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Literature and Cartography in Early Modern Spain: Etymologies and Conjectures Simone Pinet
18 • Literature and Cartography in Early Modern Spain: Etymologies and Conjectures Simone Pinet By the time Don Quijote began to tilt at windmills, maps footprints they leave on the surface of the earth they and mapping had made great advances in most areas— touch, they become one with the maps of their voyages. administrative, logistic, diplomatic— of the Iberian To his housekeeper Don Quijote retorts, world.1 Lines of inquiry about literature and cartography Not all knights can be courtiers, nor can or should all in early modern Spanish literature converge toward courtiers be knights errant: of all there must be in the Miguel de Cervantes’ Don Quijote. The return to the world, and even if all of us are knights, there is a vast heroic age of the chivalric romance, with its mysterious difference between them, because the courtiers, with- geography, contrasted with Don Quijote’s meanderings out leaving their chambers or the thresholds of the around the Iberian peninsula, is especially ironic in view court, walk the whole world looking at a map, with- of what the author, a wounded veteran of military cam- out spending a penny, or suffering heat or cold, hunger paigns (including Lepanto, a battle seen in many maps or thirst; but we, the true knights errant, exposed to the and naval views, and his captivity in Algiers, with com- sun, the cold, the air, the merciless weather night and parable cartographic resonance), probably knew about day, on foot and on horseback, we measure the whole cartography. earth with our own feet, and we do not know the ene- 2 A determining proof of the relation and a fitting epi- mies merely in painting, but in their very being. -
SPP MAB Active Body Small Planetary Platforms Assessment for Main Asteroid Belt Active Bodies
CDF STUDY REPORT SPP MAB Active Body Small Planetary Platforms Assessment for Main Asteroid Belt Active Bodies CDF-178(B) January 2018 SPP MAB Active Body CDF Study Report: CDF-178(B) January 2018 page 1 of 207 CDF Study Report SPP Main Asteroid Belt Active Body Small Planetary Platforms Assessment For Main Asteroid Belt Active Bodies ESA UNCLASSIFIED – Releasable to the Public SPP MAB Active Body CDF Study Report: CDF-178(B) January 2018 page 2 of 207 FRONT COVER Study Logo showing satellite approaching an asteroid with a swarm of nanosats ESA UNCLASSIFIED – Releasable to the Public SPP MAB Active Body CDF Study Report: CDF-178(B) January 2018 page 3 of 207 STUDY TEAM This study was performed in the ESTEC Concurrent Design Facility (CDF) by the following interdisciplinary team: TEAM LEADER AOCS PAYLOAD COMMUNICATIONS POWER CONFIGURATION PROGRAMMATICS/ AIV COST ELECTRICAL PROPULSION DATA HANDLING CHEMICAL PROPULSION GS&OPS SYSTEMS MISSION ANALYSIS THERMAL MECHANISMS Under the responsibility of: S. Bayon, SCI-FMP, Study Manager With the scientific assistance of: Study Scientist With the technical support of: Systems/APIES Smallsats Radiation The editing and compilation of this report has been provided by: Technical Author ESA UNCLASSIFIED – Releasable to the Public SPP MAB Active Body CDF Study Report: CDF-178(B) January 2018 page 4 of 207 This study is based on the ESA CDF Open Concurrent Design Tool (OCDT), which is a community software tool released under ESA licence. All rights reserved. Further information and/or additional copies of the report can be requested from: S. Bayon ESA/ESTEC/SCI-FMP Postbus 299 2200 AG Noordwijk The Netherlands Tel: +31-(0)71-5655502 Fax: +31-(0)71-5655985 [email protected] For further information on the Concurrent Design Facility please contact: M. -
Institut Für Weltraumforschung (IWF) Österreichische Akademie Der Wissenschaften (ÖAW) Schmiedlstraße 6, 8042 Graz, Austria
