44 SUPER JUPITERS within 200 PARSECS
|
PLANET |
STAR |
|||||||
|
Name |
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 |
|
BD-17 63 b 1 |
5.10 |
1.34 |
0.540 |
655 |
0.74 |
K5 |
-0.03 |
34.6 |
|
HD 47536 b |
5.20 |
1.61 |
0.200 |
712 |
1.10 |
K0 III |
-0.68 * |
121 |
|
HD 68988 c |
5.29 |
5.32 |
0.010 |
4100 |
1.18 |
G0 |
+0.324 |
58.8 |
|
81 Ceti b 2 |
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 3 |
6.7 |
1.10 |
0.050 |
379 |
1.24 |
G5 |
+0.240 |
39.56 |
|
HD 145377 b 1 |
5.76 |
0.45 |
0.307 |
104 |
1.12 |
G3 |
+0.12 |
57.7 |
|
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 3 |
6.7 |
1.90 |
0.200 |
1118 |
0.75 |
G5 |
-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 4 |
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 |
|
Name |
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 5 |
8.03 |
3.35 |
0.430 |
2477 |
1.24 |
G0 |
+0.310 |
64.6 |
|
HD 104985 b 2 |
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 6 |
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 |
+0.03 * |
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 2 |
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 7 |
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 131664 b 1 |
18.15 |
3.17 |
0.638 |
1951 |
1.10 |
G3 |
+0.32 |
55.43 |
|
HD 137510 b |
22.7 |
1.91 |
0.359 |
805 |
1.42 |
G0 IV |
+0.373 |
41.8 |
|
Name |
Mjup |
a |
e |
Per. |
Msol |
Type |
[Fe/H] |
Dist. |
|
PLANET |
STAR |
|||||||
Name = planet name. Mjup = planet mass in units of Jupiter mass. a = planet semimajor axis in astronomical units (AU). e = orbital eccentricity. Per. = orbital period in days. Msol = star mass in units of Solar mass. Type = star spectral type; if no Roman numeral is appended, the luminosity class is V, indicating a main sequence star. [Fe/H] = star metallicity (Solar = 0). Dist. = star distance in parsecs (1 parsec = 3.26 light years).
Last update December 2008. System parameters follow the Catalog of Nearby Exoplanets, July 2008, except as indicated.
* Extrasolar Planets Encyclopaedia (EPE), December 2008.
1 Moutou et al. 2008, A&A, in press.
2 Sato et al. 2008a, PASJ 60: 539-550; Sato et al. 2008b, in press.
3 Minniti et al. 2008, ApJ, in press.
4 Joshi et al. 2008, MNRAS, in press.
5 Bean et al. 2008, ApJ 672: 1202-1208.
6 Torres et al. 2008, ApJ 677: 1324-1342.
7 Winn et al. 2008, ApJ 683: 1076-1084.
Note: Five candidate Super Jupiters listed in EPE are excluded:
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 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).
HD 41004 Bb is excluded because the system parameters are consistent with a binary comprising an M dwarf and a brown dwarf, rather than an M dwarf orbited by a planet (Zucker et al. 2004, A&A 426: 695–698).
HD 43848 b is excluded because, with a minimum mass of 25 Mjup and an actual mass almost certainly larger, the discovery team consider it a likely brown dwarf rather than a bona fide exoplanet (Minniti et al. 2008, ApJ in press).
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.
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