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Martian Crater Morphology
ANALYSIS OF THE DEPTH-DIAMETER RELATIONSHIP OF MARTIAN CRATERS A Capstone Experience Thesis Presented by Jared Howenstine Completion Date: May 2006 Approved By: Professor M. Darby Dyar, Astronomy Professor Christopher Condit, Geology Professor Judith Young, Astronomy Abstract Title: Analysis of the Depth-Diameter Relationship of Martian Craters Author: Jared Howenstine, Astronomy Approved By: Judith Young, Astronomy Approved By: M. Darby Dyar, Astronomy Approved By: Christopher Condit, Geology CE Type: Departmental Honors Project Using a gridded version of maritan topography with the computer program Gridview, this project studied the depth-diameter relationship of martian impact craters. The work encompasses 361 profiles of impacts with diameters larger than 15 kilometers and is a continuation of work that was started at the Lunar and Planetary Institute in Houston, Texas under the guidance of Dr. Walter S. Keifer. Using the most ‘pristine,’ or deepest craters in the data a depth-diameter relationship was determined: d = 0.610D 0.327 , where d is the depth of the crater and D is the diameter of the crater, both in kilometers. This relationship can then be used to estimate the theoretical depth of any impact radius, and therefore can be used to estimate the pristine shape of the crater. With a depth-diameter ratio for a particular crater, the measured depth can then be compared to this theoretical value and an estimate of the amount of material within the crater, or fill, can then be calculated. The data includes 140 named impact craters, 3 basins, and 218 other impacts. The named data encompasses all named impact structures of greater than 100 kilometers in diameter. -
The Composition of the Lunar Crust: Radiative Transfer Modeling and Analysis of Lunar Visible and Near-Infrared Spectra
THE COMPOSITION OF THE LUNAR CRUST: RADIATIVE TRANSFER MODELING AND ANALYSIS OF LUNAR VISIBLE AND NEAR-INFRARED SPECTRA A DISSERTATION SUBMITTED TO THE GRADUATE DIVISION OF THE UNIVERSITY OF HAWAI‘I IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY IN GEOLOGY AND GEOPHYSICS DECEMBER 2009 By Joshua T.S. Cahill Dissertation Committee: Paul G. Lucey, Chairperson G. Jeffrey Taylor Patricia Fryer Jeffrey J. Gillis-Davis Trevor Sorensen Student: Joshua T.S. Cahill Student ID#: 1565-1460 Field: Geology and Geophysics Graduation date: December 2009 Title: The Composition of the Lunar Crust: Radiative Transfer Modeling and Analysis of Lunar Visible and Near-Infrared Spectra We certify that we have read this dissertation and that, in our opinion, it is satisfactory in scope and quality as a dissertation for the degree of Doctor of Philosophy in Geology and Geophysics. Dissertation Committee: Names Signatures Paul G. Lucey, Chairperson ____________________________ G. Jeffrey Taylor ____________________________ Jeffrey J. Gillis-Davis ____________________________ Patricia Fryer ____________________________ Trevor Sorensen ____________________________ ACKNOWLEDGEMENTS I must first express my love and appreciation to my family. Thank you to my wife Karen for providing love, support, and perspective. And to our little girl Maggie who only recently became part of our family and has already provided priceless memories in the form of beautiful smiles, belly laughs, and little bear hugs. The two of you provided me with the most meaningful reasons to push towards the "finish line". I would also like to thank my immediate and extended family. Many of them do not fully understand much about what I do, but support the endeavor acknowledging that if it is something I’m willing to put this much effort into, it must be worthwhile. -
Reader 19 05 19 V75 Timeline Pagination
