| Revision as of 16:41, 23 December 2004 edit132.205.45.148 (talk) →External links← Previous edit | Revision as of 18:59, 4 January 2005 edit undo208.16.206.57 (talk) →Multiple planet systemsNext edit → | ||
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| ! star || planet || minimum mass<br>(x Jupiter) || orbital distance<br>(x Earth) || orbital period<br>(days) | ! star || planet || minimum mass<br>(x Jupiter) || orbital distance<br>(x Earth) || orbital period<br>(days) | ||
| |- | |- | ||
| | rowspan="2" | ] || b || 2.41 || 2.10 || 1095 | | rowspan="2" | ] || b || 2.41 || 2.10 || 1095 | ||
| |- | |- | ||
| | c || 0.76 || 3.73 || 2594 | | c || 0.76 || 3.73 || 2594 | ||
Revision as of 18:59, 4 January 2005
The following are lists of stars with confirmed extrasolar planets. Note that the masses of the planets are (for the most part) lower bounds only. If a planet is detected by the spectral line displacement method, no information is gained about the inclination of the planet's plane of orbit around its star, and a value for this is needed to calculate the mass. It has become customary to arbitrarily assume that the plane is exactly lined up with the line of sight from Earth (this produces the lowest possible mass consistent with the spectral line measurements). The planets are listed with indications of their approximate masses as multiples of Jupiter's mass (MJ = 1.898 x 10 kg) or multiples of Earth's mass (ME = 5.9737 x 10 kg), and some also have approximate distances in astronomical units (1 AU = 1.496 x 10 km) from their parent stars. For more information on how planets may be detected, see extrasolar planet.
Normal stars
Multiple planet systems
| star | planet | minimum mass (x Jupiter) |
orbital distance (x Earth) |
orbital period (days) |
|---|---|---|---|---|
| 47 poop | b | 2.41 | 2.10 | 1095 |
| c | 0.76 | 3.73 | 2594 | |
| 55 Cancri (Rho Cancri) |
e | 14 MEarth | 0.038 | 2.81 |
| b | 0.84 | 0.11 | 14.65 | |
| c | 0.21? | 0.24? | 44.28? | |
| d | 4.05 | 5.9 | 5360 | |
| Gliese 876 | c | 0.56 | 0.13 | 30.1 |
| b | 1.98 | 0.21 | 61.02 | |
| HD 12661 | b | 2.30 | 0.83 | 263.6 |
| c | 1.57 | 2.56 | 1444.5 | |
| HD 37124 | b | 0.75 | 0.54 | 152.4 |
| c | 1.2 | 2.5 | 1495 | |
| HD 38529 | b | 0.78 | 0.129 | 14.309 |
| c | 12.70 | 3.68 | 2174.3 | |
| HD 74156 | b | 1.86 | 0.294 | 51.643 |
| c | > 6.17 | 3.40 | 2025 | |
| HD 82943 | b | 0.88 | 0.73 | 221.6 |
| c | 1.63 | 1.16 | 444.6 | |
| HD 168443 | b | 7.7 | 0.29 | 58.116 |
| c | 16.9 | 2.85 | 1739.50 | |
| HD 169830 | b | 2.88 | 0.81 | 225.62 |
| c | 4.04 | 3.60 | 2102 | |
| Mu Arae | d | 13 MEarth | 0.09 | 9.55 |
| b | 1.7 | 1.5 | 638 | |
| c | 3.1 | 4.17 | 2986 | |
| Upsilon Andromedae | b | 0.69 | 0.059 | 4.6170 |
| c | 1.19 | 0.829 | 241.5 | |
| d | 3.75 | 2.53 | 1284. |
Note:
Planet confirmed astrometrically.
