Designation (name)
|
Constellation
|
Discovery
|
Apparent magnitude (Maximum)
|
Apparent magnitude (Minimum)
|
Range of magnitude
|
Period
|
Type
|
Comment
|
R And
|
Andromeda
|
|
5.8
|
14.9
|
9.1
|
409 d
|
Mira variable (M)
|
|
S And (Supernova 1885)
|
Andromeda
|
Ernst Hartwig, August 20, 1885
|
5.8
|
16
|
10.2
|
|
Supernova (SNI)
|
|
U Ant
|
Antlia
|
|
8.1 (p)
|
9.7 (p)
|
1.6
|
|
LB
|
|
θ Aps
|
Apus
|
|
6.4 (p)
|
8.6 (p)
|
2.2
|
119 d
|
Semiregular (SRB)
|
|
η Aql
|
Aquila
|
Pigott, 1784
|
3.48
|
4.39
|
0.91
|
7.17664 d
|
Classical Cepheid (DCEP)
|
|
R Aql
|
Aquila
|
|
5.5
|
12.0
|
6.5
|
284 d
|
Mira variable (M)
|
|
V Aql
|
Aquila
|
|
6.6
|
8.4
|
1.8
|
353 d
|
Semiregular (SRB)
|
|
R Aqr
|
Aquarius
|
Karl Ludwig Harding, 1810
|
5.8
|
12.4
|
6.9
|
387 d
|
Mira variable (M)
|
|
T Aqr
|
Aquarius
|
|
7.2
|
14.2
|
7.0
|
202 d
|
Mira variable (M)
|
|
U Ara
|
Ara
|
|
7.7
|
14.1
|
6.4
|
225 d
|
Mira variable (M)
|
|
R Ari
|
Aries
|
|
7.4
|
13.7
|
6.3
|
187 d
|
Mira variable (M)
|
|
U Ari
|
Aries
|
|
7.2
|
15.2
|
8.0
|
371 d
|
Mira variable (M)
|
|
ε Aur (Almaaz)
|
Auriga
|
Johann Heinrich Fritsch, 1821
|
2.92
|
3.83
|
0.91
|
27.08 years
|
Eclipsing binary Algol type (EA/GS)
|
|
R Aur
|
Auriga
|
|
6.7
|
13.9
|
7.2
|
458 d
|
Mira variable (M)
|
|
AE Aur
|
Auriga
|
|
5.78
|
6.08
|
0.30
|
|
Orion variable (INA)
|
|
R Boo
|
Boötes
|
|
6.2
|
13.1
|
6.9
|
223 d
|
Mira variable (M)
|
|
W Boo
|
Boötes
|
|
4.73
|
5.4
|
0.67
|
450 d
|
Semiregular (SRB:)
|
|
X Cam
|
Camelopardalis
|
|
7.4
|
14.2
|
6.8
|
144 d
|
Mira variable (M)
|
|
VZ Cam
|
Camelopardalis
|
|
4.80
|
4.96
|
0.16
|
23.7 d
|
Semiregular (SR)
|
|
R Cap
|
Capricornus
|
Hind, 1848
|
9.4
|
14.9
|
5.5
|
345 d
|
Mira variable (M)
|
|
η Car
|
Carina
|
Burchell, 1827
|
-0.8
|
7.9
|
8.6
|
|
S Doradus (SDOR)
|
"The unpredictable supergiant"
|
l Car
|
Carina
|
|
3.28
|
4.18
|
0.90
|
35.53584 d
|
Classical Cepheid (DCEP)
|
|
R Car
|
Carina
|
|
3.9
|
10.5
|
6.6
|
309 d
|
Mira variable (M)
|
|
S Car
|
Carina
|
|
4.5
|
9.9
|
5.4
|
149 d
|
Mira variable (M)
|
|
γ Cas
|
Cassiopeia
|
|
1.6
|
3.0
|
1.4
|
|
Gamma Cassiopeiae (GCAS)
|
|
R Cas
|
Cassiopeia
|
|
4.7
|
13.5
|
8.9
|
430 d
|
Mira variable (M)
|
|
S Cas
|
Cassiopeia
|
|
7.9
|
16.1
|
8.2
|
612 d
|
Mira variable (M)
|
|
W Cas
|
Cassiopeia
|
|
7.8
|
12.5
|
4.7
|
406 d
|
Mira variable (M)
|
|
WZ Cas
|
Cassiopeia
|
|
6.3
|
8.5
|
2.2
|
|
Semiregular (SRB)
|
Visual double star, visible through binoculars
|
R Cen
|
Centaurus
|
|
5.3
|
11.8
|
6.5
|
546 d
|
Mira variable (M)
|
|
S Cen
|
Centaurus
|
|
9.2 (p)
|
10.7 (p)
|
1.5
|
65 d
|
Semiregular (SR)
|
|
T Cen
|
Centaurus
|
|
5.5
|
9.0
|
3.5
|
90.44 d
|
Semiregular (SRA)
|
|
V645 Cen (Proxima Centauri)
|
Centaurus
|
|
12.1 (B)
|
13.12 (B)
|
1.02
|
|
UV Ceti (UV)
|
|
δ Cep
|
Cepheus
|
John Goodricke, 1784
|
3.48
|
4.37
|
0.89
|
5.36634 d
|
Classical Cepheid (DCEP) prototype
|
double star, visible in binoculars
|
Vega
|
Lyra
|
|
-0.02
|
0.07
|
0.09
|
0.107 d
|
Delta Scuti variable
|
Brightest variable star in the sky.
