 91125, U.S.A. aBstraCt...chromium sulfide mineral, discovered in the Murchison CM2 meteorite. The type material occurs as one subhedral...iron, schreibersite, and a Ca-,Al-rich glass, all of which are included in an isolated forsteritic olivine...composition determined by electron microprobe analysis of the type material is (wt%) Cr 53.32, S 42.87, V 1 |  | | Report (issue) | | Mineral-Chemistry, and Composition of the Murchison (C2) Meteorite LOUIS H. FUCHS, EDWARD OLSEN, and...PUBLICATIONS OF THE SMITHSONIAN INSTITUTION The emphasis upon publications as a means of diffusing knowledge...knowledge was expressed by the first Secretary of the Smithsonian Institution. In his formal plan for the...publish a series of reports, giving an account of the new discoveries in science, and of the changes made...made from year to year in all branches of knowledge.” This keynote of basic research has been adhered to |  | BRAATZ, A., OTT, U., HENNING, Th., JÄGER, C., JESCHKE, G. (2000) Infrared, ultraviolet, and electron paramagnetic resonance measurements on presolar diamonds: Implications for optical features and origin. Meteoritics & Planetary Science, 35 (1) 75-84 doi:10.1111/j.1945-5100.2000.tb01975.x | Journal (article/letter/editorial) | | were obtained for diamonds from the Allende and Murchison meteorites. In addition, and for the first time...suspicion of Russell et al. (1996) that N in presolar diamonds predominantly appears in the form of dispersed...twin microstructures of presolar diamonds (Daulton et al., 1996) and the absence of graphite with the same...homogeneous nucleation of presolar diamonds from a gas phase. Based on our results for detection of diamonds in...searching for the N-induced IR and UV absorption features of type Ib diamonds. Other characteristic diamond features |  | | Journal (article/letter/editorial) | | reconstructions of ancient meteorite fluxes 1* € Karolina BJARNBORG and Birger SCHMITZ2,3 1 Department of Geology...University of Lund, S€ olvegatan 12, Lund SE-22362, Sweden Department of Physics, University of Lund, P...Center for Meteoritics and Polar Studies, Department of Geology, The Field Museum, 1400 S. Lake Shore Drive...29 October 2012) Abstract–By dissolving 30–400 kg of marine limestone in HCl and HF acid, our group has...has previously recovered common relict chromite grains (approximately 63–250 lm) from ordinary chondritic |  | | Journal (article/letter/editorial) | | anomalies of noble gases in meteorites and their origins-VI. Presolar components in the Murchison C2 chondrite...Enrico Fermi Institute and Department of Chemistry, University of Chicago. Chicago, IL 60437. U.S.A. Abstract-Noble...heating in 5 fractions of a chemically resistant residue (0.27pJ from Murchison that had been separated...resistance to HCIO,. Nine gas components were recognized, of which 3 appear to be presolar. (1) Ne-E(H): (NeZo/NeZ2...<8W and apparently located in a carbonaceous phase of grain size up to 10pm. Both seem to be unaccompanied |  | Bunch, T.E., Chang, S., Frick, U., Neil, J., Moreland, G. (1979) Carbonaceous chondrites—I. Characterization and significance of carbonaceous chondrite (CM) xenoliths in the Jodzie howardite. Geochimica et Cosmochimica Acta, 43 (11) 1727-1742 doi:10.1016/0016-7037(79)90021-8 | Journal (article/letter/editorial) | | Car~naceous chondrites-I. Characterization and si~ificance of carbonaceous chondrite (CM) xenoliths in the Jodzie...94035, U.S.A. %zpartment of Physics and ?Space Science Laboratory, University of California-Berkeley, Berkeley...Berkeley, CA 94720, U.S.A. ‘Division of Meteorites, Smithsonian Institution, Washington, DC 20560, U.S...Abstract-Mineralogical, chemical, textural, and isotopic studies of the abundant carbonaceous inclusions in the Jodzie...alteration on a level comparable to the Murray and Murchison meteorites but less than Nagoya, flow-oriented |  | | Journal (article/letter/editorial) | | MSA