List of stars in Andromeda

This is the list of notable stars in the constellation Andromeda, sorted by decreasing brightness.

Notes

Alpheratz

α, (δ)^[1]

21

358

677

00^h 08^m 23.17^s

+29° 05′ 27.0″

2.07

−0.30

97

B9p

Alpheratz, Sirrah; α² CVn variable, ΔV = 0.04^m, P = 0.966222 d; spectroscopic binary, also δ Peg

Mirach

β

43

6860

5447

01^h 09^m 43.80^s

+35° 37′ 15.0″

2.07

−1.86

199

M0IIIvar

Mirach; variable

γ¹ And

γ¹

57

12533

9640

02^h 03^m 53.92^s

+42° 19′ 47.5″

2.10

−3.08

355

K3IIb

Almach; quadruple star system

δ And

δ

31

3627

3092

00^h 39^m 19.60^s

+30° 51′ 40.4″

3.27

0.81

101

K3III...

Sadiradra; spectroscopic binary; suspected variable

Andromeda Galaxy

(n)^[2]

33

00^h 42^m 44.31^s

+41° 16′ 09.4″

3.44^[3]
(nebulous)

2540000

BD+40°148; naked eye spiral galaxy in the Local group

51 And

(υ)^[4]^[5]

51

9927

7607

01^h 37^m 59.50^s

+48° 37′ 42.6″

3.59

−0.04

174

K3III

Nembus; multiple star

ο And

ο

1

217675

113726

23^h 01^m 55.25^s

+42° 19′ 33.5″

3.62

−3.01

692

B6pv SB

quadruple star system; γ Cas variable, V_max = 3.55^m, V_min = 3.78^m

λ And

λ

16

222107

116584

23^h 37^m 33.71^s

+46° 27′ 33.0″

3.81

1.75

84

G8III-IV

RS CVn variable, V_max = 3.65^m, V_min = 4.05^m, P = 53.95 d

μ And

μ

37

5448

4436

00^h 56^m 45.10^s

+38° 29′ 57.3″

3.86

0.75

136

A5V

multiple star

ζ And

ζ

34

4502

3693

00^h 47^m 20.39^s

+24° 16′ 02.6″

4.08

0.35

181

K1II

β Lyr/RS CVn variable, V_max = 3.92^m, V_min = 4.14^m, P = 17.7696 d

υ And

^[6]^[7]

50

9826

7513

01^h 36^m 47.98^s

+41° 24′ 23.0″

4.10

3.45

44

F8V

Titawin,^[8] has four planets (b, c, d & e)

κ And

κ

19

222439

116805

23^h 40^m 24.44^s

+44° 20′ 02.3″

4.15

0.57

170

B9IVn

triple star, has a planet (b)

φ And

φ

42

6811

5434

01^h 09^m 30.12^s

+47° 14′ 30.6″

4.26

−2.51

736

B7III

emission-line star

ι And

ι

17

222173

116631

23^h 38^m 08.18^s

+43° 16′ 05.1″

4.29

−1.65

502

B8V

Keff al Salsalat, Manus Catenata^[9]

π And

π

29

3369

2912

00^h 36^m 52.84^s

+33° 43′ 09.7″

4.34

−2.18

656

B5V

spectroscopic binary; suspected variable

ε And

ε

30

3546

3031

00^h 38^m 33.50^s

+29° 18′ 44.5″

4.34

0.77

169

G5III...

η And

η

38

5516

4463

00^h 57^m 12.43^s

+23° 25′ 03.9″

4.40

0.04

243

G8III-IV

spectroscopic binary

σ And

σ

25

1404

1473

00^h 18^m 19.71^s

+36° 47′ 07.2″

4.51

1.33

141

A2V

suspected variable

ν And

ν

35

4727

3881

00^h 49^m 48.83^s

+41° 04′ 44.2″

4.53

−2.06

679

B5V SB

spectroscopic binary

7 And

7

219080

114570

23^h 12^m 32.92^s

+49° 24′ 21.5″

4.53

2.58

80

F0V

θ And

θ

24

1280

1366

00^h 17^m 05.54^s

+38° 40′ 54.0″

4.61

0.16

253

A2V

suspected variable

3 And

3

218031

113919

23^h 04^m 10.83^s

+50° 03′ 06.1″

4.64

0.94

179

K0III

65 And

65

14872

11313

02^h 25^m 37.40^s

+50° 16′ 43.2″

4.73

−0.39

345

K4III

triple star

58 And

58

13041

9977

02^h 08^m 29.15^s

+37° 51′ 33.1″

4.78

0.86

198

A5IV-V

8 And

8

219734

115022

23^h 17^m 44.62^s

+49° 00′ 55.0″

4.82

−1.69

655

M2III

suspected variable

ω And

ω^[10]

