List of variable stars

There are over 41,638 known variable stars (2008), with more being discovered regularly, so a complete list of every single variable is impossible at this place (cf. GCVS). The following is a list of variable stars that are well-known, bright, significant, or otherwise interesting.

Designation (name) Constellation Discovery Apparent magnitude (Maximum)[1] Apparent magnitude (Minimum)[2] Range of magnitude Period Type Comment
R And Andromeda   5m.8 14m.9 9.1 409 d Mira variable (M)  
S And (Supernova 1885) Andromeda Ernst Hartwig, August 20, 1885 5m.8 16m 10.2 Supernova (SNI)  
U Ant Antlia   8m.1 (p) 9m.7 (p) 1.6 LB  
θ Aps Apus   6m.4 (p) 8m.6 (p) 2.2 119 d Semiregular (SRB)  
η Aql Aquila Pigott, 1784 3m.48 4m.39 0.91 7.17664 d Classical Cepheid (DCEP)  
R Aql Aquila   5m.5 12m.0 6.5 284 d Mira variable (M)  
V Aql Aquila   6m.6 8m.4 1.8 353 d Semiregular (SRB)  
R Aqr Aquarius Karl Ludwig Harding, 1810 5m.8 12m.4 6.9 387 d Mira variable (M)  
T Aqr Aquarius   7m.2 14m.2 7.0 202 d Mira variable (M)  
U Ara Ara   7m.7 14m.1 6.4 225 d Mira variable (M)  
R Ari Aries   7m.4 13m.7 6.3 187 d Mira variable (M)  
U Ari Aries   7m.2 15m.2 8.0 371 d Mira variable (M)  
ε Aur (Almaaz) Auriga Johann Heinrich Fritsch, 1821 2m.92 3m.83 0.91 27.08 years Eclipsing binary Algol type (EA/GS)  
R Aur Auriga   6m.7 13m.9 7.2 458 d Mira variable (M)  
AE Aur Auriga   5m.78 6m.08 0.30 Orion variable (INA)  
R Boo Boötes   6m.2 13m.1 6.9 223 d Mira variable (M)  
W Boo Boötes   4m.73 5m.4 0.67 450 d Semiregular (SRB:)  
X Cam Camelopardalis   7m.4 14m.2 6.8 144 d Mira variable (M)  
VZ Cam Camelopardalis   4m.80 4m.96 0.16 23.7 d Semiregular (SR)  
R Cap Capricornus Hind, 1848 9m.4 14m.9 5.5 345 d Mira variable (M)  
η Car Carina Burchell, 1827 -0m.8 7m.9 8.6 S Doradus (SDOR) "The unpredictable supergiant"
l Car Carina   3m.28 4m.18 0.90 35.53584 d Classical Cepheid (DCEP)  
R Car Carina   3m.9 10m.5 6.6 309 d Mira variable (M)  
S Car Carina   4m.5 9m.9 5.4 149 d Mira variable (M)  
γ Cas Cassiopeia   1m.6 3m.0 1.4 Gamma Cassiopeiae (GCAS)  
R Cas Cassiopeia   4m.7 13m.5 8.9 430 d Mira variable (M)  
S Cas Cassiopeia   7m.9 16m.1 8.2 612 d Mira variable (M)  
W Cas Cassiopeia   7m.8 12m.5 4.7 406 d Mira variable (M)  
WZ Cas Cassiopeia   6m.3 8m.5 2.2 Semiregular (SRB) Visual double star, visible through binoculars
R Cen Centaurus   5m.3 11m.8 6.5 546 d Mira variable (M)  
S Cen Centaurus   9m.2 (p) 10m.7 (p) 1.5 65 d Semiregular (SR)  
