IC 2395 is a star cluster located in the constellation of Vela in the Milky Way galaxy. It is categorized as an open cluster, meaning it is a group of stars that formed together from the same molecular cloud and are loosely bound by gravity. IC 2395 is relatively young, with an estimated age of around 45 million years, and contains over 100 stars. Research on IC 2395 primarily focuses on studying the properties and evolution of its individual stars, as well as the cluster as a whole. Scientists use various observational techniques, such as photometry and spectroscopy, to analyze the temperature, luminosity, composition, and other characteristics of the stars in IC 2395. This research helps to improve our understanding of stellar formation and evolution processes, as well as the dynamics and structure of star clusters in the Milky Way.