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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. -
Gnc 2021 Abstract Book
GNC 2021 ABSTRACT BOOK Contents GNC Posters ................................................................................................................................................... 7 Poster 01: A Software Defined Radio Galileo and GPS SW receiver for real-time on-board Navigation for space missions ................................................................................................................................................. 7 Poster 02: JUICE Navigation camera design .................................................................................................... 9 Poster 03: PRESENTATION AND PERFORMANCES OF MULTI-CONSTELLATION GNSS ORBITAL NAVIGATION LIBRARY BOLERO ........................................................................................................................................... 10 Poster 05: EROSS Project - GNC architecture design for autonomous robotic On-Orbit Servicing .............. 12 Poster 06: Performance assessment of a multispectral sensor for relative navigation ............................... 14 Poster 07: Validation of Astrix 1090A IMU for interplanetary and landing missions ................................... 16 Poster 08: High Performance Control System Architecture with an Output Regulation Theory-based Controller and Two-Stage Optimal Observer for the Fine Pointing of Large Scientific Satellites ................. 18 Poster 09: Development of High-Precision GPSR Applicable to GEO and GTO-to-GEO Transfer ................. 20 Poster 10: P4COM: ESA Pointing Error Engineering -
New Opportunities for Ice Sheet Observations
Remote Sens. 2015, 7, 9371-9389; doi:10.3390/rs70709371 OPEN ACCESS remote sensing ISSN 2072-4292 www.mdpi.com/journal/remotesensing Article The Sentinel-1 Mission: New Opportunities for Ice Sheet Observations Thomas Nagler 1,*, Helmut Rott 1,2, Markus Hetzenecker 1, Jan Wuite 1 and Pierre Potin 3 1 ENVEO IT GmbH, Technikerstrasse 21a, A-6020 Innsbruck, Austria; E-Mails: [email protected] (H.R.); [email protected] (M.H.); [email protected] (J.W.) 2 Institute for Meteorology and Geophysics, University of Innsbruck, A-6020 Innsbruck, Austria 3 European Space Agency/ESRIN, via Galileo Galilei, I-00044 Frascati, Italy; E-Mail: [email protected] * Author to whom correspondence should be addressed; E-Mail: [email protected]; Tel.: +43-512-507-48300; Fax: +43-512-507-48319. Academic Editors: Nicolas Baghdadi and Prasad S. Thenkabail Received: 28 May 2015 / Accepted: 14 July 2015 / Published: 22 July 2015 Abstract: The Sentinel satellite constellation series, developed by the European Space Agency, represents the dedicated space component of the European Copernicus program, committed to long-term operational services in a wide range of application domains. Here, we address the potential of the Sentinel-1 mission for mapping and monitoring the surface velocity of glaciers and ice sheets. We present an ice velocity map of Greenland, derived from synthetic aperture radar (SAR) data acquired in winter 2015 by Sentinel-1A, the first satellite of the Copernicus program in orbit. The map is assembled from about 900 SAR scenes acquired in Interferometric Wide swath (IW) mode, applying the offset tracking technique. -
ESA Strategy for Science at the Moon
ESA UNCLASSIFIED - Releasable to the Public ESA Strategy for Science at the Moon ESA UNCLASSIFIED - Releasable to the Public EXECUTIVE SUMMARY A new era of space exploration is beginning, with multiple international and private sector actors engaged and with the Moon as its cornerstone. This renaissance in lunar exploration will offer new opportunities for science across a multitude of disciplines from planetary geology to astronomy and astrobiology whilst preparing the knowledge humanity will need to explore further into the Solar System. Recent missions and new analyses of samples retrieved during Apollo have transformed our understanding of the Moon and the science that can be performed there. We now understand the scientific importance of further exploration of the Moon to understand the origins and evolution of Earth and the cosmic context of life’s emergence on Earth and our future in space. ESA’s priorities for scientific activities at the Moon in the next ten years are: • Analysis of new and diverse samples from the Moon. • Detection and characterisation of polar water ice and other lunar volatiles. • Deployment of geophysical instruments and the build up a global geophysical network. • Identification and characterisation of potential resources for future exploration. • Deployment long wavelength radio astronomy receivers on the lunar far side. • Characterisation of the dynamic dust, charge and plasma environment. • Characterisation of biological sensitivity to the lunar environment. ESA UNCLASSIFIED - Releasable to the Public -
