List of stars in Cancer

This is the list of notable stars in the constellation Cancer. The 121 stars are sorted by decreasing brightness, beginning with Beta Cancri, the brightest star in Cancer.

Notes

β Cnc

β

17

69267

40526

08^h 16^m 30.95^s

+09° 11′ 08.4″

3.53

−1.22

290

K4III

Tarf, Al Tarf; variable star, ΔV = 0.005^m, P = 6.01 d, has a planet (b)

δ Cnc

δ

47

74442

42911

08^h 44^m 41.11^s

+18° 09′ 17.5″

3.94

0.84

136

K0III

Asellus Australis

ι Cnc A

ι

48

74739

43103

08^h 46^m 41.83^s

+28° 45′ 36.0″

4.03

−0.77

298

G8Iab:

component of the ι Cnc system

α Cnc

α

65

76756

44066

08^h 58^m 29.20^s

+11° 51′ 28.0″

4.26

0.63

173

A5m

Acubens, Sertan; suspected variable, V_max = 4.20^m, V_min = 4.27^m

γ Cnc

γ

43

74198

42806

08^h 43^m 17.21^s

+21° 28′ 06.9″

4.66

1.23

181

A1IV

Asellus Borealis

ζ Cnc

ζ

16

68255
68256
68257

40167

08^h 12^m 12.71^s

+17° 38′ 53.3″

4.67

2.63

83

F7V+F9V
+G0V+?

Tegmine, quaternary star

HD 71115

71115

41325

08^h 25^m 54.79^s

+07° 33′ 52.3″

5.13

−0.08

359

G8II

double star

8 Cnc

8

66664

39567

08^h 05^m 04.51^s

+13° 07′ 06.1″

5.14

1.09

210

A1V

χ Cnc

χ

18

69897

40843

08^h 20^m 03.87^s

+27° 13′ 07.0″

5.14

3.84

59

F6V

suspected variable

ξ Cnc

ξ

77

78515

44946

09^h 09^m 21.53^s

+22° 02′ 43.6″

5.16

−0.18

380

K0III

Nahn

ο¹ Cnc

ο¹

62

76543

43970

08^h 57^m 14.91^s

+15° 19′ 21.8″

5.22

1.77

160

A5III

α² CVn variable

ρ² Cnc

ρ²

58

76219

43834

08^h 55^m 39.69^s

+27° 55′ 39.2″

5.23

−1.00

574

G8II-III

σ³ Cnc

σ³

64

76813

44154

08^h 59^m 32.68^s

+32° 25′ 07.1″

5.23

0.27

320

G9III

suspected variable

κ Cnc

κ

76

78316

44798

09^h 07^m 44.82^s

+10° 40′ 05.6″

5.23

−0.63

484

B8IIImnp

α² CVn variable, V_max = 5.22^m, V_min = 5.27^m, P = 5.0035 d

μ² Cnc

μ²

10

67228

39780

08^h 07^m 45.84^s

+21° 34′ 55.1″

5.30

3.46

76

G2IV

θ Cnc

θ

31

72094

41822

08^h 31^m 35.77^s

+18° 05′ 40.4″

5.33

−0.57

494

K5III

suspected variable

η Cnc

η

33

72292

41909

08^h 32^m 42.52^s

+20° 26′ 28.6″

5.33

0.43

312

K3III

82 Cnc

π²

82

79554

45410

09^h 15^m 13.88^s

+14° 56′ 29.5″

5.36

−1.30

701

K1III

57 Cnc

57

75959

43721

08^h 54^m 14.70^s

+30° 34′ 45.0″

5.40

0.15

365

G7III

τ Cnc

τ

72

78235

44818

09^h 08^m 00.07^s

+29° 39′ 15.2″

5.42

0.91

260

G8III

60 Cnc

60

76351

43851

08^h 55^m 55.56^s

+11° 37′ 33.8″

5.44

−0.82

582

K5III

σ² Cnc

σ²

59

76398

43932

08^h 56^m 56.63^s

+32° 54′ 38.1″

5.44

1.56

195

A7IV

ν Cnc

ν

69

77350

44405

09^h 02^m 44.27^s

+24° 27′ 10.6″

5.45

−0.28

457

A0pSi

α² CVn variable, V_max = 5.33^m, V_min = 5.49^m, P = 4.20 d

27 Cnc

27

BP

71250

41400

08^h 26^m 43.95^s

+12° 39′ 17.5″

5.56

−1.98

1052

M3III

semiregular variable, V_max = 5.41^m, V_min = 5.75^m, P = 40 d

φ¹ Cnc

φ¹

22

71093

41377

08^h 26^m 27.73^s

+27° 53′ 37.9″

5.58

0.15

398

K5III

3 Cnc

3

65759

39177

08^h 00^m 47.31^s

+17° 18′ 31.4″

5.60

−1.12

721

K3III

15 Cnc

15

BM

68351

40240

08^h 13^m 08.87^s

+29° 39′ 23.7″

5.62

−1.52

872

B9p SiCr

α² CVn variable, V_max = 5.53^m, V_min = 5.65^m, P = 3.31 d

45 Cnc

A¹

45

74228

42795

08^h 43^m 12.34^s

+12° 40′ 51.1″

5.62

−1.87

1028

A3V+...

suspected variable

49 Cnc

b

49

BI

74521

42917

08^h 44^m 45.04^s

+10° 04′ 54.2″

5.63

0.15

408

A1p...