WWW.OEAW.AC.AT ANNUAL REPORT 2018 IWF INSTITUT FÜR WELTRAUMFORSCHUNG WWW.IWF.OEAW.AC.AT ANNUAL REPORT 2018 COVER IMAGE Artist's impression of the BepiColombo spacecraft in cruise configuration, with Mercury in the background (© spacecraft: ESA/ATG medialab; Mercury: NASA/JPL). TABLE OF CONTENTS INTRODUCTION 5 NEAR-EARTH SPACE 7 SOLAR SYSTEM 13 SUN & SOLAR WIND 13 MERCURY 15 VENUS 16 MARS 17 JUPITER 18 COMETS & DUST 20 EXOPLANETARY SYSTEMS 21 SATELLITE LASER RANGING 27 INFRASTRUCTURE 29 OUTREACH 31 PUBLICATIONS 35 PERSONNEL 45 IMPRESSUM INTRODUCTION INTRODUCTION The Space Research Institute (Institut für Weltraum- ESA's Cluster mission, launched in 2000, still provides forschung, IWF) in Graz focuses on the physics of space unique data to better understand space plasmas. plasmas and (exo-)planets. With about 100 staff members MMS, launched in 2015, uses four identically equipped from 20 nations it is one of the largest institutes of the spacecraft to explore the acceleration processes that Austrian Academy of Sciences (Österreichische Akademie govern the dynamics of the Earth's magnetosphere. der Wissenschaften, ÖAW, Fig. 1). The China Seismo-Electromagnetic Satellite (CSES) was IWF develops and builds space-qualified instruments and launched in February to study the Earth's ionosphere. analyzes and interprets the data returned by them. Its core engineering expertise is in building magnetometers and NASA's InSight (INterior exploration using Seismic on-board computers, as well as in satellite laser ranging, Investigations, Geodesy and Heat Transport) mission was which is performed at a station operated by IWF at the launched in May to place a geophysical lander on Mars Lustbühel Observatory. -
March 21–25, 2016
FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk, -
The Universal Quixote: Appropriations of a Literary Icon
THE UNIVERSAL QUIXOTE: APPROPRIATIONS OF A LITERARY ICON A Dissertation by MARK DAVID MCGRAW Submitted to the Office of Graduate Studies of Texas A&M University in partial fulfillment of the requirements for the degree of DOCTOR OF PHILOSOPHY Chair of Committee, Eduardo Urbina Committee Members, Paul Christensen Juan Carlos Galdo Janet McCann Stephen Miller Head of Department, Steven Oberhelman August 2013 Major Subject: Hispanic Studies Copyright 2013 Mark David McGraw ABSTRACT First functioning as image based text and then as a widely illustrated book, the impact of the literary figure Don Quixote outgrew his textual limits to gain near- universal recognition as a cultural icon. Compared to the relatively small number of readers who have actually read both extensive volumes of Cervantes´ novel, an overwhelming percentage of people worldwide can identify an image of Don Quixote, especially if he is paired with his squire, Sancho Panza, and know something about the basic premise of the story. The problem that drives this paper is to determine how this Spanish 17th century literary character was able to gain near-univeral iconic recognizability. The methods used to research this phenomenon were to examine the character´s literary beginnings and iconization through translation and adaptation, film, textual and popular iconography, as well commercial, nationalist, revolutionary and institutional appropriations and determine what factors made him so useful for appropriation. The research concludes that the literary figure of Don Quixote has proven to be exceptionally receptive to readers´ appropriative requirements due to his paradoxical nature. The Quixote’s “cuerdo loco” or “wise fool” inherits paradoxy from Erasmus of Rotterdam’s In Praise of Folly. -
CASTALIA – a MISSION to a MAIN BELT COMET. G. H. Jones1, K