T Cen Centaurus   5m.5 9m.0 3.5 90.44 d Semiregular (SRA)  
V645 Cen (Proxima Centauri) Centaurus   12m.1 (B) 13m.12 (B) 1.02 UV Ceti (UV)  
δ Cep Cepheus John Goodricke, 1784 3m.48 4m.37 0.89 5.36634 d Classical Cepheid (DCEP) prototype double star, visible in binoculars
μ Cep (Herschel's Garnet Star) Cepheus William Herschel, 1782 3m.43 5m.1 1.67 730 d Semiregular (SRC)  
S Cep Cepheus   7m.4 12m.9 5.5 487 d Mira variable (M)  
T Cep Cepheus   5m.2 11m.3 6.1 388 d Mira variable (M)  
U Cep Cepheus   6m.75 9m.24 2.49 2.49305 d Eclipsing binary Algol type (EA/SD)  
SS Cep Cepheus   8m.0 (p) 9m.1 (p) 1.1 90 d Semiregular (SRB)  
AR Cep Cepheus   7m.0 7m.9 0.9 Semiregular (SRB)  
ο Cet (Mira) Cetus David Fabricius, 1596; variability may have been first noted by Johannes Fokkes Holwarda, 1638 2m.0 10m.1 8.1 332 d Mira variable (M) "The miraculous"
The first discovered non-ephemeral/cataclysmic variable star.
T Cet Cetus   5m.0 6m.9 1.9 159 d Semiregular (SRC)  
U Cet Cetus   6m.8 13m.4 6.6 235 d Mira variable (M)  
W Cet Cetus   7m.1 14m.8 7.7 351 d Mira variable (M)  
R Cha Chamaeleon   7m.5 14m.2 6.7 335 d Mira variable (M)  
R CMa Canis Major   5m.70 6m.34 0.64 1.13594 d Eclipsing binary Algol type (EA/SD)  
VY CMa Canis Major   6m.5 9m.6 3.1 unique (*)  
FW CMa Canis Major   5m.00 5m.50 0.50 Gamma Cassiopeiae (GCAS)  
S CMi Canis Minor   6m.6 13m.2 6.6 333 d Mira variable (M)  
R Cnc Cancer   6m.07 11m.8 5.73 362 d Mira variable (M)  
S Cnc Cancer Hind, 1848 8m.29 10m.25 1.96 9.48455 d Eclipsing binary Algol type (EA/DS)  
T Cnc Cancer Hind, 1850 7m.6 10m.5 2.9 482 d Semiregular (SRB)  
X Cnc Cancer   5m.6 7m.5 1.9 195 d Semiregular (SRB)  
T Col Columba   6m.6 12m.7 6.1 226 d Mira variable (M)  
R Com Coma Berenices   7m.1 14m.6 7.5 363 d Mira variable (M)  
α CrB (Alphecca or Gemma) Corona Borealis   2m.21 (B) 2m.32 (B) 0.11 17.35991 d Eclipsing binary Algol type (EA/DM)  
R CrB Corona Borealis Piggott, 1795 5m.71 14m.8 9.09 R Coronae Borealis (RCB)  
S CrB Corona Borealis   5m.8 14m.1 8.7 360 d Mira variable (M)  
T CrB Corona Borealis   2m.0 10m.8 8.8 (80 years) recurrent nova (NR)  
U CrB Corona Borealis   7m.66 8m.79 1.13 3.45220 d Eclipsing binary Algol type (EA/SD)  
V CrB Corona Borealis   6m.9 12m.6 5.3 358 d Mira variable (M)  
W CrB Corona Borealis   7m.8 14m.3 6.5 238 d Mira variable (M)  
R Cru Crux   6m.40 7m.23 0.83 5.82575 d Classical Cepheid (DCEP)  
R Crv Corvus   6m.7 14m.4 7.7 317 d Mira variable (M)  