|
μ Cep (Herschel's Garnet Star)
|
Cepheus
|
William Herschel, 1782
|
3.43
|
5.1
|
1.67
|
730 d
|
Semiregular (SRC)
|
|
S Cep
|
Cepheus
|
|
7.4
|
12.9
|
5.5
|
487 d
|
Mira variable (M)
|
|
T Cep
|
Cepheus
|
|
5.2
|
11.3
|
6.1
|
388 d
|
Mira variable (M)
|
|
U Cep
|
Cepheus
|
|
6.75
|
9.24
|
2.49
|
2.49305 d
|
Eclipsing binary Algol type (EA/SD)
|
|
SS Cep
|
Cepheus
|
|
8.0 (p)
|
9.1 (p)
|
1.1
|
90 d
|
Semiregular (SRB)
|
|
ST Cep
|
Cepheus
|
|
7.8
|
|
|
None
|
Mira variable (M)
|
|
AR Cep
|
Cepheus
|
|
7.0
|
7.9
|
0.9
|
|
Semiregular (SRB)
|
|
ο Cet (Mira)
|
Cetus
|
David Fabricius, 1596; variability may have been first noted by Johannes Fokkes Holwarda, 1638
|
2.0
|
10.1
|
8.1
|
332 d
|
Mira variable (M)
|
"The miraculous" The first discovered non-ephemeral/cataclysmic variable star.
|
T Cet
|
Cetus
|
|
5.0
|
6.9
|
1.9
|
159 d
|
Semiregular (SRC)
|
|
U Cet
|
Cetus
|
|
6.8
|
13.4
|
6.6
|
235 d
|
Mira variable (M)
|
|
W Cet
|
Cetus
|
|
7.1
|
14.8
|
7.7
|
351 d
|
Mira variable (M)
|
|
R Cha
|
Chamaeleon
|
|
7.5
|
14.2
|
6.7
|
335 d
|
Mira variable (M)
|
|
R CMa
|
Canis Major
|
|
5.70
|
6.34
|
0.64
|
1.13594 d
|
Eclipsing binary Algol type (EA/SD)
|
|
VY CMa
|
Canis Major
|
|
6.5
|
9.6
|
3.1
|
|
unique (*)
|
|
FW CMa
|
Canis Major
|
|
5.00
|
5.50
|
0.50
|
|
Gamma Cassiopeiae (GCAS)
|
|
S CMi
|
Canis Minor
|
|
6.6
|
13.2
|
6.6
|
333 d
|
Mira variable (M)
|
|
R Cnc
|
Cancer
|
|
6.07
|
11.8
|
5.73
|
362 d
|
Mira variable (M)
|
|
S Cnc
|
Cancer
|
Hind, 1848
|
8.29
|
10.25
|
1.96
|
9.48455 d
|
Eclipsing binary Algol type (EA/DS)
|
|
T Cnc
|
Cancer
|
Hind, 1850
|
7.6
|
10.5
|
2.9
|
482 d
|
Semiregular (SRB)
|
|
X Cnc
|
Cancer
|
|
5.6
|
7.5
|
1.9
|
195 d
|
Semiregular (SRB)
|
|
T Col
|
Columba
|
|
6.6
|
12.7
|
6.1
|
226 d
|
Mira variable (M)
|
|
R Com
|
Coma Berenices
|
|
7.1
|
14.6
|
7.5
|
363 d
|
Mira variable (M)
|
|
α CrB (Alphecca or Gemma)
|
Corona Borealis
|
|
2.21 (B)
|
2.32 (B)
|
0.11
|
17.35991 d
|
Eclipsing binary Algol type (EA/DM)
|
|
R CrB
|
Corona Borealis
|
Piggott, 1795
|
5.71
|
14.8
|
9.09
|
|
R Coronae Borealis (RCB)
|
|
S CrB
|
Corona Borealis
|
|
5.8
|
14.1
|
8.7
|
360 d
|
Mira variable (M)
|
|
T CrB
|
Corona Borealis
|
|
2.0
|
10.8
|
8.8
|
(80 years)
|
recurrent nova (NR)
|
|
