# List of variable stars

As of 2017, there are over 52,011 known variable stars, 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) | Apparent magnitude (Minimum) | Range of magnitude | Period | Type | Comment |
| R And | Andromeda | | 5$^m$.8 | 14$^m$.9 | 9.1 | 409 d | Mira variable (M) | |
| S And (Supernova 1885) | Andromeda | Ernst Hartwig, August 20, 1885 | 5$^m$.8 | 16$^m$ | 10.2 | | Supernova (SNI) | |
| U Ant | Antlia | | 8$^m$.1 (p) | 9$^m$.7 (p) | 1.6 | | LB | |
| θ Aps | Apus | | 6$^m$.4 (p) | 8$^m$.6 (p) | 2.2 | 119 d | Semiregular (SRB) | |
| η Aql | Aquila | Pigott, 1784 | 3$^m$.48 | 4$^m$.39 | 0.91 | 7.17664 d | Classical Cepheid (DCEP) | |
| R Aql | Aquila | | 5$^m$.5 | 12$^m$.0 | 6.5 | 284 d | Mira variable (M) | |
| V Aql | Aquila | | 6$^m$.6 | 8$^m$.4 | 1.8 | 353 d | Semiregular (SRB) | |
| R Aqr | Aquarius | Karl Ludwig Harding, 1810 | 5$^m$.8 | 12$^m$.4 | 6.9 | 387 d | Mira variable (M) | |
| T Aqr | Aquarius | | 7$^m$.2 | 14$^m$.2 | 7.0 | 202 d | Mira variable (M) | |
| U Ara | Ara | | 7$^m$.7 | 14$^m$.1 | 6.4 | 225 d | Mira variable (M) | |
| R Ari | Aries | | 7$^m$.4 | 13$^m$.7 | 6.3 | 187 d | Mira variable (M) | |
| U Ari | Aries | | 7$^m$.2 | 15$^m$.2 | 8.0 | 371 d | Mira variable (M) | |
| ε Aur (Almaaz) | Auriga | Johann Heinrich Fritsch, 1821 | 2$^m$.92 | 3$^m$.83 | 0.91 | 27.08 years | Eclipsing binary Algol type (EA/GS) | |
| R Aur | Auriga | | 6$^m$.7 | 13$^m$.9 | 7.2 | 458 d | Mira variable (M) | |
| AE Aur | Auriga | | 5$^m$.78 | 6$^m$.08 | 0.30 | | Orion variable (INA) | |
| R Boo | Boötes | | 6$^m$.2 | 13$^m$.1 | 6.9 | 223 d | Mira variable (M) | |
| W Boo | Boötes | | 4$^m$.73 | 5$^m$.4 | 0.67 | 450 d | Semiregular (SRB:) | |
| X Cam | Camelopardalis | | 7$^m$.4 | 14$^m$.2 | 6.8 | 144 d | Mira variable (M) | |
| VZ Cam | Camelopardalis | | 4$^m$.80 | 4$^m$.96 | 0.16 | 23.7 d | Semiregular (SR) | |
| R Cap | Capricornus | Hind, 1848 | 9$^m$.4 | 14$^m$.9 | 5.5 | 345 d | Mira variable (M) | |
| η Car | Carina | Burchell, 1827 | -0$^m$.8 | 7$^m$.9 | 8.6 | | S Doradus (SDOR) | "The unpredictable supergiant" |
| l Car | Carina | | 3$^m$.28 | 4$^m$.18 | 0.90 | 35.53584 d | Classical Cepheid (DCEP) | |
| R Car | Carina | | 3$^m$.9 | 10$^m$.5 | 6.6 | 309 d | Mira variable (M) | |
