Lista de exoplanetas descobertos em 2021
Esta é uma Lista de exoplanetas descobertos em 2021.
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) | Método de descoberta | Distância (ly) | Massa da estrela-mãe (M☉) | Temperatura da estrela-mãe (K) | Observações |
|---|---|---|---|---|---|---|---|---|---|---|
| HD 108236 f | 0.17406+0.00482 −0.00437 |
29.54255±0.00069 | 0.1759±0.0037 | Trânsito | 211 | 0.853±0.047 | 5720.0±50.0 | [1][2] | ||
| NGTS-14Ab | 0.092±0.012 | 0.444±0.030 | 3.5357173±0.0000069 | 0.0403±0.0071 | 1143±139 | Trânsito | 1060 | 0.898±0.035 | 5187±11 | [3] |
| TOI-1259 Ab | 0.441+0.049 −0.047 |
1.022+0.030 −0.037 |
3.4779780+0.0000019 −0.0000017 |
0.04070+0.00114 −0.00110 |
936 | Trânsito | 385±1 | 0.68+0.1 −0.01 |
4,775±100 | Também uma anã branca em uma órbita ampla[4] |
| NGTS-13b | 4.84±0.44 | 1.142±0.046 | 4.12 | 0.0549+0.0015 −0.0025 |
1605±30 | Trânsito | 2150 | 1.30+0.11 −0.18 |
5819±73 | [5] |
| TOI-628 b | 6.33+0.29 −0.31 |
1.060+0.041 −0.034 |
3.4095675+0.0000070 −0.0000069 |
0.04860+0.00080 −0.00094 |
1586+52 −40 |
Trânsito | 582 | 1.311+0.066 −0.075 |
6250+220 −190 |
Estrela-mãe também conhecida como HD 288842[6] |
| TOI-640 b | 0.88±0.16 | 1.771+0.060 −0.056 |
5.0037775±0.0000048 | 0.06608+0.00098 −0.0011 |
1749+26 −30 |
Trânsito | 1115 | 1.536+0.069 −0.076 |
6460+130 −150 |
[6] |
| TOI-1333 Ab | 2.37±0.24 | 1.396+0.056 −0.054 |
4.720219±0.000011 | 0.0626+0.0011 −0.0012 |
1679+35 −34 |
Trânsito | 653 | 1.464+0.076 −0.079 |
6274±97 | Estrela-mãe também conhecida como BD+47 3521A[6] |
| TOI-1478 b | 0.847+0.052 −0.048 |
1.061+0.040 −0.038 |
10.180249±0.000015 | 0.0903+0.0018 −0.0013 |
918±11 | Trânsito | 498 | 0.946+0.059 −0.041 |
5595+83 −81 |
[6] |
| TOI-1601 b | 0.99±0.11 | 1.239+0.046 −0.039 |
5.331751±0.000011 | 0.06864+0.00079 −0.00075 |
1619+24 −23 |
Trânsito | 1096 | 1.517+0.053 −0.049 |
5948+87 −89 |
[6] |
| OGLE-2019-BLG-0960Lb | 0.0071±0.0027 | 1.75±0.55 | Microlente | 2900±1000 | 0.45±0.15 | O menor exoplaneta descoberto por microlente[7] | ||||
| HD 110113 b | 0.0143±0.0020 | 0.183±0.011 | 2.541+0.0005 −0.001 |
0.035±0.001 | 1371±14 | Trânsito | 346.5±2.3 | 0.99±0.08 | 5,730 | Exoplaneta com intervalo de raio, estrela-mãe também conhecida como TOI-755[8] |
| HD 110113 c | 0.0330±0.0038 | 6.744+0.008 −0.009 |
0.068+0.001 −0.002 |
990±10 | Vel. radial | 346.5±2.3 | 0.99±0.08 | 5730 | Estrela-mãe também conhecida como TOI-755[8] | |
| KOI-5Ab | 0.179 | 0.63 | 5 | Trânsito | 1870±70 | 1.13 | 5861 | Támbem conhecido como TOI-1241 b[9][10] | ||
| TOI-178 b | 0.0047+0.0012 −0.0013 |
0.102±0.006 | 1.914558±0.000018 | 0.02607±0.00078 | 1040+22 −21 |
Trânsito | 205.16±0.03 | 0.650+0.027 −0.029 |
4316±70 | [11] |
| TOI-178 c | 0.015+0.0017 −0.0021 |
0.149+0.01 −0.008 |
3.238450+0.000020 −0.000019 |
0.0370±0.0011 | 873±18 | Trânsito | 205.16±0.03 | 0.650+0.027 −0.029 |
4316±70 | [11] |
| TOI-178 d | 0.0094+0.0025 −0.0032 |
0.229±0.006 | 6.557700±0.000016 | 0.0592±0.0018 | 690±14 | Trânsito | 205.16±0.03 | 0.650+0.027 −0.029 |
4316±70 | [11] |
| TOI-178 e | 0.0121+0.0039 −0.0029 |
0.197+0.007 −0.008 |
9.961881±0.000042 | 0.0783+0.0023 −0.0024 |
600±12 | Trânsito | 205.16±0.03 | 0.650+0.027 −0.029 |
4316±70 | [11] |
| TOI-178 f | 0.0242+0.0052 −0.0047 |
0.204±0.009 | 15.231915+0.000115 −0.000095 |
0.1039±0.0031 | 521±11 | Trânsito | 205.16±0.03 | 0.650+0.027 −0.029 |
4316±70 | [11] |
| TOI-178 g | 0.0123+0.0041 −0.0050 |
0.256+0.012 −0.011 |
20.70950+0.00014 −0.00011 |
0.1275+0.0038 −0.0039 |
470±10 | Trânsito | 205.16±0.03 | 0.650+0.027 −0.029 |
4316±70 | [11] |
| HD 183579 b | 0.0620+0.0126 −0.0123 |
0.317+0.013 −0.011 |
17.471278+0.000058 −0.000060 |
0.1334+0.0062 −0.0061 |
769+17 −13 |
Trânsito | 186.1±0.8 | 1.031+0.025 −0.026 |
5788±44 | Estrela-mãe também conhecida como TOI-1055[12][13][14] |
| KMT-2019-BLG-0371b | 7.70+11.34 −3.90 |
0.79+0.14 −0.16 |
Microlente | 23000+3000 −4000 |
0.09+0.14 −0.05 |
Múltiplas soluções para separação orbital[15] | ||||
| HD 5278 b | 0.0245+0.0047 −0.0044 |
0.219±0.004 | 14.339156+0.000049 −0.000047 |
0.1202±0.0013 | 943±13 | Trânsito | 183.1±2.7 | 1.126+0.036 −0.035 |
6203±64 | Estrela-mãe também conhecida como TOI-130[16] |
| HD 5278 c | 0.0579+0.0057 −0.0060 |
0.2416±0.0027 | 0.1202±0.0013 | 943±13 | Vel. radial | 183.1±2.7 | 1.126+0.036 −0.035 |
6203±64 | Estrela-mãe também conhecida como TOI-130[16] | |
| KMT-2018-BLG-1025Lb | 0.0191+0.0258 −0.0104 |
1.305+0.194 −0.227 |
Microlente | 22000±3000 | 0.219+0.297 −0.120 |
Múltiplas soluções para parâmetros orbitais[17] | ||||
| TOI-558 b | 3.61±0.15 | 1.086+0.041 −0.038 |
14.574071±0.000026 | 0.1291+0.0020 −0.0021 |
1061+13 −12 |
Trânsito | 1312±17 | 1.349+0.064 −0.065 |
6466+95 −93 |
[18] |
| TOI-559 b | 6.01+0.24 −0.23 |
1.091+0.028 −0.025 |
6.9839095±0.0000051 | 0.0723±0.0013 | 1180+18 −16 |
Trânsito | 761±7 | 1.026±0.057 | 5925+85 −76 |
[18] |
| Candidate 1 | 0.3011-0.6386 | 0.062-0.157 | Imagem direta | 4.37 | Fotografado próximo de Alpha Centauri A | |||||
| HD 13808 b | 0.0346 | 14.2 | 0.11 | Vel. radial | 92.2 | 0.771±0.022 | 5,035±50 | Candidato desde 2011, confirmado em 2021[19] confirmado em 2021[20] | ||
| HD 13808 c | 0.0315 | 53.8 | 0.26 | Vel. radial | 92.2 | 0.771±0.022 | 5035±50 | Candidato desde 2011,[19] confirmado em 2021[20] | ||
| TOI-451 b | 0.1732+0.0134 −0.0116 |
1.858701+0.000027 −0.000033 |
0.0271+0.0023 −0.0038 |
1524+100 −60 |
Trânsito | 405.1±1.3 | 0.94±0.025 | 5550±56 | Planetas orbitando primários de amplo sistema binário.[21][22] Estrela-mãe também conhecida como CD-38 1467 | |
| TOI-451 c | 0.2741±0.0125 | 9.192523+0.000064 −0.000084 |
0.0771+0.0066 −0.0093 |
903+53 −36 |
Trânsito | 405.1±1.3 | 0.94±0.025 | 5550±56 | Planetas orbitando primários de amplo sistema binário.[21][22] Estrela-mãe também conhecida como CD-38 1467. | |
| TOI-451 d | 0.3598±0.0134 | 16.364981+0.000047 −0.000049 |
0.1255+0.0057 −0.0065 |
708+15 −12 |
Trânsito | 405.1±1.3 | 0.94±0.025 | 5550±56 | Planetas orbitando primários de amplo sistema binário.[21][22] Estrela-mãe também conhecida como CD-38 1467. | |
| HD 110082 b | 0.2857±0.0089 | 10.18271±0.00004 | 0.113+0.009 −0.013 |
Trânsito | 342.8±0.9 | 1.21±0.06 | 6200±100 | Orbitando um sistema binário primário ou amplo.[23] Estrela-mãe também conhecida como TOI-1098. | ||
| OGLE-2018-BLG-0567Lb | 0.32+0.34 −0.16 |
2.72+0.49 −0.55 |
Microlente | 23000±3000 | 0.24+0.16 −0.13 |
[24] | ||||
| OGLE-2018-BLG-0962Lb | 1.37+0.80 −0.72 |
3.57+0.68 −1.02 |
Microlente | 21000+3000 −5000 |
0.55+0.32 −0.29 |
[24] | ||||
| Gliese 740 b | 0.0093±0.0016 | 2.37756+0.00013 −0.00011 |
0.029±0.001 | 829+40 −50 |
Vel. radial | 36.21±0.02 | 0.58±0.06 | 3913±21 | [25] | |
| OGLE-2018-BLG-1428Lb | 0.77+0.77 −0.53 |
3.30+0.59 −0.83 |
Microlente | 20000+3000 −5000 |
0.43+0.33 −0.22 |
[26] | ||||
| LHS 1478 b | 0.0073±0.0006 | 0.111±0.004 | 1.9495378+0.0000040 −0.0000041 |
0.01848+0.00061 −0.0006 |
595+10 −9 |
Trânsito | 59.40±0.03 | 0.236±0.012 | 3381±54 | [27] Estrela-mãe também conhecida como TOI-1640 ou G 245-61 |
| TOI-1685 b | 0.0121±0.030 | 0.131±0.006 | 0.6691425±0.0000037 | 0.01156±0.00009 | 1052±21 | Trânsito | 122.68±0.09 | 0.495±0.019 | 3434±51 | [28][29] Estrela-mãe também conhecida como UCAC4 666-026266 |
| TOI-1685 c | 0.0290±0.0065 | 9.025+0.104 −0.119 |
449.1±6.9 | Vel. radial | 122.68±0.09 | 0.495±0.019 | 3434±51 | Não confirmado[28] | ||
| KMT-2020-BLG-0414Lb | 0.0032 | 0.15 | Microlente | 3300±300 | 0.3 | Também uma anã marrom com massa 17MJ no sistema na separação de 15 UA[30] | ||||
| HD 39474 b | 0.42+0.05 −0.03 |
1.008+0.012 −0.015 |
52.97818+0.00004 −0.00004 |
0.30+0.02 −0.03 |
759+37 −26 |
Trânsito | 372.5±1.1 | 1.316±0.027 | 6394±75 | Estrela-mãe também conhecida como TOI-201[31] |
| Gliese 486 b | 0.0089±0.0004 | 0.117±0.006 | 1.467119+0.000031 −0.000030 |
0.01734+0.00026 −0.00027 |
701±13 | Trânsito | 26.344±0.013 | 0.323±0.015 | 3340±54 | Exoplaneta pode ter uma atmosfera mensurável[32] |
| NGTS-15b | 0.751+0.102 −0.088 |
