Carl Sagan by Abby Weaver

Total Page:16

File Type:pdf, Size:1020Kb

Carl Sagan by Abby Weaver FFaammoouuss SScciieennttiissttss by Ms. Amatucci’s th 4 Graders Stony Point Elementary School December 2005 We dedicate this book to all children who will be the "discoverers" of the future and who will some day fulfill their dreams in the world of science. The Process The Virginia 4th Grade Standards of Learning set an expectation that while studying different topics in science (Life Science, Physical Science, and Earth Science) students will become familiar with historical contributions made by individuals. This book came about as a consequence of our desire to meet the standards as well as to produce a book of artistic and literary merit. Initially, we immersed ourselves in the information contained in piles of books from our classroom and library. We created a brainstorming chart and a list of fascinating scientists. Later, each student thought about the field of science that most interested them and settled on one scientist. Each student studied their person and thought about questions like: o What did the scientist do to make him/her well known in the scientific world? o Briefly describe the discovery, invention, or research. o What prompted him/her to do his/her work? The first step in the art process was to sketch our image. We sketched the scientist in portrait style. We made adjustments and started on another sketch. Using our pencil sketches, we used colored pencils to recreate the portraits. We used normal pencils very lightly to get the general idea of what it would look like. Then we colored it in with colored pencils. We layered (using different shades of similar colors to make it stand out) and burnished our picture to give it a waxy, glazed look. For the writing process, we talked about what would be interesting to read. With this information in hand, we did more research on our scientists and collected interesting words and phrases. We answered questions in a template – Scientist Research By First Last Name Who: Where: When: What: How: Why: We took the prases and made them into sentences with whole sentences. We wrote our paragraphs and did the word processing on the computer. The final step was to mount our portraits and paragraphs in an aesthetic manner and prepare them for our group display. Carl Sagan By Abby Weaver Carl Sagan was born in New York on November 9, 1934. He died on December 20, 1996. He wrote books, had a TV show called “Cosmos”, and he also had a movie that was seen by about 500 million people. He was a consultant and advisor to NASA since the 1950s. He was one of the first to think that there was life on other planets, especially Mars. He helped design the Mariner 2 mission to Venus and the Mariner 9 and Viking trips to Mars. He also worked on the Voyager mission to the outer solar system and the Galileo mission to Jupiter. He helped solve the mysteries of the high temperatures in Venus. As a boy he loved to read science fiction books and was very interested in Astronomy. His parents taught him to search for his answers to his many questions. As an adult he continued to search for his answers to his questions about science. Robert Oppenheimer By Alex Houchens He did his research at Los Alamos in New Mexico. He did his research around June 1942. He is no longer living. Robert Oppenheimer invented the first atomic/nuclear bomb. Oppenheimer began to look for a way to separate Uranium 235 from natural uranium and to find out the mass that was to make an atomic bomb. The atomic bomb was used during World War II. It ended the war with Japan. Tycho Brahe by Alex McNair Tycho Brahe was born in Denmark and lived from 1546 to 1601. He created more accurate astronomy instruments and more accurate ways to observe the planets and the moon. His observations showed that the planets and other objects (comets, stars) were behind the moon and that planets and the moon moved in orbits. Brahe observed the moon and the planets and their orbits very carefully with the best instruments. He was very careful with his observations. He kept very accurate records of the movements of the planets and the moon. Brahe went to many colleges and got interested in astronomy. He even bought some astronomy instruments. He wanted to teach people more about astronomy and he believed he could do it by using accurate observations. King Frederick II gave him money to start an observatory. In a dual with a student while he was at college, in Wittenberg in 1566, Brahe lost part of his nose. For the rest of his life, he wore a metal insert over the missing part. ^tàx ZÄxtáÉÇ By Allison Keenan Kate Gleason was born November 25, 1865 in New York. She also did her work in New York. She studied mechanical arts at Cornell University in 1884. Kate helped her father invent and improve a machine that made gears. Henry Ford said it was "the most remarkable machine work ever done by a woman." She also was the first woman president of the First National Bank in Rochester, New York. Kate began working in her father's tool company when she was just 12 years old. She went around the world selling the tools. She was very smart and got along well with people. Thomas Alva Edison By Chandler Hamilton Thomas Edison, known as the Wizard of Menlo Park, was born in 1847 and started inventing in 1868. He died in 1931. He was