Design of a Science Operations Centre for the ExoMars 2016 Trace Gas Orbiter Mission A. Cardesin Moinelo, D. Frew, L. Metcalfe, P. Martin, N. Manaud, A.

Slides:



Advertisements
Similar presentations
1 Location of Partners and customers Who are our customers? MSSL Centre for Process engineering European Space Agency JOANNEUM RESEARCH Swedish Research.
Advertisements

The BepiColombo Mission
Overview of the Data Archive Plan by Luc Joudrier & Dave Heather
World Meteorological Organization Working together in weather, climate and water WMO OMM WMO Inventory & Evaluation of Space-based Instruments:
Michel Denis, ExoMars Ground Segment Manager, HSO-OPM
Modern Exploration Global Surveyor.  Objectives:  High resolution imaging of the surface  Study the topography and gravity  Study the role of water.
Polar Highly Elliptical / Molniya Orbit Science (PHEMOS) Mission Phase 0/A Studies Mid-Term Review Meetings January 12-14th, 2011.
The Lunar Reconnaissance Orbiter (LRO) is the first mission in NASA's Vision for Space Exploration, a plan to return to the moon and then to travel to.
Turin. ALTEC. ExoMars Progress Report ExoMars Science Working Team
1 Briefing to the CAA on the Terrestrial Planet Finder (TPF): Finding and Characterizing Earth-like Planets Zlatan Tsvetanov, NASA Program Scientist Charles.
ESA SSA SWE element status and near future plans 7th European Space Weather Week November, Brugge, Belgium Juha-Pekka Luntama Space Weather.
Astronomical GRID Applications at ESAC Science Archives and Computer Engineering Unit Science Operations Department ESA/ESAC.
System Design/Implementation and Support for Build 2 PDS Management Council Face-to-Face Mountain View, CA Nov 30 - Dec 1, 2011 Sean Hardman.
The Pursuit for Efficient S/C Design The Stanford Small Sat Challenge: –Learn system engineering processes –Design, build, test, and fly a CubeSat project.
“ PHOBOS - SOIL ” Phobos Sample Return Mission 1. goals, methods of study A.Zakharov, Russian academy of sciences Russian aviation.
All rights reserved © Altec ExoMars 2018 Rover Operations Control Centre Available Tools for planning and Data Processing I. Musso.
Hunt for Molecules, Paris, 2005-Sep-20 Software Development for ALMA Robert LUCAS IRAM Grenoble France.
Rational Unified Process Fundamentals Module 4: Disciplines II.
SOPS: The Science Operations Planning System for the first ESA Lunar Mission SMART-1.
NASA’s Goddard Space Flight Center LRO Operations Concept Richard Saylor Jr. HTSI/Code 444 August 16-17, 2005.
Presentation EddiCam consortium, FF, Madrid 13/06/2002 Eddington programmatic status Fully approved by SPC as part of ESA’s science program as project.
Cubesats A spacecraft concept to provide advances in international cooperation From: Doug Rowland, NASA GSFC Alexi Glover, ESA.
MASSACHUSETTS INSTITUTE OF TECHNOLOGY NASA GODDARD SPACE FLIGHT CENTER ORBITAL SCIENCES CORPORATION NASA AMES RESEARCH CENTER SPACE TELESCOPE SCIENCE INSTITUTE.
SGS: Activities and Requests Helen Middleton. Hermean Environment Working Group Meeting | SGS Team | Key Largo | 16/05/2013 | Slide 2 Contents 1.ESAC.
Mars 2020 Project Matt Wallace Deputy Project Manager August 3, 2015.
CAPACITY Operational Atmospheric Chemistry Monitoring Missions CAPACITY Final Meeting - WP Ground Segment synthesis Final Meeting ESTEC02/06/05.
The Solar System Chapter 6 COPY DOWN THE LEARNING GOALS ON PG SKIP 5 LINES BETWEEN EACH!
DOC-TAS-EN-002 ALTEC Auditorium - Torino - Italy December 9-10, 2014 Bruno MUSETTI ESWT#7 – ESWT#7.
