The PLATO mission, part of the Cosmic Vision Programme M3 mission set for launch in 2026, aims to detect and characterize terrestrial exoplanets in habitable zones of solar-type stars. Utilizing a multi-camera approach with 24 Normal Cameras and two Fast Cameras, the mission's payload is designed to monitor a vast field of stars in the extended visible light range. This innovative approach ensures thermal and structural stability, optimizing the observation of numerous targets across varying brightness levels, thereby enhancing the mission's scientific yield.

J. Farinato, V.V. (2018). TOU Prototype Assembly and Integration Report.

TOU Prototype Assembly and Integration Report

G. Umbriaco;
2018

Abstract

The PLATO mission, part of the Cosmic Vision Programme M3 mission set for launch in 2026, aims to detect and characterize terrestrial exoplanets in habitable zones of solar-type stars. Utilizing a multi-camera approach with 24 Normal Cameras and two Fast Cameras, the mission's payload is designed to monitor a vast field of stars in the extended visible light range. This innovative approach ensures thermal and structural stability, optimizing the observation of numerous targets across varying brightness levels, thereby enhancing the mission's scientific yield.
2018
J. Farinato, V.V. (2018). TOU Prototype Assembly and Integration Report.
J. Farinato, V. Viotto, M. Bergomi, L. Marafatto, D. Piazza, D. Magrin, R. Ragazzoni, F. Biondi, D. Greggio, G. Umbriaco, S Chinellato, D. Vassallo
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/958654
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