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| | 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 | 👁 Image
| 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 | 👁 Image
| | 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 | 👁 Image
| | 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 | 👁 Image
| 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 | 👁 Image
| | 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 | 👁 Image
| | 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 | 👁 Image
| | 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 | 👁 Image
| 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 | 👁 Image
| 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
S. B. 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 | 👁 Image
| | 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 | 👁 Image
| | 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 | 👁 Image
| | 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 | 👁 Image
| 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 | 👁 Image
| 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...310-8512, Japan
2Department 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 | 👁 Image
| | 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 | 👁 Image
| | Journal (article/letter/editorial) | | S.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 | 👁 Image
| | 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 | 👁 Image
| | 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: | 👁 Image
| | 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 | 👁 Image
| 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 | 👁 Image
| 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 | 👁 Image
| Croat, T.Kevin, Bernatowicz, Thomas, Amari, Sachiko, Messenger, Scott, Stadermann, Frank J (2003) Structural, chemical, and isotopic microanalytical investigations of graphite from supernovae. Geochimica et Cosmochimica Acta, 67 (24) 4705-4725 doi:10.1016/s0016-7037(03)00463-0 | Journal (article/letter/editorial) | | chemical, and isotopic microanalytical investigations of graphite from
supernovae
T. KEVIN CROAT,* THOMAS...SCOTT MESSENGER, and FRANK J. STADERMANN
Department of Physics and McDonnell Center for the Space Sciences...results of coordinated ion microprobe and transmission electron microscope (TEM)
studies of presolar...separate (1.65–1.72 g/cm3) of the Murchison CM2 meteorite.
Isotopic analysis of individual graphites (1–12...indicative of a supernova (SN) origin. Transmission
electron microscopy (TEM) of ultramicrotome slices of these | 👁 Image
| 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 | 👁 Image
| | 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 |
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