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Link to original content: http://pt.wikipedia.org/wiki/Lista_de_exoplanetas_descobertos_em_2014
Lista de exoplanetas descobertos em 2014 – Wikipédia, a enciclopédia livre Saltar para o conteúdo

Lista de exoplanetas descobertos em 2014

Origem: Wikipédia, a enciclopédia livre.

Esta é uma Lista de exoplanetas descobertos em 2014.

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-11 4672 b 0.53 1667 2.28 Vel. radial 89 0.57 4475 [2]
Beta Cancri b 7.8 605.2 1.7 Vel. radial 290.4 1.7 4092.1 [3]
Beta Ursae Minoris b 6.1 522.3 1.4 Vel. radial 126.5 1.4 4126 [3]
COROT-22b 0.038 0.435 9.75598 0.092 885 Trânsito 1930 1.1 5939 [4]
COROT-24b 0.018 0.33 5.1134 0.056 1070 Trânsito 2000 0.91 4950 [5]
COROT-24c 0.088 0.44 11.759 0.098 850 Trânsito 2000 0.91 4950 [5]
COROT-27b 10.39 1.007 3.57532 0.0476 1500 Trânsito 3400±200 1.05 5900 [6] Planeta perdido[7]
Gliese 15 Ab 0.017 11.4433 0.0717 Vel. radial 11.6 0.38 3567 [8]
Gliese 27.1 b 0.0409 15.819 0.101 Vel. radial 77.05 0.53 3542 Também conhecido como Gliese 9018,[9] não relacionado a Gliese 27.
Gliese 160.2 b 0.0321 5.2354 0.053 Vel. radial 84.39 0.69 4347 Alternativamente conhecido como Gliese 9144, não relacionado ao Gliese 160. Exoplaneta comprovado[9][10]
Gliese 180 b 0.0261 17.380 0.103 Vel. radial 38.95 0.43 3371 [9]
Gliese 180 c 0.0201 24.329 0.129 Vel. radial 38.95 0.43 3371 [9]
Gliese 229 Ab 0.10 471 0.970 Vel. radial 18.77 0.58 3564 [9]
Gliese 433 c 0.14 4900+1800
−1000 		4.7+1.2
−0.8 		Vel. radial 29.57 0.48 3472 [9]
Gliese 422 b 0.0311 26.161 0.119 Vel. radial 41.32 0.35 3323 [9]
Gliese 682 b 0.014 17.478 0.080 Vel. radial 16.33 0.27 3028 Exoplaneta comprovado[9][10]
Gliese 682 c 0.0274 57.32 0.176 Vel. radial 16.33 0.27 3028 Exoplaneta comprovado[9][10]
Gliese 687 b 0.058 38.14 0.16353 Vel. radial 14.8 0.41 3413 [11]
Gliese 832 c 0.017 35.68 0.163 Vel. radial 16.1 0.45 3472 Exoplaneta potencialmente habitável,[12] provavelmente não existe[13]
Gliese 3293 b 0.07406 30.5987 0.14339 Vel. radial 51.4 0.42 3466 [14]
Gliese 3293 c 0.06636 122.6196 0.36175 Vel. radial 51.4 0.42 3466 [14]
Gliese 3341 b 0.0208 14.207 0.089 Vel. radial 77.1 0.47 3526 [14]
GU Piscium b 11.3 1.265 2000 Imagem direta 160 0.33 3250±32 [15]
HAT-P-49b 1.73 1.413 2.691548 0.0438 2131 Trânsito 1050 1.54 6820 [16]
HAT-P-54b 0.76 0.944 3.799847 0.04117 Trânsito 443 0.65 4390 [17] Disputed in 2016,[18] reconfirmed in 2021.[19]
HATS-4b 1.323 1.02 2.516729 0.0362 1315 Trânsito 1400 1 5403 [20]
HATS-5b 0.237 0.912 4.763387 0.0542 1025 Trânsito 840 0.94 5304 [21]
HATS-6b 0.319 0.998 3.3252725 0.03623 Transito 484 0.57 3724 [22]
HD 564 b 0.33 492.3 1.2 Vel. radial 175 0.96 5902 [2]
HD 4203 c 2.17 6700 6.95 Vel. radial 253.8 1.13 5702 [23]
HD 5319 c 1.15 886 2.071 Vel. radial 370 1.51 4958 [24]
HD 10442 b 2.1 1043 2.335 Vel. radial 443±4 1.56 5034 [24]
HD 11506 c 0.408±0.057 223.41±0.32 0.774±0.038 Vel. radial 167.4±0.4 1.12±0.02 5833±28 [24]
HD 14067 b 7.8 1455 3.4 Vel. radial 533 2.4 4815 [25]
HD 30669 b 0.47 1684 2.69 Vel. radial 186 0.92 5400 [2]
HD 75784 b 1.15 341.7 1.073 Vel. radial 224 1.41 4917 [24]
HD 100546 b 6.9 53 Imagem direta 320 2.4 10500 Maior exoplaneta descoberto[26]
HD 103720 b 0.62 4.5557 0.0498 Vel. radial 136 0.79 5017 [2]
HD 108341 b 3.5 1129 2 Vel. radial 161 0.84 5122 [2]
HD 114613 b 0.48 3827 5.16 Vel. radial 66.8 1.36 5729 [27]
HD 141399 b 0.451 94.44 0.415 Vel. radial 118 1.07 5600 [28]
HD 141399 c 1.33 201.99 0.689 Vel. radial 118 1.07 5600 [28]
HD 141399 d 1.18 1069.8 2.09 Vel. radial 118 1.07 5600 [28]
HD 141399 e 0.66 5000 5 Vel. radial 118 1.07 5600 [28]
HD 154857 c 2.58 3452 5.36 Vel. radial 223.5 1.72 5605 [27]
HIP 67851 b 1.38 88.9 0.46 Vel. radial 208.3±0.6 1.63 4890 [29]
HIP 67851 c 4.34±0.59 1741±39 3.09±0.18 Vel. radial 208.3±0.6 1.63 4890 [30]
HIP 97233 b 20 1058.8 2.55 Vel. radial 347 1.93 5020 [29]
HIP 105854 b 8.2 184.2 0.81 Vel. radial 276 2.1 4780 [31]
HIP 116454 b 0.037 0.226 9.1205 0.0906 Vel. radial 180 0.78 5089 [32]
Kapteyn b 0.015 48.616+0.036
−0.032 		0.168 Vel. radial 12.8 0.28 3550 A existência do planeta foi disputada[33][34]
Kapteyn c 0.022 121.54 0.311 Vel. radial 12.8 0.28 3550 A existência do planeta foi disputada[33][34]
KIC 10001893 b 0.2197 Modulação de brilho orbital 5700±500 27500 Exoplaneta comprovado[35][36]
KIC 10001893 c 0.32528 Modulação de brilho orbital 5700±500 27500 Exoplaneta comprovado[35][36]
KIC 10001893 d 0.81161 Modulação de brilho orbital 5700±500 27500 Exoplaneta comprovado[35][36]
Kepler-23d 0.196 15.274299 0.124 Trânsito 2600 1.11 5828 [37]
Kepler-24d 0.149 4.244384 0.051 Trânsito 3900 1.03 5897 [37]
Kepler-24e 0.248 18.998355 0.138 Trânsito 3900 1.03 5897 [37]
Kepler-25d 0.283 123 Vel. radial 798±4 1.19 6270 [38][37]
Kepler-26d 0.095 3.543919 0.039 Trânsito 1104±10 0.54 3914 [37]
Kepler-26e 0.215 46.827915 0.22 Trânsito 1104±10 0.54 3914 [37]
Kepler-31d 6.8 0.348 87.6451 0.4 Trânsito 6800 1.21 6340 [37]
Kepler-37e 51.196 Tempo 220 0.8 5417 [37]
Kepler-48d 0.025 0.182 42.8961 Trânsito 1009±5 0.88 5194 [38][37]
Kepler-48e 2.067 982 Vel. radial 1009±5 0.88 5194 [38]
Kepler-49d 0.143 2.576549 0.031 Trânsito 1024±8 0.55 4252 [37]
Kepler-49e 0.139 18.596108 0.116 Trânsito 1024±8 0.55 4252 [37]
Kepler-51d 0.024 0.865 130.194 0.509 Trânsito 2610±50 1.04 6018 [37]
Kepler-52d 0.174 36.445171 0.182 Trânsito 1058±7 0.54 4263 [37]
Kepler-53d 0.189 9.751962 0.091 Trânsito 4600±200 0.98 5858 [37]
Kepler-54d 0.136 20.995694 0.126 Trânsito 893±9 0.51 4252 [37]
Kepler-55d 0.142 2.211099 0.029 Trânsito 1920±30 0.62 4503 [37]
Kepler-55e 0.138 4.617534 0.048 Trânsito 1920±30 0.62 4503 [37]
Kepler-55f 0.142 10.198545 0.081 Trânsito 1920±30 0.62 4503 [37]
Kepler-58d 0.262 40.101371 0.236 Trânsito 3250±80 0.95 6099 [37]
Kepler-79d 0.019 0.639 52.0902 0.287 553 Trânsito 3230±60 1.17 6174 [37]
Kepler-79e 0.013 0.311 81.0659 0.386 477 Trânsito 3230±60 1.17 6174 [37]
Kepler-80d 0.02124 0.136 3.07222 0.0372 Trânsito 1160 0.73 4540 [37]
Kepler-80e 0.01299 0.143 4.64489 0.0491 Trânsito 1160 0.73 4540 [37]
Kepler-81d 0.108 20.837846 0.128 Trânsito 1147±10 0.64 4500 [37]
Kepler-82d 0.158 2.382961 0.034 Trânsito 3030±80 0.85 5428 [37]
Kepler-82e 0.22 5.902206 0.063 Trânsito 3030±80 0.85 5428 [37]
Kepler-83d 0.173 5.169796 0.051 Trânsito 1320±17 0.66 4648 [37]
Kepler-84d 0.123 4.224537 0.052 Trânsito 4700±500 1 6031 [37]
Kepler-84e 0.232 27.434389 0.181 Trânsito 4700±500 1 6031 [37]
Kepler-84f 0.196 44.552169 0.25 Trânsito 4700±500 1 6031 [37]
Kepler-85d 0.107 17.91323 0.13 Trânsito 2550±50 0.92 5436 [37]
Kepler-85e 0.113 25.216751 0.163 Trânsito 2550±50 0.92 5436 [37]
Kepler-93b 0.01265 0.132 4.72673978 0.053 1037 Trânsito 313.7±0.7 0.91 5669 [38]
Kepler-93c 3 1460 Vel. radial 313.7±0.7 0.91 5669 [38]
Kepler-94b 0.034 0.313 2.50806 Trânsito 629±2 0.81 4781 [38]
Kepler-94c 9.836 820.3 Vel. radial 629±2 0.81 4781 [38]
Kepler-95b 0.041 0.305 11.5231 Trânsito 1472±18 1.08 5699 [38]
Kepler-96b 0.027 0.238 16.2385 Trânsito 402.2±1.3 1 5690 [38]
Kepler-97b 0.011 0.132 2.58664 Trânsito 1322±11 0.94 5779 [38]
Kepler-97c 1.08 789 Vel. radial 1322±11 0.94 5779 [38]
Kepler-98b 0.011 0.178 1.54168 Trânsito 1154±9 0.99 5539 [38]
Kepler-99b 0.019 0.132 4.60358 Trânsito 683±3 0.79 4782 [38]
Kepler-100b 0.023 0.118 6.88705 Trânsito 1002±5 1.08 5825 [38][37]
Kepler-100c 0.196 12.8159 Trânsito 1002±5 1.08 5825 [38][37]
Kepler-100d 0.144 35.3331 Trânsito 1002±5 1.08 5825 [38][37]
Kepler-101b 0.16 0.51 3.4876812 0.0474 Trânsito 3110±50 1.17 5667 [37]
Kepler-101c 0.01 0.112 6.02976 0.0684 Trânsito 3110±50 1.17 5667 [37]
Kepler-102b 0.042 5.28696 792 Trânsito 352.7±0.7 0.81 4909 [38][37]
Kepler-102c 0.052 7.07142 718 Trânsito 352.7±0.7 0.81 4909 [38][37]
Kepler-102d 0.012 0.105 10.3117 Trânsito 352.7±0.7 0.81 4909 [38][37]
Kepler-102f 0.079 27.4536 457 Trânsito 352.7±0.7 0.81 4909 [38][37]
Kepler-103b 0.031 0.301 15.9654 Trânsito 1637±19 1.09 5845 [38][37]
Kepler-103c 0.114 0.459 179.612 Trânsito 1637±19 1.09 5845 [38][37]
Kepler-104b 0.277 11.427548 0.094 Trânsito 1322±14 0.81 5711 [37]
Kepler-104c 0.279 23.668205 0.153 Trânsito 1322±14 0.81 5711 [37]
Kepler-104d 0.319 51.755394 0.257 Trânsito 1322±14 0.81 5711 [37]
Kepler-105c 0.01447 0.117 7.1262 Trânsito 1517±18 0.96 5827 [37]
Kepler-106b 0.073 6.16486 Trânsito 1470±20 1 5858 [38]
Kepler-106c 0.033 0.223 13.5708 Trânsito 1470±20 1 5858 [38][37]
Kepler-106d 0.085 23.9802 Trânsito 1470±20 1 5858 [38][37]
Kepler-106e 0.035 0.228 43.8445 Trânsito 1470±20 1 5858 [38][37]
Kepler-107b 0.139 3.179997 0.044 Trânsito 1741±18 5851 [37]
Kepler-107c 0.161 4.901425 0.059 Trânsito 1741±18 5851 [37]
Kepler-107d 0.095 7.958203 0.082 Trânsito 1741±18 5851 [37]
Kepler-107e 0.308 14.749049 0.123 Trânsito 1741±18 5851 [37]
Kepler-108b 0.772 49.183921 0.292 Trânsito 4200±500 0.87 5854 [37]
Kepler-108c 0.73 190.323494 0.721 Trânsito 4200±500 0.87 5854 [37]
Kepler-109b 0.211 6.48163 Trânsito 1570±17 1.04 5952 [38][37]
Kepler-109c 0.225 21.2227 Trânsito 1570±17 1.04 5952 [38][37]
Kepler-110b 0.163 12.691112 0.107 Trânsito 1950±30 5960 [37]
Kepler-110c 0.197 31.719775 0.198 Trânsito 1950±30 5960 [37]
Kepler-111b 0.141 3.341815 0.046 Trânsito 2190±20 5952 [37]
Kepler-111c 0.651 224.784608 0.761 Trânsito 2190±20 5952 [37]
Kepler-112b 0.211 8.408878 0.076 Trânsito 1698±14 5544 [37]
Kepler-112c 0.214 28.574263 0.172 Trânsito 1698±14 5544 [37]
Kepler-113b 0.037 0.162 4.754 Trânsito 862±3 0.75 4725 [38][37]
Kepler-113c 0.194 8.92507 Trânsito 862±3 0.75 4725 [38][37]
Kepler-114b 0.112 5.188549 0.053 722 Trânsito 852±4 0.56 4605 [37]
Kepler-115b 0.097 2.403679 0.036 Trânsito 2070±20 1 5979 [37]
Kepler-115c 0.232 8.990889 0.087 Trânsito 2070±20 1 5979 [37]
Kepler-116b 0.305 5.968734 0.069 Trânsito 3200±50 1.16 6142 [37]
Kepler-116c 0.205 13.07163 0.116 Trânsito 3200±50 1.16 6142 [37]
Kepler-117b 0.094 0.719 18.7959228 0.1445 Trânsito 4700 1.13 6150 [37]
Kepler-117c 1.84 1.101 50.790391 0.2804 Trânsito 4700 1.13 6150 [37]
Kepler-118b 0.175 7.518496 0.073 Trânsito 1900±20 0.86 5274 [37]
Kepler-118c 0.685 20.17202 0.141 Trânsito 1900±20 0.86 5274 [37]
Kepler-119b 0.321 2.422082 0.035 Trânsito 2340±40 5595 [37]
Kepler-119c 0.082 4.125103 0.049 Trânsito 2340±40 5595 [37]
Kepler-120b 0.192 6.312501 0.055 Trânsito 1281±10 4096 [37]
Kepler-120c 0.136 12.794585 0.088 Trânsito 1281±10 4096 [37]
Kepler-121b 0.209 3.177422 0.039 Trânsito 1690±20 5311 [37]
Kepler-121c 0.203 41.008011 0.216 Trânsito 1690±20 5311 [37]
Kepler-122b 0.209 5.766193 0.064 Trânsito 3450±70 0.99 6050 [37]
Kepler-122c 0.524 12.465988 0.108 Trânsito 3450±70 0.99 6050 [37]
Kepler-122d 0.196 21.587475 0.155 Trânsito 3450±70 0.99 6050 [37]
Kepler-122e 0.232 37.993273 0.227 Trânsito 3450±70 0.99 6050 [37]
Kepler-122f 0.113 0.156 56.268 Tempo 3450±70 0.99 6050 ?
