2011年发现的系外行星列表

维基媒体列表条目

这是2011年发现的系外行星列表[1]

仅由径向速度发现的太陽系外行星,下列表格記載的质量為其下限

名称 质量(MJ 半径(RJ 轨道周期(天) 半长轴(AU) 温度K 发现方式 距离(ly) 主星质量(M 主星温度(K) 注释
7 Canis Majoris b英语7 Canis Majoris b 1.85 735.1 1.758 径向速度 64.65 1.34 4826 [2]
天园增三b 0.0085 18.315 0.1207 660 径向速度 19.57 0.7 5401 [3]
天园增三c 0.0076 40.114 0.2036 508 径向速度 19.57 0.7 5401 [3]
天园增三d 0.015 90.309 0.3499 388 径向速度 19.57 0.7 5401 [3]
BD+48 738 b英语BD+48 738 b 0.91 392.6 1.0 径向速度 2910 0.74 4414 [4]
CFBDSIR J145829+101343 b英语CFBDSIR J145829+101343 b 10.5 10037.5 2.6 370 影像 75.34 0.02 580 可能是褐矮星[5]
COCONUTS-2b 6.3+1.5
−1.9
400000000 7506+5205
−2060
434+9
影像 35.6 0.37+0.02
3406+69
2021年,行星被归为WISEPA J075108.79−763449.6。轨道周期最长的系外行星[6]
柯洛16b英语CoRoT-16b 0.535 1.17 5.35227 0.0618 1086 凌日 2740 1.1 5650 [7]
柯洛17b英语CoRoT-17b 2.43 1.02 3.7681 0.0461 1626 凌日 3001 1.04 5740 [8]
柯洛18b英语CoRoT-18b 3.47 1.31 1.9000693 0.0295 1550 凌日 2838 0.95 5440 [9]
柯洛19b英语CoRoT-19b 1.11 1.29 3.89713 0.0518 2000 凌日 2511 1.21 6090 [10]
柯洛20b英语CoRoT-20b 4.3 0.84 9.24285 0.09 1024 凌日 2819 1.14 4947 [11]
柯洛23b英语CoRoT-23b 2.8 1.05 3.6313 0.048 1660 凌日 1957 1.14 5900 [12]
格利泽433b 0.01901 7.3705 0.062 径向速度 29.58 0.48 3461 [13]
格利泽667Cc 0.012 28.14 0.125 径向速度 22.18 0.33 3350 [13]可能宜居的行星
格利泽785b英语Gliese 785 b 0.0532 74.72 0.32 355 径向速度 28.7 0.8 5166 [3]
格利泽785c英语Gliese 785 c 0.076 525.8 1.18 185 径向速度 28.7 0.8 5166 [3]
HAT-P-27b英语HAT-P-27 0.62 1.02 3.039577 0.04 凌日 665.38 0.94 5300 [14]
HAT-P-28b英语HAT-P-28 0.626 1.212 3.257215 0.0434 1384 凌日 1288 1.02 5680 [15]
HAT-P-29b英语HAT-P-29 0.88 1.17 5.72319 0.0667 1271 凌日 1032 1.45 6087 [15]正式名
Surt
HAT-P-30b英语HAT-P-30 0.83 1.44 2.8106 0.0419 1630 凌日 702.2 1.55 6304 独立发现[16][17]
HAT-P-31b 2.27 1.09 5.00542 0.061 1450 凌日 1133 1.31 6065 该恒星系可能还有其他行星[18]
HAT-P-32b 0.68 1.98 2.1500082 0.03397 1836 凌日 950.81 1.13 6001 [19]
HAT-P-33b英语HAT-P-33b 0.92 1.85 3.47447 0.04995 1782 凌日 1306 1.82 6446 [19]
HD 1502 b 2.75 428.5 1.262 径向速度 626.11 1.46 4947 [20]正式名
Indépendance
HD 5891 b 7.63 177.11 0.64 径向速度 932.02 1.93 4673 [20]
HD 7199 b英语HD 7199 b 0.27 615 1.36 径向速度 118.04 0.77 5371 [21]正式名
Hairu
