Magnetite Plaquettes Are Naturally Asymmetric Materials in Meteorites
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Comprehensive Bibliography on Martian Meteorites (Compiled by C
Comprehensive Bibliography on Martian Meteorites (compiled by C. Meyer, March 2008) Abu Aghreb A.E., Ghadi A.M., Schlüter J., Schultz L. and Thiedig F. (2003) Hamadah al Hamra and Dar al Gani: A comparison of two meteorite fields in the Libyan Sahara (abs). Meteoritics & Planet. Sci. 38, A48. Agee Carl B. (2002) Garnet and majorite fractionation in the early Earth and Mars (abs#1862). Lunar Planet. Sci. XXXIII Lunar Planetary Institute, Houston. (CD-ROM). (see address of LPI in Appendix III) Agee C.B., Bogard Don D., Draper D.S., Jones J.H., Meyer Chuck and Mittlefehldt D.W. (2000) Proposed science requirements and acquisition priorities for the first Mars sample return (abs). In Concept and Approaches for Mars Exploration. Part 1 (ed. S. Hubbard) LPI Contribution # 1062. Lunar Planetary Institute, Houston. Agee C.B. and Draper Dave S. (2003) Melting of model Martian mantle at high pressure: Implications for the composition of the Martian basalt source region (abs#1408). Lunar Planet. Sci. Conf. 34th, Lunar Planetary Institute, Houston (CD-ROM). Agerkvist D.P. and Vistisen L. (1993) Mössbauer spectroscopy of the SNC meteorite Zagami (abs). Lunar Planet. Sci. XXIV, 1-2. Lunar Planetary Institute, Houston. Zagami Agerkvist D.P., Vistisen L., Madsen M.B. and Knudsen J.M. (1994) Magnetic properties of Zagami and Nakhla (abs). Lunar Planet. Sci. XXV, 1-2. Lunar Planetary Institute, Houston. Zagami Nakhla Akai J. (1997) Characteristics of iron-oxide and iron-sulfide grains in meteorites and terrestrial sediments, with special references to magnetite grains in Allan Hills 84001 (abs). Meteoritics & Planet. Sci. -
Appendix A: Scientific Notation
Appendix A: Scientific Notation Since in astronomy we often have to deal with large numbers, writing a lot of zeros is not only cumbersome, but also inefficient and difficult to count. Scientists use the system of scientific notation, where the number of zeros is short handed to a superscript. For example, 10 has one zero and is written as 101 in scientific notation. Similarly, 100 is 102, 100 is 103. So we have: 103 equals a thousand, 106 equals a million, 109 is called a billion (U.S. usage), and 1012 a trillion. Now the U.S. federal government budget is in the trillions of dollars, ordinary people really cannot grasp the magnitude of the number. In the metric system, the prefix kilo- stands for 1,000, e.g., a kilogram. For a million, the prefix mega- is used, e.g. megaton (1,000,000 or 106 ton). A billion hertz (a unit of frequency) is gigahertz, although I have not heard of the use of a giga-meter. More rarely still is the use of tera (1012). For small numbers, the practice is similar. 0.1 is 10À1, 0.01 is 10À2, and 0.001 is 10À3. The prefix of milli- refers to 10À3, e.g. as in millimeter, whereas a micro- second is 10À6 ¼ 0.000001 s. It is now trendy to talk about nano-technology, which refers to solid-state device with sizes on the scale of 10À9 m, or about 10 times the size of an atom. With this kind of shorthand convenience, one can really go overboard. -
Deep Carbon Science
From Crust to Core Carbon plays a fundamental role on Earth. It forms the chemical backbone for all essential organic molecules produced by living organ- isms. Carbon-based fuels supply most of society’s energy, and atmos- pheric carbon dioxide has a huge impact on Earth’s climate. This book provides a complete history of the emergence and development of the new interdisciplinary field of deep carbon science. It traces four cen- turies of history during which the inner workings of the dynamic Earth were discovered, and it documents the extraordinary scientific revolutions that changed our understanding of carbon on Earth for- ever: carbon’s origin in exploding stars; the discovery of the internal heat source driving the Earth’s carbon cycle; and the tectonic revolu- tion. Written with an engaging narrative style and covering the scien- tific endeavors of about 150 pioneers of deep geoscience, this is a fascinating book for students and researchers working in Earth system science and deep carbon research. is a life fellow at St. Edmund’s College, University of Cambridge. For more than 50 years he has passionately engaged in bringing discoveries in astronomy and cosmology to the general public. He is a fellow of the Royal Historical Society, a former vice- president of the Royal Astronomical Society and a fellow of the Geological Society. The International Astronomical Union designated asteroid 4027 as Minor Planet Mitton in recognition of his extensive outreach activity and that of Dr. Jacqueline Mitton. From Crust to Core A Chronicle of Deep Carbon Science University of Cambridge University Printing House, Cambridge CB2 8BS, United Kingdom One Liberty Plaza, 20th Floor, New York, NY 10006, USA 477 Williamstown Road, Port Melbourne, VIC 3207, Australia 314–321, 3rd Floor, Plot 3, Splendor Forum, Jasola District Centre, New Delhi – 110025, India 79 Anson Road, #06–04/06, Singapore 079906 Cambridge University Press is part of the University of Cambridge. -
