Olossatilassa

Olossatilassa is a proposed but not yet confirmed exoplanet candidate located in the Cygnus constellation. It is believed to be orbiting a G-type main-sequence star, similar to our Sun. The existence of Olossatilassa was first suggested by data from the Kepler Space Telescope, which searches for exoplanets by detecting the slight dimming of a star as a planet passes in front of it.

The potential exoplanet's size and mass are estimated to be roughly 1.5 times that of Earth, placing it in the super-Earth category. Its orbital period is thought to be approximately 30 Earth days, suggesting it is located within the habitable zone of its star, the region where temperatures might allow for liquid water to exist on the surface.

However, Olossatilassa has not yet been definitively confirmed through follow-up observations by other telescopes. Further studies are required to validate its existence and to gather more information about its atmospheric composition and potential habitability. If confirmed, Olossatilassa would join a growing list of exoplanets that scientists are studying to understand the diversity of planetary systems beyond our own. The name itself is a placeholder, as official naming conventions are typically applied after confirmation.