NGC 2132
NGC 2132 is a bright open star cluster located in the constellation of Hydra. It is approximately 2,000 light-years away from Earth and contains several young, hot stars. The cluster is notable for its relatively high concentration of stars, making it an interesting target for amateur astronomers.
Discovered by John Herschel in 1834, NGC 2132 is part of a larger group of star clusters in the Milky Way. Its stars are primarily composed of hydrogen and helium, typical of young stellar populations. Observations of NGC 2132 can provide insights into stellar formation and evolution.