NGC_2011 is an open star cluster located in the constellation Tucana. It is part of the Large Magellanic Cloud, a satellite galaxy of the Milky Way. This cluster is approximately 160,000 light-years away from Earth and contains several young, bright stars. Discovered by John Herschel in 1834, NGC 2011 is notable for its relatively high concentration of stars. The cluster is estimated to be around 200 million years old, making it a relatively young formation in astronomical terms. Observations of NGC 2011 provide valuable insights into stellar evolution and the dynamics of star clusters.