Encyclopedia of Astrobiology

2015 Edition
| Editors: Muriel Gargaud, William M. Irvine, Ricardo Amils, Henderson James (Jim) CleavesII, Daniele L. Pinti, José Cernicharo Quintanilla, Daniel Rouan, Tilman Spohn, Stéphane Tirard, Michel Viso

PLATO 2.0 Satellite

Reference work entry
DOI: https://doi.org/10.1007/978-3-662-44185-5_1760

Synonyms

Definition

PLATO 2.0 (PLAnetary Transits and Oscillations of stars) is a mission for the detection and characterization (radius, mass, age) of transiting exoplanets at orbital distances up to the habitable zone of solar-like stars. In addition, PLATO 2.0 will study the stellar structure through asteroseismology.

Overview

PLATO 2.0 is the first space mission designed for the simultaneous search for transiting exoplanets and study of their host stars through  asteroseismology (Rauer et al. 2014). Selected as the 3rd mission of the cosmic vision science programe of ESA, it is planned for a launch in 2024, PLATO 2.0 will be developed in a partnership between  ESA(providing the spacecraft, launch, and elements of the operation) and a scientific consortium (providing the payload, including the telescopes, elements of the operations, and scientific planning), led by Germany (DLR) and consisting of elements from essentially all of the...

Keywords

Exoplanet Transit Asteroseismology Stars 
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References and Further Reading

  1. Alonso R, Guillot T, Mazeh T et al (2009a) The secondary eclipse of the transiting exoplanet CoRoT-2b. Astron Astrophys 501:23–26ADSCrossRefGoogle Scholar
  2. Alonso R, Alapini A, Aigrain S et al (2009b) The secondary eclipse of CoRoT-1b. Astron Astrophys 506:331–336ADSCrossRefGoogle Scholar
  3. Baglin A et al (2007) The CoRoT mission and its scientific objectives. AIP Conf Proc 895:201–209ADSCrossRefGoogle Scholar
  4. Basri G, Borucki WJ, Koch D (2005) The Kepler mission: a wide-field transit search for terrestrial planets. New Astron Rev 49(7–9 Special Issue):478–485ADSCrossRefGoogle Scholar
  5. Rauer H, Catala C, Aerts C et al (2014) The PLATO 2.0 mission. Exp Astron. 38, 249–330, doi:10.1007/s10686-014-9383-4Google Scholar

Copyright information

© Springer-Verlag Berlin Heidelberg 2015

Authors and Affiliations

  1. 1.German Aerospace Center (DLR)BerlinGermany
  2. 2.Max-Planck-Institut für AstronomieHeidelbergGermany