α² CVn variable, V_max = 5.58^m, V_min = 5.71^m, P = 6.91 d

σ¹ Cnc

σ¹

51

75698

43584

08^h 52^m 34.62^s

+32° 28′ 26.8″

5.67

1.69

204

A8Vms

suspected variable

ο² Cnc

ο²

63

76582

44001

08^h 57^m 35.16^s

+15° 34′ 52.4″

5.68

2.22

161

F0IV

υ¹ Cnc

υ¹

30

72041

41816

08^h 31^m 30.57^s

+24° 04′ 52.4″

5.71

1.40

237

F0IIIn

suspected variable

ψ² Cnc

ψ²

14

67767

40023

08^h 10^m 27.23^s

+25° 30′ 29.4″

5.73

2.61

137

G8IV

suspected variable

1 Cnc

1

64960

38848

07^h 56^m 59.47^s

+15° 47′ 25.4″

5.80

0.04

462

K3III

HD 69994

69994

40866

08^h 20^m 20.93^s

+20° 44′ 52.2″

5.80

−0.17

510

K1III

HD 77445

77445

44406

09^h 02^m 44.82^s

+07° 17′ 53.7″

5.85

−0.69

664

K3III:

suspected variable

ω¹ Cnc

ω¹

2

65714

39191

08^h 00^m 55.87^s

+25° 23′ 34.2″

5.87

−1.82

660

G8III:

50 Cnc

A²

50

74873

43121

08^h 46^m 56.06^s

+12° 06′ 36.3″

5.89

1.96

199

A1V

66 Cnc

66

77104

44307

09^h 01^m 24.13^s

+32° 15′ 08.3″

5.89

−0.08

509

A2V

HD 72945

72945

42172

08^h 35^m 51.05^s

+06° 37′ 13.9″

5.91

3.79

87

F8V

Binary star with a co-moving companion

λ Cnc

λ

19

70011

40881

08^h 20^m 32.15^s

+24° 01′ 20.5″

5.92

0.37

419

B9.5V

Piautos

36 Cnc

c

36

73143

42265

08^h 37^m 05.79^s

+09° 39′ 20.1″

5.92

0.17

461

A3V

suspected eclipsing binary

20 Cnc

d¹

20

70569

41117

08^h 23^m 21.87^s

+18° 19′ 56.2″

5.94

0.52

395

A9V

29 Cnc

29

71555

41578

08^h 28^m 37.35^s

+14° 12′ 39.1″

5.94

1.07

308

A5V

75 Cnc

75

78418

44892

09^h 08^m 47.42^s

+26° 37′ 48.0″

5.95

3.47

102

G5IV

1 LMi

(1)

73192

42365

08^h 38^m 19.00^s

+32° 48′ 07.3″

5.96

0.70

367

K2III:

55 Cnc

ρ¹

55

75732

43587

08^h 52^m 36.13^s

+28° 19′ 53.0″

5.96

5.47

41

G8V

Copernicus,^[1] binary star; has five planets (b, c, d, e, f)

μ¹ Cnc

μ¹

9

BL

66875

39659

08^h 06^m 18.40^s

+22° 38′ 07.8″

5.97

−0.45

626

M3III

semiregular variable, V_max = 5.97^m, V_min = 6.04^m

5 Cnc

5

65873

39236

08^h 01^m 30.29^s

+16° 27′ 19.2″

5.99

0.19

472

B9.5Vn

HD 68461

68461

40231

08^h 12^m 59.74^s

+16° 30′ 51.7″

6.03

−0.02

528

G8III

HD 72617

72617

42049

08^h 34^m 13.35^s

+08° 27′ 08.5″

6.04

2.22

189

F3IV

79 Cnc

79

78715

45033

09^h 10^m 20.86^s

+21° 59′ 47.1″

6.04

0.49

420

G8III

RS Cnc

RS

78712

45058

09^h 10^m 38.81^s

+30° 57′ 47.6″

6.04

0.61

397

M6S

Technetium star; semiregular variable, V_max = 5.33^m, V_min = 6.94^m, P = 242.2 d