Kepler-123b 0.262 17.232366 0.135 Trânsito 3430±80 1.03 6089 [37]
Kepler-123c 0.132 26.695074 0.181 Trânsito 3430±80 1.03 6089 [37]
Kepler-124b 0.065 3.410493 0.039 Trânsito 1386±10 4984 [37]
Kepler-124c 0.156 13.821375 0.1 Trânsito 1386±10 4984 [37]
Kepler-124d 0.099 30.950851 0.17 Trânsito 1386±10 4984 [37]
Kepler-125b 0.211 4.164389 0.041 Trânsito 601±3 0.55 3810 [37]
Kepler-125c 0.066 5.774464 0.051 Trânsito 601±3 0.55 3810 [37]
Kepler-126b 0.136 10.495711 0.099 Trânsito 779±5 6239 [37]
Kepler-126c 0.141 21.869741 0.162 Trânsito 779±5 6239 [37]
Kepler-126d 0.223 100.283134 0.448 Trânsito 779±5 6239 [37]
Kepler-127b 0.125 14.435889 0.125 Trânsito 1162±8 6106 [37]
Kepler-127c 0.237 29.393195 0.2 Trânsito 1162±8 6106 [37]
Kepler-127d 0.236 48.630408 0.28 Trânsito 1162±8 6106 [37]
Kepler-129b 0.211 15.79186 0.131 Trânsito 1349±14 1.18 5770 [37]
Kepler-129c 0.227 82.20017 0.393 Trânsito 1349±14 1.18 5770 [37]
Kepler-130c 0.259 27.50868 0.178 Trânsito 1042±7 1 5884 [37]
Kepler-130d 0.146 87.517905 0.377 Trânsito 1042±7 1 5884 [37]
Kepler-131b 0.051 0.215 16.092 Trânsito 750±4 1.02 5685 [38][37]
Kepler-131c 0.026 0.075 25.5169 Trânsito 750±4 1.02 5685 [38][37]
Kepler-132b 0.108 6.178196 0.067 Trânsito 900±70 6003 [37]
Kepler-132c 0.114 6.414914 0.068 Trânsito 900±70 6003 [37]
Kepler-132d 0.138 18.010199 0.136 Trânsito 900±70 6003 [37]
Kepler-133b 0.157 8.129976 0.083 Trânsito 2170±60 5736 [37]
Kepler-133c 0.253 31.517586 0.204 Trânsito 2170±60 5736 [37]
Kepler-134b 0.178 5.317429 0.06 Trânsito 1102±7 5983 [37]
Kepler-134c 0.112 10.105785 0.092 Trânsito 1102±7 5983 [37]
Kepler-135b 0.161 6.00253 0.067 Trânsito 2060±40 6090 [37]
Kepler-135c 0.103 11.448708 0.103 Trânsito 2060±40 6090 [37]
Kepler-136b 0.183 11.5789 0.106 Trânsito 1389±14 1.2 6165 [37]
Kepler-136c 0.178 16.399235 0.133 Trânsito 1389±14 1.2 6165 [37]
Kepler-137b 0.131 8.436387 0.077 Trânsito 996±6 5187 [37]
Kepler-137c 0.168 18.735753 0.13 Trânsito 996±6 5187 [37]
Kepler-138b 0.00021 0.047 10.3126 Trânsito 218.5±0.3 0.52 3841 [37]
Kepler-138c 0.0062 0.107 13.7813 Trânsito 218.5±0.3 0.52 3841 [37]
Kepler-138d 0.00201 0.108 23.0881 431 Trânsito 218.5±0.3 0.52 3841 [37]
Kepler-139b 0.262 15.771044 0.127 Trânsito 1289±13 1.08 5594 [37]
Kepler-139c 0.302 157.072878 0.586 Trânsito 1289±13 1.08 5594 [37]
Kepler-140b 0.144 3.25427 0.045 Trânsito 1940±20 6077 [37]
Kepler-140c 0.161 91.353282 0.414 Trânsito 1940±20 6077 [37]
Kepler-141b 0.062 3.107675 0.039 Trânsito 990±4 1 4910 [37]
Kepler-141c 0.126 7.010606 0.067 Trânsito 990±4 1 4910 ?
Kepler-142b 0.178 2.024152 0.032 Trânsito 1818±13 0.99 5790 [37]
Kepler-142c 0.255 4.761702 0.057 Trânsito 1818±13 0.99 5790 [37]
Kepler-142d 0.193 41.809118 0.242 Trânsito 1818±13 0.99 5790 [37]
Kepler-143b 0.215 16.007583 0.127 Trânsito 2700±40 5848 [37]
Kepler-143c 0.301 27.082511 0.181 Trânsito 2700±40 5848 [37]
Kepler-144b 0.119 5.885273 0.066 Trânsito 1269±10 1.03 6075 [37]
Kepler-144c 0.12 10.104665 0.094 Trânsito 1269±10 1.03 6075 [37]
Kepler-146b 0.331 31.158799 0.2 Trânsito 2390±30 5948 [37]
Kepler-146c 0.279 76.732171 0.364 Trânsito 2390±30 5948 [37]
Kepler-147b 0.136 12.610584 0.113 Trânsito 3500±90 1.01 6012 [37]
Kepler-147c 0.217 33.416423 0.216 Trânsito 3500±90 1.01 6012 [37]
Kepler-148b 0.161 1.729366 0.028 Trânsito 2640±50 5272 [37]
Kepler-148c 0.321 4.180043 0.05 Trânsito 2640±50 5272 [37]
Kepler-149b 0.376 29.198943 0.184 Trânsito 1893±19 5381 [37]
Kepler-149c 0.144 55.328328 0.281 Trânsito 1893±19 5381 [37]
Kepler-149d 0.353 160.018032 0.571 Trânsito 1893±19 5381 [37]
Kepler-150b 0.112 3.428054 0.044 Trânsito 2980±60 5560 [37]
Kepler-150c 0.329 7.381998 0.073 Trânsito 2980±60 5560 [37]
Kepler-150d 0.249 12.56093 0.104 Trânsito 2980±60 5560 [37]
Kepler-150e 0.278 30.826557 0.189 Trânsito 2980±60 5560 [37]
Kepler-151b 0.273 15.228958 0.116 Trânsito 2160±30 0.83 5460 [37]
Kepler-151c 0.186 24.674612 0.16 Trânsito 2160±30 0.83 5460 [37]
Kepler-152b 0.249 18.207973 0.124 Trânsito 1457±10 5088 [37]
Kepler-152c 0.213 88.255055 0.356 Trânsito 1457±10 5088 [37]
Kepler-153b 0.261 18.870227 0.129 Trânsito 1518±11 5404 [37]
Kepler-153c 0.226 46.90232 0.237 Trânsito 1518±11 5404 [37]
Kepler-154b 0.202 33.040532 0.198 Trânsito 3070±60 0.89 5690 [37]
Kepler-154c 0.263 62.303276 0.303 Trânsito 3070±60 0.89 5690 [37]
Kepler-155b 0.186 5.931194 0.056 Trânsito 965±7 0.58 4508 [37]
Kepler-155c 0.2 52.661793 0.242 Trânsito 965±7 0.58 4508 [37]
Kepler-156b 0.205 4.973456 0.054 Trânsito 1465±11 5094 [37]
Kepler-156c 0.227 15.906801 0.117 Trânsito 1465±11 5094 [37]
Kepler-157b 0.118 1.732342 0.028 Trânsito 2580±40 5774 [37]
Kepler-157c 0.2 13.5405 0.11 Trânsito 2580±40 5774 [37]
Kepler-158b 0.189 16.709184 0.111 Trânsito 1037±6 4623 [37]
Kepler-158c 0.17 28.551383 0.158 Trânsito 1037±6 4623 [37]
Kepler-159b 0.212 10.139623 0.082 Trânsito 1232±10 4625 [37]
Kepler-159c 0.304 43.595792 0.218 Trânsito 1232±10 4625 [37]
Kepler-160b 0.137 4.309427 0.05 Trânsito 3140±60 0.88 5471+115
−37 		[37][39]
Kepler-160c 0.322 13.699087 0.109 Trânsito 3140±60 0.88 5471+115
−37 		[37][39]
Kepler-161b 0.189 4.921355 0.054 Trânsito 1435±10 0.77 5078 [37]
Kepler-161c 0.183 7.06424 0.068 Trânsito 1435±10 0.77 5078 [37]
Kepler-162b 0.112 6.919798 0.069 Trânsito 2860±50 5816 [37]
Kepler-162c 0.27 19.446355 0.137 Trânsito 2860±50 5816 [37]
Kepler-163b 0.094 7.810937 0.078 Trânsito 2300±40 0.96 5776 [37]
Kepler-163c 0.202 21.347262 0.152 Trânsito 2300±40 0.96 5776 [37]
Kepler-164b 0.126 5.03503 0.058 Trânsito 2980±50 1.11 5888 [37]
Kepler-164c 0.244 10.945723 0.097 Trânsito 2980±50 1.11 5888 [37]
Kepler-164d 0.219 28.986769 0.187 Trânsito 2980±50 1.11 5888 [37]
Kepler-165b 0.207 8.180848 0.072 Trânsito 1860±20 5211 [37]
Kepler-165c 0.199 15.31299 0.11 Trânsito 1860±20 5211 [37]
Kepler-166b 0.203 7.650254 0.072 Trânsito 2000±20 5413 [37]
Kepler-166c 0.212 34.260281 0.195 Trânsito 2000±20 5413 [37]
Kepler-167b 0.144 4.3931632 0.0483 Trânsito 1100 0.77 4890 [37]
Kepler-167c 0.138 7.406114 0.0684 Trânsito 1100 0.77 4890 [37]
Kepler-168b 0.13 4.425391 0.056 Trânsito 4550±160 6282 [37]
Kepler-168c 0.24 13.193242 0.116 Trânsito 4550±160 6282 [37]
Kepler-169b 0.101 3.250619 0.04 Trânsito 1341±9 0.86 4997 [37]
Kepler-169c 0.108 6.195469 0.062 Trânsito 1341±9 0.86 4997 [37]
Kepler-169d 0.112 8.348125 0.075 Trânsito 1341±9 0.86 4997 [37]
Kepler-169e 0.196 13.767102 0.105 Trânsito 1341±9 0.86 4997 [37]
Kepler-169f 0.23 87.090195 0.359 Trânsito 1341±9 0.86 4997 [37]
Kepler-170b 0.285 7.930592 0.08 Trânsito 2460±40 5679 [37]
Kepler-170c 0.255 16.665863 0.131 Trânsito 2460±40 5679 [37]
Kepler-171b 0.209 4.166972 0.05 Trânsito 2890±60 5642 [37]
Kepler-171c 0.228 11.463462 0.098 Trânsito 2890±60 5642 [37]
Kepler-171d 0.169 39.595519 0.223 Trânsito 2890±60 5642 [37]
Kepler-172b 0.21 2.940309 0.04 Trânsito 2770±60 0.86 5526 [37]
Kepler-172c 0.255 6.388996 0.068 Trânsito 2770±60 0.86 5526 [37]
Kepler-172d 0.201 14.627119 0.118 Trânsito 2770±60 0.86 5526 [37]
Kepler-172e 0.246 35.118736 0.211 Trânsito 2770±60 0.86 5526 [37]
Kepler-173b 0.115 4.263742 0.048 Trânsito 2780±50 0.78 6031 [37]
Kepler-173c 0.217 8.005777 0.074 Trânsito 2780±50 0.78 6031 [37]
Kepler-174b 0.175 13.98179 0.1 Trânsito 1268±8 4880 [37]
Kepler-174c 0.133 44.000529 0.214 Trânsito 1268±8 4880 [37]
Kepler-174d 0.195 247.35373 0.677 Trânsito 1268±8 4880 [37]
Kepler-175b 0.228 11.903515 0.105 Trânsito 4450±150 1.04 6064 [37]
Kepler-175c 0.277 34.035257 0.213 Trânsito 4450±150 1.04 6064 [37]
Kepler-176b 0.128 5.433074 0.058 Trânsito 1750±20 5232 [37]
Kepler-176c 0.232 12.759712 0.102 Trânsito 1750±20 5232 [37]
Kepler-176d 0.224 25.751974 0.163 Trânsito 1750±20 5232 [37]
Kepler-178b 0.259 9.576694 0.085 Trânsito 2380±30 5676 [37]
Kepler-178c 0.257 20.552802 0.142 Trânsito 2380±30 5676 [37]
Kepler-178d 0.352 96.678988 0.397 Trânsito 2380±30 5676 [37]
Kepler-179b 0.146 2.735926 0.036 Trânsito 2010±20 5302 [37]
Kepler-179c 0.178 6.40013 0.064 Trânsito 2010±20 5302 [37]
Kepler-180b 0.134 13.817124 0.109 Trânsito 2320±30 0.84 5731 [37]
Kepler-180c 0.269 41.885775 0.229 Trânsito 2320±30 0.84 5731 [37]
Kepler-181b 0.113 3.137873 0.04 Trânsito 2020±30 5333 [37]
Kepler-181c 0.178 4.302149 0.049 Trânsito 2020±30 5333 [37]
Kepler-182b 0.23 9.825792 0.096 Trânsito 5290±180 1.14 6250 [37]
Kepler-182c 0.306 20.684342 0.157 Trânsito 5290±180 1.14 6250 [37]
Kepler-183b 0.184 5.687945 0.064 Trânsito 3530±100 5888 [37]
Kepler-183c 0.203 11.637071 0.103 Trânsito 3530±100 5888 [37]
Kepler-184b 0.211 10.687576 0.092 Trânsito 2030±20 5788 [37]
Kepler-184c 0.176 20.303005 0.141 Trânsito 2030±20 5788 [37]
Kepler-184d 0.222 29.022358 0.179 Trânsito 2030±20 5788 [37]
Kepler-185b 0.104 1.6329 0.026 Trânsito 1542±15 0.79 5208 [37]
Kepler-185c 0.18 20.729042 0.139 Trânsito 1542±15 0.79 5208 [37]
Kepler-186b 0.095 3.8867907 0.0343 Trânsito 560 0.54 3755 [37]
Kepler-186c 0.112 7.267302 0.0451 Trânsito 560 0.54 3755 [37]
Kepler-186d 0.125 13.342996 0.0781 Trânsito 560 0.54 3755 [37]
Kepler-186e 0.113 22.407704 0.11 Trânsito 560 0.54 3755 [37]
Kepler-186f 0.104 129.9441 0.432 Trânsito 560 0.54 3755 Exoplaneta potencialmente habitável
Kepler-187b 0.126 4.938864 0.059 Trânsito 3850±110 0.85 6105 [37]
Kepler-187c 0.238 10.640263 0.099 Trânsito 3850±110 0.85 6105 [37]
Kepler-188b 0.15 2.061897 0.032 Trânsito 3250±80 6021 [37]
Kepler-188c 0.285 5.996553 0.066 Trânsito 3250±80 6021 [37]
Kepler-189b 0.108 10.399931 0.088 Trânsito 1960±20 0.79 5235 [37]
Kepler-189c 0.212 20.134866 0.137 Trânsito 1960±20 0.79 5235 [37]
Kepler-190b 0.139 2.019999 0.03 Trânsito 1431±9 0.84 5106 [37]
Kepler-190c 0.13 3.763024 0.045 Trânsito 1431±9 0.84 5106 [37]
Kepler-191b 0.12 9.939632 0.087 Trânsito 1970±30 0.85 5282 [37]
Kepler-191c 0.166 17.738506 0.128 Trânsito 1970±30 0.85 5282 [37]
Kepler-192b 0.244 9.926746 0.09 Trânsito 2170±20 5479 [37]
Kepler-192c 0.249 21.2234 0.15 Trânsito 2170±20 5479 [37]
Kepler-193b 0.213 11.38848 0.106 Trânsito 3390±80 6335 [37]
Kepler-193c 0.245 50.697494 0.286 Trânsito 3390±80 6335 [37]
Kepler-194b 0.135 2.092281 0.032 Trânsito 3700±100 6089 [37]
Kepler-194c 0.231 17.308032 0.131 Trânsito 3700±100 6089 [37]
Kepler-194d 0.214 52.814973 0.275 Trânsito 3700±100 6089 [37]
Kepler-195b 0.181 8.307872 0.077 Trânsito 2170±30 5329 [37]
Kepler-195c 0.138 34.096863 0.197 Trânsito 2170±30 5329 [37]
Kepler-196b 0.17 20.739886 0.138 Trânsito 1491±10 5128 [37]
Kepler-196c 0.2 47.427737 0.24 Trânsito 1491±10 5128 [37]
Kepler-197b 0.091 5.599308 0.06 Trânsito 1088±7 6004 [37]
Kepler-197c 0.11 10.349695 0.09 Trânsito 1088±7 6004 [37]
Kepler-197d 0.109 15.677563 0.119 Trânsito 1088±7 6004 [37]
Kepler-197e 0.081 25.209715 0.164 Trânsito 1088±7 6004 [37]
Kepler-198b 0.252 17.790037 0.131 Trânsito 1638±14 0.93 5574 [37]
Kepler-198c 0.22 49.567416 0.259 Trânsito 1638±14 0.93 5574 [37]
