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The ESA mission PLATO (Planetary Transits and Oscillations of stars) has the goal to detect terrestrial exoplanets in the habitable zone of solar-type stars and characterizing their bulk properties from 2024 onwards. Even though many exoplanets have been detected over the last 20 years, non of them could be characterized as a habitable earth like planet. PLATO aims to do better and will answer the profound and captivating question: “How common are worlds like ours and are they suitable for the development of live?”.  To answer this question key information on the planet and its star are needed such as the planet radius, mean density, stellar irradiation, and planetary composition.  To do so, the mission will combine:

  1. planet detection and radius determination from photometric transits
  2. determination of planet masses from ground-based radial velocity follow up
  3. determination of accurate stellar masses, radii, and ages from asteroseismology, and
  4. identification of bright targets for atmospheric spectroscopy.

To accomplish this goal, a new type of space telescope was conceived. PLATO will make use of 34 telescopes with CCD-based focal planes, operating in white light and providing a very wide field-of-view. The telescopes can be used in different combinations or be bundled allowing the detection of bright as well as faint stars. PLATO will be launched on a Soyuz rocket from Europe’s Spaceport in Kourou in 2024 for an initial six-year mission. It will operate from L2, a virtual point in space 1.5 million km beyond Earth as seen from the sun. The first discovery of earth-like planets is expected within the first three years of observations.

The Institute of Astronomy (IoA) has been involved in this mission for over 10 years in close collaboration with scientists from different national and international institutes. Conny Aerts (expert in asteroseismology) is not only the Belgian PI of PLATO but she also represents the Belgian Science community in the board of the space mission. The Centre Spatial in Liège developed the camera system in close collaboration with the engineers from IoA who where led by Bart Vandenbussche.  Joris De Ridder is in charge for Leuven’s contribution to the software that needs to convert raw data into interpretable data. The IoA is thus involved in the three major work packages: instrumentation, software development and scientific preparations for the asteroseismic analysis. 

People involved

Conny Aerts,  Joris De Ridder, Bart Vandenbusche, Pablo Marcos ArenalRik Huygen Ehsan Moravveji, Peter PapicsSara RegiboPierre Royer, Andrew Tkachenko,  Konstanze Zwintz


Related links

PLATO simulator

PLATO Complementary Science

PLATO Homepage
ESA PLATO Information

Instrumentation Publication

Related missions:
KEPLER webpage
COROT webpage
COROT webpage (Laboratoire d'Astrophysique de Marseille)
MOST webpage

Asteroseismology in Belgium:
Belgian Asteroseismology Group


Plato in the news:

Il simulatore di PLATO


PLATO Simulator has been released

The PLATO SIMULATOR is a end-to-end simulation software tool designed for the performance of realistic simulations of the expected observations of the PLATO mission but easily adaptable to similar types of missions.

PLATO Simulator has been released - Read More…

PLATO2.0 zoekt nieuwe werelden

PLATO2.0 zoekt nieuwe werelden

Ruimtemissie met 34 telescopen zal een miljoen sterren onderzoeken

PLATO2.0 zoekt nieuwe werelden - Read More…

Searching for New Worlds with PLATO2.0

Searching for New Worlds with PLATO2.0

Space eye with 34 telescopes will investigate one million stars

Searching for New Worlds with PLATO2.0 - Read More…