Reviewing the Outreach Around ESA's Rosetta Mission
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Characterization of the Stray Light in a Space Borne Atmospheric AOTF Spectrometer
Characterization of the stray light in a space borne atmospheric AOTF spectrometer Korablev Oleg 1, Fedorova Anna 1, Eric Villard 2,3, Lilian Joly 4, Alexander Kiselev 1, Denis Belyaev 1, Jean-Loup Bertaux 2 1Space Research Institute (IKI), 84/32 Profsoyuznaya, 117997 Moscow, Russia; Moscow Institute of Physics and Technology, Institutsky dr. 9, 141700 Dolgoprudnyi, Russia 2LATMOS/CNRS, 78280 Guyancourt , France. 3ALMA/European Southern Observatory, Santiago, Chile 4GSMA/CNRS Univ. de Reims, Moulin de la Housse, BP 1039, 51687 Reims, France. [email protected] Abstract : Acousto-optic tunable filter (AOTF) spectrometers are being criticized for spectral leakage, distant side lobes of their spectral response (SRF) function, or the stray light. SPICAM-IR is the AOTF spectrometer in the range 1000-1700 nm with a resolving power of 1800-2200 operating on the Mars Express interplanetary probe. It is primarily dedicated to measurements of water vapor in the Martian atmosphere. SPICAM H2O retrievals are generally lower than simultaneous measurements with other instruments, the stray light suggested as a likely explanation. We report the results of laboratory measurements of water vapor in quantity characteristic for the Mars atmosphere with the Flight Spare model of SPICAM-IR. The level of the stray light is below 1.3·10 -4, and the accuracy to measure water vapor is ~0.2 pr. µm, mostly determined by measurement uncertainties and the accuracy of the synthetic modeling. We demonstrate that the AOTF spectrometer dependably measures the water abundance and can be employed as an atmospheric spectrometer. References and links 1. N. J. Chanover, D. A. -
Status After the Venus Flybys
Acta Astronautica 63 (2008) 68–73 www.elsevier.com/locate/actaastro The MESSENGER mission to Mercury: Status after the Venusflybys Ralph L. McNutt Jr.a,∗, Sean C. Solomonb, David G. Granta, Eric J. Finnegana, Peter D. Bedinia, the MESSENGER Team aThe Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723, USA bDepartment of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad Branch Road, N.W., Washington, DC 20015, USA Available online 21 April 2008 Abstract NASA’s MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft, launched on 3 August 2004, is well into its voyage to initiate a new era in our understanding of the terrestrial planets. The mission, spacecraft, and payload are designed to answer six fundamental questions regarding the innermost planet during three flybys and a one-year-long, near-polar-orbital observational campaign. The cruise phase to date has been used to commission the spacecraft and instruments and begin the transition to automated use of the instruments with on-board, time-tagged commands. An Earth flyby one year after launch, a large propulsive maneuver in December 2005, and Venus flybys in October 2006 and June 2007 began the process of changing MESSENGER’s heliocentric motion. The second Venus flyby was also used to complete final rehearsals for Mercury flyby operations in January 2008 while coordinating observations with the European Space Agency’s Venus Express mission. The upcoming Mercury flyby will be the first since that of Mariner 10 in 1975. Along with the second and third MESSENGER flybys in October 2008 and September 2009, that flyby will provide images of the hemisphere of Mercury never seen before by spacecraft as well as the first high-resolution information on Mercury’s surface mineralogy. -
Navigation Challenges During Exomars Trace Gas Orbiter Aerobraking Campaign
