Galaxy: structure; stars: abundances; stars: fundamental parameters; stars: oscillations; surveys
Abstract :
[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 it 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 prerequisite to then reach the more ambitious goal of a similar level of accuracy, which will be possible only if we have at hand a careful appraisal of systematic uncertainties on age deriving from our limited understanding of stellar physics, a goal that conveniently falls within the main aims of PLATO's core science. We therefore strongly endorse PLATO's current design and proposed observational strategy, and conclude that PLATO, as it is, will be a legacy mission for Galactic archaeology.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Miglio, A.; School of Physics and Astronomy, University of Birmingham, Birmingham, UK ; Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Aarhus, Denmark
Chiappini, C.; Leibniz-Institut für Astrophysik Potsdam (AIP), Potsdam, Germany
Mosser, B.; LESIA, Observatoire de Paris, PSL Research University, CNRS, Université Pierre et Marie Curie, Université Paris Diderot, Meudon, France
Davies, G. R.; School of Physics and Astronomy, University of Birmingham, Birmingham, UK ; Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Aarhus, Denmark
Freeman, K.; Research School of Astronomy and Astrophysics, Mount Stromlo Observatory, The Australian National University, ACT, Australia
Girardi, L.; INAF - Osservatorio Astronomico di Padova, Padova, Italy
Jofré, P.; Institute of Astronomy, University of Cambridge, Cambridge, UK ; Núcleo de Astronomía, Facultad de Ingeniería, Universidad Diego Portales, Santiago, Chile
Kawata, D.; Mullard Space Science Laboratory, University College London, Surrey, UK
Rendle, B. M.; School of Physics and Astronomy, University of Birmingham, Birmingham, UK ; Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Aarhus, Denmark
Valentini, Marica ; Leibniz-Institut für Astrophysik Potsdam (AIP), Potsdam, Germany
Casagrande, L.; Research School of Astronomy and Astrophysics, Mount Stromlo Observatory, The Australian National University, ACT, Australia
Chaplin, W. J.; School of Physics and Astronomy, University of Birmingham, Birmingham, UK ; Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Aarhus, Denmark
Gilmore, G.; Institute of Astronomy, University of Cambridge, Cambridge, UK
Hawkins, K.; Institute of Astronomy, University of Cambridge, Cambridge, UK ; Department of Astronomy, Columbia University, New York, New York,
Holl, B.; School of Physics and Astronomy, University of Birmingham, Birmingham, UK ; Department of Astronomy, University of Geneva, Versoix, Switzerland
Appourchaux, T.; Institut d'Astrophysique Spatiale, Université Paris-Sud, UMR 8617, CNRS, Orsay Cedex, France
Belkacem, K.; LESIA, Observatoire de Paris, PSL Research University, CNRS, Université Pierre et Marie Curie, Université Paris Diderot, Meudon, France
Bossini, D.; School of Physics and Astronomy, University of Birmingham, Birmingham, UK ; Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Aarhus, Denmark
Brogaard, K.; School of Physics and Astronomy, University of Birmingham, Birmingham, UK ; Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Aarhus, Denmark
Goupil, M.-J.; LESIA, Observatoire de Paris, PSL Research University, CNRS, Université Pierre et Marie Curie, Université Paris Diderot, Meudon, France
Montalbán, J.; Dipartimento di Fisica e Astronomia, Universitá di Padova, Padova, Italy
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