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PLATO as it is: a legacy mission for Galactic archaeology

hal.structure.identifierInstitut d'Astrophysique et de Géophysique [Liège]
dc.contributor.authorMIGLIO, A.
dc.contributor.authorCHIAPPINI, C.
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
dc.contributor.authorMOSSER, B.
dc.contributor.authorDAVIES, G. R.
hal.structure.identifierArizona State University [Tempe] [ASU]
dc.contributor.authorFREEMAN, K.
dc.contributor.authorGIRARDI, L.
dc.contributor.authorJOFRE, P.
dc.contributor.authorKAWATA, D.
dc.contributor.authorRENDLE, B. M.
hal.structure.identifierLeibniz-Institut für Astrophysik Potsdam [AIP]
dc.contributor.authorVALENTINI, M.
dc.contributor.authorCASAGRANDE, L.
hal.structure.identifierDepartment of Physics and Astronomy [Aarhus]
hal.structure.identifierSchool of Physics and Astronomy [Birmingham]
dc.contributor.authorCHAPLIN, W. J.
dc.contributor.authorGILMORE, G.
dc.contributor.authorHAWKINS, K.
hal.structure.identifierHeckscher-Klinikum
dc.contributor.authorHOLL, B.
dc.contributor.authorAPPOURCHAUX, T.
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
dc.contributor.authorBELKACEM, K.
dc.contributor.authorBOSSINI, D.
hal.structure.identifierDanish AsteroSeismology Centre [DASC]
dc.contributor.authorBROGAARD, K.
dc.contributor.authorGOUPIL, M. -J.
dc.contributor.authorMONTALBAN, J.
dc.contributor.authorNOELS, A.
dc.contributor.authorANDERS, F.
hal.structure.identifierFederal University of Sao Paulo [Unifesp]
dc.contributor.authorRODRIGUES, T.
dc.contributor.authorPIOTTO, G.
dc.contributor.authorPOLLACCO, D.
hal.structure.identifierDLR Institut für Planetenforschung
dc.contributor.authorRAUER, H.
dc.contributor.authorPRIETO, C. Allende
dc.contributor.authorAVELINO, P. P.
dc.contributor.authorBABUSIAUX, C.
dc.contributor.authorBARBAN, C.
dc.contributor.authorBARBUY, B.
hal.structure.identifierDepartment of Astronomy [New Haven]
dc.contributor.authorBASU, S.
hal.structure.identifierUniversité Paris-Saclay
hal.structure.identifierInstitut d'astrophysique spatiale [IAS]
dc.contributor.authorBAUDIN, Frédéric
dc.contributor.authorBENOMAR, O.
dc.contributor.authorBIENAYME, O.
dc.contributor.authorBINNEY, J.
dc.contributor.authorBLAND-HAWTHORN, J.
dc.contributor.authorBRESSAN, A.
hal.structure.identifierDepartment of Biomedical, Metabolic and Neural Sciences [Modena]
dc.contributor.authorCACCIARI, C.
hal.structure.identifierSchool of Physics and Astronomy [Birmingham]
dc.contributor.authorCAMPANTE, T. L.
dc.contributor.authorCASSISI, S.
hal.structure.identifierDanish AsteroSeismology Centre [DASC]
dc.contributor.authorCHRISTENSEN-DALSGAARD, J.
hal.structure.identifierCollège de France - Chaire Galaxies et cosmologie
dc.contributor.authorCOMBES, F.
hal.structure.identifierInstitut d'astrophysique spatiale [IAS]
dc.contributor.authorCREEVEY, O.
hal.structure.identifierUniversidade de Aveiro
dc.contributor.authorCUNHA, M. S.
dc.contributor.authorDE JONG, R. S.
hal.structure.identifierJoseph Louis LAGRANGE [LAGRANGE]
dc.contributor.authorDE LAVERNY, P.
dc.contributor.authorDEGL'INNOCENTI, S.
