It is believed to by a young star, only 200 million years old. The surface temperature of the star is around 8500° Kelvin, it has a mass of around 2.3 times that of Sol, 15 times the luminosity and is roughly 1.7 times the diameter. It is surrounded by an enormous disk of dust in a torus shape (5 AU to 90 AU), believed to be protoplanetary, and this emits considerable infrared radiation. A planet, designated Fomalhaut b, has been inferred from analysis of the dust cloud in 1998.
Over history there have been a large number of variations on the star's name. It was first identified in pre-history and there is archaeological evidence that it was part of rituals in 2500s BCE Persia.
Right Ascension 22 57 39.05
Declination -29 37 20
Spectral Type A3V
Apparent Magnitude 1.16
B-V Colour 0.09
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