Kepler-199b 0.277 23.637604 0.158 Trânsito 1725±14 5644 [37]
Kepler-199c 0.29 67.093408 0.316 Trânsito 1725±14 5644 [37]
Kepler-200b 0.19 8.594805 0.08 Trânsito 2210±20 5678 [37]
Kepler-200c 0.142 10.222157 0.09 Trânsito 2210±20 5678 [37]
Kepler-201b 0.219 25.672083 0.175 Trânsito 2240±30 1.17 6065 [37]
Kepler-201c 0.254 151.884058 0.573 Trânsito 2240±30 1.17 6065 [37]
Kepler-202b 0.145 4.069427 0.045 Trânsito 937±3 4668 [37]
Kepler-202c 0.165 16.282493 0.113 Trânsito 937±3 4668 [37]
Kepler-203b 0.229 3.162697 0.043 Trânsito 2340±30 0.98 5821 [37]
Kepler-203c 0.22 5.370647 0.061 Trânsito 2340±30 0.98 5821 [37]
Kepler-203d 0.128 11.32972 0.1 Trânsito 2340±30 0.98 5821 [37]
Kepler-204b 0.226 14.400974 0.117 Trânsito 2280±20 0.96 5812 [37]
Kepler-204c 0.16 25.660593 0.173 Trânsito 2280±20 0.96 5812 [37]
Kepler-205b 0.135 2.75564 0.032 Trânsito 523.4±1.1 4321 [37]
Kepler-205c 0.146 20.306546 0.122 Trânsito 523.4±1.1 4321 [37]
Kepler-206b 0.107 7.781987 0.078 Trânsito 1972±16 0.94 5764 [37]
Kepler-206c 0.158 13.137471 0.111 Trânsito 1972±16 0.94 5764 [37]
Kepler-206d 0.106 23.44281 0.163 Trânsito 1972±16 0.94 5764 [37]
Kepler-207b 0.14 1.611865 0.029 Trânsito 2920±30 5920 [37]
Kepler-207c 0.134 3.071571 0.044 Trânsito 2920±30 5920 [37]
Kepler-207d 0.295 5.868075 0.068 Trânsito 2920±30 5920 [37]
Kepler-208b 0.145 4.22864 0.054 Trânsito 2580±20 1.03 6092 [37]
Kepler-208c 0.124 7.466623 0.079 Trânsito 2580±20 1.03 6092 [37]
Kepler-208d 0.107 11.131786 0.103 Trânsito 2580±20 1.03 6092 [37]
Kepler-208e 0.132 16.259458 0.132 Trânsito 2580±20 1.03 6092 [37]
Kepler-209b 0.202 16.087845 0.122 Trânsito 1913±18 5513 [37]
Kepler-209c 0.277 41.749882 0.231 Trânsito 1913±18 5513 [37]
Kepler-210b 0.262 2.453234 0.032 Trânsito 764±2 4559 [37]
Kepler-210c 0.323 7.972513 0.07 Trânsito 764±2 4559 [37]
Kepler-211b 0.112 4.138575 0.048 Trânsito 1018±5 0.97 5123 [37]
Kepler-211c 0.115 6.04045 0.062 Trânsito 1018±5 0.97 5123 [37]
Kepler-212b 0.097 16.257582 0.133 Trânsito 2280±20 1.16 5852 [37]
Kepler-212c 0.244 31.805174 0.207 Trânsito 2280±20 1.16 5852 [37]
Kepler-213b 0.145 2.46236 0.036 Trânsito 2100±20 0.94 5696 [37]
Kepler-213c 0.209 4.822962 0.057 Trânsito 2100±20 0.94 5696 [37]
Kepler-214b 0.233 15.660544 0.13 Trânsito 4080±70 6169 [37]
Kepler-214c 0.19 28.7798 0.194 Trânsito 4080±70 6169 [37]
Kepler-215b 0.145 9.360672 0.084 Trânsito 1607±12 0.77 5739 [37]
Kepler-215c 0.158 14.667108 0.113 Trânsito 1607±12 0.77 5739 [37]
Kepler-215d 0.213 30.864423 0.185 Trânsito 1607±12 0.77 5739 [37]
Kepler-215e 0.156 68.16101 0.314 Trânsito 1607±12 0.77 5739 [37]
Kepler-216b 0.21 7.693641 0.079 Trânsito 4000±70 6091 [37]
Kepler-216c 0.271 17.406669 0.136 Trânsito 4000±70 6091 [37]
Kepler-217b 0.199 5.374943 0.065 Trânsito 3720±50 6171 [37]
Kepler-217c 0.165 8.586004 0.089 Trânsito 3720±50 6171 [37]
Kepler-218b 0.132 3.619337 0.046 Trânsito 2180±20 5502 [37]
Kepler-218c 0.28 44.699576 0.248 Trânsito 2180±20 5502 [37]
Kepler-219b 0.263 4.585512 0.057 Trânsito 2620±30 5786 [37]
Kepler-219c 0.319 22.714613 0.165 Trânsito 2620±30 5786 [37]
Kepler-219d 0.251 47.903645 0.272 Trânsito 2620±30 5786 [37]
Kepler-220b 0.072 4.159807 0.046 Trânsito 560±2 4632 [37]
Kepler-220c 0.14 9.034199 0.076 Trânsito 560±2 4632 [37]
Kepler-220d 0.087 28.122397 0.163 Trânsito 560±2 4632 [37]
Kepler-220e 0.119 45.902733 0.226 Trânsito 560±2 4632 [37]
Kepler-221b 0.153 2.795906 0.037 Trânsito 1270±9 0.72 5243 [37]
Kepler-221c 0.261 5.690586 0.059 Trânsito 1270±9 0.72 5243 [37]
Kepler-221d 0.244 10.04156 0.087 Trânsito 1270±9 0.72 5243 [37]
Kepler-221e 0.235 18.369917 0.13 Trânsito 1270±9 0.72 5243 [37]
Kepler-222b 0.282 3.936981 0.048 Trânsito 2520±40 5433 [37]
Kepler-222c 0.414 10.08881 0.091 Trânsito 2520±40 5433 [37]
Kepler-222d 0.329 28.081912 0.18 Trânsito 2520±40 5433 [37]
Kepler-223b 0.02328 0.267 7.38449 Trânsito 6400±400 1.12 [37]
Kepler-223c 0.01605 0.307 9.84564 Trânsito 6400±400 1.12 [37]
Kepler-223d 0.02517 0.467 14.78869 Trânsito 6400±400 1.12 [37]
Kepler-223e 0.0151 0.41 19.72567 Trânsito 6400±400 1.12 [37]
Kepler-224b 0.124 3.132924 0.038 Trânsito 2600±60 0.74 5018 [37]
Kepler-224c 0.278 5.925003 0.058 Trânsito 2600±60 0.74 5018 [37]
Kepler-224d 0.205 11.349393 0.089 Trânsito 2600±60 0.74 5018 [37]
Kepler-224e 0.176 18.643577 0.124 Trânsito 2600±60 0.74 5018 [37]
Kepler-225b 0.107 6.738975 0.056 Trânsito 1850±40 3682 [37]
Kepler-225c 0.164 18.794234 0.111 Trânsito 1850±40 3682 [37]
Kepler-226b 0.138 3.940997 0.047 Trânsito 3280±80 0.86 5571 [37]
Kepler-226c 0.203 5.349555 0.058 Trânsito 3280±80 0.86 5571 [37]
Kepler-226d 0.109 8.109044 0.076 Trânsito 3280±80 0.86 5571 [37]
Kepler-227b 0.277 9.488015 0.09 Trânsito 3640±100 5854 [37]
Kepler-227c 0.271 54.418694 0.29 Trânsito 3640±100 5854 [37]
Kepler-228b 0.136 2.566546 0.038 Trânsito 5600±300 6043 [37]
Kepler-228c 0.241 4.134444 0.052 Trânsito 5600±300 6043 [37]
Kepler-228d 0.36 11.094286 0.101 Trânsito 5600±300 6043 [37]
Kepler-229b 0.196 6.252972 0.062 Trânsito 2750±70 5120 [37]
Kepler-229c 0.439 16.068638 0.117 Trânsito 2750±70 5120 [37]
Kepler-229d 0.343 41.194912 0.22 Trânsito 2750±70 5120 [37]
Kepler-230b 0.38 32.625555 0.191 Trânsito 2460±40 5588 [37]
Kepler-230c 0.182 91.773242 0.38 Trânsito 2460±40 5588 [37]
Kepler-231b 0.154 10.065275 0.074 Trânsito 988±9 0.58 3767 [37]
Kepler-231c 0.172 19.271566 0.114 Trânsito 988±9 0.58 3767 [37]
Kepler-232b 0.275 4.431222 0.054 Trânsito 4570±160 5847 [37]
Kepler-232c 0.342 11.379349 0.101 Trânsito 4570±160 5847 [37]
Kepler-233b 0.217 8.472382 0.077 Trânsito 2860±60 5360 [37]
Kepler-233c 0.242 60.418955 0.287 Trânsito 2860±60 5360 [37]
Kepler-234b 0.33 2.711506 0.04 Trânsito 5900±300 6224 [37]
Kepler-234c 0.313 7.21205 0.077 Trânsito 5900±300 6224 [37]
Kepler-235b 0.199 3.340222 0.037 Trânsito 1410±20 0.59 4255 [37]
Kepler-235c 0.114 7.824904 0.065 Trânsito 1410±20 0.59 4255 [37]
Kepler-235d 0.183 20.060548 0.122 Trânsito 1410±20 0.59 4255 [37]
Kepler-235e 0.198 46.183669 0.213 Trânsito 1410±20 0.59 4255 [37]
Kepler-236b 0.14 8.295611 0.065 Trânsito 949±7 0.56 3750 [37]
Kepler-236c 0.178 23.968127 0.132 Trânsito 949±7 0.56 3750 [37]
Kepler-237b 0.126 4.715106 0.05 Trânsito 2180±30 0.7 4861 [37]
Kepler-237c 0.186 8.103636 0.071 Trânsito 2180±30 0.7 4861 [37]
Kepler-238b 0.154 2.090876 0.034 Trânsito 6200±300 1.06 5751 [37]
Kepler-238c 0.213 6.155557 0.069 Trânsito 6200±300 1.06 5751 [37]
Kepler-238d 0.274 13.233549 0.115 Trânsito 6200±300 1.06 5751 [37]
Kepler-239b 0.208 11.763051 0.095 Trânsito 2150±40 0.74 4914 [37]
Kepler-239c 0.224 56.228098 0.268 Trânsito 2150±40 0.74 4914 [37]
Kepler-240b 0.122 4.144495 0.048 Trânsito 2480±60 4985 [37]
Kepler-240c 0.196 7.953528 0.074 Trânsito 2480±60 4985 [37]
Kepler-241b 0.208 12.718092 0.094 Trânsito 1980±130 4699 [37]
Kepler-241c 0.229 36.065978 0.189 Trânsito 1980±130 4699 [37]
Kepler-242b 0.233 8.20395 0.075 Trânsito 1990±30 5020 [37]
Kepler-242c 0.178 14.496481 0.109 Trânsito 1990±30 5020 [37]
Kepler-243b 0.219 5.715442 0.062 Trânsito 2300±30 0.89 5228 [37]
Kepler-243c 0.178 20.026218 0.142 Trânsito 2300±30 0.89 5228 [37]
Kepler-244b 0.246 4.311792 0.05 Trânsito 3480±120 5554 [37]
Kepler-244c 0.183 9.767292 0.087 Trânsito 3480±120 5554 [37]
Kepler-244d 0.206 20.050401 0.14 Trânsito 3480±120 5554 [37]
Kepler-245b 0.229 7.49019 0.071 Trânsito 2870±80 0.8 5100 [37]
Kepler-245c 0.194 17.460812 0.124 Trânsito 2870±80 0.8 5100 [37]
Kepler-245d 0.27 36.277108 0.202 Trânsito 2870±80 0.8 5100 [37]
Kepler-246b 0.209 4.60182 0.052 Trânsito 2070±20 0.86 5206 [37]
Kepler-246c 0.134 11.187161 0.095 Trânsito 2070±20 0.86 5206 [37]
Kepler-247b 0.146 3.33616 0.042 Trânsito 2200±40 5100 [37]
Kepler-247c 0.365 9.439452 0.084 Trânsito 2200±40 5100 [37]
Kepler-247d 0.352 20.477912 0.14 Trânsito 2200±40 5100 [37]
Kepler-248b 0.269 6.308205 0.066 Trânsito 2460±40 5190 [37]
Kepler-248c 0.363 16.239494 0.123 Trânsito 2460±40 5190 [37]
Kepler-249b 0.097 3.306539 0.035 Trânsito 624±3 3568 [37]
Kepler-249c 0.135 7.113702 0.058 Trânsito 624±3 3568 [37]
Kepler-249d 0.14 15.368459 0.097 Trânsito 624±3 3568 [37]
Kepler-250b 0.101 4.148141 0.048 Trânsito 2530±50 0.8 5160 [37]
Kepler-250c 0.203 7.156804 0.069 Trânsito 2530±50 0.8 5160 [37]
Kepler-250d 0.194 17.648312 0.127 Trânsito 2530±50 0.8 5160 [37]
Kepler-251b 0.119 4.790936 0.053 Trânsito 3090±90 0.91 5526 [37]
Kepler-251c 0.247 16.514043 0.122 Trânsito 3090±90 0.91 5526 [37]
Kepler-251d 0.247 30.133001 0.182 Trânsito 3090±90 0.91 5526 [37]
Kepler-251e 0.247 99.640161 0.404 Trânsito 3090±90 0.91 5526 [37]
Kepler-252b 0.11 6.668391 0.058 Trânsito 1251±11 0.52 4208 [37]
Kepler-252c 0.192 10.848463 0.08 Trânsito 1251±11 0.52 4208 [37]
Kepler-253b 0.145 3.783986 0.046 Trânsito 2800±60 5208 [37]
Kepler-253c 0.236 10.281951 0.089 Trânsito 2800±60 5208 [37]
Kepler-253d 0.283 18.119869 0.13 Trânsito 2800±60 5208 [37]
Kepler-254b 0.345 5.826662 0.064 Trânsito 4700±200 5957 [37]
Kepler-254c 0.192 12.412183 0.105 Trânsito 4700±200 5957 [37]
Kepler-254d 0.223 18.746477 0.139 Trânsito 4700±200 5957 [37]
Kepler-255b 0.138 5.714606 0.063 Trânsito 3530±100 0.97 5573 [37]
Kepler-255c 0.267 9.946047 0.092 Trânsito 3530±100 0.97 5573 [37]
Kepler-256b 0.142 1.620493 0.027 Trânsito 3440±80 1.02 5551 [37]
Kepler-256c 0.192 3.38802 0.045 Trânsito 3440±80 1.02 5551 [37]
Kepler-256d 0.221 5.839172 0.064 Trânsito 3440±80 1.02 5551 [37]
Kepler-256e 0.21 10.681572 0.096 Trânsito 3440±80 1.02 5551 [37]
Kepler-257b 0.233 2.382667 0.034 Trânsito 2600±50 5180 [37]
Kepler-257c 0.483 6.581484 0.066 Trânsito 2600±50 5180 [37]
Kepler-257d 0.442 24.664551 0.16 Trânsito 2600±50 5180 [37]
Kepler-258b 0.362 13.19722 0.103 Trânsito 1900±20 0.8 4942 [37]
Kepler-258c 0.322 33.653079 0.193 Trânsito 1900±20 0.8 4942 [37]
Kepler-259b 0.25 8.115317 0.079 Trânsito 3360±80 5938 [37]
Kepler-259c 0.241 36.924931 0.217 Trânsito 3360±80 5938 [37]
Kepler-260b 0.179 8.187399 0.075 Trânsito 2080±20 0.88 5250 [37]
Kepler-260c 0.155 76.050178 0.332 Trânsito 2080±20 0.88 5250 [37]
Kepler-261b 0.194 10.381227 0.088 Trânsito 1044±5 0.87 5098 [37]
Kepler-261c 0.178 24.570858 0.156 Trânsito 1044±5 0.87 5098 [37]
Kepler-262b 0.121 13.060855 0.108 Trânsito 2030±20 5841 [37]
Kepler-262c 0.146 21.853722 0.152 Trânsito 2030±20 5841 [37]
Kepler-263b 0.238 16.568087 0.12 Trânsito 2510±50 5265 [37]
Kepler-263c 0.22 47.332773 0.242 Trânsito 2510±50 5265 [37]
Kepler-264b 0.297 40.806231 0.249 Trânsito 3150±60 1.32 6158 [37]
Kepler-264c 0.252 140.101261 0.566 Trânsito 3150±60 1.32 6158 [37]
Kepler-265b 0.166 6.846262 0.069 Trânsito 4330±160 1.03 5835 [37]
Kepler-265c 0.235 17.028937 0.127 Trânsito 4330±160 1.03 5835 [37]
Kepler-265d 0.222 43.130617 0.236 Trânsito 4330±160 1.03 5835 [37]
Kepler-265e 0.231 67.831024 0.319 Trânsito 4330±160 1.03 5835 [37]
