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<publisher>HAL CCSD</publisher>
<title lang=en>PLATO as it is: a legacy mission for Galactic archaeology</title>
<creator>Miglio, A.</creator>
<creator>Chiappini, C.</creator>
<creator>Mosser, B.</creator>
<creator>Davies, G. R.</creator>
<creator>Freeman, K.</creator>
<creator>Girardi, L.</creator>
<creator>Jofre, P.</creator>
<creator>Kawata, D.</creator>
<creator>Rendle, B. M.</creator>
<creator>Valentini, M.</creator>
<creator>Casagrande, L.</creator>
<creator>Chaplin, W. J.</creator>
<creator>Gilmore, G.</creator>
<creator>Hawkins, K.</creator>
<creator>Holl, B.</creator>
<creator>Appourchaux, T.</creator>
<creator>Belkacem, K.</creator>
<creator>Bossini, D.</creator>
<creator>Brogaard, K.</creator>
<creator>Goupil, M. -J.</creator>
<creator>Montalban, J.</creator>
<creator>Noels, A.</creator>
<creator>Anders, F.</creator>
<creator>Rodrigues, T.</creator>
<creator>Piotto, G.</creator>
<creator>Pollacco, D.</creator>
<creator>Rauer, H.</creator>
<creator>Prieto, C. Allende</creator>
<creator>Avelino, P. P.</creator>
<creator>Babusiaux, C.</creator>
<creator>Barban, C.</creator>
<creator>Barbuy, B.</creator>
<creator>Basu, S.</creator>
<creator>Baudin, F.</creator>
<creator>Benomar, O.</creator>
<creator>Bienayme, O.</creator>
<creator>Binney, J.</creator>
<creator>Bland-Hawthorn, J.</creator>
<creator>Bressan, A.</creator>
<creator>Cacciari, C.</creator>
<creator>Campante, T. L.</creator>
<creator>Cassisi, S.</creator>
<creator>Christensen-Dalsgaard, J.</creator>
<creator>Combes, F.</creator>
<creator>Creevey, O.</creator>
<creator>Cunha, M. S.</creator>
<creator>de Jong, R. S.</creator>
<creator>De Laverny, P.</creator>
<creator>Degl'Innocenti, S.</creator>
<creator>Deheuvels, S.</creator>
<creator>Depagne, E.</creator>
<creator>DeRidder, J.</creator>
<creator>DiMatteo, P.</creator>
<creator>Di Mauro, M. P.</creator>
<creator>Dupret, M. -A.</creator>
<creator>Eggenberger, P.</creator>
<creator>Elsworth, Y.</creator>
<creator>Famaey, B.</creator>
<creator>Feltzing, S.</creator>
<creator>Garcia, R. A.</creator>
<creator>Gerhard, O.</creator>
<creator>Gibson, B. K.</creator>
<creator>Gizon, Laurent</creator>
<creator>Haywood, M.</creator>
<creator>Handberg, R.</creator>
<creator>Heiter, U.</creator>
<creator>Hekker, S.</creator>
<creator>Huber, D.</creator>
<creator>Ibata, R.</creator>
<creator>Katz, D.</creator>
<creator>Kawaler, S. D.</creator>
<creator>Kjeldsen, H.</creator>
<creator>Kurtz, D. W.</creator>
<creator>Lagarde, N.</creator>
<creator>Lebreton, Y.</creator>
<creator>Lund, M. N.</creator>
<creator>Majewski, S. R.</creator>
<creator>Marigo, P.</creator>
<creator>Martig, M.</creator>
<creator>Mathur, S.</creator>
<creator>Minchev, I.</creator>
<creator>Morel, T.</creator>
<creator>Ortolani, S.</creator>
<creator>Pinsonneault, M. H.</creator>
<creator>Plez, B.</creator>
<creator>Moroni, P. G. Prada</creator>
<creator>Pricopi, D.</creator>
<creator>Recio-Blanco, A.</creator>
<creator>Reyle, C.</creator>
<creator>Robin, A.</creator>
<creator>Roxburgh, I. W.</creator>
<creator>Salaris, M.</creator>
<creator>Santiago, B. X.</creator>
<creator>Schiavon, R.</creator>
<creator>Serenelli, A.</creator>
<creator>Sharma, S.</creator>
<creator>Aguirre, V. Silva</creator>
<creator>Soubiran, C.</creator>
<creator>Steinmetz, M.</creator>
<creator>Stello, D.</creator>
<creator>Strassmeier, K. G.</creator>
<creator>Ventura, P.</creator>
<creator>Ventura, R.</creator>
<creator>Walton, N. A.</creator>
<creator>Worley, C. C.</creator>
<contributor>Institut d'Astrophysique et de Géophysique [Liège] ; Université de Liège</contributor>