.1 RESEARCH & TECHNOLOGY DEVELOPMENT CENTER SYSTEM AND INFORMATION SCIENCES JHU/MIT Proprietary Titan MESSENGER Autonomy Experiment.
Jay H. Grinstead Aerothermodynamics Branch, NASA Ames Research Center Airborne Observation of NEO/Asteroid Entries – Rapid Response Capability Airborne.
All rights reserved © Altec ExoMars 2018 Rover Operations Control Centre Planned Organization of ROCC Operations I. Musso.
NMP EO-1 TECHNOLOGY WORKSHOP Section 2 Meeting Objectives.
Planetary Motion By Carol Greco. Why do planets move the around the sun the way they do? First you need to understand that scientists have discovered.
Consortium Meeting La Palma October PV-Phase & Calibration Plans Sarah Leeks 1 SPIRE Consortium Meeting La Palma, Oct. 1 – PV Phase and.
ESWT # Rover operations concept
PDS Geosciences Node Page 1 Archiving Mars Mission Data Sets with the Planetary Data System Report to MEPAG Edward A. Guinness Dept. of Earth and Planetary.
JAXA’s Exploration of the Solar System Beyond the Moon and Mars.
US BENEFITS. It Addresses Priorities The US and Canada have common scientific, economic and strategic interests in arctic observing: marine and air transportation.
Oct.10, 2007EAMA7 The next-generation Infrared astronomy mission SPICA Outline of SPICA Scientific Research Concept (SciReC) SPICA 研究コンセプト概要 17 th May.
1 Mission Discussion & Project Reviews 祝飛鴻 10/14/93.
Planetary Science Archive PSA User Group Meeting #1 PSA UG #1  July 2 - 3, 2013  ESAC PSA Introduction / Context.
EUM/SAF/VWG/02/0010, Rev. 3, May 2003 Page 1 The SAF Network Concept and Status Juha-Pekka Luntama, EUMETSAT GRAS Mission Scientist
Diane E. Wickland NPP Program Scientist NPP Science: HQ Perspective on VIIRS May 18, 2011.
Navigation and Ancillary Information Facility NIF Introduction to WebGeocalc October 2014 SPICE components and services are not restricted under ITAR and.
All rights reserved © Altec ExoMars 2018 Rover Operations Control Centre Science instruments data pipeline G. Martucci.
Dr. Richard R. Vondrak Director, Robotic Lunar Exploration Program Science Mission Directorate NASA Headquarters September 2004 NASA Robotic Lunar Exploration.
By: Kiana Gathers. Objectives  To study the climate, the planet’s structure, its geology, and to search for traces of water.  To take global surveys.
Godwin and Cole. Mission Objectives  To determine the composition and geology of the planet’s surface  To detect evidence for water and ice  Study.
Solar Probe Plus A NASA Mission to Touch the Sun March 2015 Instrument Suite Name Presenter's Name.
Aquarius Mission Simulation A realistic simulation is essential for mission readiness preparations This requires the ability to produce realistic data,
Interlude  Viking mission operations ended in the early 1980s  Viking missions gave scientists the most complete picture of Mars to date. What does this.
LRO SRR LRO Mission Overview.
Solar System Division DVK, 10 Jul 2001 Rosetta Science Operations Experimenter to RSOC interfaces Detlef Koschny Space Science Department ESA/ESTEC
Background  EM16 SGS+TEC met with FD 1 year ago  Both sides agreed that there was a “performance gap:  SGS prepared a TN with 2 main options to bridge.
Zou Ziming 1 Ma Wenzhen Li Lei Zhao Hua Wang Chi 1: Center for Space Science and Applied Research Chinese Academy of Sciences Moscow ·
ESA UNCLASSIFIED – For Official Use HSO-OP - Solar and Planetary Missions Division Solar Orbiter Instrument Operations, Data Handling and FDIR Ignacio.
Project Introduction Spring InSPIRESS Challenge 2 Design an autonomous science payload for the Titan Environmental and Atmospheric Measurement (TEAM)
SwCDR (Peer) Review 1 UCB MAVEN Particles and Fields Flight Software Critical Design Review Peter R. Harvey.
