List of stars in Aries

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

Notes

α Ari

α

13

12929

9884

02^h 07^m 10.29^s

+23° 27′ 46.0″

2.01

0.48

66

K2III

Hamal, Hemal, Hamul, Ras Hammel, El Nath; suspected variable, V_max = 1.98^m, V_min = 2.04^m; has a planet (b)

β Ari

β

6

11636

8903

01^h 54^m 38.35^s

+20° 48′ 29.9″

2.64

1.33

60

A5V...

Sheratan, Sharatan, Al Sharatain; suspected variable, V_max = 2.56^m, V_min = 2.70^m

41 Ari

c

41

17573

13209

02^h 49^m 58.99^s

+27° 15′ 38.8″

3.61

0.16

159

B8Vn

Bharani; suspected variable, V_max = 3.60^m, V_min = 3.64^m

δ Ari

δ

57

19787

14838

03^h 11^m 37.67^s

+19° 43′ 36.1″

4.35

0.79

168

K2IIIvar

Botein, Nir al Botain, Lucida Ventris,[1] part of Al Buṭain;[2][3] suspected variable, V_max = 4.33^m, V_min = 4.37^m

HD 20644

20644

15549

03^h 20^m 20.37^s

+29° 02′ 54.6″

4.47

−2.00

640

K2II-III

39 Ari

39

17361

13061

02^h 47^m 54.44^s

+29° 14′ 50.7″

4.52

0.80

181

K1III

Lilii Borea

γ² Ari

γ²

5

11503

01^h 53^m 31.80^s

+19° 17′ 45.0″

4.62

1.11

164.0

kA0hA3(IV)SiSr

Mesarthim, Mesartim; binary star; α² CVn variable, ΔV = 0.04^m, P = 1.6092 d

35 Ari

35

16908

12719

02^h 43^m 27.11^s

+27° 42′ 25.8″

4.65

−0.62

370

B3V

γ¹ Ari

γ¹

5

11502

8832

01^h 53^m 31.77^s

+19° 17′ 38.7″

4.70

1.19

164.0

B9.5IV

component of the γ Ari system

λ Ari

λ

9

11973

9153

01^h 57^m 55.78^s

+23° 35′ 45.9″

4.79

1.73

133

F0V

binary star

ζ Ari

ζ

58

20150

15110

03^h 14^m 54.11^s

+21° 02′ 40.7″

4.87

−0.22

340

A1V

part of Al Buṭain[2][3]

14 Ari

14

13174

10053

02^h 09^m 25.29^s

+25° 56′ 23.9″

4.98

0.02

320

F2III

κ Ari

κ

12

12869

9836

02^h 06^m 33.91^s

+22° 38′ 54.3″

5.03

1.23

187

A2m

spectroscopic binary

ι Ari

ι

8

11909

9110

01^h 57^m 21.03^s

+17° 49′ 03.3″

5.09

−1.44

659

K1p...

