Lista de exoplanetas descobertos em 2017
Esta é uma Lista de exoplanetas descobertos em 2017.
Para exoplanetas detectados apenas pela velocidade radial, o valor da massa é na verdade um limite inferior. (Consulte a massa mínima para obter mais informações)
Nome | Massa (MJ) | Raio (RJ) | Período (dais) | Semieixo maior (AU) | Temp. (K)[1] | Método de descoberta | Distância (ly) | Massa da estrela-mãe (M☉) | Temperatura da estrela-mãe (K) | Observações |
---|---|---|---|---|---|---|---|---|---|---|
BD+03 2562 b | 6.4 | 481.9 | 1.3 | Vel. radial | 8540 | 1.14 | 4095 | [2] | ||
CoRoT-30 b | 2.90±0.22 | 1.009±0.076 | 9.06005±0.00024 | 0.0844±0.0012 | Trânsito | 3100±200 | 0.98+0.03 −0.05 | 5650±100 | [3] | |
CoRoT-31 b | 0.84±0.34 | 1.46±0.30 | 4.62941±0.00075 | 0.0586±0.0034 | Trânsito | 7000±2000 | 1.25+0.22 −0.21 | 5700±120 | [3] | |
CoRoT-32 b | 0.15 | 0.57 | 6.71837 | 0.071 | 938 | Trânsito | 1.08 | 5970 | Estrela-mãe também conhecida como CoRoT 223977153[4] | |
Gliese 273 b | 0.00909 | 18.6498 | 0.091101 | 259 | Vel. radial | 12 | 0.29 | 3382 | Também conhecido como Luyten b, exoplaneta potencialmente habitável.[5] | |
Gliese 273 c | 0.00371 | 4.7234 | 0.036467 | Vel. radial | 12 | 0.29 | 3382 | [5] | ||
Gliese 625 b | 0.00887 | 14.628 | 0.078361 | Vel. radial | 21 | 0.30 | 3499 | [6] | ||
Gliese 1148 c | 0.2141 | 532.58 | 0.912 | Vel. radial | 35.98 | 0.357±0.013 | Estrela-mãe também conhecida como Ross 1003[7] | |||
Gliese 3138 b | 0.0056 | 1.22003 | 0.0197 | Vel. radial | 92.9 | 0.68 | 3717 | |||
Gliese 3138 c | 0.01315 | 5.974 | 0.057 | Vel. radial | 92.9 | 0.68 | 3717 | |||
Gliese 3138 d | 0.03304 | 257.8 | 0.698 | Vel. radial | 92.9 | 0.68 | 3717 | |||
Gliese 3293 d | 0.02391 | 48.1345 | 0.19394 | Vel. radial | 51.4 | 0.42 | 3466 | |||
Gliese 3293 e | 0.01032 | 13.2543 | 0.08208 | Vel. radial | 51.4 | 0.42 | 3466 | |||
Gliese 3323 b | 0.00636 | 5.3636 | 0.03282 | Vel. radial | 17.4 | 0.16 | 3159 | |||
Gliese 3323 c | 0.00727 | 40.54 | 0.1264 | Vel. radial | 17.4 | 0.16 | 3159 | |||
Gliese 3942 b | 0.0225 | 6.905 | 0.0608 | 590 | Vel. radial | 55.3 | 0.63 | 3867 | [8] | |
HAT-P-67b | 0.34 | 2.085 | 4.81010250 | 0.06505 | Trânsito | 1000 | 1.642 | 6406 | [9] | |
HATS-36b | 2.79±0.40 | 1.263±0.045 | 4.1752379±0.0000021 | 0.0529±0.0011 | 1363±40 | Trânsito | 2860±70 | 1.135±0.067 | 5970±160 | Estrela-mãe também conhecida como K2-145[10] |
HATS-43b | 0.261±0.054 | 1.180±0.050 | 4.3888497 | 0.04944±0.00046 | 1003±27 | Trânsito | 1194.1±7.4 | 0.837±0.023 | 5099±61 | [11] |
HATS-44b | 0.56±0.11 | 1.067+0.125 −0.071 | 2.7439004 | 0.03649±0.00030 | 1161±34 | Trânsito | 1474±11 | 0.860±0.021 | 5080±100 | [11] |
HATS-45b | 0.70±0.15 | 1.286±0.093 | 4.1876244 | 0.05511±0.00069 | 1518±45 | Trânsito | 2575±38 | 1.272±0.048 | 6450±110 | [11] |
HATS-46b | 0.173±0.062 | 0.903+0.058 −0.045 | 4.7423729 | 0.05367±0.00053 | 1054±29 | Trânsito | 1500±13 | 0.917±0.027 | 5495±69 | [11] |
HATS-50b | 0.39 | 1.130 | 3.8297015 | 0.05046 | Trânsito | 2340 | 1.17 | 5990 | [12] | |
HATS-51b | 0.768 | 1.41 | 3.3488702 | 0.04639 | 1553 | Trânsito | 1560 | 1.17 | 5758 | |
HATS-52b | 2.24 | 1.382 | 1.36665436 | 0.02498 | 1834 | Trânsito | 2060 | 1.11 | 6010 | |
HATS-53b | 0.595 | 1.340 | 3.8537768 | 0.04753 | 1312 | Trânsito | 2000 | 0.96 | 5644 | |
HD 3167 d | 0.0217 | 8.509 | 0.07757 | Vel. radial | 149 | 0.86 | 5261 | [13] | ||
HD 17674 b | 0.87 | 623.8 | 1.42 | Vel. radial | 145 | 0.98 | 5904 | [14] | ||
HD 20781 d | 0.0061+0.0012 −0.0011 | 0.2052 | 5.3135±0.001 | 0.0529+0.0024 −0.0027 | radial vel. | 115.36±4.4 | 0.7 | 5256±29 | [15] | |
HD 20781 e | 0.0168+0.0022 −0.0021 | 0.2183 | 13.8905+0.0033 −0.0034 | 0.1004+0.0046 −0.0051 | radial vel. | 115.36±4.4 | 0.7 | 5256±29 | [15] | |
HD 20794 e | 0.0150 | 147.02 | 0.509 | Vel. radial | 19.8 | 0.7 | 5401 | [16] | ||
HD 27894 c | 0.162 | 36.07 | 0.198 | Vel. radial | 138.2 | 0.8 | 4875 | [17] | ||
HD 27894 d | 5.415 | 5174 | 5.448 | Vel. radial | 138.2 | 0.8 | 4875 | [17] | ||
HD 29021 b | 2.4 | 1362.3 | 2.28 | Vel. radial | 100 | 0.85 | 5560 | [14] | ||
HD 34445 c | 0.168 | 214.67 | 0.7181 | Vel. radial | 146.8 | 1.07 | 5836 | [18] Likely a false positive[19] | ||
HD 34445 d | 0.0970 | 117.87 | 0.4817 | Vel. radial | 146.8 | 1.07 | 5836 | [18] Provavelmente um falso positivo[19] | ||
HD 34445 e | 0.0529 | 49.175 | 0.2687 | Vel. radial | 146.8 | 1.07 | 5836 | [18] Provavelmente um falso positivo[19] | ||
HD 34445 f | 0.119 | 676.8 | 1.543 | Vel. radial | 146.8 | 1.07 | 5836 | [18] Provavelmente um falso positivo[19] | ||
