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Summary

Summary

 

PLATO
PLAnetary Transits and Oscillations of stars
Theme What are the conditions for planet formation and the emergence of life?
Primary Goal Detection and characterisation of terrestrial exoplanets around bright solar-type stars, with emphasis on planets orbiting in the habitable zone.
Measurements
  • Photometric monitoring of a large number of bright stars for the detection of planetary transits and the determination of the planetary radii (around 3% accuracy)
  • Ground-based radial velocity follow-up observations for the determination of the planetary masses (around 10% accuracy)
  • Asteroseismology for the determination of stellar masses, radii, and ages (up to 10% of the main sequence lifetime)
  • Identification of bright targets for spectroscopic follow-up observations of planetary atmospheres with other ground and space facilities
Wavelength Optical
Telescope A number of small, optically fast, wide-field telescopes
Orbit Large amplitude libration orbit around Sun-Earth Lagrangian point, L2
Lifetime 4 years of nominal science operations; satellite built and verified for an in-orbit lifetime of 6.5 years, accommodating consumables for 8.5 years
Type M-class Mission

 

Mission Timeline

Last Update: 1 September 2019
20-Sep-2019 15:56 UT

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https://sci.esa.int/s/AM9KdoA

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