spectroscopic binary

τ² Ari

τ²

63

20893

15737

03^h 22^m 45.27^s

+20° 44′ 31.6″

5.10

0.15

319

K3III

38 Ari

38

UV

17093

12832

02^h 44^m 57.51^s

+12° 26′ 45.5″

5.18

2.26

125

A7III-IV

δ Sct variable, V_max = 5.18^m, V_min = 5.22^m, P = 0.0355 d

ε Ari A

ε

48

18519

02^h 59^m 12.70^s

+21° 20′ 25.0″

5.2

0.16

332

A2Vs

part of Al Buṭain;[2][3] binary star

η Ari

η

17

13555

10306

02^h 12^m 47.98^s

+21° 12′ 39.5″

5.23

2.84

98

F5V

π Ari

π

42

17543

13165

02^h 49^m 17.56^s

+17° 27′ 51.6″

5.26

−1.07

603

B6V

part of Al Buṭain;[2][3] spectroscopic binary

τ¹ Ari

τ¹

61

20756

15627

03^h 21^m 13.61^s

+21° 08′ 49.7″

5.27

−0.49

462

B5IV

triple star system; Beta Lyrae variable

33 Ari

33

16628

12489

02^h 40^m 41.03^s

+27° 03′ 39.6″

5.30

1.03

233

A3V

ν Ari

ν

32

16432

12332

02^h 38^m 49.00^s

+21° 57′ 41.2″

5.45

0.32

346

A7V

52 Ari A

52

19134

14376

03^h 05^m 26.69^s

+25° 15′ 18.7″

5.45

0.00

402

B7Vn

binary star

ξ Ari

ξ

24

14951

11249

02^h 24^m 49.04^s

+10° 36′ 38.2″

5.48

−0.85

603

B7IV

variable star, ΔV = 0.007^m, P = 1.73515 d

ε Ari B

ε

48

18519

13914

02^h 59^m 12.73^s

+21° 20′ 25.6″

5.5

0.46

332

A2Vs

component of the ε Ari system

64 Ari

64

21017

15861

03^h 24^m 18.46^s

+24° 43′ 27.1″

5.50

1.26

230

K4III

σ Ari

σ

43

17769

13327

02^h 51^m 29.57^s

+15° 04′ 55.7″

5.52

−0.32

479

B7V

62 Ari

62

20825

15696

03^h 22^m 11.89^s

+27° 36′ 27.3″

5.55

−1.82

973

G5III

21 Ari

21

13872

10535

02^h 15^m 42.83^s

+25° 02′ 35.7″

5.57

2.16

157

F6V

θ Ari

θ

22

14191

10732

02^h 18^m 07.55^s

+19° 54′ 04.2″

5.58

0.21

387

A1Vn

ρ³ Ari

ρ³

46

18256

13702

02^h 56^m 25.98^s

+18° 01′ 25.1″

5.58

2.83

115

F6V

part of Al Buṭain;[2][3] suspected BY Dra variable

HD 20149

20149

15154

03^h 15^m 20.45^s

+30° 33′ 24.0″

5.61

−0.01

434

A1Vs

10 Ari

10

12558

9621

02^h 03^m 39.26^s

+25° 56′ 07.6″

5.64

2.02

172

F8IV

31 Ari

31

16234

12153

02^h 36^m 37.75^s

+12° 26′ 52.2″

5.64

2.91

115

F7V

HD 19270

19270

14439

03^h 06^m 23.69^s

+13° 11′ 14.6″

5.64

0.69

319

K3III

15 Ari

15

AV

13325

10155

02^h 10^m 37.54^s

+19° 30′ 01.5″

5.68

−0.87

665

M3III

semiregular variable, V_max = 5.67^m, V_min = 5.74^m, P = 5.0320 d

19 Ari

19

13596

10328

02^h 13^m 03.25^s

+15° 16′ 47.7″

5.72

−0.38

541

M0III

suspected variable, V_max = 5.68^m, V_min = 5.76^m

μ Ari

μ

34

16811

12640

02^h 42^m 21.92^s

+20° 00′ 41.7″

5.74

0.66

338

A0V

55 Ari

55

19548

14677

03^h 09^m 36.73^s

+29° 04′ 37.6″

5.74

−1.96

1128

B8III

7 Ari

7

RR

11763

8993

01^h 55^m 51.03^s

+23° 34′ 38.4″

5.76

−0.26

522

K1III

not variable

ρ² Ari

ρ²

45

RZ

18191

13654

02^h 55^m 48.50^s

+18° 19′ 54.0″

5.76

0.30

403

M6IIIvar

semiregular variable, V_max = 5.45^m, V_min = 6.01^m

ο Ari

ο

37

17036

12803

02^h 44^m 32.97^s

+15° 18′ 42.8″

5.78

−0.07

482

B9Vn

56 Ari

56

SX

19832

14893

03^h 12^m 14.24^s

+27° 15′ 25.2″

5.78

0.50

371

B9p Si

prototype SX Ari variable, V_max = 5.75^m, V_min = 5.81^m, P = 0.727902 d

20 Ari

20

13871

10540

02^h 15^m 45.94^s

+25° 46′ 59.2″

5.79

2.77

131

F6IV-V

47 Ari

47

18404

13834

02^h 58^m 05.08^s

+20° 40′ 07.7″

5.80

3.29

104

F5IV

suspected variable

1 Ari A

1

11154

8544

01^h 50^m 08.58^s

+22° 16′ 31.3″

5.83

−0.40

574

K1III+...