<contributor>Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA) ; Université Pierre et Marie Curie - Paris 6 (UPMC) - Institut national des sciences de l'Univers (INSU - CNRS) - Observatoire de Paris - Université Paris Diderot - Paris 7 (UPD7) - Centre National de la Recherche Scientifique (CNRS)</contributor>
<contributor>Arizona State University [Tempe] (ASU)</contributor>
<contributor>Leibniz-Institut für Astrophysik Potsdam (AIP)</contributor>
<contributor>Department of Physics and Astronomy [Aarhus] ; Aarhus University [Aarhus]</contributor>
<contributor>School of Physics and Astronomy [Birmingham] ; University of Birmingham [Birmingham]</contributor>
<contributor>Heckscher-Klinikum ; Heckscher-Klinikum</contributor>
<contributor>Danish AsteroSeismology Centre (DASC) ; Aarhus University [Aarhus]</contributor>
<contributor>Universidade Federal de São Paulo (UNIFESP)</contributor>
<contributor>DLR Institut für Planetenforschung ; Deutsches Zentrum für Luft- und Raumfahrt [Berlin] (DLR)</contributor>
<contributor>Department of Astronomy [New Haven] ; Yale University [New Haven]</contributor>
<contributor>Evolution et Modélisation des Bassins Sédimentaires (EMBS) ; Institut des Sciences de la Terre de Paris (iSTeP) ; Université Pierre et Marie Curie - Paris 6 (UPMC) - Centre National de la Recherche Scientifique (CNRS) - Université Pierre et Marie Curie - Paris 6 (UPMC) - Centre National de la Recherche Scientifique (CNRS)</contributor>
<contributor>Department of Biomedical, Metabolic and Neural Sciences [Modena] ; Università degli Studi di Modena e Reggio Emilia [Reggio Emilia] (UNIMORE)</contributor>
<contributor>School of Physics and Astronomy, University of Birmingham ; University of Birmingham [Birmingham]</contributor>
<contributor>Institut d'astrophysique spatiale (IAS) ; Université Paris-Sud - Paris 11 (UP11) - Institut national des sciences de l'Univers (INSU - CNRS) - Centre National de la Recherche Scientifique (CNRS)</contributor>
<contributor>Universidade de Aveiro</contributor>
<contributor>Lagrange (UMR 7293) ; Observatoire de la Côte d'Azur</contributor>
<contributor>Institut de recherche en astrophysique et planétologie (IRAP) ; Université Paul Sabatier - Toulouse 3 (UPS) - Observatoire Midi-Pyrénées (OMP) - Centre National de la Recherche Scientifique (CNRS)</contributor>
<contributor>Las Cumbres Observatory (LCO)</contributor>
<contributor>Observatoire Astronomique de l'Université de Genève (ObsGE) ; Université de Genève (UNIGE)</contributor>
<contributor>Université de Strasbourg (UNISTRA)</contributor>
<contributor>Observatoire astronomique de Strasbourg (OAS) ; Institut national des sciences de l'Univers (INSU - CNRS) - Centre National de la Recherche Scientifique (CNRS)</contributor>
<contributor>University of Girona - Spain</contributor>
<contributor>Max-Planck-Institut für Extraterrestrische Physik (MPE)</contributor>
<contributor>Max-Planck-Institut für Sonnensystemforschung (MPS)</contributor>
<contributor>SETI Institute</contributor>
<contributor>University of Illinois at Urbana Champaign (UIUC) ; University of Illinois at Urbana-Champaign [Urbana]</contributor>
<contributor>Universidade Federal de Santa Catarina [Florianópolis] (UFSC)</contributor>
<contributor>Institut de Physique de Rennes (IPR) ; Université de Rennes 1 (UR1) - Centre National de la Recherche Scientifique (CNRS)</contributor>
<contributor>Galaxies, Etoiles, Physique, Instrumentation (GEPI) ; Institut national des sciences de l'Univers (INSU - CNRS) - Observatoire de Paris - Université Paris Diderot - Paris 7 (UPD7) - Centre National de la Recherche Scientifique (CNRS)</contributor>
<contributor>Space Science Institute, 4750 Walnut St., Boulder, CO 80301, United States</contributor>
