These phenomena lie far beyond j Centauri, though the star itself is nonetheless relatively distant from the Sun at an estimated 710 light years. This is a main-sequencestar, but nonetheless a much hotter and more luminous such star than the Sun. The spectrum of j Centauri implies that it belongs to the class known as 'Be stars', stars that rotate at an unusually rapid rate, and are commonly surrounded by rings or shells of matter.