Lacaille 9352 is a red dwarf star located approximately 10.74 light-years away from Earth in the constellation of Lupus. It is part of the Lacaille catalog, which was created by the French astronomer Nicolas Louis de Lacaille in the 18th century. This star is relatively small and cool compared to our Sun, with a surface temperature of about 3,200 Kelvin. Discovered in 1752, Lacaille 9352 is notable for being one of the closest stars to our solar system. It has a low luminosity, making it difficult to observe without a telescope. The star is of particular interest to astronomers studying the characteristics of red dwarfs and their potential for hosting exoplanets.