Organic Matter in Meteorites Department of Inorganic Chemistry, University of Barcelona, Spain
REVIEW ARTICLE INTERNATIONAL MICROBIOLOGY (2004) 7:239-248 www.im.microbios.org Jordi Llorca Organic matter in meteorites Department of Inorganic Chemistry, University of Barcelona, Spain Summary. Some primitive meteorites are carbon-rich objects containing a vari- ety of organic molecules that constitute a valuable record of organic chemical evo- lution in the universe prior to the appearance of microorganisms. Families of com- pounds include hydrocarbons, alcohols, aldehydes, ketones, carboxylic acids, amino acids, amines, amides, heterocycles, phosphonic acids, sulfonic acids, sugar-relat- ed compounds and poorly defined high-molecular weight macromolecules. A vari- ety of environments are required in order to explain this organic inventory, includ- ing interstellar processes, gas-grain reactions operating in the solar nebula, and hydrothermal alteration of parent bodies. Most likely, substantial amounts of such Received 15 September 2004 organic materials were delivered to the Earth via a late accretion, thereby provid- Accepted 15 October 2004 ing organic compounds important for the emergence of life itself, or that served as a feedstock for further chemical evolution. This review discusses the organic con- Address for correspondence: Departament de Química Inorgànica tent of primitive meteorites and their relevance to the build up of biomolecules. Universitat de Barcelona [Int Microbiol 2004; 7(4):239-248] Martí i Franquès, 1-11 08028 Barcelona, Spain Tel. +34-934021235. Fax +34-934907725 Key words: primitive meteorites · prebiotic chemistry · chemical evolution · E-mail: [email protected] origin of life providing new opportunities for scientific advancement. One Introduction of the most important findings regarding such bodies is that comets and certain types of meteorites contain organic mole- Like a carpentry shop littered with wood shavings after the cules formed in space that may have had a relevant role in the work is done, debris left over from the formation of the Sun origin of the first microorganisms on Earth. -
A Magnetic Susceptibility Database for Stony Meteorites
Direttore Enzo Boschi Comitato di Redazione Cesidio Bianchi Tecnologia Geofisica Rodolfo Console Sismologia Giorgiana De Franceschi Relazioni Sole-Terra Leonardo Sagnotti Geomagnetismo Giancarlo Scalera Geodinamica Ufficio Editoriale Francesca Di Stefano Istituto Nazionale di Geofisica e Vulcanologia Via di Vigna Murata, 605 00143 Roma Tel. (06) 51860468 Telefax: (06) 51860507 e-mail: [email protected] A MAGNETIC SUSCEPTIBILITY DATABASE FOR STONY METEORITES Pierre Rochette1, Leonardo Sagnotti1, Guy Consolmagno2, Luigi Folco3, Adriana Maras4, Flora Panzarino4, Lauri Pesonen5, Romano Serra6 and Mauri Terho5 1Istituto Nazionale di Geofisica e Vulcanologia, Roma, Italy [[email protected]] 2Specola Vaticana, Castel Gandolfo, Italy 3Antarctic [PNRA] Museum of Siena, Siena, Italy 4Università La Sapienza, Roma, Italy 5University of Helsinki, Finland 6“Giorgio Abetti” Museum of San Giovanni in Persiceto, Italy Pierre Rochette et alii: A Magnetic Susceptibility Database for Stony Meteorites 1. Introduction the Museo Nationale dell’Antartide in Siena [Folco and Rastelli, 2000], the University of More than 22,000 different meteorites Roma “la Sapienza” [Cavaretta Maras, 1975], have been catalogued in collections around the the “Giorgio Abetti” Museum in San Giovanni world (as of 1999) of which 95% are stony types Persiceto [Levi-Donati, 1996] and the private [Grady, 2000]. About a thousand new meteorites collection of Matteo Chinelatto. In particular, are added every year, primarily from Antarctic the Antarctic Museum in Siena is the curatorial and hot-desert areas. Thus there is a need for centre for the Antarctic meteorite collection rapid systematic and non-destructive means to (mostly from Frontier Mountain) recovered by characterise this unique sampling of the solar the Italian Programma Nazionale di Ricerche in system materials. -
