V602 Kiel - a variable star and a red supergiant in the constellation Kiel .
| V602 Kiel | |||
|---|---|---|---|
| Star | |||
 Star location | |||
| Observational data ( Age J2000.0 ) | |||
| Type of | Red supergiant , variable star | ||
| Right ascension | |||
| Declination | |||
| Distance | 6524 St. years (1977 pc ) [2] | ||
| Visible magnitude ( V ) | 8.39 [3] (7.6 - 9.1) [4] | ||
| Constellation | Keel | ||
| Astrometry | |||
| Own movement (μ) | RA: −7.4 [5] Dec: 0.2 [5] | ||
| Absolute magnitude (V) | −5.85 [6] | ||
| Specifications | |||
| Spectral class | M3 Ia-Iab [7] | ||
| Color Index ( B - V ) | +2.52 [3] | ||
| Color Index ( U - B ) | +2.59 [3] | ||
| Variability | SRc [4] | ||
| physical characteristics | |||
| Weight | 17.7 [8] M ☉ | ||
| Radius | 1050 [2] R ☉ | ||
| Temperature | 3432 [2] K | ||
| Luminosity | 138000 [2] L ☉ | ||
| |||
| Database Information | |||
| SIMBAD | data | ||
Features
A star radiates a huge amount of energy. It is assumed that it is surrounded by a giant cloud of dust [9] . V602 Kiel is located from the Sun at a distance of 6524 St. years old . The temperature is 3432 K. The mass of the star is about 18 solar . It shines brighter than the Sun more than 100 thousand times, and the radius is 1050 solar , which allows us to attribute this star to the largest of the known .
See also
- List of the biggest stars
- M Kiel
- PP keel
Notes
- ↑ 1 2 Hog, E .; Kuzmin, A .; Bastian, U .; Fabricius, C .; Kuimov, K .; Lindegren, L .; Makarov, VV; Roeser, S. (1998). "The TYCHO Reference Catalog". Astronomy and Astrophysics. 335: L65. (eng.)
- ↑ 1 2 3 4 Arroyo-Torres, B .; Wittkowski, M .; Chiavassa, A .; Scholz, M .; Freytag, B .; Marcaide, JM; Hauschildt, PH; Wood, PR; Abellan, FJ (2015). "What causes the large extensions of red supergiant atmospheres ?. Comparisons of interferometric observations with 1D hydrostatic, 3D convection, and 1D pulsating model atmospheres." Astronomy & Astrophysics. 575: A50. (eng.)
- ↑ 1 2 3 Mauron, N .; Josselin, E. (February 2011), "The mass-loss rates of red supergiants and the de Jager prescription", Astronomy and Astrophysics, 526: A156. (eng.)
- ↑ 1 2 Samus, NN; Durlevich, OV; et al. (2009). "VizieR Online Data Catalog: General Catalog of Variable Stars (Samus + 2007-2013)." VizieR On-line Data Catalog: B / gcvs. Originally published in: 2009yCat .... 102025S. 1. (English)
- ↑ 1 2 Høg, E .; Fabricius, C .; Makarov, VV; Urban, S .; Corbin, T .; Wycoff, G .; Bastian, U .; Schwekendiek, P .; Wicenec, A. (2000). "The Tycho-2 catalog of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27. (eng.)
- ↑ Levesque, Emily M .; Massey, Philip; Olsen, KAG; Plez, Bertrand; Josselin, Eric; Maeder, Andre; Meynet, Georges (2005). "The Effective Temperature Scale of Galactic Red Supergiants: Cool, but Not as Cool as We Thought." The Astrophysical Journal. 628 (2): 973–985. (eng.)
- ↑ Keenan, Philip C .; McNeil, Raymond C. (1989). "The Perkins catalog of revised MK types for the cooler stars." Astrophysical Journal Supplement Series. 71: 245. (English)
- ↑ Fadeyev, Yu. A. (2012). "Nonlinear pulsations of red supergiants." Astronomy Letters. 38 (4): 260-270. (eng.)
- ↑ Humphreys, Roberta M .; Strecker, Donald W .; Ney, EP (February 1972), "Spectroscopic and Photometric Observations of M Supergiants in Carina", Astrophysical Journal, 172: 75 .