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PLATO Mission

PLATO (PLAnetary Transits and Oscillations of stars) is a medium-class mission in ESA’s Cosmic Vision program. 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. PLATO has also been designed to investigate seismic activity in stars, enabling the precise characterization of the planet host star, including its age.

Two DLR institutes are contributing to the PLATO Mission: The principal investigator, Prof. Dr. Heike Rauer, is from the DLR-Institute of Planetary Research. Several key positions in the project are held by engineers of the Institute of Optical Sensor Systems and several major work packages are assigned to the Institute, above all those for system engineering: OS is responsible for the payload systems engineering, modelling and verification of the payload performance and the data processing system including fine guidance system for highly accurate alignment of the satellite in orbit.

The launch of PLATO is planned in 2026.

Plato Scientific Goals

PLATO (PLAnetary Transits and Oscillations of stars) is the third medium-class mission in ESA's Cosmic Vision program. 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.

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PLATO Mission

PLATO is the M3 mission in the Cosmic Vision 2015-2025 Program of the European Space Agency. With 26 telescopes of 20 cm class, that all togheter collect photons like a telescope of 1 m class covering a field of view 10,000 times the area of the full Moon, it will survey the brightest stars in the sky for transiting planets.

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PLATO Payload Organization

The payload is developed by the payload mission consortium in Europe under the lead of ESA. The satellite is built by an industrial consortium led by OHB as prime contracted by ESA. The launch of the satellite is planned for 2026.

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PLATO Design

PLATO has been designed to investigate seismic activity in stars, enabling the precise characterization of the planet host star, including its age.

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Involved Institutes & Partners
Plato Publications
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