binary star

40 Ari

40

17459

13108

02^h 48^m 32.06^s

+18° 17′ 01.9″

5.83

−0.11

502

K1III

4 Ari

4

10982

8387

01^h 48^m 10.90^s

+16° 57′ 20.3″

5.86

1.14

287

B9.5V

HD 15524

15524

11670

02^h 30^m 32.31^s

+25° 14′ 06.8″

5.88

2.34

166

F6IV

HD 12139

12139

9307

01^h 59^m 35.60^s

+21° 03′ 31.0″

5.89

0.45

399

K0III-IV

HR 830

(16)

VZ

17471

13121

02^h 48^m 45.87^s

+25° 11′ 17.1″

5.89

0.14

460

A0V

16 Trianguli; Alpha² CVn variable, V_max = 5.82^m, V_min = 5.89^m

1 Ari B

1

11155

01^h 50^m 08.50^s

+22° 16′ 33.0″

5.90

component of the 1 Ari system

49 Ari

49

18769

14109

03^h 01^m 54.15^s

+26° 27′ 44.4″

5.91

1.82

214

A3m

suspected variable, V_max = 5.90^m, V_min = 5.94^m

59 Ari

59

20618

15514

03^h 19^m 55.81^s

+27° 04′ 16.7″

5.91

1.91

205

G8IV

54 Cet

(54)

11257

8588

01^h 50^m 52.01^s

+11° 02′ 36.4″

5.93

2.77

139

F2Vw

suspected variable, V_max = 5.93^m, V_min = 5.97^m

HD 18700

18700

14036

03^h 00^m 44.09^s

+10° 52′ 13.7″

5.93

0.27

441

K6

HD 13522

13522

10296

02^h 12^m 37.51^s

+24° 10′ 04.1″

5.96

−0.23

565

K0

HD 12479

12479

9533

02^h 02^m 35.08^s

+13° 28′ 36.2″

5.97

−1.10

845

M2III

suspected variable

HD 19698

19698

14764

03^h 10^m 38.78^s

+11° 52′ 21.7″

5.97

−0.05

522

B8V

29 Ari

29

15814

11843

02^h 32^m 54.15^s

+15° 02′ 04.1″

6.00

3.71

94

F8V

11 Ari

11

12885

9859

02^h 06^m 49.22^s

+25° 42′ 16.5″

6.01

−1.75

1160

B9IV-Vn

16 Ari

16

13363

10203

02^h 11^m 12.06^s

+25° 56′ 13.0″

6.01

−0.94

801

K4III

HD 19637

19637

14748

03^h 10^m 27.04^s

+26° 53′ 45.9″

6.02

0.54

406

K3III

66 Ari

66

21467

16181

03^h 28^m 26.57^s

+22° 48′ 15.4″

6.03

1.83

226

K0IV

65 Ari

65

21050

15870

03^h 24^m 26.11^s

+20° 48′ 12.6″

6.07

1.23

303

A1V

HD 12140

12140

9295

01^h 59^m 25.88^s

+12° 17′ 41.8″

6.09

1.51

269

A6V

HD 19789

19789

14821

03^h 11^m 21.93^s

+13° 02′ 52.1″

6.11

0.99

344

K0IIIp

53 Ari

53

UW

19374

14514

03^h 07^m 25.69^s

+17° 52′ 47.9″

6.13

−0.69

755

B1.5V

not variable; runaway star

HD 15152

15152

11415

02^h 27^m 07.26^s

+27° 00′ 45.3″

6.14

0.37

464

K5III

suspected variable

26 Ari

26

UU

15550

11678

02^h 30^m 38.37^s

+19° 51′ 19.4″

6.14

1.94

226

A9V

δ Sct variable, V_max = 6.10^m, V_min = 6.15^m, P = 0.0676 d

60 Ari

60

20663

15557

03^h 20^m 25.57^s

+25° 39′ 46.7″

6.14

1.40

289

K3III:

HD 15385

15385

11578

02^h 29^m 13.63^s

+23° 28′ 08.7″

6.20

1.65

264

A5m

27 Ari

27

15596

11698

02^h 30^m 54.38^s

+17° 42′ 14.6″

6.21

1.30

313

G5III-IV

HD 12594

12594

9627

02^h 03^m 42.61^s

+18° 15′ 11.8″

6.24

−1.83

1342

K4III

54 Ari

54

19460

14586

03^h 08^m 21.09^s

+18° 47′ 42.3″

6.25

0.03

570

M0III

semiregular variable, V_max = 6.25^m, V_min = 6.28^m

HD 17918

17918

13448

02^h 53^m 11.66^s

+16° 29′ 01.0″

6.30

1.14

352

F5III

85 Cet

(85)

16861

12647

02^h 42^m 28.95^s

+10° 44′ 30.4″

6.32

0.74

426

A2V

suspected variable, V_max = 6.28^m, V_min = 6.34^m

HD 16955

16955

12744

02^h 43^m 51.25^s

+25° 38′ 18.0″

6.35

1.19

352

A3V

HD 19080

19080

14318

03^h 04^m 40.65^s

+15° 51′ 22.5″

6.37

−0.06

631

K3III

HD 18928

18928

14232

03^h 03^m 30.11^s

+28° 16′ 11.8″

6.38

2.89

163

F0V

HD 13201

13201

10050

02^h 09^m 23.03^s

+17° 13′ 28.7″

6.40

3.43

128

F5V

HD 20367

20367

15323

03^h 17^m 40.12^s

+31° 07′ 37.9″

6.40

4.23

88

G0V

has a planet (b)

HD 19549

19549

14649

03^h 09^m 20.10^s

+20° 45′ 40.1″

6.41

0.45

506

K2

HD 19600

19600

14719

03^h 10^m 08.83^s

+27° 49′ 11.6″

6.42

0.09

601

A0V

HD 14262

14262

10795

02^h 18^m 57.96^s

+23° 10′ 04.2″

6.45

1.34

343

A7V

36 Ari

36

17017

12784

02^h 44^m 19.09^s

+17° 45′ 50.5″

6.46

0.89

413

K2III

suspected variable, ΔV = 0.07^m

UX Ari

UX

21242

16042

03^h 26^m 35.36^s

+28° 42′ 55.2″

6.47

2.97

164

G5IV

RS CVn variable, V_max = 6.35^m, V_min = 6.71^m, P = 6.388 d

30 Ari A

30

16246

12189

02^h 37^m 00.44^s

+24° 38′ 50.1″

6.48

3.46

131

F6III

binary star

HD 14067

14067

10657

02^h 17^m 10.4^s

+23° 46′ 04″

6.51

0.44

533

G9 III

has a planet (b)

51 Ari

51

18803

14150

03^h 02^m 25.87^s

+26° 36′ 34.7″

6.62

4.99

69

G8V

VW Ari

VW

15165

11390

02^h 26^m 45.65^s

+10° 33′ 55.1″

6.69

1.16

416

F0IV

δ Sct variable, V_max = 6.64^m, V_min = 6.76^m, P = 0.1606 d

AF Ari

AF

14595

11035

02^h 22^m 06.62^s

+22° 52′ 24.9″

6.71

0.50

615

G3III

Algol type variable, V_max = 6.30^m, V_min = 7.10^m, P = 153 d

VY Ari

VY

17433

13118

02^h 48^m 43.72^s

+31° 06′ 54.7″

6.76

3.65

136.5

K0

RS CVn variable, V_max = 6.68^m, V_min = 7.15^m, P = 16.1996 d

50 Ari

50

18654

14021

03^h 00^m 31.50536^s

+18° 00′ 17.9143″

6.80

A0V

[4][5]