HD 65257

65257

38975

07^h 58^m 31.48^s

+16° 31′ 07.3″

6.05

−2.11

1399

K0

suspected variable

HD 65522

65522

39067

07^h 59^m 35.07^s

+13° 14′ 31.9″

6.05

1.22

301

K2

28 Cnc

28

CX

71496

41574

08^h 28^m 36.80^s

+24° 08′ 42.2″

6.05

1.45

271

F0Vn

δ Sct variable, ΔV = 0.025^m, P = 0.096 d

67 Cnc

67

77190

44342

09^h 01^m 48.88^s

+27° 54′ 10.0″

6.07

2.23

191

A8Vn

suspected variable

HD 68099

68099

40085

08^h 11^m 16.60^s

+09° 49′ 16.6″

6.08

−1.06

872

B6III

21 Cnc

21

70734

41163

08^h 23^m 55.21^s

+10° 37′ 55.6″

6.11

−1.56

1113

M2III

suspected variable

25 Cnc

d²

25

71030

41319

08^h 25^m 49.99^s

+17° 02′ 47.9″

6.11

2.85

147

F6V

46 Cnc

46

74485

42954

08^h 45^m 21.42^s

+30° 41′ 51.9″

6.12

0.30

477

G5III

φ² Cnc A

φ²

23

71150

41404

08^h 26^m 47.08^s

+26° 56′ 07.7″

6.14

1.50

276

A3V

component of the φ² Cnc system; suspected variable

HD 80546

80546

45896

09^h 21^m 27.17^s

+32° 54′ 07.9″

6.16

1.22

317

K3III

HD 76508

76508

43957

08^h 57^m 08.30^s

+17° 08′ 37.8″

6.17

0.82

384

K1III

φ² Cnc B

φ²

23

71151

08^h 26^m 47.00^s

+26° 56′ 07.0″

6.19

1.55

276

A6V

component of the φ² Cnc system

HD 76629

76629

44010

08^h 57^m 42.03^s

+09° 23′ 16.0″

6.19

−1.15

956

G8III

HD 66552

66552

39535

08^h 04^m 45.32^s

+18° 50′ 31.4″

6.21

1.40

299

B9V

HD 66684

66684

39607

08^h 05^m 37.05^s

+27° 31′ 47.1″

6.21

−1.08

934

A0V

suspected variable, V_max = 6.16^m, V_min = 6.21^m

4 LMi

(4)

73596

42538

08^h 40^m 18.31^s

+31° 56′ 31.1″

6.21

1.05

350

F5III

suspected variable

HD 67959

67959

40058

08^h 10^m 58.90^s

+14° 37′ 46.3″

6.22

−0.04

581

A1V

12 Cnc

12

67483

39874

08^h 08^m 42.44^s

+13° 38′ 27.4″

6.25

1.59

278

F3V

53 Cnc

53

BO

75716

43575

08^h 52^m 28.60^s

+28° 15′ 33.0″

6.25

−0.92

886

M3III

slow irregular variable, V_max = 5.9^m, V_min = 6.37^m

61 Cnc

61

76572

44031

08^h 57^m 58.63^s

+30° 14′ 01.5″

6.25

2.75

164

F6V

HD 72505

72505

42010

08^h 33^m 45.06^s

+13° 15′ 26.7″

6.26

1.40

306

K0III

HD 69478

69478

40617

08^h 17^m 31.66^s

+08° 51′ 58.8″

6.28

−1.28

1062

G8III

ε Cnc

ε

41

73731

42556

08^h 40^m 27.03^s

+19° 32′ 41.4″

6.29

0.16

548

Am

Meleph, in Beehive Cluster

HD 65735

65735

39180

08^h 00^m 48.10^s

+19° 48′ 58.4″

6.30

1.18

345

K1III

FZ Cnc

FZ

76830

44126

08^h 59^m 10.76^s

+18° 08′ 06.1″

6.30

−0.35

697

M4IIIvar

semiregular variable

4 Cnc

ω²

4

65856

39263

08^h 01^m 43.77^s

+25° 05′ 22.0″

6.32

0.00

598

A1V

HD 72943

72943

42187

08^h 36^m 07.71^s

+15° 18′ 49.3″

6.33

1.77

267

F0IV

HD 65757

65757

39194

08^h 01^m 00.79^s

+23° 34′ 59.4″

6.34

1.70

276

K1III-IV

υ² Cnc

υ²

32

72324

41940

08^h 33^m 00.14^s

+24° 05′ 05.7″

6.35

0.80

421

G9III

54 Cnc

54

75528

43454

08^h 51^m 01.53^s

+15° 21′ 01.7″

6.36

3.35

130

G2IV

HD 68776

68776

40354

08^h 14^m 21.01^s

+13° 02′ 54.0″

6.39

−0.49

776

G8III

39 Cnc

39

73665

42516

08^h 40^m 06.44^s

+20° 00′ 28.1″

6.39

0.11

587

K0III

in Beehive Cluster; suspected variable

HD 78175

78175

44768

09^h 07^m 27.01^s

+22° 58′ 51.1″

6.39

2.54

192

F5V

X Cnc

X

76221

43811

08^h 55^m 22.88^s

+17° 13′ 52.5″

6.40

−3.95

3622

C6,4

semiregular variable, V_max = 5.69^m, V_min = 6.94^m, P = 180 d

HD 80064

80064

45614

09^h 17^m 51.36^s

+11° 30′ 04.1″

6.40

0.30

542

A2IV

HD 75469

75469

43427

08^h 50^m 45.13^s

+18° 49′ 56.1″

6.41

−0.43

762

A2Vs

HD 69629

69629

40675

08^h 18^m 14.43^s

+15° 40′ 40.6″

6.42

0.56

485

K0

HD 73710

73710

42549

08^h 40^m 22.11^s

+19° 40′ 11.9″

6.42

−0.41

756

K0III

in Beehive Cluster

ψ¹ Cnc

ψ¹

13

67690

40007

08^h 10^m 13.12^s

+25° 50′ 40.4″

6.44

−1.06

1032

K0

HD 73599

73599

42462

08^h 39^m 24.57^s

+08° 01′ 03.6″

6.46

0.32

551

K1III

HD 77660

77660

44574

09^h 04^m 55.12^s

+32° 22′ 37.2″

6.46

1.96

259

A8V

HD 67542

67542

39958

08^h 09^m 35.19^s

+29° 05′ 35.1″

6.47

−3.93

3928

G0II

HD 68703

68703

40342

08^h 14^m 11.14^s

+17° 40′ 33.3″

6.47

1.45

329

A0Vne...

