Paper
6 July 2018 PLATO: the ESA mission for exo-planets discovery
Demetrio Magrin, Roberto Ragazzoni, Heike Rauer, Isabella Pagano, Valerio Nascimbeni, Giampaolo Piotto, Valentina Viotto, Daniele Piazza, Timothy Bandy, Stefano Basso, Willy Benz, Maria Bergomi, Federico Biondi, Francesco Borsa, Anko Börner, Alexis Brandeker, Mathias Brändli, Giordano Bruno, Juan Cabrera, Flavia Calderone, Virginie Cessa, Simonetta Chinellato, Thierry De Roche, Marco Dima, Anders Erikson, Jacopo Farinato, Mauro Ghigo, Davide Greggio, Maximilian Klebor, Luca Marafatto, Matteo Munari, Valery Mogulsky, Martin Pertenais, Gisbert Peter, Elisa Portaluri, Martin Rieder, Steve Rockstein, Mario Schweitzer, Daniela Sicilia, Gabriele Umbriaco, Matthias Wieser, Ana M. Heras, Filippo Marliani, Simone Pirrotta, Mario Salatti, Elisabetta Tommasi, Riccardo Bardazzi, Enrico Battistelli, Mauro Brotini, Matteo Burresi, Emanuele Capuano, Massimo Marinai, Andrea Novi, Claude Català
Author Affiliations +
Abstract
PLATO (PLAnetary Transits and Oscillation of stars) is the ESA Medium size dedicated to exo-planets discovery, adopted in the framework of the Cosmic Vision program. The PLATO launch is planned in 2026 and the mission will last at least 4 years in the Lagrangian point L2. The primary scientific goal of PLATO is to discover and characterize a large amount of exo-planets hosted by bright nearby stars, constraining with unprecedented precision their radii by mean of transits technique and the age of the stars through by asteroseismology. By coupling the radius information with the mass knowledge, provided by a dedicated ground-based spectroscopy radial velocity measurements campaign, it would be possible to determine the planet density. Ultimately, PLATO will deliver the largest samples ever of well characterized exo-planets, discriminating among their ‘zoology’. The large amount of required bright stars can be achieved by a relatively small aperture telescope (about 1 meter class) with a wide Field of View (about 1000 square degrees). The PLATO strategy is to split the collecting area into 24 identical 120 mm aperture diameter fully refractive cameras with partially overlapped Field of View delivering an overall instantaneous sky covered area of about 2232 square degrees. The opto-mechanical sub-system of each camera, namely Telescope Optical Unit, is basically composed by a 6 lenses fully refractive optical system, presenting one aspheric surface on the front lens, and by a mechanical structure made in AlBeMet.
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Demetrio Magrin, Roberto Ragazzoni, Heike Rauer, Isabella Pagano, Valerio Nascimbeni, Giampaolo Piotto, Valentina Viotto, Daniele Piazza, Timothy Bandy, Stefano Basso, Willy Benz, Maria Bergomi, Federico Biondi, Francesco Borsa, Anko Börner, Alexis Brandeker, Mathias Brändli, Giordano Bruno, Juan Cabrera, Flavia Calderone, Virginie Cessa, Simonetta Chinellato, Thierry De Roche, Marco Dima, Anders Erikson, Jacopo Farinato, Mauro Ghigo, Davide Greggio, Maximilian Klebor, Luca Marafatto, Matteo Munari, Valery Mogulsky, Martin Pertenais, Gisbert Peter, Elisa Portaluri, Martin Rieder, Steve Rockstein, Mario Schweitzer, Daniela Sicilia, Gabriele Umbriaco, Matthias Wieser, Ana M. Heras, Filippo Marliani, Simone Pirrotta, Mario Salatti, Elisabetta Tommasi, Riccardo Bardazzi, Enrico Battistelli, Mauro Brotini, Matteo Burresi, Emanuele Capuano, Massimo Marinai, Andrea Novi, and Claude Català "PLATO: the ESA mission for exo-planets discovery", Proc. SPIE 10698, Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave, 106984X (6 July 2018); https://doi.org/10.1117/12.2313538
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CITATIONS
Cited by 4 scholarly publications.
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KEYWORDS
Cameras

Planets

Stars

Exoplanets

Space telescopes

Telescopes

Optical filters

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