ESA’s mission Plato, PLAnetary Transits and Oscillations of stars, will use its 26 cameras to study terrestrial exoplanets in orbits up to the habitable zone of Sun-like stars. The mission will measure the sizes of exoplanets and discover exomoons and rings around them. Plato will also characterise planets' host stars by studying tiny light variations in the starlight it receives. Teledyne e2v supplied 104 CCD Bruyères sensors for this mission, and this presentation summarises what ESA wants to achieve and provides an update on its current progress. Jose Lorenzo Alvarez is ESA’s Plato Mission and Payload Manager.