UY Scuti

From Wikipedia, the free encyclopedia
Jump to navigation Jump to search
Dense starfield around the red hypergiant star UY Scuti. It is the brightest star in the image. Taken at the Rutherfurd Observatory in Columbia University, New York, 2011

UY Scuti is a red supergiant (RSG) or red Hypergiant (RHG) star. It is a pulsating variable star in the constellation Scutum and possibly the largest known star in the Milky Way Galaxy. It is also one of the most luminous and well-known of its kind.[1][2]

The star has an estimated average median radius of 1,708 times that of the Sun, or a diameter of 2.4 billion km (1.5 billion mi; 15.9 AU); thus a volume 5 billion times that of the Sun.

It is about 2.9 kiloparsecs (9,500 light years) from Earth, so it is one of the nearest known hypergiants.[3] If placed at the center of the Solar system, its photosphere would engulf the orbit of Jupiter. The radius is not known for certain, and may be larger than the orbit of Saturn.

References[change | change source]

  1. International Variable Star Index. "Detail for UY Sct". [1]
  2. Arroyo-Torres B. et al 2013. The atmospheric structure and fundamental parameters of the red supergiants AH Scorpii, UY Scuti, and KW Sagittarii. Astronomy & Astrophysics 554: A76. [2]
  3. Jura M. & Kleinmann S.G. 1990. Mass-losing M supergiants in the solar neighborhood. The Astrophysical Journal Supplement Series 73: 769. [3]