Exomars 2016 En Route to Mars
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COPERNICUS MARITIME SURVEILLANCE SERVICE OVERVIEW Copernicus Maritime Surveillance Service
European Maritime Safety Agency COPERNICUS MARITIME SURVEILLANCE SERVICE OVERVIEW Copernicus Maritime Surveillance Service THE COPERNICUS PROGRAMME Copernicus is a European Union Programme aimed at developing European information services based on satellite Earth Observation and in situ (non-space) data analyses. The programme is managed by the European Commission, and implemented in partnership with the member states and other organisations, including the European Maritime Safety Agency (EMSA). Copernicus is served by a set of dedicated satellites (the Sentinels) and contributing missions (existing commercial and public satellites). Copernicus services address six main thematic areas: Security; Land Monitoring; Marine Monitoring; Atmosphere Monitoring; Emergency Management; and Climate Change. THE SECURITY SERVICE The Copernicus Security Service supports EU policy by providing information in response to Europe’s security challenges. It improves crisis prevention, preparedness and response in three key areas: maritime surveillance (implemented by EMSA) border surveillance support to EU External Action The Copernicus service for security applications is distinct from other services in the Copernicus programme. Data obtained directly through the Copernicus programme is combined with data from other sources, which may be sensitive or restricted. The end services are then provided directly to authorised national administrations and to a limited number of EU institutions and bodies, in accordance with their access rights. European Maritime Safety Agency THE COPERNICUS MARITIME SURVEILLANCE SERVICE The Copernicus Maritime Surveillance Service supports improved monitoring of activities at sea. The goal of the Copernicus Maritime Surveillance Service, implemented by EMSA, is to support its users by providing a better understanding and improved monitoring of activities at sea that have an impact on areas such as: fisheries control maritime safety and security law enforcement marine environment (pollution monitoring) support to international organisations. -
Argops) Solution to the 2017 Astrodynamics Specialist Conference Student Competition
AAS 17-621 THE ASTRODYNAMICS RESEARCH GROUP OF PENN STATE (ARGOPS) SOLUTION TO THE 2017 ASTRODYNAMICS SPECIALIST CONFERENCE STUDENT COMPETITION Jason A. Reiter,* Davide Conte,1 Andrew M. Goodyear,* Ghanghoon Paik,* Guanwei. He,* Peter C. Scarcella,* Mollik Nayyar,* Matthew J. Shaw* We present the methods and results of the Astrodynamics Research Group of Penn State (ARGoPS) team in the 2017 Astrodynamics Specialist Conference Student Competition. A mission (named Minerva) was designed to investigate Asteroid (469219) 2016 HO3 in order to determine its mass and volume and to map and characterize its surface. This data would prove useful in determining the necessity and usefulness of future missions to the asteroid. The mission was designed such that a balance between cost and maximizing objectives was found. INTRODUCTION Asteroid (469219) 2016 HO3 was discovered recently and has yet to be explored. It lies in a quasi-orbit about the Earth such that it will follow the Earth around the Sun for at least the next several hundred years providing many opportunities for relatively low-cost missions to the body. Not much is known about 2016 HO3 except a general size range, but its close proximity to Earth makes a scientific mission more feasible than other near-Earth objects. A Request For Proposal (RFP) was provided to university teams searching for cost-efficient mission design solutions to assist in the characterization of the asteroid and the assessment of its potential for future, more in-depth missions and possible resource utilization. The RFP provides constraints on launch mass, bus size as well as other mission architecture decisions, and sets goals for scientific mapping and characterization. -
CNES Miniaturization Policy: an Answer to Nanosatellites Challenges