Workshop proposal to ISSI Quantifying the Martian Geochemical reservoirs.
Exploitation of ISS Scientific data EGI-Aparsen Workshop March Science Park– Amsterdam – The Netherlands Cooperative ISS Research data Conservation.
Instrument Teams to SOC Test Specifications
Charles Acton NAIF Manager JPL July 18, 2007
ROCC Operations and The PSA RSP Archive Concept Review 28 September 2017 Tanya Lim Archive Scientist.
PDS4 Data From The Rover RSP Archive Concept Review 28 September 2017
SPICE, el servicio de información geométrica para ciencias planetarias
Mars Swingby (MSB) information
Detlef Koschny Research and Scientific Support Department ESA/ESTEC
ExoMars RSP Science Archive Concept Review [an informal non-corporate Workshop] 28 September 2017 Leo Metcalfe Science Operations Development Manager.
The RSP Archive System RSP Archive Concept Review 28 September 2017
Project Introduction Spring 2017.
Presentation transcript:

Design of a Science Operations Centre for the ExoMars 2016 Trace Gas Orbiter Mission A. Cardesin Moinelo, D. Frew, L. Metcalfe, P. Martin, N. Manaud, A. Villacorta, J. Brumfitt (1) and O. Witasse (2) (1) ESA-ESAC, European Space Astronomy Centre, Villanueva de la Cañada, Madrid, Spain (2) ESA-ESTEC, European Space Research Centre, Norwijk, The Netherlands Introduction Abstract This contribution describes the design of the Science Operations Centre being developed at the European Space and Astronomy Centre (ESAC) for the ExoMars 2016 Trace Gas Orbiter mission. This technical contribution describes the assumptions and design decisions that have been taken in order to meet all the scientific requirements of the mission considering the tight schedule imposed by the launch date in early In order to meet all the requirements, the system design takes advantage of the existing expertise and the tools available from previous planetary missions, which will serve as a solid starting point for the development of the core critical elements of the science operations uplink system. Additionally the system design is taking advantage of the collaboration with other development frameworks existing at ESAC for future planetary missions and the further support obtained by the Russian collaboration establishing synergies and improving the baseline core system with advanced state-of-the-art techniques and methods. Uplink System ExoMars 2016 Ground Segment ExoMars 2016 Mission The first mission of the ExoMars programme consists of a Trace Gas Orbiter plus an Entry, Descent and Landing Demonstrator Module (EDM) that will be launched together in January 2016 on a Proton rocket and will fly to Mars in a mated configuration scheduled for arrival after a 9-month cruise phase. Three days before reaching the atmosphere of Mars, the EDM will be ejected from the Orbiter entering the Martian atmosphere and landing on the surface of the planet. The ExoMars Trace Gas Orbiter will be inserted into an elliptical orbit around Mars and then sweep through the atmosphere during a long aerobraking phase of several months to finally settle into a circular, ~400km altitude orbit ready to conduct its scientific mission starting in late The main objectives of this mission are to search for evidence of trace atmospheric gases that could be signatures of active biological or geological processes and to test key technologies in preparation for ESA's contribution to subsequent missions to Mars. The Trace Gas Orbiter will also serve as a data relay asset for the 2018 rover mission of the ExoMars programme until the end of SegmentStakeholderInterface Science Management Project Scientist Science management and main interface to principal investigators  Assessment and approval of science plans Science Working Team  Definition, refinement and categorization of science goals  Identification of contributing observations MOC Mission Operations Centre Data Systems  Distribution of science and housekeeping telemetry  Distribution of auxiliary data products Mission Planning  Validation of payload operations timelines  Implementation of spacecraft timelines  Spacecraft-ground communication schedules  Generation of time correlation information  Provision of spacecraft and ground system configuration Flight Dynamics  Validation of spacecraft attitude timelines  Implementation of spacecraft trajectory and orientation.  