 | | Journal (article/letter/editorial) | | of petrographic thin sections of the Orgueil carbonaceous meteorite has led to the determination of the...has been confirmed in Orgueil. Gypsum has been tentatively identified in Orgueil; this is in agreement...Anders, 1962). A phosphate mineral, possibly merrillite, NarCaa(PO+)zO,which is known to occur in some...and Larsen, 1925),has also been identified in Orgueil. The electron probe microanalyzer, first developed...approximately two micra for r-ray data (Davidson et ol., 1962). Quantitative measurementscan be made |  | | Journal (article/letter/editorial) | | rights reserved. Keywords: IāXe chronometer; Meteorite evolution; Cooling rates 1. Introduction The...17 Ma) was ļ¬rst reported in the Richardton H4 meteorite by Reynolds (1960a). Radiogenic 129Xe in Richardton...iodine within the solar nebula (Crabb et al., 1982; Jordan et al., 1980) to interpretations of the observed...āādeadāā 129I in extrasolar grains (Clayton, 1975; Crabb et al., 1982), thus of no chronological signiļ¬cance...among the earliest solar system condensates (Amelin et al., 2002). Thus, reported IāXe ages began to fall |  | | Journal (article/letter/editorial) | | microscopist, Gustav Tschermak, and the outstanding meteorite collection of that day, the Vienna collection...meteorites. Table 1 traces the development of meteorite mineralogy over the following seventy years. It...extracted sulfur with alcohol from the Cold Bokkeveld meteorite, and later investigators extracted it from other...Magnetite Chromite Quartz Tridymite Chlorapatite Merrillite (Whitlockite) Olivine Orthopyroxene Clinopyroxene...weathering. In 1955, therefore, to specializein meteorite mineralogy might well have beenconsideredthe refugeol |  | | Journal (article/letter/editorial) | | identification has elucidated many aspects of meteorite formation. Of particular interest are five phosphate...calcium- and aluminum-rich silicates in the Allende meteorite, a Type 1II carbonaceous chondrite which fell...(Mason, 1962), when I wrote an account of the meteorite minerals then recognized, see Table 1, the list...12. 13. 14. Kullerud and El Goresy (1969) Clarke et al. (1971) Frondel and Marvin (1967) Vdovykin (1969)...(1971) Marvin et al. (1970) Keil and Fuchs (1971) Fuchs et al. (1970) Fuchs (1969a) Binns et at. (1969) |  | | Journal (article/letter/editorial) | | Aqueous, low temperature environment of the Orgueil meteorite parent body' Ann. N. Y. Acad. Sci. 108' 534552...534552 PrsaNr, F. (1864) Etude chimique et analyse de l'aerolithe d'Orgueil. Compt. tend,. 59, 132-135...132-135. SnaNNoN,E. V. eNn E. S. Lansrr (1925) Merrillite and chlorapatite from stony meteorites. Am. J our...(Heinrich et al., 1962). Such variation in color is due in part to included hematite (Heinrich et al., 1962)...most abundant ianthanides is also given (Heinrich et al., 1962). As the distribution of yttrium and the |  | | Book | | obtain a panorama of the scope and substance of meteorite research. I endeavored to remedy this situation...not exhaustively discussedāthe great upsurge in meteorite research along many new lines in recent years...and conservation of meteoritic material. Every meteorite is to some degree unique; and meteorites, unlike...I not been favored bv the curatorship of the meteorite collection of The American Museum of Natural History...Chicago Natural History Museum, the Nininger Meteorite Collection (Arizona State University, Tempe), |  | Barrat, J.A., Zanda, B., Moynier, F., Bollinger, C., Liorzou, C., Bayon, G. (2012) Geochemistry of CI chondrites: Major and trace elements, and Cu and Zn Isotopes. Geochimica et Cosmochimica Acta, 83. 79-92 doi:10.1016/j.gca.2011.12.011 | Journal (article/letter/editorial) | | Available online at www.sciencedirect.com Geochimica et Cosmochimica Acta 83 (2012) 79ā92 www.elsevier.com/locate/gca...Bayon e a UniversiteĢ EuropeĢenne de Bretagne, France CNRS UMR 6538 (Domaines OceĢaniques), U.B.O.