| S Car | Carina | | 4$^m$.5 | 9$^m$.9 | 5.4 | 149 d | Mira variable (M) | |
| γ Cas | Cassiopeia | | 1$^m$.6 | 3$^m$.0 | 1.4 | | Gamma Cassiopeiae (GCAS) | |
| R Cas | Cassiopeia | | 4$^m$.7 | 13$^m$.5 | 8.9 | 430 d | Mira variable (M) | |
| S Cas | Cassiopeia | | 7$^m$.9 | 16$^m$.1 | 8.2 | 612 d | Mira variable (M) | |
| W Cas | Cassiopeia | | 7$^m$.8 | 12$^m$.5 | 4.7 | 406 d | Mira variable (M) | |
| WZ Cas | Cassiopeia | | 6$^m$.3 | 8$^m$.5 | 2.2 | | Semiregular (SRB) | Visual double star, visible through binoculars |
| R Cen | Centaurus | | 5$^m$.3 | 11$^m$.8 | 6.5 | 546 d | Mira variable (M) | |
| S Cen | Centaurus | | 9$^m$.2 (p) | 10$^m$.7 (p) | 1.5 | 65 d | Semiregular (SR) | |
| T Cen | Centaurus | | 5$^m$.5 | 9$^m$.0 | 3.5 | 90.44 d | Semiregular (SRA) | |
| V645 Cen (Proxima Centauri) | Centaurus | | 12$^m$.1 (B) | 13$^m$.12 (B) | 1.02 | | UV Ceti (UV) | |
| δ Cep | Cepheus | John Goodricke, 1784 | 3$^m$.48 | 4$^m$.37 | 0.89 | 5.36634 d | Classical Cepheid (DCEP) prototype | double star, visible in binoculars |
| Vega | Lyra | | -0$^m$.02 | 0$^m$.07 | 0.09 | 0.107 d | Delta Scuti variable | Brightest variable star in the sky. |
| μ Cep (Herschel's Garnet Star) | Cepheus | William Herschel, 1782 | 3$^m$.43 | 5$^m$.1 | 1.67 | 730 d | Semiregular (SRC) | |
| S Cep | Cepheus | | 7$^m$.4 | 12$^m$.9 | 5.5 | 487 d | Mira variable (M) | |
| T Cep | Cepheus | | 5$^m$.2 | 11$^m$.3 | 6.1 | 388 d | Mira variable (M) | |
| U Cep | Cepheus | | 6$^m$.75 | 9$^m$.24 | 2.49 | 2.49305 d | Eclipsing binary Algol type (EA/SD) | |
| SS Cep | Cepheus | | 8$^m$.0 (p) | 9$^m$.1 (p) | 1.1 | 90 d | Semiregular (SRB) | |
| ST Cep | Cepheus | | 7$^m$.8 | | | None | Mira variable (M) | |
| AR Cep | Cepheus | | 7$^m$.0 | 7$^m$.9 | 0.9 | | Semiregular (SRB) | |
| ο Cet (Mira) | Cetus | David Fabricius, 1596; variability may have been first noted by Johannes Fokkes Holwarda, 1638 | 2$^m$.0 | 10$^m$.1 | 8.1 | 332 d | Mira variable (M) | "The miraculous" The first discovered non-ephemeral/cataclysmic variable star. |
| T Cet | Cetus | | 5$^m$.0 | 6$^m$.9 | 1.9 | 159 d | Semiregular (SRC) | |
| U Cet | Cetus | | 6$^m$.8 | 13$^m$.4 | 6.6 | 235 d | Mira variable (M) | |
| W Cet | Cetus | | 7$^m$.1 | 14$^m$.8 | 7.7 | 351 d | Mira variable (M) | |
| R Cha | Chamaeleon | | 7$^m$.5 | 14$^m$.2 | 6.7 | 335 d | Mira variable (M) | |
