利用者:GeeKay/sandbox2
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一覧
[編集]色がついた惑星は以下の凡例で示す。
凡例
[編集]惑星の種類 | |
---|---|
周連星惑星 | |
連星系の中の恒星を公転している惑星 | |
Kepler community planet | |
* | トランジット法以外の手法で発見された惑星 |
一覧
[編集]惑星名 | KOI | 質量 | 半径 | 平衡温度 (K) |
公転周期 (日) |
軌道長半径 (au) |
軌道離心率 | 軌道傾斜角 (°) |
主星名 | 距離 (pc) |
発見年 | 出典 | ||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
(MJ) | (M⊕) | (RJ) | (R⊕) | |||||||||||
ケプラー1b(TrES-2b) | 1.01 | 1.199 | 381.066 | 1.272 | 14.258 | 1495 | 2.47063 | 0.03556 | 0 | 83.62 | ケプラー1A(TrES-1A) | 213 | 2006 | [1] |
ケプラー2b(HAT-P-7b) | 2.01 | 1.781 | 566.037 | 1.431 | 16.040 | 2470 | 2.20473506 | 0.0379 | 0 | 86.68 | ケプラー2(HAT-P-7) | 320 | 2008 | [2][3] |
ケプラー3b(HAT-P-11b) | 3.01 | 0.081 | 25.74 | 0.422 | 4.730 | 878 | 4.8878162 | 0.053 | 0.0198 | 88.5 | ケプラー3(HAT-P-11) | 38 | 2009 | [4] |
ケプラー4b | 7.01 | 0.077 | 24.47 | 0.357 | 4.002 | 1650 | 3.21346 | 0.0456 | 0.25[5] | 89.76 | ケプラー4 | 550 | 2010 | [6] |
ケプラー5b | 18.01 | 2.114 | 671.871 | 1.431 | 16.042 | 1868 | 3.548460 | 0.05064 | 0 | 86.3 | ケプラー5 | 923 | 2010 | [7] |
ケプラー6b | 17.01 | 0.669 | 212.622 | 1.323 | 14.831 | 1500 | 3.234723 | 0.04567 | 0 | 86.8 | ケプラー6 | 597 | 2010 | [8] |
ケプラー7b | 97.01 | 0.433 | 137.616 | 1.478 | 16.568 | 1540 | 4.885525 | 0.06067 | 0 | 86.5 | ケプラー7 | 947 | 2010 | [9] |
ケプラー8b | 10.01 | 0.603 | 191.645 | 1.419 | 15.907 | 1764 | 3.52254 | 0.0483 | 0 | 84.07 | ケプラー8 | 1053 | 2010 | [10] |
ケプラー9b | 377.01 | 0.137 | 43.4 | 0.740 | 8.29 | 19.23891 | 0.143 | 0.0609 | 88.982 | ケプラー9 | 614 | 2010 | [11] | |
ケプラー9c | 377.02 | 0.094 | 29.9 | 0.721 | 8.08 | 38.9853 | 0.227 | 0.06691 | 89.188 | ケプラー9 | 614 | 2010 | [11] | |
ケプラー9d | 377.03 | 0.146 | 1.64 | 2026 | 1.592851 | 0.0273 | ケプラー9 | 614 | 2010 | [12] | ||||
ケプラー10b | 72.01 | 0.010 | 3.33 | 0.131 | 1.47 | 2169 | 0.837495 | 0.01684 | 0 | 84.4 | ケプラー10 | 173 | 2011 | [13][14] |
ケプラー10c | 72.02 | 0.023 | 7.37[15] | 0.199 | 2.227 | 485 | 42.29485 | 0.2407 | 0.025[16] | 89.65 | ケプラー10 | 173 | 2011 | [17] |
ケプラー11b | 157.06 | 0.006 | 1.9 | 0.161 | 1.80 | 10.3039 | 0.091 | 0.045 | 89.64 | ケプラー11 | 659 | 2011 | [18] | |
