41 Super Jupiters Within 200 Parsecs

September 2008

 

Planet

Mjup

a

e

Per.

Msol

Type

[Fe/H]

Dist.

14 Herculis b

5.07

2.85

0.373

1755

0.99

K0

+0.46

18.15

HD 47536 b

5.20

1.61

0.200

712

1.10

K0 III

-0.680*

121

HD 68988 c

5.29

5.32

0.010

4100

1.18

G0

+0.324

58.8

81 Ceti b 1

5.30

2.50

0.206

953

2.4

G5 III

-0.060

97.2

HD 132406 b

5.61

1.98

0.340

974

1.09

G0

+0.180

71.0

HD 28185 b

5.72

1.03

0.070

383

0.99

G5

+0.220

39.6

HD 70573 b*

6.10

1.76

0.400

852

1

G1

-0.180

45.7

HD 2039 b

6.11

2.23

0.715

1120

1.17

G2

+0.315

89.9

HD 10697 b

6.38

2.16

0.102

1076

1.16

G5 IV

+0.194

32.6

HD 11977 b

6.52

1.94

0.400

711

1.91

G5 III

-0.210

66.5

HD 111232 b

6.84

1.97

0.200

1143

0.78

G8

-0.360

28.9

HD 81040 b

6.88

1.94

0.526

1002

0.96

G0

-0.160

32.6

HD 106252 b

7.10

2.60

0.586

1516

1.02

G0

-0.076

37.4

4 Ursae Majoris b

7.13

0.88

0.432

269

1.23

K1 III

-0.250

62.4

HD 178911 B b

7.35

0.35

0.139

72

1.06

G1

+0.285

46.7

70 Virginis b

7.49

0.48

0.401

117

1.11

G5

-0.012

18.1

Epsilon Tauri b

7.62

1.93

0.151

595

2.70

K0 III

+0.170

47.5

WASP-14 b 2

7.73

0.04

0.095

2.24

1.32

F5

0.0

160

HD 222582 b

7.76

1.35

0.725

572

0.99

G5

+0.029

42.0

HD 23596 b

7.80

2.83

0.292

1565

1.23

F8

+0.314

52.0

Planet

Mjup

a

e

Per.

Msol

Type

[Fe/H]

Dist.

HD 168443 b

8.02

0.30

0.528

58

1.05

G5

+0.077

37.9

HD 74156 c 3

8.03

3.35

0.430

2477

1.24

G0

+0.310

64.6

HD 104985 b 1

8.30

0.95

0.080

199

2.3

G9 III

-0.350

102

HD 89744 b

8.58

0.93

0.677

257

1.56

F7

+0.265

39.0

HAT-P-2 b 4
(HD 147506 b)

8.78

0.07

0.507

5.63

1.31

F8

+0.120

110

Iota Draconis b

8.82

1.27

0.712

511

1.05

K2 III

+0.030*

31.3

HD 33564 b

9.13

1.12

0.340

388

1.25

F6

-0.120

21.0

HD 33636 b

9.28

3.27

0.480

2128

1.02

G0

-0.126

28.7

HD 141937 b

9.68

1.52

0.410

653

1.08

G2

+0.129

33.5

18 Delphini b 1

10.3

2.60

0.080

993

2.3

G6 III

-0.050

73.0

Pi Mensae

10.3

3.38

0.640

2151

1.10

G1

+0.048

18.2

HD 30177 b

10.5

3.95

0.193

2770

1.07

G8

+0.394

54.7

HD 156846 b

11.0

1.12

0.847

359

1.43

G1

+0.220

49.0

HD 114762 b

11.7

0.36

0.336

84

0.89

F9

-0.653

40.6

XO-3 b 5

11.8

0.05

0.260

3.19

1.21

F5

-0.180

174

HD 136118 b

12.0

2.37

0.351

1193

1.23

F8

-0.050

52.3

HD 38529 c

13.1

3.74

0.356

2163

1.47

G4 IV

+0.445

42.4

HD 162020 b

15.0

0.08

0.277

8.43

0.78

K2

+0.112

31.3

HD 202206 b

17.3

0.82

0.435

256

1.12

G6

+0.354

46.3

HD 168443 c

18.1

2.91

0.218

1753

1.05

G5

+0.077

37.9

HD 137510 b

22.7

1.91

0.359

805

1.42

G0 IV

+0.373

41.8

Planet

Mjup

a

e

Per.

Msol

Type

[Fe/H]

Dist.

 

Column 1 gives the planet name. Column 2 gives the planet mass in units of Jupiter mass. Column 3 gives the planet semimajor axis in astronomical units (AU). Column 4 gives the orbital eccentricity. Column 5 gives the orbital period in days. Column 6 gives the star mass in units of Solar mass. Column 7 gives the star spectral type; if no Roman numeral is appended, the luminosity class is V, indicating a main sequence star. Column 8 gives the star metallicity (Solar = 0). Column 9 gives the star distance in parsecs (1 parsec = 3.26 light years).

 

Last update July 2008.  System parameters follow the Catalog of Nearby Exoplanets, July 2008, except as indicated.

 

*  Extrasolar Planets Encyclopaedia (EPE), July 2008.

1  Sato et al. 2008a, PASJ 60: 539-550;  Sato et al. 2008b, in press.

2  Joshi et al. 2008, MNRAS, in press.

3  Bean et al. 2008, ApJ 672: 1202-1208.

4  Torres et al. 2008, ApJ 677: 1324-1342.

5  Winn et al. 2008, in press.

 

Note: Four candidate Super Jupiters  listed in EPE are excluded:

 

HD 59686 b was originally announced in a BAAS abstract by Mitchell et al. (2003).  However, the discovery was never formally published, and the planet has not been listed in the Catalog of Nearby Exoplanets (which shares authors with the abstract) since 2006.  These omissions cast doubt on the object’s existence.

 

HD 13189 b is excluded because its host star’s mass is poorly constrained, preventing an accurate estimate of the planet’s mass and semimajor axis (Hatzes et al. 2005, A&A 437: 743).

 

ChaHa8 b is excluded because the system can be interpreted as a binary comprising two brown dwarfs, rather than as a star orbited by a planet (Joergens & Muller 2007, ApJ 666: L113). 

 

HD 41004 Bb is excluded because the system parameters are consistent with a binary comprising an M dwarf and a brown dwarf, rather than a star orbited by a planet (Zucker et al. 2004, A&A 426: 695–698).

 

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