HD 34445 g | 0.38 | 5700 | 6.36 | Vel. radial | 146.8 | 1.07 | 5836 | [18] Provavelmente um falso positivo[19] | ||
HD 40956 b | 2.7 | 578.6 | 1.4 | Vel. radial | 385 | 2.00 | 4869 | [20] | ||
HD 42012 b | 1.6 | 857.5 | 1.67 | Vel. radial | 121 | 0.83 | 5405 | [14] | ||
HD 45184 c | 0.0277+0.0034 −0.0032 | 13.1354+0.0026 −0.0025 | 0.11+0.0034 −0.0036 | radial vel. | 71.36±0.62 | 1.03 | 5869±14 | [21] | ||
HD 76920 b | 3.93 | 415.891+0.043 −0.039 | 1.149 | Vel. radial | 602.7 | 1.17 | 4698 | Órbita extremamente excêntrica em torno de uma gigante vermelha evoluída[22][23][24] | ||
HD 93385 Ab | 0.0125±0.0015 | 7.3422±0.0014 | 0.0749±0.0017 | 1129±19 | Vel. radial | 141.6±0.2 | 1.04±0.01 | 5823±35 | [21] Confirmado em 2021, renomeado de HD 93385 d[25] | |
HD 106315 b | 0.0255 | 0.207 | 9.55804 | 0.0905 | 1046 | Trânsito | 358 | 1.08 | 6277 | Estrela-mãe também conhecida como K2-109[26] |
HD 106315 c | 0.0560 | 0.385 | 21.05788 | 0.1533 | 804 | Trânsito | 358 | 1.08 | 6277 | Estrela-mãe também conhecida como K2-109[26] |
HD 111591 b | 4.4 | 1056.4 | 2.5 | Vel. radial | 352 | 1.94 | 4884 | [20] | ||
HD 113996 b | 6.3 | 610.2 | 1.6 | Vel. radial | 331.4 | 1.49 | 4181 | [20] | ||
HD 147379 b | 0.0777 | 86.54 | 0.3193 | Vel. radial | 35.01 | 0.58 | 4090 | [27] | ||
HD 176986 b | 0.0181 | 6.48980 | 0.06296 | Vel. radial | 86.1 | 0.79 | 4931 | [28] | ||
HD 176986 c | 0.02888 | 16.8191 | 0.11878 | Vel. radial | 86.1 | 0.79 | 4931 | [28] | ||
HD 177565 b | 0.04751 | 44.505 | 0.246 | Vel. radial | 56 | 1.0 | [29] | |||
HD 208897 b | 1.40 | 352.7 | 1.05 | Vel. radial | 211 | 1.25 | 4860 | [30] | ||
HIP 65426 b | 9.0 | 92 | 1450 | Imagem direto | 363 | 1.96 | 8840 | Estrela-mãe também conhecida como HD 116434[31] | ||
K2-18c | 0.0236 | 8.962 | 0.060 | 363 | Vel. radial | 110 | 0.36 | 3547 | [32] | |
K2-105b | 0.09439 | 0.369 | 8.266902 | 0.081 | Trânsito | 760 | 1.01 | 5434 | [33] | |
K2-106b | 0.0263 | 0.136 | 0.571292 | 0.0116 | 2333 | Trânsito | 798 | 0.95 | 5470 | [34] Estrela-mãe também conhecida como EPIC 220674823 |
K2-106c | 0.226 | 13.341245 | Trânsito | 830 | 0.93 | 5590 | [34] Estrela-mãe também conhecida como EPIC 220674823 | |||
K2-108b | 0.18689 | 0.471 | 4.73401 | 0.0573 | 1446 | Trânsito | 1530 | 1.12 | 5474 | [35] |
K2-111b | 0.0271 | 0.17 | 5.35117 | 0.0621 | 1309 | Trânsito | 680 | 0.88 | 5730 | [36] |
K2-114b | 1.85 | 0.942 | 11.39109 | 0.09309 | 719 | Trânsito | 1570 | 0.83 | 5027 | [37] |
K2-115b | 0.84 | 1.115 | 20.273034 | 0.1367 | 682 | Trânsito | 1360 | 0.83 | 5560 | [37] |
K2-116b | 0.062 | 4.655411 | 0.048 | Trânsito | 183.1 | 0.69 | 4348 | [38] Estrela-mãe também conhecida como BD-12 6259 | ||
K2-117b | 0.175 | 1.291505 | 0.019 | Trânsito | 333.5 | 0.58 | 3842 | [39] | ||
K2-117c | 0.181 | 5.444820 | 0.051 | Trânsito | 333.5 | 0.58 | 3842 | [39] | ||
K2-118b | 0.227 | 50.92092 | 0.245 | Trânsito | 1057 | 0.76 | 4726 | [38] | ||
K2-119b | 0.204 | 7.728578 | 0.070 | Trânsito | 1180 | 0.76 | 4753 | [38] | ||
K2-120b | 0.179 | 9.562742 | 0.078 | Trânsito | 950 | 0.69 | 4350 | [38] | ||
K2-121b | 0.814 | 5.185754 | 0.052 | Trânsito | 552 | 0.71 | 4471 | [38] | ||
K2-122b | 0.114 | 2.219405 | 0.029 | Trânsito | 236 | 0.63 | 3993 | [38][39] | ||
K2-123b | 0.236 | 30.956763 | 0.167 | Trânsito | 529 | 0.65 | 4076 | [38][39] | ||
K2-124b | 0.236 | 6.413539 | 0.051 | Trânsito | 448 | 0.44 | 3561 | [38] | ||
K2-125b | 0.194 | 21.750264 | 0.121 | Trânsito | 415 | 0.49 | 3654 | [38] | ||
K2-126b | 0.164 | 7.387073 | 0.066 | Trânsito | 332 | 0.70 | 4368 | [38] | ||
K2-127b | 0.773 | 3.588165 | 0.041 | Trânsito | 2370 | 0.70 | 4388 | [38] | ||
K2-128b | 0.127 | 5.675819 | 0.056 | Trânsito | 373 | 0.71 | 4470 | [38] | ||
K2-129b | 0.0928 | 8.239493 | 0.057 | Trânsito | 90.19±0.07 | 0.36 | 3459 | [38] Estrela-mãe também conhecida como LP 868-19 | ||
K2-130b | 0.112 | 2.494120 | 0.032 | Trânsito | 384.4±0.6 | 0.70 | 4356 | [38] | ||
K2-131b | 0.017 | 0.152 | 0.36931 | 0.009500 | 2062 | Trânsito | 501 | 0.84 | 5245 | [40] |
K2-132b | 1.30 | 9.1751 | Trânsito | 568 | 1.08±0.08 | 4840±90 | [41] | |||
K2-133b | 0.117 | 3.0712 | 0.033 | Trânsito | 245.3±0.7 | 0.46±0.01 | 3655±80 | Estrela-mãe também conhecida como LP 358-499, 4 planetas no sistema[42] | ||
K2-133c | 0.132 | 4.8682 | 0.045 | Trânsito | 245.3±0.7 | 0.46±0.01 | 3655±80 | Estrela-mãe também conhecida como LP 358-499, 4 planetas no sistema[42] | ||
K2-135b | 0.180 | 11.0234 | 0.077 | Trânsito | 245.3±0.7 | 0.46±0.01 | 3655±80 | Estrela-mãe também conhecida como LP 358-499, 4 planetas no sistema[42] | ||