known as the Wizard of Menlo Park because he was born in Menlo Park, New Jersey. Edison invented the light bulb, phonograph, and the mimeograph. That is what made Edison famous. Edison made lots of stuff. I will tell you about the light bulb. He tried lots of substances and failed until he tried carbonated cotton. Edison was very curious so he made much much more! Alexander Graham Bell by Alyssa Carroll Alexander Graham Bell was born in Edinburgh, Scotland in the 1870s on March 3rd. He died in Canada. He invented the telephone, photo phone, and the telegraph. He did it by connecting two wires, one for the sound and one for receiving. He liked to invent things. He was very interested in communication and wanted to help deaf people. Jane Goodall By Brandon Wiseman I did my research about Jane Goodall. Jane was born in 1934 in England. She currently lives in Nobory, Kenya. In 1985, she observed chimps. She watched them nurse their babies, eat, and catch food. She was awarded the J. Paul Getty Wildlife Conservation prize. She wanted to help us all better understand the relationship between all creatures. William Ryan and Walter Pitman by Brittany Murphy William Ryan does research at Columbia University. Walter Pitman does research at Colombia University. During the 1990’s they did research and in 1997, they published a book about Noah’s flood. They discovered Noah’s flood was real by studying the earth’s surface and other clues. They looked at everything from the past like pottery and they discovered that there had to be a flood. They studied sediments in the rock from the bottom of the Black Sea. They discovered as the climate got warmer, the seas started to rise. The water rose quickly and homes were washed away. Scared people told their story to others. They were curious about the flood. They wanted to know if it was it real and when did it happen. Francis William Aston By Cage Lambert Francis William Aston researched in Birmingham, England. He was born on September 1, 1877 and died on November 20, 1945. Francis researched chemistry and then turned to physics. He won the Forster scholarship in 1898. That allowed him to work on the optical properties of tartaric acid derivatives. Francis developed mass spectrograph, a device that separates atoms or molecular fragments. He went to collage and was trained as a chemist. He was a chemist when he evolved into a psychologist. Thomas Jefferson By Chloe Herring Thomas Jefferson lived in Shadwell and Charlottesville, Va and Paris, France between 1743-1826. He was an inventor, astronomer, a man of science, a paleontologist, and an expert on anatomy. He was an architect. He designed “Monticello”. He liked farming and was an observer of nature. He invented the polygraph, a machine that copied each letter as he was writing. He always wanted to learn about science and study a lot of things. Benjamin Franklin by Cody Herring Ben Franklin was born on Milk Street in Boston Massachusetts on January 17, 1706. He died April 17, 1789. Franklin wanted to answer the question “Are lightning and electricity the same thing?” He made a strange looking kite – it had a rod at the top and a key on a silk cord at the end. On a stormy day, he and his son, Billy went outside with the kite. When lightning hit the rod, Mr. Franklin was holding the key. He got a “tingle” in his hand and figured out that lightning and electricity were the same thing. Mr. Franklin wanted to be able to control electricity. By taking a metal rod and putting it on top of a house he could help prevent homes from catching on fire caused by lightning. He had invented the “lightning rod”. People weren’t so afraid of lightning. Jacques Cousteau By: Cole Dickerson Jacques Cousteau was born in St. Andre- Cubzac, France on June 11th, 1910. He died on June 25th, 1997 in Paris, France.
Recommended publications
  • Mary Anning Information Sheets
    Mary Anning information sheets Mary Anning was born in 1799 in the Dorset town of Lyme Regis. Her dad was a keen fossil hunter and showed Mary and her brother, Joseph, how to find and collect fossils from the local beaches. This part of the coast is now known as the Jurassic Coast due to the high number of pre-historic fossils found there. When Anning was 11 her dad died but she carried on looking for and collecting fossils in order to sell them. Anning’s family was very poor so they needed to earn as much money as possible from the sale of the fossils. Anning didn’t attend school as she needed to earn money for the family, and it was too expensive at the time to attend. She taught herself how to read, write and draw, and read all about anatomy to help her understand the way the fossilised animals that she found were formed. When she was 12, Anning’s brother spotted the fossilised skull of an Ichthyosaur. Anning uncovered it and discovered what turned out to be the first complete Ichthyosaur fossil to be found. This was an important discovery because it challenged the way scientists had thought the natural world had developed. In 1823 Anning discovered a Plesiosaurus and in 1828 she discovered a Pterodactylus. Many scientists came to visit Anning because she was so knowledgeable about her finds and the many other pre-historic fossils she had uncovered. She corresponded regularly with scientists, including Adam Sedgewick, who taught geology at Cambridge University.
