Supergiants form initially the same way other regular stars do, from a cloud of [[hydrogen]] gas and interstellar dust that compresses under its gravitational attraction until the center of the cloud is hot enough to fuse hydrogen at its core. What determines if a star will become a supergiant is the amount of mass the star contains. A star needs to contain at least ten solar masses in order to evolve into a supergiant.<ref>http://encarta.msn.com/encyclopedia_761587630/Supergiant_%28star%29.html</ref> | Supergiants form initially the same way other regular stars do, from a cloud of [[hydrogen]] gas and interstellar dust that compresses under its gravitational attraction until the center of the cloud is hot enough to fuse hydrogen at its core. What determines if a star will become a supergiant is the amount of mass the star contains. A star needs to contain at least ten solar masses in order to evolve into a supergiant.<ref>http://encarta.msn.com/encyclopedia_761587630/Supergiant_%28star%29.html</ref> |