Kepler-266b 0.221 6.61833 0.071 Trânsito 4640±190 0.99 5885 [37]
Kepler-266c 0.347 107.723601 0.457 Trânsito 4640±190 0.99 5885 [37]
Kepler-267b 0.177 3.353728 0.037 Trânsito 870±8 0.56 4258 [37]
Kepler-267c 0.19 6.87745 0.06 Trânsito 870±8 0.56 4258 [37]
Kepler-267d 0.203 28.464515 0.154 Trânsito 870±8 0.56 4258 [37]
Kepler-268b 0.227 25.934138 0.18 Trânsito 2840±30 6081 [37]
Kepler-268c 0.302 83.446393 0.391 Trânsito 2840±30 6081 [37]
Kepler-269b 0.22 5.326718 0.061 Trânsito 7900±600 0.98 5847 [37]
Kepler-269c 0.151 8.127899 0.081 Trânsito 7900±600 0.98 5847 [37]
Kepler-270b 0.179 11.476094 0.107 Trânsito 3180±40 6067 [37]
Kepler-270c 0.158 25.262887 0.18 Trânsito 3180±40 6067 [37]
Kepler-271b 0.079 5.217738 0.056 Trânsito 1334±12 5524 [37]
Kepler-271c 0.089 7.410935 0.071 Trânsito 1334±12 5524 [37]
Kepler-272b 0.128 2.971353 0.038 Trânsito 2970±40 0.79 5297 [37]
Kepler-272c 0.16 6.057342 0.061 Trânsito 2970±40 0.79 5297 [37]
Kepler-272d 0.201 10.937304 0.091 Trânsito 2970±40 0.79 5297 [37]
Kepler-273b 0.134 2.936532 0.037 Trânsito 2370±30 5626 [37]
Kepler-273c 0.177 8.014927 0.073 Trânsito 2370±30 5626 [37]
Kepler-274b 0.137 11.634788 0.101 Trânsito 4510±140 6023 [37]
Kepler-274c 0.164 33.197861 0.204 Trânsito 4510±140 6023 [37]
Kepler-275b 0.209 10.300682 0.098 Trânsito 7000±500 1.24 6165 [37]
Kepler-275c 0.302 16.088134 0.132 Trânsito 7000±500 1.24 6165 [37]
Kepler-275d 0.297 35.676062 0.224 Trânsito 7000±500 1.24 6165 [37]
Kepler-276b 0.256 14.12841 0.119 Trânsito 3850±150 1.1 6105 [37]
Kepler-278b 0.363 30.160546 0.207 Trânsito 1460±20 4991 [37]
Kepler-278c 0.32 51.078775 0.294 Trânsito 1460±20 4991 [37]
Kepler-280b 0.129 2.139542 0.032 Trânsito 2600±30 0.91 5744 [37]
Kepler-280c 0.179 4.807091 0.056 Trânsito 2600±30 0.91 5744 [37]
Kepler-281b 0.252 14.646008 0.117 Trânsito 6000±300 0.98 5723 [37]
Kepler-281c 0.474 36.337373 0.215 Trânsito 6000±300 0.98 5723 [37]
Kepler-282b 0.09 9.220524 0.082 Trânsito 4530±150 0.97 5602 [37]
Kepler-282c 0.107 13.638723 0.106 Trânsito 4530±150 0.97 5602 [37]
Kepler-283b 0.19 11.008151 0.082 Trânsito 1540±20 4351 [37]
Kepler-283c 0.162 92.743711 0.341 Trânsito 1540±20 4351 [37]
Kepler-284b 0.2 12.699149 0.104 Trânsito 3460±110 5615 [37]
Kepler-284c 0.233 37.514456 0.213 Trânsito 3460±110 5615 [37]
Kepler-285b 0.12 2.633867 0.036 Trânsito 2750±50 0.85 5411 [37]
Kepler-285c 0.1 6.186676 0.064 Trânsito 2750±50 0.85 5411 [37]
Kepler-286b 0.111 1.796302 0.027 Trânsito 4100±400 5580 [37]
Kepler-286c 0.122 3.468095 0.042 Trânsito 4100±400 5580 [37]
Kepler-286d 0.119 5.914323 0.061 Trânsito 4100±400 5580 [37]
Kepler-286e 0.158 29.221289 0.176 Trânsito 4100±400 5580 [37]
Kepler-287b 0.208 20.342199 0.145 Trânsito 2790±50 5806 [37]
Kepler-287c 0.291 44.851896 0.246 Trânsito 2790±50 5806 [37]
Kepler-288b 0.149 6.097326 0.065 Trânsito 4030±110 0.89 5918 [37]
Kepler-288c 0.254 19.305772 0.14 Trânsito 4030±110 0.89 5918 [37]
Kepler-288d 0.238 56.633742 0.287 Trânsito 4030±110 0.89 5918 [37]
Kepler-289b 0.023 0.192 34.545 0.21 Trânsito 2340±20 1.08 5990 [37]
Kepler-289c 0.42 1.034 125.8518 0.51 Trânsito 2340±20 1.08 5990 [37]
Kepler-289d 0.013 0.239 66.0634 0.33 Trânsito 2340±20 1.08 5990 ?
Kepler-290b 0.201 14.589347 0.11 Trânsito 2310±40 5147 [37]
Kepler-290c 0.241 36.77031 0.205 Trânsito 2310±40 5147 [37]
Kepler-291b 0.193 3.546511 0.047 Trânsito 6100±400 1.03 6002 [37]
Kepler-291c 0.168 5.700786 0.065 Trânsito 6100±400 1.03 6002 [37]
Kepler-292b 0.118 2.580827 0.035 Trânsito 3540±150 0.88 5299 [37]
Kepler-292c 0.131 3.715335 0.045 Trânsito 3540±150 0.88 5299 [37]
Kepler-292d 0.199 7.055679 0.068 Trânsito 3540±150 0.88 5299 [37]
Kepler-292e 0.238 11.97901 0.097 Trânsito 3540±150 0.88 5299 [37]
Kepler-292f 0.21 20.834237 0.141 Trânsito 3540±150 0.88 5299 [37]
Kepler-293b 0.274 19.254196 0.144 Trânsito 3260±70 1.01 5804 [37]
Kepler-293c 0.342 54.155743 0.286 Trânsito 3260±70 1.01 5804 [37]
Kepler-294b 0.158 3.701212 0.048 Trânsito 4600±200 5913 [37]
Kepler-294c 0.242 6.6264 0.071 Trânsito 4600±200 5913 [37]
Kepler-295b 0.109 12.645164 0.099 Trânsito 5800±300 5603 [37]
Kepler-295c 0.104 21.526258 0.142 Trânsito 5800±300 5603 [37]
Kepler-295d 0.121 33.884054 0.192 Trânsito 5800±300 5603 [37]
Kepler-296b 0.144 10.864384 0.079 Trânsito 740 0.5 3740 [37]
Kepler-296c 0.178 5.8416366 0.0521 Trânsito 740 0.5 3740 [37]
Kepler-296d 0.186 19.850291 0.118 Trânsito 740 0.5 3740 [37]
Kepler-296e 0.136 34.14211 0.169 Trânsito 740 0.5 3740 [37]
Kepler-296f 0.161 63.33627 0.255 Trânsito 740 0.5 3740 [37]
Kepler-297b 0.256 38.871826 0.217 Trânsito 2300±20 5619 [37]
Kepler-297c 0.583 74.920137 0.336 Trânsito 2300±20 5619 [37]
Kepler-298b 0.175 10.475464 0.08 Trânsito 1710±20 0.65 4465 [37]
Kepler-298c 0.172 22.92881 0.136 Trânsito 1710±20 0.65 4465 [37]
Kepler-298d 0.223 77.473633 0.305 Trânsito 1710±20 0.65 4465 [37]
Kepler-299b 0.118 2.927128 0.04 Trânsito 3530±80 0.97 5617 [37]
Kepler-299c 0.236 6.885875 0.07 Trânsito 3530±80 0.97 5617 [37]
Kepler-299d 0.166 15.054786 0.118 Trânsito 3530±80 0.97 5617 [37]
Kepler-299e 0.167 38.285489 0.22 Trânsito 3530±80 0.97 5617 [37]
Kepler-300b 0.149 10.446347 0.094 Trânsito 3690±60 0.94 5986 [37]
Kepler-300c 0.201 40.714955 0.232 Trânsito 3690±60 0.94 5986 [37]
Kepler-301b 0.12 2.508553 0.036 Trânsito 2390±30 0.91 5815 [37]
Kepler-301c 0.12 5.419026 0.06 Trânsito 2390±30 0.91 5815 [37]
Kepler-301d 0.156 13.751243 0.112 Trânsito 2390±30 0.91 5815 [37]
Kepler-302b 0.362 30.184104 0.193 Trânsito 4760±190 5740 [37]
Kepler-302c 1.111 127.282184 0.503 Trânsito 4760±190 5740 [37]
Kepler-303b 0.079 1.937055 0.024 Trânsito 688±3 0.59 3944 [37]
Kepler-303c 0.102 7.061149 0.057 Trânsito 688±3 0.59 3944 [37]
Kepler-304b 0.255 3.295709 0.039 Trânsito 1435±17 0.8 4731 [37]
Kepler-304c 0.194 5.315946 0.054 Trânsito 1435±17 0.8 4731 [37]
Kepler-304d 0.245 9.653471 0.08 Trânsito 1435±17 0.8 4731 [37]
Kepler-305d 0.242 16.738661 0.121 Trânsito 2900±80 0.76 5100 [37]
Kepler-306b 0.136 4.646186 0.05 Trânsito 2580±60 0.82 4954 [37]
Kepler-306c 0.21 7.240193 0.067 Trânsito 2580±60 0.82 4954 [37]
Kepler-306d 0.22 17.326644 0.12 Trânsito 2580±60 0.82 4954 [37]
Kepler-306e 0.203 44.840975 0.227 Trânsito 2580±60 0.82 4954 [37]
Kepler-308b 0.189 9.694928 0.09 Trânsito 4500±200 5895 [37]
Kepler-308c 0.193 15.38231 0.123 Trânsito 4500±200 5895 [37]
Kepler-309b 0.139 5.923653 0.059 Trânsito 1804±19 4713 [37]
Kepler-309c 0.224 105.356383 0.401 Trânsito 1804±19 4713 [37]
Kepler-310b 0.106 13.930698 0.111 Trânsito 1990±20 0.85 5797 [37]
Kepler-310c 0.302 56.47542 0.281 Trânsito 1990±20 0.85 5797 [37]
Kepler-310d 0.22 92.876125 0.392 Trânsito 1990±20 0.85 5797 [37]
Kepler-311b 0.152 9.176092 0.087 Trânsito 2590±30 1.06 5905 [37]
Kepler-311c 0.128 19.738286 0.145 Trânsito 2590±30 1.06 5905 [37]
Kepler-312b 0.115 1.772419 0.031 Trânsito 2660±40 1.23 6115 [37]
Kepler-312c 0.281 19.747412 0.153 Trânsito 2660±40 1.23 6115 [37]
Kepler-313b 0.226 14.970418 0.125 Trânsito 3500±300 0.9 5727 [37]
Kepler-313c 0.229 32.273273 0.208 Trânsito 3500±300 0.9 5727 [37]
Kepler-314b 0.074 2.461069 0.035 Trânsito 883±5 1.02 5378 [37]
Kepler-314c 0.259 5.960392 0.064 Trânsito 883±5 1.02 5378 [37]
Kepler-315b 0.336 96.101141 0.402 Trânsito 3910±120 0.78 5796 [37]
Kepler-315c 0.37 265.469335 0.791 Trânsito 3910±120 0.78 5796 [37]
Kepler-316b 0.095 2.240508 0.027 Trânsito 1269±12 0.53 4204 [37]
Kepler-316c 0.103 6.827766 0.058 Trânsito 1269±12 0.53 4204 [37]
Kepler-317b 0.186 5.524242 0.061 Trânsito 3150±80 0.95 5497 [37]
Kepler-317c 0.153 8.77501 0.083 Trânsito 3150±80 0.95 5497 [37]
Kepler-318b 0.42 4.662715 0.056 Trânsito 1618±10 1.05 5746 [37]
Kepler-318c 0.328 11.815007 0.105 Trânsito 1618±10 1.05 5746 [37]
Kepler-319b 0.145 4.362705 0.051 Trânsito 1666±15 1.29 5526 [37]
Kepler-319c 0.235 6.941357 0.069 Trânsito 1666±15 1.29 5526 [37]
Kepler-319d 0.204 31.781925 0.191 Trânsito 1666±15 1.29 5526 [37]
Kepler-320b 0.102 8.371554 0.085 Trânsito 2760±30 6435 [37]
Kepler-320c 0.122 17.934937 0.142 Trânsito 2760±30 6435 [37]
Kepler-321b 0.158 4.915379 0.057 Trânsito 1268±11 1.01 5740 [37]
Kepler-321c 0.207 13.093921 0.11 Trânsito 1268±11 1.01 5740 [37]
Kepler-322b 0.09 1.653888 0.027 Trânsito 1321±8 0.91 5388 [37]
Kepler-322c 0.149 4.337234 0.051 Trânsito 1321±8 0.91 5388 [37]
Kepler-323b 0.128 1.678327 0.028 Trânsito 1500±20 1.09 5987 [37]
Kepler-323c 0.145 3.553822 0.046 Trânsito 1500±20 1.09 5987 [37]
Kepler-324b 0.102 4.385315 0.05 Trânsito 1659±12 0.86 5194 [37]
Kepler-324c 0.281 51.805612 0.26 Trânsito 1659±12 0.86 5194 [37]
Kepler-325b 0.26 4.544439 0.053 Trânsito 2740±40 0.87 5752 [37]
Kepler-325c 0.227 12.762172 0.105 Trânsito 2740±40 0.87 5752 [37]
Kepler-325d 0.249 38.715185 0.22 Trânsito 2740±40 0.87 5752 [37]
Kepler-326b 0.136 2.248329 0.032 Trânsito 1610±30 0.98 5105 [37]
Kepler-326c 0.125 4.580358 0.051 Trânsito 1610±30 0.98 5105 [37]
Kepler-326d 0.108 6.766888 0.066 Trânsito 1610±30 0.98 5105 [37]
Kepler-327b 0.099 2.549575 0.029 Trânsito 794±4 0.55 3799 [37]
Kepler-327c 0.092 5.212333 0.047 Trânsito 794±4 0.55 3799 [37]
Kepler-327d 0.154 13.969457 0.09 Trânsito 794±4 0.55 3799 [37]
Kepler-329b 0.125 7.416397 0.061 Trânsito 1450±20 0.53 4257 [37]
Kepler-329c 0.172 18.684737 0.113 Trânsito 1450±20 0.53 4257 [37]
Kepler-330b 0.12 8.25978 0.075 Trânsito 2380±40 0.78 5117 [37]
Kepler-330c 0.174 15.955387 0.116 Trânsito 2380±40 0.78 5117 [37]
Kepler-331b 0.162 8.457496 0.065 Trânsito 1920±40 0.51 4347 [37]
Kepler-331c 0.164 17.28111 0.105 Trânsito 1920±40 0.51 4347 [37]
Kepler-331d 0.146 32.134328 0.159 Trânsito 1920±40 0.51 4347 [37]
Kepler-332b 0.104 7.626324 0.07 Trânsito 1133±5 0.8 4955 [37]
Kepler-332c 0.097 15.995622 0.114 Trânsito 1133±5 0.8 4955 [37]
Kepler-332d 0.105 34.21154 0.189 Trânsito 1133±5 0.8 4955 [37]
Kepler-333b 0.118 12.551158 0.087 Trânsito 1068±7 0.54 4259 [37]
Kepler-333c 0.099 24.08821 0.135 Trânsito 1068±7 0.54 4259 [37]
Kepler-334b 0.1 5.470319 0.061 Trânsito 1408±14 1 5828 [37]
Kepler-334c 0.128 12.758005 0.107 Trânsito 1408±14 1 5828 [37]
Kepler-334d 0.126 25.09849 0.168 Trânsito 1408±14 1 5828 [37]
Kepler-335b 0.302 6.562331 0.075 Trânsito 4320±100 0.99 5877 [37]
Kepler-335c 0.274 67.844469 0.356 Trânsito 4320±100 0.99 5877 [37]
Kepler-336b 0.091 2.024823 0.033 Trânsito 8000±7000 0.89 5867 [37]
Kepler-336c 0.187 9.600001 0.092 Trânsito 8000±7000 0.89 5867 [37]
Kepler-336d 0.211 20.678772 0.154 Trânsito 8000±7000 0.89 5867 [37]
Kepler-337b 0.137 3.292781 0.045 Trânsito 2250±30 0.96 5684 [37]
Kepler-337c 0.183 9.693201 0.093 Trânsito 2250±30 0.96 5684 [37]
Kepler-338b 0.218 13.726976 0.117 Trânsito 1830±20 1.1 5923 [37]
Kepler-338c 0.209 24.310856 0.172 Trânsito 1830±20 1.1 5923 [37]
Kepler-338d 0.268 44.431014 0.257 Trânsito 1830±20 1.1 5923 [37]
Kepler-338e 0.027 0.139 9.341 Tempo 1830±20 1.1 5923 ?
