Overview of PLATO's cameras on-ground and in-orbit calibration and characterisation

Kurzfassung

The PLAnetary Transits and Oscillations of stars mission (PLATO) is the M3 mission in ESA’s Cosmic Vision 2015-2025 Programme, see Rauer et al. (2014).1 The PLATO mission aims at detecting and characterizing extrasolar planetary systems, including terrestrial exoplanets around bright solar-type stars up to the habitable zone. In order to achieve its scientific objectives, PLATO must perform uninterrupted high precision photometric monitoring of large samples of stars during long periods to detect and characterize planetary transits. The PLATO light curves will also contain information on the seismic activity of the stars, which can help to constrain mass, radii and ages of the exoplanet host stars. The scientific payload of PLATO, developed and provided by the PLATO Mission Consortium (PMC) and ESA, is based on a multi-telescope configuration consisting of 24 Normal Cameras (N-CAM) and 2 Fast Cameras (F-CAM), so as to provide simultaneously a large field of view and a large collecting aperture. The optical design is identical for all cameras and consists of a 6-lens dioptric design with a 120 mm entrance pupil and an effective field of view of more than 1000 deg2. The calibration and characterization of PLATO’s cameras is a real challenge, especially in terms of quantities: there are 26 Flight Models + 3 Flight Spares + 2 Qualification Models and finally 1 Engineering Model to calibrate. In this context, the on-ground calibration and characterization plan of the cameras was optimized, meaning that all the measurements that can be performed in-orbit will not be calibrated on-ground. Our aim is to give an overview of the on-ground activities planned in the coming years to calibrate and characterize PLATO’s cameras. In particular, a detailed description of the geometric calibration used for the Fine Guidance System (FGS) and the focusing calibration will be given. A description of the in-flight calibration plan will then be presented to get the full overview of the calibration and characterization of PLATO’s cameras. Calibrating so many cameras in space, without any calibration targets/sources on board, only using pointing capabilities of the satellite, stellar targets and advanced data processing is a key aspect for this mission.