χ Cyg Cygnus Kirch, 1686 3m.3 14m.2 10.9 408 d Mira variable (M)  
R Cyg Cygnus   6m.1 14m.4 8.3 426 d Mira variable (M)  
U Cyg Cygnus   5m.9 12m.1 6.2 463 d Mira variable (M)  
W Cyg Cygnus   6m.80 (B) 8m.9 (B) 2.1 131 d Semiregular (SRB)  
X Cyg Cygnus   5m.85 6m.91 1.06 16.38633 d Classical Cepheid (DCEP)  
RT Cyg Cygnus   6m.0 13m.1 7.1 190 d Mira variable (M)  
SS Cyg Cygnus   7m.7 12m.4 4.7 (49.5 d) dwarf nova UGSS prototype  
SU Cyg Cygnus   6m.44 7m.22 0.78 3.84555 d Classical Cepheid (DCEP)  
CH Cyg Cygnus   5m.60 8m.49 2.89 Z Andromedae (ZAND+SR)  
R Del Delphinus   7m.6 13m.8 6.2 285  d Mira variable (M)  
U Del Delphinus   7m.6 (p) 8m.9 (p) 1.3 110 d Semiregular (SRB)  
EU Del Delphinus   5m.79 6m.9 1.11 59.7 d Semiregular (SRB)  
β Dor Dorado   3m.46 4m.08 0.62 9.8426 d Classical Cepheid (DCEP)  
S Dor Dorado   8m.6 (B) 11m.5 (B) 2.9 S Doradus (SDOR) (prototype) in the Large Magellanic Cloud
R Dra Draco   6m.7 13m.2 6.5 246 d Mira variable (M)  
T Eri Eridanus   7m.2 13m.2 6.0 252 d Mira variable (M)  
R For Fornax   7m.5 13m.0 5.5 389 d Mira variable (M)  
η Gem (Propus) Gemini   3m.15 3m.9 0.75 233 d Semiregular (SRA+EA)  
ζ Gem (Mekbuda) Gemini   3m.62 4m.18 0.56 10.15073 d Classical Cepheid (DCEP)  
R Gem Gemini Hind, 1848 6m.0 14m.0 8.0 370 d Mira variable (M)  
S Gem Gemini Hind, 1848 8m.0 14m.7 6.7 293 d Mira variable (M)  
T Gem Gemini Hind, 1848 8m.0 15m.0 7.0 288 d Mira variable (M)  
U Gem Gemini   8m.2 14m.9 6.7 (105.2 d) dwarf nova (UGSS+E)  
S Gru Grus   6m.0 15m.0 9.0 402 d Mira variable (M)  
α Her (Rasalgethi) Hercules William Herschel, 1759 2m.74 4m.0 1.26 Semiregular (SRC)  
g Her (30 Her) Hercules   4m.3 6m.3 2.0 89.2 d Semiregular (SRB)  
u Her (68 Her) Hercules   4m.69 5m.37 0.68 2.05103 d Eclipsing binary Algol type (EA/SD)  
S Her Hercules   6m.4 13m.8 7.4 307 d Mira variable (M)  
U Her Hercules   6m.4 13m.4 7.0 406 d Mira variable (M)  
X Her Hercules   7m.5 (p) 8m.6 (p) 1.1 95.0 d Semiregular (SRB)  
R Hor Horologium   4m.7 14m.3 9.6 408 d Mira variable (M)  
U Hor Horologium   7m.8 (p) 15m.1 (p) 6.3 348 d Mira variable (M)  
R Hya Hydra Maraldi, 1704 3m.5 10m.9 7.4 389 d Mira variable (M)  
S Hya Hydra Hind, 1848 7m.2 13m.3 6.1 257 d Mira variable (M)  
U Hya Hydra   7m.0 (B) 9m.4 (B) 2.4 ~450 d Semiregular (SRB)  
VW Hya Hydra   10m.5 14m.1 3.6 2.69642 d Eclipsing binary Algol type (EA/SD)  
BL Lac Lacerta   12m.4 (B) 17m.2 (B) 4.8 BLLAC prototype originally thought to be a variable star, but later