Kepler-339b 0.127 4.977656 0.055 Trânsito 2040±30 0.84 5631 [37]
Kepler-339c 0.103 6.988055 0.069 Trânsito 2040±30 0.84 5631 [37]
Kepler-339d 0.104 10.558345 0.091 Trânsito 2040±30 0.84 5631 [37]
Kepler-340b 0.226 14.844387 0.134 Trânsito 2690±60 2.11 6620 [37]
Kepler-340c 0.301 22.824669 0.178 Trânsito 2690±60 2.11 6620 [37]
Kepler-341b 0.105 5.195528 0.06 Trânsito 3520±60 0.94 6012 [37]
Kepler-341c 0.152 8.01041 0.08 Trânsito 3520±60 0.94 6012 [37]
Kepler-341d 0.165 27.666313 0.182 Trânsito 3520±60 0.94 6012 [37]
Kepler-341e 0.178 42.473269 0.242 Trânsito 3520±60 0.94 6012 [37]
Kepler-342b 0.201 15.170318 0.128 Trânsito 2600±30 1.13 6175 [37]
Kepler-342c 0.175 26.234138 0.185 Trânsito 2600±30 1.13 6175 [37]
Kepler-342d 0.222 39.459357 0.242 Trânsito 2600±30 1.13 6175 [37]
Kepler-343b 0.215 8.96855 0.088 Trânsito 3100±60 1.04 5807 [37]
Kepler-343c 0.18 23.22182 0.167 Trânsito 3100±60 1.04 5807 [37]
Kepler-344b 0.233 21.963945 0.153 Trânsito 3360±100 0.9 5774 [37]
Kepler-344c 0.263 125.596809 0.488 Trânsito 3360±100 0.9 5774 [37]
Kepler-345b 0.066 7.415563 0.066 Trânsito 1180±50 0.59 4504 [37]
Kepler-345c 0.107 9.387427 0.077 Trânsito 1180±50 0.59 4504 [37]
Kepler-346b 0.237 6.511127 0.071 Trânsito 3300±80 0.97 6033 [37]
Kepler-346c 0.274 23.851549 0.168 Trânsito 3300±80 0.97 6033 [37]
Kepler-347b 0.176 12.79836 0.11 Trânsito 4400±90 1.04 6088 [37]
Kepler-347c 0.156 27.320871 0.183 Trânsito 4400±90 1.04 6088 [37]
Kepler-348b 0.136 7.05677 0.076 Trânsito 1890±20 1.15 6177 [37]
Kepler-348c 0.119 17.265427 0.138 Trânsito 1890±20 1.15 6177 [37]
Kepler-349b 0.17 5.929778 0.065 Trânsito 3150±60 0.97 5956 [37]
Kepler-349c 0.175 12.247629 0.105 Trânsito 3150±60 0.97 5956 [37]
Kepler-350b 0.165 11.189562 0.104 Trânsito 3200±60 1 6186 [37]
Kepler-351b 0.273 37.054919 0.214 Trânsito 3640±40 0.89 5643 [37]
Kepler-351c 0.285 57.24809 0.287 Trânsito 3640±40 0.89 5643 [37]
Kepler-352b 0.077 10.05537 0.085 Trânsito 830±4 0.79 5212 [37]
Kepler-352c 0.111 16.332995 0.118 Trânsito 830±4 0.79 5212 [37]
Kepler-353b 0.079 5.795278 0.051 Trânsito 1268±16 0.54 3903 [37]
Kepler-353c 0.123 8.410894 0.065 Trânsito 1268±16 0.54 3903 [37]
Kepler-354b 0.164 5.47666 0.054 Trânsito 1830±20 0.65 4648 [37]
Kepler-354c 0.117 16.934402 0.115 Trânsito 1830±20 0.65 4648 [37]
Kepler-354d 0.111 24.209842 0.146 Trânsito 1830±20 0.65 4648 [37]
Kepler-355b 0.13 11.03189 0.102 Trânsito 4870±160 1.05 6184 [37]
Kepler-355c 0.242 25.762294 0.179 Trânsito 4870±160 1.05 6184 [37]
Kepler-356b 0.14 4.612696 0.057 Trânsito 2350±30 0.97 6133 [37]
Kepler-356c 0.161 13.121632 0.115 Trânsito 2350±30 0.97 6133 [37]
Kepler-357b 0.164 6.475434 0.063 Trânsito 2290±40 0.78 5036 [37]
Kepler-357c 0.238 16.85837 0.12 Trânsito 2290±40 0.78 5036 [37]
Kepler-357d 0.306 49.499875 0.246 Trânsito 2290±40 0.78 5036 [37]
Kepler-358b 0.243 34.060467 0.21 Trânsito 3700±130 0.95 5908 [37]
Kepler-358c 0.254 83.488369 0.381 Trânsito 3700±130 0.95 5908 [37]
Kepler-359b 0.315 25.563222 0.178 Trânsito 4900±300 1.07 6248 [37]
Kepler-359c 0.384 57.68802 0.307 Trânsito 4900±300 1.07 6248 [37]
Kepler-359d 0.358 77.095691 0.372 Trânsito 4900±300 1.07 6248 [37]
Kepler-360b 0.147 3.289672 0.044 Trânsito 2930±50 0.95 6053 [37]
Kepler-360c 0.187 7.186434 0.075 Trânsito 2930±50 0.95 6053 [37]
Kepler-361b 0.129 8.486616 0.086 Trânsito 3110±50 1.07 6169 [37]
Kepler-361c 0.225 55.188023 0.3 Trânsito 3110±50 1.07 6169 [37]
Kepler-362b 0.079 10.327186 0.087 Trânsito 3660±180 0.77 5788 [37]
Kepler-362c 0.129 37.866281 0.207 Trânsito 3660±180 0.77 5788 [37]
Kepler-363b 0.103 3.614568 0.048 Trânsito 2540±20 1.23 5593 [37]
Kepler-363c 0.151 7.542427 0.079 Trânsito 2540±20 1.23 5593 [37]
Kepler-363d 0.183 11.932125 0.107 Trânsito 2540±20 1.23 5593 [37]
Kepler-364b 0.138 25.745718 0.178 Trânsito 2980±30 1.2 6108 [37]
Kepler-364c 0.192 59.980627 0.312 Trânsito 2980±30 1.2 6108 [37]
Kepler-365b 0.182 10.664903 0.098 Trânsito 2800±200 0.99 6012 [37]
Kepler-365c 0.146 17.784129 0.137 Trânsito 2800±200 0.99 6012 [37]
Kepler-366b 0.13 3.281959 0.045 Trânsito 6400±400 1.05 6209 [37]
Kepler-366c 0.16 12.51616 0.11 Trânsito 6400±400 1.05 6209 [37]
Kepler-367b 0.116 37.815724 0.201 Trânsito 616±2 0.75 4710 [37]
Kepler-367c 0.107 53.578637 0.253 Trânsito 616±2 0.75 4710 [37]
Kepler-368b 0.291 26.84768 0.186 Trânsito 2570±40 0.71 5502 [37]
Kepler-368c 0.346 72.379334 0.36 Trânsito 2570±40 0.71 5502 [37]
Kepler-369b 0.101 2.732756 0.03 Trânsito 840±120 0.54 3591 [37]
Kepler-369c 0.126 14.871572 0.094 Trânsito 840±120 0.54 3591 [37]
Kepler-370b 0.142 4.57953 0.054 Trânsito 3930±120 0.94 5852 [37]
Kepler-370c 0.17 19.02293 0.14 Trânsito 3930±120 0.94 5852 [37]
Kepler-371b 0.169 34.763278 0.2 Trânsito 2710±40 0.94 5666 [37]
Kepler-371c 0.159 67.968015 0.313 Trânsito 2710±40 0.94 5666 [37]
Kepler-372b 0.121 6.849692 0.075 Trânsito 5090±170 1.15 6509 [37]
Kepler-372c 0.186 20.053763 0.154 Trânsito 5090±170 1.15 6509 [37]
Kepler-372d 0.151 30.092568 0.201 Trânsito 5090±170 1.15 6509 [37]
Kepler-373b 0.121 5.535309 0.06 Trânsito 3670±70 0.87 5787 [37]
Kepler-373c 0.111 16.725948 0.126 Trânsito 3670±70 0.87 5787 [37]
Kepler-374b 0.092 1.897806 0.029 Trânsito 4280±120 0.84 5977 [37]
Kepler-374c 0.098 3.282807 0.042 Trânsito 4280±120 0.84 5977 [37]
Kepler-374d 0.117 5.028219 0.056 Trânsito 4280±120 0.84 5977 [37]
Kepler-375b 0.129 12.125934 0.101 Trânsito 4180±180 0.89 5826 [37]
Kepler-375c 0.236 19.986326 0.141 Trânsito 4180±180 0.89 5826 [37]
Kepler-376b 0.095 4.920199 0.057 Trânsito 3090±50 1.05 5900 [37]
Kepler-376c 0.16 14.172327 0.115 Trânsito 3090±50 1.05 5900 [37]
Kepler-377b 0.124 12.509529 0.109 Trânsito 2750±40 0.88 5949 [37]
Kepler-377c 0.184 27.014976 0.182 Trânsito 2750±40 0.88 5949 [37]
Kepler-378b 0.067 16.092361 0.112 Trânsito 498.3±1.4 0.96 4661 [37]
Kepler-378c 0.062 28.906009 0.166 Trânsito 498.3±1.4 0.96 4661 [37]
Kepler-379b 0.148 20.09838 0.152 Trânsito 2430±20 1.08 6054 [37]
Kepler-379c 0.204 62.784697 0.326 Trânsito 2430±20 1.08 6054 [37]
Kepler-380b 0.106 3.930821 0.05 Trânsito 2710±40 1.05 6045 [37]
Kepler-380c 0.113 7.630004 0.078 Trânsito 2710±40 1.05 6045 [37]
Kepler-381b 0.088 5.629021 0.066 Trânsito 878±5 1.34 6152 [37]
Kepler-381c 0.1 13.391635 0.117 Trânsito 878±5 1.34 6152 [37]
Kepler-382b 0.118 5.262155 0.055 Trânsito 3130±60 0.8 5600 [37]
Kepler-382c 0.142 12.162701 0.097 Trânsito 3130±60 0.8 5600 [37]
Kepler-383b 0.118 12.904532 0.095 Trânsito 1695 0.67 4710 [37]
Kepler-383c 0.111 31.200751 0.172 Trânsito 1695 0.67 4710 [37]
Kepler-384b 0.1 22.597053 0.148 Trânsito 2990±30 0.76 5577 [37]
Kepler-384c 0.101 45.348269 0.236 Trânsito 2990±30 0.76 5577 [37]
Kepler-385b 0.244 10.043686 0.097 Trânsito 4870±160 1.09 6326 [37]
Kepler-385c 0.271 15.163161 0.127 Trânsito 4870±160 1.09 6326 [37]
Kepler-386b 0.124 12.31043 0.096 Trânsito 2950±90 0.74 5178 [37]
Kepler-386c 0.141 25.193458 0.155 Trânsito 2950±90 0.74 5178 [37]
Kepler-387b 0.092 6.791636 0.068 Trânsito 2670±30 1.03 5774 [37]
Kepler-387c 0.079 11.837549 0.098 Trânsito 2670±30 1.03 5774 [37]
Kepler-388b 0.072 3.173315 0.036 Trânsito 2000±200 0.59 4498 [37]
Kepler-388c 0.077 13.297004 0.093 Trânsito 2000±200 0.59 4498 [37]
Kepler-389b 0.135 3.244107 0.041 Trânsito 2720±70 0.78 5376 [37]
Kepler-389c 0.13 14.51143 0.11 Trânsito 2720±70 0.78 5376 [37]
Kepler-390b 0.073 6.738088 0.065 Trânsito 1437±12 0.67 5166 [37]
Kepler-390c 0.07 13.060022 0.101 Trânsito 1437±12 0.67 5166 [37]
Kepler-391b 0.285 7.416755 0.082 Trânsito 2900±40 1.22 4940 [37]
Kepler-391c 0.316 20.485435 0.161 Trânsito 2900±40 1.22 4940 [37]
Kepler-392b 0.089 5.341853 0.059 Trânsito 2260±20 1.13 5938 [37]
Kepler-392c 0.098 10.423118 0.093 Trânsito 2260±20 1.13 5938 [37]
Kepler-393b 0.115 9.182417 0.091 Trânsito 2940±40 1.32 6189 [37]
Kepler-393c 0.119 14.613612 0.124 Trânsito 2940±40 1.32 6189 [37]
Kepler-394b 0.143 8.005013 0.083 Trânsito 3560±80 1.11 6402 [37]
Kepler-394c 0.148 12.130686 0.11 Trânsito 3560±80 1.11 6402 [37]
Kepler-395b 0.092 7.054346 0.061 Trânsito 1390±20 0.53 4262 [37]
Kepler-395c 0.118 34.989262 0.177 Trânsito 1390±20 0.53 4262 Exoplaneta potencialmente habitável[37]
Kepler-397b 0.219 22.250949 0.144 Trânsito 3760 5307 [37]
Kepler-397c 0.551 135.498527 0.48 Trânsito 3760 5307 [37]
Kepler-398b 0.083 4.081423 0.044 Trânsito 581.4±1.8 4493 [37]
Kepler-398c 0.09 11.419412 0.087 Trânsito 581.4±1.8 4493 [37]
Kepler-399b 0.086 14.425281 0.103 Trânsito 4400±700 5502 [37]
Kepler-399c 0.128 26.67569 0.155 Trânsito 4400±700 5502 [37]
Kepler-399d 0.169 58.034616 0.261 Trânsito 4400±700 5502 [37]
Kepler-400b 0.147 9.024389 0.087 Trânsito 2340 5886 [37]
Kepler-400c 0.133 17.340824 0.134 Trânsito 2340 5886 [37]
Kepler-401b 0.153 14.383035 0.122 Trânsito 3230±50 6117 [37]
Kepler-401c 0.192 47.318218 0.269 Trânsito 3230±50 6117 [37]
Kepler-402b 0.109 4.028751 0.051 Trânsito 2070±20 6090 [37]
Kepler-402c 0.139 6.124821 0.068 Trânsito 2070±20 6090 [37]
Kepler-402d 0.123 8.921099 0.087 Trânsito 2070±20 6090 [37]
Kepler-402e 0.13 11.242861 0.102 Trânsito 2070±20 6090 [37]
Kepler-403b 0.112 7.031462 0.076 Trânsito 2800±50 6090 [37]
Kepler-403c 0.156 54.280749 0.297 Trânsito 2800±50 6090 [37]
Kepler-404b 0.113 11.829851 0.102 Trânsito 2710±40 5654 [37]
Kepler-404c 0.153 14.751166 0.118 Trânsito 2710±40 5654 [37]
Kepler-405b 0.186 10.613839 0.095 Trânsito 3570±140 5818 [37]
Kepler-405c 0.416 29.726682 0.188 Trânsito 3570±140 5818 [37]
Kepler-406b 0.02 0.128 2.42629 Trânsito 1199±11 1.07 5538 [38]
Kepler-406c 0.009 0.076 4.62332 Trânsito 1199±11 1.07 5538 [38]
Kepler-407b 0.095 0.66931 Trânsito 1114±8 1 5476 [38]
Kepler-407c 12.6 3000 Vel. radial 1114±8 1 5476 [38]
Kepler-408b 0.073 2.46502 Trânsito 290.3±0.9 1.08 6104 Estrela-mãe conhecida como HD 176693 ou KOI-1612. Relatado como 2.1% provável falso positivo em 2014,[38] mas confirmado em 2016[40]
Kepler-409b 0.106 68.9584 Trânsito 222.8±0.3 0.92 5460 Estrela-mãe conhecida como Gliese 409[38]
Kepler-412b 0.941 1.341 1.7208604 0.02897 Trânsito 3650±60 1.17 5750 [41]
Kepler-413b 0.211 0.388 66.262 0.3553 Trânsito 2830±70 0.82 4700 [42]
Kepler-414b 0.011 0.153 4.7 Tempo 1364±9 0.89 [43]
Kepler-414c 0.094 0.269 7.171 Tempo 1364±9 0.89 [43]
Kepler-415b 0.377 0.108 4.176 Tempo 1750±30 0.67 [43]
Kepler-415c 8.708 Trânsito 1750±30 0.67 ?