1.10±0.10 | 3.27623±0.00001 | 0.0441±0.0046 | 1146±47 | Trânsito | 2580±60 | 0.995±0.015 | 5600±150 | [33] |
| NGTS-16b | 0.667+0.157 −0.129 |
1.30+0.13 −0.12 |
4.84532±0.00002 | 0.0523±0.0064 | 1177±59 | Trânsito | 2910+95 −75 |
1.002±0.011 | 5550±150 | [33] |
| NGTS-17b | 0.764+0.195 −0.164 |
1.24±0.11 | 3.24253±0.00001 | 0.0391±0.0043 | 1457±50 | Trânsito | 3420±90 | 1.025+0.015 −0.014 |
5650±100 | [33] |
| NGTS-18b | 0.409+0.081 −0.063 |
1.21±0.18 | 3.05125±0.00001 | 0.0448±0.0068 | 1381+55 −53 |
Trânsito | 3610±140 | 1.003+0.020 −0.012 |
5610±150 | [33] |
| OGLE-2019-BLG-1053Lb | 0.0078+0.0037 −0.0031 |
3.4±0.5 | Microlente | 22000+3000 −2000 |
0.61+0.29 −0.24 |
[34] | ||||
| TOI-1634 b | 0.0313±0.0030 | 0.158±0.007 | 0.9893457±0.0000034 | 0.01491±0.00015 | 921±21 | Trânsito | 114.40±0.08 | 0.452±0.014 | 3472±48 | [29][35] |
| KMT-2019-BLG-1715 | 2.56+1.13 −1.16 |
3.32+0.82 −0.92 |
Microlente | 13000±3000 | 0.61+0.27 −0.28 |
Soluções múltiplas para separação orbital, também 0.15M☉ de uma anã vermelha no sistema.[36] | ||||
| OGLE-2018-BLG-1185b | 0.026+0.025 −0.015 |
1.54+0.18 −0.22 |
Microlente | 24000+2000 −3000 |
0.37+0.35 −0.21 |
Múltiplas soluções para planetas e massas estelares.[37] | ||||
| TOI-1260 b | 0.0271+0.0043 −0.0037 |
0.208+0.009 −0.008 |
3.12748+0.000047 −0.000038 |
0.0366+0.0022 −0.0036 |
860+47 −31 |
Trânsito | 239.5±0.3 | 0.66±0.01 | 4227±85 | [38] |
| TOI-1260 c | 0.0373+0.0106 −0.0102 |
0.252±0.013 | 7.49325+0.00015 −0.00013 |
0.0656+0.0039 −0.0065 |
643+35 −23 |
Trânsito | 239.5±0.3 | 0.66±0.01 | 4227±85 | [38] |
| KMT-2018-BLG-1976Lb | 1.96+1.23 −1.12 |
2.04+0.72 −0.83 |
Microlente | 19000±2000 | 0.65+0.41 −0.37 |
[39] | ||||
| KMT-2018-BLG-1996Lb | 1.22+0.72 −0.63 |
1.97+0.51 −0.25 |
Microlente | 19000±2000 | 0.69+0.40 −0.38 |
[39] | ||||
| OGLE-2019-BLG-0954Lb | 14.2+9.9 −7.5 |
2.65+0.89 −1.20 |
Microlente | 12000+1000 −2000 |
0.80+0.55 −0.42 |
[39] | ||||
| YSES 2b | 6.3+1.6 −0.9 |
115 | Imagem direta | 356.4±0.5 | 1.10±0.03 | 4749±40 | [40] | |||
| KMT-2016-BLG-2605b | 0.8+1.2 −0.4 |
0.68±0.11 | Microlente | 21000±3000 | 0.065+0.10 −0.035 |
[41] | ||||
| TOI-1431 b | 3.14+0.19 −0.18 |
1.51±0.06 | 2.65022±0.00001 | 0.047±0.002 | 2370±100 | Trânsito | 488±3 | 1.90+0.10 −0.08 |
7690+400 −250 |
Também conhecido como MASCARA-5b[42][43] |
| TOI-269 b | 0.0277±0.0044 | 0.247±0.011 | 3.697723+0.000018 −0.000017 |
0.0345±0.0015 | 531±25 | Trânsito | 186.01±0.25 | 0.3917±0.0095 | 3514±70 | [44] |
| TOI-220 b | 0.0434±0.0031 | 0.271±0.013 | 10.695264 | 0.08911±0.0010 | 805±21 | Trânsito | 290±13 | 0.825±0.028 | 5298±65 | Suspeita-se de planeta adicional de longo período[45] |
| TOI-1062 b | 0.0320±0.0026 | 0.202±0.008 | 4.11412+0.0014 −0.0015 |
0.052 | 1077+10 −9 |
Trânsito | 268.7±0.2 | 0.94±0.02 | 5328±56 | [46] |
| TOI-1062 c | 0.0294±0.0039 | 7.978+0.021 −0.023 |
0.080+0.013 −0.012 |
859+9 −8 |
Vel. radial | 268.7±0.2 | 0.94±0.02 | 5328±56 | [46] | |
| Kepler-129d | 8.3+1.1 −0.7 |
2646+140 −94 |
4.0±0.1 | Vel. radial | 1349±14 | 1.18 | 5770 | [47] | ||
| Gliese 9689 b | 0.0304±0.0046 | 18.27±0.01 | 0.1139±0.0039 | 453±39 | Vel. radial | 100.10±0.04 | 0.59±0.06 | 3836±69 | [48] | |
| TOI-1231 b | 0.0485±0.0104 | 0.326±0.014 | 24.245586+0.000064 −0.000066 |
0.1288+0.0021 −0.0022 |
330 | Trânsito | 89.68±0.04 | 0.485±0.024 | 3553±31 | [49] |
| TIC 172900988 b | 2.84±0.25 | 1.009±0.043 | 196.5±7.7 | Trânsito | 799±9 | 1.24 e 1.20 | 6050 e 5983 | Planeta circumbinário[50] | ||
| TOI-1444 b | 0.0122±0.0022 | 0.125±0.006 | 0.4702694±0.0000044 | 0.1288+0.0021 −0.0022 |
330 | Trânsito | 408.9±0.5 | 0.934±0.038 | 5430±90 | [51] |
| BD+45 0564 b | 1.36±0.12 | 307.88±1.47 | 0.83±0.04 | Vel. radial | 174±2 | 0.81±0.07 | 5004±50 | [52] | ||
| BD+55 0362 b | 0.72±0.08 | 265.59±1.04 | 0.78±0.05 | Vel. radial | 168±2 | 0.909±0.099 | 5012±78 | Suspeita-se de planeta gigante adicional[52] | ||
| BD+63 1405 b | 3.96±0.31 | 1198.48±60.79 | 2.06±0.14 | Vel. radial | 124.4±1.2 | 0.82±0.08 | 5000±53 | Órbita extremamente excêntrica[52] | ||
| HD 124330 b | 0.75±0.06 | 270.66±1.21 | 0.86±0.04 | Vel. radial | 198±3 | 1.15±0.079 | 5873±19 | Suspeita-se de planeta gigante adicional[52] | ||
| HD 155193 b | 0.75±0.06 | 352.65±2.58 | 1.04±0.04 | Vel. radial | 186±6 | 1.221±0.083 | 6239±20 | [52] | ||
| HD 331093 b | 1.50±0.11 | 621.62±16.11 | 1.44±0.07 | Vel. radial | 164.07±0.14 | 1.030±0.079 | 5544±33 | [52] | ||
| HD 107148 c | 0.0626+0.0097 −0.0098 |
18.3267+0.0022 −0.0024 |
0.1406±0.0018 | Vel. radial | 161.4±0.4 | 1.1±0.1 | 5789±36 | [53] | ||
| HD 136925 b | 0.84+0.078 −0.074 |
4540+160 −140 |
5.13+0.12 −0.11 |
Vel. radial | 156.2 | 5715 | Suspeita de planeta adicional[53] | |||
| Lambda Serpentis b | 0.0428+0.0047 −0.0045 |
15.5083+0.0016 −0.0018 |
0.1238±0.002 | Vel. radial | 38.87±0.07 | 1.14 | 5884±4 | [53] | ||
| HD 156668 c | 0.0991+0.0079 −0.0077 |
811.3+5.2 −5.3 |
1.570±0.017 | Vel. radial | 79.34±0.03 | 0.772±0.020 | 4850±88 | Há suspeita de corpo adicional no sistema[53] | ||
| HD 164922 e | 0.0331±0.0031 | 41.763±0.012 | 0.2293+0.0026 −0.0027 |
Vel. radial | 71.69±0.03 | 0.874±0.012 | 5293±32 | [53] | ||
| HD 168009 b | 0.0300+0.0038 −0.0037 |
15.1479+0.0035 −0.0037 |
0.1192+0.0017 −0.0018 |
Vel. radial | 75.97±0.03 | 0.99 | 5792±80 | [53] | ||
| HD 213472 b | 3.48+1.10 −0.59 |
16700+12000 −4800 |
13.0+5.7 −2.6 |
Vel. radial | 210.6 | [53] | ||||
| HD 24040 c | 0.201±0.027 | 515.4+2.2 −2.5 |
1.3±0.021 | Vel. radial | 152.3±0.4 | 1.14±0.02 | 5917±52 | [53] | ||
| HD 26161 b | 13.5+8.5 −3.7 |
32000+21000 −10000 |
20.4+7.9 −4.9 |
Vel. radial | 133.6±0.3 | Órbita muito excêntrica, e também tem uma anã vermelha no sistema[53] | ||||
| HD 3765 b | 0.173+0.014 −0.013 |
1211+15 −16 |
2.108+0.032 −0.033 |
Vel. radial | 78.5±0.1 | [53] | ||||
| HD 66428 c | 27+22 −17 |
39000+56000 −18000 |
23.0+19.0 −7.6 |
Vel. radial | 174.1±0.7 | 1.09±0.02 | 5773±55 | [53] | ||
| HD 68988 c | 15.0+2.8 −1.5 |
16100+11000 −3500 |
13.2+5.3 −2.0 |
Vel. radial | 198.8±0.6 | 1.16±0.01 | 5919±11 | Suspeito desde 2006[53] | ||
| Lalande 21185 c | 0.0568+0.0091 −0.0083 |
3190+200 −170 |
3.1+0.13 −0.11 |
Vel. radial | 8.31±0.01 | 0.390±0.011 | 3601±51 | [53] | ||
| G 264-12 b | 0.0079±0.0009 | 2.30538±0.00031 | 0.02279±0.00061 | 587±16 | Vel. radial | 52.14±0.03 | 0.297±0.024 | 3326±54 | [54] | |
| G 264-12 c | 0.0118±0.0015 | 8.0518±0.0034 | 0.0525±0.0014 | 387±11 | Vel. radial | 52.14±0.03 | 0.297±0.024 | 3326±54 | [54] | |
| Gliese 393 b | 0.0054±0.0008 | 7.02679+0.00082 −0.00085 |
0.05402±0.00072 | 485±11 | Vel. radial | 22.956±0.008 | 0.426±0.017 | 3579±51 | [54] | |
| TOI-674 b | 0.0739±0.0104 | 0.470±0.016 | 1.977143±0.000003 | 0.0231±0.0007 | 661±14 | Trânsito | 150.86±0.11 | 0.442±0.007 | 3505+28 −32 |
[55] Possivelmente atmosfera de vapor[56] |
| HD 152843 b | 0.0364+0.0207 −0.0193 |
0.304±0.012 | 11.6264+0.0022 −0.0025 |
0.1053+0.003 −0.0031 |
Trânsito | 352.0±1.0 | 1.15±0.04 | 6310±100 | [57] | |
| HD 152843 c | 0.0865 | 0.521±0.013 | 24.38+6.23 −3.4 |
Trânsito | 352.0±1.0 | 1.15±0.04 | 6310±100 | [57] | ||
| KMT-2019-BLG-0253b | 0.029+0.016 −0.013 |
3.1+0.8 −0.9 |
Microlente | 16000+6000 −5000 |
0.70+0.34 −0.31 |
[58] | ||||
| OGLE-2018-BLG-0506 | 0.051+0.038 −0.027 |
3.0+0.7 −0.8 |
Microlente | 18000±5000 | 0.63+0.37 −0.32 |
[58] | ||||
| OGLE-2018-BLG-0516 | 0.063+0.052 −0.034 |
2.2+0.8 −0.7 |
Microlente | 7000+3000 −2000 |
0.47+0.38 −0.25 |
[58] | ||||
| OGLE-2019-BLG-1492 | 0.117+0.079 −0.061 |
2.7±0.9 | Microlente | 18000+6000 −7000 |
0.68±0.34 | [58] | ||||
| OGLE-2018-BLG-0977 | 0.020+0.016 −0.012 |
2.0+0.6 −0.5 |
Microlente | 7000±2000 | 0.47+0.38 −0.27 |
[58] | ||||
| TOI-1789 b | 0.70±0.16 | 1.40+0.22 −0.13 |
3.208666±0.000016 | 0.04873+0.00065 −0.0016 |
1929+28 −18 |
Trânsito | 729±3 | 1.499+0.061 −0.15 |
5984+55 −57 |
[59] |
| TOI-942 b | 0.347+0.022 −0.020 |
4.32421±0.000019 | 0.04866+0.00016 −0.00013 |
Trânsito | 493.9±1.0 | 0.8220+0.0079 −0.0064 |
[60] | |||
| TOI-942 c | 0.417+0.030 −0.027 |
10.156272+0.000037 −0.000034 |
0.08598+0.00027 −0.00022 |