hal.structure.identifierInstitut de recherche en astrophysique et planétologie [IRAP]
dc.contributor.authorDEHEUVELS, S.
hal.structure.identifierLas Cumbres Observatory [LCO]
dc.contributor.authorDEPAGNE, E.
dc.contributor.authorDERIDDER, J.
dc.contributor.authorDIMATTEO, P.
dc.contributor.authorDI MAURO, M. P.
hal.structure.identifierInstitut d'Astrophysique et de Géophysique [Liège]
dc.contributor.authorDUPRET, M. -A.
hal.structure.identifierObservatoire Astronomique de l'Université de Genève [ObsGE]
dc.contributor.authorEGGENBERGER, P.
dc.contributor.authorELSWORTH, Y.
hal.structure.identifierUniversité de Strasbourg [UNISTRA]
hal.structure.identifierObservatoire astronomique de Strasbourg [ObAS]
dc.contributor.authorFAMAEY, B.
dc.contributor.authorFELTZING, S.
hal.structure.identifierUniversitat de Girona = University of Girona [UdG]
dc.contributor.authorGARCIA, R. A.
hal.structure.identifierMax-Planck-Institut für Extraterrestrische Physik [MPE]
dc.contributor.authorGERHARD, O.
dc.contributor.authorGIBSON, B. K.
hal.structure.identifierMax-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
dc.contributor.authorGIZON, Laurent
hal.structure.identifierGalaxies, Etoiles, Physique, Instrumentation [GEPI]
dc.contributor.authorHAYWOOD, M.
hal.structure.identifierDepartment of Physics and Astronomy [Aarhus]
dc.contributor.authorHANDBERG, R.
dc.contributor.authorHEITER, U.
dc.contributor.authorHEKKER, S.
hal.structure.identifierSETI Institute
hal.structure.identifierDepartment of Physics and Astronomy [Aarhus]
dc.contributor.authorHUBER, D.
dc.contributor.authorIBATA, R.
hal.structure.identifierUniversity of Illinois at Urbana-Champaign [Urbana] [UIUC]
dc.contributor.authorKATZ, D.
dc.contributor.authorKAWALER, S. D.
hal.structure.identifierDanish AsteroSeismology Centre [DASC]
dc.contributor.authorKJELDSEN, H.
hal.structure.identifierUniversidade Federal de Santa Catarina = Federal University of Santa Catarina [Florianópolis] [UFSC]
dc.contributor.authorKURTZ, D. W.
hal.structure.identifierUnivers, Théorie, Interfaces, Nanostructures, Atmosphère et environnement, Molécules (UMR 6213) [UTINAM]
dc.contributor.authorLAGARDE, N.
hal.structure.identifierInstitut de Physique de Rennes [IPR]
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
dc.contributor.authorLEBRETON, Y.
dc.contributor.authorLUND, M. N.
dc.contributor.authorMAJEWSKI, S. R.
dc.contributor.authorMARIGO, P.
dc.contributor.authorMARTIG, M.
hal.structure.identifierSpace Science Institute [Boulder] [SSI]
dc.contributor.authorMATHUR, S.
hal.structure.identifierLeibniz-Institut für Astrophysik Potsdam [AIP]
dc.contributor.authorMINCHEV, I.
dc.contributor.authorMOREL, T.
dc.contributor.authorORTOLANI, S.
dc.contributor.authorPINSONNEAULT, M. H.
hal.structure.identifierLaboratoire Univers et Particules de Montpellier [LUPM]
dc.contributor.authorPLEZ, B.
dc.contributor.authorMORONI, P. G. Prada
dc.contributor.authorPRICOPI, D.
hal.structure.identifierJoseph Louis LAGRANGE [LAGRANGE]
dc.contributor.authorRECIO-BLANCO, A.
hal.structure.identifierUnivers, Théorie, Interfaces, Nanostructures, Atmosphère et environnement, Molécules (UMR 6213) [UTINAM]
dc.contributor.authorREYLÉ, C.