ケプラー11c | 157.01 | 0.009 | 2.9 | 0.256 | 2.87 | 13.0241 | 0.107 | 0.026 | 89.59 | ケプラー11 | 659 | 2011 | [18] | |
ケプラー11d | 157.02 | 0.023 | 7.3 | 0.278 | 3.12 | 22.6845 | 0.155 | 0.004 | 89.67 | ケプラー11 | 659 | 2011 | [18] | |
ケプラー11e | 157.03 | 0.025 | 8.0 | 0.374 | 4.19 | 31.9996 | 0.195 | 0.012 | 88.89 | ケプラー11 | 659 | 2011 | [18] | |
ケプラー11f | 157.04 | 0.006 | 2.0 | 0.222 | 2.49 | 46.6887 | 0.250 | 0.013 | 89.47 | ケプラー11 | 659 | 2011 | [18] | |
ケプラー11g | 157.05 | <0.079 | <25 | 0.297 | 3.33 | 118.3809 | 0.466 | <0.15 | 89.87 | ケプラー11 | 659 | 2011 | [18] | |
ケプラー12b | 20.01 | 0.431 | 136.98 | 1.695 | 18.98 | 1338 | 4.4379637 | 0.0556 | <0.01 | 88.76 | ケプラー12 | 600 | 2011 | [19] |
ケプラー13b | 13.01 | 9.28 | 2949.37 | 1.512 | 16.93 | 2750 | 1.763588 | 0.03641 | 0.00064 | 86.77 | ケプラー13A | 530 | 2011 | [20] |
ケプラー14b | 98.01 | 8.40 | 2669.66 | 1.136 | 12.733 | 1445 | 6.790123 | 0.078 | 0.035 | 90.0 | ケプラー14A | 980 | 2011 | [21] |
ケプラー15b | 128.01 | 0.66 | 209.76 | 0.96 | 10.76 | 1008 | 4.942782 | 0.05714 | 0.06 | 87.44 | ケプラー15 | 755 | 2011 | [22] |
ケプラー16b | 1611.02 | 0.333 | 105.83 | 0.754 | 8.449 | 228.776 | 0.7048 | 0.0069 | 90.0322 | ケプラー16 | 75 | 2011 | [23][24] | |
ケプラー17b | 203.01 | 2.45 | 778.66 | 1.31 | 14.69 | 1746 | 1.4857108 | 0.02591 | <0.011 | 87.2 | ケプラー17 | 800 | 2011 | [25] |
ケプラー18b | 137.03 | 0.022 | 6.9 | 0.178 | 2.00 | 3.504725 | 0.0447 | 0 | 84.92 | ケプラー18 | 439 | 2011 | [26] | |
ケプラー18c | 137.01 | 0.054 | 17.3 | 0.49 | 5.49 | 7.64159 | 0.0752 | 0 | 87.68 | ケプラー18 | 439 | 2011 | [26] | |
ケプラー18d | 137.02 | 0.052 | 16.4 | 0.623 | 6.98 | 14.85888 | 0.1172 | 0 | 88.07 | ケプラー18 | 439 | 2011 | [26] | |
ケプラー19b | 84.01 | 0.026 | 8.4 | 0.197 | 2.209 | 9.28716 | 0.0846[27] | 0.12 | 89.94 | ケプラー19 | 2119 | 2011 | [28][29] | |
ケプラー19c* | — | 0.041 | 13.1 | 28.731 | 0.21 | ケプラー19 | 2119 | 2011 | [29] | |||||
ケプラー19d* | — | 0.071 | 22.5 | 62.95 | 0.05 | ケプラー19 | 2119 | 2011 | [29] | |||||
ケプラー20b | 70.02 | 0.031 | 9.70 | 0.167 | 1.868 | 1105 | 3.69611525 | 0.0463 | 0.03 | 87.355 | ケプラー20 | 290 | 2011 | [30][31] |
ケプラー20c | 70.01 | 0.040 | 12.75 | 0.272 | 3.047 | 772 | 10.85409089 | 0.0949 | 0.16 | 89.815 | ケプラー20 | 290 | 2011 | [30][31] |