Trânsito | 493.9±1.0 | 0.8220+0.0079 −0.0064 |
[60] | |||
| KMT-2018-BLG-1743 | 0.245+0.339 −0.135 |
1.449+0.209 −0.229 |
Microlente | 21000±3000 | 0.193+0.268 −0.107 |
Soluções orbitais múltiplas, estrela-mãe binária[61] | ||||
| TOI-1749 b | 0.060+0.07 −0.04 |
0.124±0.018 | 2.388821+0.000057 −0.000073 |
0.0291±0.0005 | 831±18 | Trânsito | 324.8±0.4 | 0.58±0.03 | 3985±55 | [62] |
| TOI-1749 c | 0.007+0.018 −0.005 |
0.189±0.011 | 4.489010+0.000040 −0.000061 |
0.0443±0.0008 | 673±15 | Trânsito | 324.8±0.4 | 0.58±0.03 | 3985±55 | [62] |
| TOI-1749 d | 0.014+0.020 −0.011 |
0.225±0.013 | 9.04455±0.00012 | 0.0707±0.0012 | 533±12 | Trânsito | 324.8±0.4 | 0.58±0.03 | 3985±55 | [62] |
| HD 27969 b | 4.80+0.24 −0.23 |
654.5+5.7 −5.8 |
1.552+0.032 −0.033 |
261±11 | Vel. radial | 1.16±0.07 | 5966±21 | [63] | ||
| HD 80869 b | 4.86+0.65 −0.29 |
1711.7+9.3 −9.6 |
2.878+0.045 −0.046 |
203.2+6.8 −5.5 |
Vel. radial | 1.08±0.05 | 5837±15 | Órbita muito excêntrica[63] | ||
| HD 95544 b | 6.84±0.31 | 2172+23 −21 |
3.386+0.075 −0.077 |
156.5+5.4 −5.5 |
Vel. radial | 1.09±0.07 | 5722±15 | [63] | ||
| HD 109286 b | 2.99±0.15 | 520.1±2.3 | 1.259±0.021 | 259.4±5.5 | Vel. radial | 0.98±0.05 | 5694±23 | [63] | ||
| HD 115954 b | 8.29+0.75 −0.58 |
3700+1500 −390 |
5.00+1.3 −0.36 |
144.9+8.1 −13 |
Vel. radial | 1.18±0.06 | 5957±26 | [63] | ||
| HD 211403 b | 5.54+0.39 −0.38 |
223.8±0.41 | 0.768±0.013 | 380±13 | Vel. radial | 1.20±0.06 | 6273±44 | [63] | ||
| Kepler-1704b | 4.15±0.29 | 1.065+0.043 −0.041 |
988.88113+0.00091 −0.00092 |
2.026+0.024 −0.031 |
253.8+3.7 −4.1 |
Trânsito | 2690±40 | 1.131+0.040 −0.051 |
5745+88 −89 |
Órbita muito excêntrica (e=0.921)[64] |
| TOI-532b | 0.1935+0.0305 −0.0293 |
0.520±0.017 | 2.3266508±0.0000030 | 0.0296±0.00035 | 867±18 | Trânsito | 439.1±1.2 | 0.639±0.023 | 3927±37 | Exoplaneta deserto netuniano[65] |
| TOI-2406b | 0.0286+0.0223 −0.0126 |
0.263+0.015 −0.014 |
3.0766896±0.0000065 | 0.0228±0.0016 | 447±15 | Trânsito | 181.4±0.4 | 0.162±0.008 | 3100±75 | [66] |
| KIC 8121913 b | 2.1±0.4 | 3.294601+0.000013 −0.00022 |
Modulação de brilho orbital | 2350 | 1.456+0.069 −0.15 |
5975.3+110.2 −109.4 |
[67] | |||
| KIC 10068024 b | 2.0±0.4 | 2.073549+0.000008 −0.000177 |
Modulação de brilho orbital | 3600 | 1.22+0.175 −0.139 |
6118.4+127.2 −121.2 |
[67] | |||
| KIC 5479689 b | 0.5+0.4 −0.1 |
1.701531+0.000008 −0.000419 |
Modulação de brilho orbital | 1504 | 0.966+0.03 −0.04 |
5459.1+90.0 −85.2 |
[67] | |||
| LTT 1445 Ac | 0.0048±0.0006 | 0.103 | 3.12390 | 0.02661+0.00047 −0.00049 |
Trânsito | 22.41±0.01 | 0.256±0.014 | 3337±150 | [68] | |
| Luyten 98-59 e | 0.0094 | 12.8 | 0.071 | 342+20 −18 |
Vel. radial | 34.6 | 0.32±0.03 | 3500±150 | [69] | |
| Luyten 98-59 f | 0.0078 | 23.2 | 0.103 | 285+18 −17 |
Vel. radial | 34.6 | 0.32±0.03 | 3500±150 | Exoplaneta não confirmado, potencialmente habitável[69] | |
| HD 191939 e | 0.34±0.01 | 101.4±0.4 | 0.397±0.005 | 397±16 | Vel. radial | 175.1±0.2 | 0.92 | 5400 | Também suspeita de anã marrom em órbita mais ampla[70] | |
| OGLE-2019-BLG-1058 | 6.836±6.027 | Microlente | 8000±5000 | Múltiplas soluções, planeta interestelar.[71] | ||||||
| TOI-2184 b | 0.65±0.16 | 1.017±0.051 | 6.90683±0.00009 | Trânsito | 2515±22 | 1.53±0.12 | 5966±136 | [72] | ||
| TOI-431 b | 0.0097±0.0011 | 0.0014±0.004 | 0.490047+0.000010 −0.000007 |
0.0113+0.0002 −0.0003 |
1862±42 | Trânsito | 106.37±0.03 | 0.78±0.07 | 4850±75 | Estrela-mãe também conhecida como CD-26 2288 ou HIP 26013[73] |
| TOI-431 c | 0.0089+0.0013 −0.0011 |
4.8494+0.0003 −0.0002 |
0.0052±0.001 | 867±20 | Vel. radial | 106.37±0.03 | 0.78±0.07 | 4850±75 | Estrela-mãe também conhecida como CD-26 2288 ou HIP 26013[73] | |
| TOI-431 d | 0.0312±0.0047 | 0.294±0.008 | 12.46103±0.00002 | 0.098±0.002 | 633±14 | Trânsito | 106.37±0.03 | 0.78±0.07 | 4850±75 | Estrela-mãe também conhecida como CD-26 2288 ou HIP 26013[73] |
| TOI-2202 b | 0.927+0.047 −0.048 |
1.01+0.522 −0.080 |
11.9108+0.0009 −0.0009 |
0.0956+0.0015 −0.0016 |
Trânsito | 770±3 | 0.823+0.027 −0.023 |
5144±50 | [74] | |
| TOI-2202 c | 0.191+0.033 −0.030 |
24.7545+0.0073 −0.0078 |
0.1558+0.0025 −0.0026 |
Tempo | 770±3 | 0.823+0.027 −0.023 |
5144±50 | [74] | ||
| EPIC 211314705.01 | 0.139±0.007 | 3.793306+0.000324 −0.000343 |
543+8 −9 |
Trânsito | 300.0±1.7 | 0.43±0.01 | 3669+88 −82 |
[75] Two more planets in system are suspected.[76] | ||
| EPIC 211401787.01 | 0.247+0.013 −0.008 |
13.774798+0.000028 −0.000028 |
969±9 | Trânsito | 525±5 | 1.23±0.02 | 6232+33 −39 |
[75] Estrela-mãe também conhecida como BD+12 1842 | ||
| K2-268f | 0.199+0.013 −0.008 |
26.270570+0.000105 −0.000109 |
492+8 −10 |
Trânsito | 1079±10 | 0.84±0.02 | 5106+70 −61 |
Mais dois exoplanetas eram conhecidos anteriormente, estrela-mãe também conhecida como EPIC 211413752[75] | ||
| K2-268d | 0.133+0.013 −0.006 |
4.528598+0.000016 −0.000015 |
888+16 −15 |
Trânsito | 1079±10 | 0.84±0.02 | 5106+70 −61 |
Mais dois exoplanetas eram conhecidos anteriormente, estrela-mãe também conhecida como EPIC 211413752[75] | ||
| K2-268e | 0.119+0.010 −0.007 |
6.131243+0.000032 −0.000033 |
801±13 | Trânsito | 1079±10 | 0.84±0.02 | 5106+70 −61 |
Mais dois exoplanetas eram conhecidos anteriormente, estrela-mãe também conhecida como EPIC 211413752[75] | ||
| EPIC 211502222.01 | 0.243+0.013 −0.009 |
22.996591+0.001848 −0.001859 |
673+12 −11 |
Trânsito | 694±6 | 1.10+0.03 −0.04 |
5994+93 −91 |
[75] | ||
| EPIC 211502222.02 | 0.160+0.013 −0.009 |
9.398977+0.001506 −0.001348 |
909±14 | Trânsito | 694±6 | 1.10+0.03 −0.04 |
5994+93 −91 |
[75] | ||
| EPIC 211579112.01 | 0.196+0.017 −0.014 |
17.706320±0.000063 | 266+5 −8 |
Trânsito | 403±5 | 0.27+0.01 −0.02 |
3315+137 −152 |
[75] | ||
| K2-185c | 0.213±0.008 | 52.713494+0.000155 −0.000164 |
477+14 −17 |
Trânsito | 882±11 | 0.96+0.05 −0.07 |
5788+190 −157 |
Estrela-mãe também conhecida como EPIC 211611158[75] | ||
| EPIC 211647930.01 | 0.552+0.025 −0.022 |
14.759287+0.000243 −0.000240 |
826+14 −17 |
Trânsito | 1133±17 | 1.06±0.04 | 5880+85 −82 |
[75] | ||
| EPIC 211730024.01 | 0.504+0.032 −0.025 |
5.113981+0.000061 −0.000062 |
1380+34 −30 |
Trânsito | 1226±21 | 1.36±0.05 | 6502+132 −130 |
[75] | ||
| EPIC 211743874.01 | 0.197+0.016 −0.013 |
12.283211±0.000051 | 949+21 −26 |
Trânsito | 1850±60 | 1.23±0.04 | 6222+96 −91 |
[75] | ||
| EPIC 211763214.01 | 0.109+0.008 −0.005 |
21.194733+0.000108 −0.000107 |
569+15 −22 |
Trânsito | 786±9 | 0.86+0.03 −0.05 |
5424+192 −144 |
[75] | ||
| EPIC 211770696.01 | 0.234+0.017 −0.013 |
16.273563+0.000054 −0.000053 |
850+19 −18 |
Trânsito | 1390±30 | 0.94+0.04 −0.03 |
5869+88 −81 |
[75] | ||
| EPIC 211779390.01 | 0.092+0.010 −0.005 |
3.850614±0.000012 | 783+12 −14 |
Trânsito | 514±2 | 0.66±0.02 | 4558+91 −81 |
[75] | ||
| EPIC 211897691.02 | 0.171+0.017 −0.011 |
19.507428+0.000116 −0.000113 |
508±12 | Trânsito | 1187±17 | 0.74+0.04 −0.03 |
4857+86 −84 |
[75] | ||
| EPIC 211923431.01 | 0.300+0.039 −0.029 |
29.740451+0.000169 −0.000161 |
606+31 −36 |
Trânsito | 2460±70 | 0.93±0.04 | 5532±90 | [75] | ||
| EPIC 211978988.01 | 0.287+0.022 −0.017 |
36.552551+0.000127 −0.000122 |
598+16 −15 |
Trânsito | 1390±20 | 0.98±0.07 | 5817+45 −48 |
[75] | ||
| TOI-1518 b | 2.3 | 1.875±0.053 | 1.902603±0.000011 | 0.0389±0.0011 | 3237±59 | Trânsito | 742±6 | 1.79±0.26 | 7300±100 | [75] |
| EPIC 212058012.01 | 0.181+0.012 −0.008 |
11.561052+0.000690 −0.000668 |
861+14 −15 |
Trânsito | 684±6 | 1.01±0.05 | 5920±104 | [75] | ||
| EPIC 212072539.01 | 0.180+0.009 −0.006 |
7.676972+0.000012 −0.000012 |
465±7 | Trânsito | 545±3 | 0.49±0.01 | 3804+93 −74 |
[75] | ||
| EPIC 212072539.02 | 0.147+0.015 −0.007 |
2.787174±0.000004 | 653+10 −12 |
Trânsito | 545±3 | 0.49±0.01 | 3804+93 −74 |
[75] | ||
| EPIC 212081533.01 | 0.142+0.009 −0.004 |
3.355850+0.000091 −0.000093 |
722+7 −10 |
Trânsito | 245.8 | 0.51±0.01 | 4374+38 −34 |
[75] | ||
| EPIC 212088059.01 | 0.188+0.018 −0.008 |
10.367437+0.000020 −0.000019 |
437+4 −5 |
Trânsito | 532±3 | 0.56±0.01 | 3779+30 −26 |
[75] | ||
| EPIC 212132195.01 | 0.202+0.017 −0.009 |
