Ice & Stone 2020
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Martin Horejsi Jim’S Fragments by Jim Tobin Bob’S Findings by Robert Verish Micro Visions by John Kashuba Mitch’S Universe by Mitch Noda
Meteorite Times Magazine Contents Paul Harris Featured Articles Accretion Desk by Martin Horejsi Jim’s Fragments by Jim Tobin Bob’s Findings by Robert Verish Micro Visions by John Kashuba Mitch’s Universe by Mitch Noda 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 2002–2021 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. Meteorite Times Magazine Ogi Japan: Meteorite Worship Then and Now Martin Horejsi Way back in 2003, in this very meteorite forum, I wrote: If only all meteorites could be as rich in tradition as the Ogi meteorite. -
Curt Teich Postcard Archives Towns and Cities
Curt Teich Postcard Archives Towns and Cities Alaska Aialik Bay Alaska Highway Alcan Highway Anchorage Arctic Auk Lake Cape Prince of Wales Castle Rock Chilkoot Pass Columbia Glacier Cook Inlet Copper River Cordova Curry Dawson Denali Denali National Park Eagle Fairbanks Five Finger Rapids Gastineau Channel Glacier Bay Glenn Highway Haines Harding Gateway Homer Hoonah Hurricane Gulch Inland Passage Inside Passage Isabel Pass Juneau Katmai National Monument Kenai Kenai Lake Kenai Peninsula Kenai River Kechikan Ketchikan Creek Kodiak Kodiak Island Kotzebue Lake Atlin Lake Bennett Latouche Lynn Canal Matanuska Valley McKinley Park Mendenhall Glacier Miles Canyon Montgomery Mount Blackburn Mount Dewey Mount McKinley Mount McKinley Park Mount O’Neal Mount Sanford Muir Glacier Nome North Slope Noyes Island Nushagak Opelika Palmer Petersburg Pribilof Island Resurrection Bay Richardson Highway Rocy Point St. Michael Sawtooth Mountain Sentinal Island Seward Sitka Sitka National Park Skagway Southeastern Alaska Stikine Rier Sulzer Summit Swift Current Taku Glacier Taku Inlet Taku Lodge Tanana Tanana River Tok Tunnel Mountain Valdez White Pass Whitehorse Wrangell Wrangell Narrow Yukon Yukon River General Views—no specific location Alabama Albany Albertville Alexander City Andalusia Anniston Ashford Athens Attalla Auburn Batesville Bessemer Birmingham Blue Lake Blue Springs Boaz Bobler’s Creek Boyles Brewton Bridgeport Camden Camp Hill Camp Rucker Carbon Hill Castleberry Centerville Centre Chapman Chattahoochee Valley Cheaha State Park Choctaw County -
1950 Da, 205, 269 1979 Va, 230 1991 Ry16, 183 1992 Kd, 61 1992
Cambridge University Press 978-1-107-09684-4 — Asteroids Thomas H. Burbine Index More Information 356 Index 1950 DA, 205, 269 single scattering, 142, 143, 144, 145 1979 VA, 230 visual Bond, 7 1991 RY16, 183 visual geometric, 7, 27, 28, 163, 185, 189, 190, 1992 KD, 61 191, 192, 192, 253 1992 QB1, 233, 234 Alexandra, 59 1993 FW, 234 altitude, 49 1994 JR1, 239, 275 Alvarez, Luis, 258 1999 JU3, 61 Alvarez, Walter, 258 1999 RL95, 183 amino acid, 81 1999 RQ36, 61 ammonia, 223, 301 2000 DP107, 274, 304 amoeboid olivine aggregate, 83 2000 GD65, 205 Amor, 251 2001 QR322, 232 Amor group, 251 2003 EH1, 107 Anacostia, 179 2007 PA8, 207 Anand, Viswanathan, 62 2008 TC3, 264, 265 Angelina, 175 2010 JL88, 205 angrite, 87, 101, 110, 126, 168 2010 TK7, 231 Annefrank, 274, 275, 289 2011 QF99, 232 Antarctic Search for Meteorites (ANSMET), 71 2012 DA14, 108 Antarctica, 69–71 2012 VP113, 233, 244 aphelion, 30, 251 2013 TX68, 64 APL, 275, 292 2014 AA, 264, 265 Apohele group, 251 2014 RC, 205 Apollo, 179, 180, 251 Apollo group, 230, 251 absorption band, 135–6, 137–40, 145–50, Apollo mission, 129, 262, 299 163, 184 Apophis, 20, 269, 270 acapulcoite/ lodranite, 87, 90, 103, 110, 168, 285 Aquitania, 179 Achilles, 232 Arecibo Observatory, 206 achondrite, 84, 86, 116, 187 Aristarchus, 29 primitive, 84, 86, 103–4, 287 Asporina, 177 Adamcarolla, 62 asteroid chronology function, 262 Adeona family, 198 Asteroid Zoo, 54 Aeternitas, 177 Astraea, 53 Agnia family, 170, 198 Astronautica, 61 AKARI satellite, 192 Aten, 251 alabandite, 76, 101 Aten group, 251 Alauda family, 198 Atira, 251 albedo, 7, 21, 27, 185–6 Atira group, 251 Bond, 7, 8, 9, 28, 189 atmosphere, 1, 3, 8, 43, 66, 68, 265 geometric, 7 A- type, 163, 165, 167, 169, 170, 177–8, 192 356 © in this web service Cambridge University Press www.cambridge.org Cambridge University Press 978-1-107-09684-4 — Asteroids Thomas H. -
