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PLAnetary Transits and Oscillations of stars (PLATO) is a space observatory developed by the European Space Agency (ESA) to discover and characterise exoplanets around bright, nearby stars, with a particular focus on Earth-sized worlds and super-Earths orbiting within the habitable zone of Sun-like stars. Operating from the Sun–Earth Lagrange point L2, the spacecraft uses a suite of 26 cameras, each built around multiple CCD detectors with maximum resolutions of around 4,500 × 4,500 pixels, enabling long-duration, high-precision monitoring of stellar brightness. Over the course of its survey, PLATO observes up to a million stars, searching for tiny dips in light caused by transiting planets. Launch's in early 2027*on an Ariane 6 rocket, PLATO conducts a four-year observing campaign that measures planetary radii and, through asteroseismology, determines stellar ages and internal properties with high accuracy. This combination allows researchers to identify the most Earth-like planetary systems discovered to date and to assemble a high-quality target list for detailed atmospheric studies by other observatories. The PLATO mission builds on data from the Gaia spacecraft, whose precise stellar measurements help refine planet candidates and system parameters.
