Journal article
The PLATO mission
- Abstract:
- PLATO (PLAnetary Transits and Oscillations of stars) is ESA’s M3 mission designed to detect and characterise extrasolar planets and perform asteroseismic monitoring of a large number of stars. PLATO will detect small planets (down to <2REarth) around bright stars (<11 mag), including terrestrial planets in the habitable zone of solar-like stars. With the complement of radial velocity observations from the ground, planets will be characterised for their radius, mass, and age with high accuracy (5%, 10%, 10% for an Earth-Sun combination respectively). PLATO will provide us with a large-scale catalogue of well-characterised small planets up to intermediate orbital periods, relevant for a meaningful comparison to planet formation theories and to better understand planet evolution. It will make possible comparative exoplanetology to place our Solar System planets in a broader context. In parallel, PLATO will study (host) stars using asteroseismology, allowing us to determine the stellar properties with high accuracy, substantially enhancing our knowledge of stellar structure and evolution. The payload instrument consists of 26 cameras with 12cm aperture each. For at least four years, the mission will perform high-precision photometric measurements. Here we review the science objectives, present PLATO‘s target samples and fields, provide an overview of expected core science performance as well as a description of the instrument and the mission profile towards the end of the serial production of the flight cameras. PLATO is scheduled for a launch date end 2026. This overview therefore provides a summary of the mission to the community in preparation of the upcoming operational phases.
- Publication status:
- Published
- Peer review status:
- Peer reviewed
Actions
Access Document
- Files:
-
-
(Preview, Version of record, pdf, 6.0MB, Terms of use)
-
- Publisher copy:
- 10.1007/s10686-025-09985-9
Authors
+ Belgian Federal Science Policy Office
More from this funder
- Funder identifier:
- https://ror.org/01fapfv42
+ French National Centre for Scientific Research
More from this funder
- Funder identifier:
- https://ror.org/02feahw73
- Publisher:
- Springer
- Journal:
- Experimental Astronomy More from this journal
- Volume:
- 59
- Issue:
- 3
- Article number:
- 26
- Publication date:
- 2025-04-21
- Acceptance date:
- 2025-02-07
- DOI:
- EISSN:
-
1572-9508
- ISSN:
-
0922-6435
- Language:
-
English
- Keywords:
- Source identifiers:
-
2875573
- Deposit date:
-
2025-04-21
This ORA record was generated from metadata provided by an external service. It has not been edited by the ORA Team.
If you are the owner of this record, you can report an update to it here: Report update to this record