Single planet systems
sorted by increasing mass
| star | planet | minimum mass (x Jupiter) |
orbital distance (x Earth) |
orbital period (days) |
|---|---|---|---|---|
| GJ 436 | b | 21 MEarth | 0.0278 | 2.6441 |
| HD 49674 | b | 0.12 | 0.0568 | 4.948 |
| HD 117618 | b | 0.16 | ~0.15 | 25.8 |
| HD 102117 | b | 0.18 | ~0.15 | 20.8 |
| HD 76700 | b | 0.197 | 0.049 | 3.971 |
| 54 Piscium | b | 0.2 | 0.284 | 62.23 |
| HD 168746 | b | 0.23 | 0.065 | 6.403 |
| 79 Ceti | b | 0.23 | 0.35 | 75.560 |
| HD 46375 | b | 0.249 | 0.041 | 3.024 |
| HD 88133 | b | 0.29 | 0.046 | 3.415 |
| HD 208487 | b | 0.41 | ~0.5 | 129 |
| HD 83443 | b | 0.41 | 0.04 | 2.985 |
| HD 108147 | b | 0.41 | 0.104 | 10.901 |
| HD 75289 | b | 0.42 | 0.046 | 3.51 |
| 51 Pegasi | b "Bellerophon" |
0.468 | 0.052 | 4.23077 |
| BD-10°3166 | b | 0.48 | 0.046 | 3.487 |
| HD 6434 | b | 0.48 | 0.15 | 22.09 |
| HD 187123 | b | 0.52 | 0.042 | 3.097 |
| OGLE-TR-111 | b | 0.53 | 0.047 | 4.02 |
| HD 216770 | b | 0.65 | 0.46 | 118.45 |
| HD 209458 | b "Osiris" |
0.69 | 0.045 | 3.524738 |
| HD 192263 | b | 0.72 | 0.15 | 24.348 |
| GSC 02652-01324 | TrES-1 | 0.75 | 0.0393 | 3.030065 |
| HD 330075 | b | 0.76 | 0.043 | 3.369 |
| HD 4208 | b | 0.80 | 1.67 | 812.197 |
| HD 114729 | b | 0.82 | 2.08 | 1131.478 |
| HD 179949 | b | 0.84 | 0.045 | 3.093 |
| Epsilon Eridani | b | 0.86 | 3.3 | 2502.1 |
| HD 121504 | b | 0.89 | 0.32 | 64.6 |
| HD 114783 | b | 0.9 | 1.20 | 501.0 |
| HD 10647 | b | 0.91 | 2.10 | 1040 |
| HD 114386 | b | 0.99 | 1.62 | 872 |
| HD 147513 | b | 1. | 1.26 | 540.4 |
| HD 150706 | b | 1.0 | 0.82 | 264.9 |
| OGLE-TR-132 | b | 1.01 | 0.0306 | 1.69 |
| Rho Coronae Borealis | b | 1.04 | 0.22 | 39.845 |
| HD 20367 | b | 1.07 | 1.25 | 500 |
| HD 130322 | b | 1.08 | 0.088 | 10.724 |
| HD 52265 | b | 1.13 | 0.49 | 118.96 |
| HD 65216 | b | 1.21 | 1.37 | 613.1 |
| HD 217107 | b | 1.28 | 0.07 | 7.11 |
| HD 177830 | b | 1.28 | 1.00 | 391 |
| HD 210277 | b | 1.28 | 1.097 | 437 |
| Epsilon Reticuli | b | 1.28 | 1.18 | 423.841 |
| Gliese 777 | b | 1.33 | 4.8 | 2902 |
| OGLE-TR-113 | b | 1.35 | 0.0228 | 1.43 |
| HD 142 | b | 1.36 | 0.980 | 338.0 |
| OGLE-TR-56 | b | 1.45 | 0.0225 | 1.2 |
| Tau Grucis | b | 1.49 | 2.7 | 1442.919 |
| OGLE 2003-BLG-235 (MOA 2003-BLG-53) |
1.5-2.5 | 2.8 | unknown | |
| 23 Librae | b | 1.58 | 0.78 | 260 |
| Errai (Gamma Cephei) |
b | 1.59 | 2.03 | 902.96 |
| HD 142415 | b | 1.62 | 1.05 | 386.3 |
| HD 108874 | b | 1.65 | 1.07 | 401 |
| HD 4203 | b | 1.65 | 1.09 | 400.944 |
| 16 Cygni B | b | 1.69 | 1.67 | 798.938 |
| HD 154857 | b | 1.80 | 1.11 | 398 |
| HD 73256 | b | 1.85 | 0.037 | 2.54863 |
| HD 68988 | b | 1.90 | 0.071 | 6.276 |
