Gamma Telescopii is a binary star system located in the constellation of Telescopium. It is approximately 130 light-years away from Earth and consists of two stars that orbit each other. The system is classified as a spectroscopic binary, meaning that the stars are too close together to be resolved individually through a telescope. The primary star in Gamma Telescopii is a B-type main-sequence star, which is hotter and more massive than our Sun. The secondary star is less massive and cooler. Together, they provide valuable insights into stellar evolution and the dynamics of binary systems in the universe.