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Lista de exoplanetas descobertos em 2018

Esta é uma Lista de exoplanetas descobertos em 2018.[1]

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)[2] Método de descoberta Distância (ly) Massa da estrela-mãe (M☉) Temperatura da estrela-mãe (K) Observações
24 Boötis b 0.91+0.13
−0.10 		30.3506+0.0078
−0.0077 		0.190+0.012
−0.009 		Vel. radial 313.9±2.1 0.99+0.19
−0.13 		4893±15 [3]
40 Eridani Ab 0.0266±0.0015 42.378±0.010 0.2190+0.0073
−0.0078 		Vel. radial 16.426±0.042 0.78±0.08 5072±53 [4]
Barnard's Star b 0.0102±0.0013 0.122+0
−0.122 		232.8+0.38
−0.41 		0.404±0.018 105±3 Vel. radial 6 0.144 3134 [5]
COROT-20c 17±1 1675+19
−17 		2.90±0.07 Vel. radial 2819±80 1.14±0.08 6050±200 Anã marrom (possivelmente)[6]
DE Canum Venaticorum b 12±3 4098.1±131.5 5.75±2.02 Tempo 99.64±0.09 0.51 [7]
Gamma Librae b 1.02±0.14 415.2+1.8
−1.9 		1.24±0.10 Vel. radial 154.7±2.9 1.47±0.20 4822±15 [3]
Gamma Librae c 4.58+0.45
−0.43 		964.6±3.1 2.17±0.10 Vel. radial 154.7±2.9 1.47±0.20 4822±15 [3]
Gliese 15 Ac 0.11 7600 5.4 Vel. radial 11.6 0.38 3567 [8]
Gliese 96 b 0.06186+0.00761
−0.00724 		73.94+0.33
−0.38 		0.291±0.005 Vel. radial 38.929±0.0302 0.60±0.07 3785±62 [9]
Gliese 143 b 0.09637+0.00827
−0.00840 		0.228±0.028 35.589+0.006
−0.005 		0.1932±0.0002 Trânsito 53.25±0.02 0.76+0.03
−0.02 		[10]
Gliese 1132 c 0.00831±0.00138 8.929±0.010 0.0476±0.0017 300±5 Vel. radial 41.153±0.023 0.181±0.019 3270±140 [11]
Gliese 1265 b 0.023±0.002 3.6511±0.0012 0.026±0.001 Vel. radial 33.45±0.02 0.18±0.02 3236±51 Estrela-mãe também conhecida como LP 819-052[12]
Gliese 3779 b 0.025±0.002 3.0232±0.0013 0.026±0.001 Vel. radial 44.84±0.04 0.27±0.02 3324±51 Estrela-mãe também conhecida como Ross 1020[12]
HAT-P-11c 1.60+0.09
−0.08 		3407+360
−190 		4.13+0.29
−0.16 		Vel. radial 123.31±0.11 0.809+0.020
−0.030 		4780±50 [13]
HATS-39b 0.63±0.13 1.57±0.12 4.5776348 0.06007±0.00058 1645±43 Trânsito 2910±240 1.379±0.040 6572±83 [14]
HATS-40b 1.59±0.24 1.58+0.16
−0.12 		3.2642736 0.04997±0.00074 2101±69 Trânsito 4550±110 1.561±0.069 6460±130 [14]
HATS-41b 9.7±1.6 1.33+0.29
−0.20 		4.193649 0.0583+0.0015
−0.0010 		1710+170
−120 		Trânsito 2457±47 1.496+0.115
−0.078 		6424±91 [14]
HATS-42b 1.88±0.15 1.40+0.25
−0.14 		2.2921020 0.03689±0.00065 1856+105
−75 		Trânsito 2672±35 1.273±0.067 6060±120 [14]
HATS-54b 0.753±0.057 1.015±0.024 2.5441765±0.0000024 0.0370±0.001 1429±24 Trânsito 2350±30 1.05±0.05 5621±70 [15] Host star also known as NGTS-22[16]
HATS-55b 0.921 1.251 4.2042001 0.05412 1367 Trânsito 2034 1.20 6214 [15]
HATS-56b 0.602 1.688 4.324799 0.06043 1902 Trânsito 1882 1.57 6536 [15]
HATS-57b 3.147 1.139 2.3506210 0.03493 1413.4 Trânsito 913 1.03 5587 [15]
HATS-58Ab 1.03 1.095 4.2180896 0.05798 1721 Trânsito 1605 1.46 7175 [15]
HATS-59b 0.806±0.069 1.126±0.077 5.416081±0.000016 0.06112±0.00076 1128±40 Trânsito 2140±50 1.04±0.04 5670±91 [17]
HATS-59c 12.70±0.87 1422±14 2.504±0.035 175.9±6.4 Vel. radial 2140±50 1.04±0.04 5670±91 [17]
HATS-60b 0.662±0.055 1.153±0.053 3.560829±0.000032 0.04708+0.00015
−0.00023 		1528±11 Trânsito 1609±28 1.097+0.010
−0.016 		5688±20 [18]
HATS-61b 3.40±0.14 1.195±0.067 7.817953±0.000024 0.07908±0.00033 1226.1±7.3 Trânsito 2262±29 1.08±0.01 5542±21 [18]
HATS-62b 0.179+0
−0.179 		1.055±0.025 3.2768837±0.0000033 0.04163+0.00024
−0.00016 		1237±12 Trânsito 1731±34 0.90+0.02
−0.01 		5416+19
−13 		[18]
HATS-63b 0.960±0.120 1.207±0.039 3.0566527±0.0000049 0.04026±0.00028 1398.3±9.0 Trânsito 2070±20 0.93±0.02 5627±18 [18]
HATS-64b 0.960±0.200 1.679±0.081 4.908897±0.000013 0.06562±0.00039 1793±27 Trânsito 3640±140 1.56±0.03 6554±27 [18]
HATS-65b 0.821±0.083 1.501±0.050 3.1051610±0.0000016 0.04497±0.00033 1634±18 Trânsito 1631±41 1.26±0.03 6277±30 [18]
HATS-66b 5.33±0.68 1.411±0.084 3.1414391±0.0000074 0.04714±0.00025 1998±21 Trânsito 5040±130 1.41±0.02 6625±35 [18]
HATS-67b 1.45±0.12 1.685±0.047 1.6091788±0.0000040 0.03032±0.00015 2193±22 Trânsito 3219±80 1.44±0.02 6594±33 [18]
HATS-68b 1.290±0.059 1.232+0.039
−0.029 		3.5862202±0.0000047 0.05071±0.00018 1741±12 Trânsito 2004±34 1.35±0.01 6147±22 [18]
HATS-69b 0.577+0
−0.577 		0.945±0.022 2.2252577±0.0000019 0.03211+0.00014
−0.00019 		1295.7±6.9 Trânsito 1368±11.7 0.89+0.01