23 Ari

23

14305

10810

02^h 19^m 08.72041^s

+19° 41′ 15.7463″

6.83

F8V

52 Ari B

52

19135

03^h 05^m 26.70^s

+25° 15′ 19.0″

7.00

component of the 52 Ari system

ρ¹ Ari

ρ¹

44

18091

13579

02^h 54^m 55.17^s

+17° 44′ 05.3″

7.01

2.10

313

A3

30 Ari B

30

16232

12184

02^h 36^m 57.64^s

+24° 38′ 53.1″

7.09

4.11

129

F6V

component of the 30 Ari system; has a planet (b)

R Ari

R

13913

10576

02^h 16^m 07.11^s

+25° 03′ 23.7″

7.40

-2.99

3900

M3-6e

Mira variable, V_max = 7.1^m, V_min = 14.3^m, P = 185.67 d

HD 12661

12661

9683

02^h 04^m 34.29^s

+25° 24′ 51.5″

7.44

4.59

121

K0V

has two planets (b & c)

HD 17674

17674

13291

02^h 51^m 04.3^s

+30° 17′ 12″

7.56

145

G0V

has two planets (b)

HD 14787

14787

11130

02^h 50^m 53.0^s

+29° 01′ 21″

7.63

390

G5

has a planet (b)

HIP 14810

14810

03^h 11^m 14.23^s

+21° 05′ 50.5″

8.52

4.90

172

G5V

has three planets (b, c & d)

BD +20°307

8920

01^h 54^m 50.79^s

+21° 18′ 22.5″

9.01

4.19

300

G0V

has a circumstellar disk

X Ari

X

19510

14601

03^h 08^m 30.89^s

+10° 26′ 45.2″

9.04

-1.23

3700

F0.5

RR Lyr variable, V_max = 9.036^m, V_min = 9.966^m, P = 0.6511796 d

RX Ari

RX

02^h 15^m 20.78^s

+22° 34′ 11.1″

9.41

F2V

Algol variable, V_max = 9.40^m, V_min = 10.1^m, P = 1.029626 d

HAT-P-47

02^h 33^m 14.0^s

+30° 21′ 38″

10.6

874

has a transiting planet (b)

SS Ari

SS

02^h 04^m 18.41^s

+24° 00′ 02.2″

10.15

3.52

692

G0

W UMa variable, V_max = 10.10^m, V_min = 10.63^m, P = 0.40598257 d

TT Ari

TT

02^h 06^m 53.08^s

+15° 17′ 41.8″

10.2

Bep:

VY Scl star, V_max = 10.2^m, V_min = 16.5^m, P = 0.137551 d

RV Ari

RV

02^h 15^m 07.50^s

+18° 04′ 27.9″

11.61

A0

double-mode δ Sct variable, V_max = 11.61^m, V_min = 12.30^m, P = 0.0931281 d

WASP-11/HAT-P-10

03^h 09^m 28.55^s

+30° 40′ 24.9″

11.89

6.41

408

K3V

has a transiting planet (b)

HAT-P-48

02^h 57^m 53.0^s

+30° 37′ 33″

12.16

995

has a transiting planet (b)

L 1159-16

TZ

02^h 00^m 12.79^s

+13° 03′ 11.2″

12.26

13.99

14.5

M4.5

flare star and BY Dra variable

LkHα 264

WY

02^h 56^m 37.56^s

+20° 05′ 37.1″

12.46

K5/6e

T Tau star, V_max = 12.25^m, V_min = 12.88^m

RW Ari

RW

02^h 16^m 03.72^s

+17° 31′ 59.0″

12.51

B8

RR Lyr variable, V_max = 12.12^m, V_min = 12.60^m, P = 0.3543006 d

HAT-P-25

03^h 13^m 45^s

+25° 11′ 51″

13.19

5.83

969

G5

has a transiting planet (b)