K2-135b | 0.156 | 1.208957 | 0.020 | 1043.5 | Trânsito | 98.8 | 0.66 | 4255 | [43] | |
K2-135c | 0.121 | 3.64802 | 0.042 | 721.9 | Trânsito | 98.8 | 0.66 | 4255 | [43] | |
K2-135d | 0.187 | 6.20141 | 0.060 | 604.9 | Trânsito | 98.8 | 0.66 | 4255 | [43] | |
K2-136b | 0.0883 | 7.975292 | 553 | Trânsito | 0.74 | 4499 | [44] | |||
K2-136c | 0.057±0.006 | 0.260 | 17.307137 | 0.11728 | 425 | Trânsito | 0.74 | 4499 | [44][45] | |
K2-136d | 0.129 | 25.575065 | 373 | Trânsito | 0.74 | 4499 | [44] | |||
K2-137b | 0.5 | 0.079 | 0.179715 | 0.0058 | 1471 | Trânsito | 0.46 | 3492 | [46] | |
K2-139b | 0.387 | 0.808 | 28.38236 | 0.179 | 565 | Trânsito | 496 | 1.8 | 5340 | [47] |
K2-140b | 0.211 | 1.093 | 6.56918 | 0.0687 | 957 | Trânsito | 1110 | 1.00 | 5705 | [48] |
K2-141b | 0.0160±0.0013 | 0.135±0.004 | 0.2803226 | 0.00716+0.00055 −0.00065 | 2039+87 −48 | Trânsito | 202.16±0.54 | 0.708±0.028 | 4599±79 | [49][50] |
K2-146b | 0.196±0.021 | 2.644646 | 0.0266±0.0010 | Trânsito | 259.2±1.5 | 0.358±0.042 | 3385±70 | [39] | ||
K2-147b | 0.123+0.015 −0.013 | 0.961917 | 0.0159±0.0005 | Trânsito | 296.10±0.90 | 0.583±0.059 | 3672±70 | [39] Também chamado de EPIC 213715787[51] | ||
K2-148b | 0.119+0.017 −0.016 | 4.38395±0.00080 | 0.0454±0.0014 | Trânsito | 407.4±2.0 | 0.650±0.061 | 4079±70 | [39] | ||
K2-148c | 0.154+0.021 −0.019 | 6.92260±0.00070 | 0.0616±0.0019 | Trânsito | 407.4±2.0 | 0.650±0.061 | 4079±70 | [39] | ||
K2-148d | 0.146+0.021 −0.019 | 9.7579±0.0010 | 0.0774±0.0024 | Trânsito | 407.4±2.0 | 0.650±0.061 | 4079±70 | [39] | ||
K2-149b | 0.146+0.018 −0.016 | 11.3320±0.0013 | 0.0830±0.0027 | Trânsito | 404.8±1.8 | 0.595±0.059 | 3745±70 | [39] | ||
K2-150b | 0.178+0.024 −0.019 | 10.59357±0.00084 | 0.0727±0.0027 | Trânsito | 335.2±2.6 | 0.457±0.051 | 3499±70 | [39] | ||
K2-151b | 0.120+0.014 −0.012 | 3.835592 | 0.0365±0.0014 | Trânsito | 227.07±0.49 | 0.440±0.050 | 3585±70 | [39] | ||
K2-152b | 0.204+0.022 −0.021 | 32.6527±0.0035 | 0.1716±0.0012 | 337±3 | Trânsito | 354.8±1.3 | 0.63±0.01 | 4044+34 −35 | [39] | |
K2-153b | 0.178+0.019 −0.016 | 7.51554 | 0.0614±0.0004 | 497±6 | Trânsito | 468.7±3.0 | 0.55±0.01 | 3845±37 | [39] | |
K2-154b | 0.178+0.019 −0.010 | 3.67635 | 0.0405±0.0003 | 715+9 −8 | Trânsito | 423.5±1.5 | 0.65+0.02 −0.01 | 4097+40 −45 | [39] | |
K2-154c | 0.185+0.016 −0.012 | 7.95478 | 0.0677±0.0005 | 552±7 | Trânsito | 423.5±1.5 | 0.65+0.02 −0.01 | 4097+40 −45 | [39] | |
KELT-9b | 2.88 | 1.891 | 1.4811235 | 0.03462 | 4050 | Trânsito | 615.5 | 2.52 | 10170 | Exoplaneta mais quente confirmado[52] |
KELT-18b | 1.18 | 1.570 | 2.8717518 | 0.04550 | 2085 | Trânsito | 1.52 | 6670 | [53] | |
KELT-19Ab | <4.07 | 1.91 | 4.6117093 | 0.0637 | 1935 | Trânsito | 950 | 1.62 | 7500 | [54] |
KELT-20b | 1.741 | 3.4741085 | 0.0542 | 2262 | Trânsito | 455.6 | 1.76 | 8720 | [55] Também conhecido como MASCARA-2b[56] | |
KELT-21b | 3.91+0 −3.91 | 1.586+0.039 −0.040 | 3.6127647 | 0.05224+0.00035 −0.00034 | 2051+29 −30 | Trânsito | 1557±21 | 1.458+0.029 −0.028 | 7598+81 −84 | [57] |
Kepler-19d | 0.0708 | 62.95 | Vel. radial | 6910 | 0.94 | 5541 | [58] | |||
Kepler-80g | 0.101 | 14.64558 | 418 | Trânsito | 1160 | 0.73 | 4540 | [59] | ||
Kepler-90i | 0.118 | 14.44912 | 709 | Trânsito | 2540 | 1.2 | 6080 | [59] | ||
Kepler-150f | 0.325 | 637.2093 | 1.24 | Trânsito | 2980±50 | 5560 | [60] | |||
Kepler-1649b | 0.0964 | 8.689090 | 0.0514 | Trânsito | 0.22 | 3240 | [61] | |||
Kepler-1650b | 0.0856 | 1.53818001 | Trânsito | 393 | 0.33 | 3410 | [62] | |||
Kepler-1651b | 0.164 | 9.87863917 | Trânsito | 226 | 0.52 | 3713 | [62] | |||
Kepler-1652b | 0.143 | 38.09722 | 0.1654 | 268 | Trânsito | 822 | 0.40 | 3638 | [63] | |
Kepler-1653b | 0.194 | 140.2524 | 0.4706 | 284 | Trânsito | 2460 | 0.72 | 4807 | [63] | |
LHS 1140 b | 0.0209 | 0.128 | 24.73712 | 0.0875 | 254 | Trânsito | 40.7 | 0.18 | 3216 | Exoplaneta potencialmente habitável[64] |
MASCARA-1b | 3.7 | 1.5 | 2.148780 | 0.043 | 2570 | Trânsito | 615.5 | 1.72 | 7554 | [65] |
MOA-2010-BLG-117Lb | 0.54±0.10 | 2369+835 −2717 | 2.9+1.6 −0.6 | Microlente | 11400±1300 | 0.58±0.11 | 4000+450 −350 | [66] | ||
MOA-2012-BLG-006Lb | 8.40 | 10.2 | Microlente | 17000 | 0.49 | [67] | ||||
MOA-2012-BLG-505Lb | 0.02108 | 0.900 | Microlente | 23500 | 0.10 | [68] | ||||
MOA-2016-BLG-227Lb | 2.8 | 1.67 | Microlente | 21000 | 0.29 | [69] | ||||
MXB 1658-298 b | 23.7 | 760 | 1.613 | Tempo | 1.98 | Planeta circumbinário[70] | ||||
