WR 102 is a Wolf–Rayet star in the constellation Sagittarius, an extremely rare star on the WO oxygen sequence. It is a luminous and very hot star, highly...

are three stars with over 1 million L☉ and visible to the naked eye: WR 22, WR 24 and Eta Carinae. All of these stars are located in the Carina nebula...

Wolf–Rayet stars, often abbreviated as WR stars, are a rare heterogeneous set of stars with unusual spectra showing prominent broad emission lines of ionised...

1013 astro: luminosity per square meter of the hottest normal star known, WR 102 5–20 × 1013 weather: rate of heat energy release by a hurricane[citation...

calculated that WR 93b will explode as a supernova within 8,000 years. WR 102 WR 142 WR 30a List of supernova candidates Brown, A. G. A.; et al. (Gaia collaboration)...

approximately 2,000 years. The mass and rapid rotation make a GRB likely. WR 102 WR 30a WR 93b List of supernova candidates Zacharias, N.; et al. (2003). "The...

seen from Earth Maximum brightness; brightest moon of Uranus +14.1 star WR 102 seen from Earth Hottest known star +15.4 centaur Chiron seen from Earth...

population of the superbubble N 206 in the LMC. II. Parameters of the OB and WR stars, and the total massive star feedback". Astronomy and Astrophysics. 615:...

star with strong OVI emission in 1971, alongside other WO stars like WR 102, WR 142 and SMC AB8. Most stars with strong OVI emission known at the time...

Tuthill, Peter G.; et al. (March 2008). "The Prototype Colliding-Wind Pinwheel WR 104". The Astrophysical Journal. 675 (1): 698–710. arXiv:0712.2111. Bibcode:2008ApJ...