| R CMa | Canis Major | | 5$^m$.70 | 6$^m$.34 | 0.64 | 1.13594 d | Eclipsing binary Algol type (EA/SD) | |
| VY CMa | Canis Major | | 6$^m$.5 | 9$^m$.6 | 3.1 | | unique (*) | |
| FW CMa | Canis Major | | 5$^m$.00 | 5$^m$.50 | 0.50 | | Gamma Cassiopeiae (GCAS) | |
| S CMi | Canis Minor | | 6$^m$.6 | 13$^m$.2 | 6.6 | 333 d | Mira variable (M) | |
| R Cnc | Cancer | | 6$^m$.07 | 11$^m$.8 | 5.73 | 362 d | Mira variable (M) | |
| S Cnc | Cancer | Hind, 1848 | 8$^m$.29 | 10$^m$.25 | 1.96 | 9.48455 d | Eclipsing binary Algol type (EA/DS) | |
| T Cnc | Cancer | Hind, 1850 | 7$^m$.6 | 10$^m$.5 | 2.9 | 482 d | Semiregular (SRB) | |
| X Cnc | Cancer | | 5$^m$.6 | 7$^m$.5 | 1.9 | 195 d | Semiregular (SRB) | |
| T Col | Columba | | 6$^m$.6 | 12$^m$.7 | 6.1 | 226 d | Mira variable (M) | |
| R Com | Coma Berenices | | 7$^m$.1 | 14$^m$.6 | 7.5 | 363 d | Mira variable (M) | |
| α CrB (Alphecca or Gemma) | Corona Borealis | | 2$^m$.21 (B) | 2$^m$.32 (B) | 0.11 | 17.35991 d | Eclipsing binary Algol type (EA/DM) | |
| R CrB | Corona Borealis | Piggott, 1795 | 5$^m$.71 | 14$^m$.8 | 9.09 | | R Coronae Borealis (RCB) | |
| S CrB | Corona Borealis | | 5$^m$.8 | 14$^m$.1 | 8.7 | 360 d | Mira variable (M) | |
| T CrB | Corona Borealis | | 2$^m$.0 | 10$^m$.8 | 8.8 | (80 years) | recurrent nova (NR) | |
| U CrB | Corona Borealis | | 7$^m$.66 | 8$^m$.79 | 1.13 | 3.45220 d | Eclipsing binary Algol type (EA/SD) | |
| V CrB | Corona Borealis | | 6$^m$.9 | 12$^m$.6 | 5.3 | 358 d | Mira variable (M) | |
| W CrB | Corona Borealis | | 7$^m$.8 | 14$^m$.3 | 6.5 | 238 d | Mira variable (M) | |
| R Cru | Crux | | 6$^m$.40 | 7$^m$.23 | 0.83 | 5.82575 d | Classical Cepheid (DCEP) | |
| R Crv | Corvus | | 6$^m$.7 | 14$^m$.4 | 7.7 | 317 d | Mira variable (M) | |
| χ Cyg | Cygnus | Kirch, 1686 | 3$^m$.3 | 14$^m$.2 | 10.9 | 408 d | Mira variable (M) | |
| R Cyg | Cygnus | | 6$^m$.1 | 14$^m$.4 | 8.3 | 426 d | Mira variable (M) | |
| U Cyg | Cygnus | | 5$^m$.9 | 12$^m$.1 | 6.2 | 463 d | Mira variable (M) | |
| W Cyg | Cygnus | | 6$^m$.80 (B) | 8$^m$.9 (B) | 2.1 | 131 d | Semiregular (SRB) | |
| X Cyg | Cygnus | | 5$^m$.85 | 6$^m$.91 | 1.06 | 16.38633 d | Classical Cepheid (DCEP) | |
| RT Cyg | Cygnus | | 6$^m$.0 | 13$^m$.1 | 7.1 | 190 d | Mira variable (M) | |