Centennial Symposium An evolutionary system of mineralogy. Part I: Stellar mineralogy (>13 to 4...Minerals preserve records of the physical, chemical, and biological histories of their origins and subsequent...vivid narrative of the evolution of Earth and other worlds through billions of years of cosmic history...properties, including trace and minor elements, ratios of isotopes, solid and fluid inclusions, external morphologies...represent information that points to specific modes of formation and subsequent environmental histories—information |  | Simon, S.B., Grossman, L., Podosek, F.A., Zinner, E., Prombo, C.A. (1994) Petrography, composition, and origin of large, chromian spinels from the Murchison meteorite. Geochimica et Cosmochimica Acta, 58 (4) 1313-1334 doi:10.1016/0016-7037(94)90384-0 | Journal (article/letter/editorial) | | composition, and origin of large, chromian spinels from the Murchison meteorite SIMON.’ L. GROSSMAN,‘...C. A. PROMBO~.~ ‘Department of Geophysical Sciences, The University of Chicago, 5734 South Ellis Avenue...60637, USA *Enrico Fermi Institute, The University of Chicago. 5630 South Ellis Avenue. Chicago, IL 60637...Drive, St. Louis, MO 63 130-4899, USA 4Department of Earth and Planetary Sciences, Washington University...University. St. Louis, MO 63 130, USA ‘Department of Physics, Washington University. St. Louis. MO 63 130. USA |  | | Journal (article/letter/editorial) | | Netherlands [61 IRON-NICKEL SULFIDES IN THE MURCHISON METEORITE AND THEIR RELATIONSHIP TO PHASE Q1 JOHN F...Scripps Institution o f Oceanography, University of California, La Jolla, CA 92093 (U.S.A.) Received...received January 2, 1979 Pentlandite from the Murchison meteorite survivesHF-HCIattack and dissolvesin HNO3...satisfying the operational definition of phase Q 1, the proposed major carrier of carbonaceous chondrite fission...However, identification of pentlandite with that phase is problematical in view of apparently differing |  | | Journal (article/letter/editorial) | | isotope anomalies and large 13C enrichments in a family of exotic SiC grains J. Stone *, I . D . H u t c h e...Wasserburg ** Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena...suite of morphologically distinctive silicon carbide (SIC) grains from the Orgueil and Murchison carbonaceous...meteorites contains Si and C of highly anomalous isotopic composition. All of the SiC grains in this suite...from other types of SiC found in the host meteorites. The 629Si and 63~)Si values of individual SiC crystals |  | | Journal (article/letter/editorial) | | chromium isotope measurement of chromium-rich fine grains in the Murchison CM2 chondrite W. FUJIYA ,1*...HIYAGON1 2 1 Department of Earth and Planetary Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku...Atmosphere and Ocean Research Institute, The University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa-shi, Chiba 277-8568...2010; Accepted February 9, 2011) Isotopic anomalies of 54Cr have been reported in bulk chondrites. Stepwise...have suggested the presence of a carrier of the 54Cr anomaly, probably of presolar origin. Although stepwise |  | | Report (issue) | | 2 Luster: n.d. X-ray Powder Pattern: Murchison CM2 meteorite. 2.074 (100), 2.654 (86), 1.727 (86), 2...98.97 (2) 57.47 42.53 . 100.00 (1) Murchison CM2 meteorite; average electron microprobe analysis;...serpentine, chromite, eskolaite (crystal 2). Distribution: From the Murchison CM2 meteorite. Name: For...For the Murchison meteorite. Type Material: National Museum of Natural History, Washington, D.C., USA (USNM...mineral from the Murchison meteorite. Amer. Mineral., 96, 1905-1908. Mineralogical Society of America Handbook |  | Croat, T. K., Berg, T., Bernatowicz, T., Groopman, E., Jadhav, M. (2013) Refractory metal nuggets within presolar graphite: First condensates from a circumstellar environment. Meteoritics & Planetary Science, 48 (4) 686-699 doi:10.1111/maps.12093 | Journal (article/letter/editorial) | | Germany 4 Hawai‘i Institute of Geophysics and Planetology, University of Hawai‘i at Manoa, Honolulu,...presolar graphites, from both the high-density (HD) Murchison (MUR) and low-density (LD) Orgueil (ORG) fractions...compositions one can infer a temperature of last equilibration with the gas of 1405–1810 K (e.g., Berg et al. [2009]...too small for detection of isotopic anomalies, NanoSIMS isotopic measurements of their host graphites confirm...graphites show evidence of a supernova (SN) origin, whereas the stellar origins of the pRMNs in HD graphite |  | Noguchi, Takaaki, Nakamura, Tomoki, Okudaira, Kyoko, Yano, Hajime, Sugita, Seiji, Burchell, Mark J. (2007) Thermal alteration of hydrated minerals during hypervelocity capture to silica aerogel at the flyby speed of Stardust. Meteoritics & Planetary Science, 42 (3) 357-372 doi:10.1111/j.1945-5100.2007.tb00239.x | Journal (article/letter/editorial) | | alteration of hydrated minerals during hypervelocity capture to silica aerogel at the flyby speed of Stardust...Seiji SUGITA5, and Mark J. BURCHELL6 1Department of Materials and Biological Sciences, Ibaraki University...Bunkyo, Mito 310-8512, Japan of Earth and Planetary Sciences, Faculty of Science, Kyushu University, 6-10-1...University of Advanced Studies (Sokendai), 3-1-1 Yoshinodai, Sagamihara 229-8510, Japan 4Institute of Space...229-8510, Japan 5Graduate School of Frontier Sciences, University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa |  | | Journal (article/letter/editorial) | | A. 0067037/88/$3.@3 + .oo Isotopic anomalies of Ne, Xe, and C in meteorites. III. Local and exotic...Enrico Fermi Institute and Department of Chemistry, University of Chicago, Chicago, IL 60637, U.S.A. (Received...ambitions are obtained for Ne-A1 and Ne-A2,two su~rn~nen~ of “planetary” Ne: NeZo/NeZZ = 8.86 f 0.09. 8.46 f 0...+ 0.0012. Ne-Al is associated with a special type of planetary Xe (Xe-P3). Both Ne-Al and Xe-P3 closely...Xe-HL, but are located in a separate carrier (Co of high chemical but low thermal resistance (amorphous |  | | Journal (article/letter/editorial) | | Isotopic anomalies of noble gases in meteorites and their origins-VII. C3V carbonaceous ~hondrites JIJN-ICHI... Fermi Institute and Department of Chemistry. University of Chicago. Chicago. 1L 60637 U.S.A. ...AbstractNoble gases were measured in bulk samples of the C3V chondrites Grosnaja, Vigarano. and Leoville...(>98”, of the meteorite), ‘phuw Q.‘ a poorly characterized and an insoluble residue, consisting of mineral...and spinel. Bulk meteorites show some correlation of the noble-gas pattern with McSween’s subclasses: |  | | Journal (article/letter/editorial) | | and stepwise pyrolyses of insoluble organic matter from the Murchison meteorite revealing chemical structure...distribution Fumiaki Okumura 1, Koichi Mimura ⇑ Department of Earth and Environmental Sciences, Nagoya University...heterogeneity of the insoluble organic matter (IOM) of the Murchison meteorite, we performed two types of pyrolytic...and the compositions of these pyrolysates demonstrated that the IOM is composed of a thermally unstable...IOM. The linkage and substituent portion consisted of aliphatic hydrocarbons from C4 to C8, aromatic hydrocarbons |  | | Journal (article/letter/editorial) | | Department of Chemistry, University of Canterbury, Christchurch 8001, New Zealand Institute of Plant Sciences...Sciences, Swiss Federal Institute of Technology Zurich (ETHZ), Postfach 185, CH-83-15 Eschikon Lindau,...extraction contributes to the formation and weathering of planetary materials and renders electrolytes such...available for biology. In this context, the solubility of phosphate is measured in planetary materials, represented...