    [Show full text]
  • Almost Forgotten Anniversaries in 2019 Introduction
    Almost Forgotten Anniversaries in 2019 Katharina Lodders Department of Earth and Planetary Sciences and Mc Donnell Center for the Space Sciences, Campus Box 1169, Washington University, Saint Louis MO 63130, USA Keywords: history, chemical elements, abundances Abstract: As we celebrate the International Year of the Periodic Table, the 50th anniversary of Apollo 11 and the meteorite falls of Allende and Murchison in 1969, other noteworthy science events with round birthdays seem to be overlooked and almost forgotten Several scientific organizations celebrate the birthdays of their foundation; and key events and discoveries related to meteoritics, astronomy, geo- and cosmochemistry, and nuclear sciences can be commemorated this year, including the anniversaries of the discoveries of eleven chemical elements, and the advancements of our knowledge of the elemental and isotopic abundances. Introduction. Introduction The 150th anniversary of the discovery of the periodic system of the elements by Dmitri Ivanovich Mendeleev (8 Feb. 1834 – 2 Feb. 1907) and independently by Julius Lothar Meyer (19 August 1830 – 11 April 1895) is the reason for celebrating the International Year of the Periodic Table in 2019. Not only that, but several scientific organizations celebrate the birthdays of their foundation: The Astronomical Society of the Pacific (1889), The American Astronomical Society (1899), the American Geophysical Union (1919), the Mineralogical Society of America (1919), and the International Astronomical Union IAU (1919). The anniversaries in 2019 give us reasons to reflect on the major impacts of space exploration. In 1969, the first men landed on the moon and Apollo 11 safely returned with lunar rocks for study. The same year was blessed by the fall of the important carbonaceous chondrites Allende and Murchison.
    [Show full text]
  • See Science Everywhere​(Lesson 5) Mary Anning
    See Science Everywhere (Lesson 5) ​ Mary Anning: The Princess of Paleontology Lesson Overview: Students, in this lesson, will be introduced to an often overlooked figure in ​ history: Mary Anning. Born in England in 1799, Anning was a pioneer in paleontology and an avid fossil collector. She is credited with many monumental geological discoveries; notably the discovery of the first Ichthyosaurus. She also uncovered the fossilized remains of the first ​ ​ winged dinosaur, the plesiosaur. Read to your student about her inspiring life in Dinosaur Lady: ​ The Daring Discoveries of Mary Anning, the First Paleontologist, and explore the fascinating ​ world of fossils with a hands-on activity. 1. Pre-reading: ​ Vocabulary: (These terms can be found at the end of the picture book.) ● Fossil ● Paleontology ● Ammonite ● Belemnite ● Coprolites ● Petricola pholadiformis ● Plesiosaurus ● Ichthyosaurus ● Dinosaur ● Jurassic Period 2. Read: Follow this link to read the picture book Dinosaur Lady: The Daring Discoveries ​ ​ of Mary Anning, the First Paleontologist by Linda Skeers. ​ 3. Watch: View this brief video clip from The Smithsonian about Mary Anning. ​ ​ ​ The Princess of Paleontology ​ 4. Further Exploration: Explain to your student that during this time in history, the field of ​ paleontology had not been widely studied. Anning’s contributions were controversial; and the fact that she was not only a woman, but a poor, uneducated woman did not help gain her high ranking status among professional scientists. She is truly an unsung hero in this
    [Show full text]
  • Historical Development of the Periodic Classification of the Chemical Elements
    THE HISTORICAL DEVELOPMENT OF THE PERIODIC CLASSIFICATION OF THE CHEMICAL ELEMENTS by RONALD LEE FFISTER B. S., Kansas State University, 1962 A MASTER'S REPORT submitted in partial fulfillment of the requirements for the degree FASTER OF SCIENCE Department of Physical Science KANSAS STATE UNIVERSITY Manhattan, Kansas 196A Approved by: Major PrafeLoor ii |c/ TABLE OF CONTENTS t<y THE PROBLEM AND DEFINITION 0? TEH-IS USED 1 The Problem 1 Statement of the Problem 1 Importance of the Study 1 Definition of Terms Used 2 Atomic Number 2 Atomic Weight 2 Element 2 Periodic Classification 2 Periodic Lav • • 3 BRIEF RtiVJiM OF THE LITERATURE 3 Books .3 Other References. .A BACKGROUND HISTORY A Purpose A Early Attempts at Classification A Early "Elements" A Attempts by Aristotle 6 Other Attempts 7 DOBEREBIER'S TRIADS AND SUBSEQUENT INVESTIGATIONS. 8 The Triad Theory of Dobereiner 10 Investigations by Others. ... .10 Dumas 10 Pettehkofer 10 Odling 11 iii TEE TELLURIC EELIX OF DE CHANCOURTOIS H Development of the Telluric Helix 11 Acceptance of the Helix 12 NEWLANDS' LAW OF THE OCTAVES 12 Newlands' Chemical Background 12 The Law of the Octaves. .........' 13 Acceptance and Significance of Newlands' Work 15 THE CONTRIBUTIONS OF LOTHAR MEYER ' 16 Chemical Background of Meyer 16 Lothar Meyer's Arrangement of the Elements. 17 THE WORK OF MENDELEEV AND ITS CONSEQUENCES 19 Mendeleev's Scientific Background .19 Development of the Periodic Law . .19 Significance of Mendeleev's Table 21 Atomic Weight Corrections. 21 Prediction of Hew Elements . .22 Influence
    [Show full text]
  • 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.