HD 7449 A b英语HD 7449 0.508 1255.5 2.38 径向速度 126.26 1.05 6024 [21]
HD 14651 b 47+3.4
79.4179+0.0021
0.361+0.013
径向速度 127 0.96+0.03
5491+26
褐矮星或恒星[22]
HD 18742 b 3.4 766 1.82 径向速度 532.86 1.36 4940 [20]正式名
Bagan
HD 20781 b英语HD 20781 b 0.0061+0.0012
−0.0011
0.2052 5.3135+0.001
0.0529+0.0024
−0.0027
径向速度 115.36+4.4
0.7 5256+29
HD 20781 c英语HD 20781 c 0.0168+0.0022
−0.0021
0.2183 13.8905+0.0033
−0.0034
0.1004+0.0046
−0.0051
径向速度 115.36+4.4
0.7 5256+29
HD 22781 b英语HD 22781 13.65 528.07 1.167 径向速度 106.43 0.75 5027 [22]
HD 28678 b 1.542 380.2 1.18 径向速度 622.72 1.53 4972 [20]正式名
Tassili
HD 30246 b 55.1+20.3
−8.2
990.7+5.6
2.012+0.069
径向速度 160 1.05+0.04
5833+44
褐矮星或恒星[22]
HD 30856 b 1.547 847 1.85 径向速度 429.56 1.17 4895 [20]正式名
Nakanbé
HD 33142 b 1.385 326 1.07 径向速度 397.27 1.41 4978 [20]
HD 82886 b英语HD 82886 2.33 705 1.58 径向速度 415.93 2.53 4953 [20]正式名
Arber
HD 85512 b 0.01 58.43 0.26 298 径向速度 36.79 0.43 4300 [3]
HD 96063 b 1.27 362.5 1.11 径向速度 458.66 1.37 5020 [20]正式名
Ramajay
HD 96127 b 20.96 647.3 1.42 径向速度 1949 10.94 3943 [4]可能不是行星,而是恒星[23]
HD 98219 b英语HD 98219 1.964 433.8 1.26 径向速度 372.06 1.41 4925 [20]正式名
Ixbalanqué
HD 99706 b英语HD 99706 1.23 841 1.98 径向速度 480.15 1.46 4862 [20]
HD 100655 b 1.61 157.57001 0.68 径向速度 449.2 2.28 4891 [24]正式名
Sazum
HD 102329 b 8.16 778.1 1.81 径向速度 712.41 3.21 4745 [20]
HD 106270 b 10.13 1888 3.34 径向速度 306.79 1.39 5509 [20]
HD 108863 b英语HD 108863 2.414 437.7 1.32 径向速度 539.87 1.59 4878 [20]
HD 116029 b英语HD 116029 1.4 670 1.65 径向速度 403.4 0.83 4819 [20]该恒星系可能有两颗行星
HD 131496 b英语HD 131496 1.8 896 2.01 径向速度 431.65 1.34 4846 [20]正式名
Madriu
HD 132563 Bb英语HD 132563 Bb 1.49 1544 2.62 径向速度 344.01 1.08 6073 [25]
HD 137388 b英语HD 137388 0.2 330 0.89 径向速度 132.2 0.68 5181 [21]正式名
Kererū
HD 142245 b英语HD 142245 3.07 1299 2.78 径向速度 318.01 3.5 4922 [20]
HD 152581 b 1.869 686.5 1.66 径向速度 543.2 1.3 5027 [20]正式名
Ganja
HD 156279 b英语HD 156279 9.88 131.05 0.49 径向速度 118.17 0.95 5453 [22]
HD 158038 b 1.53 521 1.5 径向速度 310.25 1.3 4860 [20]
HD 163607 b英语HD 163607 b 0.7836 75.2203 0.362 径向速度 221.53 1.12 5522 [26]
HD 163607 c英语HD 163607 c 2.201 1272 2.39 径向速度 221.53 1.12 5522 [26]
