NGC_1883 is an open star cluster located in the constellation of Puppis. It was discovered by the astronomer John Herschel in 1834 and is approximately 4,000 light-years away from Earth. The cluster contains several hundred stars, many of which are relatively young and bright. The stars in NGC_1883 are primarily composed of hydrogen and helium, typical of open clusters. It is part of a larger group of clusters known as the Puppis constellation, which is rich in stellar formations. Observations of NGC_1883 contribute to our understanding of stellar evolution and the dynamics of star clusters.