European Space Agency is opening the doors to Slovenia Ljubljana, 31 Mar 2010 1 ESA Future Projects and Missions Opportunity for Slovenia Marcos Bavdaz.

Slides:



Advertisements
Similar presentations
THESIS – the Terrestrial and Habitable-zone Exoplanet Spectroscopy Infrared Spacecraft a concept for a joint NASA/ESA exoplanet characterization mission.
Advertisements

EUCLID : From Dark Energy to Earth mass planets and beyond Jean-Philippe Beaulieu Institut dAstrophysique de Paris Dave Bennett University of Notre Dame.
ATHENA WFI Meeting Garching, January 28, 2014 Markus Plattner.
AXSIO: The Advanced X-ray Spectroscopic Imaging Observatory AXSIO Jay Bookbinder, Randall Smith On behalf of the AXSIO Team.
ATHENA: The Advanced Telescope for High Energy Astrophysics
The Mercury Imaging X-ray Spectrometer (MIXS): Lessons learned for the ATHENA Wide Field Imager (WFI) GW Fraser, A Martindale and C Thomas Space Research.
PLATO Phase A/B1 Status TOU Meeting Catania 28 Feb 2011 PLAnetary Transits and Oscillation of stars.
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.
Australian Centre for Space Photonics Andrew McGrath Anglo-Australian Observatory.
1 Briefing to the CAA on the Terrestrial Planet Finder (TPF): Finding and Characterizing Earth-like Planets Zlatan Tsvetanov, NASA Program Scientist Charles.
Millimetron mision sensitivities and instrumentation concept
PLATO kick-off meeting 09-Nov-2010 PLATO Payload overall architecture.
1.B – Solar Dynamo 1.C – Global Circulation 1.D – Irradiance Sources 1.H – Far-side Imaging 1.F – Solar Subsurface Weather 1.E – Coronal Magnetic Field.
PLAnetary Transits and Oscillations of stars Thierry Appourchaux for the PLATO Consortium
SDW2005, juin, Taormina The Corot Space instrument.
The Universe in the Infrared What is the Spitzer Space Telescope, and how does it work? Funded by NASA’s Spitzer Science Center Images courtesy NASA/JPL.
Athena – Advanced Telescope for High Energy Astrophysics ATHENA: The Advanced Telescope for High Energy Astrophysics Nicholas E. White, NASA/GSFC On behalf.
Final Version Wes Ousley Dan Nguyen May 13-17, 2002 Micro-Arcsecond Imaging Mission, Pathfinder (MAXIM-PF) Thermal.
1L. Piro – IXO – Polarimetry Workshop, Oct Luigi Piro IXO Coordination Group.
X-ray Timing and Polarization mission & instrumentation DONG Yongwei Center for Particle Astrophysics Institute of High Energy Physics, Chinese Academy.
Advanced Concepts & Science Payloads Office Eddicam/EST MeetingPage 1 CCD Procurement Schedule driven Review off-the shelf availability Specific mode of.
Presentation EddiCam consortium, FF, Madrid 13/06/2002 Eddington programmatic status Fully approved by SPC as part of ESA’s science program as project.
JAXA’s Space Exploration Scenario for the Next Twenty Years - Science Strategy - Masato Nakamura Steering Committee of Space Science Institute of Space.
Harvey Tananbaum Director Chandra X-ray Center Harvard-Smithsonian Center for Astrophysics 13th HEAD Meeting April 8, 2013 Building International Space.
FIRST/Planck 12 December 2000PT The FIRST Mission Implementation Status and Schedule T. Passvogel The Promise of FIRST.
A Search for Earth-size Planets Borucki – Page 1 Roger Hunter (Ames Research Center) & Kepler Team March 26, 2010.
NMP EO-1 TECHNOLOGY WORKSHOP Section 2 Meeting Objectives.
1 Science and Robotic Exploration (SRE) ESA’s planetary probes 10 th International Planetary Probe Workshop David Agnolon & Peter Falkner, Solar System.
Space Research Centre EDDICAM Interests in EDDINGTON Professor Alan Wells and Dr Matthew Burleigh Space Research Centre, University of Leicester.
Jenam 2010 Exoplanet Targets for Upcoming Cosmic Visions Space Missions James Frith September 8 th 2010 University of Hertfordshire.
China National Report , Uppsala, Sweden China National Space Administration.
Key Ideas Describe characteristics of the universe in terms of time, distance, and organization. Identify the visible and nonvisible parts of the electromagnetic.
The ESA Science Program for the progress of European society Luigi Colangeli Head, ESA Solar System Missions Division and Coordinator, ESA Solar System.