Kepler-416b 0.183 0.221 6.319 Tempo 2290±30 1 [43]
Kepler-416c 12.209 Trânsito 2290±30 1 ?
Kepler-417b 0.035 0.206 12.331 Trânsito 3250±150 0.9 [43]
Kepler-417c 15.943 Trânsito 3250±150 0.9 ?
Kepler-418b 1.1 1.2 86.67856 Trânsito 3360±60 0.98 5820 [44]
Kepler-419b 2.5 0.96 69.7546 0.37 Trânsito 3390±80 1.39 6430 [45]
Kepler-419c 7.3 675.47 1.68 Tempo 3390±80 1.39 6430 [45]
Kepler-420Ab 1.45 0.94 86.647661 0.382 511 Trânsito 2900 0.99 5520 [46]
Kepler-421b 0.371 704.1984 1.219 Trânsito 1148±6 0.79 5308 [47]
Kepler-422b 0.43 1.15 7.8914483 0.082 Trânsito 2400±20 1.15 5972 [48]
Kepler-423b 0.595 1.192 2.6843285 0.03585 1605 Trânsito 2520±40 0.85 5560 [48]
Kepler-424b 1.03 0.89 3.3118644 0.044 Trânsito 2320±30 1.01 5460 [48]
Kepler-424c 6.97 223.3 0.73 Vel. radial 2320±30 1.01 5460 [48]
Kepler-425b 0.25 0.978 3.79701816 0.0464 1070 Trânsito 2140±30 0.93 5170 [49]
Kepler-426b 0.34 1.09 3.21751883 0.0414 1300 Trânsito 2810±40 0.91 5725 [49]
Kepler-427b 0.29 1.23 10.290994 0.091 1100 Trânsito 3410±50 0.96 5800 [49]
Kepler-428b 1.27 1.08 3.52563254 0.0433 1070 Trânsito 2280±50 0.87 5150 [49]
Kepler-430b 0.29 35.968 0.2244 667 Trânsito 3070±50 1.17 5884 [50]
Kepler-430c 0.16 110.979 0.4757 458 Trânsito 3070±50 1.17 5884 [50]
Kepler-431b 0.068 6.803 0.0719 1032 Trânsito 1609±15 1.07 6004 [50]
Kepler-431c 0.06 8.703 0.0847 951 Trânsito 1609±15 1.07 6004 [50]
Kepler-431d 0.1 11.922 0.1045 856 Trânsito 1609±15 1.07 6004 [50]
Kepler-432b 5.41 1.145 52.501129 0.301 Trânsito 2830±60 1.32 4995 Órbita excêntrica[51]
Kepler-432c 2.43+0.22
−0.24 		406.2+3.9
−2.5 		Vel. radial 2830±60 1.32 4995 [51]
Kepler-453b 0.00063 0.553 240.503 0.7903 Trânsito 1463±9 0.94 5527 [52]
Mu Leonis b 2.4 357.8 1.1 Vel. radial 133.0 1.5 4538.2 [3]
OGLE-2008-BLG-355Lb 4.6 1.7 Microlente 22000 0.37 [53]
OGLE-2008-BLG-92Lb 0.18 18 Microlente 26000 0.71 [54]
OGLE-2011-BLG-265Lb 0.88 1.89 Microlente 14300 0.21 [55]
OGLE-2013-BLG-102Lb 12.569 0.8 Microlente 9900 0.1 Planeta adicional ou anã marrom no sistema[56]
OGLE-2013-BLG-341LBb 0.0073 0.883 Microlente 3790 0.15 Mais uma anã vermelha no sistema[57]
OGLE-2014-BLG-0124Lb 0.51 3.11 Microlente 13000 0.71 [58]
SAND364 b 1.54 121.71 Vel. radial 2730±130 1.35 4284 Pertence a Messier 67, também conhecido como BD+12 1917b[59]
TYC 1422-614-1 b 2.5 198.4 0.69 Vel. radial 2480 1.15 4806 [60]
TYC 1422-614-1 c 10 559.3 1.37 Vel. radial 2480 1.15 4806 [60]
WASP-20Ab 0.72±0,06 1.32±0.03 3.16158 0.04317 Trânsito 663.39 1.05 5990 Binário com planeta orbitando estrela primária[61][62]
WASP-74b 0.95 1.56 2.13775 0.037 1910 Trânsito 390 1.48 5970 [63]
WASP-83b 0.3 1.04 4.971252 0.059 1120 Trânsito 980 1.11 5510 [63]
WASP-85Ab 1.265 1.24 2.6556777 0.039 1452 Trânsito 243 1.09 6112 [64]
WASP-87b 2.18±0.15 1.39±0.06 1.6828 0.0295±0.0008 Trânsito 982±12 1.20±0.09 6450±120 [65] Estrela-mãe também conhecida como CD-52 4998.
WASP-89b 5.9 1.04 3.3564227 0.0427 1120 Trânsito 957 0.92 5130 [63]
WASP-94Ab 0.452 1.72 3.9501907 0.055 1604 Trânsito 590 1.45 6153 [66]
WASP-94Bb 0.618 2.00839 0.0335 Vel. radial 590 1.24 6040 [66]
WASP-103b 1.49 1.528 0.925542 0.01985 2508 Trânsito 1500 1.22 6110 Planeta perto da perturbação de maré[67][68]
WASP-104b 1.272 1.137 1.7554137 0.02918 1516 Trânsito 470 1.08 5475 [69]
WASP-106b 1.925 1.085 9.289715 0.0917 1140 Trânsito 920 1.19 6055 [69]
WASP-108b 1.167+0.092
−0.091 		1.215±0.040 2.6755463±0.0000021 0.0397±0.001 1590 Trânsito 717.6±0.3 1.167±0.092 6000±140 [65] Estrela-mãe também conhecida como TYC 8254-1624-1
WASP-109b 0.91±0.13 1.443±0.053 3.3190233±0.0000042 0.0463±0.0011 1695 Trânsito 1173±16 1.203±0.090 6520±140 [65] Estrela-mãe também conhecida como TYC 6184-1397-1
WASP-110b 0.515±0.064 1.238±0.056 3.7783977±0.0000031 0.0457±0.0012 1134 Trânsito 904±10 0.892±0.072 5400±140 [65]
WASP-111b 1.85±0.16 1.442±0.094 2.310965±0.0000034 0.03914±0.00098 2140 Trânsito 980±20 1.50±0.11 6400±150 [65] Estrela-mãe também conhecida como HD 208180
WASP-112b 0.88±0.12 1.191±0.049 3.0353992±0.0000038 0.0382±0.0011 1395 Trânsito 1900±40 0.807±0.073 5610±130 [65]
WASP-116b 0.59±0.05 1.43±0.07 6.61321±0.00002 0.0730±0.0011 1400±4 Trânsito 1770±60 1.25±0.18 5950±100 [64]
WASP-117b 0.2755 1.021 10.02165 0.09459 1024 Trânsito 518±2 1.13 6038 [70][71]
WASP-149b 1.02±0.04 1.32±0.04 1.332811±0.000001 0.0247±0.0004 1870±1 Trânsito 1770±60 1.12±0.17 5750±100 [64]
XO-2Sb 0.259 18.157 0.1344 Vel. radial 480 0.98 5399 [72]
XO-2Sc 1.37 120.8 0.4756 Vel. radial 480 0.98 5399 [72]
YBP 1194 b 0.32 6.959 Vel. radial 2920±100 1.01 5780 Pertence a Messier 67[59]
YBP 1514 b 0.4 5.118 Vel. radial 3060±100 0.96 5725 Pertence a Messier 67[59]

Listas específicas de exoplanetas

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Referências

  1. ↑ «The Extrasolar Planets Encyclopaedia». Consultado em 9 de novembro de 2015 
  2. ↑ a b c d e Moutou, C.; Lo Curto, G.; Mayor, M.; Bouchy, F.; Benz, W.; Lovis, C.; Naef, D.; Pepe, F.; Queloz, D.; Santos, N. C.; Ségransan, D.; Sousa, S. G.; Udry, S. (2014), «The HARPS search for southern extra-solar planets XXXVI: Five new long-period giant planets and a system update», Astronomy & Astrophysics, 576: A48, arXiv:1412.6591Acessível livremente, doi:10.1051/0004-6361/201424965 
  3. ↑ a b c Lee, B.-C.; et al. (2014). «Planetary Companions in K giants β Cancri, μ Leonis, and β Ursae Minoris». Astronomy & Astrophysics. 566. 7 páginas. Bibcode:2014A&A...566A..67L. arXiv:1405.2127Acessível livremente. doi:10.1051/0004-6361/201322608. A67 
  4. ↑ Moutou, C.; et al. (2014), «CoRoT-22 b: A validated 4.9 R⊕ exoplanet in 10-d orbit★†», Monthly Notices of the Royal Astronomical Society, 444 (3): 2783–2792, arXiv:1408.2576Acessível livremente, doi:10.1093/mnras/stu1645 
  5. ↑ a b Alonso, R.; et al. (2014), «Transiting exoplanets from the CoRoT space mission», Astronomy & Astrophysics, 567: A112, arXiv:1406.1270Acessível livremente, doi:10.1051/0004-6361/201118662 
  6. ↑ Parviainen, H.; et al. (2014), «Transiting exoplanets from the CoRoT space mission», Astronomy & Astrophysics, 562: A140, arXiv:1401.1122Acessível livremente, doi:10.1051/0004-6361/201323049 
  7. ↑ Raetz, St; Heras, A. M.; Fernández, M.; Casanova, V.; Marka, C. (2018), «Transit analysis of the CoRoT-5, CoRoT-8, CoRoT-12, CoRoT-18, CoRoT-20, and CoRoT-27 systems with combined ground- and space-based photometry», Monthly Notices of the Royal Astronomical Society, 483: 824–839, arXiv:1812.01536Acessível livremente, doi:10.1093/mnras/sty3085 
  8. ↑ Howard, Andrew W.; Marcy, Geoffrey W.; Fischer, Debra A.; Isaacson, Howard; Muirhead, Philip S.; Henry, Gregory W.; Boyajian, Tabetha S.; von Braun, Kaspar; Becker, Juliette C.; Wright, Jason T.; Johnson, John Asher (2014), «The Nasa-Uc-Uh Eta-Earth Program. Iv. A Low-Mass Planet Orbiting an M Dwarf 3.6 Pc from Earth», The Astrophysical Journal, 794 (1): 51, Bibcode:2014ApJ...794...51H, arXiv:1408.5645Acessível livremente, doi:10.1088/0004-637X/794/1/51 
  9. ↑ a b c d e f g h i Tuomi, Mikko; Jones, Hugh R. A.; Barnes, John R.; Anglada-Escudé, Guillem; Jenkins, James S. (2014), «Bayesian search for low-mass planets around nearby M dwarfs – estimates for occurrence rate based on global detectability statistics», Monthly Notices of the Royal Astronomical Society, 441 (2): 1545–1569, arXiv:1403.0430Acessível livremente, doi:10.1093/mnras/stu358 
  10. ↑ a b c Feng, Fabo; Butler, R. Paul; Shectman, Stephen A.; Crane, Jeffrey D.; Vogt, Steve; Chambers, John; Jones, Hugh R. A.; Wang, Sharon Xuesong; Teske, Johanna K.; Burt, Jenn; Díaz, Matías R.; Thompson, Ian B. (8 de janeiro de 2020). «Search for Nearby Earth Analogs. II. Detection of Five New Planets, Eight Planet Candidates, and Confirmation of Three Planets around Nine Nearby M Dwarfs». The Astrophysical Journal Supplement Series. 246 (1): 11. Bibcode:2020ApJS..246...11F. arXiv:2001.02577Acessível livremente. doi:10.3847/1538-4365/ab5e7c 
  11. ↑ Burt, Jennifer; Vogt, Steven S.; Butler, R. Paul; Hanson, Russell; Meschiari, Stefano; Rivera, Eugenio J.; Henry, Gregory W.; Laughlin, Gregory (2014). «The Lick–Carnegie exoplanet survey: Gliese 687 b: A Neptune-mass planet orbiting a nearby red dwarf». The Astrophysical Journal. 789 (2): 114. Bibcode:2014ApJ...789..114B. arXiv:1405.2929Acessível livremente. doi:10.1088/0004-637X/789/2/114 
  12. ↑ Wittenmyer, R. A.; et al. (agosto de 2014). «GJ 832c: A super-earth in the habitable zone». The Astrophysical Journal. 791 (2). 114 páginas. Bibcode:2014ApJ...791..114W. arXiv:1406.5587Acessível livremente. doi:10.1088/0004-637X/791/2/114. 114 
  13. ↑ Gorrini, P.; Astudillo-Defru, N.; Dreizler, S.; Damasso, M.; Díaz, R. F.; Bonfils, X.; Jeffers, S. V.; Barnes, J. R.; Del Sordo, F.; Almenara, J.-M.; Artigau, E.; Bouchy, F.; Charbonneau, D.; Delfosse, X.; Doyon, R.; Figueira, P.; Forveille, T.; Haswell, C. A.; López-González, M. J.; Melo, C.; Mennickent, R. E.; Gaisné, G.; Morales, N. Morales; Murgas, F.; Pepe, F.; Rodríguez, E.; Santos, N. C.; Tal-Or, L.; Tsapras, Y.; Udry, S. (2022), «Detailed stellar activity analysis and modelling of GJ 832», Astronomy & Astrophysics, 664: A64, arXiv:2206.07552Acessível livremente, doi:10.1051/0004-6361/202243063 
  14. ↑ a b c Astudillo-Defru, Nicola; Bonfils, Xavier; Delfosse, Xavier; Ségransan, Damien; Forveille, Thierry; Bouchy, François; Gillon, Michaël; Lovis, Christophe; Mayor, Michel; Neves, Vasco; Pepe, Francesco; Perrier, Christian; Queloz, Didier; Rojo, Patricio; Santos, Nuno C.; Udry, Stéphane (2015). «Planetary systems and stellar activity of the M dwarfs GJ 3293, GJ 3341, and GJ 3543». Astronomy & Astrophysics. 575: A119. Bibcode:2015A&A...575A.119A. arXiv:1411.7048v1Acessível livremente. doi:10.1051/0004-6361/201424253 
  15. ↑ Marie-Eve Naud; Étienne Artigau; Lison Malo; Loïc Albert; René Doyon; David Lafrenière; Jonathan Gagné; Didier Saumon; Caroline V. Morley; France Allard; Derek Homeier; Charles A. Beichman; Christopher R. Gelino; Anne Boucher (12 de maio de 2014). «Discovery of a Wide Planetary-mass Companion to the Young M3 Star GU Psc» (publicado em maio de 2014). The Astrophysical Journal. 787 (1): 16. Bibcode:2014ApJ...787....5N. arXiv:1405.2932Acessível livremente. doi:10.1088/0004-637X/787/1/5. 5 
  16. ↑ Bieryla, A.; Hartman, J. D.; Bakos, G. Á.; Bhatti, W.; Kovács, G.; Boisse, I.; Latham, D. W.; Buchhave, L. A.; Csubry, Z.; Penev, K.; De Val-Borro, M.; Béky, B.; Falco, E.; Torres, G.; Noyes, R. W.; Berlind, P.; Calkins, M. C.; Esquerdo, G. A.; Lázár, J.; Papp, I.; Sári, P. (2014), «HAT-P-49b: A 1.7MJPLANET TRANSITING a BRIGHT 1.5M☉F-STAR», The Astronomical Journal, 147 (4): 84, Bibcode:2014AJ....147...84B, arXiv:1401.5460Acessível livremente, doi:10.1088/0004-6256/147/4/84 
  17. ↑ Bakos, G. Á.; Hartman, J. D.; Bhatti, W.; Bieryla, A.; Val-Borro, M. de; Latham, D. W.; Buchhave, L. A.; Csubry, Z.; Penev, K.; Kovács, G.; Béky, B.; Falco, E.; Kovács, T.; Howard, A. W.; Johnson, J. A.; Isaacson, H.; Marcy, G. W.; Torres, G.; Noyes, R. W.; Berlind, P.; Calkins, M. L.; Esquerdo, G. A.; Lázár, J.; Papp, I.; Sári, P. (2014), «HAT-P-54b: A HOT JUPITER TRANSITING a 0.64M⊙STAR IN FIELD 0 OF THE K2 MISSION», The Astronomical Journal, 149 (4): 149, arXiv:1404.4417Acessível livremente, doi:10.1088/0004-6256/149/4/149 
  18. ↑ Crossfield, Ian J. M.; et al. (2021), «197 CANDIDATES AND 104 VALIDATED PLANETS IN K2 's FIRST FIVE FIELDS», The Astrophysical Journal Supplement Series, 226: 7, arXiv:1607.05263Acessível livremente, doi:10.3847/0067-0049/226/1/7 