SSC19-I-02 CNES miniaturization policy: an answer to Nanosatellites challenges C. Dudal, C. Laporte, T. Floriant, P. Lafabrie CNES 18, avenue Edouard Belin 31401 Toulouse Cedex 9, France; +33561283070 [email protected] ABSTRACT The reduction of mass and size with improvement of the performance of a device is a permanent challenge for the space industry. The French National Space Agency has funded hundreds of R&D activities in the past, in all dedicated technical areas to facilitate these kind of technological evolution. Miniaturization efforts have, more recently, encountered a growing field of application, the one of Nanosatellites. For these applications, performance/cost trade-off is largely dominated by full cost, that is to say the cost including the entire satellite system development, from the initial idea to the end of life, including operations, data processing and its distribution. The carried out trade-offs are therefore based on a different constraints environment, in which the risk variable is systematically re-evaluated considering the cost/performance couple; the methods, the development process and the planning of delivery being directly impacted by this challenge. In this logic, and while continuing its efforts to miniaturize and improve performance for conventional markets (Earth observation, science, telecommunications, ...), CNES has adapted its working environment around the Nanosats domain to accelerate the development of adapted solutions. This adaptation being made both in terms of new development processes and of use of new COTS technology for equipment themselves. Moreover, projects in New Space are changing the historical relationship between CNES and its industrial partners and are encouraging a transition from a client/provider approach to a more co-partners approach. -
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. -
Exploration of Mars by the European Space Agency 1
Exploration of Mars by the European Space Agency Alejandro Cardesín ESA Science Operations Mars Express, ExoMars 2016 IAC Winter School, November 20161 Credit: MEX/HRSC History of Missions to Mars Mars Exploration nowadays… 2000‐2010 2011 2013/14 2016 2018 2020 future … Mars Express MAVEN (ESA) TGO Future ESA (ESA- Studies… RUSSIA) Odyssey MRO Mars Phobos- Sample Grunt Return? (RUSSIA) MOM Schiaparelli ExoMars 2020 Phoenix (ESA-RUSSIA) Opportunity MSL Curiosity Mars Insight 2020 Spirit The data/information contained herein has been reviewed and approved for release by JPL Export Administration on the basis that this document contains no export‐controlled information. Mars Express 2003-2016 … First European Mission to orbit another Planet! First mission of the “Rosetta family” Up and running since 2003 Credit: MEX/HRSC First European Mission to orbit another Planet First European attempt to land on another Planet Original mission concept Credit: MEX/HRSC December 2003: Mars Express Lander Release and Orbit Insertion Collission trajectory Bye bye Beagle 2! Last picture Lander after release, release taken by VMC camera Insertion 19/12/2003 8:33 trajectory Credit: MEX/HRSC Beagle 2 was found in January 2015 ! Only 6km away from landing site OK Open petals indicate soft landing OK Antenna remained covered Lessons learned: comms at all time! Credit: MEX/HRSC Mars Express: so many missions at once Mars Mission Phobos Mission Relay Mission Credit: MEX/HRSC Mars Express science investigations Martian Moons: Phobos & Deimos: Ionosphere, surface, -
Range Resolution Enhancement of WISDOM/Exomars
Range resolution enhancement of WISDOM/ExoMars radar soundings by the Bandwidth Extrapolation technique: Validation and application to field campaign measurements Nicolas Oudart, Valérie Ciarletti, Alice Le Gall, Marco Mastrogiuseppe, Yann Herve, Wolf-Stefan Benedix, Dirk Plettemeier, Vivien Tranier, Rafik Hassen-Khodja, Christoph Statz, et al. To cite this version: Nicolas Oudart, Valérie Ciarletti, Alice Le Gall, Marco Mastrogiuseppe, Yann Herve, et al.. Range resolution enhancement of WISDOM/ExoMars radar soundings by the Bandwidth Extrapolation tech- nique: Validation and application to field campaign measurements. Planetary and Space Science, Elsevier, 2021, 197 (March), pp.105173. 10.1016/j.pss.2021.105173. insu-03114236v2 HAL Id: insu-03114236 https://hal-insu.archives-ouvertes.fr/insu-03114236v2 Submitted on 28 Jan 2021 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 Planetary and Space Science 197 (2021) 105173 Contents lists available at ScienceDirect Planetary -
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. -