−-0.02 		5137±16 [18]
HATS-70b 12.9+1.8
−1.6 		1.384+0.079
−0.074 		1.8882378±0.0000015 0.03632+0.00074
−0.00087 		2730+140
−160 		Trânsito 4263+196
−202 		0.81+0.50
−0.33 		1.08+0.16
−0.14 		[19]
id 0.415±0.020 1.026+0.025
−0.027 		11.53533+0.00079
−0.00080 		0.1097+0.0011
−0.0013 		1228.3+10.0
−9.9 		Trânsito 260.121 1.324+0.042
−0.046 		5521±60 [20][21]
id 1.17±0.12 1.44±0.05 4.12688+0.00005
−0.00004 		0.0568±0.0006 2061±28 Trânsito 645.72+2.77
−2.28 		1.43+0.05
−0.04 		6801±76 [22]
HD 4917 b 1.615±0.092 1.224 400.5±1.7 1.167±0.065 Vel. radial 670.1±8.1 1.32 4802 Dois exoplanetas adicionais no sistema são suspeitos[23]
HD 13167 b 3.31±0.16 1.167 2613±17 4.10±0.34 Vel. radial 487.8±3.5 1.35 5671 [23][24]
HD 14787 b 1.121±0.069 1.250 676.6±8.1 1.70±0.19 Vel. radial 389.9±2.5 1.43 4946 [23]
HD 18015 b 3.18±0.23 1.170 2278±71 3.87±0.32 Vel. radial 405.2±2.6 1.49 5603 [23]
HD 23472 b 0.05638+0.00444
−0.04405 		0.179±0.009 17.667+0.142
−0.095 		0.121±0.001 543±18 Trânsito 127.48±0.06 0.67±0.03 4684±99 [10][25]
HD 23472 c 0.05405+0.00337
−0.04333 		0.167±0.010 29.625+0.224
−0.171 		0.170±0.001 467+19
−18 		transit 127.48±0.06 0.67±0.03 4684±99 [10][25]
HD 33142 c 5.97+1.04
−0.80 		834+29
−24 		Vel. radial 37.34±0.18 1.78±0.31 5009±15 Detecção de margem[23]
HD 55696 b 3.87±0.72 1827±10 3.18±0.18 Vel. radial 255±1 1.29±0.20 6012 [26]
HD 72490 b 1.768±0.080 1.218 858±12 1.88±0.21 Vel. radial 413.5±3.6 1.21 4934 [23]
HD 72490 c 4.5±1.2 3878±261 5.22±0.58 Vel. radial 224±20 1.26±0.25 4867 [23]
HD 89345 b 0.110 0.660 11.81430 0.1066 1089 Trânsito 433.1 1.16 5576 [27] Estrela-mãe também conhecida como K2-234[28]
HD 94834 b 1.26±0.17 1.242 1576±76 2.74±0.18 Vel. radial 321.0±2.1 1.11 4798 [23]
HD 98736 b 2.33±0.78 968.8±2.2 1.864±0.091 Vel. radial 106±0.2 0.92±0.13 5271 [26]
HD 125390 b 22.16 1756.2 3.16 Vel. radial 503 1.36 4850 [23]
HD 148164 b 1.23±0.25 328.55±0.41 0.9930±0.0660 Vel. radial 252±1.0 1.21±0.24 6032 [26]
HD 148164 c 5.16±0.82 5062±114 6.15±0.50 Vel. radial 252±1.0 1.21±0.24 6032 [26]
HD 148284 b 33.7±5.5 339.331±0.018 0.9740±0.0790 Vel. radial 400±2 1.07±0.26 5572 [23]Anã marrom[26]
HD 158996 b 14.0±2.3 820.2±14.0 2.1±0.2 Vel. radial 933±15 1.8±0.3 4069±30 [29]
HD 180053 b 2.194±0.064 1.203 213.72±0.47 0.843±0.063 Vel. radial 448.7±2.0 1.75 5131 [23]
HD 180617 b 0.03839+0.00315
−0.0044 		105.9+0.09
−0.1 		0.3357+0.0099
−0.01 		Vel. radial 19.28±0.07 0.45±0.04 3557±51 Planetary orbit partly in habitable zone[30]
HD 202772 Ab 1.017+0.070
−0.068 		1.545+0.052
−0.060 		3.308958±0.000083 0.05208+0.00064
−0.00068 		2132+28
−30 		Trânsito 480.1+8.2
−7.8 		1.72+0.06
−0.07 		6272+77
−71 		[31]
HD 203473 b 7.8±1.1 1552.9±3.4 2.73±0.17 Vel. radial 237±1.0 1.12±0.21 5780 [26]
HD 211810 b 0.670±0.440 1558±22 2.656±0.043 Vel. radial 211±0.4 1.03±0.02 5652 [26]
HD 215152 b 0.0057+0.0016
−0.0020 		5.7600+0.0016
−0.0018 		0.05764+0.00074
−0.00076 		Vel. radial 70.48±0.16 0.770±0.015 4935±76 [32]
HD 215152 e 0.0091+0.0033
−0.0047 		25.197+0.048
−0.051 		0.1542±0.0020 Vel. radial 70.48±0.16 0.770±0.015 4935±76 [32]
HD 217850 b 21.6±2.6 3501.3±2.1 4.56±0.24 Vel. radial 215±3 1.03±0.16 5544 Provavelmente uma anã marrom[26]
HD 219666 b 0.0552±0.0041 0.4202±0.0152 6.03607±0.00064 0.06356±0.00265 1073±20 Trânsito 307.89±0.98 0.92±0.03 5527±65 [33] Host star also known as TOI-118[34]
HD 220197 b 0.20 1728 2.729 Vel. radial 210 0.91 5683 [35]
HD 233832 b 1.78 2058 2.827 Vel. radial 192 0.71 4981 [35]
HD 238914 b 6.0 4100 5.7 Vel. radial 982 1.47 4769 [36]
IC 4651 9122 b 6.3±0.5 734.0±8.1 2.038±0.039 Vel. radial 2870±110 2.1 9000 [37] Disputed[38]
K2-80d 0.228+0.025
−0.012 		28.8673+0.0051
−0.0046 		0.1778+0.0051
−0.0055 		Trânsito 658.7±5.7 0.90±0.08 5441±249 [24]
K2-138b 0.140 2.35322 0.03380 Trânsito 597 0.93 5378 [39]
K2-138c 0.225 3.55987 0.04454 Trânsito 597 0.93 5378 [39]
K2-138d 0.237 5.40478 0.05883 Trânsito 597 0.93 5378 [39]
K2-138e 0.294 8.26144 0.07807 Trânsito 597 0.93 5378 [39]
K2-138f 0.251 12.75759 0.10430 Trânsito 597 0.93 5378 [39]
K2-141c 0.023+0
−0.023 		0.624+0.410
−0.250 		7.74850 0.06739+0.00089
−0.00091 		Trânsito 202.16±0.54 0.708±0.028 4599±79 [40]
K2-155b 0.015+0.002
−0.001 		0.138+0.018
−0.015 		6.34365 0.0546+0.0013
−0.0014 		708+38