Spacecraft Reconnaissance of Asteroid and Comet Interiors (2015) 6019.pdf CASTALIA – A MISSION TO A MAIN BELT COMET. G. H. Jones1, K. Altwegg2 , I. Bertini3, A. Bieler4, H. Boehnhardt5, N. Bowles6, A. Braukhane7, M. T. Capria8, A. J. Coates1, V. Ciarletti9, B. Davidsson10, C. Engrand11, A. Fitzsimmons12, A. Gibbings13, O. Hainaut14, M. Hallmann15, A. Herique16, M. Hilchenbach5, M. Homeister13, H. Hsieh17, E. Jehin18 W. Kofman16, L. M. Lara19, J. Licandro20, S. C. Lowry21, F. Moreno19, K. Muinonen22 , M. Paetzold23, A. Penttilä22, Dirk Plettemeier24, D. Prialnik25, U. Marboeuf 2, F. Marzari26, K. Meech27, A. Rotundi28,29, A. Smith1, C. Snodgrass30, I. Thomas6, M. Trieloff31, 1UCL Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, UK ( [email protected] ), 2U. Bern, CH, 3U. Padova, IT, 4U. Michigan, USA, 5MPS, Göttingen, DE, 6U. Oxford, UK, 7DLR, Bremen, DE, 8INAF/IAPS, Rome, IT, 9LATMOS/UVSQ, Guyancourt, FR, 10U. Uppsala, SE, 11CNRS, Paris, FR, 12QUB, Belfast, UK, 13OHB System AG, Bremen, DE, 14ESO, 15DLR, Bremen, DE, 16IPA/UJF, Grenoble, FR, 17Academia Sinica, Institute of Astronomy & Astrophysics, Taiwan, 18U. Liège, BE, 19IAA, Granada, ES, 20IAC, Tenerife, ES, 21U. Kent, Canterbury, UK, 22U. Helsinki, FI, 23U. Köln, DE, 24TU Dresden, DE, 25U. Tel Aviv, IL, 26 INFN, Padova, IT, 27IfA, Honolulu, USA, 28Università di Napoli “Parthenope”, IT, 29 INAF-IAPS, Roma, IT, 30Open U., UK, 31U. Heidelberg, DE Main Belt Comets (MBCs), a type of Active Aster- Radio science, Subsurface radar, Dust impact detector, oid, constitute a newly identified class of solar system Dust composition analyser, Neutral/ion mass spec- objects. -
Detecting the Yarkovsky Effect Among Near-Earth Asteroids From
Detecting the Yarkovsky effect among near-Earth asteroids from astrometric data Alessio Del Vignaa,b, Laura Faggiolid, Andrea Milania, Federica Spotoc, Davide Farnocchiae, Benoit Carryf aDipartimento di Matematica, Universit`adi Pisa, Largo Bruno Pontecorvo 5, Pisa, Italy bSpace Dynamics Services s.r.l., via Mario Giuntini, Navacchio di Cascina, Pisa, Italy cIMCCE, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universits, UPMC Univ. Paris 06, Univ. Lille, 77 av. Denfert-Rochereau F-75014 Paris, France dESA SSA-NEO Coordination Centre, Largo Galileo Galilei, 1, 00044 Frascati (RM), Italy eJet Propulsion Laboratory/California Institute of Technology, 4800 Oak Grove Drive, Pasadena, 91109 CA, USA fUniversit´eCˆote d’Azur, Observatoire de la Cˆote d’Azur, CNRS, Laboratoire Lagrange, Boulevard de l’Observatoire, Nice, France Abstract We present an updated set of near-Earth asteroids with a Yarkovsky-related semi- major axis drift detected from the orbital fit to the astrometry. We find 87 reliable detections after filtering for the signal-to-noise ratio of the Yarkovsky drift esti- mate and making sure the estimate is compatible with the physical properties of the analyzed object. Furthermore, we find a list of 24 marginally significant detec- tions, for which future astrometry could result in a Yarkovsky detection. A further outcome of the filtering procedure is a list of detections that we consider spurious because unrealistic or not explicable with the Yarkovsky effect. Among the smallest asteroids of our sample, we determined four detections of solar radiation pressure, in addition to the Yarkovsky effect. As the data volume increases in the near fu- ture, our goal is to develop methods to generate very long lists of asteroids with reliably detected Yarkovsky effect, with limited amounts of case by case specific adjustments. -
Photometric Survey of 67 Near-Earth Objects S
