The debris, or dust, disk that surrounds Fomalhaut was first discovered in 1983. The disk itself has a very defined inner edge at 133 AU from the star. Because the disk is inclined at some 24 degrees from the plane of the star system, it appears to have a toroidal shape. The disk is seen as a younger version of our own [[Kuiper Belt]].<ref>http://arxiv.org/abs/astro-ph/0506574</ref> It was the observations of the debris disk that lead scientists to first conclude there was likely a planet just inside the inner edge of the disk. | The debris, or dust, disk that surrounds Fomalhaut was first discovered in 1983. The disk itself has a very defined inner edge at 133 AU from the star. Because the disk is inclined at some 24 degrees from the plane of the star system, it appears to have a toroidal shape. The disk is seen as a younger version of our own [[Kuiper Belt]].<ref>http://arxiv.org/abs/astro-ph/0506574</ref> It was the observations of the debris disk that lead scientists to first conclude there was likely a planet just inside the inner edge of the disk. |