48

8799

6813

01^h 27^m 39.09^s

+45° 24′ 25.0″

4.83

2.57

92

F5IV

γ² And

γ²

57

12534

02^h 03^m 54.70^s

+42° 19′ 51.0″

4.84

-0.3

350

B8V

component of the γ And system; triple star system

60 And

b

60

13520

10340

02^h 13^m 13.34^s

+44° 13′ 54.1″

4.84

−1.32

556

K4III

suspected variable

ξ And

ξ^[10]

46

8207

6411

01^h 22^m 20.39^s

+45° 31′ 43.5″

4.87

0.98

195

K0III-IV

Adhil

τ And

τ

53

10205

7818

01^h 40^m 34.80^s

+40° 34′ 37.6″

4.96

−1.64

681

B8III

suspected variable

41 H. And

υ^[11]

10307

7918

01^h 41^m 46.52^s

+42° 36′ 49.7″

4.96

4.45

41

G2V

spectroscopic binary

ψ And

ψ

20

223047

117221

23^h 46^m 02.04^s

+46° 25′ 13.0″

4.97

−3.05

1309

G5Ib

multiple star

22 And

22

571

841

00^h 10^m 19.24^s

+46° 04′ 20.2″

5.01

−2.44

1006

F2II

χ And

χ^[12]

52

10072

7719

01^h 39^m 21.02^s

+44° 23′ 10.1″

5.01

0.66

242

G8III...

41 And

(d)^[13]

41

6658

5317

01^h 08^m 00.72^s

+43° 56′ 32.1″

5.04

1.14

196

A3m

2 And

2

217782

113788

23^h 02^m 36.34^s

+42° 45′ 28.1″

5.09

−0.06

349

A3Vn

multiple star

V428 And

V428

3346

2900

00^h 36^m 46.47^s

+44° 29′ 18.6″

5.14

−1.38

656

K5III

semiregular variable, ΔV = 0.06^m, P = 11.5 d; has a possible planetary system

ρ And

ρ

27

1671

1686

00^h 21^m 07.23^s

+37° 58′ 07.3″

5.16

1.71

160

F5III

HD 2421

2421

2225

00^h 28^m 13.59^s

+44° 23′ 40.2″

5.18

0.63

265

A2Vs

spectroscopic binary

64 And

64

14770

11220

02^h 24^m 24.89^s

+50° 00′ 23.9″

5.19

−0.11

375

G8III

GN And

28

GN

2628

2355

00^h 30^m 07.34^s

+29° 45′ 06.1″

5.20

1.43

185

A7III

low-amplitude δ Sct variable, ΔV = 0.05^m, P = 0.0693041 d

14 And

14

221345

116076

23^h 31^m 17.20^s

+39° 14′ 11.0″

5.22

0.80

249

K0III

Veritate,^[8] suspected variable; has a planet (b)

49 And

A^[14]

49

9057

6999

01^h 30^m 06.10^s

+47° 00′ 26.6″

5.27

0.53

290

K0III

32 And

32

3817

3231

00^h 41^m 07.20^s

+39° 27′ 31.2″

5.30

0.18

344

G8III

4 And

4

218452

114200

23^h 07^m 39.28^s

+46° 23′ 14.3″

5.30

0.20

342

K5III

double star

6 Per

^[15]

(6)^[16]