Aqueous Alteration on Main Belt Primitive Asteroids: Results from Visible Spectroscopy1
Aqueous alteration on main belt primitive asteroids: results from visible spectroscopy1 S. Fornasier1,2, C. Lantz1,2, M.A. Barucci1, M. Lazzarin3 1 LESIA, Observatoire de Paris, CNRS, UPMC Univ Paris 06, Univ. Paris Diderot, 5 Place J. Janssen, 92195 Meudon Pricipal Cedex, France 2 Univ. Paris Diderot, Sorbonne Paris Cit´e, 4 rue Elsa Morante, 75205 Paris Cedex 13 3 Department of Physics and Astronomy of the University of Padova, Via Marzolo 8 35131 Padova, Italy Submitted to Icarus: November 2013, accepted on 28 January 2014 e-mail: [email protected]; fax: +33145077144; phone: +33145077746 Manuscript pages: 38; Figures: 13 ; Tables: 5 Running head: Aqueous alteration on primitive asteroids Send correspondence to: Sonia Fornasier LESIA-Observatoire de Paris arXiv:1402.0175v1 [astro-ph.EP] 2 Feb 2014 Batiment 17 5, Place Jules Janssen 92195 Meudon Cedex France e-mail: [email protected] 1Based on observations carried out at the European Southern Observatory (ESO), La Silla, Chile, ESO proposals 062.S-0173 and 064.S-0205 (PI M. Lazzarin) Preprint submitted to Elsevier September 27, 2018 fax: +33145077144 phone: +33145077746 2 Aqueous alteration on main belt primitive asteroids: results from visible spectroscopy1 S. Fornasier1,2, C. Lantz1,2, M.A. Barucci1, M. Lazzarin3 Abstract This work focuses on the study of the aqueous alteration process which acted in the main belt and produced hydrated minerals on the altered asteroids. Hydrated minerals have been found mainly on Mars surface, on main belt primitive asteroids and possibly also on few TNOs. These materials have been produced by hydration of pristine anhydrous silicates during the aqueous alteration process, that, to be active, needed the presence of liquid water under low temperature conditions (below 320 K) to chemically alter the minerals. -
The Origin of Ancient Magnetic Activity on Small Planetary Bodies: a Nanopaleomagnetic Study
The Origin of Ancient Magnetic Activity on Small Planetary Bodies: A Nanopaleomagnetic Study James Francis Joseph Bryson Department of Earth Sciences University of Cambridge This dissertation is submitted for the degree of Doctor of Philosophy Selwyn College October 2014 To my family and teachers Declaration I hereby declare that except where specific reference is made to the work of others, the contents of this dissertation are original and have not been submitted in whole or in part for consideration for any other degree or qualification in this, or any other University. This dissertation is the result of my own work and includes nothing which is the outcome of work done in collaboration, except where specifically indicated in the text. This dissertation contains fewer than 225 pages of text, appendices, illustrations, captions and bibliography. James Francis Joseph Bryson October 2014 Acknowledgements First and foremost, I would like to acknowledge my supervisors, Richard Harrison and Simon Redfern. Without Richard’s hard work, dedication, supervision and direction this project would not have been possible, and I feel privileged to have worked with him. Simon should be thanked for his guidance, hours of entertainment and awful jokes. I would like to acknowledge all of my collaborators, in particular Nathan Church, Claire Nichols, Roberts Blukis, Julia Herrero-Albillos, Florian Kronast, Takeshi Kasama and Francis Nimmo. Each has played an invaluable role in acquiring and understanding the data in this thesis and I would not have reached this point without their expertise and help. Martin Walker must be thanked for his assistance and calming influence. I would like to also thank Ioan Lascu for proof-reading this thesis and general advice. -
Evolution of the Lunar Crust Recorded in the Meteoritic