NGTS-1b | 0.812 | 1.33 | 2.647298 | 0.0326 | 790 | Trânsito | 731 | 0.617 | 3916 | Maior exoplaneta em relação à sua estrela[71] |
OGLE-2013-BLG-0132Lb | 0.29 | 3.6 | Microlente | 13000 | 0.54 | [72] | ||||
OGLE-2013-BLG-1721Lb | 0.64 | 2.6 | Microlente | 21000 | 0.46 | [72] | ||||
OGLE-2013-BLG-1761Lb | 2.7+2.5 −1.5 | 1.8±0.5 | Microlente | 23000+3300 −3900 | 0.33+0.32 −0.19 | [73] | ||||
OGLE-2016-BLG-0263Lb | 4.10 | 5.4 | Microlente | 21000 | 0.13 | [74] | ||||
OGLE-2016-BLG-0613(AB)b | 4.18 | 6.40 | Microlente | 11100 | 0.72 | [75] | ||||
OGLE-2016-BLG-1190Lb | 13.38 | 1224 | 2.17 | Microlente | 22100 | 0.88 | Extremamente massivo; possível anã marrom[76] | |||
OGLE-2016-BLG-1195Lb | 0.031 | 2.62±0.28 | Microlente | 22000±2000 | 0.57±0.06 | [77] </ref>[78] | ||||
OGLE-2017-BLG-0173Lb | 0.0103+0.0121 −0.0063 | 4493+3090 −7055 | 3.9±1.6 | Microlente | 15700+4900 −5900 | 0.40+0.39 −0.23 | 3500+1500 −500 | Atypical lensing event[79] Not an OGLE-2011-BLG-0173Lb! | ||
PSR B0329+54 b | 0.00620 | 10140 | 10.26 | Tempo | 1600 | 1.44 | Duvidoso[80] | |||
PSR J2322-2650 b | 0.7949 | 0.322963997 | 0.0102 | Tempo | 750 | 1.4 | [81] | |||
Qatar-6b | 0.668 | 1.062 | 3.506195 | 0.0423 | Trânsito | 330 | 0.822 | 5052 | [82] | |
Ross 128 b | 0.00440 | 9.8658 | 0.0496 | 301 | Vel. radial | 11.03 | 0.17 | 3192 | [83] | |
SAND978 b | 2.18 | 511.21 | Vel. radial | 2051.3 | 1.37 | 4200 | [84] Red giant host star, belonging to M67, is also known as NGC 2682 108 Estrela-mãe gigante vermelha, pertencente a M67, também conhecida como NGC 2682 108 | |||
TAP 26 b | 1.66 | 10.79 | 0.0968 | Vel. radial | 480 | 1.04 | 4620 | Estrela-mãe também conhecida como V1069 Tauri[85] | ||
Tau Ceti g | 0.00551 | 20.00 | 0.133 | Vel. radial | 12 | 0.78 | [86] | |||
Tau Ceti h | 0.00576 | 49.41 | 0.243 | Vel. radial | 12 | 0.78 | [86] | |||
TRAPPIST-1e | 0.00195 | 0.082 | 6.099615 | 0.02817 | 251 | Trânsito | 39 | 0.08 | 2559 | Exoplaneta potencialmente habitável[87] |
TRAPPIST-1f | 0.00214 | 0.093 | 9.20669 | 0.0371 | 219 | Trânsito | 39 | 0.08 | 2559 | Exoplaneta potencialmente habitável[87] |
TRAPPIST-1g | 0.00422 | 0.101 | 12.35294 | 0.0451 | 199 | Trânsito | 39 | 0.08 | 2559 | Exoplaneta potencialmente habitável[87] |
TRAPPIST-1h | 0.067 | 20 | 0.063 | 168 | Trânsito | 39 | 0.08 | 2559 | [87] | |
TYC 4282-605-1 b | 10.78 | 101.54 | 0.422 | Vel. radial | 2300 | 0.97 | 4300 | [88] | ||
WASP-91b | 1.34 | 1.03 | 2.798581 | 0.037 | 1160 | Trânsito | 490 | 0.84 | 4920 | [89] |
WASP-105b | 1.8 | 0.96 | 7.87288 | 0.075 | 900 | Trânsito | 0.89 | 5070 | [89] | |
WASP-107b | 0.12 | 0.94 | 5.721490 | 0.055 | 770 | Trânsito | 0.69 | 4430 | [89] | |
WASP-151b | 0.31 | 1.13 | 4.533471 | 0.055 | 1290 | Trânsito | 1570 | 1.01 | 5871 | [90] Estrela-mãe também conhecida como K2-134 |
WASP-153b | 0.39 | 1.55 | 3.332609 | 0.048 | 1700 | Trânsito | 1400 | 1.34 | 5914 | [90] |
WASP-156b | 0.128 | 0.51 | 3.836169 | 0.0453 | 970 | Trânsito | 460 | 0.84 | 4910 | [90] Estrela-mãe também conhecida como TOI-465 |
WASP-167b | 1.58 | 2.0219596 | 0.0365 | 2329 | Trânsito | 1240 | 1.59 | 7000 | Estrela-mãe também conhecida como KELT-13[91] | |
YZ Ceti b | 0.0024 | 1.96876 | 0.01634+0.00035 −0.00041 | Vel. radial | 12.122±0.002 | 0.130±0.013 | 3056±60 | [92] | ||
YZ Ceti c | 0.00308 | 3.06008 | 0.02156+0.00046 −0.00054 | Vel. radial | 12.122±0.002 | 0.130±0.013 | 3056±60 | [92] | ||
YZ Ceti d | 0.00359 | 4.65627 | 0.02851+0.00061 −0.00071 | Vel. radial | 12.122±0.002 | 0.130±0.013 | 3056±60 | [92] |
Listas específicas de exoplanetas
[editar | editar código-fonte]- Listas de exoplanetas
- Lista de exoplanetas descobertos antes de 2000 (32)
- Lista de exoplanetas descobertos entre 2000-2009 (379)
- Lista de exoplanetas descobertos em 2010 (109)
- Lista de exoplanetas descobertos em 2011 (179)
- Lista de exoplanetas descobertos em 2012 (149)
- Lista de exoplanetas descobertos em 2013 (151)
- Lista de exoplanetas descobertos em 2014 (878)
- Lista de exoplanetas descobertos em 2015 (151)
- Lista de exoplanetas descobertos em 2016 (1.513)
- Lista de exoplanetas descobertos em 2017 (158)
- Lista de exoplanetas descobertos em 2018 (306)
- Lista de exoplanetas descobertos em 2019 (172)
- Lista de exoplanetas descobertos em 2020 (264)
- Lista de exoplanetas descobertos em 2021 (242)
- Lista de exoplanetas descobertos em 2022 (314)
- Lista de exoplanetas descobertos em 2023 (75)
- Lista de exoplanetas potencialmente habitáveis
- Lista de nomes próprios de exoplanetas
- Lista de sistemas multiplanetários
- Lista dos primeiros exoplanetas