discovered to be a blazar

R Leo Leo J.A. Koch, 1782 4m.4 11m.3 6.9 310 d Mira variable (M)  
R Lep Lepus   5m.5 11m.7 6.2 427 d Mira variable (M) Hind's Crimson Star
RX Lep Lepus   5m.0 7m.4 2.4 ~60 d Semiregular (SRB)  
R LMi Leo Minor   6m.3 13m.2 6.9 372 d Mira variable (M)  
RU Lup Lupus   9m.6 (p) 13m.4 (p) 3.8 Orion variable (INT)  
β Lyr (Sheliak) Lyra John Goodricke, 1784 3m.25 4m.36 1.11 12.91383 d Eclipsing binary Beta Lyrae type (prototype)  
R Lyr Lyra   3m.88 5m.0 1.12 ~46 d Semiregular (SRB)  
RR Lyr Lyra   7m.06 8m.12 1.06 0.566868 d RR Lyrae variable (prototype)  
U Mic Microscopium   7m.0 14m.4 7.7 334 d Mira variable (M)  
U Mon Monoceros   6m.1 (p) 8m.8 (p) 2.7 91.3 d RV Tauri variable (RVB)  
V Mon Monoceros   6m.0 13m.9 7.9 341 d Mira variable (M)  
R Nor Norma   6m.5 (p) 13m.9 (p) 7.4 508 d Mira variable (M)  
T Nor Norma   6m.2 13m.6 7.4 241 d Mira variable (M)  
R Oct Octans   6m.4 13m.2 6.8 405 d Mira variable (M)  
S Oct Octans   7m.2 14m.0 6.8 259 d Mira variable (M)  
V Oph Ophiuchus   7m.3 11m.6 4.3 297 d Mira variable (M)  
X Oph Ophiuchus   5m.9 9m.2 3.3 329 d Mira variable (M)  
RS Oph Ophiuchus   4m.3 12m.5 8.2 recurrent nova (NR)  
BF Oph Ophiuchus   6m.93 7m.71 0.78 4.06775 d Classical Cepheid (DCEP)  
α Ori (Betelgeuse) Orion John Herschel, 1840 0m.0 1m.3 1.3 6.39 years Semiregular (SRC)  
δ Ori (Mintaka) Orion John Herschel, 1834 2m.14 2m.26 0.12 5.73248 d Eclipsing binary Algol type (EA/DM)  
R Ori Orion Hind, 1848 9m.05 13m.4 4.35 377 d Mira variable (M)  
U Ori Orion   4m.8 13m.0 8.5 368 d Mira variable (M)  
W Ori Orion   8m.2 (p) 12m.4 (p) 4.2 212 d Semiregular (SRB)  
VV Ori Orion   5m.31 5m.66 0.35 1.48538 d Eclipsing binary Algol type (EA/KE:)  
CK Ori Orion   5m.9 7m.1 1.2 ~120 d Semiregular (SR:)  
κ Pav Pavo   3m.91 4m.78 0.87 9.09423 d Type II Cepheid (CW)  
S Pav Pavo   6m.6 10m.4 3.8 381 d Semiregular (SRA)  
β Peg (Scheat) Pegasus Schmidt, 1847 2m.31 2m.74 0.43 LB  
ε Peg (Enif) Pegasus 0m.7 3m.5 2.8 LC  
R Peg Pegasus Hind, 1848 6m.9 13m.8 6.9 378 d Mira variable (M)  
X Peg Pegasus   8m.8 14m.4 5.8 201 d Mira variable (M)  
β Per (Algol) Perseus Geminiano Montanari, 1669 2m.12 3m.39 1.27 2.86730 d Eclipsing binary Algol type (EA/SD) (prototype) The Demon Star
DY Persei Perseus R Coronae Borealis / DY Persei / (prototype)
φ Per Perseus   3m.96 4m.11 0.15 19.5 d Gamma Cassiopeiae (GCAS)  
ρ Per Perseus   3m.30 4m.0 0.70 ~50 d Semiregular (SRB)  
X Per Perseus   6m.03 7m.0 0.97 Gamma Cassiopeiae (GCAS+XP)  
ζ Phe (Wurren) Phoenix   3m.91 4m.42 0.51 1.66977 d Eclipsing binary Algol type (EA/DM)  
R Pic Pictor   6m.35 10m.1 3.75 171 d Semiregular (SR)  
R Psc Pisces Hind, 1850 7m.0 14m.8 7.8 345 d Mira variable (M)  
TX Psc Pisces   4m.79 5m.20 0.42 LB  
L2 Pup Puppis   2m.6 6m.2 3.6 141 d Semiregular (SRB)  
RS Pup Puppis   6m.52 7m.67 1.15 41.3876 d Classical Cepheid (DCEP)  
T Pyx Pyxis   7m.0 (B) 15m.77 (B) 8.77 (20 years) recurrent nova (NR)  