ケプラー20d | 70.03 | 0.032 | 10.07 | 0.245 | 2.744 | 401 | 77.61130017 | 0.3506 | <0.6 | 89.708 | ケプラー20 | 290 | 2011 | [30][31] |
ケプラー20e | 70.04 | <0.010 | <3.08 | 0.077 | 0.865 | 1040 | 6.09852281 | 0.0639 | <0.28 | 87.632 | ケプラー20 | 290 | 2011 | [30][31] |
ケプラー20f | 70.05 | <0.045 | <14.3 | 0.090 | 1.003 | 705 | 19.57758478 | 0.1396 | <0.32 | 88.788 | ケプラー20 | 290 | 2011 | [30][31] |
ケプラー20g* | — | ≥0.063 | ≥19.96 | 34.940 | 0.2055 | 0.15 | ケプラー20 | 290 | 2016 | [31] | ||||
ケプラー21b | 975.01 | 0.016 | 5.08 | 0.146 | 1.639 | 2025 | 2.7858212 | 0.04285 | 0.02 | 83.20 | ケプラー21 | 109 | 2011 | [32] |
ケプラー22b | 87.01 | <0.113 | <36 | 0.212 | 2.38 | 262 | 289.8623 | 0.849 | 89.764 | ケプラー22 | 190 | 2011 | [33] | |
ケプラー23b | 168.03 | 0.048 | 15.2[34] | 0.17 | 1.9 | 7.1073 | 0.075 | ケプラー23 | 800 | 2011 | [35][36] | |||
ケプラー23c | 168.01 | 0.189 | 60.2[34] | 0.285 | 3.2 | 10.7421 | 0.099 | ケプラー23 | 800 | 2011 | [35][36] | |||
ケプラー23d | 168.02 | 0.055 | 17.6[34] | 0.16 | 2.20 | 15.274299 | 0.125 | ケプラー23 | 800 | 2014 | [35][36] | |||
ケプラー24b | 1102.02 | 0.105 | 33.3[34] | 0.214 | 2.4 | 8.1453 | 0.08 | ケプラー24 | 1200 | 2011 | [35][36] | |||
ケプラー24c | 1102.01 | 0.106 | 33.6[34] | 0.25 | 2.8 | 12.3335 | 0.106 | ケプラー24 | 1200 | 2011 | [35][36] | |||
ケプラー24d | 1102.04 | 0.149 | 1.67 | 4.244384 | 0.052 | ケプラー24 | 1200 | 2014 | [35][36] | |||||
ケプラー24e | 1102.03 | 0.248 | 2.78 | 18.998355 | 0.141 | ケプラー24 | 1200 | 2014 | [35][36] | |||||
ケプラー25b | 244.02 | 0.027 | 8.7 | 0.245 | 2.748 | 6.238297 | 0.068 | 0.0029 | 92.827 | ケプラー25A | 245 | 2012 | [37][38] | |
ケプラー25c | 244.01 | 0.048 | 15.2 | 0.465 | 5.217 | 12.7207 | 0.110 | 0.0061 | 92.764 | ケプラー25A | 245 | 2012 | [37][38] | |
ケプラー25d* | 244.10 | 0.226 | 71.9 | 122.4 | 0.13 | ケプラー25A | 245 | 2014 | [38] | |||||
ケプラー26b | 250.01 | 0.016 | 5.12 | 0.248 | 2.78 | 12.2829 | 0.085 | ケプラー26 | 339 | 2012 | [37][39] | |||
ケプラー26c | 250.02 | 0.020 | 6.20 | 0.243 | 2.72 | 17.2513 | 0.107 | ケプラー26 | 339 | 2012 | [37][39] | |||
ケプラー26d | 250.03 | 0.096 | 1.07 | 3.543919 | 0.039 | ケプラー26 | 339 | 2012 | [36] | |||||
ケプラー26e | 250.04 | 0.215 | 2.41 | 46.827915 | 0.220 | ケプラー26 | 339 | 2012 | [36] | |||||
