PLATO – Searching for a second Earth

ESA Mission PLATO

PLATO searching for exoplanets

In early 2027, PLATO (PLAnetary Transits and Oscillations of stars) will begin its search for Earth-sized planets. Its stated aim is to find Earth-like planets orbiting a Sun-like star within the habitable zone. These could include planets on which life has developed or could develop.

In early 2027, PLATO (PLAnetary Transits and Oscillations of stars) will begin its search for Earth-sized planets. Its stated aim is to find Earth-like planets orbiting a Sun-like star within the habitable zone. These could include planets on which life has developed or could develop.

It may allow us to answer questions that previous generations asked themselves:

  • Is our solar system unique?
  • Are there planets orbiting other stars that offer conditions suitable for life?
  • How do planets and planetary systems form and evolve?

PLATO is an M3 mission of the European Space Agency (ESA) under the Cosmic Vision programme, selected in 2014. The German Aerospace Centre (DLR) leads the international consortium and the consortium is responsible together with ESA for the construction of the science payload. Furthermore DLR contributes to the mission operation under the ESA leadership.

Using a special telescope design comprising 26 individual cameras, PLATO will observe a large field of view for more than two years. It will record the brightness curves of thousands of stars and search for periodic dips in these light curves. This method, known as the transit method, allows us to discover planets, as when they pass between the star and the telescope, they cause a slight dimming of the star’s light.  Of great interest are the planets that lie within the habitable zone of their star. In this zone, liquid water could exist on the surface of a rocky planet.

To detect the very small dips in brightness caused by a planet, PLATO must be very precisely aligned with the sky and continuously measure the brightness of tens of thousands of stars. By carefully analysing the light curves and making further measurements with ground-based telescopes, it is possible to precisely determine the planet’s radius and mass, as well as the age of the planetary system.

This marks the first time that a very large number of planetary systems have been characterised with such high accuracy. This will give us a better understanding of how planets form, how stars and planetary systems evolve, and whether there are life-friendly conditions anywhere beyond our solar system.

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Dr. Juan Cabrera Perez

Department Head
Institute of Space Research
Extrasolar Planets and Atmospheres
Rutherfordstr. 2, 12489 Berlin

Dipl.-Ing. (FH) Gisbert Peter

Department Head
Institute of Space Research
Space Instruments
Rutherfordstraße 2, 12489 Berlin-Adlershof

Dr. Matthias Grott

Department Head
Institute of Space Research
Planetary Sensor Systems
Rutherfordstr. 2, 12489 Berlin

Dr David Krutz

Head of Department Space Instruments
Institute of Space Research
Optical Sensors and Electronics
Rutherfordstraße 2, 12489 Berlin-Adlershof