European Space Agency and CNES Endorse Expansion of Kayrros Methane Detection Technology with New €2.4 Million Contract
European Space Agency and CNES endorse expansion of Kayrros methane detection technology with new €2.4 million contract New funding from ESA Space Solutions – with support from the Centre National d’Études Spatiales – extends geographical coverage, adds data sources and boosts field operations. Paris, 31 March 2021 — Kayrros, the leading advanced data analytics company focused on satellite imagery and alternative data for more-timely decision making, announced today that it has received a contract of €2.4 million from the European Space Agency (ESA), an initiative supported by the Centre National d’Études Spatiales (CNES). Kayrros and ESA began their collaboration in early 2020 on the basis of Kayrros’ use of Sentinel-5P data, after working closely with CNES on the project since 2019. This contract will supplement Kayrros’ own fundraising to invest in the company’s breakthrough Methane Watch technology, bringing the total investment to €5 million. Methane is the second-largest driver of global warming after carbon dioxide and Kayrros Methane Watch is the first commercially available geospatial technology to detect, measure and attribute methane leaks to their sources worldwide. The technology: - Combines data from different ESA Sentinel satellite sensors within the Copernicus constellation. - Allows energy stakeholders and industry asset owners to take action on methane emissions using near-real time measurements and rapid processing on the world-leading Kayrros global asset observation platform. - Has already revealed dramatic increases in large methane leaks around the world and exposed significantly different regional trends likely due to activity changes, operational practices and infrastructure issues. The contract provided by ESA is for a targeted collaboration between Kayrros and ESA’s Space Solutions’ Business Applications program. -
Supporting the Sustainable Development Goals
UNITED NATIONS OFFICE FOR OUTER SPACE AFFAIRS European Global Navigation Satellite System and Copernicus: Supporting the Sustainable Development Goals BUILDING BLOCKS TOWARDS THE 2030 AGENDA UNITED NATIONS Cover photo: ©ESA/ATG medialab. Adapted by the European GNSS Agency, contains modified Copernicus Sentinel data (2017), processed by ESA, CC BY-SA 3.0 IGO OFFICE FOR OUTER SPACE AFFAIRS UNITED NATIONS OFFICE AT VIENNA European Global Navigation Satellite System and Copernicus: Supporting the Sustainable Development Goals BUILDING BLOCKS TOWARDS THE 2030 AGENDA UNITED NATIONS Vienna, 2018 ST/SPACE/71 © United Nations, January 2018. All rights reserved. The designations employed and the presentation of material in this publication do not imply the expression of any opinion whatsoever on the part of the Secretariat of the United Nations concern- ing the legal status of any country, territory, city or area, or of its authorities, or concerning the delimitation of its frontiers or boundaries. Information on uniform resource locators and links to Internet sites contained in the present pub- lication are provided for the convenience of the reader and are correct at the time of issue. The United Nations takes no responsibility for the continued accuracy of that information or for the content of any external website. This publication has not been formally edited. Publishing production: English, Publishing and Library Section, United Nations Office at Vienna. Foreword by the Director of the Office for Outer Space Affairs The 2030 Agenda for Sustainable Development came into effect on 1 January 2016. The Agenda is anchored around 17 Sustainable Development Goals (SDGs), which set the targets to be fulfilled by all governments by 2030. -
EXM Mobility Paper