    [Show full text]
  • A Brief History of Nuclear Astrophysics
    A BRIEF HISTORY OF NUCLEAR ASTROPHYSICS PART I THE ENERGY OF THE SUN AND STARS Nikos Prantzos Institut d’Astrophysique de Paris Stellar Origin of Energy the Elements Nuclear Astrophysics Astronomy Nuclear Physics Thermodynamics: the energy of the Sun and the age of the Earth 1847 : Robert Julius von Mayer Sun heated by fall of meteors 1854 : Hermann von Helmholtz Gravitational energy of Kant’s contracting protosolar nebula of gas and dust turns into kinetic energy Timescale ~ EGrav/LSun ~ 30 My 1850s : William Thompson (Lord Kelvin) Sun heated at formation from meteorite fall, now « an incadescent liquid mass » cooling Age 10 – 100 My 1859: Charles Darwin Origin of species : Rate of erosion of the Weald valley is 1 inch/century or 22 miles wild (X 1100 feet high) in 300 My Such large Earth ages also required by geologists, like Charles Lyell A gaseous, contracting and heating Sun 푀⊙ Mean solar density : ~1.35 g/cc Sun liquid Incompressible = 4 3 푅 3 ⊙ 1870s: J. Homer Lane ; 1880s :August Ritter : Sun gaseous Compressible As it shrinks, it releases gravitational energy AND it gets hotter Earth Mayer – Kelvin - Helmholtz Helmholtz - Ritter A gaseous, contracting and heating Sun 푀⊙ Mean solar density : ~1.35 g/cc Sun liquid Incompressible = 4 3 푅 3 ⊙ 1870s: J. Homer Lane ; 1880s :August Ritter : Sun gaseous Compressible As it shrinks, it releases gravitational energy AND it gets hotter Earth Mayer – Kelvin - Helmholtz Helmholtz - Ritter A gaseous, contracting and heating Sun 푀⊙ Mean solar density : ~1.35 g/cc Sun liquid Incompressible = 4 3 푅 3 ⊙ 1870s: J.
    [Show full text]
  • Warfare in a Fragile World: Military Impact on the Human Environment
    Recent Slprt•• books World Armaments and Disarmament: SIPRI Yearbook 1979 World Armaments and Disarmament: SIPRI Yearbooks 1968-1979, Cumulative Index Nuclear Energy and Nuclear Weapon Proliferation Other related •• 8lprt books Ecological Consequences of the Second Ihdochina War Weapons of Mass Destruction and the Environment Publish~d on behalf of SIPRI by Taylor & Francis Ltd 10-14 Macklin Street London WC2B 5NF Distributed in the USA by Crane, Russak & Company Inc 3 East 44th Street New York NY 10017 USA and in Scandinavia by Almqvist & WikseH International PO Box 62 S-101 20 Stockholm Sweden For a complete list of SIPRI publications write to SIPRI Sveavagen 166 , S-113 46 Stockholm Sweden Stoekholol International Peace Research Institute Warfare in a Fragile World Military Impact onthe Human Environment Stockholm International Peace Research Institute SIPRI is an independent institute for research into problems of peace and conflict, especially those of disarmament and arms regulation. It was established in 1966 to commemorate Sweden's 150 years of unbroken peace. The Institute is financed by the Swedish Parliament. The staff, the Governing Board and the Scientific Council are international. As a consultative body, the Scientific Council is not responsible for the views expressed in the publications of the Institute. Governing Board Dr Rolf Bjornerstedt, Chairman (Sweden) Professor Robert Neild, Vice-Chairman (United Kingdom) Mr Tim Greve (Norway) Academician Ivan M£ilek (Czechoslovakia) Professor Leo Mates (Yugoslavia) Professor
    [Show full text]
  • New Chryse and the Provinces
    New Chryse and the Provinces The city of New Chryse is actually several connected cities. The Upper City is located on a break in the crater rim, looking down past a steep rock to the Lower City. Inside the da Vinci crater rim lies the Inner City, also known as the Old City – Red Era tunnels and cave shelters, as well as several nanocomposite towers and cupolas on Mona Lys Ridge looking down on the lower parts of the city. The Lower city lies in a valley sloping down to the Harbour City, which fills a crater 20 kilometres to the East. The Harbour City crater is connected to Camiling Bay and the sea through two canyons and is very well protected from both wind and ice. South of the Lower City and Harbour City lies The Slopes, a straight slope into the sea that is covered with sprawl and slums. Mona Lys Ridge is a mixture of palatial estates surrounded by gardens, imposing official imperial buildings and towering ancient structures used by the highest ranks of the Empire. The central imperial administration and especially the Council is housed in the Deimos Needle, a diamondoid tower that together with its sibling the Phobos Needle dominate the skyline. Escalators allow swift and discreet transport down to the lower levels of the city, and can easily be defended by the police force. North of Mona Lys lies a secluded garden city for higher administrators, guild officials and lesser nobility. The Inner City is to a large extent part of Mona Lys, although most of the inhabitants of Mona Lys do not care much for the dusty old tunnels and hidden vaults – that is left to the Guild of Antiquarians who maintain and protect it.