−31 		Trânsito 237.94±0.93 0.65+0.06
−0.03 		4258±150 [41]
K2-155c 0.020+0.005
−0.002 		0.174+0.024
−0.020 		13.85402 0.0946+0.0031
−0.0030 		583+52
−35 		Trânsito 237.94±0.93 0.65+0.06
−0.03 		4258±150 [41]
K2-155d 0.015+0.005
−0.002 		0.146+0.016
−0.015 		40.6835±0.0031 0.1937+0.0064
−0.0059 		381+47
−25 		Trânsito 237.94±0.93 0.65+0.06
−0.03 		4258±150 [41]
K2-156b 0.103+0.009
−0.006 		0.813149 0.0149±0.0001 1347+18
−19 		Trânsito 492.0±3.5 0.66+0.02
−0.01 		4597±50 [42][43]
K2-157b 0.094 0.365257 Trânsito 0.94 5456 [42][43]
K2-158b 0.236+0.014
−0.009 		10.0605+0.0013
−0.0015 		0.0887±0.0008 794±11 Trânsito 647.1±6.7 0.92+0.03
−0.02 		5503+51
−48 		[42]
K2-158c 0.114+0.012
−0.009 		5.9028+0.0019
−0.0023 		0.0622±0.0006 948±13 Trânsito 647.1±6.7 0.92+0.03
−0.02 		5503+51
−48 		[44]
K2-159b 0.202+0.015
−0.010 		12.4221±0.0018 0.1013+0.0008
−0.0009 		684±8 Trânsito 560.4±4.6 0.90+0.02
−0.03 		5425±44 [42]
K2-160b 0.284+0.019
−0.013 		3.705871 0.04660+0.00037
−0.00041 		Trânsito 1038±15 0.983+0.023
−0.025 		5649±50 [42]
K2-161b 0.546+0.146
−0.070 		9.283188 0.0861+0.0018
−0.0023 		Trânsito 3070±160 0.987+0.082
−0.060 		4972±50 [42]
K2-162b 0.128+0.010
−0.006 		9.4589+0.0010
−0.0011 		0.0795±0.0006 631±8 Trânsito 407.3±2.0 0.75±0.02 4842+49
−45 		[42]
K2-163b 0.220+0.023
−0.011 		6.673117 0.06509+0.00050
−0.00060 		Trânsito 684±14 0.826+0.019
−0.023 		4937±50 [42]
K2-164b 0.290+0.046
−0.037 		17.3551+0.0041
−0.0038 		0.1387+0.0036
−0.0025 		Trânsito 1238±25 1.181+0.093
−0.061 		5791±50 [42]
K2-165b 0.1137+0.0129
−0.0087 		2.35499 0.03262±0.00040 Trânsito 440.6±3.9 0.835+0.031
−0.030 		5185±50 [42]
K2-165c 0.1386+0.0187
−0.0098 		4.38275 0.04935±0.00061 Trânsito 440.6±3.9 0.835+0.031
−0.030 		5185±50 [42]
K2-165d 0.236+0.023
−0.013 		14.1014±0.0011 0.1076±0.0013 Trânsito 440.6±3.9 0.835+0.031
−0.030 		5185±50 [42]
K2-166b 0.195+0.018
−0.017 		8.5272±0.0020 0.08583+0.00123
−0.00076 		Trânsito 1577±32 1.16+0.05
−0.03 		5960+52
−53 		[42]
K2-167b 0.252+0.046
−0.040 		9.9775±0.0010 0.0912+0.0036
−0.0029 		Trânsito 264.5±1.5 1.02+0.12
−0.09 		5908±50 [42]
K2-168b 0.191+0.018
−0.012 		15.8540±0.0014 0.1195+0.0013
−0.0014 		Trânsito 801±14 0.907+0.029
−0.032 		5554±50 [42]
K2-169b 0.1136+0.0096
−0.0069 		6.38080 0.06764+0.00063
−0.00061 		Trânsito 774±15 0.986+0.028
−0.026 		5548±50 [42]
K2-170b 0.127+0.018
−0.012 		7.5765+0.0018
−0.0017 		0.07457+0.00083
−0.00086 		Trânsito 1296±21 0.964±0.032 5748±50 [42]
K2-170c 0.161+0.022
−0.014 		12.4000+0.0017
−0.0019 		0.1036+0.0011
−0.0012 		Trânsito 1296±21 0.964±0.032 5748±50 [42]
K2-171b 0.240+0.036
−0.030 		5.6285+0.0017
−0.0015 		0.05960+0.00132
−0.00062 		Trânsito 2010±61 0.892+0.060
−0.027 		5250±50 [42]
K2-172b 0.1486+0.014
−0.0085 		14.3169±0.0014 0.1128+0.0010
−0.0011 		Trânsito 820.3±9.6 0.934+0.026
−0.027 		5569±50 [42]
K2-172c 0.286+0.017
−0.012 		29.6268±0.0016 0.1832+0.0017
−0.0018 		Trânsito 820.3±9.6 0.934+0.026
−0.027 		5569±50 [42]
K2-173b 0.1435+0.0143
−0.0094 		5.86870 0.06105+0.00078
−0.00085} 		Trânsito 750.6±6.4 0.881+0.034
−0.036 		5580±70 [42]
K2-174b 0.2223+0.0157
−0.0087 		19.56274 0.1242±0.0013 Trânsito 326.9±1.2 0.668+0.022
−0.021 		4500±50 [42]
K2-175b 0.182+0.032
−0.024 		9.5260+0.0012
−0.0013 		0.0906+0.0016
−0.0011 		Trânsito 812.2±9.1 1.095+0.057
−0.039 		5909±50 [42]
K2-176b 0.1330+0.0110
−0.0083 		5.32944 0.05846+0.00042
−0.00052 		Trânsito 812±12 0.939+0.020
−0.025 		5428±50 [42]
K2-177b 0.189+0.025
−0.014 		14.1552+0.0032
−0.0030 		0.1221+0.0011
−0.0013 		Trânsito 1628±42 1.211+0.032
−0.038 		6063±50 [42]
K2-178b 0.317+0.018
−0.012 		8.74782 0.08171+0.00066
−0.00081 		Trânsito 704.7±6.0 0.951+0.023
−0.027 		5525±50 [42]
K2-179b 0.224+0.015
−0.011 		5.17219 0.05488+0.00048
−0.00060 		Trânsito 625.7±6.9 0.824+0.022
−0.027 		5015±50 [42]
K2-180b 0.2150+0.0184
−0.0098 		8.86593 0.07550+0.00070
−0.00075 		Trânsito 668.9±5.7 0.730+0.020
−0.022 		5263±50 [42]
K2-181b 0.241+0.028
−0.016 		6.89425 0.07191+0.00055
−0.00067 		Trânsito 1189±17 1.044+0.024
−0.029 		5609±50 [42]
K2-182b 0.063±0.016 0.2469+0.0152
−0.0089 		4.736884 0.05223+0.00048
−0.00064 		Trânsito 507.2±4.1 0.847+0.024
−0.031 		5159±50 [42][24] Confirmado em 2021[45]
K2-183b 0.098±0.090 0.469269 0.011586+0.00010
−0.000087 		Trânsito 1083±14 0.942+0.021