NON-PEER REVIEW Please select category below: Normal Paper Student Paper Young Engineer Paper Navigation Challenges during ExoMars Trace Gas Orbiter Aerobraking Campaign Gabriele Bellei 1, Francesco Castellini 2, Frank Budnik 3 and Robert Guilanyà Jané 4 1 DEIMOS Space located at ESA/ESOC, Robert-Bosch-Str. 5, Darmstadt, 64293, Germany 2 Telespazio VEGA located at ESA/ESOC, Robert-Bosch-Str. 5, Darmstadt, 64293, Germany 3 ESA/ESOC, Robert-Bosch-Str. 5, Darmstadt, 64293, Germany 4 GMV INSYEN located at ESA/ESOC, Robert-Bosch-Str. 5, Darmstadt, 64293, Germany Abstract The ExoMars Trace Gas Orbiter satellite spent one year in aerobraking operations at Mars, lowering its orbit period from one sol to about two hours. This delicate phase challenged the operations team and in particular the navigation system due to the highly unpredictable Mars atmosphere, which imposed almost continuous monitoring, navigation and re-planning activities. An aerobraking navigation concept was, for the first time at ESA, designed, implemented and validated on-ground and in-flight, based on radiometric tracking data and complemented by information extracted from spacecraft telemetry. The aerobraking operations were successfully completed, on time and without major difficulties, thanks to the simplicity and robustness of the selected approach. This paper describes the navigation concept, presents a recollection of the main in-flight results and gives a retrospective of the main lessons learnt during this activity. Keywords: ExoMars, Trace Gas Orbiter, aerobraking, navigation, orbit determination, Mars atmosphere, accelerometer Introduction The ExoMars program is a cooperation between the European Space Agency (ESA) and Roscosmos for the robotic exploration of the red planet. -
The Pancam Instrument for the Exomars Rover
ASTROBIOLOGY ExoMars Rover Mission Volume 17, Numbers 6 and 7, 2017 Mary Ann Liebert, Inc. DOI: 10.1089/ast.2016.1548 The PanCam Instrument for the ExoMars Rover A.J. Coates,1,2 R. Jaumann,3 A.D. Griffiths,1,2 C.E. Leff,1,2 N. Schmitz,3 J.-L. Josset,4 G. Paar,5 M. Gunn,6 E. Hauber,3 C.R. Cousins,7 R.E. Cross,6 P. Grindrod,2,8 J.C. Bridges,9 M. Balme,10 S. Gupta,11 I.A. Crawford,2,8 P. Irwin,12 R. Stabbins,1,2 D. Tirsch,3 J.L. Vago,13 T. Theodorou,1,2 M. Caballo-Perucha,5 G.R. Osinski,14 and the PanCam Team Abstract The scientific objectives of the ExoMars rover are designed to answer several key questions in the search for life on Mars. In particular, the unique subsurface drill will address some of these, such as the possible existence and stability of subsurface organics. PanCam will establish the surface geological and morphological context for the mission, working in collaboration with other context instruments. Here, we describe the PanCam scientific objectives in geology, atmospheric science, and 3-D vision. We discuss the design of PanCam, which includes a stereo pair of Wide Angle Cameras (WACs), each of which has an 11-position filter wheel and a High Resolution Camera (HRC) for high-resolution investigations of rock texture at a distance. The cameras and electronics are housed in an optical bench that provides the mechanical interface to the rover mast and a planetary protection barrier. -
First Year of Coordinated Science Observations by Mars Express and Exomars 2016 Trace Gas Orbiter
MANUSCRIPT PRE-PRINT Icarus Special Issue “From Mars Express to ExoMars” https://doi.org/10.1016/j.icarus.2020.113707 First year of coordinated science observations by Mars Express and ExoMars 2016 Trace Gas Orbiter A. Cardesín-Moinelo1, B. Geiger1, G. Lacombe2, B. Ristic3, M. Costa1, D. Titov4, H. Svedhem4, J. Marín-Yaseli1, D. Merritt1, P. Martin1, M.A. López-Valverde5, P. Wolkenberg6, B. Gondet7 and Mars Express and ExoMars 2016 Science Ground Segment teams 1 European Space Astronomy Centre, Madrid, Spain 2 Laboratoire Atmosphères, Milieux, Observations Spatiales, Guyancourt, France 3 Royal Belgian Institute for Space Aeronomy, Brussels, Belgium 4 European Space Research and Technology Centre, Noordwijk, The Netherlands 5 Instituto de Astrofísica de Andalucía, Granada, Spain 6 Istituto Nazionale Astrofisica, Roma, Italy 7 Institut d'Astrophysique Spatiale, Orsay, Paris, France Abstract Two spacecraft launched and operated by the European Space Agency are currently performing observations in Mars orbit. For more than 15 years Mars Express has been conducting global surveys of the surface, the atmosphere and the plasma environment of the Red Planet. The Trace Gas Orbiter, the first element of the ExoMars programme, began its science phase in 2018 focusing on investigations of the atmospheric composition with unprecedented sensitivity as well as surface and subsurface studies. The coordination of observation programmes of both spacecraft aims at cross calibration of the instruments and exploitation of new opportunities provided by the presence of two spacecraft whose science operations are performed by two closely collaborating teams at the European Space Astronomy Centre (ESAC). In this paper we describe the first combined observations executed by the Mars Express and Trace Gas Orbiter missions since the start of the TGO operational phase in April 2018 until June 2019. -
