The LHS 1140 System is a star system located approximately 40 light-years away in the constellation of Centaurus. It consists of a red dwarf star, known as LHS 1140, which is smaller and cooler than our Sun. This system has gained interest due to its potential for hosting exoplanets. Within the LHS 1140 System, two confirmed exoplanets, LHS 1140 b and LHS 1140 c, have been identified. Both planets are classified as super-Earths, meaning they are larger than Earth but smaller than gas giants. Their proximity to the host star makes them intriguing candidates for studying planetary atmospheres and potential habitability.