| SS Cyg | Cygnus | | 7$^m$.7 | 12$^m$.4 | 4.7 | (49.5 d) | dwarf nova UGSS prototype | |
| SU Cyg | Cygnus | | 6$^m$.44 | 7$^m$.22 | 0.78 | 3.84555 d | Classical Cepheid (DCEP) | |
| CH Cyg | Cygnus | | 5$^m$.60 | 8$^m$.49 | 2.89 | | Z Andromedae (ZAND+SR) | |
| R Del | Delphinus | | 7$^m$.6 | 13$^m$.8 | 6.2 | 285 d | Mira variable (M) | |
| U Del | Delphinus | | 7$^m$.6 (p) | 8$^m$.9 (p) | 1.3 | 110 d | Semiregular (SRB) | |
| EU Del | Delphinus | | 5$^m$.79 | 6$^m$.9 | 1.11 | 59.7 d | Semiregular (SRB) | |
| β Dor | Dorado | | 3$^m$.46 | 4$^m$.08 | 0.62 | 9.8426 d | Classical Cepheid (DCEP) | |
| S Dor | Dorado | | 8$^m$.6 (B) | 11$^m$.5 (B) | 2.9 | | S Doradus (SDOR) (prototype) | in the Large Magellanic Cloud |
| R Dra | Draco | | 6$^m$.7 | 13$^m$.2 | 6.5 | 246 d | Mira variable (M) | |
| T Eri | Eridanus | | 7$^m$.2 | 13$^m$.2 | 6.0 | 252 d | Mira variable (M) | |
| R For | Fornax | | 7$^m$.5 | 13$^m$.0 | 5.5 | 389 d | Mira variable (M) | |
| η Gem (Propus) | Gemini | | 3$^m$.15 | 3$^m$.9 | 0.75 | 233 d | Semiregular (SRA+EA) | |
| ζ Gem (Mekbuda) | Gemini | | 3$^m$.62 | 4$^m$.18 | 0.56 | 10.15073 d | Classical Cepheid (DCEP) | |
| R Gem | Gemini | Hind, 1848 | 6$^m$.0 | 14$^m$.0 | 8.0 | 370 d | Mira variable (M) | |
| S Gem | Gemini | Hind, 1848 | 8$^m$.0 | 14$^m$.7 | 6.7 | 293 d | Mira variable (M) | |
| T Gem | Gemini | Hind, 1848 | 8$^m$.0 | 15$^m$.0 | 7.0 | 288 d | Mira variable (M) | |
| U Gem | Gemini | | 8$^m$.2 | 14$^m$.9 | 6.7 | (105.2 d) | dwarf nova (UGSS+E) | |
| S Gru | Grus | | 6$^m$.0 | 15$^m$.0 | 9.0 | 402 d | Mira variable (M) | |
| α Her (Rasalgethi) | Hercules | William Herschel, 1759 | 2$^m$.74 | 4$^m$.0 | 1.26 | | Semiregular (SRC) | |
| g Her (30 Her) | Hercules | | 4$^m$.3 | 6$^m$.3 | 2.0 | 89.2 d | Semiregular (SRB) | |
| u Her (68 Her) | Hercules | | 4$^m$.69 | 5$^m$.37 | 0.68 | 2.05103 d | Eclipsing binary Algol type (EA/SD) | |
| S Her | Hercules | | 6$^m$.4 | 13$^m$.8 | 7.4 | 307 d | Mira variable (M) | |
| U Her | Hercules | | 6$^m$.4 | 13$^m$.4 | 7.0 | 406 d | Mira variable (M) | |
| X Her | Hercules | | 7$^m$.5 (p) | 8$^m$.6 (p) | 1.1 | 95.0 d | Semiregular (SRB) | |
| R Hor | Horologium | | 4$^m$.7 | 14$^m$.3 | 9.6 | 408 d | Mira variable (M) | |
