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    Mission Summary

    PLATO
    PLAnetary Transits and Oscillations of stars
    Theme What are the conditions for planet formation and the emergence of life?
    Primary Goal Discover and characterise a large number of close-by exoplanetary systems, with a precision in the determination of mass and radius of 1%
    Targets
  • Detect Earth sized planets around solar-type stars
  • Detect super-earths around solar-type stars
  • Measure solar oscillations in the host stars of exoplanets
  • Measure oscillations of classical pulsators
  • Wavelength Optical
    Telescope A number of small, optically fast, wide-field telescopes
    Orbit Large amplitude libration orbit around Sun-Earth Lagrangian point, L2
    Lifetime min. 6 years
    Partners To be confirmed
    Type M-class Mission

    Mission home: http://sci.esa.int/plato

    NEWS AND ANNOUNCEMENTS
    Dark and bright: ESA chooses next two science missions
    ESA chooses three scientific missions for further study

     

     

    NEWS FEED
    Stay up to date: Cosmic Vision 2015-2025
    RSS feed
    HIGHLIGHTS
    M-class missions presentation event 2009
    (1 Dec 2009)
    LATEST PUBLICATIONS
    PLATO definition study report, ESA/SRE(2011)13
    PLATO Mission Assessment Study - Executive Summary (Thales)
    PLATO Mission Assessment Study - Executive Summary (EADS Astrium)
    ESA Technical Review Report - PLATO (SRE-PA/2009.081)
    PLATO Assessment Study Report (ESA/SRE-2009-4)


    Last Update: 21 Feb 2012

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