−0.025 		5482±50 [42][24][43]
K2-183c 0.224+0.024
−0.012 		10.79347 0.09371+0.00070
−0.00083 		Trânsito 1083±14 0.942+0.021
−0.025 		5482±50 [42][24][43]
K2-183d 0.227+0.025
−0.013 		22.6295+0.0018
−0.0019 		0.1535+0.0014
−0.0012 		Trânsito 1083±14 0.942+0.021
−0.025 		5482±50 [43]
K2-184b 0.1372+0.0134
−0.0080 		16.99344 0.1210+0.0014
−0.0015 		Trânsito 247.1±1.1 0.819+0.028
−0.030 		5252±50 [42][24]
K2-185b 0.117+0.020
−0.010 		10.6166+0.0016
−0.0018 		0.09378+0.00088
−0.00093 		Trânsito 882±11 0.976+0.027
−0.028 		5722±50 [42]
K2-186b 0.283+0.024
−0.015 		41.4742+0.0033
−0.0043 		0.2359+0.0018
−0.0021 		Trânsito 1089±18 1.019+0.023
−0.027 		5784±50 [42]
K2-187b 0.123 0.773981 Trânsito 0.97 5477 [42][24]
K2-187c 0.152+0.022
−0.010 		2.87179 0.03910+0.00034
−0.00033 		Trânsito 1089±19 0.967+0.025
−0.024 		5477±50 [42][24]
K2-187d 0.287+0.045
−0.022 		7.14908 0.07182+0.00062
−0.00061 		Trânsito 1089±19 0.967+0.025
−0.024 		5477±50 [42][24]
K2-187e 0.201+0.019
−0.012 		13.6083+0.0017
−0.0016 		0.11031+0.00096
−0.00094 		Trânsito 1089±19 0.967+0.025
−0.024 		5477±50 [42][24]
K2-188b 0.112+0.015
−0.010 		1.74298 0.02932+0.000276
−0.000225 		Trânsito 1476±28 1.107+0.031
−0.025 		5982±50 [42][24]
K2-188c 0.234+0.028
−0.016 		7.80760 0.07967+0.00075
−0.00061 		Trânsito 1476±28 1.107+0.031
−0.025 		5982±50 [42][24]
K2-189b 0.1349+0.0136
−0.0085 		5.17630 0.05711+0.00049
−0.00057 		Trânsito 795.2±6.3 0.928+0.024
−0.027 		5503±50 [42][24]
K2-189c 0.222+0.028
−0.012 		6.67934 0.06769+0.00058
−0.00068 		Trânsito 795.2±6.3 0.928+0.024
−0.027 		5503±50 [42][24]
K2-190b 0.1210+0.0157
−0.0091 		10.09886 0.0884+0.0011
−0.0012 		Trânsito 526.5±3.7 0.905+0.033
−0.036 		5631±50 [42]
K2-190c 0.0975+0.0135
−0.0082 		21.5740+0.0057
−0.0043 		0.1467+0.0018
−0.0020 		Trânsito 526.5±3.7 0.905+0.033
−0.036 		5631±50 [42]
K2-191b {{0.141+0.024
−0.012 		2.85865 0.03807+0.00036
−0.00040 		Trânsito 944.5±7.8 0.901+0.026
−0.028 		5176±50 [42]
K2-192b 0.1405+0.0135
−0.0099 		4.16322 0.04840+0.00045
−0.00058 		Trânsito 727.9±5.9 0.873+0.024
−0.031 		5252±50 [42][24]
K2-193b 0.358+0.031
−0.018 		14.78721 0.1177±0.0011 Trânsito 1360±12 0.994+0.029
−0.027 		5623±50 [42] Baixa fidelidade[24]
K2-194b 0.325+0.055
−0.045 		39.7214+0.0057
−0.0056 		0.2359+0.0032
−0.0025 		Trânsito 2090±61 1.110+0.046
−0.035 		5979±52 [42]
K2-195b 0.262+0.018
−0.012 		15.85354 0.1220+0.0012
−0.0014 		Trânsito 1037±14 0.963+0.028
−0.031 		5712±50 [42][24]
K2-195c 0.230+0.024
−0.013 		28.4828+0.0064
−0.0073 		0.1803+0.0018
−0.0020 		Trânsito 1037±14 0.963+0.028
−0.031 		5712±50 [42]
K2-196b 0.321+0.054
−0.045 		48.3242+0.0085
−0.0087 		0.2730+0.0058
−0.0036 		Trânsito 1938±73 1.162+0.075
−0.045 		6045±50 [42]
K2-197b 0.223+0.017
−0.010 		8.35795 0.07992+0.00068
−0.00080 		Trânsito 813.4±7.8 0.975+0.025
−0.029 		5675±50 [42] Baixa fidelidade[24]
K2-198b 0.367+0.023
−0.015 		17.04318 0.1221±0.0014 Trânsito 361.7±2.8 0.836±0.029 5262±50 [42]
K2-199b 0.022±0.006 0.1679+0.0167
−0.0079 		3.225423 0.03804+0.00043
−0.00042 		Trânsito 351.8±2.0 0.706+0.024
−0.023 		4681±50 [42][24][45]
K2-199c 0.039±0.007 0.253+0.015
−0.010 		7.37450 0.06601+0.00075
−0.00074 		Trânsito 351.8±2.0 0.706+0.024
−0.023 		4681±50 [42][24][45]
K2-200b 0.1217+0.0128
−0.0094 		2.84988 0.03741+0.00033
−0.00040 		Trânsito 603.7±6.1 0.860+0.023
−0.027 		5233±50 [42]
K2-201b 0.1249+0.0120
−0.0069 		1.059790 0.02004+0.00014
−0.00015 		Trânsito 649.2±5.4 0.956+0.020
−0.021 		5507±50 [42]
K2-201c 0.293+0.036
−0.016 		22.7799+0.0020
−0.0019 		0.1549+0.0011
−0.0012 		Trânsito 649.2±5.4 0.956+0.020
−0.021 		5507±50 [42]
K2-202b 0.205+0.016
−0.011 		3.40516 0.04387+0.00044
−0.00042 		Trânsito 988.2±8.7 0.971+0.030
−0.028 		5491±58 [42]
K2-203b 0.122+0.025
−0.011 		9.6951±0.0013 0.08238+0.00112
−0.00098 		Trânsito 544.5±5.1 0.794+0.033
−0.028 		5000±50 [42]
K2-204b 0.272+0.039
−0.033 		7.05578 0.07222+0.00074
−0.00066 		Trânsito 1914±58 1.009+0.031
−0.027 		5755±50 [42]
K2-205b 0.178+0.024
−0.021 		26.6723+0.0042
−0.0037 		0.1718+0.0023
−0.0022 		Trânsito 1337±30 0.951+0.038
−0.036 		5890±50 [42]
K2-206b 0.249+0.020
−0.014 		18.2945+0.0017
−0.0016 		0.1256+0.0016
−0.0015 		Trânsito 803±10 0.789+0.030
−0.028 		5043±50 [42]
K2-207b 0.232+0.033
