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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


Referências

  1. ↑ «HD 108236 f», exoplanet.eu, consultado em 4 de janeiro de 2021 
  2. ↑ 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 
  3. ↑ 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 
  4. ↑ 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 
  5. ↑ 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 
  6. ↑ 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 
  7. ↑ 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 
  8. ↑ 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 
  9. ↑ 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 
  10. ↑ «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 
  11. ↑ 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 
  12. ↑ 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 
  13. ↑ 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 
  14. ↑ 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 
  15. ↑ 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 
  16. ↑ 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 
  17. ↑ 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 
  18. ↑ 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 
  19. ↑ 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] 
  20. ↑ 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 
  21. ↑ 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 
  22. ↑ 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 
  23. ↑ 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 
  24. ↑ 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 
  25. ↑ 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 
  26. ↑ 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 
  27. ↑ 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 
  28. ↑ 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 
  29. ↑ 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 
  30. ↑ 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 
  31. ↑ 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 
  32. ↑ 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 
  33. ↑ 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 
  34. ↑ 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 
  35. ↑ 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 
  36. ↑ 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 
  37. ↑ 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 
  38. ↑ 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 
  39. ↑ 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 
  40. ↑ 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 
  41. ↑ 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 
  42. ↑ 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 
  43. ↑ 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 
  44. ↑ 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 
  45. ↑ 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 
  46. ↑ 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 
  47. ↑ 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 
  48. ↑ 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 
  49. ↑ 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  
  50. ↑ 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 
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  114. ↑ Cañas, Caleb I.; Mahadevan, Suvrath; Cochran, William D.; Bender, Chad F.; Feigelson, Eric D.; Harman, C. E.; Kopparapu, Ravi Kumar; Caceres, Gabriel A.; Diddams, Scott A.; Endl, Michael; Ford, Eric B.; Halverson, Samuel; Hearty, Fred; Jones, Sinclaire; Kanodia, Shubham; Lin, Andrea S. J.; Metcalf, Andrew J.; Monson, Andrew; Ninan, Joe P.; Ramsey, Lawrence W.; Robertson, Paul; Roy, Arpita; Schwab, Christian; Stefánsson, Guđmundur (2022), «A Hot Mars-sized Exoplanet Transiting an M Dwarf», The Astronomical Journal, 163 (1): 3, Bibcode:2022AJ....163....3C, arXiv:2112.03958 , doi:10.3847/1538-3881/ac3088 
  115. ↑ 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 
  116. ↑ Janson, Markus; Gratton, Raffaele; Rodet, Laetitia; Vigan, Arthur; Bonnefoy, Mickaël; Delorme, Philippe; Mamajek, Eric E.; Reffert, Sabine; Stock, Lukas; Marleau, Gabriel-Dominique; Langlois, Maud; Chauvin, Gaël; Desidera, Silvano; Ringqvist, Simon; Mayer, Lucio; Viswanath, Gayathri; Squicciarini, Vito; Meyer, Michael R.; Samland, Matthias; Petrus, Simon; Helled, Ravit; Kenworthy, Matthew A.; Quanz, Sascha P.; Biller, Beth; Henning, Thomas; Mesa, Dino; Engler, Natalia; Carson, Joseph C. (2021), «A wide-orbit giant planet in the high-mass b Centauri binary system», Nature, 600 (7888): 231–234, Bibcode:2021Natur.600..231J, PMID 34880428, arXiv:2112.04833 , doi:10.1038/s41586-021-04124-8 
  117. ↑ a b c d e f g h i Teng, Huan-Yu; Sato, Bun'ei; Takarada, Takuya; Omiya, Masashi; Harakawa, Hiroki; Izumiura, Hideyuki; Kambe, Eiji; Takeda, Yoichi; Yoshida, Michitoshi; Itoh, Yoichi; Ando, Hiroyasu; Kokubo, Eiichiro (2021), «Regular radial velocity variations in nine G- and K-type giant stars: Eight planets and one planet candidate», Publications of the Astronomical Society of Japan, 74: 92–127, arXiv:2112.07169 , doi:10.1093/pasj/psab112 
  118. ↑ Xie, Xiao-Jia; Dong, Subo; Shvartzvald, Yossi; Gould, Andrew; Udalski, Andrzej; Beaulieu, Jean-Philippe; Beichman, Charles; Close, Laird Miller; b. Henderson, Calen; r. Males, Jared; Marquette, Jean-Baptiste; m. Morzinski, Katie; r. Gelino, Christopher (2022), «Characterizing microlensing planetary system OGLE-2014-BLG-0676Lb with adaptive optics imaging», Research in Astronomy and Astrophysics, 21 (12): 303, arXiv:2112.08030 , doi:10.1088/1674-4527/ac2a09 
  119. ↑ a b Sreenivas, K. R.; Perdelwitz, V.; Tal-Or, L.; Trifonov, T.; Zucker, S.; Mazeh, T. (2022), «Analysis of the public HARPS/ESO spectroscopic archive», Astronomy & Astrophysics, 660: A124, arXiv:2112.09029 , doi:10.1051/0004-6361/202142612 
  120. ↑ 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  
  121. ↑ 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 
  122. ↑ Wang(王涵悦), Hanyue; et al. (2022), «Systematic Korea Microlensing Telescope Network planetary anomaly search – III. One wide-orbit planet and two stellar binaries», Monthly Notices of the Royal Astronomical Society, 510 (2): 1778–1790, arXiv:2112.02414 , doi:10.1093/mnras/stab3581 
Obtida de "https://pt.wikipedia.org/w/index.php?title=Lista_de_exoplanetas_descobertos_em_2021&oldid=66466502"