U CrB
|
Corona Borealis
|
|
7.66
|
8.79
|
1.13
|
3.45220 d
|
Eclipsing binary Algol type (EA/SD)
|
|
V CrB
|
Corona Borealis
|
|
6.9
|
12.6
|
5.3
|
358 d
|
Mira variable (M)
|
|
W CrB
|
Corona Borealis
|
|
7.8
|
14.3
|
6.5
|
238 d
|
Mira variable (M)
|
|
R Cru
|
Crux
|
|
6.40
|
7.23
|
0.83
|
5.82575 d
|
Classical Cepheid (DCEP)
|
|
R Crv
|
Corvus
|
|
6.7
|
14.4
|
7.7
|
317 d
|
Mira variable (M)
|
|
χ Cyg
|
Cygnus
|
Kirch, 1686
|
3.3
|
14.2
|
10.9
|
408 d
|
Mira variable (M)
|
|
R Cyg
|
Cygnus
|
|
6.1
|
14.4
|
8.3
|
426 d
|
Mira variable (M)
|
|
U Cyg
|
Cygnus
|
|
5.9
|
12.1
|
6.2
|
463 d
|
Mira variable (M)
|
|
W Cyg
|
Cygnus
|
|
6.80 (B)
|
8.9 (B)
|
2.1
|
131 d
|
Semiregular (SRB)
|
|
X Cyg
|
Cygnus
|
|
5.85
|
6.91
|
1.06
|
16.38633 d
|
Classical Cepheid (DCEP)
|
|
RT Cyg
|
Cygnus
|
|
6.0
|
13.1
|
7.1
|
190 d
|
Mira variable (M)
|
|
SS Cyg
|
Cygnus
|
|
7.7
|
12.4
|
4.7
|
(49.5 d)
|
dwarf nova UGSS prototype
|
|
SU Cyg
|
Cygnus
|
|
6.44
|
7.22
|
0.78
|
3.84555 d
|
Classical Cepheid (DCEP)
|
|
CH Cyg
|
Cygnus
|
|
5.60
|
8.49
|
2.89
|
|
Z Andromedae (ZAND+SR)
|
|
R Del
|
Delphinus
|
|
7.6
|
13.8
|
6.2
|
285 d
|
Mira variable (M)
|
|
U Del
|
Delphinus
|
|
7.6 (p)
|
8.9 (p)
|
1.3
|
110 d
|
Semiregular (SRB)
|
|
EU Del
|
Delphinus
|
|
5.79
|
6.9
|
1.11
|
59.7 d
|
Semiregular (SRB)
|
|
β Dor
|
Dorado
|
|
3.46
|
4.08
|
0.62
|
9.8426 d
|
Classical Cepheid (DCEP)
|
|
S Dor
|
Dorado
|
|
8.6 (B)
|
11.5 (B)
|
2.9
|
|
S Doradus (SDOR) (prototype)
|
in the Large Magellanic Cloud
|
R Dra
|
Draco
|
|
6.7
|
13.2
|
6.5
|
246 d
|
Mira variable (M)
|
|
T Eri
|
Eridanus
|
|
7.2
|
13.2
|
6.0
|
252 d
|
Mira variable (M)
|
|
R For
|
Fornax
|
|
7.5
|
13.0
|
5.5
|
389 d
|
Mira variable (M)
|
|
η Gem (Propus)
|
Gemini
|
|
3.15
|
3.9
|
0.75
|
233 d
|
Semiregular (SRA+EA)
|
|
ζ Gem (Mekbuda)
|
Gemini
|
|
3.62
|
4.18
|
0.56
|
10.15073 d
|
Classical Cepheid (DCEP)
|
|
R Gem
|
Gemini
|
Hind, 1848
|
6.0
|
14.0
|
8.0
|
370 d
|
Mira variable (M)
|
|
S Gem
|
Gemini
|
Hind, 1848
|
8.0
|
14.7
|
6.7
|
293 d
|
Mira variable (M)
|
|
T Gem
|
Gemini
|
Hind, 1848
|
8.0
|
15.0
|
7.0
|
288 d
|
Mira variable (M)
|
|
U Gem
|
Gemini
|
|
8.2
|
14.9
|
6.7
|
(105.2 d)
|
dwarf nova (UGSS+E)
|
|
S Gru
|
Grus
|
|
6.0
|
15.0
|
9.0
|
402 d
|