| 94 Ceti | b | 2.0 | 1.3 | 454 |
| HD 70642 | b | 2.0 | 3.3 | 2231 |
| Rho Indi | b | 2.1 | 2.7 | 1294 |
| HD 8574 | b | 2.23 | 0.76 | 228.8 |
| Iota Horologii | b | 2.26 | 0.925 | 320.1 |
| HD 41004 | b | 2.3 | 1.31 | 655 |
| HD 72659 | b | 2.55 | 3.24 | 2185 |
| HD 23079 | b | 2.61 | 1.65 | 738.459 |
| HD 128311 | b | 2.63 | 1.06 | 414 |
| HD 37605 | b | 2.85 | 0.26 | 55.2 |
| Psi Aquarii | b | 2.9 | ~0.3 | 182 |
| HD 73526 | b | 3.0 | 0.66 | 190.5 |
| HD 196050 | b | 3.0 | 2.5 | 1289 |
| GJ 3021 | b | 3.21 | 0.49 | 133.82 |
| HD 40979 | b | 3.32 | 0.811 | 267.2 |
| HD 80606 | b | 3.41 | 0.439 | 111.78 |
| HD 195019 | b | 3.43 | 0.14 | 18.3 |
| HD 92788 | b | 3.8 | 0.94 | 340 |
| Tau Boötis | b | 3.87 | 0.0462 | 3.3128 |
| Gliese 86 | b | 4. | 0.11 | 15.78 |
| HD 213240 | b | 4.5 | 2.03 | 951 |
| 14 Herculis | b | 4.74 | 2.80 | 1796.4 |
| HD 2039 | b | 4.85 | 2.19 | 1192.582 |
| HD 50554 | b | 4.9 | 2.38 | 1279.0 |
| HD 47536 | b | 4.96-9.67 | 1.61-2.25 | 712.13 |
| HD 190228 | b | 4.99 | 2.31 | 1127 |
| 2M1207 | b | ~5 | > 55 | > 2450 years |
| HD 222582 | b | 5.11 | 1.35 | 572.0 |
| HD 28185 | b | 5.6 | 1.0 | 385 |
| 109 Piscium | b | 6.12 | 2.13 | 1077.906 |
| HD 178911 B | b | 6.292 | 0.32 | 71.487 |
| HD 104985 | b | 6.3 | 0.78 | 198.2 |
| HD 59686 | b | 6.5 | ~0.8 | 303 |
| HD 111232 | b | 6.8 | 1.97 | 1143 |
| HD 106252 | b | 6.81 | 2.61 | 1500 |
| HD 23596 | b | 7.19 | 2.72 | 1558 |
| 70 Virginis | b "Goldilocks" |
7.44 | 0.48 | 116.689 |
| HD 89744 | b | 7.99 | 0.89 | 256.6 |
| Edasich (Iota Draconis) |
b | 8.64 | 1.34 | 550.651 |
| HD 30177 | b | 9.17 | 3.86 | 2819.654 |
| HD 33636 | b | 9.28 | 3.56 | 2447.292 |
| HD 141937 | b | 9.7 | 1.52 | 653.22 |
| Pi Mensae | b | 10.35 | 3.29 | 2063.818 |
| HD 114762 | b | 11. | 0.3 | 84.03 |
| HD 136118 | b | 11.9 | 2.335 | 1209.6 |
| HD 162020 | b | 13.75 | 0.072 | 8.428198 |
Note:
Transit detected, absolute mass of the planet.
Planet found by gravitational lensing method.
Planet imaged, mass derived from surface temperature of the planet.
Pulsars
| pulsar | planet | mass (x Earth) | orbital distance (x Earth) |
orbital period (days) |
|---|---|---|---|---|
| PSR B1620-26 | C "Methuselah" |
2.5 MJupiter | 23 | ~ 100 years |
| PSR 1257+12 | A | 0.020 | 0.19 | 25.262 |
| B | 4.3 | 0.36 | 66.5419 | |
| C | 3.9 | 0.46 | 98.2114 |
See also
- Extrasolar planet
- Pulsar planets
- Hypothetical planet - also has unconfirmed and disproven planets
External links
- Extrasolar Planets Catalog - Observatory of Paris
- List of planet discoveries and confirmations from Geneva Observatory
- Almanac of planets - California & Carnegie Planet Search
- XML catalogue of known extrasolar planets