HD 164509 b英语HD 164509 0.443 280.17 0.87 径向速度 173.49 1.12 5922 [26]
HD 192310 c英语HD 192310 c 0.076 525.8 1.18 径向速度 28.7 0.78 5069 [3]
HD 204941 b 0.266 1733 2.55 径向速度 93.74 0.58 5026 [21]
HD 240237 b英语HD 240237 b 15.89 745.7 1.92 径向速度 3125 8.76 3926 [4]
HIP 5158 c英语HIP 5158 c 15.04 9017.76 7.7 径向速度 168.56 0.78 4962 [27]
HIP 57274 b英语HIP 57274 0.02 8.1352 0.07 径向速度 84.41 0.29 4510 [28]
HIP 57274 c英语HIP 57274 0.40902 32.03 0.178 径向速度 84.41 0.29 4510 [28]
HIP 57274 d 0.5267 431.7 1.01 径向速度 84.41 0.29 4510 [28]
HU Aquarii b 5.9 2390 3.6 计时 626.89 0.88 5952 有争议
HU Aquarii c英语HU Aquarii c 4.5 4368 5.4 计时 626.89 0.88 5952 有争议
开普勒-10b 0.0145 0.132 0.837491 0.0172 2130 凌日 608.3 0.91 5708 [29]
克卜勒-10c 0.02319 0.207 45.2946 0.241 584 凌日 608.3 0.91 5708 [30]
开普勒-11b英语Kepler-11b 0.006 0.161 10.3039 0.091 凌日 2148 0.96 5663 [31]
开普勒-11c英语Kepler-11c 0.009 0.256 13.0241 0.107 凌日 2148 0.96 5663 [31]
开普勒-11d英语Kepler-11d 0.023 0.278 22.6845 0.155 凌日 2148 0.96 5663 [31]
开普勒-11e英语Kepler-11e 0.025 0.374 31.9996 0.195 凌日 2148 0.96 5663 [31]
开普勒-11f英语Kepler-11f 0.006 0.222 46.6888 0.25 凌日 2148 0.96 5663 [31]
开普勒-11g英语Kepler-11g 0.079 0.297 118.3807 0.466 凌日 2148 0.96 5663 [31]
开普勒-12b英语Kepler-12b 0.432 1.754 4.4379629 0.0553 1480 凌日 2950 1.17 5947 [32]
开普勒-13b英语Kepler-13 9.28 1.512 1.763588 0.03641 2550 凌日 1354 1.72 7650 [33]
开普勒-14b英语Kepler-14b 8.4 1.136 6.790123 0.0771 1605 凌日 3196 1.51 6395 [34]
开普勒-15b英语Kepler-15b 0.66 0.96 4.942782 0.05714 1251 凌日 2464 1.02 5515 [35]
克卜勒16b 0.333 0.754 228.776 0.7048 凌日 245.44 0.69 4450 [36]
开普勒-17b英语Kepler-17b 2.45 1.31 1.4857108 0.02591 1570 凌日 2609 1.16 5781 [37]
开普勒-18b英语Kepler-18 0.022 0.178 3.504725 0.0447 凌日 1430 0.97 5345 [38]
开普勒-18c英语Kepler-18 0.054 0.49 7.64159 0.0752 凌日 1430 0.97 5345 [38]
开普勒-18d英语Kepler-18 0.052 0.623 14.85888 0.1172 凌日 1430 0.97 5345 [38]
克卜勒-19b 0.02643 0.197 9.28716 0.085 凌日 717.4 0.94 5544 [39]
克卜勒-19c 0.04122 28.731 计时 717.4 0.94 5544 [39]
克卜勒20b 0.03052 0.167 3.69611525 0.0463 1105 凌日 929.18 0.95 5495 [40]
克卜勒20c 0.04012 0.272 10.85409089 0.0949 772 凌日 929.18 0.95 5495 [40]
