Kepler445

Kepler-445 is an exoplanet orbiting the star Kepler-445. It was discovered by NASA's Kepler Space Telescope. The planet is a super-Earth, meaning it is larger than Earth but smaller than Neptune. Kepler-445 is located approximately 700 light-years away from Earth in the constellation Cygnus.

The exoplanet orbits its star within the habitable zone, the region where conditions might be right for liquid water to exist on the surface of a planet. This makes Kepler-445 a candidate for further study in the search for extraterrestrial life. However, its exact composition and atmospheric properties are not yet known, and further observations are needed to determine its habitability.

Kepler-445 has an orbital period of about 30 Earth days. Its host star, Kepler-445, is a G-type star, similar to our Sun, though slightly cooler and smaller. The discovery of Kepler-445 was part of the Kepler mission's ongoing efforts to find Earth-sized planets in the habitable zones of other stars. Scientists use the transit method to detect these planets, observing the slight dimming of a star's light as a planet passes in front of it.