HD 78234

78234

44825

09^h 08^m 04.21^s

+32° 32′ 25.6″

6.47

1.32

349

F2V

34 Cnc

34

72359

41904

08^h 32^m 39.87^s

+10° 03′ 57.7″

6.48

0.38

541

A1V

suspected variable

HD 78661

78661

44984

09^h 09^m 46.45^s

+11° 33′ 52.3″

6.48

3.60

123

F2p

suspected variable

HD 79248

79248

45272

09^h 13^m 37.27^s

+21° 16′ 59.6″

6.48

0.57

496

A2V

HD 76908

76908

44148

08^h 59^m 26.89^s

+13° 04′ 27.9″

6.49

−1.50

1294

K5III

81 Cnc

π¹

81

79096

45170

09^h 12^m 17.87^s

+14° 59′ 43.6″

6.49

4.93

67

G9V

HD 72115

72115

41833

08^h 31^m 41.31^s

+18° 59′ 16.0″

6.50

−0.99

1025

K0

24 Cnc A

24

71152

41389

08^h 26^m 39.82^s

+24° 32′ 03.7″

6.51

2.11

248

F0III

component of the 24 Cnc system; suspected variable

37 Cnc

37

73316

42353

08^h 38^m 05.19^s

+09° 34′ 28.7″

6.54

1.25

373

A1V

35 Cnc

35

72779

42133

08^h 35^m 19.47^s

+19° 35′ 24.3″

6.55

0.28

585

G0III

ι Cnc B

ι

48

74738

43100

08^h 46^m 40.00^s

+28° 45′ 54.6″

6.58

2.77

188

G8II...

component of the ι Cnc system

40 Cnc

40

73666

42523

08^h 40^m 11.47^s

+19° 58′ 16.2″

6.61

0.40

570

A1V

in Beehive Cluster; blue straggler

83 Cnc

83

80218

45699

09^h 18^m 58.91^s

+17° 42′ 20.4″

6.61

3.64

128

F5

38 Cnc

38

BT

73575

42485

08^h 39^m 42.68^s

+19° 46′ 42.5″

6.66

0.59

531

F0III

in Beehive Cluster; δ Sct variable, ΔV = 0.06^m, P = 0.10 d

70 Cnc

70

77557

44512

09^h 04^m 09.87^s

+27° 53′ 53.9″

6.67

0.33

605

A1V

2 LMi

(2)

73427

42472

08^h 39^m 31.87^s

+32° 30′ 56.2″

6.69

−1.18

1220

K5

3 LMi

(3)

73508

42503

08^h 39^m 56.35^s

+32° 43′ 38.2″

6.71

0.66

528

K0

EP Cnc

EP

73819

42600

08^h 40^m 56.30^s

+19° 34′ 49.2″

6.76

0.6

556

A6Vn

in Beehive Cluster; δ Sct variable, ΔV = 0.03^m

42 Cnc

42

73785

42578

08^h 40^m 43.23^s

+19° 43′ 09.6″

6.83

0.87

506

A9III

in Beehive Cluster

7 Cnc

7

66347

39447

08^h 03^m 50.48^s

+22° 04′ 14.9″

6.84

0.28

668

K0

80 Cnc

80

79009

45153

09^h 11^m 56.93^s

+18° 02′ 39.0″

6.87

1.08

470

A0

^[2]^[3]

11 Cnc

11

67402

39888

08^h 08^m 49.60^s

+27° 28′ 49.5″

6.88

0.15

944

K0III

Double

78 Cnc

78

78479

44918

09^h 09^m 02.31^s

+17° 28′ 10.7″

7.18

0.5

706

K3III

VZ Cnc

VZ

73857

42594

08^h 40^m 52.13^s

+09° 49′ 27.1″

7.18

1.21

509

A9III

double-mode δ Sct variable, V_max = 7.18^m, V_min = 7.91^m, P = 0.18 d

ADS 7284

IP

79969

45617

09^h 17^m 53.46^s

+28° 33′ 37.9″

7.21

6.03

56.28

K3V

BY Dra variable, ΔV = 0.02^m, P = 43.4 d

52 Cnc

52

75558

43463

08^h 51^m 10.83^s

+15° 59′ 57.8″

7.38

1.03

607

G5

68 Cnc

68

77230

44336

09^h 01^m 43.66^s

+17° 04′ 51.8″

7.38

620

A2Vn

^[4]^[3]

V Cnc

V

70276

40977

08^h 21^m 42.84^s

+17° 17′ 07.2″

7.50

S0-6/6e

Mira variable, V_max = 7.5^m, V_min = 13.9^m, P = 270 d

T Cnc

T

43905

08^h 56^m 40.15^s

+19° 50′ 57.0″

7.60

C

semiregular variable, V_max = 7.6^m, V_min = 10.5^m, P = 482 d

BU Cnc

BU

73576

08^h 39^m 44.67^s

+19° 16′ 30.8″

7.68

1.44

577

A7Vn

in Beehive Cluster; δ Sct variable, ΔV = 0.03^m, P = 0.071 d

BN Cnc

BN

73763

08^h 40^m 39.24^s

+19° 13′ 41.8″

7.80

1.56

577

A9V

in Beehive Cluster; δ Sct variable, ΔV = 0.03^m, P = 0.039 d

HD 72490

72490

41997

08^h 33^m 36.6^s

+13° 33′ 03″

7.8

405

G5

has a planet (b)