| U Hor | Horologium | | 7$^m$.8 (p) | 15$^m$.1 (p) | 6.3 | 348 d | Mira variable (M) | |
| R Hya | Hydra | Maraldi, 1704 | 3$^m$.5 | 10$^m$.9 | 7.4 | 389 d | Mira variable (M) | |
| S Hya | Hydra | Hind, 1848 | 7$^m$.2 | 13$^m$.3 | 6.1 | 257 d | Mira variable (M) | |
| U Hya | Hydra | | 7$^m$.0 (B) | 9$^m$.4 (B) | 2.4 | ~450 d | Semiregular (SRB) | |
| VW Hya | Hydra | | 10$^m$.5 | 14$^m$.1 | 3.6 | 2.69642 d | Eclipsing binary Algol type (EA/SD) | |
| BL Lac | Lacerta | | 12$^m$.4 (B) | 17$^m$.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 | 4$^m$.4 | 11$^m$.3 | 6.9 | 310 d | Mira variable (M) | |
| R Lep | Lepus | | 5$^m$.5 | 11$^m$.7 | 6.2 | 427 d | Mira variable (M) | Hind's Crimson Star |
| RX Lep | Lepus | | 5$^m$.0 | 7$^m$.4 | 2.4 | ~60 d | Semiregular (SRB) | |
| R LMi | Leo Minor | | 6$^m$.3 | 13$^m$.2 | 6.9 | 372 d | Mira variable (M) | |
| RU Lup | Lupus | | 9$^m$.6 (p) | 13$^m$.4 (p) | 3.8 | | Orion variable (INT) | |
| β Lyr (Sheliak) | Lyra | John Goodricke, 1784 | 3$^m$.25 | 4$^m$.36 | 1.11 | 12.91383 d | Eclipsing binary Beta Lyrae type (prototype) | |
| R Lyr | Lyra | | 3$^m$.88 | 5$^m$.0 | 1.12 | ~46 d | Semiregular (SRB) | |
| RR Lyr | Lyra | | 7$^m$.06 | 8$^m$.12 | 1.06 | 0.566868 d | RR Lyrae variable (prototype) | |
| U Mic | Microscopium | | 7$^m$.0 | 14$^m$.4 | 7.7 | 334 d | Mira variable (M) | |
| U Mon | Monoceros | | 6$^m$.1 (p) | 8$^m$.8 (p) | 2.7 | 91.3 d | RV Tauri variable (RVB) | |
| V Mon | Monoceros | | 6$^m$.0 | 13$^m$.9 | 7.9 | 341 d | Mira variable (M) | |
| R Nor | Norma | | 6$^m$.5 (p) | 13$^m$.9 (p) | 7.4 | 508 d | Mira variable (M) | |
| T Nor | Norma | | 6$^m$.2 | 13$^m$.6 | 7.4 | 241 d | Mira variable (M) | |
| R Oct | Octans | | 6$^m$.4 | 13$^m$.2 | 6.8 | 405 d | Mira variable (M) | |
| S Oct | Octans | | 7$^m$.2 | 14$^m$.0 | 6.8 | 259 d | Mira variable (M) | |
| V Oph | Ophiuchus | | 7$^m$.3 | 11$^m$.6 | 4.3 | 297 d | Mira variable (M) | |
| X Oph | Ophiuchus | | 5$^m$.9 | 9$^m$.2 | 3.3 | 329 d | Mira variable (M) | |
| RS Oph | Ophiuchus | | 4$^m$.3 | 12$^m$.5 | 8.2 | | recurrent nova (NR) | |
| BF Oph | Ophiuchus | | 6$^m$.93 | 7$^m$.71 | 0.78 | 4.06775 d | Classical Cepheid (DCEP) | |
| α Ori (Betelgeuse) | Orion | John Herschel, 1840 | 0$^m$.0 | 1$^m$.3 | 1.3 | 6.39 years | Semiregular (SRC) | |
