Abstract
PLATO is the M3 (medium-class) mission in the ESA Cosmic Vision 2015–2025 program, with a planned launch date in 2026. PLATO will carry out transit surveys to detect and characterize planets around bright stars, with special emphasis on small planets orbiting in the habitable zone of solar-like stars. PLATO will allow us to determine the planets’ radii with unprecedented accuracy, and, thanks to the brightness of its targets, also the planets’ masses through ground-based radial velocity observations. With the asteroseismology analysis of the light curves, it will be possible to characterize the planet host stars and to determine their precise ages, covering a large diversity of planetary systems. The PLATO payload consists of 24 telescopes with CCD-based focal planes, which will monitor stars with V >8 over a wide sky field of view of ~2232°2 per pointing. Two additional “fast” cameras will be used for stars with V~4–8. The nominal duration of the science operations is 4 years.
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References
Baglin A, Michel E, Noels A (2013) Recent CoRoT achievements in stellar physics. In: Shibahashi H, Lynas-Gray AE (eds) Progress in physics of the sun and stars: a new era in helio- and asteroseismology. ASPC479: 461 Astronomical Society of the Pacific Conference Series 479: 461, http://aspbooks.org/publications/479/461.pdf
Batalha NM, Borucki WJ, Bryson ST et al (2011) Kepler’s first rocky planet: Kepler-10b. Astrophys J 729:27–47. doi:10.1088/0004-637X/729/1/27
Benomar O, Masuda K, Shibahashi H et al (2014) Determination of three-dimensional spin-orbit angle with joint analysis of asteroseismology, transit lightcurve, and the Rossiter-McLaughlin effect: cases of HAT-P-7 and Kepler-25. Publ Astron Soc Jpn 66:94. doi:10.1093/pasj/psu069. 1407.7332
Borucki WJ, Koch D, Basri G et al (2010) Kepler planet-detection mission: introduction and first results. Science 327:977. doi:10.1126/science.1185402
Broeg C, Fortier A, Ehrenreich D et al (2013) CHEOPS: a transit photometry mission for ESA’s small mission programme. In: Saglia R (ed) Hot planets and cool stars, Garching, Germany, EPJ Web of Conferences EPJWC 47: 03005. doi:10.1051/epjconf/20134703005, 1305.2270
Buldgen G, Reese DR, Dupret MA et al (2015) Stellar acoustic radii, mean densities, and ages from seismic inversion techniques. Astron Astrophys 574:A42. doi:10.1051/0004-6361/201424613, 1411.2416
Cabrera J, Bruntt H, Ollivier M et al (2010) Transiting exoplanets from the CoRoT space mission. XIII. CoRoT-13b: a dense hot Jupiter in transit around a star with solar metallicity and super-solar lithium content. Astron Astrophys 522:A110. doi:10.1051/0004-6361/201015154, 1007.5481
Cabrera J, Csizmadia S, Lehmann H et al (2014) The planetary system to KIC 11442793: a compact analogue to the solar system. Astrophys J 781:18–30. doi:10.1088/0004-637X/781/1/18, 1310.6248
Campante TL, Schofield M, Kuszlewicz JS et al (2016) The asteroseismic potential of TESS: exoplanet-host stars. Astrophys J 830:138. doi:10.3847/0004-637X/830/2/138, 1608.01138
Chaplin WJ, Sanchis-Ojeda R, Campante TL et al (2013) Asteroseismic determination of obliquities of the exoplanet systems Kepler-50 and Kepler-65. Astrophys J 766:101–119. doi:10.1088/0004-637X/766/2/101, 1302.3728
Doyle LR, Carter JA, Fabrycky DC et al (2011) Kepler-16: a transiting Circumbinary planet. Science 333:1602. doi:10.1126/science.1210923, 1109.3432
ESA-SCI (2017) 1 PLATO definition study report, stars
European Space Agency, http://sci.esa.int/plato/59252-plato-definition-study-report-red-book/