Production of spacecraft auxiliary data products  Provision of spacecraft trajectory and attitude rules and constraints SGS Science Ground Segment Instrument Team Payload operation and achievement of science objectives:  Definition of science observations  Refinement of science observation timelines  Handling and archiving of science products Science Archives Team  Long term archiving of science data  Dissemination of science data products to science community Russian SOC (NNK)  Visibility of Science Operations Uplink system  Support to downlink system on instrument data handling  Replication of Deep Science Archive SystemFunctionalityMain Capabilities Uplink Opportunity Analysis  Definition of the contributing observation conditions with expert instrument team support  Calculation of science opportunities defined by geometrical and operational conditions  Analysis of opportunity events based on contextual geometrical and operational information. Scheduling and Planning  Support the science working team and the instrument teams in the preparation of the science plans.  Scheduling of the science observations timeline, assigning times for each observation operation.  Definition of the detailed observation timelines, including instrument pointing, operations and resource profiles. Plan Simulation  Simulation of the operations plan for the payload and spacecraft models.  Computation of all geometry parameters, operational timeline and resource profiles. Plan Validation  Validation of the operations plan within all payload and spacecraft constraints.  Validation of all geometrical, operational and resource checks. Product Generation  Generate all operational products for the Long/Medium/Short Term Planning for iteration with the PI teams  Export of the observation timeline into MOC compatible request formats (POR/PTR) Auxiliary Data Conversion  Convert SOC planning products and MOC products to SPICE format  Make auxiliary spacecraft data available to the instrument teams in SPICE format Operations Data Management  Configuration and management of observation definitions and plans  Configuration and management of instrument and spacecraft models  Configuration and management of system constraints and settings  Validation of submitted observation timelines Downlink Data Handling  Data Acquisition of science and housekeeping telemetry from the ESOC Data Dissemination System  Data Processing of the input telemetry to generate PDS4 raw science and housekeeping data products.  Data acquisition and processing of auxiliary data: Events, Out-of-Limits, TM gap reports, etc Archiving  Generation of PDS4 data bundles from PDS4 science and housekeeping data products at all processing levels.  Validation and Ingestion of PDS 4 bundle data at all data processing levels.  Validation and archiving of calibrated data delivered by PI teams Feedback* Observations Log Database  List of planned observations  Traceability of operations and data processing  Planning, execution and data processing status  Geometric, scientific and instrument performance quality control  Monitoring of science coverage goals Science Quick-Look  Quick-look visualization of science data to identify problems and issues relevant to science planning in order to allow rapid corrections or rescheduling Engineering Housekeeping Monitoring  Monitoring of engineering data to identify problems and issues relevant to science planning in order to allow rapid corrections or rescheduling TGO InstrumentScience Objectives ACS (Atmospheric Chemistry Suite) This suite of 3 infrared instruments will investigate the chemistry and structure of the Martian atmosphere. ACS will complement NOMAD by extending the coverage at infrared wavelengths, and by taking images of the Sun to better analyse the solar occultation data. CaSSIS (Colour and Stereo Surface Imaging System) A high-resolution camera (5 metres per pixel) capable of obtaining colour and stereo images over a wide swathe. CaSSIS will provide the geological and dynamical context for sources or sinks of trace gases detected by NOMAD and ACS. FREND (Fine Resolution Epithermal Neutron Detector) This neutron detector will be used to map the presence of hydrogen on the Martian surface, targeting deposits of near-surface water ice. NOMAD (Nadir and Occultation for MArs Discovery) A spectrometer suite, covering a wide range of wavelengths (including infrared to ultraviolet), to identify the components of the Martian atmosphere. Ground Segment Architecture Ground Segment Parties Science Ground Segment Top Level Design ExoMars 2016 Science Operations Centre Design SGS Data Archiving Sub-System Design SGS Data Handling: Acquisition and Processing System SGS Uplink System ArchitectureSGS Centralized Uplink Processes Downlink System *Feedback processes are considered “Optional/Enhanced Design”, and are not described here as they will not be implemented in the first stage. They are considered only here as non-critical processes that could extend the future SOC capabilities if available during the science phase of the mission. System and Sub-System Functionalities