EVOLUTION OF THE LUNAR CRUST RECORDED IN THE METEORITIC FELDSPATHIC REGOLITH BRECCIAS NORTHWEST AFRICA 10291 AND 11182: INSIGHTS INTO THE HETEROGENEITY AND PETROGENESIS OF CRUSTAL LITHOLOGIES USING PETROLOGY AND MINERAL CHEMISTRY By SHANNON BOYLE A thesis submitted to the School of Graduate Studies Rutgers, The State University of New Jersey In partial fulfillment of the requirements For the degree of Master of Science Graduate Program in Earth and Planetary Science Written under the direction of Doctor Juliane Gross And approved by _____________________________________ _____________________________________ _____________________________________ _____________________________________ New Brunswick, New Jersey October 2019 TITLE PAGE ABSTRACT OF THE THESIS Evolution of the lunar crust recorded in the meteoritic feldspathic regolith breccias Northwest Africa 10291 and 11182: Insights into the heterogeneity and petrogenesis of crustal lithologies using petrology and mineral chemistry by SHANNON BOYLE Thesis Director: Doctor Juliane Gross Abstract The geology of the Moon represents nearly a continuous geological record from its formation during the giant impact that resulted in the Earth-Moon system, to its state today. Therefore, it is a prime location for understanding one path of planetary evolution. Lunar meteorites are on average samples of rock and regolith from random areas on the lunar surface. As such, they represent our best available tools to study the crustal evolution of the Moon because they provide data on lunar petrology, geochemistry, and chronology, as well as data on the variety of existing lunar lithologies different from Apollo and Luna mission sample return sites. We investigated two lunar feldspathic regolith breccias found in 2017, Northwest Africa (NWA) 10291 and NWA 11182, to understand their petrogenetic origin and, more broadly, the evolution of lithologies present in unsampled areas of the Moon and place constraints on lunar crustal evolution in these areas. -
Lev A. Muravyev , Viktor I. Grokhovsky
The Chrono List of Bad Meteorites Harmful № Date Name Place Type Fall Description Source 1Ural Federal University, specimen 1,2 Lombardia, Doubtful 2 1 04.09.1511 Crema shwr several killed birds, sheep, and a man (dbt) [3, 7] Lev A. Muravyev , Institute of Geophysics Ural Branch of RAS, Italy meteorite Doubtful 2 04.09.1654 Milan Italy {?} - killed a monk (dbt) [3, 7] 1 Ekaterinburg, Russia; meteorite Aquitaine, crushed cottage, killed farmer and Viktor I. Grokhovsky 3 24.07.1790 Barbotan H5 shwr - [1, 10] [email protected], [email protected] France some cattle (dbt) Uttar Pradesh, [7, 9, Abstract. The problem of the asteroid-comet hazard is now being 4 19.12.1798 Benares (a) LL4 shwr 0,9 kg building India 10] actively discussed, because the consequences of the fall of large cosmic Bayern, 5 13.12.1803 Mässing Howardite U - building struck [1, 10] bodies on the earth can be catastrophic and affect the survival of Germany humanity and all living things. Fragments of smaller celestial bodies - Moscow, 6 05.09.1812 Borodino H5 U 0,5 kg observed by a soldier on guard [7] meteorites, fall to the earth much more often, and they can also emanate Russia a certain danger. In several papers that were published about 20 years Rajasthan, Doubtful killed a men and injured a women 7 16.01.1825 Oriang {?} - [3, 7] ago, attempts were made to compile a list of events related to the India meteorite (dbt) Uttar Pradesh, [3, 7, 9, damage caused by meteorites falling from the sky. -
Parauapebas Meteorite from Pará, Brazil, a “Hammer” Breccia Chondrite