Sensitron Space Diodes
AS9100 Registered ISO 9001:2000 Registered Your Power Solutions Provider MIL-PRF-19500 JANS Qualified MIL-PRF-38534 Class H Qualified Sensitron Space Diodes: The Sensitron Advantage Sensitron is a major supplier of discrete diodes to the worldwide hi-reliability market, with over 45 years heritage in diode manufacturing. Sensitron has received JANTXV/JANS qualification per MIL-PRF-19500 on 19 slash sheets, encompassing over 250 JANS part numbers. Sensitron manufactures their standard JANS qualified diodes to our “JANS PLUS” flow, which exceeds the already stringent MIL-PRF-19500 requirements while offering our customers a significant cost savings. SENSITRON DIODES SENSITRON SPACE HERITAGE__________________________________________________________________________ . Sensitron has supplied Axial and MELF diodes to the space market for over 15 years . Sensitron has shipped over 3 million JANS and JANS-equivalent diodes to space applications . Sensitron is the second largest supplier of Space Level Diodes with the second largest portfolio of Space Level Rectifiers, Zener Diodes, Transient Voltage Suppressors, and Switching Diodes in the world . Sensitron is JANTXV / JANS qualified on 19 individual MIL-PRF-19500 slash sheets, encompassing over 250 JANS part numbers, with more coming every quarter! VALUE PROPOSITION_______________________________________________________________________ . Sensitron offers the 2nd Largest QPL portfolio of JANS discrete diode semiconductors in the world, and offers highly competitive pricing . While continuing to add more JAN/JANTX/JANTXV and JANS products, we are now adding at “No Charge “ our JANS PLUS Program to all of our JANS product lines . Additional cost savings for our customer comes from our standard process flow: . All parts are Hot Solder Dipped, therefore there is no need to send Sensitron diodes to a third party plating house or to pay a manufacturer for “special plating services” . -
Astronomy News KW RASC FRIDAY JANUARY 8 2021
Astronomy News KW RASC FRIDAY JANUARY 8 2021 JIM FAIRLES What to expect for spaceflight and astronomy in 2021 https://astronomy.com/news/2021/01/what-to-expect-for- spaceflight-and-astronomy-in-2021 By Corey S. Powell | Published: Monday, January 4, 2021 Whatever craziness may be happening on Earth, the coming year promises to be a spectacular one across the solar system. 2020 - It was the worst of times, it was the best of times. First landing on the lunar farside, two impressive successes in gathering samples from asteroids, the first new pieces of the Moon brought home in 44 years, close-up explorations of the Sun, and major advances in low-cost reusable rockets. First Visit to Jupiter's Trojan Asteroids First Visit to Jupiter's Trojan Asteroids In October, NASA is set to launch the Lucy spacecraft. Over its 12-year primary mission, Lucy will visit eight different asteroids. One target lies in the asteroid belt. The other seven are so-called Trojan asteroids that share an orbit with Jupiter, trapped in points of stability 60 degrees ahead of or behind the planet as it goes around the sun. These objects have been trapped in their locations for billions of years, probably since the time of the formation of the solar system. They contain preserved samples of water-rich and carbon-rich material in the outer solar system; some of that material formed Jupiter, while other bits moved inward to contribute to Earth's life-sustaining composition. As a whimsical aside: When meteorites strike carbon-rich asteroids, they create tiny carbon crystals. -
Atmospheric Dynamics Mission. the Phase-A Studies Were All Completed in June 1999
