Prehistoric Hopewell Meteorite Collecting : Context and Implicatiosn
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(Sptpang Coil.) [I49] I50 Bulletin American Museum of Natural History
Article VIII.-CATALOGUE OF METEORITES IN THE COLLECTION OF THE AMERICAN MUSEUM OF NATURAL HISTORY, TO JULY i, I896. By E. 0. HOVEY. 'T'he Collection of Meteorites in the Arnerican Museum of Natural History consists of fifty-five slabs, fragments and com- plete individuals, representing twenty-six falls and finds. The foundation of the mineralogical department of the Museum was laid in I874 by the purchase of the collection of S. C. H. Bailey, in which there were a few meteorites. More were acquired with the portion of the Norman Spang Collection of Minerals which was purchased in I89I, and other meteorites have been bought by the Museum from time to time, or have been presented to it by friends. The soujrce from which each specimen came has been indicated in the following cataloguLe. This publication is made to assist. the large number of persons who have become interested in knowing the extent to which the material of various falls and finds has been distributed among collections and the present location of specimens. AEROSIDERITES. (IRON METEORI ES.) Cat. Date of NAME AND Weight No. Discovery. DE;SCRIPTION. in grams. 18 1784 Tejupilco, Toluca Valley, Mexico. A complete individual, the surface of which has scaled off somewhat. A polished and etched surface shows coarse Widmanstatten figures. 1153. (Bailey Co/i.) 17841 Xiquipilco, Toluca Valley, Mexico. A complete individual of ellipsoidal form, which had been used as a pounder by the natives. 564. (Sptpang Coil.) [I49] I50 Bulletin American Museum of Natural History. [Vol. VIII, AEROSIDERITES.-Continued. Cat. Date of NAME AND DESCRIPTION. -
Iron Meteorites Are Made of Fe-Ni Metal Phases with Such Minor Minerals As Schrebersite, Troilite, Cohenite and Other Fe-Ni Carbides
Bulk elemental analyses of iron meteorites by using INAA and LA-ICPMS. N. Shirai1, A. Yamaguchi2, M. K. Haba2, T. Ojima2, M. Ebiahra1 and H. Kojima2, 1Tokyo Metropolitan Univer- sity, 2National Institute of Polar Research. Introduction: Iron meteorites are made of Fe-Ni metal phases with such minor minerals as schrebersite, troilite, cohenite and other Fe-Ni carbides. As most iron meteorites are believed to be samples from the metallic core of differentiated planetesimals, petrological, mineralogical and chemi- cal studies of iron meteorites are fundamental for unraveling the process of planetary differentiation. Based on the structures, iron meteorites are originally classified into hexahedrites, octahedrites and ataxites. Hexahedrites and ataxites are nearly made of kamacite and taenite, respectively. Octahedrites consist of kamacite and taenite, and they are further divided into six subgroups on the basis of the width of the kamcite from finest (>0.2 mm) to coarsest (>3.3 mm). Almost all iron meteorites are classified into octahedrites. The chemical clas- sification of iron meteorites is based on their trace element compositions (Ni, Ga, Ge and Ir). Bulk elemental abundances for iron meteorites have been obtained by using neutron activation analysis (NAA). Other analytical methods such as laser ablation inductively coupled plasma mass spectrometry (LA-ICPMS) have not been very often applied to iron meteorites. In this study, we present simple and effective procedures for the chemical classification of iron meteorites by using INAA and LA-ICPMS. Based on the analytical data obtained by two analytical techniques, we discuss the accuracy and the precision of our data and how promisingly our analytical methods can be applied to classifica- tion of iron meteorites.r 9, 2016 (12:00 pm, JST) Experimental: Canyon Diablo (IAB), Toluca (IAB), Cape York (IIIAB), Muonionalusta (IVA) and Dronino (ungrouped) were analyzed by using two analytical methods (INAA and LA-ICPMS). -
Problems of Planetology, Cosmochemistry and Meteoritica Alexeev V.A., Ustinova G.K
