Solar System Roadmap, When Relevant to Solar System Research Questions
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Modelling and the Transit of Venus
Modelling and the transit of Venus Dave Quinn University of Queensland <[email protected]> Ron Berry University of Queensland <[email protected]> Introduction enior secondary mathematics students could justifiably question the rele- Svance of subject matter they are being required to understand. One response to this is to place the learning experience within a context that clearly demonstrates a non-trivial application of the material, and which thereby provides a definite purpose for the mathematical tools under consid- eration. This neatly complements a requirement of mathematics syllabi (for example, Queensland Board of Senior Secondary School Studies, 2001), which are placing increasing emphasis on the ability of students to apply mathematical thinking to the task of modelling real situations. Success in this endeavour requires that a process for developing a mathematical model be taught explicitly (Galbraith & Clatworthy, 1991), and that sufficient opportu- nities are provided to students to engage them in that process so that when they are confronted by an apparently complex situation they have the think- ing and operational skills, as well as the disposition, to enable them to proceed. The modelling process can be seen as an iterative sequence of stages (not ) necessarily distinctly delineated) that convert a physical situation into a math- 1 ( ematical formulation that allows relationships to be defined, variables to be 0 2 l manipulated, and results to be obtained, which can then be interpreted and a n r verified as to their accuracy (Galbraith & Clatworthy, 1991; Mason & Davis, u o J 1991). The process is iterative because often, at this point, limitations, inac- s c i t curacies and/or invalid assumptions are identified which necessitate a m refinement of the model, or perhaps even a reassessment of the question for e h t which we are seeking an answer. -
An Evolved International Lunar Decade Global Exploration Roadmap
Lunar Exploration Analysis Group (2015) 2016.pdf An Evolved International Lunar Decade Global Exploration Roadmap. David Dunlop. Author1 and Kim Hold- er. Author2, 1 National Space Society, 410 Ashland Ave, Green Bay Wisconsin, [email protected], 2 National Space Society (Patzcuaro, Michoacan, Mexico, Kim [email protected]). Introduction: Since 2007 an International 1 The 2013 GER edition did not reflect the Chinese Space Exploration Coordination Group (ISECG) of 14 government lunar mission series beginning with the of the largest national space agencies has met to look at 2013 Chang’e III successful landing, and reflecting the potential of collaborative planning and coordina- Chang’e IV (now scheduled for 2020 targeting the tion of their national space exploration activities. lunar farside, Change’e V (sample return now sched- While these meetings have generally been closed door uled for 2017) with a Change’6 Mission indicated as a back-up to the sample return mission. (3) events a 2013 edition Global Exploration Roadmap 2 The GER did not reflect any of the Google Lunar X- (GER) was produced (signed off) by 12 of the 14 coun- Prize Missions. Several teams such as Astrobotic and tries reflecting their projected space program activities Moon-X and Team Space IL have received significant in the categories: Low Earth Orbit, Lunar Vicinity, financial support, have developed flight hardware, and Moon, Mars, Asteroids, and Transportation.(1) This while slipping behind the earlier 2015 deadline are GER is a formidable measure of collaborative efforts planning missions to the Moon perhaps succeeding in and spirits and a reflection of significant global coop- 2016 or when more affordable reusable launchers be- eration. -
ESA Technology Programmes A
ESA Technology Programmes A. Tobias European Space Agency Directorate of Technical and Quality Management January 2013 1. Strategic objectives and Technology The strategic objectives in the DG’s proposal to the 2012 Council at Ministerial level •Pushing the frontiers of knowledge Top class Science of space, in space and from Space •Enabling Services Earth observation, meteorology and environmental monitoring, navigation, telecommunications, space situation awareness, integrated applications •Supporting an innovative and competitive Europe 35 % of the satcom market, 50 % of launches to GTO, high multiplicative effort downstream, a sector of high gross added value, with high spin factor The keys: sustaining innovation, strengthening competitiveness and assuring a robust supply chain, and it all •Enabled by technology •Made possible by a competitive industry built during decades of technology and industrial policies and public investments in shared assets 1 • • • • The domains when theytakeoveratTRL5/6fromtechnologypreparation lines Investments intechnologydevelopmentsarefurther continuedinprojects for industry’scompetitivenessintheworldmarket investments inmissions/launchersspaceinfrastructures developmentsand 350 Exploration (Exomars),EarthObservation(MTG,MetOpSG,GSC) areas, orstabilizationinareaswithmajormissionprogrammes,e.g.Robotic Funding fortechnologydevelopmentwithanincreasingtrendinnearlyall Successful CM12,10B The programmes 2. ESATechnologyProgrammes 2. ESATechnologyProgrammes – 400 M € / yearintechnologydevelopmentlinesprepare3B -
Instruction Manual