26.201446+0.003331 −0.003124 |
450±5 | Trânsito | 345.5±1.6 | 0.71±0.02 | 4801±49 | [75] | ||
| EPIC 212161956.01 | 0.215+0.010 −0.009 |
7.187257+0.000020 −0.000021 |
640+20 −21 |
Trânsito | 1055±13 | 0.66±0.03 | 4599+178 −152 |
[75] | ||
| EPIC 212204403.01 | 0.291+0.020 −0.010 |
4.688418+0.000119 −0.000117 |
908+12 −11 |
Trânsito | 662±5 | 0.83+0.02 −0.01 |
5077+40 −39 |
[75] | ||
| EPIC 212204403.02 | 0.238+0.021 −0.010 |
12.550171+0.001018 −0.001057 |
655+7 −9 |
Trânsito | 662±5 | 0.83+0.02 −0.01 |
5077+40 −39 |
[75] | ||
| K2-304c | 0.203+0.017 −0.011 |
5.213965±0.000442 | 866+27 −37 |
Trânsito | 1380±20 | 0.83+0.05 −0.04 |
5171+172 −130 |
Estrela-mãe também conhecida como EPIC 212297394[75] | ||
| EPIC 212420823.01 | 0.123+0.009 −0.006 |
9.032178±0.000874 | 518+5 −4 |
Trânsito | 1450±20 | 0.54±0.01 | 4385+29 −31 |
[75] | ||
| EPIC 212440430.02 | 0.138+0.013 −0.010 |
4.163873+0.000022 −0.000023 |
1158+29 −34 |
Trânsito | 1620±20 | 0.98±0.02 | 5789+46 −50 |
[75] | ||
| EPIC 212543933.01 | 0.227+0.023 −0.017 |
7.806164+0.000673 −0.000623 |
934+28 −32 |
Trânsito | 1310±50 | 1.02±0.02 | 5769+39 −37 |
[75] | ||
| K2-307c | 0.207+0.017 −0.011 |
23.228555+0.000068 −0.000071 |
658+13 −14 |
Trânsito | 1050±20 | 0.99+0.03 −0.04 |
6004+77 −78 |
Estrela-mãe também conhecida como EPIC 212587672[75] | ||
| EPIC 251319382.01 | 0.171+0.012 −0.006 |
8.234885+0.000508 −0.000475 |
885+12 −14 |
Trânsito | 577±6 | 0.95±0.02 | 5791±81 | [75] | ||
| EPIC 251319382.02 | 0.199+0.012 −0.008 |
14.871387+0.000916 −0.000936 |
727±10 | Trânsito | 577±6 | 0.95±0.02 | 5791±81 | [75] | ||
| EPIC 251319382.03 | 0.122+0.009 −0.006 |
3.665912+0.000273 −0.000295 |
1160+16 −15 |
Trânsito | 577±6 | 0.95±0.02 | 5791±81 | [75] | ||
| EPIC 251554286.01 | 0.496+0.020 −0.018 |
15.466805+0.000572 −0.000565 |
735+13 −14 |
Trânsito | 883±12 | 0.87±0.02 | 5698±55 | [75] | ||
| Gliese 146 b | 0.0175+0.0023 −0.0021 |
5.09071 ± 0.00026 | 0.0510+0.0024 −0.0026 |
573+63 −69 |
Vel. radial | 44.37±0.01 | 0.684±0.013 | 4385±21 | Estrela-mãe também conhecida como HD 22496[77] | |
| EPIC 211525753.01 | 0.201+0.020 −0.014 |
5.7385647+0.0013939 −0.0011048 |
0.0632+0.0096 −0.0176 |
1066+190 −77 |
Trânsito | 0.96+0.05 −0.06 |
5790+177 −147 |
[78] | ||
| EPIC 211537087.01 | 0.204+0.013 −0.011 |
21.0267366+0.0036912 −0.0038993 |
0.1599+0.0178 −0.0306 |
624+0 −37 |
Trânsito | 0.90+0.05 −0.06 |
5568+178 −150 |
[78] | ||
| EPIC 211730267.01 | 0.332+0.021 −0.019 |
16.3488637+0.0013811 −0.0014022 |
0.1450+0.0136 −0.0235 |
735+8 −39 |
Trânsito | 0.98±0.07 | 5794+210 −169 |
[78] | ||
| EPIC 211914998.01 | 0.239+0.015 −0.013 |
11.2510285+0.0018188 −0.0017892 |
0.0863+0.0079 −0.0159 |
888+0 −47 |
Trânsito | 0.93±0.06 | 5650+193 −152 |
[78] | ||
| TOI-3362 b | 5.029+0.668 −0.646 |
1.142+0.043 −0.041 |
18.09547±0.00003 | 0.153+0.002 −0.003 |
Trânsito | 1198±18 | 1.445+0.069 −0.073 |
6532+88 −86 |
Órbita de alta excentricidade[79] | |
| KMT-2017-BLG-2509b | 2.09+1.68 −1.26 |
2.14+0.27 −0.39 |
Microlente | 23000±3000 | 0.46+0.37 −0.27 |
[80] | ||||
| OGLE-2017-BLG-1099b | 3.02+2.43 −1.81 |
2.73+0.40 −0.53 |
Microlente | 24000±3000 | 0.45+0.36 −0.27 |
[80] | ||||
| OGLE-2019-BLG-0299b | 6.22+3.80 −3.67 |
2.80+0.58 −0.89 |
Microlente | 19000±4000 | 0.59+0.36 −0.35 |
[80] | ||||
| TOI-1296b | 0.298±0.039 | 1.231±0.031 | 3.9443715±0.0000058 | 0.0497+0.0023 −0.0028 |
1,562+43 −31 |
Trânsito | 1,023±4 | 1.17±0.14 | 5,603±47 | [81] |
| TOI-1298b | 0.356±0.032 | 0.841±0.021 | 4.537164±0.000012 | 0.0590±0.0023 | 1,388±24 | Trânsito | 1,041±7 | 1.44±0.10 | 5,889±43 | [81] |
| TOI-1201 b | 0.0198±0.0027 | 0.216±0.008 | 2.4919863+0.0000030 −0.0000031 |
0.0287±0.0012 | 703+15 −14 |
Trânsito | 122.77±0.10 | 0.512±0.020 | 3,476±51 | Pertence à Híades, também anã vermelha do sistema.[82] |
| RR Caeli c | 2.7±0.7 | 14,200±300 | 9.7±0.9 | Tempo | 69.10±0.03 | 0.18+0.44 | 3,100+7,540 | Planeta circumbinário em torno das anãs vermelhas e brancas.[83] | ||
| TIC 257060897b | 0.67±0.03 | 1.49±0.04 | 3.660028±0.000006 | 0.051±0.002 | 1,762±21 | Trânsito | 1,655±8 | 1.32±0.04 | 6,128±57 | [84] |
| TOI-530b | 0.40+0.09 −0.10 |
0.83±0.06 | 6.387597+0.000019 −0.000018 |
0.052+0.005 −0.004 |
565+28 −31 |
Trânsito | 482±2 | 0.53±0.02 | 3,659±120 | [85] |
| HIP 97166b | 0.0629±0.047 | 0.245±0.012 | 10.28891±0.00004 | 0.089±0.001 | 757±25 | Trânsito | 215.54±0.33 | 0.898±0.054 | 5,198±100 | [86] |
| HIP 97166c | 9.9±1.8 | 16.84±0.22 | 0.124±0.002 | 642±22 | Vel. radial | 215.54±0.33 | 0.898±0.054 | 5,198±100 | [86] | |
| HD 63935 b | 0.0340±0.0057 | 0.267±0.013 | 9.058811+0.000017 −0.000016 |
911±27 | Trânsito | 159.36±0.15 | 0.933±0.054 | 5,534±100 | [87] | |
| HD 63935 c | 0.0349±0.0076 | 0.259±0.012 | 21.4023+0.00189 −0.00194 |
684±21 | Trânsito | 159.36±0.15 | 0.933±0.054 | 5,534±100 | [87] | |
| HD 207897 b | 0.0453±0.0050 | 0.223±0.007 | 16.202159+0.000085 −0.000083 |
0.1163+0.0017 −0.001 |
632.2+8.1 −7.0 |
Trânsito | 92.15±0.10 | 0.80+0.036 −0.030 |
5,070+60 −57 |
[88] |
| 2MASS J04372171+2651014 b | 4±1 | 115 | 1,450±50 | Imagem direta | 417.9±1.5 | 0.165±0.015 | 3,100 | [89][90] | ||
| TOI 1227 b | 0.854+0.067 −0.052 |
27.36397±0.00011 | 0.0886+0.0054 −0.0057 |
Trânsito | 329.3±0.8 | 0.170±0.015 | 3,072±74 | [91] | ||
| TOI-2285b | 0.155±0.007 | 27.26955+0.00013 −0.00010 |
0.1363±0.0010 | 284±6 | Trânsito | 138.34±0.14 | 0.454±0.010 | 3,491±58 | [92] | |
| LHS 1678 b | 0.0002±0.0003 | 0.062±0.004 | 0.8602322+0.0000068 −0.0000048 |
0.01251+0.00059 −0.00056 |
Trânsito | 64.88±0.03 | 0.345±0.014 | 3490±50 | [93] | |
| LHS 1678 c | 0.0012+0.0013 −0.0008 |
0.088±0.006 | 3.694247+0.0000024 −0.0000021 |
0.0331+0.0016 −0.0015 |
Trânsito | 64.88±0.03 | 0.345±0.014 | 3490±50 | [93] | |
| HD 73583 b | 0.0315±0.0098 | 0.253±0.009 | 6.3980418+0.0000065 −0.0000063 |
0.0601±0.0026 | 721±21 | Trânsito | 103.08±0.10 | 0.71±0.02 | 4,511±110 | Estrela-mãe também conhecida como TOI-560,[94] emissão planetária de hélio detectada.[95] |
| HD 73583 c | 0.0302±0.0055 | 0.212±0.009 | 18.8797+0.00088 −0.00073 |
0.1236+0.0053 −0.0053 |
503±15 | Trânsito | 103.08±0.10 | 0.71±0.02 | 4511±110 | Estrela-mãe também conhecida como TOI-560[94] |
| TOI-1807 b | 0.0071+0.0015 −0.0018 |
0.165±0.004 | 0.549372±0.000007 | 0.0135+0.0013 −0.0022 |
1499+82 −129 |
Trânsito | 133.88±0.25 | 0.750+0.025 −0.024 |
4757+51 −50 |
Estrela-mãe está se movendo conjuntamente com TOI-2076[96][97] |
| TOI-2076 b | 0.293±0.038 | 10.35566±0.00006 | 0.0631±0.0027 | 870±13 | Trânsito | 136.70±0.23 | 0.850+0.025 −0.026 |
5187+54 −53 |
Estrela-mãe está se movendo conjuntamente com TOI-1807[96] | |
| TOI-2076 c | 0.396±0.004 | 21.01538+0.00084 −0.00074 |
0.0885±0.0038 | 734±11 | Trânsito | 136.70±0.23 | 0.850+0.025 −0.026 |
5187+54 −53 |
[98] Estretla está se movendo junto com o TOI-1807[96] | |
| TOI-2076 d | 0.370±0.006 | 25.0893±0.01 | 0.1138+0.0048 −0.0049 |
648±10 | Trânsito | 136.70±0.23 | 0.850+0.025 −0.026 |
5187+54 −53 |
Estrela-mãe está se movendo conjuntamente com TOI-1807[96] | |
| TOI-2257 b | 0.196±0.010 | 35.189346 | 0.145±0.003 | 256+61 −17 |
Trânsito | 188.5±0.3 | 0.33±0.02 | 3430±130 | Exoplaneta em zona habitável[99] | |
| TOI-712 b | 0.0176 | 0.183+0.011 −0.007 |
9.531361+0.000018 −0.000017 |
0.07928+0.00096 −0.00091 |
650.0+6.0 −5.9 |
Trânsito | 191.2±0.4 | 0.732+0.027 −0.025 |
4622+61 −59 |
[100] |
| TOI-712 c | 0.0274 | 0.241+0.008 −0.007 |
51.69906±0.00017 | 0.2447+0.0030 −0.0028 |
369.9+3.4 −3.3 |
Trânsito | 191.2±0.4 | 0.732+0.027 −0.025 |
4622+61 −59 |
[100] |
| TOI-712 d | 0.0236 | 0.221+0.008 −0.007 |
84.83960+0.00043 −0.00040 |
0.3405+0.0041 −0.0039 |
313.6+2.9 −2.8 |
Trânsito | 191.2±0.4 | 0.732+0.027 −0.025 |
4622+61 −59 |
[100] |
| OGLE-2019-BLG-0468Lb | 3.43+1.83 −1.17 |
3.29+4.15 −2.52 |
Microlente | 14000±3000 | 0.92+0.49 −0.32 |
Múltiplas soluções para parâmetros orbitais[101] | ||||
| OGLE-2019-BLG-0468Lc | 10.22+5.46 −3.50 |
2.77+3.49 −2.12 |
Microlente | 14000±3000 | 0.92+0.49 −0.32 |
Múltiplas soluções para parâmetros orbitais[101] | ||||