Problems of Planetology… Problems of Planetology, Cosmochemistry and Meteoritica Alexeev V.A., Ustinova G.K. Meteoritic evidence radionuclides before the meteorite fall onto the Earth. The investigation of radionuclides with different T1/2 in the on peculiarities of the contemporary solar cycles chondrites with various dates of fall, which have various V.I. Vernadsky Institute of Geochemistry and Analytical Chemistry extension and inclination of orbits, provides us with such RAS, Moscow long sequences of homogeneous data on variation of the Abstract. The meteorite data on monitoring of the intensity and GCR intensity and integral gradients (E >100 MeV) in the gradient of the galactic cosmic rays (GCR) in the heliosphere 3D heliosphere [Lavrukhina,Ustinova,1990]. The long during 5 solar cycles are used for the correlative analysis with the sequences of homogeneous data on the GCR intensity in variations of the solar activity (SA), strength of the interplanetary magnetic field (IMF) and tilt angle of the heliospheric current the stratosphere [Stozhkov et al., 2009] are used for sheet (HCS). The dependence of the GCR modulation depth in the evaluation of the gradients. Nowadays, such a sequence of 11-year solar cycles on the character of the solar magnetic field certain homogeneous data on the GCR intensity and (SMF) inversions in the heliosphere at the change of the 22-year gradients in the inner heliosphere covers ~5 solar cycles magnetic cycles is revealed. (see figure 1) [Alexeev, Ustinova, 2006]. This smoothes, Key words: galactic cosmic rays, solar modulation, solar cycles, to a considerable extent, both the temporal and spatial inversion of magnetic field, solar dynamo, climate. -
Lost Lake by Robert Verish
Meteorite-Times Magazine Contents by Editor Like Sign Up to see what your friends like. Featured Monthly Articles Accretion Desk by Martin Horejsi Jim’s Fragments by Jim Tobin Meteorite Market Trends by Michael Blood Bob’s Findings by Robert Verish IMCA Insights by The IMCA Team Micro Visions by John Kashuba Galactic Lore by Mike Gilmer Meteorite Calendar by Anne Black Meteorite of the Month by Michael Johnson Tektite of the Month by Editor Terms Of Use Materials contained in and linked to from this website do not necessarily reflect the views or opinions of The Meteorite Exchange, Inc., nor those of any person connected therewith. In no event shall The Meteorite Exchange, Inc. be responsible for, nor liable for, exposure to any such material in any form by any person or persons, whether written, graphic, audio or otherwise, presented on this or by any other website, web page or other cyber location linked to from this website. The Meteorite Exchange, Inc. does not endorse, edit nor hold any copyright interest in any material found on any website, web page or other cyber location linked to from this website. The Meteorite Exchange, Inc. shall not be held liable for any misinformation by any author, dealer and or seller. In no event will The Meteorite Exchange, Inc. be liable for any damages, including any loss of profits, lost savings, or any other commercial damage, including but not limited to special, consequential, or other damages arising out of this service. © Copyright 2002–2010 The Meteorite Exchange, Inc. All rights reserved. No reproduction of copyrighted material is allowed by any means without prior written permission of the copyright owner. -
The Mineralogical Magazine Journal
THE MINERALOGICAL MAGAZINE AND JOURNAL OF THE MINERALOGICAL SOCIETY. 1~o. 40. OCTOBER 1889. Vol. VIII. On the Meteorites which have been found iu the Desert of Atacama and its neighbourhood. By L. FLETCHER, M.A., F.R.S., Keeper of Minerals in the British Museum. (With a Map of the District, Plate X.) [Read March 12th and May 7th, ]889.J 1. THE immediate object of the present paper is to place on record J- the history and characters of several Atacama meteorites of which no description has yet been published; but incidentally it is con- venient at the same time to consider the relationship of these masses to others from the same region, which either have been already described, or at least are stated to be preserved in one or more of the known Meteo. rite-Collections. 