  19. ↑ Saha, Suman; Chakrabarty, Aritra; Sengupta, Sujan (2021), «Multiband Transit Follow-up Observations of Five Hot Jupiters with Critical Noise Treatments: Improved Physical Properties», The Astronomical Journal, 162 (1): 18, Bibcode:2021AJ....162...18S, arXiv:2105.09668Acessível livremente, doi:10.3847/1538-3881/ac01dd 
  20. ↑ Jordán, Andrés; et al. (2014), «HATS-4b: A DENSE HOT JUPITER TRANSITING a SUPER METAL-RICH G STAR», The Astronomical Journal, 148 (2): 29, Bibcode:2014AJ....148...29J, arXiv:1402.6546Acessível livremente, doi:10.1088/0004-6256/148/2/29 
  21. ↑ Zhou, G.; Bayliss, D.; Penev, K.; Bakos, G. Á.; Hartman, J. D.; Jordán, A.; Mancini, L.; Mohler, M.; Csubry, Z.; Ciceri, S.; Brahm, R.; Rabus, M.; Buchhave, L.; Henning, T.; Suc, V.; Espinoza, N.; Béky, B.; Noyes, R. W.; Schmidt, B.; Butler, R. P.; Shectman, S.; Thompson, I.; Crane, J.; Sato, B.; Csák, B.; Lázár, J.; Papp, I.; Sári, P.; Nikolov, N. (2014), «HATS-5b: A TRANSITING HOT SATURN FROM THE HATSouth SURVEY», The Astronomical Journal, 147 (6): 144, Bibcode:2014AJ....147..144Z, arXiv:1401.1582Acessível livremente, doi:10.1088/0004-6256/147/6/144 
  22. ↑ Hartman, J. D.; Bayliss, D.; Brahm, R.; Bakos, G. Á.; Mancini, L.; Jordán, A.; Penev, K.; Rabus, M.; Zhou, G.; Butler, R. P.; Espinoza, N.; De Val-Borro, M.; Bhatti, W.; Csubry, Z.; Ciceri, S.; Henning, T.; Schmidt, B.; Arriagada, P.; Shectman, S.; Crane, J.; Thompson, I.; Suc, V.; Csák, B.; Tan, T. G.; Noyes, R. W.; Lázár, J.; Papp, I.; Sári, P. (2014), «HATS-6b: A WARM SATURN TRANSITING AN EARLY M DWARF STAR, AND a SET OF EMPIRICAL RELATIONS FOR CHARACTERIZING K AND M DWARF PLANET HOSTS», The Astronomical Journal, 149 (5): 166, arXiv:1408.1758Acessível livremente, doi:10.1088/0004-6256/149/5/166 
  23. ↑ Kane, Stephen R.; et al. (abril de 2014). «Limits on Stellar Companions to Exoplanet Host Stars with Eccentric Planets». The Astrophysical Journal. 785 (2). 10 páginas. Bibcode:2014ApJ...785...93K. arXiv:1401.1544Acessível livremente. doi:10.1088/0004-637X/785/2/93. 93 
  24. ↑ a b c d Giguere, Matthew J.; et al. (2015). «Newly Discovered Planets Orbiting HD 5319, HD 11506, HD 75784 and HD 10442 from the N2K Consortium». The Astrophysical Journal. 799 (1). 89. Bibcode:2015ApJ...799...89G. arXiv:1411.5374Acessível livremente. doi:10.1088/0004-637X/799/1/89 
  25. ↑ Wang, Liang; Sato, Bun'ei; Omiya, Masashi; Harakawa, Hiroki; Liu, Yujuan; Song, Nan; He, Wei; Wu, Xiaoshu; Izumiura, Hideyuki; Kambe, Eiji; Takeda, Yoichi; Yoshida, Michitoshi; Itoh, Yoichi; Ando, Hiroyasu; Kokubo, Eiichiro; Ida, Shigeru; Zhao, Gang (2014), «A long-period eccentric substellar companion to the evolved intermediate-mass star HD 14067», Publications of the Astronomical Society of Japan, 66 (6): 118, arXiv:1409.6081Acessível livremente, doi:10.1093/pasj/psu113 
  26. ↑ Acke, B.; van den Ancker, M. E. (16 de março de 2006). «Resolving the disk rotation of HD 97048 and HD 100546 in the [O I] 6300 Å line: evidence for a giant planet orbiting HD 100546». Astronomy & Astrophysics. 449 (1): 267–279. Bibcode:2006A&A...449..267A. arXiv:astro-ph/0512562Acessível livremente. doi:10.1051/0004-6361:20054330 
  27. ↑ a b Wittenmyer, Robert A.; et al. (2014). «The Anglo-Australian Planet Search. XXIII. Two New Jupiter Analogs». The Astrophysical Journal. 783 (2). 103 páginas. Bibcode:2014ApJ...783..103W. arXiv:1401.5525Acessível livremente. doi:10.1088/0004-637X/783/2/103 
  28. ↑ a b c d Vogt, Steven S.; Butler, R. Paul; Rivera, Eugenio J.; Kibrick, Robert; Burt, Jennifer; Hanson, Russell; Meschiari, Stefano; Henry, Gregory W.; Laughlin, Gregory (2014), «A Four-Planet System Orbiting the K0V Star Hd 141399», The Astrophysical Journal, 787 (2): 97, Bibcode:2014ApJ...787...97V, arXiv:1404.7462Acessível livremente, doi:10.1088/0004-637X/787/2/97 
  29. ↑ a b Jones, M. I.; Jenkins, J. S.; Rojo, P.; Melo, C. H. F.; Bluhm, P. (2015), «A planetary system and a highly eccentric brown dwarf around the giant stars HIP 67851 and HIP 97233», Astronomy & Astrophysics, 573: A3, Bibcode:2015A&A...573A...3J, arXiv:1409.7429Acessível livremente, doi:10.1051/0004-6361/201424771 
  30. ↑ Wittenmyer, Robert A.; Wang, Liang; Liu, Fan; Horner, Jonathan; Endl, Michael; Johnson, John Asher; Tinney, C. G.; Carter, B. D. (2014), «The Pan-Pacific Planet Search. Ii. Confirmation of a Two-Planet System Around Hd 121056», The Astrophysical Journal, 800: 74, arXiv:1412.6889Acessível livremente, doi:10.1088/0004-637X/800/1/74 
  31. ↑ Jones, M. I.; Jenkins, J. S.; Bluhm, P.; Rojo, P.; Melo, C. H. F. (2014), «The properties of planets around giant stars», Astronomy & Astrophysics, 566: A113, Bibcode:2014A&A...566A.113J, arXiv:1406.0884Acessível livremente, doi:10.1051/0004-6361/201323345 
  32. ↑ Vanderburg, Andrew; et al. (fevereiro de 2015). «Characterizing K2 Planet Discoveries: A super-Earth transiting the bright K-dwarf HIP 116454». The Astrophysical Journal. 800 (1). 59. Bibcode:2015ApJ...800...59V. arXiv:1412.5674Acessível livremente. doi:10.1088/0004-637X/800/1/59 
  33. ↑ a b Anglada-Escudé, Guillem; et al. (2014), «Two planets around Kapteyn's star : a cold and a temperate super-Earth orbiting the nearest halo red-dwarf», Monthly Notices of the Royal Astronomical Society: Letters, 443: L89–L93, Bibcode:2014MNRAS.443L..89A, arXiv:1406.0818Acessível livremente, doi:10.1093/mnrasl/slu076 
  34. ↑ a b Bortle, Anna; Fausey, Hallie; Ji, Jinbiao; Dodson-Robinson, Sarah; Ramirez Delgado, Victor; Gizis, John (2021), «A Gaussian Process Regression Reveals No Evidence for Planets Orbiting Kapteyn's Star», The Astronomical Journal, 161 (5): 230, Bibcode:2021AJ....161..230B, arXiv:2103.02709Acessível livremente, doi:10.3847/1538-3881/abec89 
  35. ↑ a b c Silvotti, R.; Charpinet, S.; Green, E.; Fontaine, G.; Telting, J. H.; Østensen, R. H.; Van Grootel, V.; Baran, A. S.; Schuh, S.; Fox Machado, L. (2014), «Keplerdetection of a new extreme planetary system orbiting the subdwarf-B pulsator KIC 10001893», Astronomy & Astrophysics, 570: A130, Bibcode:2014A&A...570A.130S, arXiv:1409.6975Acessível livremente, doi:10.1051/0004-6361/201424509 
  36. ↑ a b c Blokesz, A.; et al. (julho de 2019). «Analysis of putative exoplanetary signatures found in light curves of two sdBV stars observed by Kepler». Astronomy & Astrophysics. 627: A86. Bibcode:2019A&A...627A..86B. arXiv:1906.03321Acessível livremente. doi:10.1051/0004-6361/201835003 
  37. ↑ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al am an ao ap aq ar as at au av aw ax ay az ba bb bc bd be bf bg bh bi bj bk bl bm bn bo bp bq br bs bt bu bv bw bx by bz ca cb cc cd ce cf cg ch ci cj ck cl cm cn co cp cq cr cs ct cu cv cw cx cy cz da db dc dd de df dg dh di dj dk dl dm dn do dp dq dr ds dt du dv dw dx dy dz ea eb ec ed ee ef eg eh ei ej ek el em en eo ep eq er es et eu ev ew ex ey ez fa fb fc fd fe ff fg fh fi fj fk fl fm fn fo fp fq fr fs ft fu fv fw fx fy fz ga gb gc gd ge gf gg gh gi gj gk gl gm gn go gp gq gr gs gt gu gv gw gx gy gz ha hb hc hd he hf hg hh hi hj hk hl hm hn ho hp hq hr hs ht hu hv hw hx hy hz ia ib ic id ie if ig ih ii ij ik il im in io ip iq ir is it iu iv iw ix iy iz ja jb jc jd je jf jg jh ji jj jk jl jm jn jo jp jq jr js jt ju jv jw jx jy jz ka kb kc kd ke kf kg kh ki kj kk kl km kn ko kp kq kr ks kt ku kv kw kx ky kz la lb lc ld le lf lg lh li lj lk ll lm ln lo lp lq lr ls lt lu lv lw lx ly lz ma mb mc md me mf mg mh mi mj mk ml mm mn mo mp mq mr ms mt mu mv mw mx my mz na nb nc nd ne nf ng nh ni nj nk nl nm nn no np nq nr ns nt nu nv nw nx ny nz oa ob oc od oe of og oh oi oj ok ol om on oo op oq or os ot ou ov ow ox oy oz pa pb pc pd pe pf pg ph pi pj pk pl pm pn po pp pq pr ps pt pu pv pw px py pz qa qb qc qd qe qf qg qh qi qj qk ql qm qn qo qp qq qr qs qt qu qv qw qx qy qz ra rb rc rd re rf rg rh ri rj rk rl rm rn ro rp rq rr rs rt ru rv rw rx ry rz sa sb sc sd se sf sg sh si sj sk sl sm sn so sp sq sr ss st su sv sw sx sy sz ta tb tc td te tf tg th ti tj tk tl tm tn to tp tq tr ts tt tu tv tw tx ty tz ua ub uc ud ue uf ug uh ui uj uk ul um un uo up uq ur us ut uu uv uw ux uy uz va vb vc vd ve vf vg vh vi vj vk vl vm vn vo vp vq vr vs vt vu vv vw vx vy vz wa wb wc wd we wf wg wh wi wj wk wl wm wn wo wp wq wr ws wt wu wv ww wx wy wz xa xb xc xd xe xf xg xh xi xj xk xl xm xn xo xp xq xr xs xt xu xv xw xx xy xz ya yb yc yd ye yf yg yh yi yj yk yl ym yn yo yp yq yr ys yt yu yv yw yx yy yz za zb zc zd ze zf zg zh zi zj zk zl zm zn zo zp zq zr zs zt zu zv zw zx zy zz aaa aab aac aad aae aaf aag aah aai aaj aak aal aam aan aao aap aaq aar aas aat aau aav aaw aax aay aaz aba abb abc abd abe abf abg abh Rowe, Jason F.; Bryson, Stephen T.; Marcy, Geoffrey W.; Lissauer, Jack J.; Jontof-Hutter, Daniel; Mullally, Fergal; Gilliland, Ronald L.; Issacson, Howard; Ford, Eric; Howell, Steve B.; Borucki, William J.; Haas, Michael; Huber, Daniel; Steffen, Jason H.; Thompson, Susan E.; Quintana, Elisa; Barclay, Thomas; Still, Martin; Fortney, Jonathan; Gautier, T. N.; Hunter, Roger; Caldwell, Douglas A.; Ciardi, David R.; Devore, Edna; Cochran, William; Jenkins, Jon; Agol, Eric; Carter, Joshua A.; Geary, John (2014), «Validation Ofkepler's Multiple Planet Candidates. III. Light Curve Analysis and Announcement of Hundreds of New Multi-Planet Systems», The Astrophysical Journal, 784 (1): 45, Bibcode:2014ApJ...784...45R, arXiv:1402.6534Acessível livremente, doi:10.1088/0004-637X/784/1/45 
  38. ↑ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al Marcy, Geoffrey W.; et al. (2014), «Masses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets», The Astrophysical Journal Supplement Series, 210 (2): 20, Bibcode:2014ApJS..210...20M, arXiv:1401.4195Acessível livremente, doi:10.1088/0067-0049/210/2/20 
  39. ↑ a b Heller, René; Hippke, Michael; Freudenthal, Jantje; Rodenbeck, Kai; Batalha, Natalie M.; Bryson, Steve (2020). «Transit least-squares survey». Astronomy & Astrophysics. 638: A10. arXiv:2006.02123Acessível livremente. doi:10.1051/0004-6361/201936929 
  40. ↑ Campante, T. L.; Lund, M. N.; Kuszlewicz, J. S.; Davies, G. R.; Chaplin, W. J.; Albrecht, S.; Winn, J. N.; Bedding, T. R.; Benomar, O.; Bossini, D.; Handberg, R.; Santos, A. R. G.; Van Eylen, V.; Basu, S.; Christensen-Dalsgaard, J.; Elsworth, Y. P.; Hekker, S.; Hirano, T.; Huber, D.; Karoff, C.; Kjeldsen, H.; Lundkvist, M. S.; North, T. S. H.; Silva Aguirre, V.; Stello, D.; White, T. R. (2016), «Spin–Orbit Alignment of Exoplanet Systems: Ensemble Analysis Using Asteroseismology», The Astrophysical Journal, 819 (1): 85, Bibcode:2016ApJ...819...85C, arXiv:1601.06052Acessível livremente, doi:10.3847/0004-637X/819/1/85 
  41. ↑ «SOPHIE velocimetry of Kepler transit candidates XI. Kepler-412 system: probing the properties of a new inflated hot Jupiter» (PDF). www.aanda.org 
  42. ↑ Kostov, V. B.; McCullough, P. R.; Carter, J. A.; Deleuil, M.; Díaz, R. F.; Fabrycky, D. C.; Hébrard, G.; Hinse, T. C.; Mazeh, T.; Orosz, J. A.; Tsvetanov, Z. I.; Welsh, W. F. (2014), «Kepler-413B: A Slightly Misaligned, Neptune-Size Transiting Circumbinary Planet», The Astrophysical Journal, 784 (1): 14, Bibcode:2014ApJ...784...14K, arXiv:1401.7275Acessível livremente, doi:10.1088/0004-637X/784/1/14 
  43. ↑ a b c d e Ver Table 2. Planet Nominal Masses in Hadden, Sam; Lithwick, Yoram (2014). «Densities and Eccentricities of 139Keplerplanets from Transit Time Variations». The Astrophysical Journal. 787 (1): 80. Bibcode:2014ApJ...787...80H. arXiv:1310.7942Acessível livremente. doi:10.1088/0004-637X/787/1/80 