<contributor>Sciences, Philosophie, Humanités (SPH) ; Université de Bordeaux (UB) - Université Bordeaux Montaigne</contributor>
<contributor>Department of Astronomy (Ohio State University) ; Ohio State University [Columbus] (OSU)</contributor>
<contributor>Laboratoire Univers et Particules de Montpellier (LUPM) ; Centre National de la Recherche Scientifique (CNRS) - Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3) - Université Montpellier 2 - Sciences et Techniques (UM2) - Université de Montpellier (UM)</contributor>
<contributor>Univers, Transport, Interfaces, Nanostructures, Atmosphère et environnement, Molécules (UTINAM) ; Institut national des sciences de l'Univers (INSU - CNRS) - Centre National de la Recherche Scientifique (CNRS) - Université de Franche-Comté (UFC)</contributor>
<contributor>Institut universitaire de formation des maîtres - Montpellier (IUFM Montpellier) ; Université Montpellier 2 - Sciences et Techniques (UM2)</contributor>
<contributor>Institute of Space Sciences [Barcelona] (ICE-CSIC) ; Spanish National Research Council [Madrid] (CSIC)</contributor>
<contributor>Sydney Institute for Astronomy (SIfA) ; The University of Sydney [Sydney]</contributor>
<contributor>M2A 2017 ; Laboratoire d'Astrophysique de Bordeaux [Pessac] (LAB) ; Université de Bordeaux (UB) - Institut national des sciences de l'Univers (INSU - CNRS) - Centre National de la Recherche Scientifique (CNRS) - Université de Bordeaux (UB) - Institut national des sciences de l'Univers (INSU - CNRS) - Centre National de la Recherche Scientifique (CNRS)</contributor>
<contributor>Leibniz Institute for Astrophysics</contributor>
<contributor>Symbiose Marine (SM) ; Systématique, adaptation, évolution (SAE) ; Université Pierre et Marie Curie - Paris 6 (UPMC) - Centre National de la Recherche Scientifique (CNRS) - Université Pierre et Marie Curie - Paris 6 (UPMC) - Centre National de la Recherche Scientifique (CNRS) - Evolution Paris Seine ; Université Nice Sophia Antipolis (UNS) ; Université Côte d'Azur (UCA) - Université Côte d'Azur (UCA) - Centre National de la Recherche Scientifique (CNRS) - Université des Antilles et de la Guyane (UAG) - Université Pierre et Marie Curie - Paris 6 (UPMC) - Université Nice Sophia Antipolis (UNS) ; Université Côte d'Azur (UCA) - Université Côte d'Azur (UCA) - Université des Antilles et de la Guyane (UAG)</contributor>
<description>International audience</description>
<source>ISSN: 0004-6337</source>
<source>EISSN: 1521-3994</source>
<source>Astronomical Notes / Astronomische Nachrichten</source>
<publisher>Wiley-VCH Verlag</publisher>
<identifier>hal-01541393</identifier>
<identifier>https://hal.archives-ouvertes.fr/hal-01541393</identifier>
<source>https://hal.archives-ouvertes.fr/hal-01541393</source>
<source>Astronomical Notes / Astronomische Nachrichten, Wiley-VCH Verlag, 2017, 338 (6), pp.644-661. 〈10.1002/asna.201713385〉</source>
<identifier>ARXIV : 1706.3778</identifier>
<relation>info:eu-repo/semantics/altIdentifier/arxiv/1706.3778</relation>
<identifier>BIBCODE : 2017AN....338..644M</identifier>
<identifier>DOI : 10.1002/asna.201713385</identifier>
<relation>info:eu-repo/semantics/altIdentifier/doi/10.1002/asna.201713385</relation>
<language>en</language>
<subject lang=en>Astrophysics - Astrophysics of Galaxies</subject>
<subject lang=en>Astrophysics - Solar and Stellar Astrophysics</subject>
<subject>[PHYS.ASTR.SR] Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]</subject>
<type>info:eu-repo/semantics/article</type>
<type>Journal articles</type>
<description lang=en>Deciphering 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.</description>
<date>2017-06</date>
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