Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Sagittarius |
Right ascension | 18h 08m 04.04831s[2] |
Declination | −22° 13′ 26.6327″[2] |
Apparent magnitude (V) | 6.5 - 14.0[3] |
Characteristics | |
Evolutionary stage | AGB[4] |
Spectral type | M4eIa - M10eIa[5] |
Apparent magnitude (U) | 11.72 |
Apparent magnitude (B) | 9.41 |
Apparent magnitude (V) | 6.52 |
Apparent magnitude (I) | 2.11 |
Apparent magnitude (J) | 1.23 |
Apparent magnitude (H) | 0.13 |
Apparent magnitude (K) | −0.50 |
Apparent magnitude (L) | −1.61 |
Variable type | SRc[3] |
Astrometry | |
Radial velocity (Rv) | +6.47±3.37[6] km/s |
Proper motion (μ) | RA: +0.36±0.76[6] mas/yr Dec.: −2.92±0.78[6] mas/yr |
Parallax (π) | 0.64 ± 0.04 mas[6] |
Distance | 5,100 ± 300 ly (1,560 ± 100 pc) |
Details | |
Mass | 12[7] M☉ |
Radius | 1,356,[4] between 1,120 and 1,550[6], 1,350–1,940 (pulsation)[8], 1,480[9][a] R☉ |
Luminosity | 195000±62000[6] L☉ |
Temperature | 2,900[10] (near min), 3,200-3,400 (near max)[7], 2,400–3,300[8] K |
Other designations | |
Database references | |
SIMBAD | data |
VX Sagittarii is an asymptotic giant branch star located more than 1.5 kiloparsec away from the Sun in the constellation of Sagittarius. It is a pulsating variable star with an unusually large magnitude range. It is one of the largest stars discovered, with a radius varying between 1,350 and 1,940 solar radii (940,000,000 and 1.35×109 km; 6.3 and 9.0 au). It is the most luminous known AGB star, at bolometric magnitude –8.6, which is brighter than the theoretical limit at –8.0.[4]
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