13530

10366

02^h 13^m 36.02^s

+51° 03′ 58.4″

5.31

1.38

199

G8III:var

spectroscopic binary; suspected variable

62 And

c

62

14212

10819

02^h 19^m 16.85^s

+47° 22′ 48.0″

5.31

0.84

255

A1V

18 And

18

222304

116709

23^h 39^m 08.35^s

+50° 28′ 18.3″

5.35

−0.04

390

B9V

55 And

55

11428

8814

01^h 53^m 17.35^s

+40° 43′ 47.3″

5.42

−0.67

540

K1III

double star

11 And

11

219945

115152

23^h 19^m 29.79^s

+48° 37′ 30.7″

5.44

0.43

328

K0III

3421

2942

00^h 37^m 21.23^s

+35° 23′ 58.2″

5.45

−2.03

1022

G5III

36 And

36

5286

4288

00^h 54^m 58.02^s

+23° 37′ 42.4″

5.46

2.51

127

K1IV

suspected variable

V340 And

15

V340

221756

116354

23^h 34^m 37.55^s

+40° 14′ 11.6″

5.55

1.28

233

A1III

low-amplitude δ Sct variable, ΔV = 0.007^m

PZ And

63

PZ

14392

10944

02^h 20^m 58.17^s

+50° 09′ 05.5″

5.57

0.38

356

B9p Si

α² CVn variable, ΔV = 0.05^m, P = 4.189 d

47 And

47

8374

6514

01^h 23^m 40.56^s

+37° 42′ 54.0″

5.60

1.54

211

A1m

10204

7825

01^h 40^m 39.56^s

+43° 17′ 51.9″

5.63

1.05

268

A9IV:

44 And

44

6920

5493

01^h 10^m 18.85^s

+42° 04′ 53.7″

5.67

2.06

172

F8V

5 And

5

218470

114210

23^h 07^m 45.25^s

+49° 17′ 43.6″

5.68

3.02

111

F5V

HD 5788

5788

4675

01^h 00^m 03.55^s

+44° 42′ 47.9″

5.69

0.14

420

A2Vn

binary star with HD 5789

56 And

56

11749

9021

01^h 56^m 09.23^s

+37° 15′ 06.5″

5.69

0.73

320

G8III...

multiple star

23 And

23

905

1086

00^h 13^m 30.94^s

+41° 02′ 08.6″

5.71

2.99

114

F0IV

HD 16028

16028

12072

02^h 35^m 38.74^s

+37° 18′ 44.2″

5.72

−0.86

676

K4III

triple star

V388 And

13

V388

220885

115755

23^h 27^m 07.33^s

+42° 54′ 43.1″

5.75

0.97

294

B9III

α² CVn variable, V_max = 5.73^m, V_min = 5.77^m, P = 1.47931 d

12 And

12

220117

115280

23^h 20^m 53.17^s

+38° 10′ 56.9″

5.77

2.63

138

F5V

triple star

1632

1657

00^h 20^m 45.54^s

+32° 54′ 40.4″

5.79

−0.69

646

K5III

45 And

45

7019

5550

01^h 11^m 10.29^s

+37° 43′ 26.9″

5.80

−1.44

916

B7III-IV

double star

HD 14622

14622

11090

02^h 22^m 50.36^s

+41° 23′ 47.5″

5.81

2.44

154

F0III-IV

has two optical companions

10 And

10

219981

115191

23^h 19^m 52.38^s

+42° 04′ 40.9″

5.81

−0.30

542

M0III

HD 222109

222109

116582

23^h 37^m 32.03^s

+44° 25′ 44.5″

5.81

−1.20

823

B8V

double star

HD 224635

224635

118281

23^h 59^m 29.33^s

+33° 43′ 26.9″

5.81

3.50

95

F8

multiple star

OU And

OU

223460

117503

23^h 49^m 40.96^s

+36° 25′ 31.4″

5.86

0.21

440

G1IIIe

FK Com variable, ΔV = 0.07^m, P = 24.2 d

1439

1493

00^h 18^m 38.22^s

+31° 31′ 02.0″

5.88

−0.23

543

A0IV

HD 2767

2767

2475

00^h 31^m 25.61^s

+33° 34′ 54.1″

5.88

0.10

467

K1III...

binary star

HD 1606

1606

1630

00^h 20^m 24.39^s

+30° 56′ 08.2″

5.89

−0.37

582

B7V

suspected variable

11727

9001

01^h 55^m 54.47^s

+37° 16′ 40.1″

5.89

−1.52

991

K5III

optical component of 56 And

KK And

KK

9531

7321

01^h 34^m 16.60^s

+37° 14′ 13.9″

5.90

0.50

392

B8Vp(Si)