A&A 615, A127 (2018) Astronomy https://doi.org/10.1051/0004-6361/201732154 & c ESO 2018 Astrophysics Photometric survey of 67 near-Earth objects S. Ieva1, E. Dotto1, E. Mazzotta Epifani1, D. Perna1,2, A. Rossi3, M. A. Barucci2, A. Di Paola1, R. Speziali1, M. Micheli1,4, E. Perozzi5, M. Lazzarin6, and I. Bertini6 1 INAF – Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monte Porzio Catone, Rome, Italy e-mail: [email protected] 2 LESIA – Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universités, UPMC Univ. Paris 06, Univ. Paris Diderot, Sorbonne Paris Cité, 5 place Jules Janssen, 92195 Meudon, France 3 IFAC – CNR, Via Madonna del Piano 10, 50019 Sesto Fiorentino, Firenze, Italy 4 ESA SSA-NEO Coordination Centre„ Largo Galileo Galilei 1, 00044 Frascati (RM), Italy 5 Agenzia Spaziale Italiana, Via del Politecnico 1, 00100 Rome, Italy 6 Department of Physics and Astronomy “Galileo Galilei”, University of Padova, Vicolo dell’Osservatorio 3, 35122 Padova, Italy Received 23 October 2017 / Accepted 29 March 2018 ABSTRACT Context. The near-Earth object (NEO) population is a window into the original conditions of the protosolar nebula, and has the potential to provide a key pathway for the delivery of water and organics to the early Earth. In addition to delivering the crucial ingredients for life, NEOs can pose a serious hazard to humanity since they can impact the Earth. To properly quantify the impact risk, physical properties of the NEO population need to be studied. Unfortunately, NEOs have a great variation in terms of mitigation- relevant quantities (size, albedo, composition, etc.) and less than 15% of them have been characterized to date. -
Neodys (And Astdys and Priority List) Data Provision
NEODyS (and AstDyS and Priority List) Data Provision Fabrizio Bernardi CEO of SpaceDyS What is NEODyS • NEODyS is a web based service and stands for Near Earth Objects Dynamic Site: h@p://newton.dm.unipi.it/neodys • NEODyS provides informaon on the IMPACT PROBABILITY of Near Earth Objects (NEOs), typically for an horizon of 100 years • The most important output is the Risk Page: h@p://newton.dm.unipi.it/neodys2/index.php?pc=4.0 where a list of NEOs (459 on Nov 17th) with some chances of hing the Earth within the next century is posted for the public • Only JPL@NASA provides a similar service with SENTRY • NEODyS team has a technological leadership in Europe (and world) NEODyS background • NEODyS was born in 1999 at the Dep. of Mathemacs of the University of Pisa (Italy), within the CelesDal Mechanics Group (CMG) lead by Prof. Andrea Milani • The main moDvaon was the absence of a rigorous and systemac method for compuDng on a daily basis the probability that an asteroid is hing the Earth • The 1997XF11 case was a PR disaster, just for the lack of a well established system to perform such computaons NEODyS daily acDviDes • Since 1999 NEODyS is processing astrometric data of Near Earth Objects (NEOs) provided by the Minor Planet Center, the official enDty supported by the Internaonal Astronomical Union (IAU) that manages all the asteroids observaons and the official catalog of asteroids • The data are sent to NEODyS either by email or via web, through the Minor Planet Electronic Circulars (MPECs) • MPECs: – DOU à Daily Orbit Update: new observaons -
Simulation of Attitude and Orbital Disturbances Acting on ASPECT Satellite in the Vicinity of the Binary Asteroid Didymos
Simulation of attitude and orbital disturbances acting on ASPECT satellite in the vicinity of the binary asteroid Didymos Erick Flores García Space Engineering, masters level (120 credits) 2017 Luleå University of Technology Department of Computer Science, Electrical and Space Engineering Simulation of attitude and orbital disturbances acting on ASPECT satellite in the vicinity of the binary asteroid Didymos Erick Flores Garcia School of Electrical Engineering Thesis submitted for examination for the degree of Master of Science in Technology. Espoo December 6, 2016 Thesis supervisors: Prof. Jaan Praks Dr. Leonard Felicetti Aalto University Luleå University of Technology School of Electrical Engineering