NGC 6752 is a globular cluster located in the constellation Pavo. It is approximately 13,000 light-years away from Earth and contains hundreds of thousands of stars, making it one of the brightest globular clusters visible from our planet. Discovered by Abraham Ihle in 1975, NGC 6752 is notable for its relatively high concentration of stars in its core. The cluster is about 10 billion years old and is a popular target for astronomers studying stellar evolution and the dynamics of star clusters.