    [Show full text]
  • Mary Anning of Lyme Regis: 19Th Century Pioneer in British Palaeontology
    Headwaters Volume 26 Article 14 2009 Mary Anning of Lyme Regis: 19th Century Pioneer in British Palaeontology Larry E. Davis College of St. Benedict / St. John's University, [email protected] Follow this and additional works at: https://digitalcommons.csbsju.edu/headwaters Part of the Geology Commons, and the Paleontology Commons Recommended Citation Davis, Larry E. (2009) "Mary Anning of Lyme Regis: 19th Century Pioneer in British Palaeontology," Headwaters: Vol. 26, 96-126. Available at: https://digitalcommons.csbsju.edu/headwaters/vol26/iss1/14 This Article is brought to you for free and open access by DigitalCommons@CSB/SJU. It has been accepted for inclusion in Headwaters by an authorized editor of DigitalCommons@CSB/SJU. For more information, please contact [email protected]. LARRY E. DAVIS Mary Anning of Lyme Regis 19th Century Pioneer in British Palaeontology Ludwig Leichhardt, a 19th century German explorer noted in a letter, “… we had the pleasure of making the acquaintance of the Princess of Palaeontology, Miss Anning. She is a strong, energetic spinster of about 28 years of age, tanned and masculine in expression …” (Aurousseau, 1968). Gideon Mantell, a 19th century British palaeontologist, made a less flattering remark when he wrote in his journal, “… sallied out in quest of Mary An- ning, the geological lioness … we found her in a little dirt shop with hundreds of specimens piled around her in the greatest disorder. She, the presiding Deity, a prim, pedantic vinegar looking female; shred, and rather satirical in her conversation” (Curwin, 1940). Who was Mary Anning, this Princess of Palaeontology and Geological Lioness (Fig.
    [Show full text]
  • Renee M. Clary, Ph.D., F.G.S
    Renee M. Clary, Ph.D., F.G.S. P.O. Box 1705 Mississippi State, MS 39762 (337) 519-9224 [email protected] http://EarthScholars.com http://15DegreeLab.com EDUCATION 2003 Ph. D. Curriculum and Instruction, Geoscience Education, Louisiana State University 1998 M. Ed. Curriculum and Instruction, Science Education, University of Louisiana at Lafayette 1997 M.S. Geology, University of Louisiana at Lafayette 1983 B. S. Chemistry, University of Louisiana at Lafayette Additional Certifications 2010 Distance Learning, Mississippi State University 2009 ESRI Arc GIS I 1982 Scanning Electron Microscopy, McCrone Research Institute EMPLOYMENT 2012- Associate Professor, Director of the Dunn-Seiler Museum, Department of Geosciences, Mississippi State University 2007-2012 Assistant Professor, Director of the Dunn-Seiler Museum, Department of Geosciences, Mississippi State University 2006 Distance Learning Instructor, Department of Geosciences, Mississippi State University 2005-2006 Online Instructor, College of Science and Technology, Northwestern State University of Louisiana 2003-2005 Assistant Professor, Director of the X-Ray Center, Department of Geology, University of Louisiana at Lafayette 2000-2003 Adjunct Professor and Instructor, Department of Geology, University of Louisiana at Lafayette 1999-2003 Instructor, South Louisiana Community College 1998 Research Assistant, Magnetic Products International 1984-1986 Chemistry and Calculus Instructor, Episcopal School of Acadiana 1984-1985 Chemist, Applied Science and Technology Laboratories, Dow Chemical, U.S.A., Louisiana Division 1981-1983 Chief Laboratory Assistant, Asbestos Research Program Clary 2 PUBLICATIONS Refereed Journal Articles Clary, R.M. (2015). William Smith’s mapping milestone: an Interactive Historical Vignette celebrating the bicentennial of the first national geologic map. The Science Teacher, 82(7), 36-42.