24 Cnc B

24

71153

08^h 26^m 40.10^s

+24° 32′ 07.0″

7.81

component of the 24 Cnc system

BY Cnc

BY

74050

42705

08^h 42^m 10.81^s

+18° 56′ 03.7″

7.91

2.21

451

A7Vn

in Beehive Cluster; δ Sct variable, ΔV = 0.01^m, P = 0.058 d

HD 74028

BX

74028

08^h 42^m 06.50^s

+19° 24′ 40.5″

7.96

1.72

577

A7V

in Beehive Cluster; δ Sct variable, ΔV = 0.02^m, P = 0.044 d

44 Cnc

44

74200

42791

08^h 43^m 08.36^s

+18° 09′ 02.0″

8.03

1.29

726

K0

its radius is about 12.11 R_☉.^[5]^[6]

HD 79498

79498

45406

09^h 15^m 09^s

+23° 22′ 32″

8.03

4.72

150

G5

has a planet (b)

71 Cnc

71

77802

44637

09^h 05^m 45.52^s

+17° 23′ 24.5″

8.10

1.53

672

A2

CY Cnc

CY

73345

08^h 38^m 37.86^s

+19° 59′ 23.1″

8.14

1.88

582

F0V

in Beehive Cluster; δ Sct variable, ΔV = 0.02^m, P = 0.1 d

BQ Cnc

BQ

73729

08^h 40^m 26.75^s

+20° 10′ 55.2″

8.19

1.95

577

F2Vn

in Beehive Cluster; δ Sct variable, ΔV = 0.02^m, P = 0.074 d

HD 73534

73534

42446

08^h 39^m 15.80^s

+12° 57′ 37.3″

8.24

3.30

316

G5IV

Gakyid; has a planet (b)

BR Cnc

BR

73175

42319

08^h 37^m 40.71^s

+19° 31′ 06.3″

8.26

1.91

608

F0Vn

in Beehive Cluster; δ Sct variable, ΔV = 0.02^m, P = 0.038 d

S Cnc

S

74307

42853

08^h 43^m 56.14^s

+19° 02′ 03.0″

8.35

1.03

950

B9.5V+
G8-9III-IV

Algol variable, V_max = 8.29^m, V_min = 10.25^m, P = 9.48 d

BW Cnc

BW

73798

08^h 40^m 52.48^s

+20° 15′ 59.5″

8.48

2.24

577

F0Vn

in Beehive Cluster; δ Sct variable, ΔV = 0.01^m, P = 0.072 d

TW Cnc

TW

71780

08^h 29^m 37.32^s

+12° 27′ 20.3″

8.49

G8III+...

Algol variable, V_max = 8.5^m, V_min = 8.97^m, P = 70.76 d

U Cnc

U

72863

08^h 35^m 46.29^s

+18° 53′ 44.5″

8.50

M2e

Mira variable, V_max = 8.5^m, V_min = 15.5^m, P = 306 d

BS Cnc

BS

73450

08^h 39^m 09.10^s

+19° 35′ 32.6″

8.59

2.35

577

A9V

in Beehive Cluster; δ Sct variable, ΔV = 0.02^m, P = 0.051 d

R Cnc

R

69243

40534

08^h 16^m 33.90^s

+11° 43′ 35.0″

8.64

-0.36

2060

M6.5-9e

Mira variable, V_max = 6.07^m, V_min = 11.9^m, P = 357 d

BV Cnc

BV

73746

08^h 40^m 32.97^s

+19° 11′ 39.6″

8.65

2.41

577

F0V

in Beehive Cluster; δ Sct variable, ΔV = 0.02^m, P = 0.21 d

RZ Cnc

RZ

73343

42432

08^h 39^m 08.54^s

+31° 47′ 44.4″

8.67

0.48

1420

K2III

RS CVn variable, V_max = 8.67^m, V_min = 10.03^m, P = 21.64 d

HD 74721

74721

43018

08^h 45^m 59.26^s

+13° 15′ 48.6″

8.72

A0V

horizontal branch star

HD 77065

77065

44259

09^h 00^m 47.0^s

+21° 27′ 13″

8.8

6.3

103

G5

has a planet (b)

UU Cnc

UU

39341

08^h 02^m 30.90^s

+15° 10′ 41.9″

8.85

K4III...

β Lyr variable, V_max = 8.68^m, V_min = 9.35^m, P = 96.71 d

HIP 41378

41378

08^h 26^m 28.0^s

+10° 04′ 49″

8.9

3.58

378

has six planets (b, c, d, e, f & g)

RX Cnc

RX

68775

40388

08^h 14^m 43.54^s

+24° 44′ 05.3″

9.20

1.92

931

M8

semiregular variable

HD 80653

80653

09^h 21^m 21.0^s

+14° 22′ 05″

9.50

358

G5

semiregular variable

WY Cnc

WY

44349

09^h 01^m 55.45^s

+26° 41′ 22.7″

9.60

5.05

264.6

G5V

RS CVn variable, V_max = 9.51^m, V_min = 10.14^m, P = 0.83 d

TX Cnc

TX

08^h 40^m 01.70^s

+18° 59′ 59.5″

9.97

3.55

626

G0-G1V

in Beehive Cluster; W UMa variable, V_max = 10^m, V_min = 10.35^m, P = 0.38 d

RU Cnc

RU

42303

08^h 37^m 30.13^s

+23° 33′ 41.6″

10.20

2.97

911

F9V:+...