−0.019 		12.4875±0.0012 0.1033±0.0010 Trânsito 1196±18 0.942±0.028 5522±50 [42]
K2-208b 0.150+0.015
−0.011 		4.19095 0.04957+0.00053
−0.00054 		Trânsito 844±10 0.925±0.030 5582±50 [42]
K2-209b 0.0775+0.0094
−0.0056 		2.08062 0.02891+0.00033
−0.00032 		Trânsito 250.05±0.99 0.745+0.026
−0.024 		4720±50 [42]
K2-210b 0.0730+0.0090
−0.0062 		0.570233 0.01305+0.00011
−0.00014 		Trânsito 578.6±6.0 0.912+0.023
−0.029 		5396±50 [42]
K2-211b 0.1226+0.0154
−0.0091 		0.669558 0.01436+0.00011
−0.00015 		Trânsito 895±14 0.882+0.019
−0.027 		5221±50 [42] Outro planeta descoberto em 2020[43]
K2-212b 0.2135+0.0127
−0.0082 		9.79540 0.07648+0.00082
−0.00075 		Trânsito 357.3±3.0 0.622+0.020
−0.018 		4349±50 [42][24]
K2-213b 0.135+0.027
−0.019 		8.1309±0.0018 0.08093+0.00138
−0.00099 		Trânsito 1285±23 1.070+0.055
−0.038 		5794±50 [42]
K2-214b 0.198+0.034
−0.023 		8.59653 0.08273+0.00083
−0.00076 		Trânsito 989±14 1.022+0.031
−0.028 		5768±50 [42][24]
K2-215b 0.189+0.023
−0.014 		8.26965 0.08003+0.00070
−0.00073 		Trânsito 1333±21 1.000+0.026
−0.027 		5704±50 [42]
K2-216b 0.1497+0.0090
−0.0068 		2.174789 0.02916+0.00031
−0.00032 		Trânsito 377.8±2.3 0.699±0.023 4591±50 [42][24]
K2-217b 0.319+0.062
−0.043 		14.07452 0.1179+0.0016
−0.0013 		Trânsito 1259±25 1.103+0.046
−0.037 		5967±50 [42]
K2-218b 0.229+0.025
−0.014 		8.67989 0.08395+0.00082
−0.00075 		Trânsito 1299±32 1.048+0.031
−0.028 		5757±50 [42]
K2-219b 0.120+0.018
−0.016 		3.90129}} 0.04885+0.00054
−0.00048 		Trânsito 1071±16 1.022+0.034
−0.030 		5753±50 [42]
K2-219c 0.128+0.019
−0.017 		6.6677+0.0013
−0.0016 		0.06982+0.00077
−0.00070 		Trânsito 1071±16 1.022+0.034
−0.030 		5753±50 [42]
K2-219d 0.230+0.032
−0.029 		11.13728 0.09830+0.00108
−0.00097 		Trânsito 1071±16 1.022+0.034
−0.030 		5753±50 [42]
K2-220b 0.198+0.023
−0.013 		13.68251 0.11043+0.00099
−0.00112 		Trânsito 766.7±8.9 0.960+0.026
−0.029 		5599±50 [42]
K2-221b 0.1498+0.0149
−0.0085 		2.39909 0.03520+0.00028
−0.00029 		Trânsito 1049±22 1.011+0.024
−0.025 		5716±50 [42]
K2-222b 0.0252±0.0057 0.210±0.007 15.38883 0.1190+0.0016
−0.0015 		Trânsito 331.4±2.0 0.950+0.040
−0.036 		5934±50 [42][24][46]
K2-223b 0.0812+0.0088
−0.0066 		0.505570 0.012664+0.000080
−0.000081 		Trânsito 651.3±8.3 1.06±0.02 5835+38
−40 		[42]
K2-223c 0.144+0.010
−0.006 		4.56417 0.05491±0.00035 Trânsito 651.3±8.3 1.06±0.02 5835+38
−40 		[42]
K2-224b 0.139+0.014
−0.012 		4.47859 0.05422+0.00034
−0.00035 		1002±11 Trânsito 904.8±9.6 0.91±0.02 5620+42
−45 		[42]
K2-224c 0.215+0.014
−0.011 		10.0949+0.0012
−0.0011 		0.08858+0.00065
−0.00066 		764±9 Trânsito 904.8±9.6 0.91±0.02 5620+42
−45 		[42]
K2-225b 0.311+0.023
−0.018 		15.8715+0.0017
−0.0021 		0.13385+0.00140
−0.00072 		902±13 Trânsito 1179±19 1.27+0.02
−0.04 		5742+49
−47 		[42]
K2-226b 0.137+0.012
−0.008 		3.27111 0.04133+0.00047
−0.00048 		1120±16 Trânsito 693±11 0.88±0.03 5424+48
−46 		[42]
K2-227b 0.149+0.109
−0.016 		13.6218+0.0032
−0.0033 		0.1098+0.0011
−0.0012 		Trânsito 613.9±6.7 0.951+0.028
−0.030 		5673±50 [42]
K2-228b 0.108+0.009
−0.005 		2.69837 0.0338±0.0003 914+14
−13 		Trânsito 423±13 0.71±0.02 4715+48
−46 		[42]
K2-229b 0.0082±0.0014 0.102+0.005
−0.003 		0.584249 0.012888±0.00013 1818+14
−15 		Trânsito 335.5±3.5 0.87±0.01 5315+25
−31 		[42]
K2-229c 0.067+0
−0.067 		0.181+0.011
−0.005 		8.32801 0.0769±0.0003 750±6 Trânsito 335.5±3.5 0.87±0.01 5315+25
−31 		[42][44]
K2-230b 0.175+0.016
−0.014 		2.86064 0.0409+0.0003
−0.0002 		1529±22 Trânsito 1791±47 1.11±0.02 5945+23
−25 		[42]
K2-231b 0.22±0.02 13.8419±0.0014 0.1132±0.0011 Trânsito 1057±14 1.01±0.03 5695±50 [47]
K2-232b 0.398±0.037 1.000+0.022
−0.020 		11.168459 0.10356+0.00081
−0.00077 		1001±14 Trânsito 427.9±2.5 1.188+0.028
−0.026 		6154±60 [48][49]
K2-233b 0.1247+.0055
−0.0054 		2.46746 0.03317+0.00044
−0.00045 		1040+28
−26 		Trânsito 220.60±0.91 0.800±0.032 4950±100 [50]
K2-233c 0.1191+0.0074
−0.0069 		7.06142 0.06687 728+20
−19 		Trânsito 220.60±0.91 0.800±0.032 4950±100 [50]
K2-233d 0.236±0.010 24.3662±0.0021 0.1527+0.0020
−0.0021 		482+14
−13 		Trânsito 220.60±0.91 0.800±0.032 4950±100 [50]
K2-236b 0.085+0.044
−0.040 		0.546±0.009 19.49213 0.148±0.004 886±17 Trânsito 595.7±4.2 1.18+0.03
−0.04 		6025±100 [51] Primeiro exoplaneta descoberto por cientistas baseados na Índia.