Thesis advisors: M.Sc. Tuomas Tikka M.Sc. Nemanja Jovanović aalto university abstract of the school of electrical engineering master’s thesis Author: Erick Flores Garcia Title: Simulation of attitude and orbital disturbances acting on ASPECT satellite in the vicinity of the binary asteroid Didymos Date: December 6, 2016 Language: English Number of pages: 9+84 Department of Radio Science and Engineering Professorship: Automation Technology Supervisor: Prof. Jaan Praks Advisors: M.Sc. Tuomas Tikka, M.Sc. Nemanja JovanoviÊ Asteroid missions are gaining interest from the scientific community and many new missions are planned. The Didymos binary asteroid is a Near-Earth Object and the target of the Asteroid Impact and Deflection Assessment (AIDA). This joint mission, developed by NASA and ESA, brings the possibility to build one of the first CubeSats for deep space missions: the ASPECT satellite. Navigation systems of a deep space satellite differ greatly from the common planetary missions. Orbital environment close to an asteroid requires a case-by-case analysis. -
Near-Earth Objects
Near-Earth Objects 12/06/96 shows an elongated object about seen here in a NEAR spacecraft image 4.5 kilometers in extent. Veverka et al. (2000), Science, 289, Ostro et al. (1999), Icarus, 137: pp. 122-139. pp. 2088-2097. THE NEAR EARTH OBJECT POPULATION Near-Earth objects are an important area of study because they are relatively primitive bodies left over from the early solar system formation process, they can be utilized as raw materials for building future structures and habitats within the inner solar system, and their rare, but potentially catastrophic, collisions with Earth make them potential hazards. A comprehensive search for near-Earth objects (NEOs) not only ensures that there will be no surprises from Earth threatening objects but there will be new discoveries. During future close Earth approaches, these objects can be studied via ground-based programs including radar "imaging" characterizations and Earth orbital satellite observations (e.g., Hubble Space Telescope). In addition, these NE0 discoveries will provide future mission targets that are among the most accessible in terms of spacecraft energy requirements. Indeed, many near-Earth asteroids present easier rendezvous and landing opportunities than Earth's own Moon. While the vast majority of the rocky asteroids reside between the orbits of Mars and Jupiter and almost all the icy comets are resident in the so-called Kuiper belt and Oort cloud in the outer solar system, a significant number of these bodies reside in the Earth's neighborhood. Near-Earth asteroids and near-Earth comets make up the population of so-called near-Earth objects (NEOs). -
The Castalia Mission to Main Belt Comet 133P/Elst-Pizarro C
The Castalia mission to Main Belt Comet 133P/Elst-Pizarro C. Snodgrass, G.H. Jones, H. Boehnhardt, A. Gibbings, M. Homeister, N. Andre, P. Beck, M.S. Bentley, I. Bertini, N. Bowles, et al. To cite this version: C. Snodgrass, G.H. Jones, H. Boehnhardt, A. Gibbings, M. Homeister, et al.. The Castalia mission to Main Belt Comet 133P/Elst-Pizarro. Advances in Space Research, Elsevier, 2018, 62 (8), pp.1947- 1976. 10.1016/j.asr.2017.09.011. hal-02350051 HAL Id: hal-02350051 https://hal.archives-ouvertes.fr/hal-02350051 Submitted on 28 Aug 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Distributed under a Creative Commons Attribution| 4.0 International License Available online at www.sciencedirect.com ScienceDirect Advances in Space Research 62 (2018) 1947–1976 www.elsevier.com/locate/asr The Castalia mission to Main Belt Comet 133P/Elst-Pizarro C. Snodgrass a,⇑, G.H. Jones b, H. Boehnhardt c, A. Gibbings d, M. Homeister d, N. Andre e, P. Beck f, M.S. Bentley g, I. Bertini h, N. Bowles i, M.T. Capria j, C. Carr k, M.