RS CVn variable, V_max = 10.1^m, V_min = 11.25^m, P = 10.17 d

TU Cnc

TU

08^h 52^m 16.65^s

+09° 05′ 18.8″

10.53

A2

Algol variable

SY Cnc

SY

09^h 01^m 03.32^s

+17° 53′ 56.2″

10.60

G8V

Z Cam variable

EX Cnc

EX

08^h 51^m 34.32^s

+11° 51′ 10.5″

10.95

1.34

2720

A7

in Messier 67; δ Sct variable, ΔV = 0.05^m, P = 0.049 d

TT Cnc

TT

41936

08^h 32^m 55.18^s

+13° 11′ 28.5″

11.10

F0

RR Lyr variable, V_max = 10.93^m, V_min = 11.57^m, P = 0.56 d

ES Cnc

ES

08^h 51^m 20.79^s

+11° 53′ 26.2″

11.16

1.55

2720

F4

in Messier 67; RS CVn variable, V_max = 11.16^m, V_min = 11.28^m, P = 1.07 d

HAT-P-31

08^h 06^m 09^s

+26° 25′ 36″

11.66

3.91

1155

has a transiting planet (b)

CU Cnc

CU

41824

08^h 31^m 37.57^s

+19° 23′ 39.4″

11.80

11.58

36.07

M5Ve

Algol variable and flare star, V_max = 11.68^m, V_min = 11.80^m, P = 2.77 d

WASP-65

08^h 53^m 18.0^s

+08° 31′ 23″

11.9

4.44

1011

G6

has a transiting planet (b)

SS Cnc

SS

08^h 06^m 25.60^s

+23° 15′ 05.7″

12.11

A8.5

RR Lyr variable, V_max = 11.49^m, V_min = 12.72^m, P = 0.37 d

EW Cnc

EW

08^h 51^m 32.58^s

+11° 50′ 40.6″

12.27

2.66

2720

F0

in Messier 67; δ Sct variable, ΔV = 0.02^m, P = 0.053 d

HV Cnc

HV

08^h 51^m 17.99^s

+11° 45′ 54.2″

12.73

3.12

2720

in Messier 67; Algol variable

EV Cnc

EV

08^h 51^m 28.15^s

+11° 49′ 27.5″

12.78

3.17

2720

F3

in Messier 67; W UMa variable, ΔV = 0.13^m, P = 0.44 d

AD Cnc

AD

08^h 46^m 20.10^s

+10° 20′ 07.2″

13.10

K0V

W UMa variable, V_max = 13.1^m, V_min = 13.4^m, P = 0.28 d

Gliese 299

08^h 11^m 57.575^s

+08° 46′ 22.05″

13.24

22

M4.5 Ve

a red dwarf, 15.5% as massive as the Sun,^[7] 17.9% as wide,^[8] and has a surface temperature of about 3,050 K.^[9]^[10]^[11]^[12]

HAT-P-43

08^h 35^m 42.0^s

+10° 12′ 24″

13.36

1771

has a transiting planet (b)

AH Cnc

AH

08^h 51^m 37.85^s

+11° 50′ 57.1″

13.41

3.8

2720

F7V

in Messier 67; W UMa variable, V_max = 13.31^m, V_min = 13.96^m, P = 0.36 d

HU Cnc

HU

08^h 51^m 13.36^s

+11° 51′ 40.1″

13.61

4

2720

G8IV

in Messier 67; RS CVn variable, V_max = 13.45^m, V_min = 13.61^m, P = 18.39 d

AC Cnc

AC

08^h 44^m 27.11^s

+12° 52′ 31.9″

13.80

K1-3V

Algol variable and nova-like star, V_max = 13.8^m, V_min = 15.4^m, P = 0.30 d

G 9-38

EI

08^h 58^m 15.19^s

+19° 45′ 47.1″

17.2

M5.5V

flare star

YBP 1194

08^h 51^m 00.81^s

+11° 48′ 52.8″

14.61

5

2720

G5V

in Messier 67; Solar analog; has 3 planets

DX Cnc

DX

08^h 29^m 49.35^s

+26° 46′ 33.7″

14.81

17.01

11.82

M6.5V

flare star

AT Cnc

AT

08^h 28^m 36.93^s

+25° 20′ 03.0″

15.2

DAe...

Z Cam variable, V_max = 12.57^m, V_min = 15.2^m, P = 0.20 d

LHS 2090

09^h 00^m 23.59^s

+21° 50′ 05.4″

16.10

17.08

20.782

M6.5V

^[10]^[13]^[14]^[15]^[16]

YZ Cnc

YZ

08^h 10^m 56.65^s

+28° 08′ 33.5″

16.3

SU UMa variable, V_max = 10.5^m, V_min = 16.3^m, P = 0.087 d

EG Cnc

EG

08^h 43^m 03.99^s

+27° 51′ 49.7″

17.0

Huruhata's Variable; WZ Sge variable, V_max = 11.9^m, V_min = 17.0^m, P = 0.060 d

DW Cnc

DW

07^h 58^m 53.05^s

+16° 16′ 45.2″

17.5

O...