| KMT-2021-BLG-0912Lb | 0.022+0.007 −0.008 |
3.03+3.46 −2.46 |
Microlente | 22000±3000 | 0.75+0.23 −0.28 |
Múltiplas soluções para parâmetros orbitais[102] | ||||
| HD 137496 b | 0.0127±0.0017 | 0.117±0.005 | 1.62116±0.00008 | 0.02732±0.00019 | 2130+30 −29 |
Trânsito | 509±6 | 1.035±0.022 | 5799±61 | [103] |
| HD 137496 c | 7.66±0.11 | 479.9+1.1 −1.0 |
1.2163+0.0087 −0.0088 |
370±5 | Vel. radial | 509±6 | 1.035±0.022 | 5799±61 | [103] | |
| HD 19615 b | 8.5±0.7 | 402±2 | 1.1±0.1 | Vel. radial | 872±7 | 1.1±0.1 | 3,987±125 | Estrela-mãe gigante vermelha[104] | ||
| HD 150010 b | 2.4±0.4 | 562±8 | 1.1±0.1 | Vel. radial | 473.4±2.1 | 1.3±0.1 | 4256±125 | Estrela-mãe gigante vermelha[104] | ||
| HD 174205 b | 4.2±0.5 | 582±17 | 1.7±0.1 | Vel. radial | 769±5 | 1.8±0.1 | 4393±125 | Estrela-mãe gigante vermelha[104] | ||
| KMT-2018-BLG-1988Lb | 0.021+0.015 −0.011 |
2.83+1.23 −0.97 |
Microlente | 14000+6000 −5000 |
0.48+0.33 −0.25 |
Múltiplas soluções para parâmetros orbitais[105] | ||||
| KOI-984b | 0.0544±0.0094 | 0.384±0.004 | 4.2881785±0.0000035 | 0.0504±0.0006 | 1022+31 −30 |
Trânsito | 749±4 | 0.928±0.031 | 5295±150 | Outro planeta no sistema em órbita mal limitada[106] |
| TOI-2109b | 5.02±0.75 | 1.347±0.047 | 0.67247414±0.00000028 | 0.01791±0.00065 | 3631±69 | Trânsito | 846±9 | 1.447+0.075 −0.078 |
6530+160 −150 |
[107] |
| TOI-1238b | 0.0183±0.0035 | 0.108±0.010 | 0.764596+0.000016 −0.000013 |
0.0139±0.0008 | 1133±167 | Trânsito | 2030.44±0.20 | 0.59±0.02 | 4089±54 | [108] |
| TOI-1238c | 0.0262±0.0059 | 0.188±0.013 | 3.294733+0.000040 −0.000047 |
0.037±0.002 | 695±105 | Trânsito | 2030.44±0.20 | 0.59±0.02 | 4089±54 | [108] |
| K2-99c | 8.4±0.2 | 522.2±1.4 | 1.43±0.01 | 390±6 | Vel. radial | 1980 | 1.6 | 5990 | [109] | |
| HIP 5763b | 0.51 | 30.014+0.1528 −0.2842 |
0.170 | Vel. radial | 104.17±0.14 | 0.72 | [110] | |||
| HIP 34222b | 0.83 | 160.0+2.7 −2.9 |
0.492 | Vel. radial | 74.55±0.09 | 0.62 | [110] | |||
| HIP 86221b | 0.71 | 2.224+0.0004 −0.0005 |
0.031 | Vel. radial | 96±11 | 0.79 | [110] | |||
| TOI-1842b | 0.214+0.040 −0.038 |
1.04+0.06 −0.05 |
9.5739+0.0002 −0.0001 |
0.01001±0.0007 | Trânsito | 729±7 | 1.46±0.03 | 6230±50 | [111] | |
| Gliese 367b | 0.0017±0.0002 | 0.064±0.005 | 0.321962+0.000010 −0.000012 |
0.0071±0.0002 | 1745±43 | Trânsito | 30.695±0.016 | 0.45±0.011 | 3522±70 | [112] |
| HATS-74Ab | 1.46±0.14 | 1.032±0.021 | 1.73185606±0.00000055 | 0.02384±0.00011 | 895.1±5.7 | Trânsito | 952±12 | 0.601±0.008 | 3775±54 | Estrela-mãe também conhecida como TOI-737[113] |
| HATS-75b | 0.491±0.039 | 0.884±0.013 | 2.7886556±0.0000011 | 0.032742+0.000134 −0.000099 |
772.3±2.3 | Trânsito | 640±4 | 0.6017+0.0074 −0.0055 |
3812±79 | Estrela-mãe também conhecida como TOI-552[113] |
| HATS-76b | 2.629±0.089 | 1.079±0.031 | 1.9416423±0.0000014 | 0.02658+0.00021 −0.00029 |
939.8±6.7 | Trânsito | 1272±19 | 0.662+0.016 −0.021 |
3990±120 | Estrela-mãe também conhecida como TOI-555[113] |
| HATS-77b | 1.374+0.100 −0.074 |
1.165±0.021 | 3.0876262±0.0000016 | 0.03607±0.00025 | 828.3±5.9 | Trânsito | 1440±40 | 0.655±0.014 | 4082±69 | Estrela-mãe também conhecida como TOI-730[113] |
| KOI-4777b | 0.046±0.003 | 0.412000±0.000001 | 0.0080±0.0003 | 1180±20 | Trânsito | 565±4 | 0.41±0.02 | 3515±69 | [114] | |
| BD+60 1417b | 15±5 | 1.31±0.06 | 1662 | 1303±74 | Imagem direta | 146.65±0.09 | 1.0 | 4993±124 | Estrela-mãe jovem (≈100 milhões de anos)[115] | |
| b Centauri b | 10.9±1.6 | 200000±100000 | 556±17 | Imagem direta | 325±10 | 8±2 | Planeta circumbinário em sistema estelar invulgarmente massivo[116] | |||
| HD 360 b | 0.75+0.12 −0.15 |
273.1+1.6 −0.8 |
0.98+0.11 −0.03 |
Vel. radial | 362 | 1.69+0.15 −0.53 |
4770 | [117] | ||
| Epsilon Piscium b | 0.77+0.16 −0.10 |
255.3+2.1 −1.4 |
0.88+0.11 −0.10 |
Vel. radial | 183.2 | 1.41+1.45 −0.50 |
4824 | Candidato planetário, não confirmado[117] | ||
| HD 10975 b | 0.45+0.06 −0.15 |
283.8+12.7 −0.1 |
0.95+0.06 −0.08 |
Vel. radial | 379 | 1.41+0.34 −0.35 |
4840 | [117] | ||
| HD 79181 b | 0.64+0.06 −0.16 |
273.1+1.3 −0.4 |
0.90+0.07 −0.08 |
Vel. radial | 337 | 1.28+0.32 −0.28 |
4862 | [117] | ||
| HD 99183 b | 0.97+0.06 −0.25 |
310.4+5.2 −1.7 |
1.08+0.05 −0.07 |
Vel. radial | 355 | 1.76+0.31 −0.30 |
4886 | [117] | ||
| Upsilon Leonis b | 0.51+0.06 −0.26 |
385.2+2.8 −1.3 |
1.18+0.11 −0.32 |
Vel. radial | 177.8 | 1.48+0.90 −0.38 |
4836 | [117] | ||
| HD 161178 b | 0.57+0.02 −0.16 |
279.3+1.0 −0.8 |
0.85+0.05 −0.07 |
Vel. radial | 351 | 1.06+0.25 −0.17 |
4786 | [117] | ||
| HD 219139 b | 0.78+0.05 −0.20 |
275.5+2.3 −1.0 |
0.94+0.06 −0.07 |
Vel. radial | 345 | 1.46+0.31 −0.29 |
4831 | [117] | ||
| Gamma Piscium b | 1.34+0.02 −0.31 |
555.1+6.0 −2.5 |
1.32+0.05 −0.08 |
Vel. radial | 138 | 0.99+0.17 −0.13 |
4742 | [117] | ||
| OGLE-2014-BLG-0676Lb | 3.68+0.69 −1.44 |
4.53+1.49 −2.50 |
Microlente | 8700+2500 −4600 |
0.73+0.14 −0.29 |
[118] | ||||
| HD 103891 b | 1.44+0.06 −0.05 |
1919+14 −15 |
3.27+0.02 −0.01 |
Vel. radial | 179.0±0.4 | 1.28±0.01 | 6,072±20 | [119] | ||
| HD 105779 b | 0.64±0.06 | 2412+55 −52 |
3.38±0.05 | Vel. radial | 179.7±0.3 | 0.89±0.01 | 5792±16 | [119] | ||
| HD 73583b | 0.253+0.014 −0.011 |
6.3980661+0.0000095 −0.0000097 |
0.05995+0.00074 −0.00072 |
742.7+7.2 −7.0 |
Trânsito | 102.97±0.10 | 0.701+0.026 −0.025 |
4574+62 −61 |
Estrela-mãe também conhecida como TOI 560[120] | |
| HD 73583c | 0.2433+0.011 −0.0096 |
18.8805+0.0024 −0.0011 |
0.1233±0.0015 | 517.8+5 −4.9 |
Trânsito | 102.97±0.10 | 0.701+0.026 −0.025 |
4574+62 −61 |
Estrela-mãe também conhecida como TOI 560[120] | |
| OGLE-2014-BLG-0319Lb | 0.57+0.36 −0.31 |
3.49+1.17 −1.12 |
Microlente | 25000+4000 −9000 |
0.52+0.33 −0.29 |
[121] | ||||
| OGLE-2018-BLG-0383L b | 0.0201+0.0173 −0.0088 |
1.8±0.2 | Microlente | 25000±2000 | 0.10+0.13 −0.05 |
[122] |
Listas específicas de exoplanetas
editar- Listas de exoplanetas
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- 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
- ↑ «HD 108236 f», exoplanet.eu, consultado em 4 de janeiro de 2021
- ↑ Bonfanti, A.; et al. (2021), «CHEOPS observations of the HD 108236 planetary system: A fifth planet, improved ephemerides, and planetary radii», Astronomy & Astrophysics, 646: A157, Bibcode:2021A&A...646A.157B, arXiv:2101.00663
, doi:10.1051/0004-6361/202039608
- ↑ Smith, A. M. S.; et al. (2021), «NGTS-14Ab: A Neptune-sized transiting planet in the desert», Astronomy & Astrophysics, 646: A183, Bibcode:2021A&A...646A.183S, arXiv:2101.01470 , doi:10.1051/0004-6361/202039712
- ↑ Martin, David V.; et al. (2021), «TOI-1259Ab – a gas giant planet with 2.7 per cent deep transits and a bound white dwarf companion», Monthly Notices of the Royal Astronomical Society, 507 (3): 4132–4148, arXiv:2101.02707 , doi:10.1093/mnras/stab2129
- ↑ Grieves, Nolan; et al. (2021), «NGTS-13b: A hot 4.8 Jupiter-mass planet transiting a subgiant star», Astronomy & Astrophysics, 647: A180, Bibcode:2021A&A...647A.180G, arXiv:2101.04245 , doi:10.1051/0004-6361/202039586
- ↑ a b c d e Rodriguez, Joseph E.; et al. (2021), «TESS Delivers Five New Hot Giant Planets Orbiting Bright Stars from the Full-frame Images», The Astronomical Journal, 161 (4): 194, Bibcode:2021AJ....161..194R, arXiv:2101.01726 , doi:10.3847/1538-3881/abe38a
- ↑ Yee, Jennifer C.; et al. (2021), «OGLE-2019-BLG-0960 Lb: The Smallest Microlensing Planet», The Astronomical Journal, 162 (5): 180, Bibcode:2021AJ....162..180Y, arXiv:2101.04696 , doi:10.3847/1538-3881/ac1582
- ↑ a b Osborn, H. P.; et al. (2021), «A hot mini-Neptune in the radius valley orbiting solar analogue HD 110113», Monthly Notices of the Royal Astronomical Society, 502 (4): 4842–4857, Bibcode:2021MNRAS.502.4842O, arXiv:2101.04745 , doi:10.1093/mnras/stab182
- ↑ Hirsch, Lea A.; et al. (2017), «ASSESSING THE EFFECT OF STELLAR COMPANIONS FROM HIGH-RESOLUTION IMAGING OF Kepler OBJECTS OF INTEREST», The Astronomical Journal, 153 (3): 117, Bibcode:2017AJ....153..117H, arXiv:1701.06577 , doi:10.3847/1538-3881/153/3/117
