KW Sagittarii

from Wikipedia, the free encyclopedia
Star
KW Sagittarii
AladinLite
Observation
dates equinoxJ2000.0 , epoch : J2000.0
Constellation Sagittarius
Right ascension 17 h 52 m 0.73 s
declination −28 ° 01 ′ 20.5 ″
Apparent brightness 8.58 likes
Typing
Spectral class M0 I-M4 Ia
Variable star type SRC 
Astrometry
Radial velocity (−7.4) km / s
parallax (0.53 ± 0.14)  mas
distance (6200   +2200−1300Ly
(1,900)  pc
Proper movement 
Rec. Share: (+0.39 ± 1.20)  mas / a
Dec. portion: (−1.62 ± 0.76)  mas / a
Physical Properties
Dimensions (20 to 40)  M
radius (1009 ± 142)  R
Luminosity

(170000   +170000−80000L

Effective temperature (3720 ± 183)  K.
Other names
and catalog entries
Cordoba Survey CD −27 ° 12032
Henry Draper Catalog HD 316496 [1]
Hipparcos catalog HIP 87433 [2]
Tycho catalog TYC 6849-57-1 [3]Template: Infobox star / maintenance / specification of the TYC catalog
Other names KW Sagittarii

KW Sagittarii is a red supergiant in our Milky Way . It is about 9,800 light years from our Sun and one of the largest known stars .

The "KW" part of the name follows the rules for naming variable stars and states that KW Sagittarii is the 256th variable star discovered in the constellation Sagittarius .

Web links

Individual evidence

  1. a b c KW Sgr. In: SIMBAD . Center de Données astronomiques de Strasbourg , accessed September 9, 2018 .
  2. ^ Hipparcos catalog (ESA 1997)
  3. a b KW Sgr. In: VSX. AAVSO, accessed September 9, 2018 .
  4. ^ Hipparcos, the New Reduction (van Leeuwen, 2007)
  5. a b c d B. Arroyo-Torres, M. Wittkowski, JM Marcaide, PH Hauschildt: The atmospheric structure and fundamental parameters of the red supergiants AH Scorpii, UY Scuti, and KW Sagittarii. Astronomy and Astrophysics , June 2013, accessed February 24, 2015 .