dwarf nova, V_max = 11.36^m, V_min = 17.5^m, P = 0.0060 d

AZ Cnc

AZ

08^h 40^m 29.75^s

+18° 14′ 09.2″

17.59

16.86

45.7

M6.0V

flare star

GY Cnc

GY

09^h 09^m 50.55^s

+18° 49′ 47.5″

17.8

dwarf nova and eclipsing binary, V_max = 12.5^m, V_min = 17.8^m, P = 0.18 d

AR Cnc

AR

09^h 22^m 07.55^s

+31° 03′ 14.5″

18.7

dwarf nova and Algol variable, V_max = 15.3^m, V_min = 18.7^m, P = 0.21 d

RX J0806.3+1527

HM

08^h 06^m 22.95^s

+15° 27′ 31.1″

160

AM Canum Venaticorum star

AK Cnc

AK

08^h 55^m 21.18^s

+11° 18′ 15.3″

SU UMa variable

CC Cnc

CC

08^h 36^m 19.15^s

+21° 21′ 05.3″

K0V

SU UMa variable

PSR B0823+26

08^h 26^m 51.44^s

+26° 37′ 22.8″

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

↑ Final Results of NameExoWorlds Public Vote Released
↑ Abt, Helmut A. (2004). "Spectral Classification of Stars in A Supplement to the Bright Star Catalogue". The Astrophysical Journal Supplement Series. 155 (1): 175–177. Bibcode:2004ApJS..155..175A. doi:10.1086/423803.
1 2 van Leeuwen, F. (November 2007). "Validation of the new Hipparcos reduction". Astronomy & Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID 18759600.
↑ Bidelman, William P.; Ratcliff, Stephen J.; Svolopoulos, Sotirios (1988). "Spectral types of 80 early-type stars of variable radial velocity". Astronomical Society of the Pacific. 100: 828. Bibcode:1988PASP..100..828B. doi:10.1086/132242.
↑ "44 Cancri - HD74200 - HIP42791". Universe Guide. 25 January 2015. Retrieved 24 September 2017.
↑ SIMBAD, 44 Cancri (Retrieved 24 September 2017)
↑ Jenkins, J. S.; Ramsey, L. W.; Jones, H. R. A.; Pavlenko, Y.; Gallardo, J.; Barnes, J. R.; Pinfield, D. J. (2009). "Rotational Velocities for M Dwarfs". The Astrophysical Journal. 704 (2): 975–988. arXiv:0908.4092. Bibcode:2009ApJ...704..975J. doi:10.1088/0004-637X/704/2/975. S2CID 119203469.
↑ Dittmann, Jason A.; Irwin, Jonathan M.; Charbonneau, David; Berta-Thompson, Zachory K. (2014). "Trigonometric Parallaxes for 1507 Nearby Mid-to-late M Dwarfs". The Astrophysical Journal. 784 (2): 156. arXiv:1312.3241. Bibcode:2014ApJ...784..156D. doi:10.1088/0004-637X/784/2/156. S2CID 18789867.
↑ Lépine, Sébastien (2013). "A Spectroscopic Catalog of the Brightest (J < 9) M Dwarfs in the Northern Sky". The Astronomical Journal. 145 (4): 102. arXiv:1206.5991. Bibcode:2013AJ....145..102L. doi:10.1088/0004-6256/145/4/102. S2CID 117144290.
1 2 Cutri, R. M.; et al. (2003). "2MASS All-Sky Catalog of Point Sources". VizieR On-line Data Catalog. Bibcode:2003yCat.2246....0C.
↑ Wilson, Ralph Elmer (1953). "General catalogue of stellar radial velocities". Carnegie Institute Washington D.C. Publication. Bibcode:1953GCRV..C......0W.
↑ Zacharias, N. (2012). "The fourth US Naval Observatory CCD Astrograph Catalog (UCAC4)". VizieR On-line Data Catalog. Bibcode:2012yCat.1322....0Z.
↑ Alonso-Floriano, F. J.; Morales, J. C.; Caballero, J. A.; Montes, D.; Klutsch, A.; Mundt, R.; Cortés-Contreras, M.; Ribas, I.; Reiners, Ansgar; Amado, P. J.; Quirrenbach, A.; Jeffers, S. V. (2015). "CARMENES input catalogue of M dwarfs" (PDF). Astronomy & Astrophysics. 577: A128. arXiv:1502.07580. doi:10.1051/0004-6361/201525803. S2CID 53135130.
↑ Lépine, Sébastien; Shara, Michael M. (2005). "A Catalog of Northern Stars with Annual Proper Motions Larger than 0."15 (LSPM-NORTH Catalog)". The Astronomical Journal. 129 (3): 1483–1522. arXiv:astro-ph/0412070. Bibcode:2005AJ....129.1483L. doi:10.1086/427854. S2CID 2603568.
↑ "LHS 2090". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 29 January 2018.
↑ Henry, T. J.; Jao, Wei-Chun; Subasavage, John P.; Beaulieu, Thomas D.; Ianna, Philip A.; Costa, Edgardo; Méndez, René A. (2006). "The Solar Neighborhood. XVII. Parallax Results from the CTIOPI 0.9 m Program: 20 New Members of the RECONS 10 Parsec Sample" (PDF). The Astronomical Journal. 132 (6): 2360–2371. arXiv:astro-ph/0608230. Bibcode:2006AJ....132.2360H. doi:10.1086/508233. S2CID 15002841.{{cite journal}}: CS1 maint: multiple names: authors list (link)

Bibliography

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.
Gould, B. A. "Uranometria Argentina". Reprinted and updated by Pilcher, F. Archived from the original on 27 February 2012. Retrieved 19 July 2010.
Samus, N. N.; Durlevich, O. V.; et al. (2004). "Combined General Catalogue of Variable Stars (GCVS4.2)". Retrieved 4 April 2012.
Samus, N. N.; Durlevich, O. V.; et al. (2012). "General Catalog of Variable Stars (GCVS database, version 2012Feb)". Retrieved 4 April 2012.
"AAVSO Website". American Association of Variable Star Observers. Retrieved 9 March 2014.
"Naming Stars". Retrieved 4 July 2018.