Gillon M, Triaud AHMJ, Demory B-O et al (2017) Seven temperate terrestrial planets around the nearby ultracool dwarf star TRAPPIST-1. Nature 542:456–460. doi:10.1038/nature21360
Gizon L, Ballot J, Michel E et al (2013) Seismic constraints on rotation of sun-like star and mass of exoplanet. PNAS 110:13267–13271. doi:10.1073/pnas.1303291110, 1308.4352
Howell SB, Sobeck C, Haas M et al (2014) The K2 mission: characterization and early results. Publ Astron Soc Pac 126:398–408. doi:10.1086/676406, 1402.5163
Huber D, Ireland MJ, Bedding TR et al (2012) Fundamental properties of stars using asteroseismology from Kepler and CoRoT and interferometry from the CHARA array. Astrophys J 760:32–48. doi:10.1088/0004-637X/760/1/32, 1210.0012
Kipping DM, Huang X, Nesvorny D et al (2015) The possible moon of Kepler-90g is a false positive. Astrophys J Letters 799:L14. doi:10.1088/2041-8205/799/1/L14, 1411.7028
Lammer H, Erkaev NV, Fossati L et al (2016) Identifying the ‘true’ radius of the hot sub-Neptune CoRoT-24b by mass-loss modelling. Mon Not R Astron Soc 461:L62–L66. doi:10.1093/mnrasl/slw095, 1605.03595
Lebreton Y, Goupil MJ (2014) Asteroseismology for “à la carte” stellar age-dating and weighing. Age and mass of the CoRoT exoplanet host HD 52265. Astron Astrophys 569:A21. doi:10.1051/0004-6361/201423797, 1406.0652
Lebreton Y, Goupil MJ, Montalbán J (2014a) How accurate are stellar ages based on stellar models? I. The impact of stellar models uncertainties. EAS 65:99–176. doi:10.1051/eas/1465004, 1410.5336
Lebreton Y, Goupil MJ, Montalbán J (2014b) How accurate are stellar ages based on stellar models? II. The impact of asteroseismology. EAS 65:177–223. doi:10.1051/eas/1465005, 1410.5337
Lundkvist MS, Kjeldsen H, Albrecht S et al (2016) Hot super-earths stripped by their host stars. Nat Commun 7:11201. doi:10.1038/ncomms11201, 1604.05220
Mortier A, Santos NC, Sousa SG et al (2013) New and updated stellar parameters for 71 evolved planet hosts. On the metallicity-giant planet connection. Astron Astrophys 557:A70. doi:10.1051/0004-6361/201321641, 1307.7870
Namouni F (2010) The fate of moons of close-in giant exoplanets. Astrophys J Letters 719:L145–L147. doi:10.1088/2041-8205/719/2/L145, 1007.2537
Nascimbeni V, Piotto G, Ortolani S et al (2016) An all-sky catalogue of solar-type dwarfs for exoplanetary transit surveys. Mon Not R Astron Soc 463:4210–4222. doi:10.1093/mnras/stw2313, 1609.03037
Queloz D, Bouchy F, Moutou C et al (2009) The CoRoT-7 planetary system: two orbiting super-earths. Astron Astrophys 506:303–319. doi:10.1051/0004-6361/200913096
Rauer H, Catala C, Aerts C et al (2014) The PLATO 2.0 mission. Exp Astron 38:249–330. doi:10.1007/s10686-014-9383-4, 1310.0696
Ricker GR, Winn JN, Vanderspek R et al (2015) Transiting exoplanet survey satellite (TESS). JATIS 1:014003. doi:10.1117/1.JATIS.1.1.014003
Silva Aguirre V, Casagrande L, Basu S et al (2012) Verifying asteroseismically determined parameters of Kepler stars using Hipparcos parallaxes: self-consistent stellar properties and distances. Astrophys J 757:99–109. doi:10.1088/0004-637X/757/1/99, 1208.6294
White TR, Silva Aguirre V, Boyajian T et al (2015) Testing asteroseismic scaling relations with interferometry. In: García RA, Ballot J (eds) The space photometry revolution. EPJ Web of Conferences EPJWC101: 06068. doi:10.1051/epjconf/201510106068
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Rauer, H., Heras, A.M. (2017). Space Missions for Exoplanet Science: PLATO. In: Deeg, H., Belmonte, J. (eds) Handbook of Exoplanets . Springer, Cham. https://doi.org/10.1007/978-3-319-30648-3_86-1
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DOI: https://doi.org/10.1007/978-3-319-30648-3_86-1
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