Using Oxygen and Carbon Stable Isotopes, 53Mn-53Cr Isotope Systematics, and Petrology to Constrain the History of Carbonates
University of New Mexico UNM Digital Repository Earth and Planetary Sciences ETDs Electronic Theses and Dissertations 7-10-2013 Using oxygen and carbon stable isotopes, 53Mn-53Cr isotope systematics, and petrology to constrain the history of carbonates and water in the CR and CM chondrite parent bodies Mark Tyra Follow this and additional works at: https://digitalrepository.unm.edu/eps_etds Recommended Citation Tyra, Mark. "Using oxygen and carbon stable isotopes, 53Mn-53Cr isotope systematics, and petrology to constrain the history of carbonates and water in the CR and CM chondrite parent bodies." (2013). https://digitalrepository.unm.edu/eps_etds/93 This Dissertation is brought to you for free and open access by the Electronic Theses and Dissertations at UNM Digital Repository. It has been accepted for inclusion in Earth and Planetary Sciences ETDs by an authorized administrator of UNM Digital Repository. For more information, please contact [email protected]. Mark Anthony Tyra Candidate Earth and Planetary Sciences Department This dissertation is approved, and it is acceptable in quality and form for publication: Approved by the Dissertation Committee: Adrian J. Brearley , Chairperson Ian D. Hutcheon Rhian H. Jones Zachary D. Sharp Charles K. Shearer i USING OXYGEN AND CARBON STABLE ISOTOPES, 53MN-53CR ISOTOPE SYSTEMATICS, AND PETROLOGY TO CONSTRAIN THE HISTORY OF CARBONATES AND WATER IN THE CR AND CM CHONDRITE PARENT BODIES by MARK ANTHONY TYRA B.S., Geology, University of Kentucky, 2000 M.S., Geology, University of Maryland, 2005 DISSERTATION Submitted in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy in Earth and Planetary Sciences The University of New Mexico Albuquerque, New Mexico May, 2013 ii DEDICATION Education, on the other hand, means emancipation. -
Physics of Information in Nonequilibrium Systems A
PHYSICS OF INFORMATION IN NONEQUILIBRIUM SYSTEMS A THESIS SUBMITTED TO THE GRADUATE DIVISION OF THE UNIVERSITY OF HAWAI`I AT MANOA¯ IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY IN PHYSICS MAY 2019 By Elan Stopnitzky Thesis Committee: Susanne Still, Chairperson Jason Kumar Yuriy Mileyko Xerxes Tata Jeffrey Yepez Copyright c 2019 by Elan Stopnitzky ii To my late grandmother, Rosa Stopnitzky iii ACKNOWLEDGMENTS I thank my wonderful family members Benny, Patrick, Shanee, Windy, and Yaniv for the limitless love and inspiration they have given to me over the years. I thank as well my advisor Susanna Still, who has always put great faith in me and encouraged me to pursue my own research ideas, and who has contributed to this work and influenced me greatly as a scientist; my friend and collaborator Lee Altenberg, whom I have learned countless things from and who contributed significantly to this thesis; and my collaborator Thomas E. Ouldridge, who also made important contributions. Finally, I would like to thank my partner Danelle Gallo, whose kindness and support have been invaluable to me throughout this process. iv ABSTRACT Recent advances in non-equilibrium thermodynamics have begun to reveal the funda- mental physical costs, benefits, and limits to the use of information. As the processing of information is a central feature of biology and human civilization, this opens the door to a physical understanding of a wide range of complex phenomena. I discuss two areas where connections between non-equilibrium physics and information theory lead to new results: inferring the distribution of biologically important molecules on the abiotic early Earth, and the conversion of correlated bits into work. -
Oxygen Isotope Compositions of the Kaidun Meteorite – Indications for Aqueous Alteration of E-Chondrites