Mira variable (M)
|
|
α Her (Rasalgethi)
|
Hercules
|
William Herschel, 1759
|
2.74
|
4.0
|
1.26
|
|
Semiregular (SRC)
|
|
g Her (30 Her)
|
Hercules
|
|
4.3
|
6.3
|
2.0
|
89.2 d
|
Semiregular (SRB)
|
|
u Her (68 Her)
|
Hercules
|
|
4.69
|
5.37
|
0.68
|
2.05103 d
|
Eclipsing binary Algol type (EA/SD)
|
|
S Her
|
Hercules
|
|
6.4
|
13.8
|
7.4
|
307 d
|
Mira variable (M)
|
|
U Her
|
Hercules
|
|
6.4
|
13.4
|
7.0
|
406 d
|
Mira variable (M)
|
|
X Her
|
Hercules
|
|
7.5 (p)
|
8.6 (p)
|
1.1
|
95.0 d
|
Semiregular (SRB)
|
|
R Hor
|
Horologium
|
|
4.7
|
14.3
|
9.6
|
408 d
|
Mira variable (M)
|
|
U Hor
|
Horologium
|
|
7.8 (p)
|
15.1 (p)
|
6.3
|
348 d
|
Mira variable (M)
|
|
R Hya
|
Hydra
|
Maraldi, 1704
|
3.5
|
10.9
|
7.4
|
389 d
|
Mira variable (M)
|
|
S Hya
|
Hydra
|
Hind, 1848
|
7.2
|
13.3
|
6.1
|
257 d
|
Mira variable (M)
|
|
U Hya
|
Hydra
|
|
7.0 (B)
|
9.4 (B)
|
2.4
|
~450 d
|
Semiregular (SRB)
|
|
VW Hya
|
Hydra
|
|
10.5
|
14.1
|
3.6
|
2.69642 d
|
Eclipsing binary Algol type (EA/SD)
|
|
BL Lac
|
Lacerta
|
|
12.4 (B)
|
17.2 (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
|
4.4
|
11.3
|
6.9
|
310 d
|
Mira variable (M)
|
|
R Lep
|
Lepus
|
|
5.5
|
11.7
|
6.2
|
427 d
|
Mira variable (M)
|
Hind's Crimson Star
|
RX Lep
|
Lepus
|
|
5.0
|
7.4
|
2.4
|
~60 d
|
Semiregular (SRB)
|
|
R LMi
|
Leo Minor
|
|
6.3
|
13.2
|
6.9
|
372 d
|
Mira variable (M)
|
|
RU Lup
|
Lupus
|
|
9.6 (p)
|
13.4 (p)
|
3.8
|
|
Orion variable (INT)
|
|
β Lyr (Sheliak)
|
Lyra
|
John Goodricke, 1784
|
3.25
|
4.36
|
1.11
|
12.91383 d
|
Eclipsing binary Beta Lyrae type (prototype)
|
|
R Lyr
|
Lyra
|
|
3.88
|
5.0
|
1.12
|
~46 d
|
Semiregular (SRB)
|
|
RR Lyr
|
Lyra
|
|
7.06
|
8.12
|
1.06
|
0.566868 d
|
RR Lyrae variable (prototype)
|
|
U Mic
|
Microscopium
|
|
7.0
|
14.4
|
7.7
|
334 d
|
Mira variable (M)
|
|
U Mon
|
Monoceros
|
|
6.1 (p)
|
8.8 (p)
|
2.7
|
91.3 d
|
RV Tauri variable (RVB)
|
|
V Mon
|
Monoceros
|
|
6.0
|
13.9
|
7.9
|
341 d
|
Mira variable (M)
|
|
R Nor
|
Norma
|
|
6.5 (p)
|
13.9 (p)
|
7.4
|
508 d
|
Mira variable (M)
|
|
T Nor
|
Norma
|
|
6.2
|
13.6
|
7.4
|
241 d
|
Mira variable (M)
|
|
R Oct
|
Octans
|
|
6.4
|
13.2
|
6.8
|
405 d
|
Mira variable (M)
|
|
S Oct
|
Octans
|
|
7.2
|
14.0
|
6.8
|
259 d
|
Mira variable (M)
|
|
