PLAnetary Transits and Oscillations of stars space mission

PLATO
PLATO
Owner institution

    Para conseguir los objetivos, PLATO estará equipado con 26 telescopios de pequeño formato, cada uno de ellos con 4 detectores tipo CCD con un total de 80 millones de píxeles. PLATO observará las mismas estrellas durante largos periodos, de hasta 3 años, desde su posición orbital en el punto de Lagrange L2, a 1,5 millones de km de la Tierra.

    Related Projects

    • Componentes del experimento PLATO
      PLATO (PLAnetary Transits and Oscillations of stars)
      PLAnetary Transits and Oscillations of stars (PLATO) is the third medium-class mission in ESA's Cosmic Vision programme. Its objective is to find and study a large number of extrasolar planetary systems, with emphasis on the properties of terrestrial planets in the habitable zone around solar-like stars
      Hans Jörg
      Deeg Deeg

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