ケプラー27b | 841.01 | 0.132 | 41.952 | 0.357 | 4.0 | 610 | 15.3348 | 0.118 | ケプラー27 | 1080 | 2012 | [37][40] | ||
ケプラー27c | 841.02 | 0.067 | 21.294 | 0.438 | 4.9 | 481 | 31.3309 | 0.191 | ケプラー27 | 1080 | 2012 | [37][40] | ||
ケプラー28b | 870.01 | 0.028 | 8.8[34] | 0.321 | 3.6 | 5.9123 | 0.062 | ケプラー28 | 444 | 2012 | [37] | |||
ケプラー28c | 870.02 | 0.034 | 10.9[34] | 0.303 | 3.4 | 8.9858 | 0.081 | ケプラー28 | 444 | 2012 | [37] | |||
ケプラー29b | 738.01 | 0.016 | 5.0 | 0.227 | 2.55 | 10.33974 | 0.09[41] | 0 | 89.13 | ケプラー29 | 850 | 2012 | [42] | |
ケプラー29c | 738.02 | 0.014 | 4.5 | 0.209 | 2.34 | 13.28613 | 0.11[41] | ケプラー29 | 850 | 2012 | [42] | |||
ケプラー30b | 806.03 | 0.029 | 9.2 | 0.335 | 3.75 | 29.2187 | 0.18479 | 0.0770 | 89.51 | ケプラー30 | 940 | 2012 | [43] | |
ケプラー30c | 806.02 | 1.686 | 536 | 1.069 | 11.98 | 60.32503 | 0.29977 | 0.0115 | 89.74 | ケプラー30 | 940 | 2012 | [43] | |
ケプラー30d | 806.01 | 0.075 | 23.7 | 0.784 | 8.79 | 142.642 | 0.53178 | 0.0272 | 89.81 | ケプラー30 | 940 | 2012 | [43] | |
ケプラー31b | 935.01 | 0.491 | 5.5 | 20.8613 | 0.16 | ケプラー31 | 2100 | 2012 | [41] | |||||
ケプラー31c | 935.02 | 0.093 | 29.5[34] | 0.473 | 5.3 | 42.6318 | 0.26 | ケプラー31 | 2100 | 2012 | [41] | |||
ケプラー31d | 935.03 | 0.407 | 4.56 | 87.648901 | 0.39 | ケプラー31 | 2100 | 2012 | [41][36] | |||||
ケプラー32b | 952.01 | 0.030 | 9.4[34] | 0.196 | 2.2 | 530[44] | 5.90124 | 0.05 | ケプラー32 | 327 | 2012 | [41] | ||
ケプラー32c | 952.02 | 0.024 | 7.7[34] | 0.178 | 2.0 | 470[44] | 8.7522 | 0.09 | ケプラー32 | 327 | 2012 | [41] | ||
ケプラー32d[注 1] | 952.03 | 0.241 | 2.7 | 340[44] | 22.7802 | 0.128 | ケプラー32 | 303 | 2012 | [41] | ||||
ケプラー32e[注 1] | 952.04 | 0.134 | 1.5 | 680[44] | 2.8960 | 0.033 | ケプラー32 | 327 | 2012 | [41] | ||||
ケプラー32f[注 1] | 952.05 | 0.072 | 0.82 | 1100[44] | 0.74296 | 0.013 | ケプラー32 | 327 | 2012 | [41] | ||||
ケプラー33b | 707.05 | 0.155 | 1.74 | 5.66793 | 0.0677 | 0 | 86.39 | ケプラー33 | 1250 | 2012 | [45] | |||
ケプラー33c | 707.04 | 0.285 | 3.20 | 13.17562 | 0.1189 | 0 | 88.19 | ケプラー33 | 1250 | 2012 | [45] | |||
ケプラー33d | 707.01 | 0.014 | 4.3 | 0.477 | 5.35 | 21.77596 | 0.1626 | 0 | 88.71 | ケプラー33 | 1250 | 2012 | [45][46] | |