- Lista de exoplanetas extremos
- Lista de exoplanetas descobertos usando a sonda Kepler
- Lista de exoplanetas observados durante a missão K2 do Kepler
- Lista de candidatos de exoplanetas para água líquida
- Lista dos exoplanetas mais próximos
- Lista de candidatos a exoplaneta terrestres mais próximos
- Lista de exoplanetas em trânsito
Referências
- ↑ «The Extrasolar Planets Encyclopaedia». Consultado em 9 de novembro de 2015
- ↑ Villaver, E; Niedzielski, A; Wolszczan, A; Nowak, G; Kowalik, K; Adamów, M; MacIejewski, G; Deka-Szymankiewicz, B; Maldonado, J (2017). «Tracking Advanced Planetary Systems (TAPAS) with HARPS-N». Astronomy & Astrophysics. 606: A38. Bibcode:2017A&A...606A..38V. arXiv:1706.01278. doi:10.1051/0004-6361/201730471
- ↑ a b «Transiting exoplanets from the CoRoT space mission XXIX. The hot Jupiters CoRoT-30 b and CoRoT-31 b». Consultado em 1 de setembro de 2021. Cópia arquivada em 6 de dezembro de 2021
- ↑ Boufleur, Rodrigo C.; Emilio, Marcelo; Janot-Pacheco, Eduardo; Andrade, Laerte; Ferraz-Mello, Sylvio; Do Nascimento Jr, José-Dias; de la Reza, Ramiro (2017), «A modified CoRoT detrend algorithm and the discovery of a new planetary companion», Monthly Notices of the Royal Astronomical Society, 473: 710–720, arXiv:1709.00351, doi:10.1093/mnras/stx2187
- ↑ a b Astudillo-Defru, Nicola; Forveille, Thierry; Bonfils, Xavier; Ségransan, Damien; Bouchy, François; Delfosse, Xavier; et al. (2017). «The HARPS search for southern extra-solar planets. XLI. A dozen planets around the M dwarfs GJ 3138, GJ 3323, GJ 273, GJ 628, and GJ 3293». Astronomy and Astrophysics. 602. A88. Bibcode:2017A&A...602A..88A. arXiv:1703.05386. doi:10.1051/0004-6361/201630153
- ↑ Suárez Mascareño, A.; et al. (2017). «HADES RV Programme with HARPS-N at TNG. V. A super-Earth on the inner edge of the habitable zone of the nearby M dwarf GJ 625». Astronomy and Astrophysics. 605. A92. Bibcode:2017A&A...605A..92S. arXiv:1705.06537. doi:10.1051/0004-6361/201730957
- ↑ Trifonov, T.; et al. (2018), «The CARMENES search for exoplanets around M dwarfs», Astronomy & Astrophysics, 609: A117, arXiv:1710.01595, doi:10.1051/0004-6361/201731442
- ↑ Perger, M.; et al. (2017), «HADES RV Programme with HARPS-N at TNG», Astronomy & Astrophysics, 608: A63, arXiv:1709.06851, doi:10.1051/0004-6361/201731307
- ↑ Zhou, G.; et al. (2017), «HAT-P-67b: An Extremely Low Density Saturn Transiting an F-subgiant Confirmed via Doppler Tomography», The Astronomical Journal, 153 (5): 211, arXiv:1702.00106, doi:10.3847/1538-3881/aa674a
- ↑ Bayliss, D.; Hartman, J. D.; Zhou, G.; Bakos, G. Á.; Vanderburg, A.; Bento, J.; Mancini, L.; Ciceri, S.; Brahm, R.; Jordán, A.; Espinoza, N.; Rabus, M.; Tan, T. G.; Penev, K.; Bhatti, W.; De Val-Borro, M.; Suc, V.; Csubry, Z.; Henning, Th.; Sarkis, P.; Lázár, J.; Papp, I.; Sári, P. (2017), «HATS-36b and 24 Other Transiting/Eclipsing Systems from the HATSouth-K2 Campaign 7 Program», The Astronomical Journal, 155 (3): 119, arXiv:1706.03858, doi:10.3847/1538-3881/aaa8e6
- ↑ a b c d Brahm, R.; Hartman, J. D.; Jordán, A.; Bakos, G. Á.; Espinoza, N.; Rabus, M.; Bhatti, W.; Penev, K.; Sarkis, P.; Suc, V.; Csubry, Z.; Bayliss, D.; Bento, J.; Zhou, G.; Mancini, L.; Henning, T.; Ciceri, S.; Val-Borro, M. de; Shectman, S.; Crane, J. D.; Arriagada, P.; Butler, P.; Teske, J.; Thompson, I.; Osip, D.; Díaz, M.; Schmidt, B.; Lázár, J.; Papp, I.; Sári, P. (2017), «HATS-43b, HATS-44b, HATS-45b, and HATS-46b: Four Short-period Transiting Giant Planets in the Neptune–Jupiter Mass Range», The Astronomical Journal, 155 (3): 112, arXiv:1707.07093, doi:10.3847/1538-3881/aaa898
- ↑ Henning, Th.; Mancini, L.; Sarkis, P.; Bakos, G. Á.; Hartman, J. D.; Bayliss, D.; Bento, J.; Bhatti, W.; Brahm, R.; Ciceri, S.; Csubry, Z.; Val-Borro, M. de; Espinoza, N.; Fulton, B. J.; Howard, A. W.; Isaacson, H. T.; Jordán, A.; Marcy, G. W.; Penev, K.; Rabus, M.; Suc, V.; Tan, T. G.; Tinney, C. G.; Wright, D. J.; Zhou, G.; Durkan, S.; Lazar, J.; Papp, I.; Sari, P. (2018), «HATS-50b through HATS-53b: Four Transiting Hot Jupiters Orbiting G-type Stars Discovered by the HATSouth Survey», The Astronomical Journal, 155 (2): 79, arXiv:1712.04324, doi:10.3847/1538-3881/aaa254
- ↑ Christiansen, Jessie L.; Vanderburg, Andrew; et al. (setembro de 2017), «Three's Company: An Additional Non-transiting Super-Earth in the Bright HD 3167 System, and Masses for All Three Planets», The Astronomical Journal, 154 (3), Bibcode:2017AJ....154..122C, arXiv:1706.01892, doi:10.3847/1538-3881/aa832d, 122.