| δ Ori (Mintaka) | Orion | John Herschel, 1834 | 2$^m$.14 | 2$^m$.26 | 0.12 | 5.73248 d | Eclipsing binary Algol type (EA/DM) | |
| R Ori | Orion | Hind, 1848 | 9$^m$.05 | 13$^m$.4 | 4.35 | 377 d | Mira variable (M) | |
| U Ori | Orion | | 4$^m$.8 | 13$^m$.0 | 8.5 | 368 d | Mira variable (M) | |
| W Ori | Orion | | 8$^m$.2 (p) | 12$^m$.4 (p) | 4.2 | 212 d | Semiregular (SRB) | |
| VV Ori | Orion | | 5$^m$.31 | 5$^m$.66 | 0.35 | 1.48538 d | Eclipsing binary Algol type (EA/KE:) | |
| CK Ori | Orion | | 5$^m$.9 | 7$^m$.1 | 1.2 | ~120 d | Semiregular (SR:) | |
| κ Pav | Pavo | | 3$^m$.91 | 4$^m$.78 | 0.87 | 9.09423 d | Type II Cepheid (CW) | |
| S Pav | Pavo | | 6$^m$.6 | 10$^m$.4 | 3.8 | 381 d | Semiregular (SRA) | |
| β Peg (Scheat) | Pegasus | Schmidt, 1847 | 2$^m$.31 | 2$^m$.74 | 0.43 | | LB | |
| ε Peg (Enif) | Pegasus | | 0$^m$.7 | 3$^m$.5 | 2.8 | | LC | |
| R Peg | Pegasus | Hind, 1848 | 6$^m$.9 | 13$^m$.8 | 6.9 | 378 d | Mira variable (M) | |
| X Peg | Pegasus | | 8$^m$.8 | 14$^m$.4 | 5.8 | 201 d | Mira variable (M) | |
| β Per (Algol) | Perseus | Geminiano Montanari, 1669 | 2$^m$.12 | 3$^m$.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 | | 3$^m$.96 | 4$^m$.11 | 0.15 | 19.5 d | Gamma Cassiopeiae (GCAS) | |
| ρ Per | Perseus | | 3$^m$.30 | 4$^m$.0 | 0.70 | ~50 d | Semiregular (SRB) | |
| X Per | Perseus | | 6$^m$.03 | 7$^m$.0 | 0.97 | | Gamma Cassiopeiae (GCAS+XP) | |
| ζ Phe (Wurren) | Phoenix | | 3$^m$.91 | 4$^m$.42 | 0.51 | 1.66977 d | Eclipsing binary Algol type (EA/DM) | |
| R Pic | Pictor | | 6$^m$.35 | 10$^m$.1 | 3.75 | 171 d | Semiregular (SR) | |
| R Psc | Pisces | Hind, 1850 | 7$^m$.0 | 14$^m$.8 | 7.8 | 345 d | Mira variable (M) | |
| TX Psc | Pisces | | 4$^m$.79 | 5$^m$.20 | 0.42 | | LB | |
| L$^2$ Pup | Puppis | | 2$^m$.6 | 6$^m$.2 | 3.6 | 141 d | Semiregular (SRB) | |
| RS Pup | Puppis | | 6$^m$.52 | 7$^m$.67 | 1.15 | 41.3876 d | Classical Cepheid (DCEP) | |
| T Pyx | Pyxis | | 7$^m$.0 (B) | 15$^m$.77 (B) | 8.77 | (20 years) | recurrent nova (NR) | |
| S Scl | Sculptor | | 5$^m$.5 | 13$^m$.6 | 8.1 | 363 d | Mira variable (M) | |
| RR Sco | Scorpius | | 5$^m$.0 | 12$^m$.4 | 7.4 | 281 d | Mira variable (M) | |
| RS Sco | Scorpius | | 6$^m$.2 | 13$^m$.0 | 6.8 | 320 d | Mira variable (M) | |
| RT Sco | Scorpius | | 7$^m$.0 | 15$^m$.2 | 8.2 | 449 d | Mira variable (M) | |