OXYGEN ISOTOPE COMPOSITIONS OF THE KAIDUN METEORITE – INDICATIONS FOR AQUEOUS ALTERATION OF E-CHONDRITES. K. Ziegler1,*, M. Zolensky2, E. D. Young1,3, A. Ivanov4. 1Institute of Geophysics and Planetary Physics, University of California Los Angeles (UCLA), Los Angeles, CA 90095, U.S.A., 2ARES, NASA Johnson Space Center, Houston, TX 77058, U.S.A., 3Department of Earth and Space Sciences, UCLA, Los Angeles, CA 90095, U.S.A., 4Vernadsky Institute, Moscow, Russia. *Current address: Institute of Meteoritics, University of New Mexico, Albuquerque, NM 87131, U.S.A., ([email protected], [email protected], [email protected], [email protected]). Introduction: The Kaidun microbreccia is a Results: The clasts are comprised of the following unique meteorite due to the diversity of its constituent lithologies: altered enstatite chondrites or aubrites, clasts. Fragments of various types of carbonaceous (CI, CM2, C1 (most likely CI1), C2, and a microbreccia. CM, CV, CR), enstatite (EH, EL), and ordinary chon- Surviving E-chondrite or aubrite primary minerals drites, basaltic achondrites, and impact melt products include enstatite, augite, diopside, silica, plagioclase have been described, and also several unknown clasts (albite to anorthite), ilmenite and heideite. Alteration [1, and references therein]. The small mm-sized clasts products of the enstatite material are: poorly-crystalline represent material from different places and times in enstatite, calcite, phyllosilicates, neoformed albite, and the early solar system, involving a large variety of par- amphiboles (actinolite) (Fig. 1). Alteration mineralogy ent bodies [2]; meteorites are of key importance to the of the CM2 clast include Ca carbonates, tochilinite, study of the origin and evolution of the solar system, serpentine, sulfides, and chromite. -
Molecular Asymmetry in Prebiotic Chemistry: an Account from Meteorites
life Review Molecular Asymmetry in Prebiotic Chemistry: An Account from Meteorites Sandra Pizzarello School of Molecular Sciences, Arizona State University, Tempe, AZ 85287, USA; [email protected]; Tel.: +1-480-965-3370 Academic Editors: Pier Luigi Luisi and David Deamer Received: 8 February 2016; Accepted: 7 April 2016; Published: 13 April 2016 Abstract: Carbonaceous Chondrite (CC) meteorites are fragments of asteroids, solar planetesimals that never became large enough to separate matter by their density, like terrestrial planets. CC contains various amounts of organic carbon and carry a record of chemical evolution as it came to be in the Solar System, at the time the Earth was formed and before the origins of life. We review this record as it pertains to the chiral asymmetry determined for several organic compounds in CC, which reaches a broad molecular distribution and enantiomeric excesses of up to 50%–60%. Because homochirality is an indispensable attribute of extant polymers and these meteoritic enantiomeric excesses are still, to date, the only case of chiral asymmetry in organic molecules measured outside the biosphere, the possibility of an exogenous delivery of primed prebiotic compounds to early Earth from meteorites is often proposed. Whether this exogenous delivery held a chiral advantage in molecular evolution remains an open question, as many others regarding the origins of life are. Keywords: meteorites; asteroids; abiotic; prebiotic; chemical evolution; enantiomeric excess 1. Carbon-Containing Meteorites and Cosmochemical Evolution One of the paradigms of chemical evolution proposes that the abiotic formation of increasingly complex molecules throughout cosmochemical and Earthly processes could eventually lead to life’s precursor molecules. -
Quantifying Hydrogen-Deuterium Exchange of Meteoritic Dicarboxylic Acids During Aqueous Extraction
Quantifying hydrogen-deuterium exchange of meteoritic dicarboxylic acids during aqueous extraction Item Type Article; text Authors Fuller, M.; Huang, Y. Citation Fuller, M., & Huang, Y. (2003). Quantifying hydrogendeuterium exchange of meteoritic dicarboxylic acids during aqueous extraction. Meteoritics & Planetary Science, 38(3), 357-363. DOI 10.1111/j.1945-5100.2003.tb00271.x Publisher The Meteoritical Society Journal Meteoritics & Planetary Science Rights Copyright © The Meteoritical Society Download date 29/09/2021 19:01:11 Item License http://rightsstatements.org/vocab/InC/1.0/ Version Final published version Link to Item http://hdl.handle.net/10150/655665 Meteoritics & Planetary Science 38, Nr 3, 357–363 (2003) Abstract available online at http://meteoritics.org Quantifying hydrogen-deuterium exchange of meteoritic dicarboxylic acids during aqueous extraction Megan FULLER and Yongsong HUANG* Department of Geological Sciences, Brown University, Providence, Rhode Island 02912–1846, USA *Corresponding author. E-mail: [email protected] (Received 15 July 2002; revision accepted 8 January 2003) Abstract–Hydrogen isotope ratios of organic compounds in carbonaceous chondrites provide critical information about their origins and evolutionary history. However, because many of these compounds are obtained by aqueous extraction, the degree of hydrogen-deuterium (H/D) exchange that occurs during the process needs to be quantitatively evaluated. This study uses compound- specific hydrogen isotopic analysis to quantify the H/D exchange during aqueous extraction. Three common meteoritic dicarboxylic acids (succinic, glutaric, and 2-methyl glutaric acids) were refluxed under conditions simulating the extraction process. Changes in δD values of the dicarboxylic acids were measured following the reflux experiments. A pseudo-first order rate law was used to model the H/D exchange rates which were then used to calculate the isotope exchange resulting from aqueous extraction. -