XEUS  Science /Configuration Status Global Collaboration Aim of this meeting Johan Bleeker, 26 October 2004.
DARWIN The InfraRed Space Interferometer. Status of exo-planet search Stars (Solar type) observed: Planets detected: ~ 86 Radial velocity measurement.
Telescopes Key Words Optical Telescopes: make use of electromagnetic radiation in the range of visible light Refraction Telescopes: use lenses Reflecting.
TABLE OF CONTENTS Table of Contents: Mission Overview Timeline Scientific Objectives Spacecraft Launch Vehicle Equipment Nuclear Spectroscopic Telescope.
1. G O D D A R D S P A C E F L I G H T C E N T E R 2 New Budget Initiatives for NASA in FY04.
SE&I Pre-Proposal Meeting GSFC - JPL Systems Engineering Management Colleen McGraw.
Programs and plans ASI - Observation of the Universe.
1 Atmospheric Radiation – Lecture 17 PHY Lecture 17 Satellite instruments and missions.
Astrophysics Missions in ESA’s Cosmic Vision Program
1 System Architecture Mark Herring (Stephen Merkowitz Presenting)
2 Jun 2022 Jan 2030 Sep 2032 Jun months 1 month 9 months 11 months 9 months Launch Ariane-5 Jupiter orbit insertion Transfer to Callisto Europa.
1 Transiting Exoplanet Survey Satellite Daryl Swade Archive Team Meeting June 16, 2014.
1 Nicholas White NASA Project Scientist Goddard Space Flight Center.
Science investigations in the framework of expedition to Europa
KEPLER TABLE OF CONTENTS Table of Contents: Mission Overview Scientific Objectives Timeline Spacecraft Target Field of View Transit Method Johannes Kepler.
CSRP NASA Workshop NASA’s Revised Budget. CSRP NASA Workshop NASA’s New Vision and Objectives (as of January 14, 2004)  VISION  The fundamental goal.
24 JANUARY 2007BASICS OF INTERPLANETARY SPACE FLIGHT ONLINE DD- 1 Dave Doody CASSINI REALTIME OPERATIONS Basics of Interplanetary Flight.
1 June 10, 2004 Gary L. Wentz, Jr. Deputy Manager, MSFC Office of Exploration Systems MSFC Office for Exploration Systems.
MPI Semiconductor Laboratory, The XEUS Instrument Working Group, PNSensor The X-ray Evolving-Universe Spectroscopy (XEUS) mission is under study by the.
V - 1 V. System Technology for Large Space Telescopes Session Chair: Juan A. Roman.
Lunar Surface Atmosphere Spectrometer (LSAS) Objectives: The instrument LSAS is designed to study the composition and structure of the Lunar atmosphere.
Ares V an Enabling Capability for Future Space Science Missions H. Philip Stahl, Ph.D. NASA MSFC.
ESA UNCLASSIFIED – For Official Use FISO COLLOQUIUM, 18 June 2014 B. HUFENBACH ESA’S SPACE EXPLORATION STRATEGY.
© 2015 albert-learning.com Cosmic. © 2015 albert-learning.com Cosmic The Cosmic Vision is the paraphrasing name given to the roadmap for scientific space.
Il programma NHXM sviluppato dall'ASI Ing. Mauro Piermaria New Hard X-Ray Mission Workshop Nazionale 12 e 13 novembre 2009 – ASDC, Frascati.
ASI Science Programme Barbara Negri - Italian Space Agency (ASI) Head of Exploration and Observation of the Universe Department 10 Years of PAMELA.
National Goals and Objectives
JUpiter Icy Moons Explorer (JUICE)
Adam Schlesinger NASA – JSC November 3, 2011
THE EUROPEAN SPACE AGENCY
Upcoming Facilities of IIA
Fast Facts Innovative deployable systems, structures, and solar arrays for spacecraft applications State-of-the-art products that draw on years of flight.
Adam Schlesinger NASA – JSC November 3, 2011
Systems Engineering Management
Launch and On-orbit Checkout
Observational Prospect of NIREBL
CHEOPS - CHaracterizing ExOPlanet Satellite
Presentation transcript:

European Space Agency is opening the doors to Slovenia Ljubljana, 31 Mar ESA Future Projects and Missions Opportunity for Slovenia Marcos Bavdaz Head of Advanced Technologies Section Science and Robotic Exploration Projects Department

European Space Agency is opening the doors to Slovenia Ljubljana, 31 Mar Four Questions: What are the conditions for life and planetary formation? How does the Solar System work? What are the fundamental laws of the Universe? How did the Universe begin and what is it made of?

