UVCaluetta

UVCaluetta is a proposed but unconfirmed exoplanet. Its existence is hypothesized based on observations made by the Kepler space telescope. The designation suggests it is a planet orbiting the star Kepler-445. Researchers detected a dip in the star's brightness, indicating a potential transit of a planet across its face. The amount of dimming and the frequency of these dips led to estimates of UVCaluetta's size and orbital period. Initial analyses placed it as a super-Earth, larger than our planet but smaller than Neptune. Its estimated orbital period was relatively short, suggesting it orbits its star at a close distance. However, the signal was weak, and further observations or confirmations have not yet been published. The scientific community generally treats UVCaluetta as a candidate planet, awaiting more definitive data. If confirmed, its properties would contribute to understanding planetary formation and diversity around stars similar to our Sun. The research leading to its potential discovery is part of ongoing efforts to catalog exoplanets within and beyond our solar system, with the goal of identifying potentially habitable worlds.