- ↑ a b c Rey, J.; Hébrard, G.; Bouchy, F.; Bourrier, V.; Boisse, I.; Santos, N. C.; Arnold, L.; Astudillo-Defru, N.; Bonfils, X.; Borgniet, S.; Courcol, B.; Deleuil, M.; Delfosse, X.; Demangeon, O.; Díaz, R. F.; Ehrenreich, D.; Forveille, T.; Marmier, M.; Moutou, C.; Pepe, F.; Santerne, A.; Sahlmann, J.; Ségransan, D.; Udry, S.; Wilson, P. A. (2017), «The SOPHIE search for northern extrasolar planets», Astronomy & Astrophysics, 601: A9, arXiv:1702.06393, doi:10.1051/0004-6361/201630089
- ↑ a b Udry, S.; Dumusque, X.; Lovis, C.; Segransan, D.; Diaz, R. F.; Benz, W.; Bouchy, F.; Coffinet, A.; Lo Curto, G.; Mayor, M.; Mordasini, C.; Motalebi, F.; Pepe, F.; Queloz, D.; Santos, N. C.; Wyttenbach, A.; Alonso, R.; Collier Cameron, A.; Deleuil, M.; Figueira, P.; Gillon, M.; Moutou, C.; Pollacco, D.; Pompei, E. (2019), «The HARPS search for southern extra-solar planets. XLII. Eight HARPS multi-planet systems hosting 20 super-Earth and Neptune-mass companions», Astronomy & Astrophysics, A37: 622, Bibcode:2019A&A...622A..37U, arXiv:1705.05153, doi:10.1051/0004-6361/201731173
- ↑ Feng, F.; Tuomi, M.; Jones, H.R.A. (setembro de 2017). «Evidence for at least three planet candidates orbiting HD 20794». Astronomy and Astrophysics. 605 (103). 11 páginas. Bibcode:2017A&A...605A.103F. arXiv:1705.05124. doi:10.1051/0004-6361/201730406
- ↑ a b Trifonov, T.; Kürster, M.; Zechmeister, M.; Zakhozhay, O. V.; Reffert, S.; Lee, M. H.; Rodler, F.; Vogt, S. S.; Brems, S. S. (2017). «Three planets around HD 27894. A close-in pair with a 2:1 period ratio and an eccentric Jovian planet at 5.4 AU». Astronomy & Astrophysics. 602: L8. Bibcode:2017A&A...602L...8T. arXiv:1706.00509. doi:10.1051/0004-6361/201731044
- ↑ a b c d e Vogt, Steven S.; et al. (2017). «A Six-planet System around the Star HD 34445». The Astronomical Journal. 154 (5). 181 páginas. Bibcode:2017AJ....154..181V. arXiv:1710.07337. doi:10.3847/1538-3881/aa8b61
- ↑ a b c d e Rosenthal, Lee J.; Fulton, Benjamin J.; Hirsch, Lea A.; Isaacson, Howard T.; Howard, Andrew W.; Dedrick, Cayla M.; Sherstyuk, Ilya A.; Blunt, Sarah C.; Petigura, Erik A.; Knutson, Heather A.; Behmard, Aida; Chontos, Ashley; Crepp, Justin R.; Crossfield, Ian J. M.; Dalba, Paul A.; Fischer, Debra A.; Henry, Gregory W.; Kane, Stephen R.; Kosiarek, Molly; Marcy, Geoffrey W.; Rubenzahl, Ryan A.; Weiss, Lauren M.; Wright, Jason T. (2021). «The California Legacy Survey. I. A Catalog of 178 Planets from Precision Radial Velocity Monitoring of 719 Nearby Stars over Three Decades». The Astrophysical Journal Supplement Series. 255: 8. arXiv:2105.11583. doi:10.3847/1538-4365/abe23c
- ↑ a b c Jeong, G.; Lee, B.-C.; Han, I.; Omiya, M.; Izumiura, H.; Sato, B.; Harakawa, H.; Kambe, E.; Mkrtichian, D. (2017), «Detection of planet candidates around K giants. HD 40956, HD 111591, and HD 113996», Astronomy & Astrophysics, 610: A3, arXiv:1711.07173, doi:10.1051/0004-6361/201629185
- ↑ a b Gillon, M.; Demory, B.-O.; Lovis, C.; Deming, D.; Ehrenreich, D.; Lo Curto, G.; Mayor, M.; Pepe, F.; Queloz, D.; Seager, S.; Ségransan, D.; Udry, S. (2017), «The Spitzersearch for the transits of HARPS low-mass planets», Astronomy & Astrophysics, 601: A117, arXiv:1701.01303, doi:10.1051/0004-6361/201629270
- ↑ Wittenmyer, Robert A.; Jones, M. I.; Horner, Jonathan; Kane, Stephen R.; Marshall, J. P.; Mustill, A. J.; Jenkins, J. S.; Rojas, P. A. Pena; Zhao, Jinglin; Villaver, Eva; Butler, R. P.; Clark, Jake (2017), «The Pan-Pacific Planet Search. VII. The Most Eccentric Planet Orbiting a Giant Star», The Astronomical Journal, 154 (6): 274, arXiv:1711.05378, doi:10.3847/1538-3881/aa9894
- ↑ Bergmann, C.; Jones, M. I.; Zhao, J.; Mustill, A. J.; Brahm, R.; Torres, P.; Wittenmyer, R. A.; Gunn, F.; Pollard, K. R.; Zapata, A.; Vanzi, L.; Wang, Songhu (2021), «HD 76920 b pinned down: A detailed analysis of the most eccentric planetary system around an evolved star», Publications of the Astronomical Society of Australia, 38, arXiv:2102.08902, doi:10.1017/pasa.2021.8
- ↑ TESS Asteroseismic Analysis of HD 76920: The Giant Star Hosting An Extremely Eccentric Exoplanet, 2023, arXiv:2302.01102
- ↑ Unger, N.; et al. (2021), «The HARPS search for southern extra-solar planets», Astronomy & Astrophysics, 654: A104, arXiv:2108.10198, doi:10.1051/0004-6361/202141351
- ↑ a b Ferraz, Alvaro; Kochetov, Evgenii (2017), A Multi-Planet System Transiting the V = 9 Rapidly Rotating F-Star HD 106315, arXiv:1701.03808
- ↑ Reiners, A.; et al. (2017), «The CARMENES search for exoplanets around M dwarfs», Astronomy & Astrophysics, 609: L5, arXiv:1712.05797, doi:10.1051/0004-6361/201732165
- ↑ a b Suárez Mascareño, A.; González Hernández, J. I.; Rebolo, R.; Velasco, S.; Toledo-Padrón, B.; Udry, S.; Motalebi, F.; Ségrasan, D.; Wyttenbach, A.; Mayor, M.; Pepe, F.; Lovis, C.; Santos, N. C.; Figueira, P.; Esposito, M. (2018), «The RoPES project with HARPS and HARPS-N», Astronomy & Astrophysics, 612: A41, arXiv:1712.01046, doi:10.1051/0004-6361/201732042