2. The term " Desert of Atacama " is generally applied to that part of western South America which lies between the towns of Copiapo and Cobija, about 330 miles distant from each other, and which extends island as far as the Indian hamlet of Antofagasta, about 180 miles from 224 L. FLETCHER ON THE METEORITES OF ATACAMA. the coast. The Atacama meteorites preserved in the Collections have been found at several places widely separated throughout the Desert. 3. A critical examination of the descriptive literature, and a compari- son of the manuscript and printed meteorite-lists, which have been placed at my service, lead to the conclusion that all the meteoritic frag- ments from Atacama now preserved in the known Collections belong to one or other of at most thirteen meteorites, which, for reasons given below, are referred to in this paper under the following names :-- 1. -
Orbital Debris: a Chronology
NASA/TP-1999-208856 January 1999 Orbital Debris: A Chronology David S. F. Portree Houston, Texas Joseph P. Loftus, Jr Lwldon B. Johnson Space Center Houston, Texas David S. F. Portree is a freelance writer working in Houston_ Texas Contents List of Figures ................................................................................................................ iv Preface ........................................................................................................................... v Acknowledgments ......................................................................................................... vii Acronyms and Abbreviations ........................................................................................ ix The Chronology ............................................................................................................. 1 1961 ......................................................................................................................... 4 1962 ......................................................................................................................... 5 963 ......................................................................................................................... 5 964 ......................................................................................................................... 6 965 ......................................................................................................................... 6 966 ........................................................................................................................ -
Handbook of Iron Meteorites, Volume 2 (Bitburg
326 Bishop Canyon - Bitburg fibrous and brecciated, and 1-100 p wide veins through it ' l ' j are filled with a glass in which silicate fragments and a little ) ·. / troilite are embedded.lt is surprising to note how the shock . e·· f . has been able to create such heavy local transformation; 10 mm away nothing unusual is observed. The local damage resembles in several respects the structural changes associated with spot welding. Examination under the electron microprobe suggests that the unknown silicate is ~' almost pure Si02 , possibly tridymite. Bishop Canyon is chemically and structurally a typical ~ phosphorus-poor, fine octahedrite of groupiVA, . l .. resembling in particular Gibe on. It is, however, unusual in .0 its silicate inclusions, the shock damage and low hardness. ,, .• ~: :t • ·. • cr ··. @ Specimen in the U.S. National Museum in Washington: .. ~ - ,·r -. f '-' f 226 g slice (no. 770, 9.5 x 4.5 x 0.9 em) II . 0 t' / •. ' ~~ ~~ {) r ...~ · -· · ...· ~· -/~... Figure 352. Bitburg. Detail of Figure 350. The dendritic metal was Bitburg, Rhineland, Germany at high temperature austenite but transformed upon cooling to unequilibrated a • Etched. Scale bar 50 f.l. 49°58'N, 6°32'E 2 A mass said to have weighed 1.5 tons was smelted in a furnace before 1805. It was recognized as a meteorite (Chladni 1819: 353), but virtually nothing was saved of the undamaged material (Hey 1966: 57). The smelted material, e.g., no. 1881, 1534 of 546 gin .. \ . • I : '/ 'I \ ' . ~\.. // .·· Figure 350. Bit burg (Copenhagen no. 1886, 493). A rectangular bar cut from melted material of the Bitburg meteorite. -
CHAPTER 1 Introduction