SILEIR RA A D B E E G D E A O D L E O I G C I A O ARTICLE BJGEO S https://doi.org/10.1590/2317-4889202020190085 Brazilian Journal of Geology D ESDE 1946 Parauapebas meteorite from Pará, Brazil, a “hammer” breccia chondrite Daniel Atencio1* , Dorília Cunha1 , André Luiz Ribeiro Moutinho2 , Maria Elizabeth Zucolotto3 , Amanda Araujo Tosi3 , Caio Vidaurre Nassif Villaça3 Abstract The Parauapebas meteorite, third official meteorite discovered in the Brazilian Amazon region, is a “hammer meteorite” which fell on De- cember 9th, 2013, in the city of Parauapebas, Pará State, Brazil. Mineralogy is dominated by forsterite, enstatite, iron, troilite, and tetrataenite. Albite, chromite, diopside, augite, pigeonite, taenite, and merrillite are minor components. Two main clasts are separated by black shock-in- duced melt veins. One clast exhibits an abundance of chondrules with well-defined margins set on a recrystallized matrix composed mostly of forsterite and enstatite, consistent with petrologic type 4 chondrites. The other clast displays chondrules with outlines blurring into the groundmass as evidence of increasing recrystallization, consistent with petrologic type 5 chondrites. The clasts of petrologic type 4 have a fine-grained texture compared to those of type 5. It is a genomict breccia (indicated by shock melt veins) with the clasts and matrix of the same compositional group, but different petrologic types, H4 and H5. The melted outer crust of the Parauapebas meteorite is comprised of forsterite with interstitial dendritic iron oxide, and is rich in irregular vesicles, which are evidence of the rapid formation of the crust. The type specimen is deposited in the Museum of Geosciences of the University of São Paulo, Brazil. -
Wetumptka Impact Crater
DISCOVERINGAlabama Teacher’s Guide Suggested Curriculum Areas Wetumpka Impact Crater Science Geography Synopsis Social Studies labama bears the scar of an ancient terrible event, the fall Aof a giant meteorite near Wetumpka. Because this happened so long ago — near the end of the Age of Dinosaurs —scientists Suggested Grade Levels were slow to recognize the eroded four-mile wide crater, or as- 4 –12 trobleme, in Elmore County, northeast of Montgomery. Discov- ering Alabama visits this interesting spot, talks to the geologists who discovered it, and interviews scientists who have been study- Key Concepts ing it. Scientific Hypothesis Update: At the time of this video production, featured scien- & Verification tists were studying geologic samples from the astrobleme, search- ing for microscopic evidence of “shocked quartz,” uniquely frac- Catastrophic Events tured quartz grains that would confirm the meteoric origins of the crater. No other known earthly process, not even volcanos, can shatter the hard grains of quartz present in most rocks. After Key Skills this video was produced, the scientists found shocked quartz col- Map Reading lected in the drill cores from the bottom of the astrobleme — proof positive that the Wetumpka Crater was the result of the impact of a large meteorite. Discovering Alabama is a production of the Alabama Museum of Natural History in cooperation with Alabama Public Television. For a complete list of titles in the Discovering Alabama series, as well as for information about ordering videos and accompanying Teacher’s Guides, contact us at either: Discovering Alabama, Box 870340, Tuscaloosa AL 35487–0340; phone: 205–348–2036; fax: 205–348–4219; or email: [email protected]. -
Download Version of Record (PDF / 6MB)
Open Research Online The Open University’s repository of research publications and other research outputs An Isotopic Investigation Of Early Planetesimal Differentiation Processes Thesis How to cite: Windmill, Richard Joseph (2021). An Isotopic Investigation Of Early Planetesimal Differentiation Processes. PhD thesis The Open University. For guidance on citations see FAQs. c 2020 Richard Joseph Windmill https://creativecommons.org/licenses/by-nc-nd/4.0/ Version: Version of Record Link(s) to article on publisher’s website: http://dx.doi.org/doi:10.21954/ou.ro.00012472 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 AN ISOTOPIC INVESTIGATION OF EARLY PLANETESIMAL DIFFERENTIATION PROCESSES Richard J. Windmill Supervisors: Dr. I. A. Franchi Professor M. Anand Dr. R. C. Greenwood Submitted to the School of Physical Sciences at The Open University in accordance with the requirements for the degree of Doctor of Philosophy June 2020 School of Physical Sciences Robert Hooke Building The Open University Walton Hall Milton Keynes MK7 6AA United Kingdom Abstract The differentiation and early evolution of planetesimals is relatively poorly understood. The Main- Group pallasites (PMGs) and IIIAB irons are differentiated meteorite groups from deep planetesimal interiors. They provide a window into the early evolution of rocky planets because of the abundance of samples from these groups and because a common planetary provenance has been proposed. Oxygen isotope analyses are crucial in understanding these relationships. -