2004-118.Pdf
East MeetsWest in Near-Earth The Hubble Space Telescope Space SpaceTechnologies for Building Making the Most of Earth Observation Data The Hubble Space Telescope ESA's Cooperation with International Partners - Present and Future - Export Control lssues Nino Panagia Andre Farand & Ukike Bohlmann 49 ESA Reaches Out into Deep Space from Spain lntellectual Property Rights -The New Cebreros Station - A New Regime in ESA Contracts Valeriano Claros, Gisela Siiss & Manfred Warhaut tt Karl Eisermann & Christian Grafd 55 East Meets West in Near-Earth Space Programmes in Progress bU - Double Star Bodo Gramkow et al. z.t News - In Brief 76 Making the Most of Earth Observation with Publications 82 Data Assimilation Alan O'Neill, Pierre-Philippe Mathieu & Claus Zehner JJ Space Technologies for the Building Sector Fritz Gamoe 41 eso bulletin ll8-moy 2004 For over twenty yeors Gore Spoce Wire ond Cobies hcve contributed to the success of mony spoce missions, slch os Moon Londing, Spcceob, EURECA, ERSI + 2, lfolsol, SAX, SPCT, lSC, Envisot, XMM, Metop, Integrol, scienfific reseorch in spoce, Co,.lmbus As o speciol cob e supplier we support you in p onning the nexf sfep inlo spoce Coll us now. EORE IEI + 49/91 44/6 Al O Creative Technologies FAX.+ 49/91 44/6a l4 53 Worldwide e ectronics europe@w gore com www goree ecfron co com Our spoce communicotion scenqrio covers the whole ronge of sotellite ond spocecroh opplicotions: Telecommunicotions, Eorth Observotion, Science, Spoce Inlrostructure ond Novigotion. As on experienced developer & supplier of On-Boord TTC & Doto Tronsmission, Pqssive Microwoves, Digitol Processing Units. For over fifteen yeors, Alcotel Espocio hos contributed to the success of more thon 50 progroms sotellites Alcotel Espocio is o Sponish subsidiory compony of Alcotel Spoce BROADEN YOUR IIFE Nino Panogio Spoce Telexope Srience Inslilule, ISA Direclorole of Scientific Progrommes, Boltimore, USA Hubble role in n of the mosl importonl ond prolilic spoce oslronomy nissions of oll time. -
Connecting @Ll Space People Welcome Message 2
Connecting @ll Space People Welcome Message 2 IAF 2018 Events Overview 3 IAF General Assembly 4 ISF 2017 6 IAF Spring Meetings 2018 8 GLAC 2018 9 IAC 2018 10 Overview 11 Plenaries 13 Highlight Lectures 20 Late Breaking News 23 IAF Global Networking Forum (GNF) 24 IAC Special Sessions 37 IAF IDEA “3G” Diversity Events 44 IAC Hosts Summit 46 9th IAF International Meeting for Members 48 of Parliaments YPP Networking Reception 50 Emerging Space Leaders 51 Grant Programme (ESL Grants) Press Conference: Upcoming Global Conference 52 on Space for Emerging Countries, GLEC 2019 ISF 2018 54 IAF Committees’ Reports 56 Technical Committees 57 Administrative Committees 78 Published by the International Astronautical Federation (IAF) 3rd Issue - February 2019 IAF 2018 Activities 80 Copyright © International Astronautical Federation. Other 2018 Events 80 All rights reserved. No part of this magazine may be reproduced or transmitted by any form or by any The International Astronautical Federation 83 means, electronical or mechanical, including photocopying or recording by any information storage or retrieval system without prior written permission from the publishers. CONTENTS IAF 2018 Events Overview Welcome Message Spring has already event in Uruguay. For three days, than 10,000 attendees came to Meetings begun, but experts gathered in Montevideo witness this exceptional event. 2018 2019 we can look to discuss space applications back at 2018 as a very impressive with a specific focus on emerging The majority of IAF publications and successful year. This publica- space nations and Latin America. and for the first time, the IAC tion, the IAF Highlights, is sum- Final Programmes, have been marizing the main IAF events The 69th International Astro- printed in recycled paper this and activities that took place. -
Proceedings of the 2018 Conference on Adding Value and Preserving Data
