The Planetary Transits and Oscillations of stars (PLATO) mission was selected by ESA’s Science Program Committee for implementation as part of its Cosmic Vision 2015–25 Program.
The mission will address two key themes of Cosmic Vision: What are the conditions for planet formation and the emergence of life, and how does the solar system work?
PLATO will monitor relatively nearby stars, searching for tiny, regular dips in brightness as their planets transit in front of them, temporarily blocking out a small fraction of the starlight.
By using 34 separate small telescopes and cameras, PLATO will search for planets around a million stars spread over half of the sky.
It also will investigate seismic activity in the stars, enabling a precise characterization of the host sun of each planet discovered, including its mass, radius, and age.
When coupled with ground-based radial velocity observations, PLATO’s measurements will allow scientists to calculate a planet’s mass and radius, and therefore its density, providing an indication of its composition.
The mission will identify and study thousands of exoplanetary systems, with an emphasis on discovering and characterizing Earth-sized planets and super-Earths in the habitable zone of their parent stars — the distance from a star where liquid surface water could exist.
“PLATO, with its unique ability to hunt for Sun-Earth analog systems, will build on the expertise accumulated with a number of European missions, including CoRoT and Cheops,” said Alvaro Giménez from ESA.
“Its discoveries will help to place our solar system’s architecture in the context of other planetary systems.
“All M3 mission candidates presented excellent opportunities for answering the major scientific questions that define our Cosmic Vision Program.”
The four other mission concepts competing for the M3 launch opportunity were the Exoplanet Characterization Observatory (EChO), the Large Observatory For x-ray Timing (LOFT), MarcoPolo-R (to collect and return a sample from a near-Earth asteroid), and Space-Time Explorer and QUantum Equivalence principle Space Test (STE-Quest).
PLATO joins Solar Orbiter and Euclid, which were chosen in 2011 as ESA’s first M-class missions. Solar Orbiter will be launched in 2017 to study the Sun and solar wind from a distance of less than 31 million miles (50 million kilometers), while Euclid, to be launched in 2020, will focus on dark energy, dark matter, and the structure of the universe.
PLATO will be launched on a Soyuz rocket from Europe’s Spaceport in Kourou by 2024 for an initial six-year mission. It will operate from L2, a virtual point in space 930,000 miles (1.5 million km) beyond Earth as seen from the Sun.
Data from ESA’s recently launched Gaia mission will help PLATO provide precise characteristics of thousands of exoplanet systems. These systems will provide natural targets for detailed follow-up observations by future large ground- and space-based observatories.