OVERVIEW AND DEVELOPMENT STATUS OF THE EXOMARS ROVER MOBILITY SUBSYSTEM P.Poulakis (1), J.L.Vago(1), D.Loizeau(6), C.Vicente-Arevalo(5), A.Hutton(3), R.McCoubrey (4), J.Arnedo-Rodriguez(5), (3) (3) (4) (5) (1) (1) (1) (1) (1) J.Smith , B.Boyes , S.Jessen , A.Otero-Rubio , S.Durrant , G.Gould , L.Joudrier , Y.Yushtein , C.Alary , (1) (1) (2) (2) (2) (2) E.Zekri , P.Baglioni , A.Cernusco , F.Maggioni , R.Yague , F.Ravera (1)European Space Agency / ESTEC, The Netherlands (2) Thales Alenia Space Italy, Italy (3) Airbus Defence & Space, UK (4) MDA, Canada (5) Thales Alenia Space España, Spain (6) University of Lyon, France ABSTRACT planned for launch in 2018, features a decent module, which will deliver a rover and a static lander platform to The ExoMars 2018 rover mission will carry an ambi- the surface on Mars. tious payload to search for biosignatures that may pro- vide clues to whether life ever started on Mars. It will be If life ever arose on the red planet, it probably did when the first time that depth, the third dimension of Mars, Mars was warmer and wetter, sometime within the first will be explored using a sophisticated drill system that few billion years following planetary formation. Condi- will allow access to the Martian subsurface down to 2m. tions then were similar to those on Earth when microbes In that context, the rover’s mobility subsystem will be gained a foothold on our young planet. The ExoMars instrumental to reach locations with high scientific po- rover will search for two types of life-related signatures: tential. -
Caesar, French Probative Public Service for In-Orbit Collision Avoidance
CAESAR, FRENCH PROBATIVE PUBLIC SERVICE FOR IN-ORBIT COLLISION AVOIDANCE François LAPORTE(1), Monique MOURY(1) (1) CNES DCT/OP/MO, 18 av. Edouard Belin, 31401 Toulouse cedex 9, France, Email : [email protected]; [email protected] ABSTRACT 2 CONJUNCTION ASSESSMENT WITH CSMs This paper starts by describing the conjunction analysis which has to be performed using CSM data provided by Conjunction Summary Messages (CSM) are real JSpOC. This description not only demonstrates that satellite protection provided by JSpOC for all active Collision Avoidance is a 2-step process (close approach satellites. They are made available on Emergency detection followed by risk evaluation for collision Criteria which are Time of Closest Approach (TCA) avoidance decision) but also leads to the conclusion that within 72 hours combined with for Low Earth Orbit there is a need for Middle Man role. (LEO) overall miss distance lower than 1km with radial miss distance lower than 200m and for higher orbits After describing the Middle Man concept, it introduces (GEO and MEO) overall miss distance lower than the French response CAESAR and the need for 10km. CSMs include: identification of the 2 objects, collaborative work environment which is implied by TCA and for each object position, velocity, dispersion Middle Man concept. It includes a description of the and some orbit determination characteristics. environment put in place for CAESAR (secure website Nevertheless, they are advisory and informational and dedicated tools), the content of the service, the messages only and are not directly actionable: they condition for the distribution of the CNES software JAC don’t provide a direct recommendation to perform an and the advantages for subscribers. -
The CONSERT Operations Planning Process for the Rosetta Mission
SpaceOps Conferences 10.2514/6.2018-2687 28 May - 1 June 2018, Marseille, France 2018 SpaceOps Conference The CONSERT operations planning process for the Rosetta mission Y. Rogez1, P. Puget2, S. Zine3, A. Hérique4, W. Kofman5 Univ. Grenoble Alpes, CNRS, CNES, IPAG, F-38000 Grenoble, France N. Altobelli6, M. Ashman7, M. Barthelemy8, M. Costa Sitjà9, B. Geiger10, B. Grieger11, R. Hoofs12, M. Küppers13, L. O’Rourke14, C. Vallat15 European Space Astronomy Centre/European Space Agency, PO. Box 78, 28691 Villanueva de la Cañada, Spain J. Biele16, C. Fantinati17, K. Geurts18, M. Maibaum19, B. Pätz20, S. Ulamec21 Deutsches Zentrum für Luft und Raumfahrt. DLR-RB/MUSC, 51147 Köln, Germany A. Blazquez22, C. Delmas23, J.-F. Fronton24, E. Jurado25, A. Moussi26 Centre National d'Etudes Spatiales (CNES), 18 av. E. Belin, 31401 Toulouse, France C.M. Casas27, A. Hubault28, P. Muñoz29 European Space Operation Centre/European Space Agency, Germany ESOC/ESA, Germany and 1 CONSERT Operation Engineer, Radar group 2 CONSERT Project Manager, Radar group 3 CONSERT Scientist, Planeto team, Radar group 4 CONSERT Principal Investigator, Planeto team, Radar group 5 CONSERT Principal Investigator until 2018, Planeto team, Radar group 6 Rosetta Scientist, RSGS 7 Rosetta Science Operations Engineer, RSGS 8 Rosetta Archive and Liaison Scientist, RSGS 9 SPICE and Auxiliary Data Support Engineer, RSGS 10 Rosetta Liaison Scientist, RSGS 11 Rosetta Trajectory Design Scientist, RSGS 12 Rosetta Science Operations Advisor, RSGS 13 Rosetta Scientist, RSGS 14 Rosetta Downlink