Conference Proceedings RAL-CONF-2018-001 PV2018: Proceedings of the 2018 conference on adding value and preserving data Harwell, UK 15th-17th May, 2018 Esther Conway (editor), Kate Winfield (editorial assistant) May 2018 ©2018 Science and Technology Facilities Council This work is licensed under a Creative Commons Attribution 4.0 Unported License. Enquiries concerning this report should be addressed to: RAL Library STFC Rutherford Appleton Laboratory Harwell Oxford Didcot OX11 0QX Tel: +44(0)1235 445384 Fax: +44(0)1235 446403 email: [email protected] Science and Technology Facilities Council reports are available online at: http://epubs.stfc.ac.uk ISSN 1362-0231 Neither the Council nor the Laboratory accept any responsibility for loss or damage arising from the use of information contained in any of their reports or in any communication about their tests or investigations. Proceedings of the 2018 conference on adding value and preserving data This publication is a Conference report published by the This publication is a Conference report published by the Science and Technology (STFC) Library and Information Service. The scientific output expressed does not imply a policy position of STFC. Neither STFC nor any person acting on behalf of the Commission is responsible for the use that might be made of this publication. Contact information Name: Esther Conway Address: STFC, Rutherford Appleton Laboratory Harwell, Oxon, UK Email: [email protected] Tel.: +44 01235 446367 STFC https://www.stfc.ac.uk RAL-CONF-2018-001 ISSN- 1362-0231. Preface The PV2018 Conference welcomes you to its 9th edition, to be held 15th – 17th May 2018 at the Rutherford Appleton Laboratory, Harwell Space Cluster (UK), hosted by the UK Space Agency and jointly organised by STFC, NCEO and the Satellite Applications Catapult. -
VIRTIS/Venus Express Summary
VIRTIS for Venus Express Pierre Drossart# and Giuseppe Piccioni&, December 2002 #LESIA, Obs. Paris and &IASF,Rome VIRTIS (Visible and Infrared Thermal Imaging Spectrometer) is a complex instrument initially devoted to the remote sensing study of comet Wirtanen on the Rosetta mission, at wavelengths between 0.3 and 5 mm. The focal planes, with state of the art CCD and infrared detectors achieve high sensitivity for low emissivity sources. Due to the high flexibility of the operational modes of VIRTIS, these performances are also ideally adapted for the study of Venus atmosphere, both on night and day sides. VIRTIS is therefore aimed to provide a 4- dimensional study of Venus atmosphere (2D imaging + spectral dimension + temporal variations), the spectral variations permitting a sounding at different levels of the atmosphere, from the ground up to the thermosphere. The infrared capability of VIRTIS is especially well fitted to the thermal sounding of the night side atmosphere (Taylor et al, 1997), which give a tomography of the atmosphere down to the surface. Precursors: First attempts of imaging spectrometry on the Venus night side from space in the near infrared were made by NIMS/Galileo (Figure 1) in 1990 (Carlson et al, 1990) and VIMS/Cassini in 1999 (Baines et al, 2000). These fast fly-bys gave an idea of how powerful this method of investigation could be at Venus. Unfortunately, the limited duration of the fly- bys allowed only limited investigations, in particular on the meteorological evolution of the clouds. Observation of Venus with a new generation imaging spectrometer like VIRTIS would provide a unique opportunity to continue these investigations on an extended basis. -
The Science Return from Venus Express the Science Return From
The Science Return from Venus Express Venus Express Science Håkan Svedhem & Olivier Witasse Research and Scientific Support Department, ESA Directorate of Scientific Programmes, ESTEC, Noordwijk, The Netherlands Dmitri V. Titov Max Planck Institute for Solar System Studies, Katlenburg-Lindau, Germany (on leave from IKI, Moscow) ince the beginning of the space era, Venus has been an attractive target for Splanetary scientists. Our nearest planetary neighbour and, in size at least, the Earth’s twin sister, Venus was expected to be very similar to our planet. However, the first phase of Venus spacecraft exploration (1962-1985) discovered an entirely different, exotic world hidden behind a curtain of dense cloud. The earlier exploration of Venus included a set of Soviet orbiters and descent probes, the Veneras 4 to14, the US