Kepler-338 d is a charming exoplanet orbiting the star Kepler-338, discovered back in 2014 by the keen eyes of the Kepler space telescope using the clever transit method. This method involves spotting the tiny dips in a star’s brightness caused when a planet like Kepler-338 d gracefully passes in front of its host star from our vantage point. While we don’t have its exact nickname yet, Kepler-338 d floats out in the vastness of space, inviting curiosity from stargazers and space explorers alike. Thanks to the high-tech Kepler CCD Array, we’ve caught a glimpse of this distant world’s presence—an intriguing puzzle piece in our quest to understand the universe beyond our solar system.