ESA SP-1233 (4) July 1999 Reports for Mission Selection THE FOUR CANDIDATE EARTH EXPLORER CORE MISSIONS Atmospheric Dynamics Mission ESA SP-1233 (4) – The Four Candidate Earth Explorer Core Missions – ATMOSPHERIC DYNAMICS _________________________________________________________________ Report prepared by: Earth Sciences Division Scientific Co-ordinator: Paul Ingmann Earth Observation Preparatory Programme Technical Co-ordinator: Joachim Fuchs Cover: Richard Francis & Carel Haakman Published by: ESA Publications Division c/o ESTEC, Noordwijk, The Netherlands Editor: Bruce Battrick Copyright: © 1999 European Space Agency ISBN 92-9092-528-0 Price: 70 DFl CONTENTS 1 INTRODUCTION................................................................................................................................5 2 BACKGROUND AND SCIENTIFIC JUSTIFICATION...............................................................9 2.1 GLOBAL WIND PROFILE MEASUREMENTS FOR CLIMATE AND NWP........................................9 2.2 THE NEED FOR ATMOSPHERIC WIND FIELDS FOR ATMOSPHERIC ANALYSES .........................10 2.3 POTENTIAL IMPROVEMENT OF NWP BY ENHANCED WIND OBSERVATIONS ...........................14 2.4 THE NEED FOR ATMOSPHERIC WIND FIELDS FOR CLIMATE STUDIES......................................22 2.5 FUTURE STUDIES AND PERSPECTIVES AIMING AT IMPROVING THE WIND FIELD KNOWLEDGE IN THE POST-2000 TIME FRAME ................................................................................................31 2.6 CONCLUSIONS ON NWP AND CLIMATE STUDIES ......................................................................33 -
Campaigns / the Living Planet Programme / Observing the Earth / Our Activities / ESA
Campaigns / The Living Planet Programme / Observing the Earth / Our Activities / ESA → EUROPEAN SPACE ABOUT US OUR ACTIVITIES CONNECT WITH US FOR MEDIA FOR EDUCATORS FOR KIDS AGENCY ESA OBSERVING THE EARTH LIVING PLANET CAMPAIGNS About Campaigns ESA > Our Activities > Observing the Earth > The Living Planet Programme > Campaigns Recent campaigns Cryovex DomeC-air DOMEX-3 IceSAR-2012 Campaigns blog KaSAR SMOS-ice Services Subscribe Campaigns photo gallery Contact us ARCTIC TREK FOR CRYOSAT A short video from Cold Facts explains why going to the Arctic to collect snow and ice measurements ensures confidence in the data from ESA’s CryoSat mission Campaigns data Archive LATEST NEWS Focus on Gabon forests for Biomass 03 March 2016 Gabon on the radar 22 July 2015 Revealing mountains hiding under ice 29 April 2015 Ice venturers yield results for CryoSat 18 March 2015 Plant power from above 03 February 2015 http://www.esa.int/Our_Activities/Observing_the_Earth/The_Living_Planet_Programme/Campaigns[19/04/2016 12:58:52] Campaigns / The Living Planet Programme / Observing the Earth / Our Activities / ESA Air quality under new scrutiny 28 October 2014 News Archive LATEST ARTICLES MOST-VIEWED ARTICLES MOST-VIEWED IMAGES MOST-VIEWED VIDEOS · Sentinel-1 sees rice paddy drop in… · Live updates: Rosetta mission… · Welcome to a comet · Europe’s solar eclipse seen f… · Interstellar dust intercepted at S… · Touchdown! Rosetta’s Philae p… · ROLIS descent image · Rosetta’s twelve-year journey… · Nansen gives birth to two icebergs · Pioneering Philae completes m… · First comet panoramic · Ambition the film · First light for ExoMars · Rosetta to deploy lander on 1… · OSIRIS spots Philae drifting … · Reconstructing Philae’s flight · Busy spacecraft and experiment sch… · Black hole-star pair orbiting… · Comet panoramic – lander orie… · Timelapse: Canary Islands to … FAQ JOBS AT ESA SITE MAP CONTACTS TERMS AND CONDITIONS http://www.esa.int/Our_Activities/Observing_the_Earth/The_Living_Planet_Programme/Campaigns[19/04/2016 12:58:52]. -
Securing the Copernicus Programme Why EU Earth Observation Matters
Briefing April 2017 Securing the Copernicus programme Why EU earth observation matters SUMMARY The Copernicus programme is a user-driven programme which provides six free-of- charge operational services (atmosphere monitoring, marine environment monitoring, land monitoring, climate change, emergency management and security) to EU, national, and regional institutions, as well as to the private sector. The programme builds on the initiative on global monitoring for environment and security launched in 2001. It aims at filling the gaps in European earth observation capacities. Data is provided from space infrastructures, particularly the sentinel missions developed under the programme, and in situ infrastructure supported by the Member States. Copernicus services are mainly operated by European Union (EU) agencies. Copernicus requires a high level of continuity in data and service provision. A strong political commitment at EU level is required to provide adequate funding for the development of the operational earth observation missions and services. The EU – under the framework programme for research and operational programmes – and the