克卜勒20d 0.03168 0.245 77.61130017 0.3506 401 凌日 929.18 0.95 5495 [40]
克卜勒20e 0.01 0.077 6.09852281 0.0639 1040 凌日 929.18 0.95 5495 [40]
克卜勒20f 0.045 0.089 19.57758478 0.1396 705 凌日 929.18 0.95 5495 [40]
开普勒-21b英语Kepler-21b 0.01598 0.146 2.78578 0.042717 2025 凌日 370 1.41 6305 [41]
克卜勒22b 0.113 0.212 289.8623 0.849 262 凌日 619.72 0.97 5518 可能宜居的系外行星[42]
开普勒-23b英语Kepler-23b 0.8 0.17 7.1073 0.075 凌日 2793 1.1 5828 [43]
开普勒-23c英语Kepler-23c 2.7 0.285 10.7421 0.099 凌日 2793 1.1 5828 [43]
开普勒-24b英语Kepler-24b 1.6 0.214 8.1453 0.08 凌日 3901 0.98 5897 [43]
开普勒-24c英语Kepler-24c 1.6 0.25 12.3335 0.106 凌日 3901 0.98 5897 [43]
开普勒-25b英语Kepler-25b 0.0275 0.245 6.238297 0.068 凌日 798.98 1.19 6270 [44]
开普勒-25c英语Kepler-25c 0.0479 0.465 12.7207 0.11 凌日 798.98 1.19 6270 [44]
开普勒-26b英语Kepler-26 0.01611 0.248 12.28 0.08551 427 凌日 1104 0.54 3914 [44]
开普勒-26c英语Kepler-26 0.01951 0.243 17.2559 0.10725 381 凌日 1104 0.54 3914 [44]
开普勒-27b英语Kepler-27 9.11 0.357 15.3348 0.118 凌日 3507 0.65 5400 [44]
开普勒-27c英语Kepler-27 13.8 0.437 31.3309 0.191 凌日 3507 0.65 5400 [44]
开普勒-28b英语Kepler-28b 1.51 0.321 5.9123 0.062 583 凌日 1448 0.75 4590 [44]
开普勒-28c英语Kepler-28 1.36 0.303 8.9858 0.081 507 凌日 1448 0.75 4590 [44]
开普勒-29b英语Kepler-29 0.01419 0.299 10.3384 0.09 凌日 2779 0.98 5701 [45]
开普勒-29c英语Kepler-29 0.01259 0.28 13.2884 0.11 凌日 2779 0.98 5701 [45]
开普勒-31b英语Kepler-31 0.491 20.8613 0.16 凌日 5700 1.21 6340 [46]
开普勒-31c英语Kepler-31 4.7 0.473 42.6318 0.26 凌日 5700 1.21 6340 [46]
开普勒-32b英语Kepler-32b 4.1 0.196 5.90124 0.05 530 凌日 1066 0.58 3900 [46]
开普勒-32c英语Kepler-32c 0.5 0.178 8.7522 0.09 470 凌日 1066 0.58 3900 [46]
Kepler-33b 0.155 5.66793 0.0677 凌日 4086 1.29 5904 [47]
开普勒-33c 0.00123 0.285 13.17562 0.1189 凌日 4086 1.29 5904 [47]
开普勒-33d 0.0123 0.477 21.77596 0.1662 凌日 4086 1.29 5904 [47]
开普勒-33e 0.01753 0.359 31.7844 0.2138 凌日 4086 1.29 5904 [47]
开普勒-39b英语Kepler-39b 20.1 1.24 21.08721 0.164 897 凌日 3557 1.29 6350 [48]褐矮星
开普勒-41b英语Kepler-41b 0.56 1.29 1.8555582 0.03101 1790 凌日 3680 1.15 5750 [49]
开普勒-42b 0.07 1.2137672 0.0116 519 凌日 126.23 0.13 3068 [30]
开普勒-42c 0.065 0.45328509 0.006 720 凌日 126.23 0.13 3068 [30]