IINNSSTTRRUUCCTTIIOONN MMAANNUUAALL NexStar 60 . NexStar 80 . NexStar 102 . NexStar 114 . NexStar 130 T A B L E O F C O N T E N T S INTRODUCTION ............................................................................................................................................................ 4 Warning .......................................................................................................................................................................... 4 ASSEMBLY ...................................................................................................................................................................... 7 Assembling the NexStar ................................................................................................................................................. 7 Attaching the Hand Control Holder ............................................................................................................................ 8 Attaching the Fork Arm to the Tripod......................................................................................................................... 8 Attaching the Telescope to the Fork Arm ................................................................................................................... 8 The Star Diagonal ....................................................................................................................................................... 8 The Eyepiece.............................................................................................................................................................. -
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. -
THE PROPER TREATMENT of CORONAL MASS EJECTION BRIGHTNESS: a NEW METHODOLOGY and IMPLICATIONS for OBSERVATIONS Angelos Vourlidas and Russell A
The Astrophysical Journal, 642:1216–1221, 2006 May 10 A # 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A. THE PROPER TREATMENT OF CORONAL MASS EJECTION BRIGHTNESS: A NEW METHODOLOGY AND IMPLICATIONS FOR OBSERVATIONS Angelos Vourlidas and Russell A. Howard Code 7663, Naval Research Laboratory, Washington, DC 20375; [email protected] Received 2005 November 10; accepted 2005 December 30 ABSTRACT With the complement of coronagraphs and imagers in the SECCHI suite, we will follow a coronal mass ejection (CME) continuously from the Sun to Earth for the first time. The comparison, however, of the CME emission among the various instruments is not as easy as one might think. This is because the telescopes record the Thomson-scattered emission from the CME plasma, which has a rather sensitive dependence on the geometry between the observer and the scattering material. Here we describe the proper treatment of the Thomson-scattered emission, compare the CME brightness over a large range of elongation angles, and discuss the implications for existing and future white-light coronagraph observations. Subject headinggs: scattering — Sun: corona — Sun: coronal mass ejections (CMEs) Online material: color figures 1. INTRODUCTION some important implications resulting from dropping this as- It is long been established that white-light emission of the co- sumption. We conclude in x 4. rona originates by Thomson scattering of the photospheric light by coronal electrons (e.g., Minnaert 1930). Coronal mass ejec- 2. THOMSON SCATTERING GEOMETRY tions (CMEs) comprise a spectacular example of this process and The theory behind Thomson scattering is well understood are regularly recorded by ground-based and space-based corona- (Jackson 1997). -
Overview of the ISECG Mission Scenario
Overview of the ISECG Mission Scenario NASA/R. Martinez Chair, International Architecture Working Group April 10, 2014 ISECG Mission Scenario 2020 2030 Low-Earth Orbit International Space Station Robotic Mission Commercial or Government-Owned Platforms Human Mission Beyond Low-Earth Orbit Cargo Mission Test Missions Asteroid Redirection Rosetta Hayabusa-2 OSIRIS-REx (Sample Return) (Sample Return) Explore Near Earth Asteroid Near-Earth Objects Apophis Extended Staging Post for Crew Duration to Lunar Surface Lunar Vicinity Crew Missions Potential Commercial Opportunities LADEE Luna 25 Luna 26 Luna 27 RESOLVE SELENE-2 Luna 28/29 SELENE-3 Human-Assisted (Sample Sample Return Humans to Lunar Surface Chandrayaan-2 Return) Moon Potential Commercial Opportunities Human-Assisted Sample Return Sustainable Human MAVEN ISRO Mars ExoMars InSight ExoMars Mars JAXA Mars Sample Return Mission Missions to the Orbiter Mission 2016 2018 2020 Mars Opportunities Mars System Mars Precursor Human Scale EDL Test Mission Opportunities Multi-Destination Small Human Transportation Cargo Surface Capabilities Initial Lander Mobility (Planned and Conceptual) Cargo Delivery Evolvable Orion Russian Advanced Deep Space Orion Orion & Icon indicates first use opportunity. & Piloted Electric & SLS Crewed SLS Commercial/Institutional launchers not shown. Habitat SLS Propulsion (Upgrade) Lunar (Upgrade) System Lander ISS for Exploraon Maturing cri+cal systems, tes+ng technologies, human research, & tes+ng ops techniques. Explora4on of a Near Earth Asteroid Human exploraon of an asteroid which has been captured and redirected to lunar vicinity Enabling Capabilies Contribu4ons to Mars Mission Readiness Demonstraon of the following core capabili+es: • Space Launch System and Orion • 30-50kW Solar Electric Propulsion NASA’s SLS Advanced Electric Extra Vehicular System and Orion Propulsion Ac4vity • Spacewalk, rendezvous, proximity operaons, docking or grapple, deep Mission Ac4vi4es space navigaon and communicaons. -
