This is a list of the nearest hypergiant stars to Earth, located at a distance of up to 10,000 light-years (3,100 parsecs) from Earth.
While hypergiants are typically defined as stars with luminosity classes 0, Ia-0 or Ia+, other definitions exist, such as those based on stellar evolution. Therefore, stars with other luminosity classes can sometimes be considered hypergiants.
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Name | Distance (ly) | Spectral type | Stellar radius (R☉) | Stellar mass (M☉) | Stellar luminosity (L☉) | Apparent magnitude (V) | Notes and References |
---|---|---|---|---|---|---|---|
Mu Cephei | 2090-3060 | M2-Ia (M2e Ia or M2 Ia+) | 972±228 | 25 | 269000+111000 −40000 | 4.08 | [1] |
VV Cephei A | 3,319 – 4900 | M2 Iab (M1p 0) | 660, 1,050 | 2.5 or 18.2 | 72,880±16,300 | 4.91 | [2] |
VY Canis Majoris | 3820+260 −230 | M3-M4.5 (M2.5-M5Iae) | 1420±120 | 17±8 | 270000±40000 | 6.5-9.6 | [3] [4] |
HD 183143 (HT Sagittae) | 4990±550 | B6-8 Ia-0 | 109±15 | 24.2±1.4 | 288000+83000 −65000 | 6.71-6.95 | |
HD 168625 (V4030 Sagittarii) | 5000±200 | B6Ia+ (B2-B8) | 105 | 380000 | 8.30-8.41 | ||
HD 168607 (V4029 Sagittarii) | 5100±500 | B9Ia+ | 187 | 240000 | 8.12-8.29 | ||
NML Cygni | 5250+420 −360 | M4.5–M7.9 Ia–III | 1,350+195 −229 | 25 | 229,000+40,000 −41,000, 270,000+50,000 −50,000 | 16.60 | |
P Cygni | 5300±590 | B1-2Ia-0ep (B1 lapeq) | 76 | 37 | 610000 | 4.82 | |
Cygnus OB2-12 | 5300±590 | B3-4Ia+ | 264 | 110 | 1660000 | 11.702 | |
V915 Scorpii | 5600+570 −370 | K0Ia-0 | 685.6 | 14.7 | 74,100–185,200 | 6.22 - 6.64 | |
Zeta¹ Scorpii | 6000 | B1.5Ia+ | 103 to 125.5 | 36 to 53 | 8.5×105 | 4.705 | [5] |
V382 Carinae | 6,000 | G0-4-Ia+ | 485 ± 56 | 24±5.1 | 212,000 ± 12,300 | 3.83 | |
V602 Carinae | 7000 | M3 Ia-Iab | 1,015 | 17.7 - 20 | 126,000 | 8.39 | |
S Persei | 7900±300 | M3 Iae–M7 | 1,298+64-57 – 1,364±6 | 20 | 123,000 – 186,000 | 9.23 | |
6 Cassiopeiae | 8000 | A2.5Ia+ | 193 | 22.0 | 200000 | 5.34-5.45 | |
Rho Cassiopeiae | 8150±1630 | G2 0 (F8pIa-K0pIa-0) | 564 or 700 | 40 | 300000-530000 | 4.1 to 6.2 | [6] |
BP Crucis | 9915.154 | B1 Ia+ | 70 | 43 | 470,000 | 10.83 | [7] |