- ↑ «AT LAST! CONFIRMATION OF KEPLER'S SECOND PLANETARY CANDIDATE» (PDF). Consultado em 18 de janeiro de 2021. Cópia arquivada (PDF) em 15 de janeiro de 2021
- ↑ a b c d e f Leleu, A.; et al. (2021), «Six transiting planets and a chain of Laplace resonances in TOI-178», Astronomy & Astrophysics, 649: A26, Bibcode:2021A&A...649A..26L, arXiv:2101.09260 , doi:10.1051/0004-6361/202039767
- ↑ Palatnick, Skyler; et al. (2021), «Validation of HD 183579b Using Archival Radial Velocities: A Warm Neptune Orbiting a Bright Solar Analog», The Astrophysical Journal Letters, 909 (1): L6, Bibcode:2021ApJ...909L...6P, arXiv:2101.12137 , doi:10.3847/2041-8213/abe0bb
- ↑ Gan, Tianjun; et al. (2021), «HD 183579b: A Warm Sub-Neptune Transiting a Solar Twin Detected by TESS», Monthly Notices of the Royal Astronomical Society, 507 (2): 2220–2240, arXiv:2107.14015 , doi:10.1093/mnras/stab2224
- ↑ Bonfanti, A.; et al. (2023), «TOI-1055 b: Neptunian planet characterised with HARPS, TESS, and CHEOPS», Astronomy & Astrophysics, 671, pp. L8, Bibcode:2023A&A...671L...8B, arXiv:2302.10664 , doi:10.1051/0004-6361/202245607
- ↑ Yun Hak Kim; et al. (2021), «KMT-2019-BLG-0371 and the Limits of Bayesian Analysis», The Astronomical Journal, 162 (1): 17, Bibcode:2021AJ....162...17K, arXiv:2101.12206 , doi:10.3847/1538-3881/abf930
- ↑ a b Sozzetti, A.; et al. (2021), «A sub-Neptune and a non-transiting Neptune-mass companion unveiled by ESPRESSO around the bright late-F dwarf HD 5278 (TOI-130)», Astronomy & Astrophysics, 648: A75, Bibcode:2021A&A...648A..75S, arXiv:2101.12300 , doi:10.1051/0004-6361/202040034
- ↑ Han, Cheongho; et al. (2021), «KMT-2018-BLG-1025Lb: Microlensing super-Earth planet orbiting a low-mass star», Astronomy & Astrophysics, 649: A90, Bibcode:2021A&A...649A..90H, arXiv:2102.01890 , doi:10.1051/0004-6361/202039817
- ↑ a b Ikwut-Ukwa, Mma; et al. (2022), «Two Massive Jupiters in Eccentric Orbits from the TESS Full-frame Images», The Astronomical Journal, 163 (1): 9, Bibcode:2022AJ....163....9I, arXiv:2102.02222 , doi:10.3847/1538-3881/ac2ee1
- ↑ a b Mayor, M.; et al. (2011), «The HARPS search for southern extra-solar planets XXXIV. Occurrence, mass distribution and orbital properties of super-Earths and Neptune-mass planets», arXiv:1109.2497 [astro-ph.EP]
- ↑ a b Ahrer, E.; et al. (2021), «The HARPS search for southern extra-solar planets XLV. Two Neptune mass planets orbiting HD 13808: a study of stellar activity modelling's impact on planet detection», Monthly Notices of the Royal Astronomical Society, 503 (1): 1248–1263, Bibcode:2021MNRAS.503.1248A, arXiv:2102.03387 , doi:10.1093/mnras/stab373
- ↑ a b c Newton, Elisabeth R.; et al. (2021), «TESS Hunt for Young and Maturing Exoplanets (THYME) IV: Three small planets orbiting a 120 Myr-old star in the Pisces–Eridanus stream», The Astronomical Journal, 161 (2): 65, Bibcode:2021AJ....161...65N, arXiv:2102.06049 , doi:10.3847/1538-3881/abccc6
- ↑ a b c Barragán, Oscar; et al. (2021), «TESS re-observes the young multi-planet system TOI-451:refined ephemeris and activity evolution», Research Notes of the American Astronomical Society, 5 (3): 51, Bibcode:2021RNAAS...5...51B, arXiv:2103.09746 , doi:10.3847/2515-5172/abef70
- ↑ Tofflemire, Benjamin M.; et al. (2021), «TESS Hunt for Young and Maturing Exoplanets (THYME). V. A Sub-Neptune Transiting a Young Star in a Newly Discovered 250 Myr Association», The Astronomical Journal, 161 (4): 171, Bibcode:2021AJ....161..171T, arXiv:2102.06066 , doi:10.3847/1538-3881/abdf53
- ↑ a b Kil Jung, Youn; et al. (2021), «OGLE-2018-BLG-0567Lb and OGLE-2018-BLG-0962Lb: Two Microlensing Planets through the Planetary-caustic Channel», The Astronomical Journal, 161 (6): 293, Bibcode:2021AJ....161..293J, arXiv:2102.07338 , doi:10.3847/1538-3881/abf8bd
- ↑ Toledo-Padrón, B.; et al. (2021), «A super-Earth on a close-in orbit around the M1V star GJ 740», Astronomy & Astrophysics, 648: A20, arXiv:2102.09441 , doi:10.1051/0004-6361/202040099
- ↑ Kains, N.; et al. (2021), «A giant planet beyond the snow line in microlensing event OGLE-2011-BLG-0251», Astronomy & Astrophysics, 552: A70, Bibcode:2013A&A...552A..70K, arXiv:1303.1184 , doi:10.1051/0004-6361/201220626
- ↑ Soto, M. G.; et al. (2021), «Mass and density of the transiting hot and rocky super-Earth LHS 1478 b (TOI-1640 b)», Astronomy & Astrophysics, 649: A144, Bibcode:2021A&A...649A.144S, arXiv:2102.11640 , doi:10.1051/0004-6361/202140618
- ↑ a b Bluhm, P.; et al. (2021), «An ultra-short-period transiting super-Earth orbiting the M3 dwarf TOI-1685», Astronomy & Astrophysics, 650: A78, Bibcode:2021A&A...650A..78B, arXiv:2103.01016 , doi:10.1051/0004-6361/202140688
- ↑ a b Hirano, Teruyuki; et al. (2021), «Two Bright M Dwarfs Hosting Ultra-Short-Period Super-Earths with Earth-like Compositions», The Astronomical Journal, 162 (4): 161, Bibcode:2021AJ....162..161H, arXiv:2103.12760 , doi:10.3847/1538-3881/ac0fdc
- ↑ Zang, Weicheng; et al. (2021), «An Earth-mass planet in a time of COVID-19: KMT-2020-BLG-0414Lb», Research in Astronomy and Astrophysics, 21 (9): 239, Bibcode:2021RAA....21..239Z, arXiv:2103.01896 , doi:10.1088/1674-4527/21/9/239
- ↑ Hobson, Melissa J.; et al. (2021), «A Transiting Warm Giant Planet around the Young Active Star TOI-201», The Astronomical Journal, 161 (5): 235, Bibcode:2021AJ....161..235H, arXiv:2103.02685 , doi:10.3847/1538-3881/abeaa1
- ↑ Trifonov, T.; et al. (2021), «A nearby transiting rocky exoplanet that is suitable for atmospheric investigation», Science, 371 (6533): 1038–1041, Bibcode:2021Sci...371.1038T, PMID 33674491, arXiv:2103.04950 , doi:10.1126/science.abd7645
- ↑ a b c d Tilbrook, Rosanna H.; et al. (2021), «NGTS 15b, 16b, 17b, and 18b: Four hot Jupiters from the Next-Generation Transit Survey», Monthly Notices of the Royal Astronomical Society, 504 (4): 6018–6032, arXiv:2103.10302 , doi:10.1093/mnras/stab815
- ↑ Zang, Weicheng; et al. (2021), «Systematic KMTNet Planetary Anomaly Search. I. OGLE-2019-BLG-1053Lb, a Buried Terrestrial Planet», The Astronomical Journal, 162 (4): 163, Bibcode:2021AJ....162..163Z, arXiv:2103.11880 , doi:10.3847/1538-3881/ac12d4
- ↑ Cloutier, R.; et al. (2021), «TOI-1634 b: An Ultra-short-period Keystone Planet Sitting inside the M-dwarf Radius Valley», The Astronomical Journal, 162 (2): 79, Bibcode:2021AJ....162...79C, arXiv:2103.12790 , doi:10.3847/1538-3881/ac0157
- ↑ Han, Cheongho; et al. (2021), «KMT-2019-BLG-1715: Planetary Microlensing Event with Three Lens Masses and Two Source Stars», The Astronomical Journal, 161 (6): 270, Bibcode:2021AJ....161..270H, arXiv:2104.00293 , doi:10.3847/1538-3881/abf4d0
- ↑ Kondo, Iona; et al. (2021), «OGLE-2018-BLG-1185b: A Low-mass Microlensing Planet Orbiting a Low-mass Dwarf», The Astronomical Journal, 162 (2): 77, Bibcode:2021AJ....162...77K, arXiv:2104.02157 , doi:10.3847/1538-3881/ac00ba
- ↑ a b Georgieva, I. Y.; et al. (2021), «Hot planets around cool stars – two short-period mini-Neptunes transiting the late K-dwarf TOI-1260», Monthly Notices of the Royal Astronomical Society, 505 (4): 4684–4701, arXiv:2104.05653 , doi:10.1093/mnras/stab1464
- ↑ a b c Han, Cheongho; et al. (2021), «Three microlensing planets with no caustic-crossing features», Astronomy & Astrophysics, 650: A89, Bibcode:2021A&A...650A..89H, arXiv:2104.06544 , doi:10.1051/0004-6361/202140758
- ↑ Bohn, Alexander J.; et al. (2021), «Discovery of a directly imaged planet to the young solar analog YSES 2», Astronomy & Astrophysics, 648: A73, Bibcode:2021A&A...648A..73B, arXiv:2104.08285 , doi:10.1051/0004-6361/202140508
- ↑ Ryu, Yoon-Hyun; et al. (2021), «Shortest Microlensing Event with a Bound Planet: KMT-2016-BLG-2605», The Astronomical Journal, 162 (3): 96, Bibcode:2021AJ....162...96R, arXiv:2104.07906 , doi:10.3847/1538-3881/ac062a
- ↑ Brett Christopher Addison; et al. (2021), «TOI-1431b/MASCARA-5b: An Ultra-hot Jupiter Orbiting One of the Hottest & Brightest Known Exoplanet Host Stars», Posters from the Tess Science Conference Ii (Tsc2: 64, Bibcode:2021tsc2.confE..64A, arXiv:2104.12078 , doi:10.5281/zenodo.5126266