V Oph
|
Ophiuchus
|
|
7.3
|
11.6
|
4.3
|
297 d
|
Mira variable (M)
|
|
X Oph
|
Ophiuchus
|
|
5.9
|
9.2
|
3.3
|
329 d
|
Mira variable (M)
|
|
RS Oph
|
Ophiuchus
|
|
4.3
|
12.5
|
8.2
|
|
recurrent nova (NR)
|
|
BF Oph
|
Ophiuchus
|
|
6.93
|
7.71
|
0.78
|
4.06775 d
|
Classical Cepheid (DCEP)
|
|
α Ori (Betelgeuse)
|
Orion
|
John Herschel, 1840
|
0.0
|
1.3
|
1.3
|
6.39 years
|
Semiregular (SRC)
|
|
δ Ori (Mintaka)
|
Orion
|
John Herschel, 1834
|
2.14
|
2.26
|
0.12
|
5.73248 d
|
Eclipsing binary Algol type (EA/DM)
|
|
R Ori
|
Orion
|
Hind, 1848
|
9.05
|
13.4
|
4.35
|
377 d
|
Mira variable (M)
|
|
U Ori
|
Orion
|
|
4.8
|
13.0
|
8.5
|
368 d
|
Mira variable (M)
|
|
W Ori
|
Orion
|
|
8.2 (p)
|
12.4 (p)
|
4.2
|
212 d
|
Semiregular (SRB)
|
|
VV Ori
|
Orion
|
|
5.31
|
5.66
|
0.35
|
1.48538 d
|
Eclipsing binary Algol type (EA/KE:)
|
|
CK Ori
|
Orion
|
|
5.9
|
7.1
|
1.2
|
~120 d
|
Semiregular (SR:)
|
|
κ Pav
|
Pavo
|
|
3.91
|
4.78
|
0.87
|
9.09423 d
|
Type II Cepheid (CW)
|
|
S Pav
|
Pavo
|
|
6.6
|
10.4
|
3.8
|
381 d
|
Semiregular (SRA)
|
|
β Peg (Scheat)
|
Pegasus
|
Schmidt, 1847
|
2.31
|
2.74
|
0.43
|
|
LB
|
|
ε Peg (Enif)
|
Pegasus
|
|
0.7
|
3.5
|
2.8
|
|
LC
|
|
R Peg
|
Pegasus
|
Hind, 1848
|
6.9
|
13.8
|
6.9
|
378 d
|
Mira variable (M)
|
|
X Peg
|
Pegasus
|
|
8.8
|
14.4
|
5.8
|
201 d
|
Mira variable (M)
|
|
β Per (Algol)
|
Perseus
|
Geminiano Montanari, 1669
|
2.12
|
3.39
|
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
|
|
3.96
|
4.11
|
0.15
|
19.5 d
|
Gamma Cassiopeiae (GCAS)
|
|
ρ Per
|
Perseus
|
|
3.30
|
4.0
|
0.70
|
~50 d
|
Semiregular (SRB)
|
|
X Per
|
Perseus
|
|
6.03
|
7.0
|
0.97
|
|
Gamma Cassiopeiae (GCAS+XP)
|
|
ζ Phe (Wurren)
|
Phoenix
|
|
3.91
|
4.42
|
0.51
|
1.66977 d
|
Eclipsing binary Algol type (EA/DM)
|
|
R Pic
|
Pictor
|
|
6.35
|
10.1
|
3.75
|
171 d
|
Semiregular (SR)
|
|
R Psc
|
Pisces
|
Hind, 1850
|
7.0
|
14.8
|
7.8
|
345 d
|
Mira variable (M)
|
|
TX Psc
|
Pisces
|
|
4.79
|
5.20
|
0.42
|
|
LB
|
|
L Pup
|
Puppis
|
|
2.6
|
6.2
|
3.6
|
141 d
|
Semiregular (SRB)
|
|
RS Pup
|
Puppis
|
|
6.52
|
7.67
|
1.15
|
41.3876 d
|
Classical Cepheid (DCEP)
|
|
T Pyx
|
Pyxis
|
|
7.0 (B)
|
15.77 (B)
|
8.77
|
(20 years)
|
recurrent nova (NR)
|
|
S Scl
|
Sculptor
|
|
5.5
|
13.6
|
8.1
|
363 d
|