Chemical analysis of organic molecules in carbonaceous meteorites Torrao Pinto Martins, Zita Carla Citation Torrao Pinto Martins, Z. C. (2007, January 24). Chemical analysis of organic molecules in carbonaceous meteorites. Retrieved from https://hdl.handle.net/1887/9450 Version: Corrected Publisher’s Version Licence agreement concerning inclusion of doctoral License: thesis in the Institutional Repository of the University of Leiden Downloaded from: https://hdl.handle.net/1887/9450 Note: To cite this publication please use the final published version (if applicable). ______________________________________________________ CHAPTER 1 ______________________________________________________ Introduction 1.1 Heavenly stones-from myth to science Ancient chronicles, from the Egyptian, Chinese, Greek, Roman and Sumerian civilizations documented the fall1 of meteorites, with Sumerian texts from around the end of the third millennium B. C. describing possibly one of the earliest words for meteoritic iron (Fig. 1.1 Left). Egyptian hieroglyphs meaning “heavenly iron” (Fig. 1.1 Right) found in pyramids together with the use of meteoritic iron in jewellery and artefacts show the importance of meteorites in early Egypt. Meteorites were worshiped by ancient Greeks and Romans, who struck coins to celebrate their fall, with the cult to worship meteorites prevailing for many centuries. For example, some American Indian tribes paid tribute to large iron meteorites, and even in modern days the Black Stone of the Ka´bah in Mecca is worshiped and regarded by Muslims as “an object from heaven”. The oldest preserved meteorite that was observed to fall (19th May 861) was found recently (October 1979) in a Shinto temple in Nogata, Japan. It weighted 472 g and it was stored in a wooden box. -
Pallasites: Olivine-Metal Textures, Phosphoran Olivine, and Origin
Pallasites: olivine-metal textures, phosphoranolivine, and origin Ed Scott University of Hawai’i, Honolulu, HI 96822. [email protected] Four questions: 3. Origin of the four FeO-rich MG pallasites 1. Why do some pallasites have rounded olivines? 2. Why is phosphoran olivine only found in five main-group pallasites? 3. Why do four main group pallasites with rounded olivines contain abnormally Fe-rich olivine? 4. Where did main group and Eagle Station group pallasites form? a 1. Origin of rounded olivine Did cm-sized rounded olivines form before angular olivines [9], or were olivines rounded after Fig. 5. Zaisho, Springwater, Rawlinna, and Phillips Co. fragmentation of olivine [2.3,7]? Constraints: contain anomalously Fe-rich olivine, Ni-rich metal, and • Uniform size distribution of rounded olivines in farringtonite Mg3(PO4)2 [20] suggesting Fe was oxidized. Fig.1c is unlike that of angular olivine pallasites Fig. 3. Ir vs. Ni showing metal in main group pallasites and IIIAB irons. Arrows show Data from [2]. which may contain dunite fragments several cm solid and liquid Fe-Ni paths during fractional crystallization. MG pallasites were b in width (Fig. 1a.). mostly formed by mixing of residual metallic liquid from a IIIAB-like core after 75- Springwater contains 4 • Angular olivine pallasites may contain pieces of 80% crystallization [1,2]. Pavlodar (Pa) has rounded olivines and plots near the vol.% farringtonite (center) rounded olivine texture (Fig. 1b). initial melt composition showing that rounding preceded metal crystallization. enclosing olivine. Slice ~12 • Pavlodar metal matches that expected for initial Marjalahti (Ma), Huckitta (Hu) and Seymchan (Se) have angular olivines and cm wide. -
The Tawallah Valley Meteorite. General Description. the Microstructure.Records of the Australian Museum 21(1): 1–8, Plates I–Ii
AUSTRALIAN MUSEUM SCIENTIFIC PUBLICATIONS Hodge-Smith, T., and A. B. Edwards, 1941. The Tawallah Valley meteorite. General description. The Microstructure.Records of the Australian Museum 21(1): 1–8, plates i–ii. [4 July 1941]. doi:10.3853/j.0067-1975.21.1941.518 ISSN 0067-1975 Published by the Australian Museum, Sydney nature culture discover Australian Museum science is freely accessible online at http://publications.australianmuseum.net.au 6 College Street, Sydney NSW 2010, Australia THE TAW ALLAH VALLEY METEORITE. General Description. By T. HODGE-SMI'l'H, The Australian Museum. The Microstructure. By A. B. EDWARDS, Ph.D., D.I.C.,* Research