European Space Agency is opening the doors to Slovenia Ljubljana, 31 Mar Cosmic Vision timeline summary L-class missions M-class missions Laplace Tandem Lisa IXO 2012 L1 launch Euclid Plato Cross-Scale Marco-Polo M1 launch Solar Orbiter Spica M2 launch Solar Orbiter Spica TBD Plato Euclid Laplace

European Space Agency is opening the doors to Slovenia Ljubljana, 31 Mar Mission Phases First slice of Cosmic Vision Plan: Three M-Class in definition and three L-Class missions in assessment Assessment PhaseDefinition PhaseImplementation Phase ≥ 2 years ~ 5-6 years Mission selection Down-selection & Payload AO Mission adoption Launch Assessment studies Phase 0/A Design consolidation & pre-developments Phase A/B1 Development Phase B2/C/D n missions two missions one mission ESA / Member States agreements LOEMLA Spacecraft And Payload activities more on cosmic vision:

European Space Agency is opening the doors to Slovenia Ljubljana, 31 Mar Key elements of Cosmic Vision implementation plan Spacecraft Assessment Studies ESA internal studies & industrial studies Programmatic inputs for down-selection process Science Instrument Assessment Studies National activities conducted in parallel to ESA system studies Enable robust spacecraft definition and instrument selection (AO) at the beginning of the Definition Phase Technology Preparation For spacecraft and science instruments Harmonisation with Member States required for payload related activities

European Space Agency is opening the doors to Slovenia Ljubljana, 31 Mar Technology development: programmes, project phases and risks

European Space Agency is opening the doors to Slovenia Ljubljana, 31 Mar EUCLID overview Science Objective: >10000 deg 2 sky survey to characterize dark energy and dark matter Payload:  1.2 m telescope  Visible imager (weak lensing)  Near IR photometer (weak lensing)  Near IR spectrometer (BAO)

European Space Agency is opening the doors to Slovenia Ljubljana, 31 Mar EUCLID: Key Aspects driving technology:  Large area focal planes (VIS & NIR) – state of art + radiation resistance  Exceptional requirements on PSF stability and low ellipticity (0.1 arcsec)  Step and stare sky scanning strategy – duty cycle efficiency and Line of Sight Stability Very high data rate – K band

European Space Agency is opening the doors to Slovenia Ljubljana, 31 Mar Main science objectives  To search for exoplanetary transits (occultations) in front of stars  To characterize the parent stars in terms of fundamental physical parameters via asteroseismology  Accomplished through high time-resolution, high precision, and high duty-cycle visible photometry PLATO: “PLAnetary Transits and Oscillations of stars” Mission concept:  Direct insertion into Large amplitude orbit around L2 using Souyz 2-1b LV  6 year mission, 3-axis stabilized  Multi-aperture approach to allow for large FoV  Optics and detectors (CCD) operating at cold temp. (~170K)  ~0.2” pointing and stability req. (P/L  FGS)

European Space Agency is opening the doors to Slovenia Ljubljana, 31 Mar PLATO Technology Pre-developments required: CCD prototyping  Optimized high speed, high dynamic range CCD  Multi-aperture approach: many CCDs need to be produced in short time frame Refractive telescope breadboard/EM  Bread-boarding of a 6 lens telescope, with large diameter lenses and operating at low working temperature  34 telescopes to be produced: heritage from a bread-board telescope is needed

European Space Agency is opening the doors to Slovenia Ljubljana, 31 Mar

European Space Agency is opening the doors to Slovenia Ljubljana, 31 Mar Solar Orbiter technologies:  Rely on Bepi-Colombo (Mission to the planet Mercury) technology and equipments wherever possible  Double-sided solar array based on Bepi-colombo cell technology  High flux solar testing  Heat shield  Heat rejecting filters

European Space Agency is opening the doors to Slovenia Ljubljana, 31 Mar International ESA-JAXA-NASA collaboration scheme in 2008, XEUS & Constellation X merged  International X-Ray Observatory. Main observatory requirements:  Single telescope aperture with A eff = 3 m2 at 1.25 keV (0.6 m2 at 6 keV).  Telescope HEW = 5 arcsec (0.1 to 10 keV).  DE < 2.5 eV between 0.1 and 6.5 keV.  X-ray Grating Spectrometer always illuminated (IM). Five focal plane instruments on rotating platform:  Wide Field Imager (WFI)  Hard X-ray Camera (HXI)  X-ray Imaging Spectrometer (XMS)  High Time Resolution Spectrometer (HTRS)  X-ray Polarimeter (XPOL) IXO – International X-ray Observatory European Space Agency is opening the doors to Slovenia Ljubljana, 31 Mar 2010