开普勒-42d 0.051 1.865169 0.0154 450 凌日 126.23 0.13 3068 [30]
开普勒-43b英语Kepler-43 3.23 1.219 3.0240949 0.046 1620 凌日 3379 1.32 6041 [37]
开普勒-44b英语Kepler-44b 1.0 1.09 3.2467293 0.0446 1544 凌日 4009 1.12 5800 [37]
开普勒-45b英语Kepler-45b 0.505 0.96 2.455239 0.03 1000 凌日 1086 0.59 3820 [47]
开普勒-70b 0.0014 0.068 0.240104 0.006 轨道反射 3849 0.5 27730 有争议[50]
开普勒-70c英语Kepler-70c 0.0021 0.077 0.342887 0.0076 轨道反射 3849 0.5 27730 有争议[50]
MOA-2009-BLG-266Lb 0.033 2774 3.2 微重力透镜 9900 0.56 [51]
NY Vir (AB) b英语NY Virginis 2.3 3160 3.3 计时 1800 0.6 33000 环联星运转行星[52]
NY Vir (AB) c英语NY Virginis 4.49 9861.75 7.54 计时 1800 0.6 33000 环联星运转行星[53]
PSR J1719-1438 b 1.2 0.09070629 0.0044 计时 3914 1.4 4500 已知公转周期最短的系外行星[54]
Qatar-2 b英语Qatar-2 2.494 1.254 1.33711647 0.02153 1344 凌日 594.67 0.74 4645 [55]
TrES-5英语GSC 03949-00967 1.79 1.194 1.48224686 0.02459 1480 凌日 1188 0.9 5171 [56]
UZ Fornacis b英语UZ Fornacis 6.3 5840 5.9 计时 781.5 0.7 5286 不是行星
UZ Fornacis c英语UZ Fornacis 7.7 1916.25 2.8 计时 781.5 0.7 5286 未确认
WASP-35b英语WASP-35 0.72+0.06
1.32+0.03
3.16158 0.04317 凌日 663.39 1.05 5990 [16]
WASP-39b 0.28 1.27 4.055259 0.0486 1166 凌日 750.18 0.93 5400 [57]正式名
Bocaprins
WASP-43b 1.78 0.93 0.813475 0.0142 1427 凌日 260.93 0.58 4400 [58]
WASP-44b英语WASP-44b 0.87 1.1 2.423804 0.03453 1337 凌日 1201 0.94 5420 [59]
WASP-45b英语WASP-45 0.964 0.946 3.126089 0.03963 1153 凌日 693.04 0.85 5150 [59]
WASP-46b英语WASP-46 1.91 1.174 1.43036763 0.02335 1636 凌日 1237 0.83 5600 [59]
WASP-48b英语WASP-48b 0.8 1.5 2.14363 0.03444 2035 凌日 1501 0.88 5920 [16]
WASP-50 b英语WASP-50 1.4688 1.166 1.9551 0.0293 1395 凌日 606.08 0.89 5400 [60]正式名
Maeping
WD 0806-661 b 7.5 2500 323 影像 62.62 0.62 9552 Y-型褐矮星[61]


参考

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  3. ^ 3.0 3.1 3.2 3.3 3.4 3.5 3.6 Pepe, F; et al. The HARPS search for Earth-like planets in the habitable zone: I – Very low-mass planets around HD20794, HD85512 and HD192310. Astronomy & Astrophysics. 2011, 534: A58. Bibcode:2011A&A...534A..58P. S2CID 15088852. arXiv:1108.3447 . doi:10.1051/0004-6361/201117055. 
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