Pioneer Venus mission, the Soviet Vega balloons and the Venera 15, 16 and Magellan radar-mapping orbiters, the Galileo and Cassini flybys, and a variety of ground-based observations. But despite all of this exploration by more than 20 spacecraft, the so-called ‘morning star’ remains a mysterious world! Introduction All of these earlier studies of Venus have given us a basic knowledge of the conditions prevailing on the planet, but have generated many more questions than they have answered concerning its atmospheric composition, chemistry, structure, dynamics, surface-atmosphere interactions, atmospheric and geological evolution, and plasma environment. It is now high time that we proceed from the discovery phase to a thorough -
Spacewatchafrica December 2020 Edition.Cdr
How Sentinel-6 will monitor global rise in sea levels VVVolVolVolVol ol.6 ol.6 66 No.NoNo. No78 No. No. 55 5 12 December 2018 2020 AFRICA Paytv subscriptions soars amidst COVID-19 PandemicNigeria SPECIAL REPORT C O N T E N T S Vol. 8 No. 12 A space party in Africa? Editor in-chief Aliyu Bello My journey as a space STEM Ambassador Executive Manager Tonia Gerrald Measuring the impact of COVID-19 on SA to the editor in-Chief Ngozi Okey business operations and purchasing Head, Application Services M. Yakubu priorities across the space technology supply chain Editorial/ICT Services John Daniel The new Copernicus mission provides Usman Bello free data about 95% of the ocean Alozie Nwankwo COVID – 19 lockdown and television viewership Juliet Nnamdi Client Relations Sunday Tache COVID-19, Children and the Television Space Lookman Bello 5G: Billions of people cannot access Safiya Thani Internet due to infrastructure deficiencies Marketing Offy Pat The gravity of dreams Tunde Nathaniel Nigeria to establish new 165 CORS Wasiu Olatunde station beginning from 2021 How US election campaigns harness GIS Media Relations Favour Madu data for voter outreach Khadijat Yakubu New climate guardian in space: Sentinel-6 Zacheous Felicia will monitor global rise in sea levels Finance Folarin Tunde Ready to continue 20 years of progress The PicoDragon satellite Nigeria: Telecoms will facilitate digital economy drive Space Watch Magazine is a publication of DLR scientist is part of the "Young Elite 2020" Communication Science, Inc. All correspondence should be addressed to editor, space Watch Magazine. Paytv subscriptions soars amidst Abuja office: Plot 2009, Awka Street, UTC Building, COVID-19 pandemic GF 11, Area 10, Garki, Abuja, Nigeria Telescopes record last moments of star 'eaten' by a black hole Tel: 234 80336471114, 07084706167, email: [email protected] LEGAL CONSULTANTS Idowu Oriola & Co. -
Planetary & Solar System Sciences
EGU General Assembly 2012 EGU General Assembly 2012 Programme Group Programme PS – Planetary & Solar System Sciences Monday, 23 April ........................................................................................................................................................................ 2 PS1.1 ........................................................................................................................................................................................ 2 PS2.2 ........................................................................................................................................................................................ 2 GD1.1/PS2.7 .............................................................................................................................................................................. 3 PS3.3 ........................................................................................................................................................................................ 4 PS5.3/ST6.4 ............................................................................................................................................................................... 4 ST2.4/PS5.4 ............................................................................................................................................................................... 6 Tuesday, 24 April ......................................................................................................................................................................