Revision as of 13:11, 23 February 2005 editJyril (talk | contribs)Autopatrolled, Rollbackers15,217 editsm →Single planet systems: added greek letters, note on proper names← Previous edit | Revision as of 13:13, 23 February 2005 edit undoJyril (talk | contribs)Autopatrolled, Rollbackers15,217 editsm →Multiple planet systems: added Greek lettersNext edit → | ||
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===Multiple planet systems === | ===Multiple planet systems === | ||
''sorted alphabetically'' | |||
{| table border = 1 width="80%" cellpadding = 2 cellspacing = 0 | {| table border = 1 width="80%" cellpadding = 2 cellspacing = 0 | ||
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| c || 0.76 || 3.73 || 2594 | | c || 0.76 || 3.73 || 2594 | ||
|- | |- | ||
| rowspan="4" | ]<br>( |
| rowspan="4" | ]<br>(ρ<sup>1</sup> Cancri) || e || 14 M<sub>Earth</sub> || 0.038 || 2.81 | ||
|- | |- | ||
| b || 0.84 || 0.11 || 14.65 | | b || 0.84 || 0.11 || 14.65 | ||
Line 53: | Line 55: | ||
| c || 4.04 || 3.60 || 2102 | | c || 4.04 || 3.60 || 2102 | ||
|- | |- | ||
| rowspan="3" | ] || d || 13 M<sub>Earth</sub> || 0.09 || 9.55 | | rowspan="3" | ] || d || 13 M<sub>Earth</sub> || 0.09 || 9.55 | ||
|- | |- | ||
| b || 1.7 || 1.5 || 638 | | b || 1.7 || 1.5 || 638 | ||
Line 59: | Line 61: | ||
| c || 3.1 || 4.17 || 2986 | | c || 3.1 || 4.17 || 2986 | ||
|- | |- | ||
| rowspan="3" | ] || b || 0.69 || 0.059 || 4.6170 | | rowspan="3" | ] || b || 0.69 || 0.059 || 4.6170 | ||
|- | |- | ||
| c || 1.19 || 0.829 || 241.5 | | c || 1.19 || 0.829 || 241.5 |
Revision as of 13:13, 23 February 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
sorted alphabetically
star | planet | minimum mass (x Jupiter) |
orbital distance (x Earth) |
orbital period (days) |
---|---|---|---|---|
47 Ursae Majoris | b | 2.41 | 2.10 | 1095 |
c | 0.76 | 3.73 | 2594 | |
55 Cancri (ρ 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 | |
μ Arae | d | 13 MEarth | 0.09 | 9.55 |
b | 1.7 | 1.5 | 638 | |
c | 3.1 | 4.17 | 2986 | |
υ 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 99492 | b | 0.122 | 0.119 | 17.038 |
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 |
ε Eri | 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 45350 | b | 0.98 | 1.77 | 890.76 |
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 |
ρ 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 188015 | b | 1.26 | 1.19 | 456.46 |
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 |
ε 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 |
τ 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 (γ 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 |
HD 117207 | b | 2.06 | 3.78 | 2627.08 |
ρ Indi | b | 2.1 | 2.7 | 1294 |
HD 8574 | b | 2.23 | 0.76 | 228.8 |
ι 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 |
ψ 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 183263 | b | 3.69 | 1.52 | 634 |
HD 92788 | b | 3.8 | 0.94 | 340 |
τ 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 |
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 (ι 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 |
π 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.
All the proper names are totally unofficial and not used in the scientific literature.
Pulsars
pulsar | planet | mass (x Earth) | orbital distance (x Earth) |
orbital period (days) |
---|---|---|---|---|
PSR B1620-26 | C "PSR B1620-26c (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 |
Other
sorted by increasing mass
star | planet | minimum mass (x Jupiter) |
orbital distance (x Earth) |
orbital period (days) |
kind of star |
---|---|---|---|---|---|
2M1207 | b | ~5 | > 55 | > 2450 years | brown dwarf |
Planet imaged, mass derived from surface temperature of the planet.
See also
- Extrasolar planet
- Pulsar planets
- Hypothetical planet - also has unconfirmed and disproven planets
External links
- JPL Planetquest New Worlds Atlas
- 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