-I...Copernic, 29280 PlouzaneĢ Cedex, France c Laboratoire de MineĢralogie et de Cosmochimie du MuseĢum, CNRS...dāHistoire Naturelle, CP52, 57 rue Cuvier, 75005 Paris, France d Department of Earth and Planetary Sciences, McDonnell...GeĢosciences Marines, IFREMER, 29280 PlouzaneĢ, France b Received 11 July 2011; accepted in revised form |  | | Journal (volume) | | further supports the contention (Cooper, in Cooper et al., ; 1942, p. 1784) that the earliest occurrence...abounding in stromatopores on the west side of the France Stone way Company Quarry, on the north side...these important fossils were not seen. In the France Stone Quarry the String ocephalus-btdsmg gray limestone...River slightly less than a mile southwest of the France Stone Quarry, Logansport- Anoka (7^') Quadrangles...relationships, however, Company Quarry. We, is France therefore, select the west side of the quarry |  | CAPORALI, Stefano, MOGGI-CECCHI, Vanni, MUNIZ-MIRANDA, Maurizio, PAGLIAI, Marco, PRATESI, Giovanni, SCHETTINO, Vincenzo (2012) SERS investigation of possible extraterrestrial life traces: Experimental adsorption of adenine on a Martian meteorite. Meteoritics & Planetary Science, 47 (5) 853-860 doi:10.1111/j.1945-5100.2012.01361.x | Journal (article/letter/editorial) | | Experimental adsorption of adenine on a Martian meteorite Stefano CAPORALI1,2*, Vanni MOGGI-CECCHI1, Maurizio...(SERS) on different mineral phases of a Martian meteorite Dar al Gani (DaG) 670 has been adopted as a test...materials. Raman spectra of different phases of meteorite (olivine, pyroxene, and ilmenite), representative...the Martian meteorite cannot be observed in the normal Raman spectra; when, instead, meteorite is treated...subpicogram level. (El Amri et al. 2005; Busemann et al. 2007; Steele et al. 2007) and for the investigation |  | Carrillo-SĆ”nchez, Juan Diego, Bones, David L., Douglas, Kevin M., Flynn, George J., Wirick, Sue, Fegley, Bruce, Araki, Tohru, Kaulich, Burkhard, Plane, John M.C. (2020) Injection of meteoric phosphorus into planetary atmospheres. Planetary and Space Science, 187. 104926pp. doi:10.1016/j.pss.2020.104926 | Journal (article/letter/editorial) | | dust particles (IDPs) making up the other 99% (Plane et al., 2017). An alternative route to reduced forms...org/licenses/by/4.0/). J.D. Carrillo-S anchez et al. Planetary and Space Science 187 (2020) 104926...atmospheres via meteoric ablation of IDPs (Douglas et al., 2019). These vaporized P atoms will undergo...Meteor ablation Simulator (MASI) (Bones et al., 2016; G omez-MartĆn et al., 2017), an experimental setup that...different thermodynamic models of P and its oxides (Suito et al., 1981; Ban-Ya, 1993; Turkdogan, 2000; Jung and |  | | Journal (article/letter/editorial) | | (CV-3), Tagish Lake (C2-ungrouped), Alais (CI1), Orgueil (CI1) and Ivuna (CI1) meteorites were measured...observed in Orgueil. Based on eight high-precision multi-collection ICP-MS measurements of Orgueil (n= 5)...meteoritic and geological materials (Balaram, 1996; Eggins et al., 1997; Pin and Joannon, ā Corresponding author... 1997; Jarvis, 1988; Robinson et al., 1999; Yu et al., 2001; Bayon et al., 2009). While most ICP techniques...recently explored for REE measurements (Baker et al., 2002; Kent et al., 2004). The ability to simultaneously |  | | Book | | Professor of Chemistry and Geology Director, Nininger Meteorite Collection Arizona State University JOHN WILEY...Chemistry and Geology, Director of: the Nininger Meteorite Collection, Arizona State University, Tempe, Arizona...announced the transfer of the outstanding Nininger Meteorite Collection to Arizona State University. Throughethe...the National Science Foundation, the Nininger Meteorite Collection was established primarily for purposes...(minerals The of meteorites) relationship of and meteorite Moore (achondrites), studies to the Earth |  | | Book | | composition of stone meteorites. How to recognize a meteorite. Brazilian stone meteorites. 7.1. ACHONDRITES...chondrite . Parambu. Acknowledgments . References.