α² CVn variable, ΔV = 0.012^m, P = 0.6684 d

16176

12181

02^h 36^m 57.08^s

+38° 44′ 02.3″

5.91

2.24

177

F5V

6 And

6

218804

114430

23^h 10^m 27.36^s

+43° 32′ 41.1″

5.91

3.65

112

F5V

Astrometric binary

10975

8423

01^h 48^m 38.84^s

+37° 57′ 10.6″

5.94

1.06

308

K0III

39 And

39

6116

4903

01^h 02^m 54.28^s

+41° 20′ 42.7″

5.95

0.84

344

A5m

double star

8671

6711

01^h 26^m 18.60^s

+43° 27′ 28.4″

5.98

2.90

135

F7V

AN And

9

AN

219815

115065

23^h 18^m 23.33^s

+41° 46′ 25.3″

5.98

0.17

472

A7m

β Lyr variable, V_max = 5.96^m, V_min = 6.11^m, P = 3.21952 d

HD 5608

5608

4552

00^h 58^m 14.19^s

+33° 57′ 03.8″

5.99

2.17

190

K0

has a transiting planet (b)

224165

117956

23^h 55^m 33.48^s

+47° 21′ 21.0″

6.01

−2.46

1614

G8Ib

224342

118071

23^h 57^m 03.63^s

+42° 39′ 29.7″

6.01

−2.22

1442

F8III

4335

3604

00^h 46^m 10.80^s

+44° 51′ 41.4″

6.03

0.32

452

B9.5IIIMNp.

13594

10403

02^h 14^m 02.53^s

+47° 29′ 03.8″

6.05

2.96

135

F5V

HD 3883

3883

3269

00^h 41^m 35.98^s

+24° 37′ 44.6″

6.06

0.30

462

A7m

suspected variable

V439 And

V439

166

544

00^h 06^m 36.53^s

+29° 01′ 19.0″

6.07

5.39

45

K0V

BY Draconis variable, ΔV = 0.04^m, P = 6.23 d

5118

4185

00^h 53^m 28.22^s

+37° 25′ 05.9″

6.07

0.77

374

K3III:

221293

116030

23^h 30^m 39.54^s

+38° 39′ 44.0″

6.07

−0.33

621

G9III

HD 223229

223229

117340

23^h 47^m 33.05^s

+46° 49′ 57.3″

6.08

−1.96

1320

B3IV

suspected variable

225239

394

00^h 04^m 53.21^s

+34° 39′ 34.4″

6.09

3.26

120

G2V

59 And A

59

13294

10176

02^h 10^m 52.83^s

+39° 02′ 22.5″

6.09

1.56

263

B9V

binary star

26 And

26

1438

1501

00^h 18^m 42.15^s

+43° 47′ 28.1″

6.10

−0.53

692

B8V

double star

5526

4501

00^h 57^m 39.64^s

+45° 50′ 21.8″

6.10

0.45

439

K2III

HD 225218

225218

365

00^h 04^m 36.60^s

+42° 05′ 33.2″

6.11

−2.45

1680

B9III

double star

7647

5993

01^h 17^m 05.05^s

+44° 54′ 07.5″

6.11

−0.18

590

K5

HD 1185

1185

1302

00^h 16^m 21.50^s

+43° 35′ 42.4″

6.12

1.28

303

A2V

double star

218416

114162

23^h 07^m 10.05^s

+52° 48′ 59.6″

6.12

0.55

423

K0III

GO And

GO

4778

3919

00^h 50^m 18.21^s

+45° 00′ 08.1″

6.13

1.34

296

A0p...

α² CVn variable, ΔV = 0.04^m, P = 2.5481 d

7158

5650

01^h 12^m 34.06^s

+45° 20′ 14.9″

6.13

−0.52

698

M1III

66 And

66

15138

11465

02^h 27^m 51.75^s

+50° 34′ 12.7″

6.16

2.54

173

F4V

spectroscopic binary

14372

10924

02^h 20^m 41.50^s

+47° 18′ 39.0″

6.17

−0.87

836

B5V

743

967

00^h 11^m 59.03^s

+48° 09′ 08.5″

6.18

0.05

550

K4III

3411

2926

00^h 37^m 07.20^s

+24° 00′ 51.3″

6.18

1.13

334

K2III

HD 221776

221776

116365

23^h 34^m 46.73^s

+38° 01′ 26.3″

6.18

−0.41

678

K5

double star

16327

12287

02^h 38^m 17.86^s

+37° 43′ 36.6″

6.19

1.60

270

F6III

triple star

HD 221246

221246

115996

23^h 30^m 07.39^s

+49° 07′ 59.3″

6.19

−0.91

856

K5III

member of the NGC 7686 star cluster

OP And

OP

9746

7493

01^h 36^m 27.21^s

+48° 43′ 22.2″

6.20

0.65

420

K1III:

BY Dra variable, ΔV = 0.09^m

400

699

00^h 08^m 41.02^s

+36° 37′ 38.7″

6.21

3.61

108

F8IV

14213

10814

02^h 19^m 10.84^s

+46° 28′ 20.2″

6.21

0.50

452

A4V

952

1123

00^h 14^m 02.29^s

+33° 12′ 21.9″

6.22

1.45

293

A1V

HD 895

895

1076

00^h 13^m 23.93^s

+26° 59′ 15.4″

6.24

0.78

403

G0III

triple star

222451

116824

23^h 40^m 40.47^s

+36° 43′ 14.6″

6.24

3.01

144

F1V

224906

137

00^h 01^m 43.85^s

+42° 22′ 01.7″

6.25

−1.80

1331

B9IIIp Mn

11613

8922

01^h 54^m 53.75^s

+40° 42′ 07.9″

6.25

1.13

345

K2

HD 220105

220105

115261

23^h 20^m 44.11^s

+44° 06′ 58.5″

6.25

1.73

261

A5Vn

double star

221661

116292

23^h 33^m 42.99^s

+45° 03′ 29.1″

6.25

0.12

548

G8II

HD 2942

2942

2583

00^h 32^m 49.09^s

+28° 16′ 48.8″

6.26

0.47

469

G8II

triple star

8774

6776

01^h 27^m 06.21^s

+34° 22′ 39.3″

6.27

3.12

139

F7IVsvar

2507

2270

00^h 28^m 56.67^s

+36° 53′ 58.9″

6.28

0.51

464

G5III

8375

6512

01^h 23^m 37.31^s

+34° 14′ 44.2″

6.28

2.43

192

G8IV

11624

8930

01^h 54^m 57.63^s

+37° 07′ 42.0″

6.28

0.25

525

K0

7758

6087

01^h 18^m 10.14^s

+47° 25′ 11.0″

6.29

−2.07

1531

K0

16350

12305

02^h 38^m 27.94^s

+38° 05′ 21.0″

6.29

−0.47

734

B9.5V

219962

115171

23^h 19^m 41.37^s

+48° 22′ 51.1″

6.29

0.47

475

K1III

217314

113501

22^h 59^m 10.37^s

+52° 39′ 16.0″

6.31

−0.26

672

K2

10597

8127

01^h 44^m 26.53^s

+46° 08′ 23.2″

6.32

0.23

540

K5III

219290

114714

23^h 14^m 14.34^s

+50° 37′ 04.5″

6.32

0.82

411

A0V

10486

8044

01^h 43^m 16.39^s

+45° 19′ 21.5″

6.33

2.61

181

K2IV

10874

8370

01^h 47^m 48.00^s

+46° 13′ 47.6″

6.33

2.50

190

F6V

1075

1208

00^h 15^m 06.93^s

+31° 32′ 08.7″

6.34

−1.70

1320

K5

HD 8673

8673

6702

01^h 26^m 08.62^s

+34° 34′ 47.7″

6.34

3.43

125

F7V

has a planet (b)

1083

1215

00^h 15^m 10.55^s

+27° 17′ 00.5″

6.35

0.84

412

A1Vn

double star

1527

1575

00^h 19^m 41.58^s

+40° 43′ 46.2″

6.35

0.25

541

K1III

221970

116505

23^h 36^m 30.52^s

+32° 54′ 15.1″

6.35

1.92

251

F6V

CG And

CG

224801

63

00^h 00^m 43.62^s

+45° 15′ 12.0″

6.36

−0.23

678

B9p SiEu

α² CVn variable, V_max = 6.32^m, V_min = 6.42^m, P = 3.73975 d

HD 16004

16004

12057

02^h 35^m 27.89^s

+39° 39′ 52.1″

6.36

0.11

580

B9MNp...

