Hubble captures young stars in Small Magellanic Cloud

The Hubble Space Telescope has captured an amazing image of young stars forming in a cocoon of gas. This new view shows the open star cluster NGC 460, located in the Small Magellanic Cloud, a nearby dwarf galaxy. NGC 460 is surrounded by other young star clusters and nebulae, which are clouds of gas and dust that help create new stars. The area, known as N83, contains bright O-type stars. These stars are some of the hottest and most massive in our galaxy, and only about 20,000 of them are estimated to exist in the Milky Way. NASA explained that gas and dust clouds can collapse and form stars. The strong radiation and winds from young stars compress these clouds, triggering new star formation. The hydrogen clouds glow because the radiation from nearby stars ionizes them. NGC 460 is an open star cluster, meaning it is a loosely grouped collection of stars held together by gravity. It likely formed after two hydrogen clouds collided, which may have led to the birth of multiple O-type stars and nebulae in N83. NASA noted that NGC 460 is one of the youngest areas in this complex of stars and nebulae. As these stars develop, they may eventually spread out throughout the Small Magellanic Cloud. This galaxy, located about 200,000 light-years from Earth, provides a unique chance to study stellar phenomena that are not easily seen in more distant galaxies.