Plant Trivia TimeLine A Chronology of Plants and People The TimeLine presents world history from a botanical viewpoint. It includes brief stories of plant discovery and use that describe the roles of plants and plant science in human civilization. The Time- Line also provides you as an individual the opportunity to reflect on how the history of human interaction with the plant world has shaped and impacted your own life and heritage. Information included comes from secondary sources and compila- tions, which are cited. The author continues to chart events for the TimeLine and appreciates your critique of the many entries as well as suggestions for additions and improvements to the topics cov- ered. Send comments to planted[at]huntington.org 345 Million. This time marks the beginning of the Mississippian period. Together with the Pennsylvanian which followed (through to 225 million years BP), the two periods consti- BP tute the age of coal - often called the Carboniferous. 136 Million. With deposits from the Cretaceous period we see the first evidence of flower- 5-15 Billion+ 6 December. Carbon (the basis of organic life), oxygen, and other elements ing plants. (Bold, Alexopoulos, & Delevoryas, 1980) were created from hydrogen and helium in the fury of burning supernovae. Having arisen when the stars were formed, the elements of which life is built, and thus we ourselves, 49 Million. The Azolla Event (AE). Hypothetically, Earth experienced a melting of Arctic might be thought of as stardust. (Dauber & Muller, 1996) ice and consequent formation of a layered freshwater ocean which supported massive prolif- eration of the fern Azolla. -
Galileo Reveals Best-Yet Europa Close-Ups Stone Projects A
II Stone projects a prom1s1ng• • future for Lab By MARK WHALEN Vol. 28, No. 5 March 6, 1998 JPL's future has never been stronger and its Pasadena, California variety of challenges never broader, JPL Director Dr. Edward Stone told Laboratory staff last week in his annual State of the Laboratory address. The Laboratory's transition from an organi zation focused on one large, innovative mission Galileo reveals best-yet Europa close-ups a decade to one that delivers several smaller, innovative missions every year "has not been easy, and it won't be in the future," Stone acknowledged. "But if it were easy, we would n't be asked to do it. We are asked to do these things because they are hard. That's the reason the nation, and NASA, need a place like JPL. ''That's what attracts and keeps most of us here," he added. "Most of us can work elsewhere, and perhaps earn P49631 more doing so. What keeps us New images taken by JPL's The Conamara Chaos region on Europa, here is the chal with cliffs along the edges of high-standing Galileo spacecraft during its clos lenge and the ice plates, is shown in the above photo. For est-ever flyby of Jupiter's moon scale, the height of the cliffs and size of the opportunity to do what no one has done before Europa were unveiled March 2. indentations are comparable to the famous to search for life elsewhere." Europa holds great fascination cliff face of South Dakota's Mount To help achieve success in its series of pro for scientists because of the Rushmore. -
1 Fluids Mobilization in Arabia Terra, Mars
Fluids mobilization in Arabia Terra, Mars: depth of pressurized reservoir from mounds self- similar clustering Riccardo Pozzobon1, Francesco Mazzarini2, Matteo Massironi1, Angelo Pio Rossi3, Monica Pondrelli4, Gabriele Cremonese5, Lucia Marinangeli6 1 Department of Geosciences, Università degli Studi di Padova, Via Gradenigo 6 - 35131, Padova, Italy 2 Istituto Nazionale di Geofisica e Vulcanologia (INGV), Via Della Faggiola, 32 - 56100 Pisa, Italy 3 Department of Physics and Earth Sciences, Jacobs University Bremen, Campus Ring 1 -28759 Bremen, Germany 4 International Research School of Planetary Sciences, Università d'Annunzio, viale Pindaro 42 – 65127, Pescara, Italy 5 INAF, Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5 - 35122, Padova, Italy 6 Laboratorio di Telerilevamento e Planetologia, DISPUTer, Universita' G. d'Annunzio, Via Vestini 31 - 66013 Chieti, Italy Abstract Arabia Terra is a region of Mars where signs of past-water occurrence are recorded in several landforms. Broad and local scale geomorphological, compositional and hydrological analyses point towards pervasive fluid circulation through time. In this work we focus on mound fields located in the interior of three casters larger than 40 km (Firsoff, Kotido and unnamed crater 20 km to the east) and showing strong morphological and textural resemblance to terrestrial mud volcanoes and spring-related features. We infer that these landforms likely testify the presence of a pressurized fluid reservoir at depth and past fluid upwelling. We have performed morphometric analyses to characterize the mound morphologies and consequently retrieve an accurate automated mapping of the mounds within the craters for spatial distribution and fractal clustering analysis. The outcome of the fractal clustering yields information about the possible extent of the percolating fracture network at depth below the craters. -