triple star

13818

10562

02^h 15^m 57.69^s

+47° 48′ 43.4″

6.37

0.61

462

G9III-IV

LN And

LN

217811

113802

23^h 02^m 45.15^s

+44° 03′ 31.6″

6.37

−1.42

1177

B2V

double star; not variable despite designation

V385 And

V385

220524

115530

23^h 24^m 08.88^s

+41° 36′ 46.3″

6.37

−1.55

1249

M0

irregular variable, V_max = 6.36^m, V_min = 6.47^m

GY And

GY

9996

7651

01^h 38^m 31.84^s

+45° 23′ 58.9″

6.38

0.66

455

B9Vp (Cr-Eu)

Promethium lines; α² CVn variable, V_max = 6.27^m, V_min = 6.44^m, P = 8000 d

13013

9983

02^h 08^m 33.55^s

+44° 27′ 34.4″

6.38

0.78

430

G8III

218365

114152

23^h 07^m 04.99^s

+35° 38′ 11.3″

6.38

−0.08

638

K0

9712

7444

01^h 35^m 52.46^s

+41° 04′ 35.1″

6.39

1.01

388

K1III

V529 And

V529

8801

6794

01^h 27^m 26.67^s

+41° 06′ 04.0″

6.42

2.69

182

Am...

δ Scuti variable, ΔV = 0.03^m, P = 0.40331 d

217731

113750

23^h 02^m 11.32^s

+44° 34′ 22.4″

6.43

1.22

359

K0

HD 222641

222641

116941

23^h 42^m 14.68^s

+44° 59′ 30.3″

6.43

−0.48

786

K5III

suspected variable

HD 7853

7853

6140

01^h 18^m 47.02^s

+37° 23′ 10.7″

6.44

0.71

456

A5m

double star

14221

10830

02^h 19^m 22.77^s

+48° 57′ 19.0″

6.44

2.39

210

F4V

219668

114981

23^h 17^m 16.59^s

+45° 09′ 51.5″

6.44

2.10

241

K0IV

HD 6114

6114

4911

01^h 03^m 01.47^s

+47° 22′ 34.3″

6.46

1.39

337

A9V

double star

11884

9163

01^h 57^m 59.23^s

+47° 05′ 43.9″

6.48

−1.24

1140

K0

ET And

ET

219749

115036

23^h 17^m 55.99^s

+45° 29′ 20.2″

6.48

0.36

545

B9Vp(Si)

α² CVn variable, ΔV = 0.03^m, P = 1.61888 d

HD 222399

222399

116781

23^h 40^m 02.82^s

+37° 39′ 10.2″

6.49

1.74

291

F2IV

double star

PY And

PY

3322

2865

00^h 36^m 20.00^s

+27° 15′ 17″

6.50

-0.16

701

B8IIImnp...

α² CVn variable, ΔV = ~0.03^m

800

1009

00^h 12^m 34.08^s

+44° 42′ 26.1″

6.50

0.50

517

K0

59 And B

59

13295

10180

02^h 10^m 53.67^s

+39° 02′ 36.0″

6.82

−1.76

1698

A1Vn

component of the 59 And system

HD 222155

222155

116616

23^h 38^m 00^s

+48° 59′ 47″

7.1

3.65

160

G2V

has a planet (b)

HD 16175

16175

12191

02^h 37^m 01.91^s

+42° 03′ 45.5″

7.28

3.40

195

G0

Buna; has a planet (b)

R And

R

1967

1901

00^h 24^m 01.95^s

+38° 34′ 37.3″

7.39

-5.19

790

S6.5IIIeZr6Ti2

Mira variable, V_max = 5.8^m, V_min = 15.2^m, P = 409.2 d

HD 1605

1605

1640

00^h 20^m 32.0^s

+30° 58′ 29″

7.52

2.88

276

K1IV

has two planets (b & c)

HD 13931

13931

10626

02^h 16^m 47.38^s

+43° 46′ 22.8″

7.52

4.3

144

G0

has a planet (b)

HD 5583

5583

00^h 57^m 57.0^s

+34° 59′ 08″

7.6

0.88

721

K0

has a planet (b)