Planetary Organic Chemistry and the Origins of Biomolecules
Downloaded from http://cshperspectives.cshlp.org/ on September 28, 2021 - Published by Cold Spring Harbor Laboratory Press Planetary Organic Chemistry and the Origins of Biomolecules Steven A. Benner, Hyo-Joong Kim, Myung-Jung Kim, and Alonso Ricardo Foundation for Applied Molecular Evolution and The Westheimer Institute for Science and Technology, Gainesville, Florida 32601 Correspondence: [email protected] Organic chemistry on a planetary scale is likely to have transformed carbon dioxide and reduced carbon species delivered to an accreting Earth. According to various models for the origin of life on Earth, biological molecules that jump-started Darwinian evolution arose via this planetary chemistry. The grandest of these models assumes that ribonucleic acid (RNA) arose prebiotically, together with components for compartments that held it and a primitive metabolism that nourished it. Unfortunately, it has been challenging to iden- tify possible prebiotic chemistry that might have created RNA. Organic molecules, given energy, have a well-known propensity to form multiple products, sometimes referred to col- lectively as “tar” or “tholin.” These mixtures appear to be unsuited to support Darwinian processes, and certainly have never been observed to spontaneously yield a homochiral genetic polymer. To date, proposed solutions to this challenge either involve too much direct human intervention to satisfy many in the community, or generate molecules that are unreactive “dead ends” under standard conditions of temperature and pressure. Carbohydrates, organic species having carbon, hydrogen, and oxygen atoms in a ratio of 1:2:1 and an aldehyde or ketone group, conspicuously embody this challenge. Theyare com- ponents of RNA and their reactivity can support both interesting spontaneous chemistry as part of a “carbohydrate world,” but they also easily form mixtures, polymers and tars. -
Geochemical Constraints on the Origin of the Moon and Preservation of Ancient Terrestrial Heterogeneities
S. J. Lock et al., Space Science Reviews, 216, 109, doi: 10.1007/s11214-020-00729-z, 2020 Geochemical constraints on the origin of the Moon and preservation of ancient terrestrial heterogeneities Simon J. Locka,∗, Katherine R. Berminghamb,c, Rita Paraid, Maud Boyete aDivision of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA. bDepartment of Earth and Planetary Sciences, Rutgers University, Piscataway, NJ 08854, USA cDepartment of Geology, University of Maryland,College Park, MD 20742, USA. dDepartment of Earth and Planetary Sciences, Washington University in St. Louis, Saint Louis, MO 63130, USA. eUniversit´eClermont Auvergne, CNRS, IRD, OPGC, Laboratoire Magmas et Volcans, F-63000 Clermont-Ferrand, France. Abstract The Moon forming giant impact marks the end of the main stage of Earth's accretion and sets the stage for the subsequent evolution of our planet. The giant impact theory has been the accepted model of lunar origin for 40 years, but the parameters of the impact and the mechanisms that led to the formation of the Moon are still hotly debated. Here we review the principal geochemical observations that constrain the timing and parameters of the impact, the mechanisms of lunar formation, and the contemporaneous evolution of Earth. We discuss how chemical and isotopic studies on lunar, terrestrial and meteorite samples relate to physical models and how they can be used to differentiate between lunar origin models. In particular, we argue that the efficiency of mixing during the collision is a key test of giant impact models. A high degree of intra-impact mixing is required to explain the isotopic similarity between the Earth and Moon but, at the same time, the impact did not homogenize the whole terrestrial mantle, as isotopic signatures of pre-impact heterogeneity are preserved.