K2-237b 1.60±0.11 1.65+0.07
−0.08 		2.18056 0.037±0.002 1884+37
−36 		Trânsito 1036±23 1.28+0.03
−0.04 		6257±100 [52][53] Também conhecido como EPIC 229426032 b
K2-238b 0.86+0.13
−0.12 		1.30+0.15
−0.14 		3.20466 0.046± 1587+75
−76 		Trânsito 22000+13000
−50000 		1.19±0.08 5630±78 [52]Também conhecido como EPIC 246067459 b
K2-239b 0.0044±0.0013 0.098±0.009 5.240±0.001 0.0441±0.0008 502+22
−18 		Trânsito 101.48±0.27 0.40±0.01 3420±18 [54]
K2-239c 0.0028±0.0009 0.089±0.009 7.775±0.001 0.0576±0.0009 427+24
−19 		Trânsito 101.48±0.27 0.40±0.01 3420±18 [54]
K2-239d 0.0041±0.0013 0.098±0.009 10.115±0.001 0.0685±0.0012 399+18
−15 		Trânsito 101.48±0.27 0.40±0.01 3420±18 [54]
K2-240b 0.016+0.002
−0.001 		0.18+0.02
−0.01 		6.034±0.001 0.0513±0.0009 586+24
−18 		Trânsito 238.3±1.7 0.58±0.01 3810±17 [54]
K2-240c 0.014+0.002
−0.001 		0.16+0.03
−0.01 		20.523±0.001 0.1159±0.0020 389+19
−17 		Trânsito 238.3±1.7 0.58±0.01 3810±17 [54]
K2-241b 0.227+0.016
−0.009 		26.8199±0.0025 0.1567+0.0007
−0.0008 		507±5 Trânsito 489.6±3.5 0.71±0.01 5262+43
−39 		[44]
K2-242b 0.227+0.019
−0.017 		6.51389 0.0494±0.0004 416±8 Trânsito 357.4±2.0 0.38±0.01 3459+65
−38 		[44]
K2-243b 0.194+0.012
−0.011 		11.5418+0.0027
−0.0022 		0.1087±0.0014 1035+36
−35 		Trânsito 877±11 1.29+0.04
−0.06 		6570+269
−171 		[44]
K2-243c 0.179+0.013
−0.012 		24.9460+0.0049
−0.0056 		0.1817+0.0022
−0.0024 		801+27
−28 		Trânsito 877±11 1.29+0.04
−0.06 		6570+269
−171 		[44]
K2-244b 0.156+0.012
−0.009 		21.0688+0.0032
−0.0033 		0.1418+0.0010
−0.0011 		638±7 Trânsito 698.6±7.8 0.86±0.02 5677+38
−39 		[44]
K2-245b 0.387+0.017
−0.012 		11.89307 0.0959±0.0006 923±14 Trânsito 1507±28 0.83+0.02
−0.01 		5793+66
−52 		[44]
K2-246b 0.311+0.022
−0.019 		5.76918 0.0602±0.0004 977+19
−18 		Trânsito 2341±89 0.87±0.02 5610+32
−29 		[44]
K2-247b 0.189+0.017
−0.014 		2.25021 0.0304±0.0004 979+52
−51 		Trânsito 848.1±6.7 0.74±0.03 4667+305
−183 		[44]
K2-247c 0.195+0.022
−0.021 		6.4942+0.0026
−0.0025 		0.0615±0.0008 688+36
−35 		Trânsito 848.1±6.7 0.74±0.03 4667+305
−183 		[44]
K2-248b 0.229+0.018
−0.012 		7.1726+0.0015
−0.0014 		0.0699±0.0010 886+19
−18 		Trânsito 1341±16 0.88+0.04
−0.03 		5528+97
−86 		[44]
K2-249b 0.249+0.024
−0.020 		12.4090+0.0034
−0.0028 		0.1151+0.0030
−0.0031 		1061±66 Trânsito 1726±55 1.32+0.09
−0.12 		6504+329
−419 		[44]
K2-250b 0.218+0.017
−0.013 		4.01457 0.0459±0.0005 958+14
−13 		Trânsito 1369±21 0.80+0.03
−0.02 		5172+46
−44 		[44]
K2-251b 0.210+0.023
−0.019 		9.3008+0.0033
−0.0032 		0.0694±0.0005 437±9 Trânsito 481.6±3.4 0.52±0.01 3717+85
−50 		[44]
K2-252b 0.155+0.015
−0.011 		13.8151+0.0046
−0.0045 		0.1041+0.0008
−0.0007 		639±7 Trânsito 751.3±6.8 0.79+0.02
−0.01 		5152+41
−39 		[44]
K2-253b 1.130+0.062
−0.054 		4.00167 0.0506+0.0010
−0.0011 		1238+57
−53 		Trânsito 2933±95 1.08+0.05
−0.08 		6027+221
−240 		[44]
K2-254b 0.145+0.025
−0.021 		4.09639 0.0448±0.0005 791±26 Trânsito 747.8±4.2 0.71+0.02
−0.03 		4629+168
−123 		[44]
K2-254c 0.195+0.021
−0.016 		12.1184+0.0030
−0.0032 		0.0923±0.0010 551±18 Trânsito 747.8±4.2 0.71+0.02
−0.03 		4629+168
−123 		[44]
K2-255b 0.259+0.025
−0.010 		1.96417 0.0274±0.0003 1034±17 Trânsito 628.4±5.0 0.71±0.03 4676+63
−61 		[44]
K2-256b 0.235+0.022
−0.019 		5.5201+0.0024
−0.0028 		0.0578±0.0008 845±28 Trânsito 1871±49 0.84+0.03
−0.04 		5219+179
−136 		[44]
K2-257b 0.074+0.005
−0.004 		1.60588 0.0216±0.0002 789±14 Trânsito 209.14±0.84 0.52±0.01 3725+80
−46 		[44]
K2-258b 0.268+0.019
−0.018 		19.0921+0.0058
−0.0063 		0.1490+0.0025
−0.0026 		{831±30 Trânsito 2201±37 1.21+0.05
−0.08 		6351+198
−228 		[44]
K2-259b 0.207+0.018
−0.015 		15.4804+0.0033