RW And

RW

4489

00^h 47^m 18.92^s

+32° 41′ 08.6″

7.9

-0.52

1375

M5e-M10e(S6,2e)

Mira variable, V_max = 7.9^m, V_min = 15.7^m, P = 430 d

Groombridge 34

1326

1475

00^h 18^m 22.9^s

+44° 01′ 22″

8.01

10.25

11.62

M6Ve + M1Ve

16th closest star system, binary; both components GQ and GX And flare stars

HD 15082

15082

11397

02^h 26^m 51.06^s

+37° 33′ 01.7″

8.3

3.0

377

A5

has a transiting planet WASP-33b

RU And

RU

01^h 38^m 37^s

38° 40′ 12″

9.9

M5e-M6e

a variable star in the constellation of Andromeda. It is classified as a semiregular variable pulsating giant star, and varies from an apparent visual magnitude of 14.5 at minimum brightness to a magnitude of 9.9 at maximum brightness, with a period of approximately 238.3 days.^[17]^[18]

Y And

10112

01^h 39^m 36.89^s

+39° 20′ 35″

10.39

8,000

M3-4.5e

Mira Cet variable

Z And

Z

221650

116287

23^h 33^m 39.95^s

+48° 49′ 05.9″

10.53

2.38

1393

M2III + B1eq

prototype of Z And variables, V_max = 7.7^m, V_min = 11.3^m

HAT-P-6

23^h 39^m 05.81^s

+42° 27′ 57.5″

10.54

4.03

650

F

Sterrennacht; has a transiting planet (b)

HAT-P-16

00^h 38^m 17.56^s

+42° 27′ 47.2″

10.8

3.9

766

F8

has a transiting planet (b)

HAT-P-32

02^h 01^m 10^s

+46° 41′ 16″

11.29

3.76

1044

F/G

has a transiting planet (b)

WASP-1

00^h 20^m 40.08^s

+31° 59′ 23.8″

11.79

3.89

1239

F7V

has a transiting planet (b)

Ross 248

23^h 41^m 54.99^s

+44° 10′ 40.8″

12.29

14.79

10.32

M6e

HH And; 8th closest star system, flare star

HAT-P-19

00^h 38^m 04^s

+34° 42′ 42″

12.9

6.24

701

K

has a transiting planet (b)

HAT-P-28

00^h 52^m 00^s

+34° 43′ 42″

13.03

5.05

1288

G3

has a transiting planet (b)

HAT-P-53

01^h 27^m 29.0^s

+38° 58′ 05″

13.73

4.45

2345

has a transiting planet (b)

S And

S

00^h 42^m 43.11^s

+41° 16′ 04.2″

2600000

Ia

SN 1885A; BD+40°147a; type Ia supernova in the Andromeda Galaxy, V_max = 5.8^m, V_min = < 16^m

Table legend:

• Name = Proper name
• B = Bayer designation
• F or/and G. = Flamsteed designation or Gould designation
• Var = Variable star designation
• HD = Henry Draper Catalogue designation number
• HIP = Hipparcos Catalogue designation number
• RA = Right ascension for the Epoch/Equinox J2000.0
• Dec = Declination for the Epoch/Equinox J2000.0

• vis. mag. = visual magnitude (m or m_v), also known as apparent magnitude
• abs. mag. = absolute magnitude (M_v)
• Dist. (ly) = Distance in light-years from Earth
• Sp. class = Spectral class of the star in the stellar classification system
• Notes = Common name(s) or alternate name(s); comments; notable properties [for example: multiple star status, range of variability if it is a variable star, exoplanets, etc.]