Mira variable (M)
|
|
RR Sco
|
Scorpius
|
|
5.0
|
12.4
|
7.4
|
281 d
|
Mira variable (M)
|
|
RS Sco
|
Scorpius
|
|
6.2
|
13.0
|
6.8
|
320 d
|
Mira variable (M)
|
|
RT Sco
|
Scorpius
|
|
7.0
|
15.2
|
8.2
|
449 d
|
Mira variable (M)
|
|
R Sct
|
Scutum
|
Pigott, 1795
|
4.2
|
8.6
|
4.4
|
146.5 d
|
RV Tauri variable (RVA)
|
|
R Ser
|
Serpens
|
Harding, 1826
|
5.16
|
14.4
|
9.24
|
356 d
|
Mira variable (M)
|
|
S Ser
|
Serpens
|
Harding, 1828
|
7.0
|
14.1
|
7.1
|
372 d
|
Mira variable (M)
|
|
U Sge
|
Sagitta
|
|
6.45
|
9.28
|
2.83
|
3.38062 d
|
Eclipsing binary Algol type (EA/SD)
|
|
WZ Sge
|
Sagitta
|
|
7.0 (B)
|
15.53 (B)
|
8.53
|
(33 years)
|
dwarf nova (UGSU+E+ZZ)
|
|
RR Sgr
|
Sagittarius
|
|
5.4
|
14.0
|
8.6
|
336 d
|
Mira variable (M)
|
|
R Sgr
|
Sagittarius
|
|
6.7
|
12.83
|
6.13
|
270 d
|
Mira variable (M)
|
|
U Sgr
|
Sagittarius(in M25)
|
|
6.28
|
7.15
|
0.87
|
6.74523 d
|
Classical Cepheid (DCEP)
|
|
RT Sgr
|
Sagittarius
|
|
6.0
|
14.1
|
8.1
|
306 d
|
Mira variable (M)
|
|
RU Sgr
|
Sagittarius
|
|
6.0
|
13.8
|
7.8
|
240 d
|
Mira variable (M)
|
|
RY Sgr
|
Sagittarius
|
|
5.8
|
14.0
|
8.2
|
|
R Coronae Borealis (RCB)
|
|
VX Sgr
|
Sagittarius
|
|
6.52
|
14.0
|
7.08
|
732 d
|
Semiregular (SRC)
|
|
λ Tau
|
Taurus
|
Baxendell, 1848
|
3.37
|
3.91
|
0.54
|
3.95295 d
|
Eclipsing binary Algol type (EA/DM)
|
|
R Tau
|
Taurus
|
Hind, 1849
|
7.6
|
15.8
|
8.2
|
321 d
|
Mira variable (M)
|
|
T Tau
|
Taurus
|
|
9.3
|
13.5
|
4.2
|
|
Orion variable (INT)
|
|
SU Tau
|
Taurus
|
|
9.1
|
16.86
|
7.76
|
|
R Coronae Borealis (RCB)
|
|
R Tri
|
Triangulum
|
|
5.4
|
12.6
|
7.2
|
267 d
|
Mira variable (M)
|
|
R UMa
|
Ursa Major
|
|
6.5
|
13.7
|
7.2
|
302 d
|
Mira variable (M)
|
|
T UMa
|
Ursa Major
|
|
6.6
|
13.5
|
6.9
|
257 d
|
Mira variable (M)
|
|
U UMa
|
Ursa Major
|
|
6.20
|
6.25
|
0.05
|
|
-
|
|
W UMa
|
Ursa Major
|
|
7.75
|
8.48
|
0.73
|
0.3336 d
|
Eclipsing binary W Ursae Majoris type (prototype)
|
|
Z UMa
|
Ursa Major
|
|
6.2
|
9.4
|
3.2
|
196 d
|
Semiregular (SRB)
|
|
α UMi (Polaris)
|
Ursa Minor
|
|
1.86
|
2.13
|
0.27
|
3.9696 d
|
Classical Cepheid (DCEPS)
|
|
R Vir
|
Virgo
|
Harding, 1809
|
6.1
|
12.1
|
6.0
|
146 d
|
Mira variable (M)
|
|
S Vir
|
Virgo
|
|
6.3
|
13.2
|
6.9
|
375 d
|
Mira variable (M)
|
|