Graphical Evidence for the Solar Coronal Structure During the Maunder Minimum: Comparative Study of the Total Eclipse Drawings in 1706 and 1715
J. Space Weather Space Clim. 2021, 11,1 Ó H. Hayakawa et al., Published by EDP Sciences 2021 https://doi.org/10.1051/swsc/2020035 Available online at: www.swsc-journal.org Topical Issue - Space climate: The past and future of solar activity RESEARCH ARTICLE OPEN ACCESS Graphical evidence for the solar coronal structure during the Maunder minimum: comparative study of the total eclipse drawings in 1706 and 1715 Hisashi Hayakawa1,2,3,4,*, Mike Lockwood5,*, Matthew J. Owens5, Mitsuru Sôma6, Bruno P. Besser7, and Lidia van Driel – Gesztelyi8,9,10 1 Institute for Space-Earth Environmental Research, Nagoya University, 4648601 Nagoya, Japan 2 Institute for Advanced Researches, Nagoya University, 4648601 Nagoya, Japan 3 Science and Technology Facilities Council, RAL Space, Rutherford Appleton Laboratory, Harwell Campus, OX11 0QX Didcot, UK 4 Nishina Centre, Riken, 3510198 Wako, Japan 5 Department of Meteorology, University of Reading, RG6 6BB Reading, UK 6 National Astronomical Observatory of Japan, 1818588 Mitaka, Japan 7 Space Research Institute, Austrian Academy of Sciences, 8042 Graz, Austria 8 Mullard Space Science Laboratory, University College London, RH5 6NT Dorking, UK 9 LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université Paris Diderot, Sorbonne Paris Cité, 92195 Meudon, France 10 Konkoly Observatory, Hungarian Academy of Sciences, 1121 Budapest, Hungary Received 18 October 2019 / Accepted 29 June 2020 Abstract – We discuss the significant implications of three eye-witness drawings of the total solar eclipse on 1706 May 12 in comparison with two on 1715 May 3, for our understanding of space climate change. These events took place just after what has been termed the “deep Maunder Minimum” but fall within the “extended Maunder Minimum” being in an interval when the sunspot numbers start to recover. -
Godinho Vt Me Bauru.Pdf (4.652Mb)
UNIVERSIDADE ESTADUAL PAULISTA “JÚLIO DE MESQUITA FILHO” PROGRAMA DE PÓS-GRADUAÇÃO EM DOCÊNCIA PARA A EDUCAÇÃO BÁSICA ALFABETIZAÇÃO CIENTÍFICA NA EDUCAÇÃO INFANTIL: SEQUÊNCIA DE ENSINO INVESTIGATIVO SOBRE A LUA VIVIAN THAÍS GODINHO BAURU 2021 0 VIVIAN THAÍS GODINHO ALFABETIZAÇÃO CIENTÍFICA NA EDUCAÇÃO INFANTIL: SEQUÊNCIA DE ENSINO INVESTIGATIVO SOBRE A LUA Dissertação apresentada como requisito parcial para obtenção do título de Mestre a Universidade Estadual Paulista Júlio de Mesquita Filho – Faculdade de Ciências, Campus de Bauru – Programa de Pós- graduação em Docência para a Educação Básica, sob orientação do Prof. Dr. João José Caluzi. BAURU 2021 1 2 3 Dedico esse trabalho à Deus que tornou esse sonho possível, aos meus Pais que me ensinaram o verdadeiro valor da educação, aos poucos e maravilhosos amigos e em especial aos meus lindos e queridos alunos que tornaram esse trabalho um presente maravilhoso. 4 Ensinar é um exercício de imortalidade. De alguma forma continuamos a viver naqueles cujos olhos aprenderam a ver o mundo pela magia das nossas palavras. O professor, assim, não morre jamais... Rubem Alves AGRADECIMENTOS Agradeço muito aos meus pais por serem a minha base e que sempre me incentivaram a buscar o sonho do mestrado e nunca me deixaram esmorecer nos percalços dos caminhos até aqui. Agradeço muito a alguns amigos especiais que com certeza sem eles eu também não teria conseguido chegar até aqui: a minha irmã de coração Débora que sempre me incentivou e me mostrou que eu era capaz. O Guilherme um presente maravilhoso que ganhei com o mestrado, que sempre me falava pra ter calma, que tudo ia ficar bem, e ria do meu exagero e que durante esses dois anos me aturou bravamente, aguentando meus áudios de mais de dois minutos. -