European Space Agency is opening the doors to Slovenia Ljubljana, 31 Mar IXO technology activities:  Low mass X-ray optics (mission enabling): Si pore optics development and validation,  Alternative optics technology using slumped glass  Cryogenic coolers (required by Narrow Field Instrument)  Deployable structure required to increase focal length (extension mechanisms, deployable shroud). National developments:  Detectors  Associated electronics  Cooling

European Space Agency is opening the doors to Slovenia Ljubljana, 31 Mar Laplace – Europa Jupiter System Mission ESA/NASA Outer Planet candidate mission  ESA: Jupiter Ganymede Orbiter (JGO), Jupiter System Science (atmosphere, magnetosphere) with focus on Callisto and Ganymede  NASA: Jupiter Europa Orbiter (JEO). Jupiter System Science with focus on Europa, Io (NASA-JEO) Space Segment (ESA, Jupiter Ganymede Orbiter (JGO))  Launch: Ariane 5 in 2020, Transfer: VEEGA-type, no deep space manoeuvre, arrival: 2026  Jupiter tour with multiple fly-bys at Callisto and Ganymede (low altitude, typ. 200 km), then (1) Callisto resonant orbit, (2) Ganymede elliptical orbit, (3) Ganymede circular orbit  Avoidance of high radiation  Solar power LILT technology, no concentrators, no RTG or RHU  Chemical propulsion Payload: ~80kg science instruments, nationally provided JGO = Jupiter Ganymede Orbiter

European Space Agency is opening the doors to Slovenia Ljubljana, 31 Mar Laplace Technology developments:  Radiation hardening and tolerance/tailored shielding, Radiation environment; 150 krad (shielded)  Improved Environmental modelling  Solar Cell Technology (LILT)

European Space Agency is opening the doors to Slovenia Ljubljana, 31 Mar LISA: Laser Interferometer Space Antenna  ESA/NASA collaboration  Measurement of gravitational wave using laser interferometry  Constellation of 3 spacecrafts separated by 5 million km Critical areas  6 drag-free test masses  micropropulsion system  interferometrically measuring variations in distance between couples of test masses at the picometre level, at 5 million km distance  LISA Pathfinder technology validation

European Space Agency is opening the doors to Slovenia Ljubljana, 31 Mar Technology required by LISA  Low-noise, high stability mechanisms (point-ahead and optical articulation)  Highly stable materials for telescope assembly (CFRP, zerodur, inserts …)  Low-noise electronic components for GRS front-end electronics (voltage references..)  Light sources for charge management discharge (LEDs, laser diodes …)  Metrology system  High-power laser system (1-2 W EOL, redundant)  Outgassing & contamination issues  Micropropulsion (lifetime characterization)

European Space Agency is opening the doors to Slovenia Ljubljana, 31 Mar MREP Mars Robotic Exploration Programme  Foreseen in collaboration with NASA  Mars Sample Return mission is taken as long term objective  Target is to contribute to each Mars mission slot (every ~2 years)  Prepare post-ExoMars missions and enable decisions at next C-Min (2012) MREP activities: 1. Technology Development  Short term: 2020 Network scenario (TRL 5 by end 2011)  Mid term: post 2020 intermediate mission (IM)  Long term: strategic and enabling technologies for European Robotic Exploration 2. Intermediate Mission Studies 3. MSR architecture studies, in collaboration with NASA/JPL

European Space Agency is opening the doors to Slovenia Ljubljana, 31 Mar Future Missions – opportunities for Slovenia Mandatory ESA Programme: Cosmic Visions 1525 Science Programme Providing a set of carefully selected missions, covering the science priorities of Europe Phased down-selection, considering scientific excellence, technological feasibility and readiness, schedule and affordability Sliced Programme, allowing regular new entries through open Call for Missions (every ~3-4 yrs), ensuring innovation European Space Agency is opening the doors to Slovenia Ljubljana, 31 Mar 2010 Early involvement facilitates later participation in flight projects Establish awareness of the programmes and mission candidates Define strategic focus of own interests Identify competitive contribution opportunities Develop relevant capabilities and establish heritage Good investment: early and focused technology preparation Identify early the technology areas of interest for Slovenia and its industry and institutions Base developments on existing expertise and solid background Ensure strategic relevance and long-term commitment Develop technologies with solid teams working with a well defined focus Build a technological heritage and develop partnerships Achievement requires Audacity!