- ↑ Feng, F.; Tuomi, M.; Jones, H. R. A. (2017), «Agatha: Disentangling periodic signals from correlated noise in a periodogram framework», Monthly Notices of the Royal Astronomical Society, 470 (4): 4794–4814, arXiv:1705.03089, doi:10.1093/mnras/stx1126
- ↑ Yılmaz, M.; Sato, B.; Bikmaev, I.; Selam, S. O.; Izumiura, H.; Keskin, V.; Kambe, E.; Melnikov, S. S.; Galeev, A.; Özavcı, İ.; Irtuganov, E. N.; Zhuchkov, R. Ya. (2017), «A Jupiter-mass planet around the K0 giant HD 208897», Astronomy & Astrophysics, 608: A14, arXiv:1708.01895, doi:10.1051/0004-6361/201731184
- ↑ Chauvin, G.; et al. (2017), «Discovery of a warm, dusty giant planet around HIP 65426», Astronomy & Astrophysics, 605: L9, arXiv:1707.01413, doi:10.1051/0004-6361/201731152
- ↑ Cloutier, R.; Astudillo-Defru, N.; Doyon, R.; Bonfils, X.; Almenara, J.-M.; Benneke, B.; Bouchy, F.; Delfosse, X.; Ehrenreich, D.; Forveille, T.; Lovis, C.; Mayor, M.; Menou, K.; Murgas, F.; Pepe, F.; Rowe, J.; Santos, N. C.; Udry, S.; Wünsche, A. (2017), «Characterization of the K2-18 multi-planetary system with HARPS», Astronomy & Astrophysics, 608: A35, arXiv:1707.04292, doi:10.1051/0004-6361/201731558
- ↑ Narita, Norio; Hirano, Teruyuki; Fukui, Akihiko; Hori, Yasunori; Dai, Fei; Yu, Liang; Livingston, John; Ryu, Tsuguru; Nowak, Grzegorz; Kuzuhara, Masayuki; Sato, Bun'ei; Takeda, Yoichi; Albrecht, Simon; Kudo, Tomoyuki; Kusakabe, Nobuhiko; Palle, Enric; Ribas, Ignasi; Tamura, Motohide; Van Eylen, Vincent; Winn, Joshua N. (2017), «The K2-ESPRINT project. VI. K2-105 b, a hot Neptune around a metal-rich G-dwarf», Publications of the Astronomical Society of Japan, 69 (2), arXiv:1701.01294, doi:10.1093/pasj/psx002
- ↑ a b Guenther, E. W.; et al. (2017), «K2-106, a system containing a metal-rich planet and a planet of lower density», Astronomy & Astrophysics, 608: A93, Bibcode:2017A&A...608A..93G, arXiv:1705.04163, doi:10.1051/0004-6361/201730885
- ↑ Petigura, Erik A.; Sinukoff, Evan; Lopez, Eric D.; Crossfield, Ian J. M.; Howard, Andrew W.; Brewer, John M.; Fulton, Benjamin J.; Isaacson, Howard T.; Ciardi, David R.; Howell, Steve B.; Everett, Mark E.; Horch, Elliott P.; Hirsch, Lea A.; Weiss, Lauren M.; Schlieder, Joshua E. (2017), «Four Sub-Saturns with Dissimilar Densities: Windows into Planetary Cores and Envelopes», The Astronomical Journal, 153 (4): 142, arXiv:1702.00013, doi:10.3847/1538-3881/aa5ea5
- ↑ Fridlund, Malcolm; et al. (2017), «K2-111 b − a short period super-Earth transiting a metal poor, evolved old star», Astronomy & Astrophysics, 604: A16, arXiv:1704.08284, doi:10.1051/0004-6361/201730822
- ↑ a b Shporer, Avi; Zhou, George; Fulton, Benjamin J.; Vanderburg, Andrew; Espinoza, Nestor; Collins, Karen; Ciardi, David; Bayliss, Daniel; Armstrong, James D.; Bento, Joao; Bouchy, Francois; Cochran, William D.; Cameron, Andrew Collier; Colón, Knicole; Crossfield, Ian; Dragomir, Diana; Howard, Andrew W.; Howell, Steve B.; Isaacson, Howard; Kielkopf, John F.; Murgas, Felipe; Sefako, Ramotholo; Sinukoff, Evan; Siverd, Robert; Udry, Stephane (2017), «K2-114b and K2-115b: Two Transiting Warm Jupiters», The Astronomical Journal, 154 (5): 188, arXiv:1708.07128, doi:10.3847/1538-3881/aa8bb9
- ↑ a b c d e f g h i j k l m n Dressing, Courtney D.; Vanderburg, Andrew; Schlieder, Joshua E.; Crossfield, Ian J. M.; Knutson, Heather A.; Newton, Elisabeth R.; Ciardi, David R.; Fulton, Benjamin J.; Gonzales, Erica J.; Howard, Andrew W.; Isaacson, Howard; Livingston, John; Petigura, Erik A.; Sinukoff, Evan; Everett, Mark; Horch, Elliott; Howell, Steve B. (2017), «Characterizing K2 Candidate Planetary Systems Orbiting Low-mass Stars. II. Planetary Systems Observed During Campaigns 1–7», The Astronomical Journal, 154 (5): 207, arXiv:1703.07416, doi:10.3847/1538-3881/aa89f2
- ↑ a b c d e f g h i j k l m n o p Hirano, Teruyuki; et al. (2017), «Exoplanets around Low-mass Stars Unveiled byK2», The Astronomical Journal, 155 (3): 127, arXiv:1710.03239, doi:10.3847/1538-3881/aaa9c1
- ↑ Dai, Fei; et al. (2017), «The Discovery and Mass Measurement of a New Ultra-short-period Planet: K2-131b», The Astronomical Journal, 154 (6): 226, arXiv:1710.00076, doi:10.3847/1538-3881/aa9065
- ↑ Grunblatt, Samuel K.; Huber, Daniel; Gaidos, Eric; Lopez, Eric D.; Howard, Andrew W.; Isaacson, Howard T.; Sinukoff, Evan; Vanderburg, Andrew; Nofi, Larissa; Yu, Jie; North, Thomas S. H.; Chaplin, William; Foreman-Mackey, Daniel; Petigura, Erik; Ansdell, Megan; Weiss, Lauren; Fulton, Benjamin; Lin, Douglas N. C. (2017), «Seeing Double withK2: Testing Re-inflation with Two Remarkably Similar Planets around Red Giant Branch Stars», The Astronomical Journal, 154 (6): 254, arXiv:1706.05865, doi:10.3847/1538-3881/aa932d
- ↑ a b c Wells, R.; Poppenhaeger, K.; Watson, C. A. (2017), «Three small transiting planets around the M-dwarf host star LP 358-499», Monthly Notices of the Royal Astronomical Society: Letters, 473: L131–L135, arXiv:1709.01025, doi:10.1093/mnrasl/slx171
