concepts in europe - universiteit leiden · science programme • provide best space tools possible...
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Introduction
• ESAContext• NUVA• ActiveUV-relatedmissionconcepts
– Arago,ESAM4/M5,notselected– WorldSpaceObservatory(seetalkbyBorisShustov– EUVOresponsetoLargeMissioncall– ResponsetoESA2016callforideas
• EuropeinLUVOIR• Whatnext?
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ESA• 18EUstates(AT,BE,CZ,DE,
DK,ES,FI,FR,IT,GR,IE,LU,NL,PT,PL,RO,SE,UK)plusNO&CH
• Cooperation Agreements:Estonia,Slovenia,Hungary,Cyprus,Latvia,Lithuania,Malta&Slovak Republic;Bulgaria negotiating;Discussionsongoing withCroatia
• Canadatakes partinsomeprogrammesunder along-standingCooperationAgreement
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Scienceprogramme• Providebestspacetoolspossibleforscientificcommunityto
achieve&sustainexcellence,leadingtheworldwithdiscoveriesandinnovation.– Choiceofprojectsbyscientificexcellence– Selectionbycompetitioninabottom-upprocess(peerreview)– Stabilityforscientificresearchteams– Referencescienceframeworkforthecommunity,nationalagencies
andinternationalpartners• Contributetosustainabilityofspacecapabilities&infrastructuresin
Europe– Providecontinuitytoindustry– Fostertechnologicalinnovation– Attractbrightmindstospaceactivities– Provideperspectivetolaunchservicesandoperations
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Scienceprogramme
• Programmeissciencedriven– Bottom-upprocesses,relyingonbroadcommunityinput&peerreview
• Programmeismandatory– Allmemberstatescontributepro-ratatoGDP
• ESAfundsspacecraft,launcher,spacecraftoperations&partofthescienceoperations
• MemberStatesfundpayloadsandrestofscienceops.– Missionsarepartnerships
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The Networkfor UltraViolet AstronomyThe Networkfor UltraViolet Astrophysics (NUVA)is apan-european network set-upto identify the needs ofthe astronomical community inthe UVdomain andeventually propose actions to structure it around newprojects
FRANCE
SPAIN
ITALY
SWITZERLAND
THENETHERLANDS
UNITEDKINGDOM
SWEDEN
GERMANY
CZECHREP.
ACTIVITIES§ Science§ Technology§ Missions§ Workshops§ Publication series§ ESAframework§ Bilateralprograms§ Internationalprograms
Working Group on UVAstronomyDIVISIONBFacilities,Technologies&DataScience
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The NUVA publication series:• Challenges in UV Astronomy. Eds. Ana I. Gómez de Castro, Beatriz
Barbuy, Jorge Melnick, Noah Brosch & Mikhail Sachkov, 2014, Astrophysics and Space Science, Special Volume, 354
• UV Astronomy 2011. Eds. Boris Shustov, Ana I. Gómez de Castro, MikhailSachkov & Michael Dopita, 2012, Ed Springer Science+Business Media B.V., ISBN 978-94-007-2572-0
• Space Astronomy: the UV window to the Universe. Eds. Ana I Gómez de Castro & Noah Brosch, 2009,
• UV Astronomy: stars from birth to death. Eds. Ana I. Gómez de Castro & Martin A. Barstow, 2007, Ed. Universidad Complutense, ISBN: 978-84-7491-852-6
• Fundamental Questions in Astrophysics: Guidelines for future UV observations. Eds. Ana I Gómez de Castro & Willem Wamsteker, 2006, Ed. Springer, ISBN: 1-4020-4838-6, 1-4020-4839-4
UV SCIENCE: BROAD RANGE OF INTERESTNUVA WORKSHOPS
www.nuva.eu
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UV PROJECTS:BROADRANGEOFINTERESTS& ACTIVITIES
HSTTECHNOLOGICALSTRENGTHS
§ DETECTORS§ COATINGS§ OPTICALELEMENTS
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“CosmicVision”themes• Followsonfrom“Horizon
2020”and“Horizon2020+”– Whataretheconditionsfor
planetaryformation&theemergenceoflife?
– HowdoestheSolarSystemwork?
– WhatarethephysicalfundamentallawsoftheUniverse?
– HowdidtheUniverseoriginateandwhatisitmadeof?