S Scl Sculptor   5m.5 13m.6 8.1 363 d Mira variable (M)  
RR Sco Scorpius   5m.0 12m.4 7.4 281 d Mira variable (M)  
RS Sco Scorpius   6m.2 13m.0 6.8 320 d Mira variable (M)  
RT Sco Scorpius   7m.0 15m.2 8.2 449 d Mira variable (M)  
R Sct Scutum Pigott, 1795 4m.2 8m.6 4.4 146.5 d RV Tauri variable (RVA)  
R Ser Serpens Harding, 1826 5m.16 14m.4 9.24 356 d Mira variable (M)  
S Ser Serpens Harding, 1828 7m.0 14m.1 7.1 372 d Mira variable (M)  
U Sge Sagitta   6m.45 9m.28 2.83 3.38062 d Eclipsing binary Algol type (EA/SD)  
WZ Sge Sagitta   7m.0 (B) 15m.53 (B) 8.53 (33 years) dwarf nova (UGSU+E+ZZ)  
RR Sgr Sagittarius   5m.4 14m.0 8.6 336 d Mira variable (M)  
R Sgr Sagittarius   6m.7 12m.83 6.13 270 d Mira variable (M)  
U Sgr Sagittarius(in M25)   6m.28 7m.15 0.87 6.74523 d Classical Cepheid (DCEP)  
RT Sgr Sagittarius   6m.0 14m.1 8.1 306 d Mira variable (M)  
RU Sgr Sagittarius   6m.0 13m.8 7.8 240 d Mira variable (M)  
RY Sgr Sagittarius   5m.8 14m.0 8.2 R Coronae Borealis (RCB)  
VX Sgr Sagittarius   6m.52 14m.0 7.08 732 d Semiregular (SRC)  
λ Tau Taurus Baxendell, 1848 3m.37 3m.91 0.54 3.95295 d Eclipsing binary Algol type (EA/DM)  
R Tau Taurus Hind, 1849 7m.6 15m.8 8.2 321 d Mira variable (M)  
T Tau Taurus   9m.3 13m.5 4.2 Orion variable (INT)  
SU Tau Taurus   9m.1 16m.86 7.76 R Coronae Borealis (RCB)  
R Tri Triangulum   5m.4 12m.6 7.2 267 d Mira variable (M)  
R UMa Ursa Major   6m.5 13m.7 7.2 302 d Mira variable (M)  
T UMa Ursa Major   6m.6 13m.5 6.9 257 d Mira variable (M)  
U UMa Ursa Major   6m.20 6m.25 0.05 -
W UMa Ursa Major   7m.75 8m.48 0.73 0.3336 d Eclipsing binary W Ursae Majoris type (prototype)    
Z UMa Ursa Major   6m.2 9m.4 3.2 196 d Semiregular (SRB)  
α UMi (Polaris) Ursa Minor   1m.86 2m.13 0.27 3.9696 d Classical Cepheid (DCEPS)  
R Vir Virgo Harding, 1809 6m.1 12m.1 6.0 146 d Mira variable (M)  
S Vir Virgo   6m.3 13m.2 6.9 375 d Mira variable (M)  

Notes

  1. (visual magnitude, unless marked (B) (= blue) or (p) (= photographic))
  2. (visual magnitude, unless marked (B) (= blue) or (p) (= photographic))
gollark: I don't really like the current world in some ways either, but I think markets are generally a fairly okay system if managed in some ways.
gollark: Okay, continue.
gollark: Where are the actual incentives in anarchism? It seems that you basically just expect people to embark on giant construction projects and give resources out of the goodness of their hearts or something. In capitalism you actually have a decent direct reason to do that - your company can make more profit if it makes a new silicon fab or something, so you'll get money yourself, and you can get resources from other companies because you both get benefits for trading that way.
gollark: Well, that's just wrong.
gollark: You could do a *bit* of poor-people-saving.

References

See also

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