Just a Beginning: Computers and Celestial Mechanics in the Work of Wallace J
Just a Beginning: Computers and Celestial Mechanics in the work of Wallace J. Eckert by Allan Olley A thesis submitted in conformity with the requirements for the degree of Doctor of Philosophy Graduate Department of Institute for History and Philosophy of Science University of Toronto Copyright © 2011 by Allan Olley Abstract Just a Beginning: Computers and Celestial Mechanics in the work of Wallace J. Eckert Allan Olley Doctor of Philosophy Graduate Department of Institute for History and Philosophy of Science University of Toronto 2011 This thesis details and analyzes the interaction between computers and science in a particular case. The case is the career of Wallace J. Eckert (1902-1971). Eckert was a professor of astronomy at Columbia University and scientific researcher for IBM. He has received some attention in the history of computing for his significant work in machine computation in the 1930s and 1940s and was the foremost expert on lunar theory for much of his life. First the existing secondary literature on the subject is discussed. Eckert's work has rarely been the focus of sustained historical scrutiny, but the question of the relation of science and the computer has received more scholarship in the history, philosophy and sociology of science. The main narrative of the thesis begins with the history of the various mathematical techniques and external aids to computation used over the course of the history of celestial mechanics. Having set the context, Eckert's early life and career is detailed up until 1945. Here, before the modern computer as such was developed, Eckert innovated by adapting IBM punched card machines to astronomical applications. -
When Computers Were Human
When Computers Were Human When Computers Were Human David Alan Grier princeton university press princeton and oxford Copyright © 2005 by Princeton University Press Published by Princeton University Press, 41 William Street, Princeton, New Jersey 08540 In the United Kingdom: Princeton University Press, 3 Market Place, Woodstock, Oxfordshire OX20 1SY All Rights Reserved Third printing, and first paperback printing, 2007 Paperback ISBN: 978-0-691-13382-9 The Library of Congress has cataloged the cloth edition of this book as follows Grier, David Alan, 1955 Feb. 14– When computers were human / David Alan Grier. p. cm. Includes bibliographical references. ISBN 0-691-09157-9 (acid-free paper) 1. Calculus—History. 2. Science—Mathematics—History. I. Title. QA303.2.G75 2005 510.922—dc22 2004022631 British Library Cataloging-in-Publication Data is available This book has been composed in Sabon Printed on acid-free paper. ∞ press.princeton.edu Printed in the United States of America 109876543 FOR JEAN Who took my people to be her people and my stories to be her own without realizing that she would have to accept a comet, the WPA, and the oft-told tale of a forgotten grandmother Contents Introduction A Grandmother’s Secret Life 1 Part I: Astronomy and the Division of Labor 9 1682–1880 Chapter One The First Anticipated Return: Halley’s Comet 1758 11 Chapter Two The Children of Adam Smith 26 Chapter Three The Celestial Factory: Halley’s Comet 1835 46 Chapter Four The American Prime Meridian 55 Chapter Five A Carpet for the Computing Room 72 Part II: -
Science Concept 3: Key Planetary Processes Are Manifested in the Diversity of Lunar Crustal Rocks
Science Concept 3: Key Planetary Processes are Manifested in the Diversity of Lunar Crustal Rocks Science Concept 3: Key planetary processes are manifested in the diversity of crustal rocks Science Goals: a. Determine the extent and composition of the primary feldspathic crust, KREEP layer, and other products of differentiation. b. Inventory the variety, age, distribution, and origin of lunar rock types. c. Determine the composition of the lower crust and bulk Moon. d. Quantify the local and regional complexity of the current lunar crust. e. Determine the vertical extent and structure of the megaregolith. INTRODUCTION Formation and Evolution of the Moon The Moon is a unique environment, preserving crucial information about the early history and later evolution of the