• Four different mission types: Large (“L”), Medium (“M”), Small (“S”), Opportunity (“O”)
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Missions• Large- highinnovationcontent
– Europeanflagships,withnon-enablingcontributionsfrominternationalpartners
– 1B€class,1every7-8years• Medium- useofcurrentcutting-edgetechnology
– Canhavesubstantialinternationalcontributions,orcanbeacontributiontoamissionfromanotheragency
– 500M€class,1every3-4years• Small– Newelement,still“experimental”
– FastandwithESACaC =50M€– IncreaseflightopportunitiesforEuropeanscientists
• Opportunity– contributiontootheragencies
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XMM-Newton
CosmicVisionmissions• Approvedmissions,inorderoflaunchdate:
– SolarOrbiter (M1)– studyoftheSun– CHEOPS(S1)– transitsfromknownexo-planets– Euclid(M2)– searchfordarkenergy– JUICE(L1)– Jupiter&itsicymoons– PLATO(M3)– searchforexo-planetsdowntoEarthmasses
• Missionsselected,butnotfinallyapproval:– Athena(L2)– X-rayobservatory– SMILE(S2)– auroral imager
• Sciencethemeselectedfor:– Gravitationalwavemission(L3)
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JUICE
AthenaGravitational
WavesObservatory
PLATO
JWST
M4 in phase A
M6
Cheops, SMILE+
Astro-HMicroscope
ExoMars
EUCLID
Solar Orbiter
M5 in shortlist
M7
BEPICOLOMBO
COSMICVISION(2015-2035)CosmicVisionmissions
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PotentialforfutureUVmissions
• EuropeanUVObservatory(EUVO)submittedtoLthemeselectionprocess– Recognised lowlikelihoodofsuccess– PlaceholdertokeepUVinESAconsciousness
• StronginterestinUVremainspresentinEU– Arago proposalforM4/M5,butnotselected
• Responseto2016CallforIdeas• ParticipationinUSstudies
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EUROPEANULTRAVIOLET-VISIBLEOBSERVATORY“Buildinggalaxies,stars,planetsandtheingredientsforlifebetweenthestars”
Thierry Appourchaux – IAS France; Martin Barstow –University of Leicester UK; Mathieu Barthelemy - IPAG, France; Fréderic Baudin – IAS, France; Stefano Benetti –OAPD- INAF, Italy; Pere Blay - Universidad de Valencia, Spain; Noah Brosch - Tel Aviv University, Israel; Enma Bunce- University of Leicester, UK; Domitilla de Martino – OAC-INAF, Italy; Ana Ines Gomez de Castro –Universidad Complutense de Madrid, Spain; Jean-Michel Deharveng –Observatoire Astronomique Marseille-Provence, France;Roger Ferlet - Institute d'Astrophysique de Paris, France;Kevin France - University of Colorado, USA; Miriam García– IAC, Spain; Boris Gaensicke -University of Warwick, UK;Cecile Gry - Observatoire Astronomique Marseille-Provence, France; Lynne Hillenbrand – Caltech, USA; Eric Josselin -University of Montpellier, France; Carolina Kehrig – Instituto de Astrofísica de Andalucía, Spain; Laurent Lamy - LESIA, France; Jon Lapington – University of Leicester, UK; Alain Lecavelier des Etangs – Institute d'Astrophysique de Paris, France; Frank LePetit – Observatoire Paris-Meudom, France;Javier Lopez Santiago - Universidad Complutense de Madrid, Spain; Bruno Milliard- Observatoire Astronomique Marseille-Provence, France; Richard Monier - Université de Nice, France; Giampiero Naletto – University of Padova, Italy;YaelNazé - Liège University, Belgium; Coralie Neiner - LESIA, France; Jonathan Nichols – University of Leicester, UKMarina Orio – OAPD-INAF, Italy; Isabella Pagano – OACT-INAF, Italy; Céline Peroux – Observatoire AstronomiqueMarseille-Provence, France; Gregor Rauw – University of Liège, Belgium; Steven Shore – University of Pisa, Italy ; Marco Spaans - Kaptein Astronomical Institute, The Netherlands ; Gagik Tovmassian - Instit. Astr. Sede Ensenada-UNAM, Mexico; Asif ud-Doula - Penn State University, USA; José Vilchez – Instituto de Astrofísica de Andalucía, Spain and www.nuva.eu
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Ariane V fairinglimitis4mmonolithicmirror
Deployablesystemsrequired
Telescope ConceptKey Science 1The MissionKey Science 2 Planetary Science Stellar Physics Supernovae Technical
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ESACallforScienceIdeas• Europeanworkinggroupcreatedtorespond
– BuildingonAURAHDST2015report(www.hdstvision.org)
– AligningwithUSLUVOIRactivity• SubmittedSeptember2016
– “CosmicOriginsandtheSearchforLivingWorlds”– OtherexoEarth interest(e.g.SUPERSHARP)
• Deadlineforproposals– September14th• Selectionofa“limitednumberofideas”
– Selectionsnotyetannounced– Someideashavebeenrejected
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TechnicalRequirements
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• Telescopeaperture>10-12m• Coronograph orsunshade
– Contrast10-10
• Angularresolution<10mas• Rangeofspectroscopiccapability
– R~70-100(forexoEarths)– R~20,000-100,000
• Wavelengthcoveragefrom91nmto2µm
• Ultra-lowskybackground
EuropeinLUVOIR
• ObserversonSTDTteam– MartinBarstow(UK),LarsBuchhave (Denmark),MarkFerrari(France),AnaGomezdeCastro(Spain),ThomasHenning(Germany),AntonellaNota(ESA)
• CNESsponsoredinstrumentstudy– POLLUX,UVspectro-polarimeter (98-390nm,R~120,000-200,000)
– StudyleadsCoralieNeiner &Jean-ClaudeBouret
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