HAT-P-52

02^h 50^m 53.0^s

+29° 01′ 21″

14.07

6.14

1256

has a transiting planet (b)

WX Ari

WX

02^h 47^m 36.22^s

+10° 35′ 37.7″

15.3

CV

VY Scl star and eclipsing binary, V_max = 14.5^m, V_min = <16.7^m, P = 0.1393512 d

Teegarden's star

02^h 53^m 00.89^s

+16° 52′ 52.7″

15.40

17.47

12.6

M7.5

brown dwarf

XY Ari

XY

02^h 56^m 08.19^s

+19° 26′ 34.1″

WD+M0V

DQ Her variable and eclipsing binary

PSR B0301+19

03^h 04^m 33.12^s

+19° 32′ 51.4″

pulsar

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.]

References

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.
Samus, N. N.; Durlevich, O. V.; et al. (2004). "Combined General Catalogue of Variable Stars (GCVS4.2)". Retrieved 3 April 2012.
Samus, N. N.; Durlevich, O. V.; et al. (2012). "General Catalog of Variable Stars (GCVS database, version 2012Feb)". Retrieved 3 April 2012.
"AAVSO Website". American Association of Variable Star Observers. Retrieved 9 March 2014.
"Naming Stars". Retrieved 13 December 2017.

Knobel, E. B. (1895). "1895MNRAS..55..429K Page 432". Monthly Notices of the Royal Astronomical Society. 55: 429. Bibcode:1895MNRAS..55..429K. doi:10.1093/mnras/55.8.429.
Consisting with δ Ari (Botein), ε Ari, ζ Ari, π Ari, and ρ³ Ari, were Al Buṭain, the dual of Al Baṭn, the Belly. See Star Name – R.H.Allen p. 83
δ Ari as Nir al Botain or Lucida Ventris (the brightest of the belly). ε Ari, ζ Ari, π Ari, and ρ³ Ari was not designated by Al Achsasi Al Mouakket. Jack W. Rhoads was designated these stars of Al Buṭain were Al Buṭain I (π Ari), Al Buṭain II (ρ³ Ari), Al Buṭain III (ε Ari) and Al Buṭain IV (ζ Ari)
SIMBAD, 50 Arietis (Retrieved 27 July 2012)
Abt, Helmut A. (2008). "Visual Multiples. IX. MK Spectral Types". The Astrophysical Journal Supplement Series. 176 (1): 216–217. Bibcode:2008ApJS..176..216A. doi:10.1086/525529.

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[sb0-1] Knobel, E. B. (1895). "1895MNRAS..55..429K Page 432". Monthly Notices of the Royal Astronomical Society. 55: 429. Bibcode:1895MNRAS..55..429K. doi:10.1093/mnras/55.8.429.

[sb2-2] Consisting with δ Ari (Botein), ε Ari, ζ Ari, π Ari, and ρ³ Ari, were Al Buṭain, the dual of Al Baṭn, the Belly. See Star Name – R.H.Allen p. 83

[sb3-3] δ Ari as Nir al Botain or Lucida Ventris (the brightest of the belly). ε Ari, ζ Ari, π Ari, and ρ³ Ari was not designated by Al Achsasi Al Mouakket. Jack W. Rhoads was designated these stars of Al Buṭain were Al Buṭain I (π Ari), Al Buṭain II (ρ³ Ari), Al Buṭain III (ε Ari) and Al Buṭain IV (ζ Ari)

[SIMBAD-4] SIMBAD, 50 Arietis (Retrieved 27 July 2012)

[abt-5] Abt, Helmut A. (2008). "Visual Multiples. IX. MK Spectral Types". The Astrophysical Journal Supplement Series. 176 (1): 216–217. Bibcode:2008ApJS..176..216A. doi:10.1086/525529.

List of stars in Aries

See also

References