Officer, Mineragraphy Branch, Council for Scientific and Industrial Research. (Plates i-ii and Figures 1-2.) General Description. Little information is available about the finding of this meteorite. Mr. Heathcock, Constable-in-Charge of the Borroloola Police Station, Northern Territory, informed me in April, 1939, that it had been in the Police Station for eighteen months or more. It was found by Mr. Condon, presumably some time in 1937. The weight of the iron as received was 75·75 kg. (167 lb.). A small piece had been cut off, but its weight probably did not exceed 200 grammes. The main mass weighing 39·35 kg. (86i lb.) is in the collection of the Geological Survey, Department of the Interior, Canberra. A portion weighing 30·16 kg. (66~ lb.) and five pieces together weighing 1·67 kg. are in the collection of the Australian Museum, and a slice weighing 453 grammes is in the Museum of the Geology Department, the University of Melbourne. -
The Function of a Middle Woodland Site in the Central Illinois Valley: a Ceramic Study of Ogden-Fettie
Illinois State University ISU ReD: Research and eData Theses and Dissertations 11-1-2013 The Function of a Middle Woodland Site in the Central Illinois Valley: A Ceramic Study of Ogden-Fettie Montana L. Martin Illinois State University, [email protected] Follow this and additional works at: https://ir.library.illinoisstate.edu/etd Part of the History of Art, Architecture, and Archaeology Commons Recommended Citation Martin, Montana L., "The Function of a Middle Woodland Site in the Central Illinois Valley: A Ceramic Study of Ogden-Fettie" (2013). Theses and Dissertations. 60. https://ir.library.illinoisstate.edu/etd/60 This Thesis is brought to you for free and open access by ISU ReD: Research and eData. It has been accepted for inclusion in Theses and Dissertations by an authorized administrator of ISU ReD: Research and eData. For more information, please contact [email protected]. THE FUNCTION OF A MIDDLE WOODLAND SITE IN THE CENTRAL ILLINOIS VALLEY: A CERAMIC STUDY OF OGDEN-FETTIE Fv196 Montana L. Martin 147 pages December 2013 Ogden-Fettie is a Middle Woodland Havana-Hopewell mound group in the Central Illinois Valley. Fv196 is the midden area near the largest mound. The function of Fv196 is in question, because it does not conform to the settlement and function models that have been applied to other sites. The ceramic collection from Fv196 was typed and categorized into categories based on perceived function, either habitation or ceremonial. The majority of the pottery belonged to the Havana series, which is traditionally considered habitation pottery; however, many of the Havana sherds are decorated indicating a ceremonial function. -
The Hopewell Mound Group of Ohio
" -.] + ** Mv U V • THE UNIVERSITY OF ILLINOIS OKSTACKS CENTRAL C is re- The person terial ibrary from sponsible foi • before the which it wa Latest Date oks are reasons Thoft, mutilation from i dismissal for dUclpllnary the University. 8400 TO RENEW CALL tANA-CHAMPAIGN UNIVERSITY OF :9 2001 13 200Z 8 2006 due date below 79521 L162 Mfc library OF THE wmm of Illinois <*» nB*n , »it*a faun OF HOPEWELL WORKS, ROSS COUNTY, OHIO 1 Field Museum of Natural History Publication 2 1 Anthropological Series Volume VI, No. 5 THE HOPEWELL MOUND GROUP OF OHIO By Warren K. Moorehead Curator of Museum of American Archaeology Phillips Academy, Andover, Mass. 48 Plates and 68 Text-Figures Berthold Laufer Curator of Anthropology Chicago 192: FA CONTENTS Page List of Illustrations 76 Preface 79 I. Work in the Hopewell»Mound Group 82 Relation of the Hopewell Group to Other Mound Groups 82 Detailed Description of the Hopewell Group 82 Clark's Work; North Fork of Paint Creek 83 Our Survey and Measurements ; Comments on Changes since 1845 86 Exploration of Mound No. 1 88 Exploration of Mound No. 17 90 Excavation of Mound No. 18 92 Excavation of Mound No. 19 94 Excavation of Mound No. 20 94 Excavation of Mound No. 21 95 Excavation of Mound No. 2 95 Excavation of Mound No. 24 96 Excavation of Mound No. 23 97 Excavation of Mound No. 3 and No. 9 101 Mound No. 5 102 Excavation of Mound No. 8 102 Mound No. 11 103 Excavation of Mound No. 25 103 II.