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

[2] Abt, Helmut A. (2004). "Spectral Classification of Stars in A Supplement to the Bright Star Catalogue". The Astrophysical Journal Supplement Series. 155 (1): 175–177. Bibcode:2004ApJS..155..175A. doi:10.1086/423803.

[vanLeeuwen07-3] 1 2 van Leeuwen, F. (November 2007). "Validation of the new Hipparcos reduction". Astronomy & Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID 18759600.

[4] Bidelman, William P.; Ratcliff, Stephen J.; Svolopoulos, Sotirios (1988). "Spectral types of 80 early-type stars of variable radial velocity". Astronomical Society of the Pacific. 100: 828. Bibcode:1988PASP..100..828B. doi:10.1086/132242.

[5] "44 Cancri - HD74200 - HIP42791". Universe Guide. 25 January 2015. Retrieved 24 September 2017.

[6] SIMBAD, 44 Cancri (Retrieved 24 September 2017)

[7] Jenkins, J. S.; Ramsey, L. W.; Jones, H. R. A.; Pavlenko, Y.; Gallardo, J.; Barnes, J. R.; Pinfield, D. J. (2009). "Rotational Velocities for M Dwarfs". The Astrophysical Journal. 704 (2): 975–988. arXiv:0908.4092. Bibcode:2009ApJ...704..975J. doi:10.1088/0004-637X/704/2/975. S2CID 119203469.

[8] Dittmann, Jason A.; Irwin, Jonathan M.; Charbonneau, David; Berta-Thompson, Zachory K. (2014). "Trigonometric Parallaxes for 1507 Nearby Mid-to-late M Dwarfs". The Astrophysical Journal. 784 (2): 156. arXiv:1312.3241. Bibcode:2014ApJ...784..156D. doi:10.1088/0004-637X/784/2/156. S2CID 18789867.

[9] Lépine, Sébastien (2013). "A Spectroscopic Catalog of the Brightest (J < 9) M Dwarfs in the Northern Sky". The Astronomical Journal. 145 (4): 102. arXiv:1206.5991. Bibcode:2013AJ....145..102L. doi:10.1088/0004-6256/145/4/102. S2CID 117144290.

[Cutri,_R._M._2003-10] 1 2 Cutri, R. M.; et al. (2003). "2MASS All-Sky Catalog of Point Sources". VizieR On-line Data Catalog. Bibcode:2003yCat.2246....0C.

[11] Wilson, Ralph Elmer (1953). "General catalogue of stellar radial velocities". Carnegie Institute Washington D.C. Publication. Bibcode:1953GCRV..C......0W.

[12] Zacharias, N. (2012). "The fourth US Naval Observatory CCD Astrograph Catalog (UCAC4)". VizieR On-line Data Catalog. Bibcode:2012yCat.1322....0Z.

[13] Alonso-Floriano, F. J.; Morales, J. C.; Caballero, J. A.; Montes, D.; Klutsch, A.; Mundt, R.; Cortés-Contreras, M.; Ribas, I.; Reiners, Ansgar; Amado, P. J.; Quirrenbach, A.; Jeffers, S. V. (2015). "CARMENES input catalogue of M dwarfs" (PDF). Astronomy & Astrophysics. 577: A128. arXiv:1502.07580. doi:10.1051/0004-6361/201525803. S2CID 53135130.

[14] Lépine, Sébastien; Shara, Michael M. (2005). "A Catalog of Northern Stars with Annual Proper Motions Larger than 0."15 (LSPM-NORTH Catalog)". The Astronomical Journal. 129 (3): 1483–1522. arXiv:astro-ph/0412070. Bibcode:2005AJ....129.1483L. doi:10.1086/427854. S2CID 2603568.

[15] "LHS 2090". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 29 January 2018.

[16] Henry, T. J.; Jao, Wei-Chun; Subasavage, John P.; Beaulieu, Thomas D.; Ianna, Philip A.; Costa, Edgardo; Méndez, René A. (2006). "The Solar Neighborhood. XVII. Parallax Results from the CTIOPI 0.9 m Program: 20 New Members of the RECONS 10 Parsec Sample" (PDF). The Astronomical Journal. 132 (6): 2360–2371. arXiv:astro-ph/0608230. Bibcode:2006AJ....132.2360H. doi:10.1086/508233. S2CID 15002841.{{cite journal}}: CS1 maint: multiple names: authors list (link)

[1]

[2]

[3]

[4]

[5]

[6]

[7]

[8]

[9]

[10]

[11]

[12]

[13]

[14]

[15]

[16]

See also

References

Bibliography