| R Sct | Scutum | Pigott, 1795 | 4$^m$.2 | 8$^m$.6 | 4.4 | 146.5 d | RV Tauri variable (RVA) | |
| R Ser | Serpens | Harding, 1826 | 5$^m$.16 | 14$^m$.4 | 9.24 | 356 d | Mira variable (M) | |
| S Ser | Serpens | Harding, 1828 | 7$^m$.0 | 14$^m$.1 | 7.1 | 372 d | Mira variable (M) | |
| U Sge | Sagitta | | 6$^m$.45 | 9$^m$.28 | 2.83 | 3.38062 d | Eclipsing binary Algol type (EA/SD) | |
| WZ Sge | Sagitta | | 7$^m$.0 (B) | 15$^m$.53 (B) | 8.53 | (33 years) | dwarf nova (UGSU+E+ZZ) | |
| RR Sgr | Sagittarius | | 5$^m$.4 | 14$^m$.0 | 8.6 | 336 d | Mira variable (M) | |
| R Sgr | Sagittarius | | 6$^m$.7 | 12$^m$.83 | 6.13 | 270 d | Mira variable (M) | |
| U Sgr | Sagittarius(in M25) | | 6$^m$.28 | 7$^m$.15 | 0.87 | 6.74523 d | Classical Cepheid (DCEP) | |
| RT Sgr | Sagittarius | | 6$^m$.0 | 14$^m$.1 | 8.1 | 306 d | Mira variable (M) | |
| RU Sgr | Sagittarius | | 6$^m$.0 | 13$^m$.8 | 7.8 | 240 d | Mira variable (M) | |
| RY Sgr | Sagittarius | | 5$^m$.8 | 14$^m$.0 | 8.2 | | R Coronae Borealis (RCB) | |
| VX Sgr | Sagittarius | | 6$^m$.52 | 14$^m$.0 | 7.08 | 732 d | Semiregular (SRC) | |
| λ Tau | Taurus | Baxendell, 1848 | 3$^m$.37 | 3$^m$.91 | 0.54 | 3.95295 d | Eclipsing binary Algol type (EA/DM) | |
| R Tau | Taurus | Hind, 1849 | 7$^m$.6 | 15$^m$.8 | 8.2 | 321 d | Mira variable (M) | |
| T Tau | Taurus | | 9$^m$.3 | 13$^m$.5 | 4.2 | | Orion variable (INT) | |
| SU Tau | Taurus | | 9$^m$.1 | 16$^m$.86 | 7.76 | | R Coronae Borealis (RCB) | |
| R Tri | Triangulum | | 5$^m$.4 | 12$^m$.6 | 7.2 | 267 d | Mira variable (M) | |
| R UMa | Ursa Major | | 6$^m$.5 | 13$^m$.7 | 7.2 | 302 d | Mira variable (M) | |
| T UMa | Ursa Major | | 6$^m$.6 | 13$^m$.5 | 6.9 | 257 d | Mira variable (M) | |
| U UMa | Ursa Major | | 6$^m$.20 | 6$^m$.25 | 0.05 | | - | |
| W UMa | Ursa Major | | 7$^m$.75 | 8$^m$.48 | 0.73 | 0.3336 d | Eclipsing binary W Ursae Majoris type (prototype) | |
| Z UMa | Ursa Major | | 6$^m$.2 | 9$^m$.4 | 3.2 | 196 d | Semiregular (SRB) | |
| α UMi (Polaris) | Ursa Minor | | 1$^m$.86 | 2$^m$.13 | 0.27 | 3.9696 d | Classical Cepheid (DCEPS) | |
| R Vir | Virgo | Harding, 1809 | 6$^m$.1 | 12$^m$.1 | 6.0 | 146 d | Mira variable (M) | |
| S Vir | Virgo | | 6$^m$.3 | 13$^m$.2 | 6.9 | 375 d | Mira variable (M) | |