{"paper":{"title":"The PLATO 2.0 Mission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Brandeker, A. C. Birch, A. Erikson, A. F. Lanza, A. Grotsch-Noels, A. J. Norton, A. Johansen, A. Miglio, A. Mortier, A. Ofir, A. P. Hatzes, A. Quirrenbach, A. Santerne, A. S. Bonomo, A. Silva-Valio, A. Smith, A. Sozzetti, A. Tkachenko, B. Plez, B. Rojas-Ayala, C. Aerts, C. A. Haswell, C. Catala, C. Chiappini, C. Dreyer, C. Mordasini, D. Ehrenreich, D. Magrin, D. Pollacco, D. R. Reese, D. Stello, D. Valencia, E. Antonello, E. Brocato, E. G\\\"unther, E. Janot-Pacheco, E. Moravveji, E. Poretti, F. Baudin, F. Borsa, F. de Oliveira Fialho, F. Kupka, F. Sohl, F. W. Wagner, G. Bihain, G. Giuffrida, G. H\\'ebrard, G. Piotto, G. Raimondo, Gy. M. Szab\\'o, H. J. Deeg, H. Lammer, H. Moradi, H. Rauer, H. Schunker, I. Boisse, I. M. Brand\\~ao, I. Pagano, I. Skillen, I. Snellen, I. W. Roxburgh, J.-C., J. Cabrera, J. Christensen-Dalsgaard, J. Gomes da Silva, J. L. Grenfell, J.-M. Almenara, J. Martins, J. M. Jenkins, J. Montalban, J. P. Marques, J. Schneider, J. Schou, J. Weingrill, K. Belkacem, K. G. Kislyakova, K. G. Strassmeier, K. Heng, K. Zwintz, L. Gizon, L. Noack, M. Ammler-von Eiff, M. Asplund, M. B. Davies, M. Bergemann, M. B. Nielsen, M. Burleigh, M. Cunha, M. Damasso, M. Deleuil, M. Fridlund, M. Godolt, M. G\\\"udel, M.-J. Goupil, M. J. P. F. G. Monteiro, M. L. Khodachenko, M. Mas-Hesse, M. Montalto, M. Oshagh, M. Rainer, M. \\v{S}vanda, N. A. Walton, N. C. Santos, N. Krivova, P. Amaro-Seoane, P. Eggenberger, P. Eigm\\\"uller, P. Figueira, P. Giommi, P. J. Wheatley, P. Marcos-Arenal, P. M. Marrese, P. P\\'apics, P. Petit, P. Ventura, R. A. Garc\\'ia, R. Burston, R. Farmer, R. F. D\\'iaz, R. Helled, R.-M. Ouazzani, R. P. Church, R. P. Nelson, R. Ragazzoni, R. Redmer, R. Silvotti, R. Szab\\'o, S. Barnes, S. Brun, S. Cassisi, S. Charpinet, S. C. Werner, S. Dreizler, S. D. Vauclair, S. Feltzing, S. G. Sousa, S. Hekker, S. Mathis, S. Mathur, S. Messina, S. Reffert, S. Salmon, S. Schuh, Su\\'arez, S. Udry, Sz. Csizmadia, T. Appourchaux, T. Forveille, T. Granzer, T. Morel, U. Kolb, V. Adibekyan, V. C. Parro, V. Nascimbeni, V. Van Grootel, W. Ball, W. Benz, W. Chaplin, W. Kley, X. Bonfils, Y. Alibert, Y. Lebreton","submitted_at":"2013-10-02T13:17:06Z","abstract_excerpt":"PLATO 2.0 has recently been selected for ESA's M3 launch opportunity (2022/24). Providing accurate key planet parameters (radius, mass, density and age) in statistical numbers, it addresses fundamental questions such as: How do planetary systems form and evolve? Are there other systems with planets like ours, including potentially habitable planets? The PLATO 2.0 instrument consists of 34 small aperture telescopes (32 with 25 sec readout cadence and 2 with 2.5 sec candence) providing a wide field-of-view (2232 deg2) and a large photometric magnitude range (4-16 mag). It focusses on bright (4-1"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.0696","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}