Notes

↑ It was commonly with δ Peg by Bayer.
↑ Flamsteed lettered it as n.
↑ Armando Gil de Paz et al., "The GALEX Ultraviolet Atlas of Nearby Galaxies," The Astrophysical Journal Supplement Series (ApJS), American Astronomical Society, 2007, 173 185–255.
↑ Bayer designated it as υ Per.
↑ Bode lettered it as 2.υ, in his "Verzeichniss".
↑ Flamsteed lettered it as υ.
↑ Bode lettered it as 1.υ in his "Verzeichniss".
1 2 Final Results of NameExoWorlds Public Vote Released
↑ E.B Knobel – On a catalogue of stars in the Calendarium of Al Achsasi Al Mouakket
1 2 Flamsteed unlettered it in his catalogue and atlas.
↑ Bayer originally lettered it as υ.
↑ Flamsteed lettered it as λ.
↑ Flamsteed lettered it as d.
↑ Flamsteed lettered it as ξ.
↑ Flamsteed lettered it as h Per.
↑ Persei, on the constellation boundary between Andromeda with Perseus
↑ RU And, database entry, Combined General Catalog of Variable Stars (GCVS4.2, 2004 Ed.), N. N. Samus, O. V. Durlevich, et al., CDS ID II/250 Accessed on line 2009-06-30.
↑ V* RU And -- Semiregular Pulsating Variable Star, database entry, SIMBAD. Accessed on line 2009-06-30.

References

Bayer J. (1603). Uranometria. Augsburg: Christophorus Mangus.
Bevis J. (c. 1750). Uranographia Britannica.
Bode J. E. (1782). Vorstellung der Gestirne. Berlin / Stralsund: Gottlieb August Lange.
Fortin J. (1776). Atlas Celeste de Flamsteed (2^eme ed.). Paris.
ESA (1997). "The Hipparcos and Tycho Catalogues". Retrieved 26 December 2006.
Kostjuk, N. D. (2002). "HD-DM-GC-HR-HIP-Bayer-Flamsteed Cross Index". Retrieved 26 December 2006.
Roman, N. G. (1987). "Identification of a Constellation from a Position". Retrieved 26 December 2006.
"SIMBAD Astronomical Database". Centre de Données astronomiques de Strasbourg. Retrieved 4 January 2007.
Samus, N. N.; Durlevich, O. V.; et al. (2004). "Combined General Catalogue of Variable Stars (GCVS4.2)". Retrieved 28 March 2012.
Samus, N. N.; Durlevich, O. V.; et al. (2012). "General Catalog of Variable Stars (GCVS database, version 2012Feb)". Retrieved 28 March 2012.
Wagman, Morton (2003). Lost Stars: Lost, Missing and Troublesome Stars from the Catalogues of Johannes Bayer, Nicholas Louis de Lacaille, John Flamsteed, and Sundry Others. Blacksburg, Virginia: The McDonald & Woodward Publishing Company. pp. 23–24. Bibcode:2003lslm.book.....W. ISBN 978-0-939923-78-6.
Werner, Helmut; Schmeidler, Felix (1986). Synopsis der Nomenklatur der Fixsterne. Stuttgart: Wissenschaftliche Verlagsgesellschaft mbH. pp. 50–53. ISBN 978-3-8047-0739-9.

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[1] It was commonly with δ Peg by Bayer.

[2] Flamsteed lettered it as n.

[3] Armando Gil de Paz et al., "The GALEX Ultraviolet Atlas of Nearby Galaxies," The Astrophysical Journal Supplement Series (ApJS), American Astronomical Society, 2007, 173 185–255.

[4] Bayer designated it as υ Per.

[5] Bode lettered it as 2.υ, in his "Verzeichniss".

[6] Flamsteed lettered it as υ.

[7] Bode lettered it as 1.υ in his "Verzeichniss".

[NameExoWorlds-8] 1 2 Final Results of NameExoWorlds Public Vote Released

[9] E.B Knobel – On a catalogue of stars in the Calendarium of Al Achsasi Al Mouakket

[flamerror-10] 1 2 Flamsteed unlettered it in his catalogue and atlas.

[11] Bayer originally lettered it as υ.

[12] Flamsteed lettered it as λ.

[13] Flamsteed lettered it as d.

[14] Flamsteed lettered it as ξ.

[15] Flamsteed lettered it as h Per.

[16] Persei, on the constellation boundary between Andromeda with Perseus

[gcvs-17] RU And, database entry, Combined General Catalog of Variable Stars (GCVS4.2, 2004 Ed.), N. N. Samus, O. V. Durlevich, et al., CDS ID II/250 Accessed on line 2009-06-30.

[18] V* RU And -- Semiregular Pulsating Variable Star, database entry, SIMBAD. Accessed on line 2009-06-30.

[1]

[2]

[3]

[4]

[5]

[6]

[7]

[8]

[9]

[10]

[11]

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[13]

[14]

[15]

[16]

[17]

[18]

See also

References