^.. Meteorite index. Page 1 3 11 29 35 45 47 48 48 48 61 61...during the agglomeration of the meteorite parent bodies. When a meteorite is seen to fall and material is...is collected, the meteorite is referred to as a fall. On the other hand, a meteorite find is the by-chance...meteorites Figure 1 - The Bendego, Bahia, Brazil iron meteorite, weighing approximately 5,360 kg. Note the irregular |  | | Report (issue) | | Structural and compositional properties of iron meteorite groups ___________ The geochemical behavior of...ABBREVIATIONS The following abbreviations for the meteorite classes are used throughout the tables and elsewhere;...percent) ; all others (<0.01 percent). A list of meteorite minerals is provided, and a tabulation of elemental...minerals are quartz and aluminosilicates; the common meteorite minerals are anhydrous, whereas hydrated minerals...actual extraterrestrial abundances; irons dominate meteorite finds since they are resistant to weathering and |  | | Journal (article/letter/editorial) | | asteroids (Burbine et al., 2002) as well as from the Moon and Mars (e.g., Shearer et al., 1998) and possibly...possibly from comets (Gounelle et al., 2006; Gounelle et al., 2008). Micrometeorites are derived mostly...mostly from asteroids (Kurat et al., 1994; Genge et al., 1997); a minority are from comets (Engrand and Maurette...Maurette, 1998; Nakamura et al., 2005; Dartois et al., 2013). Because interplanetary dust particles (IDPs)...material to Earth may be several thousand (Taylor et al., 2016), including an unknown number of comets |  | Feng, Tian, Gull, Maheen, Omran, Arthur, Abbott-Lyon, Heather, Pasek, Matthew A. (2021) Evolution of Ephemeral Phosphate Minerals on Planetary Environments. ACS Earth and Space Chemistry, 5 (7) 1647-1656 doi:10.1021/acsearthspacechem.1c00007 | Journal (article/letter/editorial) | | apatite group Ca5(PO4)3(OH, F, Cl,) and the mineral merrillite Ca9(Mg, Fe)(Na, H)(PO4)7.15ā19 This occurs via...which would presumably be present in a typical meteorite, or on the early Earth as a constituent of basalt...dominated by these calcium phosphates including merrillite and the apatite mineral group,21 and other phosphate...phosphide mineral oxidation in iron meteorites.22 Hazen et al.23 introduced the concept of mineral evolution...was synthesized by the method described by Frost et al.56 In each reaction, the mineral was separated |  | Jenniskens, Peter, Rubin, Alan E., Yin, Qing-Zhu, Sears, Derek W. G., Sandford, Scott A., Zolensky, Michael E., Krot, Alexander N., Blair, Leigh, Kane, Darci, Utas, Jason, Verish, Robert, Friedrich, Jon M., Wimpenny, Josh, Eppich, Gary R., Ziegler, Karen, Verosub, Kenneth L., Rowland, Douglas J., Albers, Jim, Gural, Peter S., Grigsby, Bryant, Fries, Marc D., Matson, Robert, Johnston, Malcolm, Silber, Elizabeth, Brown, Peter, Yamakawa, Akane, Sanborn, Matthew E., Laubenstein, Matthias, Welten, Kees C., Nishiizumi, Kunihiko, Meier, Matthias M. M., Busemann, Henner, Clay, Patricia, Caffee, Marc W., Schmitt-Kopplin, Phillipe, Hertkorn, Norbert, Glavin, Daniel P., Callahan, Michael P., Dworkin, Jason P., Wu, Qinghao, Zare, Richard N., Grady, Monica, Verchovsky, Sasha, Emel'Yanenko, Vacheslav, Naroenkov, Sergey, Clark, David L., Girten, Beverly, Worden, Peter S., , (2014) Fall, recovery, and characterization of the Novato L6 chondrite breccia. Meteoritics & Planetary Science, 49 (8) 1388-1425 doi:10.1111/maps.12323 | Journal (article/letter/editorial) | | Beverly GIRTEN2, and Peter S. WORDEN2 (The Novato Meteorite Consortium) 1 SETI Institute, Carl Sagan Center...UCLA, Los Angeles, California 90095ā1567, USA 10 Meteorite Recovery Laboratory, P.O. Box 463084, Escondido...recovered in the town of Novato (Fig. 1). The meteorite is an L6 ordinary chondrite fragmental breccia...the meteor showers throughout the year (Jenniskens et al. 2011). The calculated downward projected path...reacted strongly to a permanent magnet. This Novato meteorite was difficult to distinguish from weathered terrestrial |  | | Journal (article/letter/editorial) | | Louis Birck, Lab Geochimie et Cosmochimie, University ofParis 6' 7, France We reviewed all of the 87Rb_86Sr...supported by NSF grant EAR 76-01146. THE SHAW METEORITE: EVIDENCE FOR AN IGNEOUS ORIGIN J.L. Berkley...Johnson Space Center, Houston, TX 77058 The Shaw meteorite has Lgroup chondritic bulk chemistry and mineralogy...recrystallization (Dodd et al., 1975), having experienced temperatures of up to 1300Ā° C (Onuma et al., 1972); alternatively...recrystallization, support