NGC 1805 is a bright star cluster located in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. It is situated approximately 163,000 light-years away from Earth and is known for its rich population of young, hot stars. The cluster is estimated to be around 40 million years old. This star cluster is part of a larger region of star formation and is often studied to understand the processes of stellar evolution. NGC 1805 is particularly notable for its high concentration of blue supergiants, which are massive stars that burn brightly and have relatively short lifespans.