- ↑ Stangret, M.; et al. (2021), «The obliquity and atmosphere of the ultra-hot Jupiter TOI-1431b (MASCARA-5b): A misaligned orbit and no signs of atomic or molecular absorptions», Astronomy & Astrophysics, 654: A73, Bibcode:2021A&A...654A..73S, arXiv:2104.12414 , doi:10.1051/0004-6361/202040100
- ↑ Cointepas, M.; et al. (2021), «TOI-269 b: An eccentric sub-Neptune transiting a M2 dwarf revisited with ExTrA», Astronomy & Astrophysics, 650: A145, Bibcode:2021A&A...650A.145C, arXiv:2104.14782 , doi:10.1051/0004-6361/202140328
- ↑ Hoyer, S.; et al. (2021), «TOI-220 b: A warm sub-Neptune discovered by TESS», Monthly Notices of the Royal Astronomical Society, 505 (3): 3361–3379, arXiv:2105.01944 , doi:10.1093/mnras/stab1427
- ↑ a b Otegi, J. F.; et al. (2021), «TESS and HARPS reveal two sub-Neptunes around TOI 1062», Astronomy & Astrophysics, 653: A105, Bibcode:2021A&A...653A.105O, arXiv:2105.01945 , doi:10.1051/0004-6361/202040247
- ↑ Zhang, Jingwen; et al. (2021), «Long-period Jovian Tilts the Orbits of Two sub-Neptunes Relative to Stellar Spin Axis in Kepler-129», The Astronomical Journal, 162 (3): 89, Bibcode:2021AJ....162...89Z, arXiv:2105.03446 , doi:10.3847/1538-3881/ac0634
- ↑ Maldonado, J.; et al. (2021), «HADES RV programme with HARPS-N at TNG», Astronomy & Astrophysics, 651: A93, arXiv:2105.06155 , doi:10.1051/0004-6361/202141141
- ↑ Burt, Jennifer A.; et al. (2021), «TOI-1231 b: A Temperate, Neptune-sized Planet Transiting the Nearby M3 Dwarf NLTT 24399», The Astronomical Journal, 162 (3): 87, Bibcode:2021AJ....162...87B, arXiv:2105.08077 , doi:10.3847/1538-3881/ac0432
- ↑ Kostov, Veselin B.; et al. (2021), «TIC 172900988: A Transiting Circumbinary Planet Detected in One Sector of TESS Data», The Astronomical Journal, 162 (6): 234, Bibcode:2021AJ....162..234K, arXiv:2105.08614 , doi:10.3847/1538-3881/ac223a
- ↑ Dai, Fei; et al. (2021), «TKS X: Confirmation of TOI-1444b and a Comparative Analysis of the Ultra-short-period Planets with Hot Neptunes», The Astronomical Journal, 162 (2): 62, Bibcode:2021AJ....162...62D, arXiv:2105.08844 , doi:10.3847/1538-3881/ac02bd
- ↑ a b c d e f Dalal, S.; et al. (2021), «The SOPHIE search for northern extrasolar planets», Astronomy & Astrophysics, 651: A11, arXiv:2105.09741 , doi:10.1051/0004-6361/202140712
- ↑ a b c d e f g h i j k l m Rosenthal, Lee J.; et al. (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 (1): 8, Bibcode:2021ApJS..255....8R, arXiv:2105.11583 , doi:10.3847/1538-4365/abe23c
- ↑ a b c Amado, Pedro J.; Bauer, Florian F.; Rodríguez López, Cristina; Rodríguez, Eloy; Cardona Guillén, C.; Perger, M.; Caballero, José A.; López-González, Maria J.; Muñoz Rodríguez, I.; Pozuelos, F. J.; Sánchez-Rivero, A.; Schlecker, M.; Quirrenbach, Andreas; Ribas, Ignasi; Reiners, Ansgar; Almenara, J.; Astudillo-Defru, N.; Azzaro, M.; Béjar, Victor J. S.; Bohemann, R.; Bonfils, X.; Bouchy, F.; Cifuentes, C.; Cortés-Contreras, M.; Delfosse, Xavier; Dreizler, Stefan; Forveille, Thierry; Hatzes, Artie P.; Henning, Thomas K.; Jeffers, Sandra V.; Kaminski, Adrian; Kürster, Martin; Lafarga, M.; Lodieu, Nicolas; Lovis, C.; Mayor, M.; Montes, David; Morales, Juan Carlos; Morales, Nicolás; Murgas, F.; Ortiz, José L.; Pepe, F.; Perdelwitz, V.; Pollaco, D.; Santos, N. C.; Schöfer, P.; Schweitzer, A.; Ségransan, N. C.; Shan, Y.; Stock, S.; Tal-Or, Lev; Udry, S.; Zapatero-Osorio, María Rosa; Zechmeister, Mathias (28 de maio de 2021). «The CARMENES search for exoplanets around M dwarfs». Astronomy & Astrophysics. 650: A188. arXiv:2105.13785 . doi:10.1051/0004-6361/202140633
- ↑ Murgas, F.; et al. (2021), «TOI-674b: An oasis in the desert of exo-Neptunes transiting a nearby M dwarf», Astronomy & Astrophysics, 653: A60, Bibcode:2021A&A...653A..60M, arXiv:2106.01246 , doi:10.1051/0004-6361/202140718
- ↑ Brande, Jonathan; Crossfield, Ian J. M.; Kreidberg, Laura; Oklopčić, Antonija; Polanski, Alex S.; Barman, Travis; Benneke, Björn; Christiansen, Jessie L.; Dragomir, Diana; Foreman-Mackey, Daniel; Fortney, Jonathan J.; Greene, Thomas P.; Howard, Andrew W.; Knutson, Heather A.; Lothringer, Joshua D.; Mikal-Evans, Thomas; Morley, Caroline V. (2022), «A Mirage or an Oasis? Water Vapor in the Atmosphere of the Warm Neptune TOI-674 B», The Astronomical Journal, 164 (5): 197, Bibcode:2022AJ....164..197B, arXiv:2201.04197 , doi:10.3847/1538-3881/ac8b7e
- ↑ a b Eisner, N. L.; et al. (2021), «Planet Hunters TESS III: Two transiting planets around the bright G dwarf HD 152843», Monthly Notices of the Royal Astronomical Society, 505 (2): 1827–1840, arXiv:2106.04603 , doi:10.1093/mnras/stab1253
- ↑ a b c d e Hwang, Kyu-Ha; et al. (2021), «Systematic KMTNet Planetary Anomaly Search, Paper II: Five New q<2×10−4 Mass-ratio Planets», arXiv:2106.06686 , doi:10.3847/1538-3881/ac38ad
- ↑ Khandelwal, Akanksha; et al. (2021), «Discovery of an inflated hot Jupiter around a slightly evolved star TOI-1789», Monthly Notices of the Royal Astronomical Society, arXiv:2106.08660 , doi:10.1093/mnras/stab2970
- ↑ a b Wirth, Christopher P.; et al. (2021), «TOI-942b: A Prograde Neptune in a ∼ 60 Myr Old Multi-transiting System», The Astrophysical Journal Letters, 917 (2): L34, Bibcode:2021ApJ...917L..34W, arXiv:2106.14968 , doi:10.3847/2041-8213/ac13a9
- ↑ Han, Cheongho; et al. (2021), «KMT-2018-BLG-1743: Planetary microlensing event occurring on two source stars», Astronomy & Astrophysics, 652: A145, Bibcode:2021A&A...652A.145H, arXiv:2107.00155 , doi:10.1051/0004-6361/202140923
- ↑ a b c Fukui, A.; et al. (2021), «TOI-1749: An M dwarf with a Trio of Planets including a Near-resonant Pair», The Astronomical Journal, 162 (4): 167, Bibcode:2021AJ....162..167F, arXiv:2107.05430 , doi:10.3847/1538-3881/ac13a5
- ↑ a b c d e f Demangeon, O. D. S.; et al. (2021), «The SOPHIE search for northern extrasolar planets», Astronomy & Astrophysics, 653: A78, arXiv:2107.05089 , doi:10.1051/0004-6361/202141079
- ↑ Dalba, Paul A.; et al. (2021), «Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey. II. Discovery of a Failed Hot Jupiter on a 2.7 Yr, Highly Eccentric Orbit», The Astronomical Journal, 162 (4): 154, Bibcode:2021AJ....162..154D, arXiv:2107.06901 , doi:10.3847/1538-3881/ac134b
- ↑ Kanodia, Shubham; et al. (2021), «TOI-532b: The Habitable-zone Planet Finder confirms a Large Super Neptune in the Neptune Desert orbiting a metal-rich M-dwarf host», The Astronomical Journal, 162 (4): 135, Bibcode:2021AJ....162..135K, arXiv:2107.13670 , doi:10.3847/1538-3881/ac1940
- ↑ Wells, R. D.; et al. (2021), «A large sub-Neptune transiting the thick-disk M4 V TOI-2406», Astronomy & Astrophysics, 653: A97, Bibcode:2021A&A...653A..97W, arXiv:2107.14125 , doi:10.1051/0004-6361/202141277
- ↑ a b c Lillo-Box, J.; et al. (2021), «Follow-up of non-transiting planets detected by Kepler», Astronomy & Astrophysics, 654: A9, arXiv:2107.14621 , doi:10.1051/0004-6361/202140746
- ↑ Winters, Jennifer G.; Cloutier, Ryan; Medina, Amber A.; Irwin, Jonathan M.; Charbonneau, David; Astudillo-Defru, Nicola; Bonfils, Xavier; Howard, Andrew W.; Isaacson, Howard; Bean, J. L.; Seifahrt, A.; Teske, J. K.; Eastman, Jason D.; Twicken, Joseph D.; Collins, K. A.; Jensen, E. L. N.; Quinn, S. N.; Payne, M. J.; Kristiansen, M. H.; Spencer, A.; Vanderburg, Andrew; Zechmeister, Mathias; Weiss, L. M.; Wang, S. X.; Wang, G.; Udry, Stéphane; Terentev, I. A.; Sturmer, J.; Stefansson, G.; Shectman, Stephen A.; Sefako, R.; Schwengeler, H. M.; Schwarz, R. P.; Scarsdale, N.; Rubenzahl, R. A.; Roy, A.; Rosenthal, L. J.; Robertson, P.; Petigura, Erik A.; Pepe, Francesco; Omohundro, M.; Murphy, J. M. A.; Murgas, Felipe; Movcnik, T.; Montet, B. T.; Mennickent, R.; Mayo, A. W.; Massey, B.; Lubin, J.; Lovis, Christophe; Lewin, P.; Kasper, D.; Kane, S. R.; Jenkins, J. M.; Huber, D.; Horne, K.; Hill, M. L.; Gorrini, P.; Giacalone, S.; Fulton, Benjamin J.; Forveille, Thierry; Figueira, Pedro; Fetherolf, T.; Dressing, Courtney D.; Díaz, Rodrigo F.; Delfosse, Xavier; Dalba, P. A.; Dai, F.; Cortes, C. C.; Crossfield, Ian J. M.; Crane, Jeffrey D.; Conti, D. M.; Collins, K. I.; Chontos, A.; Butler, R. Paul; Brown, P.; Brady, M.; Bouchy, François; Behmard, A.; Beard, C.; Batalha, Natalie M.; Almenara, José M. (2022). «A Second Planet Transiting LTT 1445A and a Determination of the Masses of Both Worlds». The Astronomical Journal. 163 (4): 168. Bibcode:2022AJ....163..168W. arXiv:2107.14737 . doi:10.3847/1538-3881/ac50a9