ケプラー33e | 707.03 | 0.019 | 6.1 | 0.359 | 4.02 | 31.78440 | 0.2092 | 0 | 88.94 | ケプラー33 | 1250 | 2012 | [45][46] | |
ケプラー33f | 707.02 | 0.034 | 10.6 | 0.398 | 4.46 | 41.02902 | 0.2480 | 0 | 89.17 | ケプラー33 | 1250 | 2012 | [45][46] | |
ケプラー34b | 2459.02 | 0.220 | 69.920 | 0.764 | 8.564 | 288.822 | 1.0896 | 0.182 | 90.355 | ケプラー34 | 1499 | 2012 | [47] | |
ケプラー35b | 2937.02 | 0.127 | 40.363 | 0.728 | 8.161 | 131.458 | 0.60347 | 0.042 | 90.76 | ケプラー35 | 1645 | 2012 | [47] |
脚注
[編集]注釈
[編集]- ^ a b c 太陽系外惑星エンサイクロペディアでは現況は「Candidate(候補)」扱いになっている。
出典
[編集]- ^ Daemgen, S.; Hormuth, F.; Brandner, W.; Bergfors, C.; Janson, M.; Hippler, S.; Henning, T. (2009). “Binarity of transit host stars — Implications for planetary parameters” (PDF). Astronomy and Astrophysics 498 (2): 567–574. arXiv:0902.2179. Bibcode: 2009A&A...498..567D. doi:10.1051/0004-6361/200810988 .
- ^ Pal, A. et al. (2008). “HAT-P-7b: An Extremely Hot Massive Planet Transiting a Bright Star in the Kepler Field”. The Astrophysical Journal 680 (2): 1450-1456 .
- ^ V. VanEylen; H. Kjeldsen; J. Christensen-Dalsgaard; C. Aerts (23 May 2014). "Properties of extrasolar planets and their host stars – a case study of HAT-P-7". arXiv:1301.1472v2 [astro-ph.EP]。
- ^ Bakos, G. Á.; Torres, G.; Pál, A.; Hartman, J.; Kovács, Géza; Noyes, R. W.; Latham, D. W.; Sasselov, D. D. et al. (2010). “HAT-P-11b: A Super-Neptune Planet Transiting a Bright K Star in the Kepler Field”. The Astrophysical Journal 710 (2): 1724–1745. arXiv:0901.0282. Bibcode: 2010ApJ...710.1724B. doi:10.1088/0004-637X/710/2/1724 .
- ^ Kipping, David; Bakos, Gáspár (2011). “An Independent Analysis of Kepler-4b through Kepler-8b”. The Astrophysical Journal 730 (1): 50. arXiv:1004.3538. Bibcode: 2011ApJ...730...50K. doi:10.1088/0004-637X/730/1/50 .
- ^ William J. Borucki; et al. (4 January 2010). "Kepler-4b: Hot Neptune-Like Planet of a G0 Star Near Main-Sequence Turnoff". arXiv:1001.0604v1 [astro-ph.EP]。
- ^ Koch, David G.; Borucki, William J. et al. (2010). “Discovery of the Transiting Planet Kepler-5b”. The Astrophysical Journal 713 (2): L131–L135. arXiv:1001.0913. Bibcode: 2010ApJ...713L.131K. doi:10.1088/2041-8205/713/2/L131. ISSN 2041-8205.