Meteors and Meteorites Lithograph
National Aeronautics and Space Administration Meteors and Meteorites www.nasa.gov “Shooting stars,” or meteors, are bits of interplanetary material Meteorites may resemble Earth rocks, but they usually have a SIGNIFICANT DATES falling through Earth’s atmosphere and heated to incandescence “burned” exterior. This fusion crust is formed as the meteorite 4.55 billion years ago — Formation age of most meteorites, by friction. These objects are called meteoroids as they are hur- is melted by friction as it passes through the atmosphere. There taken to be the age of the solar system. tling through space, becoming meteors for the few seconds they are three major types of meteorites: the “irons,” the “stones,” 65 million years ago — Chicxulub impact leads to the death of streak across the sky and create glowing trails. and the “stony-irons.” Although the majority of meteorites that 75 percent of the animals on Earth, including the dinosaurs. fall to Earth are stony, more of the meteorites that are discovered Several meteors per hour can usually be seen on any given 50,000 years — Age of Barringer Meteorite Crater in Arizona. long after they fall are “irons” — these heavy objects are easier night. Sometimes the number increases dramatically — these 1478 BCE — First recorded observation of meteors. to distinguish from Earth rocks than stony meteorites. Meteorites events are termed meteor showers. Some occur annually or at 1794 — Ernst Friedrich Chladni publishes the first book on also fall on other solar system bodies. Mars Exploration Rover regular intervals as the Earth passes through the trail of dusty meteorites, in which he proposes that they have an extra- Opportunity found the first meteorite of any type on another debris left by a comet. -
PSRD: Meteorite Collection in Moscow, Russia
PSRD: Meteorite collection in Moscow, Russia October 31, 2018 Better Know A Meteorite Collection: Fersman Mineralogical Museum in Moscow, Russia Written by Linda M. V. Martel Hawai'i Institute of Geophysics and Planetology PSRD highlights places and people around the world who play central roles in caring for and analyzing meteorites. Join us as we visit the meteorite collection at the Fersman Mineralogical Museum in Moscow and talk with the people who help make history and discoveries come alive. Next to one of Moscow's oldest gardens (the Neskuchny, which aptly translates to "not boring" garden) stands the similarly fascinating Fersman Mineralogical Museum that celebrated its 300th anniversary in 2016. Among the museum's gem and mineral treasures is a collection of meteorites of historical significance, including Pallas' Iron found in 1749 in Siberia, also known as the Krasnojarsk pallasite, pictured above [Data link from the Meteoritical Bulletin]. PSRD had the golden opportunity to visit the Fersman Mineralogical Museum in July 2018, along with other attendees of the 81st Meteoritical Society meeting, in the company of Dr. Mikhail Generalov, Collection Chief Curator, pictured below standing next to a large sample of the Seymchan meteorite [Data link from Meteoritical Bulletin]. In this article we highlight a selection of the extraordinary pieces in this meteorite collection. http://www.psrd.hawaii.edu/Oct18/Meteorites.Moscow.Museum.html PSRD: Meteorite collection in Moscow, Russia Dr. Mikhail Generalov stands next to a large sample of the Seymchan meteorite. http://www.psrd.hawaii.edu/Oct18/Meteorites.Moscow.Museum.html PSRD: Meteorite collection in Moscow, Russia A closer view of the cut, polished, and etched surface of the Seymchan meteorite showing the large schreibersite mineral grains (darker areas) and Widmanstätten pattern in the iron-nickel metal.