an igneous origin for the Shaw meteorite. Data are presently insufficient to determine |  | | Journal (article/letter/editorial) | | FRG 259 THE ALKHAMAslN, SAUDI ARABIA, IRON METEORITE A.A. Almohandl., King Saud University, Riyadh...possible on the material available suggest that the meteorite belongs to chemical group lIB. No evidence of...an unrepresentative sample. THE ALLAN HILLS METEORITE ICEFIELD - AN ALTERNATE VIEW J.O. Annex.tad, NASA/Johnson...Icefield(about 100krrr')has exceptionallyhigh meteorite concentrations while other icefields to the West...OF SILICATES AND METAL PHASES OF THE BOCAIUVA METEORITE S.I. Araujo, J. Danon, R.B. Scorzelll and I.S |  | | Journal (article/letter/editorial) | | CNRS Aix-Marseille University, Aix en Provence, France. mail : aboulahris@cerege.fr . 3UniversitĆ© de Tunis...Science Tunis, Tunisia, 4 Meteorite Laboratory Lehmweg Gifhorn, Germany, 5 Meteorite Recon MĆ¼hlendamm Hamburg...calculation of meteorite flux is possible [4]. Following previous estimation of meteorite flux based on...DCAs [8]. References: [1] Chennaoui Aoudjehane H. et al. 2013, 76th Meteoritical Society meeting, abstract...and H. Y. McSween Jr., eds.), 889-905. [4] Zolensky et al. 2006. Meteorites and the Early Solar System II |  | | Journal (article/letter/editorial) | | References: [1] Fujiwara A. et al. 2006. Science 312:1330ā 1334. [2] Abe M. et al. 2011. Abstract #1638...Fujimura A. et al., 2011. Abstract #1829. 42nd Lunar & Planetary Science Conference. [4] Nakamura T. et al. 2011...2011. Science 333: 1113-1116. [5] Ishibashi Y. et al. 2012. Abstract #2887. 43rd Lunar & Planetary Science...was incorporated. References: [1] Mittlefehldt D.W. et al. 1998. In: Planetary Materials, Min. Soc. America...M.M. 1990. GCA 54:32093218; [3] Mittlefehldt D.W. et al. 2002. MAPS 37:345-369; [4] Grady & Wright. 2003 |  | | Book | | Water-Rich Small Bodies 390 6.5 Primitive Asteroid-Meteorite Matches 394 6.6 Implications for Exploration of...Paris, CNRS, Universite Pierre et Marie Curie, Universite Paris Diderot, France Neyda M. Abreu The Pennsylvania...Paris, CNRS, Universite Pierre et Marie Curie, Universite Paris Diderot, France Christine M. Hartzell University...Pierre Beck Institut Universitaire de France, Grenoble, France Edward B. Bierhaus CO, United States ...Paris, CNRS, Universite Pierre et Marie Curie, Universite Paris Diderot, France; 3Planetary Science Institute |  | | Journal (article/letter/editorial) | | Weisberg M. K. et al. (1993) Geochimica et Cosmochimica Acta 57: 1567-1586 [2] Schrader D. L. et al. (2011)...(2011) Geochimica et Cosmochimica Acta 75: 308ā325 [3] Irving A. J. et al. (2014) LPS XLV, Abstract #2465...Sanborn M. E. et al. (2019) Geochimica et Cosmochimica Acta 245: 577ā596. [5] Gardner-Vandy K. G. et al. (2012)...(2012) Geochimica et Cosmochimica Acta 85: 142ā159. [6] Breton T.et al. (2015) Earth and Planetary Science...Science Letters 425: 193-203. [7] Nehru C. E. et al. (2014) Annual Meeting of 77th Meteoritical Society |  | | Journal (article/letter/editorial) | | Evidence for High-Pressure Transformation of Merrillite and NaBearing Phosphates A. V. Arefiev, K. D...Superimposed Processes in Chondrules of the Ochansk Meteorite A. I. Bakhtin, R. Kh. Sungatullin, A. V. Gusev...6199 A Multi-Technique Analysis of the Paris Meteorite to Characterize its Organic Content āIn Situā............................. 6230 Influence of Meteorite Structure on Nanotubes and Nanocrystals Synthesis...Particles in the Light Lithology of Chelyabinsk Meteorite E. V. Brusnitsyna, V. I. Grokhovsky, G. A. Yakovlev |  | | Journal (article/letter/editorial) | | family comet, Solar System origin, Kuiper belt, meteorite, interplanetary dust, IDP, olivine, chondrule...(McKeegan et al. 2011), and the asteroid samples collected by the Hayabusa mission (Nakamura et al. 2011)...remarkable to ļ¬nd that a comet contains abundant meteorite-like materials that are clearly similar and likely...likely identical to those that formed meteorite parent bodies an order of magnitude closer to the Sun...does not appear to match that of any speciļ¬c meteorite type. The apparent long-distance transport of |
|