  44. ↑ Tingley, B.; Parviainen, H.; Gandolfi, D.; Deeg, H. J.; Palle, E.; Montañés Rodriguez, P.; Murgas, F.; Alonso, R.; Bruntt, H.; Fridlund, M. (2014), «Confirmation of an exoplanet using the transit color signature: Kepler-418b, a blended giant planet in a multiplanet system», Astronomy & Astrophysics, 567: A14, Bibcode:2014A&A...567A..14T, arXiv:1405.5354Acessível livremente, doi:10.1051/0004-6361/201323175 
  45. ↑ a b Dawson, Rebekah I.; Johnson, John Asher; Fabrycky, Daniel C.; Foreman-Mackey, Daniel; Murray-Clay, Ruth A.; Buchhave, Lars A.; Cargile, Phillip A.; Clubb, Kelsey I.; Fulton, Benjamin J.; Hebb, Leslie; Howard, Andrew W.; Huber, Daniel; Shporer, Avi; Valenti, Jeff A. (2014), «Large Eccentricity, Low Mutual Inclination: The Three-Dimensional Architecture of a Hierarchical System of Giant Planets», The Astrophysical Journal, 791 (2): 89, Bibcode:2014ApJ...791...89D, arXiv:1405.5229Acessível livremente, doi:10.1088/0004-637X/791/2/89 
  46. ↑ Santerne, A.; et al. (2014), «SOPHIE velocimetry of Keplertransit candidates», Astronomy & Astrophysics, 571: A37, arXiv:1406.6172Acessível livremente, doi:10.1051/0004-6361/201424158 
  47. ↑ Kipping, D. M.; Torres, G.; Buchhave, L. A.; Kenyon, S. J.; Henze, C.; Isaacson, H.; Kolbl, R.; Marcy, G. W.; Bryson, S. T.; Stassun, K.; Bastien, F. (2014), «Discovery of a Transiting Planet Near the Snow-Line», The Astrophysical Journal, 795 (1): 25, Bibcode:2014ApJ...795...25K, arXiv:1407.4807Acessível livremente, doi:10.1088/0004-637X/795/1/25 
  48. ↑ a b c d Endl, Michael; Caldwell, Douglas A.; Barclay, Thomas; Huber, Daniel; Isaacson, Howard; Buchhave, Lars A.; Brugamyer, Erik; Robertson, Paul; Cochran, William D.; MacQueen, Phillip J.; Havel, Mathieu; Lucas, Phillip; Howell, Steve B.; Fischer, Debra; Quintana, Elisa; Ciardi, David R. (2014), «KEPLER-424 b: A "LONELY" HOT JUPITER THAT FOUND a COMPANION», The Astrophysical Journal, 795 (2): 151, Bibcode:2014ApJ...795..151E, arXiv:1409.8156Acessível livremente, doi:10.1088/0004-637X/795/2/151 
  49. ↑ a b c d Hébrard, G.; Santerne, A.; Montagnier, G.; Bruno, G.; Deleuil, M.; Havel, M.; Almenara, J.-M.; Damiani, C.; Barros, S. C. C.; Bonomo, A. S.; Bouchy, F.; Díaz, R. F.; Moutou, C. (2014), «Characterization of the four new transiting planets KOI-188b, KOI-195b, KOI-192b, and KOI-830b», Astronomy & Astrophysics, 572: A93, Bibcode:2014A&A...572A..93H, arXiv:1409.8554Acessível livremente, doi:10.1051/0004-6361/201424268 
  50. ↑ a b c d e Everett, Mark E.; Barclay, Thomas; Ciardi, David R.; Horch, Elliott P.; Howell, Steve B.; Crepp, Justin R.; Silva, David R. (2014), «High-Resolution Multi-Band Imaging for Validation and Characterization of Smallkeplerplanets», The Astronomical Journal, 149 (2): 55, arXiv:1411.3621Acessível livremente, doi:10.1088/0004-6256/149/2/55 
  51. ↑ a b Quinn, Samuel N.; White, Timothy R.; Latham, David W.; Chaplin, William J.; Handberg, Rasmus; Huber, Daniel; Kipping, David M.; Payne, Matthew J.; Jiang, Chen; Victor Silva Aguirre; Stello, Dennis; Sliski, David H.; Ciardi, David R.; Buchhave, Lars A.; Bedding, Timothy R.; Davies, Guy R.; Hekker, Saskia; Kjeldsen, Hans; Everett, Mark E.; Howell, Steve B.; Basu, Sarbani; Campante, Tiago L.; Christensen-Dalsgaard, Jørgen; Elsworth, Yvonne P.; Karoff, Christoffer; Kawaler, Steven D.; Lund, Mikkel N.; Lundkvist, Mia; Esquerdo, Gilbert A.; et al. (2014). «Kepler-432: A red giant interacting with one of its two long period giant planets». The Astrophysical Journal. 803 (2). 49 páginas. Bibcode:2015ApJ...803...49Q. arXiv:1411.4666Acessível livremente. doi:10.1088/0004-637X/803/2/49 
  52. ↑ Welsh, William F.; et al. (2015). «KIC 9632895 - The 10th Kepler Transiting Circumbinary Planet». The Astrophysical Journal. 809 (1). 26. Bibcode:2015ApJ...809...26W. arXiv:1409.1605Acessível livremente. doi:10.1088/0004-637X/809/1/26 
  53. ↑ Koshimoto, N.; et al. (2014), «OGLE-2008-BLG-355Lb: A MASSIVE PLANET AROUND a LATE-TYPE STAR», The Astrophysical Journal, 788 (2): 128, Bibcode:2014ApJ...788..128K, arXiv:1403.7005Acessível livremente, doi:10.1088/0004-637X/788/2/128 
  54. ↑ Poleski, Radosław; Skowron, Jan; Udalski, Andrzej; Han, Cheongho; Kozłowski, Szymon; Wyrzykowski, Łukasz; Dong, Subo; Szymański, Michał K.; Kubiak, Marcin; Pietrzyński, Grzegorz; Soszyński, Igor; Ulaczyk, Krzysztof; Pietrukowicz, Paweł; Gould, Andrew (2014), «Triple Microlens Ogle-2008-BLG-092L: Binary Stellar System with a Circumprimary Uranus-Type Planet», The Astrophysical Journal, 795 (1): 42, Bibcode:2014ApJ...795...42P, arXiv:1408.6223Acessível livremente, doi:10.1088/0004-637X/795/1/42 
  55. ↑ Skowron, J.; et al. (2014), «OGLE-2011-BLG-0265Lb: A JOVIAN MICROLENSING PLANET ORBITING AN M DWARF», The Astrophysical Journal, 804: 33, arXiv:1410.8252Acessível livremente, doi:10.1088/0004-637X/804/1/33 
  56. ↑ Jung, Y. K.; et al. (2014), «Ogle-2013-BLG-0102La,B: Microlensing Binary with Components at Star/Brown Dwarf and Brown Dwarf/Planet Boundaries», The Astrophysical Journal, 798 (2): 123, arXiv:1407.7926Acessível livremente, doi:10.1088/0004-637X/798/2/123 
  57. ↑ Gould, A.; et al. (2014), «A terrestrial planet in a ~1-AU orbit around one member of a ∼15-AU binary», Science, 345 (6192): 46–49, Bibcode:2014Sci...345...46G, PMID 24994642, arXiv:1407.1115Acessível livremente, doi:10.1126/science.1251527 
  58. ↑ Udalski, A.; Yee, J. C.; Gould, A.; Carey, S.; Zhu, W.; Skowron, J.; Kozłowski, S.; Poleski, R.; Pietrukowicz, P.; Pietrzyński, G.; Szymański, M. K.; Mróz, P.; Soszyński, I.; Ulaczyk, K.; Wyrzykowski, Ł.; Han, C.; Calchi Novati, S.; Pogge, R. W. (2014), «Spitzeras a Microlens Parallax Satellite: Mass Measurement for the Ogle-2014-BLG-0124L Planet and ITS Host Star», The Astrophysical Journal, 799 (2): 237, arXiv:1410.4219Acessível livremente, doi:10.1088/0004-637X/799/2/237 
  59. ↑ a b c Brucalassi, A.; Pasquini, L.; Saglia, R.; Ruiz, M. T.; Bonifacio, P.; Bedin, L. R.; Biazzo, K.; Melo, C.; Lovis, C.; Randich, S. (2014), «Three planetary companions around M 67 stars», Astronomy & Astrophysics, 561: L9, Bibcode:2014A&A...561L...9B, arXiv:1401.4905Acessível livremente, doi:10.1051/0004-6361/201322584 
  60. ↑ a b Niedzielski, A.; Villaver, E.; Wolszczan, A.; Adamów, M.; Kowalik, K.; MacIejewski, G.; Nowak, G.; García-Hernández, D. A.; Deka, B.; Adamczyk, M. (2014), «Tracking Advanced Planetary Systems (TAPAS) with HARPS-N», Astronomy & Astrophysics, 573: A36, arXiv:1410.5971Acessível livremente, doi:10.1051/0004-6361/201424399 
  61. ↑ Anderson, D. R.; Collier Cameron, A.; Hellier, C.; Lendl, M.; Lister, T. A.; Maxted, P. F. L.; Queloz, D.; Smalley, B.; Smith, A. M. S.; Triaud, A. H. M. J.; Brown, D. J. A.; Gillon, M.; Neveu-Vanmalle, M.; Pepe, F.; Pollacco, D.; Ségransan, D.; Udry, S.; West, R. G.; Wheatley, P. J. (2015). «WASP-20b and WASP-28b: A hot Saturn and a hot Jupiter in near-aligned orbits around solar-type stars». Astronomy & Astrophysics. 575: A61. Bibcode:2015A&A...575A..61A. arXiv:1402.1482Acessível livremente. doi:10.1051/0004-6361/201423591 
  62. ↑ Evans, Daniel F.; Southworth, John; Smalley, Barry (2016). «Wasp-20 is a Close Visual Binary with a Transiting Hot Jupiter». The Astrophysical Journal. 833 (2): L19. Bibcode:2016ApJ...833L..19E. arXiv:1611.08735Acessível livremente. doi:10.3847/2041-8213/833/2/L19 
  63. ↑ a b c Hellier, Coel; Anderson, D. R.; Collier Cameron, A.; Delrez, L.; Gillon, M.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Segransan, D.; Smalley, B.; Smith, A. M. S.; Southworth, J.; Triaud, A. H. M. J.; Turner, O. D.; Udry, S.; West, R. G. (2014), «Three WASP-South transiting exoplanets: WASP-74b, WASP-83b & WASP-89b», The Astronomical Journal, 150 (1): 18, Bibcode:2015AJ....150...18H, arXiv:1410.6358Acessível livremente, doi:10.1088/0004-6256/150/1/18 
  64. ↑ a b c Brown, D. J. A.; et al. (2014), Three transiting planet discoveries from the Wide Angle Search for Planets: WASP-85 A b; WASP-116 b, and WASP-149 b, arXiv:1412.7761Acessível livremente 
  65. ↑ a b c d e f Anderson, D. R.; Brown, D. J. A.; Collier Cameron, A.; Delrez, L.; Fumel, A.; Gillon, M.; Hellier, C.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Neveu-VanMalle, M.; Pepe, F.; Pollacco, D.; Queloz, D.; Rojo, P.; Segransan, D.; Serenelli, A. M.; Smalley, B.; Smith, A. M. S.; Southworth, J.; Triaud, A. H. M. J.; Turner, O. D.; Udry, S.; West, R. G. (2014), Six newly-discovered hot Jupiters transiting F/G stars: WASP-87b, WASP-108b, WASP-109b, WASP-110b, WASP-111b & WASP-112b, arXiv:1410.3449Acessível livremente 
  66. ↑ a b Neveu-Vanmalle, M.; Queloz, D.; Anderson, D. R.; Charbonnel, C.; Collier Cameron, A.; Delrez, L.; Gillon, M.; Hellier, C.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Ségransan, D.; Smalley, B.; Smith, A. M. S.; Southworth, J.; Triaud, A. H. M. J.; Udry, S.; West, R. G. (2014), «WASP-94 a and B planets: Hot-Jupiter cousins in a twin-star system», Astronomy & Astrophysics, 572: A49, Bibcode:2014A&A...572A..49N, arXiv:1409.7566Acessível livremente, doi:10.1051/0004-6361/201424744 
  67. ↑ Gillon, M.; Anderson, D. R.; Collier-Cameron, A.; Delrez, L.; Hellier, C.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smith, A. M. S.; Smalley, B.; Southworth, J.; Triaud, A. H. M. J.; Udry, S.; Van Grootel, V.; West, R. G. (2014), «WASP-103 b: A new planet at the edge of tidal disruption», Astronomy & Astrophysics, 562: L3, Bibcode:2014A&A...562L...3G, arXiv:1401.2784Acessível livremente, doi:10.1051/0004-6361/201323014 
  68. ↑ Southworth, John; Mancini, L.; Ciceri, S.; Budaj, J.; Dominik, M.; Figuera Jaimes, R.; Haugbølle, T.; Jørgensen, U. G.; Popovas, A.; Rabus, M.; Rahvar, S.; von Essen, C.; Schmidt, R. W.; Wertz, O.; Alsubai, K. A.; Bozza, V.; Bramich, D. M.; Calchi Novati, S.; d'Ago, G.; Hinse, T. C.; Henning, Th.; Hundertmark, M.; Juncher, D.; Korhonen, H.; Skottfelt, J.; Snodgrass, C.; Starkey, D.; Surdej, J. (2014), «High-precision photometry by telescope defocusing – VII. The ultrashort period planet WASP-103★», Monthly Notices of the Royal Astronomical Society, 447: 711–721, arXiv:1411.2767Acessível livremente, doi:10.1093/mnras/stu2394 
  69. ↑ a b Smith, A. M. S.; et al. (2014). «WASP-104b and WASP-106b: Two transiting hot Jupiters in 1.75-day and 9.3-day orbits». Astronomy and Astrophysics. 570. A64. Bibcode:2014A&A...570A..64S. arXiv:1408.0887Acessível livremente. doi:10.1051/0004-6361/201424752 
  70. ↑ Lendl, M.; Triaud, A. H. M. J.; Anderson, D. R.; Collier Cameron, A.; Delrez, L.; Doyle, A. P.; Gillon, M.; Hellier, C.; Jehin, E.; Maxted, P. F. L.; Neveu-Vanmalle, M.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, B.; Smith, A. M. S.; Udry, S.; Van Grootel, V.; West, R. G. (2014). «WASP-117b: A 10-day-period Saturn in an eccentric and misaligned orbit». Astronomy & Astrophysics. 568: A81. Bibcode:2014A&A...568A..81L. arXiv:1406.6942Acessível livremente. doi:10.1051/0004-6361/201424481 
  71. ↑ Carone, Ludmila; Mollière, Paul; Zhou, Yifan; Bouwman, Jeroen; Yan, Fei; Baeyens, Robin; Apai, Dániel; Espinoza, Nestor; Rackham, Benjamin V.; Jordán, Andrés; Angerhausen, Daniel; Decin, Leen; Lendl, Monika; Venot, Olivia; Henning, Thomas (2021). «Indications for very high metallicity and absence of methane in the eccentric exo-Saturn WASP-117b». Astronomy & Astrophysics. 646: A168. Bibcode:2021A&A...646A.168C. arXiv:2006.05382Acessível livremente. doi:10.1051/0004-6361/202038620 
  72. ↑ a b Desidera, S.; et al. (2014), «The GAPS programme with HARPS-N at TNG», Astronomy & Astrophysics, 567: L6, arXiv:1407.0251Acessível livremente, doi:10.1051/0004-6361/201424339 
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