−0.0039 		0.1271+0.0010
−0.0011 		795±13 Trânsito 1374±27 1.14±0.03 6059+62
−76 		[44]
K2-260b 1.42+0.31
−0.32 		1.552+0.048
−0.057 		2.6266657 0.0404+0.0013
−0.0016 		1957+78
−77 		Trânsito 2206±63 1.39+0.05
−0.06 		6367±250 [55]
K2-261b 0.223±0.031 0.850+0.026
−0.022 		11.63344 0.102+0.019
−0.020 		1080+110
−100 		Trânsito 699.9±6.4 1.10+0.01
−0.02 		5537±71 [55]
K2-263b 0.0466±0.0098 0.215±0.011 50.818947±0.000094 0.2573±0.0029 470±10 Trânsito 532±4 0.88±0.03 5368±44 [56]
K2-264b 0.203+0.018
−0.014 		5.839770+0.000061
−0.000063 		489+12
−13 		Trânsito 609±7 0.47±0.01 3580±70 [57][58]
K2-264c 0.247+0.018
−0.016 		19.663650+0.000303
−0.000306 		326+8
−9 		Trânsito 609±7 0.47±0.01 3580±70 [57][58]
K2-265b 0.0206±0.0026 0.153±0.010 2.369172±0.000089 0.03376±0.00021 Trânsito 454±3 0.912±0.02 5477±27 [59][60]
K2-266b 0.0356+0.0346
−0.0205 		0.29+0.16
−0.12 		0.658524±0.000017 0.01306+0.00020
−0.00021 		1515±18 Trânsito 251.7+1.95
−1.92 		0.686±0.033 4285+49
−57 		[61]
K2-266c 0.00091+0.00053
−0.00035 		0.0629+0.0086
−0.0076 		7.8140+0.0019
−0.0016 		0.0679±0.0011 664.5+8.0
−7.7 		Trânsito 251.7+1.95
−1.92 		0.686±0.033 4285+49
−57 		[61]
K2-266d 0.0296+0.0091
−0.0063 		0.261+0.012
−0.011 		14.69700+0.00034
−0.00035 		0.1035+0.0016
−0.0017 		538.3+6.5
−6.3 		Trânsito 251.7+1.95
−1.92 		0.686±0.033 4285+49
−57 		[61]
K2-266e 0.0261+0.0085
−0.0057 		0.244+0.012
−0.010 		19.4820±0.0012 0.1249+0.0019
−0.0020 		490.1+5.9
−5.7 		Trânsito 251.7+1.95
−1.92 		0.686±0.033 4285+49
−57 		Mais dois exoplanetas são suspeitos[61]
K2-267b 3.0+1.1
−1.2 		1.051±0.044 6.180235±0.000014 0.07229+0.00074
−0.00075 		1401±16 Trânsito 1098+27
−26 		1.317+0.041
−0.040 		6202+52
−50 		Estrela-mãe não confirmada, também conhecida como EPIC 246851721[62]
K2-268b 0.126±0.012 2.151894+0.000393
−0.000363 		0.0308±0.0002 1121±14 Trânsito 1081.1±10.27 0.84±0.02 5068±51 [24]
K2-268c 0.240±0.021 9.326841+0.001532
−0.001617 		0.0819±0.0006 688±8 Trânsito 1081.1±10.27 0.84±0.02 5068±51 [24]
K2-269b 0.140±0.011 4.144965+0.000817
−0.000619 		0.0531±0.0006 1429±37 Trânsito 1180.1±47.0 1.16±0.04 6209±88 [24]
K2-270b 0.123±0.010 1.543069+0.000189
−0.000185 		0.0247±0.0002 1203±17 Trânsito 924.75±7.60 0.85±0.02 4877±58 [24]
K2-270c 0.263±0.014 4.400028+0.000169
−0.000178 		0.0497±0.0004 848±12 Trânsito 924.75±7.60 0.85±0.02 4877±58 [24]
K2-271b 0.649±0.021 8.562421±0.000127 0.0770+0.0008
−0.0009 		893±17 Trânsito 1863.9±44.32 0.83±0.03 5644±71 [24]
K2-272b 0.260±0.013 14.453533+0.001328
−0.001360 		0.1081+0.0016
−0.0017 		655±12 Trânsito 1391.3±17.3 0.81±0.04 5419±79 [24]
K2-273b 0.394±0.114 11.716332+0.001172
−0.001198 		0.0974±0.0011 672±11 Trânsito 1013.0±9.39 0.90±0.03 5200±67 [24]
K2-274b 0.196±0.011 14.129714+0.0021022
−0.001876 		0.1064+0.0009
−0.0008 		589±9 Trânsito 1013.0±9.39 0.81±0.02 5065±60 [24]
K2-275b 0.200±0.011 3.280961+0.000112
−0.000107 		0.0400±0.0003 905±13 Trânsito 404.73±2.28 0.79±0.02 4812±59 [24]
K2-275c 0.209±0.009 8.438756+0.000269
−0.000271 		0.0750±0.0005 660±9 Trânsito 404.73±2.28 0.79±0.02 4812±59 [24]
K2-276b 0.336±0.019 18.718269+0.003153
−0.003008 		0.1291±0.0011 583+10
−9 		Trânsito 1597.8±23.9 0.82±0.02 5139±62 [24]
K2-277b 0.185±0.011 6.326763+0.000355
−0.000361 		0.0675±0.0006 958±14 Trânsito 370.29±2.28 1.02±0.03 5741±65 [24]
K2-278b 0.266±0.021 3.334966+0.000701
−0.000859 		0.0488±0.0009 1711±101 Trânsito 2622.7±53.7 1.40±0.08 6747±383 [24]
K2-279b 0.108±0.012 7.122605+0.001647
−0.001601 		0.0670+0.0008
−0.0009 		879±14 Trânsito 599.48±5.15 0.79±0.03 5558±70 [24]
K2-280b 0.684±0.023 19.895202+0.000774
−0.000753 		0.1488+0.0019