- ^ Dunham, Edward W.; Borucki, William J. et al. (2010). “Kepler-6b: A Transiting Hot Jupiter Orbiting a Metal-rich Star”. The Astrophysical Journal 713 (2): L136–L139. arXiv:1001.0333. Bibcode: 2010ApJ...713L.136D. doi:10.1088/2041-8205/713/2/L136. ISSN 2041-8205.
- ^ Latham, David W.; Borucki, William J. et al. (2010). “Kepler-7b: A Transiting Planet with Unusually Low Density”. The Astrophysical Journal 713 (2): L140–L144. arXiv:1001.0190. Bibcode: 2010ApJ...713L.140L. doi:10.1088/2041-8205/713/2/L140. ISSN 2041-8205.
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- ^ Torres, Guillermo; Fressin, François et al. (2011). “Modeling Kepler Transit Light Curves as False Positives: Rejection of Blend Scenarios for Kepler-9, and Validation of Kepler-9 d, A Super-earth-size Planet in a Multiple System”. The Astrophysical Journal 727 (1): 24. arXiv:1008.4393. Bibcode: 2011ApJ...727...24T. doi:10.1088/0004-637X/727/1/24.
- ^ Dumusque, Xavier; Bonomo, Aldo S.; Haywood, Raphaëlle D. et al. (2014). “The Kepler-10 planetary system revisited by HARPS-N: A hot rocky world and a solid Neptune-mass planet”. The Astrophysical Journal 789 (2): 14. arXiv:1405.7881. Bibcode: 2014ApJ...789..154D. doi:10.1088/0004-637X/789/2/154 .
- ^ Batalha, N. M.; et al. (2011). “Kepler's First Rocky Planet: Kepler-10b”. The Astrophysical Journal 729: 27. arXiv:1102.0605. Bibcode: 2011ApJ...729...27B. doi:10.1088/0004-637X/729/1/27.
- ^ Rajpaul, V.; Buchhave, L. A.; Aigrain, S. (2017). “Pinning down the mass of Kepler-10c: the importance of sampling and model comparison”. Monthly Notices of the Royal Astronomical Society: Letters 471 (1): L125-L130. arXiv:1707.06192. Bibcode: 2017MNRAS.471L.125R. doi:10.1093/mnrasl/slx116.
- ^ Fogtmann-Schulz, Alexandra; Hinrup, Brian; Van Eylen, Vincent (2014). “Accurate Parameters of the Oldest Known Rocky-exoplanet Hosting System: Kepler-10 Revisited”. The Astrophysical Journal 781 (2): 8. arXiv:1311.6336. Bibcode: 2014ApJ...781...67F. doi:10.1088/0004-637X/781/2/67.
- ^ Fressin, Francoi; Torres, Guillermo et al. (2011). “Kepler-10 c: a 2.2 Earth Radius Transiting Planet in a Multiple System”. The Astrophysical Journal Supplement 197 (1): 12. arXiv:1105.4647. Bibcode: 2011ApJS..197....5F. doi:10.1088/0067-0049/197/1/5.
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- ^ Fortney, Jonathan J.; Demory, Brice-Olivier; Désert, Jean-Michel (2011). “Discovery and Atmospheric Characterization of Giant Planet Kepler-12b: An Inflated Radius Outlier”. The Astrophysical Journal Supplement 197 (1): 12. arXiv:1109.1611. Bibcode: 2011ApJS..197....9F. doi:10.1088/0067-0049/197/1/9.
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- ^ a b c Cochran, William D.; Fabrycky, Daniel C. et al. (2011). “Kepler-18b, c, and d: A System of Three Planets Confirmed by Transit Timing Variations, Light Curve Validation, Warm-Spitzer Photometry, and Radial Velocity Measurements”. The Astrophysical Journal Supplement 197 (1): 19. arXiv:1110.0820. Bibcode: 2011ApJS..197....7C. doi:10.1088/0067-0049/197/1/7.
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