European Space Agency (ESA) have invested more than €7 billion in Copernicus since 2002. By the end of 2017, four of the six sentinel missions should be fully deployed and the last of the six services should become fully operational. As Copernicus reaches its full operational stage, the focus of the programme is shifting towards the uptake of the services and the development of a downstream sector that would provide additional commercial services to the users. This aspect is a key priority of the space strategy adopted by the European Commission in October 2016. The development of the downstream sector is dependent on the long-term continuity of service, to be ensured by improved governance of the programme and renewed long- term political and financial commitments for the next EU budgetary period. -
Global Exploration Roadmap
The Global Exploration Roadmap January 2018 What is New in The Global Exploration Roadmap? This new edition of the Global Exploration robotic space exploration. Refinements in important role in sustainable human space Roadmap reaffirms the interest of 14 space this edition include: exploration. Initially, it supports human and agencies to expand human presence into the robotic lunar exploration in a manner which Solar System, with the surface of Mars as • A summary of the benefits stemming from creates opportunities for multiple sectors to a common driving goal. It reflects a coordi- space exploration. Numerous benefits will advance key goals. nated international effort to prepare for space come from this exciting endeavour. It is • The recognition of the growing private exploration missions beginning with the Inter- important that mission objectives reflect this sector interest in space exploration. national Space Station (ISS) and continuing priority when planning exploration missions. Interest from the private sector is already to the lunar vicinity, the lunar surface, then • The important role of science and knowl- transforming the future of low Earth orbit, on to Mars. The expanded group of agencies edge gain. Open interaction with the creating new opportunities as space agen- demonstrates the growing interest in space international science community helped cies look to expand human presence into exploration and the importance of coopera- identify specific scientific opportunities the Solar System. Growing capability and tion to realise individual and common goals created by the presence of humans and interest from the private sector indicate and objectives. their infrastructure as they explore the Solar a future for collaboration not only among System. -
EUMETSAT Water Vapour Products from New Generation Satellites
EUMETSAT water vapour imagery products from new generation satellites: development and validation strategy L. Spezzi*, P. Watts, B. Fougnie, J. Chimot, E. Obligis, B. Bojkov *[email protected] 1 EUMETSAT Water Vapor Imagery products @ G-VAP Meeting (Madrid, 13/14 June 2019) Water Vapour Product map (missions & products) EUMETSAT instrumentation: IR and MW sounders, MW imagers, VIS/IR imagers, UV/VIS spectrometers Operational In development Possible Planned only Not yet committed/under study Not Applicable (not yet in plan → room for @EUMETSAT @SAFs @EUMETSAT @EUMETSAT improvement) and/or SAFs and/or SAFs E.g. talk by Sküchler: “Total water vapor column from Sentinel-5P derived by the AMC-DOAS method” Instr./ Metop MSG Sentinel 3 Metop-SG MTG AMSU IASI S5 S4 AVHRR IASI MWR MWI ICI MWS IRS Product MHS SEVIRI OLCI SLSTR VII 3MI NG UVNS FCI UVN Total Colum Water Vapour (clear-sky) Layer Precipitable Water 1=surface to 850hPa 2=850 to 500 hPa 3=500 hPa to TOA Humidity profile 2004 to present 2016 2022+ Time to present Talk by T. August: ‘’IASI retrieval and validation activities at EUMETSAT: Recent updates’’ 2 EUMETSAT Water Vapor Imagery products @ G-VAP Meeting (Madrid, 13/14 June 2019) EUMETSAT sensors for water vapour imagery High spatial resolution Main types of sensors providing imaging measurements for water vapour retrieval Current: • Multispectral Pushbroom and Dual-view radiometer: →Sentinel-3/OLCI and SLSTR ECMWF does not always S3/OLCI (300m) • Geostationary multi-spectral imagers: resolve all features →MSG/SEVIRI Future: • Geostationary multi-spectral imagers: →MTG/FCI • Polar multi-spectral imagers: →EPS-SG/METimage • Multi-directional Polarimeter: • WV concentration in the boundary layer is an indicator of →EPS-SG/3MI mesoscale developments (scale ~4km), e.g. -
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.