    [Show full text]
  • Kadiworking Paper Finalcorrected
    ACADEMY OF EUROPEAN LAW EUI Working Papers AEL 2009/10 ACADEMY OF EUROPEAN LAW CHALLENGING THE EU COUNTER-TERRORISM MEASURES THROUGH THE COURTS edited by Marise Cremona, Francesco Francioni and Sara Poli EUROPEAN UNIVERSITY INSTITUTE , FLORENCE ACADEMY OF EUROPEAN LAW ROBERT SCHUMAN CENTRE FOR ADVANCED STUDIES Challenging the EU Counter-terrorism Measures through the Courts EDITED BY MARISE CREMONA , FRANCESCO FRANCIONI AND SARA POLI EUI W orking Paper AEL 2009/10 This text may be downloaded for personal research purposes only. Any additional reproduction for other purposes, whether in hard copy or electronically, requires the consent of the author(s), editor(s). If cited or quoted, reference should be made to the full name of the author(s), editor(s), the title, the working paper or other series, the year, and the publisher. The author(s)/editor(s) should inform the Academy of European Law if the paper is to be published elsewhere, and should also assume responsibility for any consequent obligation(s). ISSN 1831-4066 © 2009 Marise Cremona, Francesco Francioni and Sara Poli (editors) Printed in Italy European University Institute Badia Fiesolana I – 50014 San Domenico di Fiesole (FI) Italy www.eui.eu cadmus.eui.eu Abstract This collection of papers examines the implications of the European Court of Justice’s approach to UN-related counter-terrorism measures against individuals (so-called ‘smart sanctions’), as expressed by its ruling in Case C-402/05P Kadi v Council and Commission , in which it annulled an EC act implementing a UN Security Council resolution. The impact of this seminal judgment on the EC legal order, on its relationship with the UN Charter, and on the case-law of the European Court of Human rights is the theme of this collection.
    [Show full text]
  • Magnetized Impact Craters
    Icarus xxx (2011) xxx–xxx Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Predicted and observed magnetic signatures of martian (de)magnetized impact craters ⇑ Benoit Langlais a, , Erwan Thébault b a CNRS UMR 6112, Université de Nantes, Laboratoire de Planétologie et Géodynamique, 2 Rue de la Houssinière, F-44000 Nantes, France b CNRS UMR 7154, Institut de Physique du Globe de Paris, Équipe de Géomagnétisme, 1 Rue Cuvier, F-75005 Paris, France article info abstract Article history: The current morphology of the martian lithospheric magnetic field results from magnetization and Received 3 May 2010 demagnetization processes, both of which shaped the planet. The largest martian impact craters, Hellas, Revised 6 January 2011 Argyre, Isidis and Utopia, are not associated with intense magnetic fields at spacecraft altitude. This is Accepted 6 January 2011 usually interpreted as locally non- or de-magnetized areas, as large impactors may have reset the mag- Available online xxxx netization of the pre-impact material. We study the effects of impacts on the magnetic field. First, a care- ful analysis is performed to compute the impact demagnetization effects. We assume that the pre-impact Keywords: lithosphere acquired its magnetization while cooling in the presence of a global, centered and mainly Mars, Surface dipolar magnetic field, and that the subsequent demagnetization is restricted to the excavation area cre- Mars, Interior Impact processes ated by large craters, between 50- and 500-km diameter. Depth-to-diameter ratio of the transient craters Magnetic fields is set to 0.1, consistent with observed telluric bodies. Associated magnetic field is computed between 100- and 500-km altitude.
    [Show full text]