Puneet Varma (Editor)

KW Sagittarii

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Luminosity (bolometric)
  
176,000-360,000 L☉

Constellation
  
Magnitude
  
11

Apparent magnitude (V)
  
11

KW Sagittarii httpsuploadwikimediaorgwikipediacommonsdd

Similar
  
V354 Cephei, KY Cygni, WOH G64, VX Sagittarii, RW Cephei

KW Sagittarii is a red supergiant, located approximately 2,400 parsecs away from our Sun in the direction of the constellation Sagittarius. It has a size of 1,009 R (up to 1,460 R by some estimates), making it one of the largest known stars. If placed at the center of the Solar System, the star's surface would engulf Mars.

Contents

Dani bosco kw sagittarii original mix


Distance

The distance of 2,400 parsecs is based on the assumption of membership on the Sagittarius OB5 association. The parallax derived from the Hipparcos mission is negative so doesn't give much information about the distance except that it is likely to be large.

Characteristics

Levesque calculate that the star has a bolometric luminosity of over 360,000 L and a radius around 1,460 R based on the assumption of an effective temperature of 3,700 K. Marcaide calculate that the star has a bolometric luminosity of less than 200,000 L based on the measured flux and an assumed distance, and a radius around 1,009 ± 142 R based on the measured angular diameter and luminosity. The effective temperature was then derived from the luminosity and radius.

References

KW Sagittarii Wikipedia