(EETA 79001), and terrestrial analogs, and in the Murchison CM2 and Allende CV3 carbonaceous chondrites. The |  | Zolensky, Michael E., Mittlefehldt, David W., Lipschutz, Michael E., Wang, Ming-Sheng, Clayton, Robert N., Mayeda, Toshiko K., Grady, Monica M., Pillinger, Colin, B, David (1997) CM chondrites exhibit the complete petrologic range from type 2 to 1. Geochimica et Cosmochimica Acta, 61 (23) 5099-5115 doi:10.1016/s0016-7037(97)00357-8 | Journal (article/letter/editorial) | | NASA Rd. 1, Houston, Texas 77058, USA 3Depamnent of Chemistry, Purdue University, West Lafayette, Indiana...Indiana 47907, USA 4Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637, USA 5Planetary...Keynes, MK7 6AA, UK 6physics Department, University of Essex, Colchester Essex CO4 3SQ, UK (Received September...characterized the most phyllosilicate-rich members of the CM chondrite group. Based upon petrographic and...lack of anhydrous silicates, CAI and (except as relicts) chondrules merits the classification of type |  | Stalport, F., Glavin, D.P., Eigenbrode, J.L., Bish, D., Blake, D., Coll, P., Szopa, C., Buch, A., McAdam, A., Dworkin, J.P., Mahaffy, P.R. (2012) The influence of mineralogy on recovering organic acids from Mars analogue materials using the “one-pot” derivatization experiment on the Sample Analysis at Mars (SAM) instrument suite. Planetary and Space Science, 67 (1) 1-13 doi:10.1016/j.pss.2012.02.010 | Journal (article/letter/editorial) | | homepage: www.elsevier.com/locate/pss The influence of mineralogy on recovering organic acids from Mars...temperature and duration of the derivatization reaction, pre-concentration of chemical derivatives, and...several minutes of a variety of terrestrial Mars analog materials facilitated the detection of amino acids...reaction of MTBSTFA with water in several analog materials that contained high abundances of hydrated...hydrated minerals, and the possible deactivation of derivatized compounds by iron oxides, as detected by XRD/XRF |  | Merchel, Silke, Ott, Ulrich, Herrmann, Siegfried, Spettel, Bernhard, Faestermann, Thomas, Knie, Klaus, Korschinek, Gunther, Rugel, Georg, Wallner, Anton (2003) Presolar nanodiamonds: faster, cleaner, and limits on platinum-HL. Geochimica et Cosmochimica Acta, 67 (24) 4949-4960 doi:10.1016/s0016-7037(03)00421-6 | Journal (article/letter/editorial) | | extraction of clean nanodiamond samples from primitive meteorites for isotopic analyses of trace elements...timescale of just a week. This procedure includes microwave digestion and optimization of existing isolation...isolation techniques for further purification. Abundances of trace elements that are difficult to dissolve using...obtained on diamond fractions from Allende and Murchison show the need for suitable matrix-adjusted standards...the abundance of 198Pt-H in nanodiamonds of ⬃1 ⫻ 1014 atoms/g. This limit is on the order of what can be |  | | Journal (article/letter/editorial) | | meteorites: I. Isolation of Sic, graphite, and diamond; size distributions of Sic and graphite SACHIKOAMARI...Enrico Fermi Institute and Department of Chemistry, University of Chicago, Chicago, IL 60637-1433, USA...three types of interstellar grains from primitive meteorites, in >90% purity and yields of generally r70%...r70%, and is here applied to the Murchison C2M meteorite. Silicates are dissolved in HF-HCl, kerogen...size distribution of SIC has been measured in the range 0.2 to 6 pm. Over part of this range, it can |  | | Journal (article/letter/editorial) | | 1979. Printed in Great Britain Isotopic anomalies of noble gases in meteorites and their origins-IV. C3...Enrico Fermi Institute and Department of Chemistry, University of Chicago, Chicago, IL 60637 and t Physikalisches...Physikalisches Institut, University of Bern, 3012 Bern, Switzerland (Received 22 December 1978; accepted...mineral fractions: NF, HCf-sofubfes (99% of the meteorite), chromite and carbon (0.3-0.9%), and ‘phase Q:...characterized trace minerai (0.05-0.4°~) containing most of the Ar, Kr, Xe. For all fractions, gas contents decline |
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