On the Autonomous Detection of Coronal Mass Ejections in Heliospheric Imager Data S
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 117, A05103, doi:10.1029/2011JA017439, 2012 On the autonomous detection of coronal mass ejections in heliospheric imager data S. J. Tappin,1 T. A. Howard,2 M. M. Hampson,1,3 R. N. Thompson,2,4 and C. E. Burns2,5 Received 7 December 2011; revised 3 April 2012; accepted 9 April 2012; published 24 May 2012. [1] We report on the development of an Automatic Coronal Mass Ejection (CME) Detection tool (AICMED) for the Solar Mass Ejection Imager (SMEI). CMEs observed with heliospheric imagers are much more difficult to detect than those observed by coronagraphs as they have a lower contrast compared with the background light, have a larger range of intensity variation and are easily confused with other transient activity. CMEs appear in SMEI images as very faint often-fragmented arcs amongst a much brighter and often variable background. AICMED operates along the same lines as Computer Aided CME Tracking (CACTus), using the Hough Transform on elongation-time J-maps to extract straight lines from the data set. We compare AICMED results with manually measured CMEs on almost three years of data from early in SMEI operations. AICMED identified 83 verifiable events. Of these 46 could be matched with manually identified events, the majority of the non-detections can be explained. The remaining 37 AICMED events were newly discovered CMEs. The proportion of false identification was high, at 71% of the autonomously detected events. We find that AICMED is very effective as a region of interest highlighter, and is a promising first step in autonomous heliospheric imager CME detection, but the SMEI data are too noisy for the tool to be completely automated. -
Science Organising Committee Local Organising Committee Katherine Joy (Chair) Romain Tartese Mahesh Anand John Pernet-Fisher
Science Organising Committee Local Organising Committee Katherine Joy (Chair) Romain Tartese (Chair) Romain Tartese Katherine Joy Mahesh Anand Patricia Clay John Pernet-Fisher Samantha Bell Kerri Donaldson-Hanna Vera Fernandes Evelyn Furi John Pernet-Fisher Jessica Flahaut Sarah Crowther Greg Schmitt Gemma Coleman James Carpenter Updated: 27 March 2019 European Lunar Symposium Manchester 2019 Meeting information Welcome you to Manchester for the 7th European Lunar Symposium (ELS). We are hoping to have a great meeting, demonstrating the diversity of the current lunar research in Europe and elsewhere, and continuing to provide a platform to the European lunar researchers for networking as well as exchanging news ideas and latest results in the field of lunar exploration. We gratefully acknowledge the support of the University of Manchester, NASA SSERVI, the Royal Astronomical Society, the Science and Technology Facilities Council, Europlanet, and the European Space Agency. Our special thanks to our SSERVI colleagues Kristina Gibbs, Jennifer Baer, Maria Leus, and Ashcon Nejad, and to Gemma Coleman at the University of Manchester for their contribution to the meeting preparation and program implementation. Members of the Science Organising Committee are thanked for their input in putting together an exciting program and for volunteering to chair various sessions in this meeting. Meeting Venue Please note that there are two different venues: • The reception event on the 20 th May will be held at the Manchester Museum in the south of the city, close to the University of Manchester. • The symposium on 21 st -23 rd May will be held at the Science and Industry Museum – Garratt suite conference facilities. -
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. -
Exploring the Bombardment History of the Moon
EXPLORING THE BOMBARDMENT HISTORY OF THE MOON Community White Paper to the Planetary Science and Astrobiology Decadal Survey 2023-2032 Sanctioned by the NASA Lunar Exploration Analysis Group July 15, 2020 Author: William F. Bottke Endorsers: Endorser Affiliation Joseph M. Boyce University of Hawaii Ian Crawford Birkbeck College, University of London, UK Qing-Zhu Yin University of California at Davis, Department of Earth and Planetary Sciences Kip Hodges Arizona State University Caitlin Ahrens University of Arkansas Stephen Elardo Department of Geological Sciences, University of Florida Kris Zacny Honeybee Robotics Daoru Han Missouri University of Science and Technology Marc Norman Australian National University Gordon Osinski University of Western Ontario Amy Mainzer University of Arizona J. R. Szalay Princeton University Shashwat Shukla University of Twente, The Netherlands Jonti Horner University of Southern Queensland Audrey Bouvier Universität Bayreuth 1 Katherine Joy The University of Manchester, UK Ross W. K. Potter Brown University Barbara Cohen NASA Goddard Space Flight Center Heather Meyer JHU APL Luke Dones Southwest Research Institute Timothy D. Swindle University of Arizona Kirby D. Runyon Johns Hopkins APL Ross A. Beyer SETI Institute and NASA Ames Research Center Stephen Mojzsis University of Colorado at Boulder Simone Marchi SwRI Dimitri A. Papanastassiou Geol. Planet. Sci., Caltech Christian Tai Udovicic Northern Arizona University Nicolle Zellner Albion College Michelle Kirchoff Southwest Research Institute Meng-Hua Zhu