solar system. The lack of major surficial tectonic processes within the past few billion years or so, as well as the lack of significant quantities of surface water, have allowed for excellent preservation of the lithologies and geomorphological features that formed during the major planetary formation events. Fundamental discoveries during the Apollo program showed that the Moon is made up of a variety of volcanic and impact rock types that exhibit a particular range of chemical and mineralogical compositions. The key planetary processes conveyed by this diversity include planetary differentiation, volcanism, and impact cratering. Analysis of Apollo, Luna, and lunar meteoritic samples, as well as orbital data from a series of lunar exploration missions, generated geophysical models that strove to tell the story of the Moon. However, such models are restricted in the sense that they are based on information gathered from the samples that have so far been acquired. -
A Bibliography of Dunes: Earth, Mars, and Venus
NASA Contractor Report 4149 A Bibliography of Dunes: Earth, Mars, and Venus N. Lancaster COOPERATIVE AGREEMENT NCC2-346 JUNE 1988 _ ..v' t_, 111111111111111111111111111111111/1/1/1/1/111 NI\S/\ NF01829 NASA Contractor Report 4149 A Bibliography of Dunes: Earth, Mars, and Venus N. Lancaster Arizona State University Tempe, Arizona Prepared for NASA Office of Space Science and Appltcations under Cooperative Agreement NCC2-346 NI\SI\ National Aeronautics and Space Administration SCientific and Techmcal Information Division 1988 T ABLE OF CONTENTS Preface.................................................................... v Acknowledgements..................................................... v Dunes as a Planetary Landform... .... .... .... ..... ..... ..... ...... 1 Facets of Dune Study .................................... ........................... 3 Characteristics of Dunes ........................................... ... .... 5 Subject Index............................................................ 11 Geographical Index..................................................... 23 Bibliography............................................................. 31 iii This Page Intentionally left Blank PREFACE Dunes are important depositional Likewise, work on aeolian sandstones landforms and sedimentary has been excluded, except where it environments on Earth and Mars, and includes a significant discussion of may be important on Venus. The modern aeolian environments. Material similarity of dune forms on Earth and on planetary aeolian processes and -
Mars As the Abode of Life
MARS AS THE ABODE OF LIFE BY PERCIVAL LOWELL, A.B., LL.D. AUTHOR OF "MARS AND ITS CANaLS," ETC. director of the observatory at flagstaff, arizona; non-resident professor of astronomy at the massachusetts institute of technology; fellow of the american academy of arts and sciences: membre de la soc1ete astronomique de france: member of the astronomical and astro- physical society of america: mitglied der astronomische ge- sellschaft; membre db la societe belge d'astronomie; honorary member of the sociedad astronomica de mex ico; janssen medalist of the societe astronomique de france, mm, for researches on mars; etc., etc. ILLUSTRATED 3?efa gorit THE MACMILLAN COMPANY 1908 All rights reserved Copyright, 1908, Bv THE MACMILLAN COMPANY. Set up and electrotyped. Published December, 1908. 371220 ,.,.;«. NortoooB jirraa J. 8. Gushing Co. — Berwick & Smith Co. Norwood, Mass., U.8.a. JkflCROFILM AVAILABLE MY BROTHER PROFESSOR ABBOTT LAWRENCE LOWELL, LL.D. WHO AS TRUSTEE OF THE LOWELL INSTITUTE PROPOSED THESE LECTURES THIS PRESENTATION OF THEM IS AFFECTIONATELY INSCRIBED PREFACE In 1906 Professor Lowell was asked by the trustee of the Lowell Institute to deliver a course of lectures there upon the planet Mars. Eleven years had elapsed since, at the invitation of the former trustee, he had done the like. When the time came for their delivery unusual interest was manifested, the course proving the most thronged of any ever given before the Insti tute. So great was the demand for seats that the hall could not contain the crowd, and the lectures had to be repeated in the afternoons, to audiences almost as large.