- ↑ a b «A warm terrestrial planet with half the mass of Venus transiting a nearby star» (PDF). Consultado em 8 de agosto de 2021. Cópia arquivada (PDF) em 13 de novembro de 2021
- ↑ Lubin, Jack; et al. (2022), «TESS-Keck Survey. IX. Masses of Three Sub-Neptunes Orbiting HD 191939 and the Discovery of a Warm Jovian plus a Distant Substellar Companion», The Astronomical Journal, 163 (2): 101, Bibcode:2022AJ....163..101L, arXiv:2108.02208 , doi:10.3847/1538-3881/ac3d38
- ↑ Shin, In-Gu; et al. (2021), «Using Source Proper Motion to Validate Terrestrial Parallax: OGLE-2019-BLG-1058», The Astronomical Journal, 162 (6): 267, Bibcode:2021AJ....162..267S, arXiv:2108.02499 , doi:10.3847/1538-3881/ac2ba5
- ↑ Saunders, Nicholas; et al. (2022), «TESS Giants Transiting Giants. I.: A Noninflated Hot Jupiter Orbiting a Massive Subgiant», The Astronomical Journal, 163 (2): 53, Bibcode:2022AJ....163...53S, arXiv:2108.02294 , doi:10.3847/1538-3881/ac38a1
- ↑ a b c Osborn, Ares; et al. (2021), «TOI-431/HIP 26013: a super-Earth and a sub-Neptune transiting a bright, early K dwarf, with a third RV planet», Monthly Notices of the Royal Astronomical Society, 507 (2): 2782–2803, arXiv:2108.02310 , doi:10.1093/mnras/stab2313
- ↑ a b Trifonov, Trifon; et al. (2021), «A Pair of Warm Giant Planets near the 2:1 Mean Motion Resonance around the K-dwarf Star TOI-2202», The Astronomical Journal, 162 (6): 283, Bibcode:2021AJ....162..283T, arXiv:2108.05323 , doi:10.3847/1538-3881/ac1bbe
- ↑ 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 De Leon, J. P.; et al. (2021), «37 New Validated Planets in Overlapping K2 Campaigns», Monthly Notices of the Royal Astronomical Society, 508: 195–218, arXiv:2108.05621 , doi:10.1093/mnras/stab2305
- ↑ Kovacs, Geza (2020), «More planetary candidates from K2 Campaign 5 using TRAN_K2», Astronomy & Astrophysics, 643: A169, Bibcode:2020A&A...643A.169K, arXiv:2008.10075 , doi:10.1051/0004-6361/202038726
- ↑ Lillo-Box, J.; et al. (2021), «HD 22496 b: The first ESPRESSO stand-alone planet discovery», Astronomy & Astrophysics, 654: A60, Bibcode:2021A&A...654A..60L, arXiv:2109.00226 , doi:10.1051/0004-6361/202141714
- ↑ a b c d Castro-González, A.; et al. (2022), «The K2-OjOS Project: New and revisited planets and candidates in K2 campaigns 5, 16, & 18», Monthly Notices of the Royal Astronomical Society, 509: 1075–1095, arXiv:2109.03346 , doi:10.1093/mnras/stab2669
- ↑ Dong, Jiayin; et al. (2021), «TOI-3362b: A Proto Hot Jupiter Undergoing High-eccentricity Tidal Migration», The Astrophysical Journal Letters, 920 (1): L16, Bibcode:2021ApJ...920L..16D, arXiv:2109.03771 , doi:10.3847/2041-8213/ac2600
- ↑ a b c Han, Cheongho; et al. (2021), «Three faint-source microlensing planets detected via the resonant-caustic channel», Astronomy & Astrophysics, 655: A21, Bibcode:2021A&A...655A..21H, arXiv:2109.07068 , doi:10.1051/0004-6361/202141517
- ↑ a b Moutou, C.; et al. (2021), «TOI-1296b and TOI-1298b observed with TESS and SOPHIE: Two hot Saturn-mass exoplanets with different densities around metal-rich stars», Astronomy & Astrophysics, 653: A147, Bibcode:2021A&A...653A.147M, arXiv:2109.09252 , doi:10.1051/0004-6361/202141151
- ↑ Kossakowski, D.; et al. (2021), «TOI-1201 b: A mini-Neptune transiting a bright and moderately young M dwarf», Astronomy & Astrophysics, 656: A124, Bibcode:2021A&A...656A.124K, arXiv:2109.09346 , doi:10.1051/0004-6361/202141587
- ↑ Rattanamala, R.; Awiphan, S.; Komonjinda, S.; Phriksee, A.; Sappankum, P.; A-thano, N.; Chitchak, S.; Rittipruk, P.; Sawangwit, U.; Poshyachinda, S.; Reichart, D. E.; Haislip, J. B. (2021), Two circumbinary planets in RR Cae eclipsing binary system, arXiv:2109.09397
- ↑ Montalto, M.; Malavolta, L.; Gregorio, J.; Mantovan, G.; Desidera, S.; Piotto, G.; Nascimbeni, V.; Granata, V.; Manthopoulou, E. E.; Claudi, R. (2022), «TIC 257060897b: An inflated, low-density, hot-Jupiter transiting a rapidly evolving subgiant star», Monthly Notices of the Royal Astronomical Society, 509 (2): 2908–2919, arXiv:2110.00489 , doi:10.1093/mnras/stab2923
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- ↑ Zhang, Michael; Knutson, Heather A.; Wang, Lile; Dai, Fei; Barragán, Oscar (2022), «Escaping Helium from TOI 560.01, a Young Mini-Neptune», The Astronomical Journal, 163 (2): 67, Bibcode:2022AJ....163...67Z, arXiv:2110.13150 , doi:10.3847/1538-3881/ac3fa7
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- ↑ Peng, Peifeng; Xiong, Hongyi; Li, He; Li, Felix; Wang, Tianqi (2022), New Parameter Measurements for the Ultra-Short-Period Planet TOI-1807b, arXiv:2210.04162
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- ↑ Han, Cheongho; et al. (2022), «KMT-2021-BLG-0912Lb: A microlensing super Earth around a K-type star», Astronomy & Astrophysics, 658: A94, Bibcode:2022A&A...658A..94H, arXiv:2111.04861 , doi:10.1051/0004-6361/202142495
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- ↑ Sun, Leilei; Ioannidis, Panagiotis; Gu, Shenghong; Schmitt, Jürgen H. M. M.; Wang, Xiaobin; Kouwenhoven, M. B. N.; Perdelwitz, Volker; Francesco Flammini Dotti; Czesla, Stefan (2022), «A highly mutually inclined compact warm-Jupiter system KOI-984?», Monthly Notices of the Royal Astronomical Society, 512 (3): 4604–4617, arXiv:2111.09668 , doi:10.1093/mnras/stab3367
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- ↑ Smith, A M S.; et al. (2021), «K2-99 revisited: A non-inflated warm Jupiter, and a temperate giant planet on a 522-d orbit around a subgiant», Monthly Notices of the Royal Astronomical Society, 510 (4): 5035–5049, arXiv:2111.14660 , doi:10.1093/mnras/stab3497
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- ↑ Wittenmyer, Robert A.; et al. (2021), «TOI-1842b: A Transiting Warm Saturn Undergoing Re-Inflation around an Evolving Subgiant», The Astronomical Journal, 163 (2): 82, Bibcode:2022AJ....163...82W, arXiv:2112.00198 , doi:10.3847/1538-3881/ac3f39
- ↑ Lam, Kristine W. F.; et al. (2021), «GJ 367b: A dense, ultrashort-period sub-Earth planet transiting a nearby red dwarf star», Science, 374 (6572): 1271–1275, Bibcode:2021Sci...374.1271L, PMID 34855492, arXiv:2112.01309 , doi:10.1126/science.aay3253
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- ↑ Faherty, Jacqueline K.; Gagné, Jonathan; Popinchalk, Mark; Vos, Johanna M.; Burgasser, Adam J.; Schümann, Jörg; Schneider, Adam C.; Kirkpatrick, J. Davy; Meisner, Aaron M.; Kuchner, Marc J.; Bardalez Gagliuffi, Daniella C.; Marocco, Federico; Caselden, Dan; Gonzales, Eileen C.; Rothermich, Austin; Casewell, Sarah L.; Debes, John H.; Aganze, Christian; Ayala, Andrew; Hsu, Chih-Chun; Cooper, William J.; Smart, R. L.; Gerasimov, Roman; Theissen, Christopher A.; The Backyard Worlds; Planet 9 Collaboration (2021), «A Wide Planetary Mass Companion Discovered through the Citizen Science Project Backyard Worlds: Planet 9», The Astrophysical Journal, 923 (1): 48, Bibcode:2021ApJ...923...48F, arXiv:2112.04678 , doi:10.3847/1538-4357/ac2499
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- ↑ a b Mohammed El Mufti; et al. (2021), TOI 560 : Two Transiting Planets Orbiting a K Dwarf Validated with iSHELL, PFS and HIRES RVs, arXiv:2112.13448
- ↑ Miyazaki, Shota; et al. (2022), «OGLE-2014-BLG-0319: A Sub-Jupiter-mass Planetary Event Encountered Degeneracy with Different Mass Ratios and Lens-source Relative Proper Motions», The Astronomical Journal, 163 (3): 123, Bibcode:2022AJ....163..123M, arXiv:2112.14997 , doi:10.3847/1538-3881/ac4960
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