- ↑ a b c Rodriguez, Joseph E; Vanderburg, Andrew; Eastman, Jason D; Mann, Andrew W; Crossfield, Ian J. M; Ciardi, David R; Latham, David W; Quinn, Samuel N (2018). «A System of Three Super Earths Transiting the Late K-Dwarf GJ 9827 at 30 pc». The Astronomical Journal. 155 (2). 72 páginas. Bibcode:2018AJ....155...72R. arXiv:1709.01957. doi:10.3847/1538-3881/aaa292
- ↑ a b c Mann, Andrew W.; Vanderburg, Andrew; Rizzuto, Aaron C.; Kraus, Adam L.; Berlind, Perry; Bieryla, Allyson; Calkins, Michael L.; Esquerdo, Gilbert A.; Latham, David W.; Mace, Gregory N.; Morris, Nathan R.; Quinn, Samuel N.; Sokal, Kimberly R.; Stefanik, Robert P. (2017), «Zodiacal Exoplanets in Time (ZEIT). VI. A Three-planet System in the Hyades Cluster Including an Earth-sized Planet», The Astronomical Journal, 155: 4, arXiv:1709.10328, doi:10.3847/1538-3881/aa9791
- ↑ HYADES MEMBER K2-136c:THE SMALLEST PLANET IN AN OPEN CLUSTER WITH A PRECISELY MEASURED MASS, 2023, arXiv:2304.02779
- ↑ Smith, A M S.; et al. (2018), «K2-137 b: An Earth-sized planet in a 4.3-h orbit around an M-dwarf», Monthly Notices of the Royal Astronomical Society, 474 (4): 5523–5533, arXiv:1707.04549, doi:10.1093/mnras/stx2891
- ↑ Barragán, O.; Gandolfi, D.; Smith, A M S.; Deeg, H. J.; Fridlund, M C V.; Persson, C. M.; Donati, P.; Endl, M.; Csizmadia, Sz; Grziwa, S.; Nespral, D.; Hatzes, A. P.; Cochran, W. D.; Fossati, L.; Brems, S. S.; Cabrera, J.; Cusano, F.; Eigmüller, Ph; Eiroa, C.; Erikson, A.; Guenther, E.; Korth, J.; Lorenzo-Oliveira, D.; Mancini, L.; Pätzold, M.; Prieto-Arranz, J.; Rauer, H.; Rebollido, I.; Saario, J.; Zakhozhay, O. V. (2017), «K2-139 b: A low-mass warm Jupiter on a 29-d orbit transiting an active K0 V star», Monthly Notices of the Royal Astronomical Society, 475 (2): 1765–1776, arXiv:1702.00691, doi:10.1093/mnras/stx3207
- ↑ Giles, H A C.; Bayliss, D.; Espinoza, N.; Brahm, R.; Blanco-Cuaresma, S.; Shporer, A.; Armstrong, D.; Lovis, C.; Udry, S.; Bouchy, F.; Marmier, M.; Jordán, A.; Bento, J.; Cameron, A Collier; Sefako, R.; Cochran, W. D.; Rojas, F.; Rabus, M.; Jenkins, J. S.; Jones, M.; Pantoja, B.; Soto, M.; Jensen-Clem, R.; Duev, D. A.; Salama, M.; Riddle, R.; Baranec, C.; Law, N. M. (2017), «K2-140b – an eccentric 6.57 d transiting hot Jupiter in Virgo», Monthly Notices of the Royal Astronomical Society, 475 (2): 1809–1818, arXiv:1706.06865, doi:10.1093/mnras/stx3300
- ↑ K2-141 b: A 5-M⊕ super-Earth transiting a K7 V star every 6.7 hours, 2017, arXiv:1711.05277
- ↑ Malavolta, Luca; et al. (2018). «An Ultra-short Period Rocky Super-Earth with a Secondary Eclipse and a Neptune-like Companion around K2-141». The Astronomical Journal. 155 (3). 107. Bibcode:2018AJ....155..107M. arXiv:1801.03502. doi:10.3847/1538-3881/aaa5b5
- ↑ Adams, Elisabeth R.; et al. (2020). «Ultra Short Period Planets in K2 III: Neighbors are Common with 13 New Multi-Planet Systems and 10 Newly Validated Planets in Campaigns 0-8, 10». The Planetary Science Journal. 2 (4): 152. Bibcode:2021PSJ.....2..152A. arXiv:2011.11698. doi:10.3847/PSJ/ac0ea0
- ↑ Gaudi, B. Scott; et al. (2017), «A giant planet undergoing extreme-ultraviolet irradiation by its hot massive-star host», Nature, 546 (7659): 514–518, PMID 28582774, arXiv:1706.06723, doi:10.1038/nature22392
- ↑ McLeod, Kim K.; Rodriguez, Joseph E.; Oelkers, Ryan J.; Collins, Karen A.; Bieryla, Allyson; Fulton, Benjamin J.; Stassun, Keivan G.; Gaudi, B. Scott; Penev, Kaloyan; Stevens, Daniel J.; et al. (1 de junho de 2017). «KELT-18b: Puffy Planet, Hot Host, Probably Perturbed». The Astronomical Journal. 153 (6). 263 páginas. Bibcode:2017AJ....153..263M. ISSN 0004-6256. arXiv:1702.01657. doi:10.3847/1538-3881/aa6d5d
- ↑ Siverd, Robert J.; et al. (2017), «KELT-19Ab: AP∼ 4.6-day Hot Jupiter Transiting a Likely Am Star with a Distant Stellar Companion», The Astronomical Journal, 155: 35, arXiv:1709.07010, doi:10.3847/1538-3881/aa9e4d
- ↑ Talens, G. J. J; et al. (2018). «MASCARA-2 b: A hot Jupiter transiting a mV = 7.6 A-star». Astronomy & Astrophysics. A57: 612. Bibcode:2018A&A...612A..57T. arXiv:1707.01500. doi:10.1051/0004-6361/201731512
- ↑ Rainer, M.; et al. (2021), «The GAPS programme at TNG», Astronomy & Astrophysics, 649: A29, arXiv:2103.10395, doi:10.1051/0004-6361/202039247
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- ↑ Schmitt, Joseph R.; Jenkins, Jon M.; Fischer, Debra A. (2017), «A Search for Lost Planets in the Kepler Multi-planet Systems and the Discovery of the Long-period, Neptune-sized Exoplanet Kepler-150 F», The Astronomical Journal, 153 (4): 180, PMID 29375142, arXiv:1703.09229, doi:10.3847/1538-3881/aa62ad
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- ↑ OGLE-2017-BLG-0173Lb: Low Mass-Ratio Planet in a "Hollywood" Microlensing Event, 2017, arXiv:1709.08476
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- ↑ Qatar Exoplanet Survey: Qatar-6b -- a grazing transiting hot Jupiter, 2017, arXiv:1712.03216
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