hal.structure.identifierUnivers, Théorie, Interfaces, Nanostructures, Atmosphère et environnement, Molécules (UMR 6213) [UTINAM]
dc.contributor.authorROBIN, A.
dc.contributor.authorROXBURGH, I. W.
hal.structure.identifierAstrophysical Research Institute [Liverpool]
dc.contributor.authorSALARIS, M.
dc.contributor.authorSANTIAGO, B. X.
dc.contributor.authorSCHIAVON, R.
hal.structure.identifierInstitute of Space Sciences [Barcelona] [ICE-CSIC]
dc.contributor.authorSERENELLI, A.
hal.structure.identifierSydney Institute for Astronomy [SIfA]
dc.contributor.authorSHARMA, S.
hal.structure.identifierDepartment of Physics and Astronomy [Aarhus]
dc.contributor.authorAGUIRRE, V. Silva
hal.structure.identifierM2A 2017
dc.contributor.authorSOUBIRAN, C.
hal.structure.identifierLeibniz-Institut für Astrophysik Potsdam [AIP]
dc.contributor.authorSTEINMETZ, M.
hal.structure.identifierDepartment of Physics and Astronomy [Aarhus]
dc.contributor.authorSTELLO, D.
hal.structure.identifierLeibniz Institute for Astrophysics Potsdam [AIP]
dc.contributor.authorSTRASSMEIER, K. G.
hal.structure.identifierSymbiose Marine [SM]
dc.contributor.authorVENTURA, P.
dc.contributor.authorVENTURA, R.
dc.contributor.authorWALTON, N. A.
dc.contributor.authorWORLEY, C. C.
dc.date.issued2017-06
dc.identifier.issn0004-6337
dc.description.abstractEnDeciphering the assembly history of the Milky Way is a formidable task, which becomes possible only if one can produce high-resolution chrono-chemo-kinematical maps of the Galaxy. Data from large-scale astrometric and spectroscopic surveys will soon provide us with a well-defined view of the current chemo-kinematical structure of the Milky Way, but will only enable a blurred view on the temporal sequence that led to the present-day Galaxy. As demonstrated by the (ongoing) exploitation of data from the pioneering photometric missions CoRoT, Kepler, and K2, asteroseismology provides the way forward: solar-like oscillating giants are excellent evolutionary clocks thanks to the availability of seismic constraints on their mass and to the tight age-initial-mass relation they adhere to. In this paper we identify five key outstanding questions relating to the formation and evolution of the Milky Way that will need precise and accurate ages for large samples of stars to be addressed, and we identify the requirements in terms of number of targets and the precision on the stellar properties that are needed to tackle such questions. By quantifying the asteroseismic yields expected from PLATO for red-giant stars, we demonstrate that these requirements are within the capabilities of the current instrument design, provided that observations are sufficiently long to identify the evolutionary state and allow robust and precise determination of acoustic-mode frequencies. This will allow us to harvest data of sufficient quality to reach a 10% precision in age. This is a fundamental pre-requisite to then reach the more ambitious goal of a similar level of accuracy, which will only be possible if we have to hand a careful appraisal of systematic uncertainties on age deriving from our limited understanding of stellar physics, a goal which conveniently falls within the main aims of PLATO's core science.
dc.language.isoen
dc.publisherWiley-VCH Verlag
dc.subject.enAstrophysics - Astrophysics of Galaxies
dc.subject.enAstrophysics - Solar and Stellar Astrophysics
dc.title.enPLATO as it is: a legacy mission for Galactic archaeology
dc.typeArticle de revue
dc.identifier.doi10.1002/asna.201713385
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
dc.identifier.arxiv1706.03778
bordeaux.journalAstronomical Notes / Astronomische Nachrichten
bordeaux.journalAstronomical Notes / Astronomische Nachrichten
bordeaux.page644-661
bordeaux.volume338
bordeaux.issue6
bordeaux.peerReviewedoui
hal.identifierhal-01541393
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01541393v1
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