swap_horiz WR 102 Alternatives
Looking for alternatives to WR 102? Compare the top Star options ranked by our AI scoring system.
WR 102
WR 102 is a WO-type Wolf-Rayet star with a surface temperature exceeding 200,000 K, making it one of the hottest known stars in the Milky Way.
apps Top WR 102 Alternatives
The top alternative to WR 102 in 2026 is Eta Carinae with a score of 9.2/10, followed by Sirius B (9.1) and R136a1 (8.8).
Eta Carinae
Eta Carinae is an exceptionally large and volatile star located within the Carina Nebula. It’s notable for its dramatic...
Sirius B
Sirius B is a dense white dwarf star orbiting within the Sirius system of Canis Major. It represents the remnant core of...
R136a1
A Wolf-Rayet star in the R136 cluster of the Large Magellanic Cloud, regarded as the most massive known star with an ini...
P Cygni
A luminous blue variable in Cygnus that erupted around 1600 CE and is the namesake of the P Cygni spectral line profile,...
40 Eridani B
A white dwarf in the triple star system 40 Eridani, historically notable as the first white dwarf whose anomalously high...
Procyon B
The white dwarf companion to Procyon A in Canis Minor, its existence inferred from Procyon's proper-motion wobble decade...
Theta1 Orionis C
Theta1 Orionis C is the most massive and luminous member of the Trapezium cluster in the Orion Nebula, an O-type star re...
NML Cygni
A red hypergiant in Cygnus and one of the largest and most luminous stars known, with a radius estimated to exceed 1,600...
Pistol Star
A luminous blue hypergiant near the Galactic Center and among the most luminous stars in the Milky Way, revealed in the...
Gamma Velorum
Gamma Velorum is the brightest Wolf-Rayet star visible to the naked eye, a multiple-star system in Vela containing a WC8...
WR 140
WR 140 is a colliding-wind binary of a Wolf-Rayet and O-type star in Cygnus with a 7.9-year eccentric orbit, producing p...
Van Maanen's Star
A white dwarf in Pisces discovered by Dutch astronomer Adriaan van Maanen in 1917, notable as the closest solitary white...
WR 104
WR 104 is a Wolf-Rayet star in Sagittarius that forms a rotating pinwheel nebula with its O-star companion and is consid...
VV Cephei
An eclipsing binary in Cepheus pairing one of the largest known red supergiants with a hot blue companion, with an orbit...
AG Carinae
A luminous blue variable in Carina, one of the most massive and luminous stars in the Milky Way, surrounded by an ejecte...
Stephenson 2-18
Stephenson 2-18 is a red supergiant in the open cluster Stephenson 2, often cited as potentially the largest known star...
Kaus Australis
Epsilon Sagittarii, the brightest star in Sagittarius, a blue-white giant about 143 light-years away and a standard star...
HR 5171
HR 5171 is a yellow hypergiant in Centaurus and one of the largest stars known by physical radius, also forming a contac...
Peony Star
The Peony Star (WR 102ka) is a Wolf-Rayet star near the Galactic center and a contender for the most luminous star in th...
LBV 1806-20
LBV 1806-20 is a luminous blue variable near the Galactic center, located in the same dense star-forming cluster as a so...
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