−0.0020 		744±15 Trânsito 1294.5±2.38 1.11±0.04 5742±90 [63][24][64][42]
K2-281b 0.730±0.019 8.687721+0.000151
−0.000150 		0.0773±0.0008 665±12 Trânsito 1520.2±23.6 0.82±0.03 4812±72 [24]
K2-282b 0.252±0.012 4.169836+0.000279
−0.000300 		0.0499+0.0006
−0.0007 		1057±20 Trânsito 1638.2±25.3 0.95±0.04 5523±82 [24]Mais dois exoplanetas descobertos em 2019 e 2020[43]
K2-283b 0.314±0.014 1.921036+0.000051
−0.000053 		0.0291±0.0003 1186±20 Trânsito 1331.5±15.7 0.89±0.03 5060±70 [24]
K2-284b 0.248+0.012
−0.011 		4.795069±0.000086 0.04771±0.00025 653+16
−14 		Trânsito 351.0±1.6 0.63±0.01 4140±50 Estrela-mãe muito jovem[65]
K2-285b 0.03046+0.00381
−0.00431 		0.231±0.005 3.471745+0.000044
−0.000046 		0.03817+0.00095
−0.00092 		1088.9+22.1
−21.9 		Trânsito 508±4 0.83±0.02 4975±95 [66]
K2-285c 0.04933+0.00717
−0.00670 		0.315±0.007 7.138048+0.000072
−0.000063 		0.0824±0.0018 741.4±14.5 Trânsito 508±4 0.83±0.02 4975±95 [66]
K2-285d 0.020±0.020 0.221±0.005 10.45582+0.00025
−0.00023 		0.1178±0.0029 619.9+12.7
−12.5 		Trânsito 508±4 0.83±0.02 4975±95 [66]
K2-285e 0.0337+0
−0.0337 		0.174±0.004 14.76289+0.00065
−0.00061 		0.18041+0.00420
−0.00430 		500.9+10.1
−9.9 		Trânsito 508±4 0.83±0.02 4975±95 [66]
K2-287b 0.315±0.027 0.847±0.013 14.893291±0.000025 0.1206±0.0008 804+8
−7 		Trânsito 518.7±4.2 1.06±0.02 5695±58 [67]
K2-292b 0.0771±0.0138 0.235+0.010
−0.009 		16.9841±0.0008 0.13±0.01 795+33
−28 		Trânsito 372.76+2.67
−2.64 		1.00±0.03 5725±65 Estrela-mãe também conhecida como HD 119130[68]
K2-295b 0.335±0.062 {0.897+0.011
−0.005 		4.024867±0.000015 0.0451+0.0006
−0.0014 		852+14
−6 		Trânsito 736.1±7.8 0.74±0.04 4444±70 [53]
K2-311b 13 1.11±0.07 3650+1280
−1130 		4.5±1.0 183+25
−18 		Trânsito 1826.48 0.90±0.09 4898±68 [69]
Kepler-730c 0.140±0.012 2.851883380 0.03997+0.00089
−0.00069 		1607+27
−29 		Trânsito 6590+254
−267 		1.05+0.07
−0.05 		5620+55
−59 		[70]
Kepler-1654b 0.819+0.019
−0.017 		1047.8356+0.0018
−0.0019 		2.026+0.037
−0.035 		206.0+3.7
−3.5 		Trânsito 1884±13 1.011+0.056
−0.052 		5597+95
−93 		[71]
Kepler-1655b 0.016+0.010
−0.009 		0.1974±0.0073 11.87290396 0.103±0.001 Trânsito 699.9±3.2 1.03±0.04 6148±71 Semelhante a um mini-Netuno[72]
Kepler-1656b 0.153+0.013
−0.012 		0.448±0.047 31.578659 0.197±0.021 651+51
−47 		Trânsito 610±3 1.03±0.04 5731±60 Órbita altamente excêntrica[73]
Kepler-1657b 1.93+0.19
−0.21 		0.990+0.060
−0.070 		141.241671±0.000086 0.534+0.012
−0.030 		347±12 Trânsito 3090±80 1.01+0.07
−0.16 		5830±100 Também conhecido como KOI-3680 b em Exoplanet Archive[74]
KMT-2016-BLG-1397Lb 7.00+5.20
−4.30 		5.1+1.5
−1.7 		Microlente 22000+3600
−4200 		0.45+0.33
−0.28 		[75]
KMT-2016-BLG-1820Lb 4.57+5.03
−2.14 		1.08+0.22
−0.24 		Microlente 20420+3720
−4170 		0.039+0.043
−0.018 		[76]
KMT-2016-BLG-2142Lb 15.49+24.99
−8.58 		0.830+0.150
−0.200 		Microlente 7010+1010
−1160 		0.0730+0.1170
−0.0400 		[76]
KPS-1b 1.090+0.086
−0.087 		1.03+0.13
−0.12 		1.706291 0.0269±0.0010 1459±56 Trânsito 863.3±8.5 0.892+0.090
−0.100 		5165±90 Primeiro exoplaneta em trânsito encontrado por um astrônomo amador[77]
LHS 1140 c 0.00569±0.00123 0.1144±0.0021 3.777931±0.000003 0.02675±0.00070 438±9 Trânsito 40.67±1.37 0.18±0.01 3216±39 [78]
MOA-2011-BLG-291Lb 0.057+0.107
−0.038 		0.69±0.24 Microlente 14000±4600 0.15+0.27
−0.10 		[79]
MOA-2015-BLG-337Lb 0.1060+0.4059
−0.0730 		0.24+0.06
−0.09 		Microlente 23000+3600
−3300 		0.00940+0.03590
−0.00650 		[80]
MOA-2016-BLG-319Lb 0.620+1.160
−0.330 		0.950+0.170
−0.200 		Microlente 22000+3900
−4600 		0.15+0.28
−0.08 		[81]
NGTS-2b 0.74+0.13
−0.12 		1.595+0.047
−0.045 		4.511164±0.000061 0.0630+0.0024
−0.0030 		1468+45
−42 		Trânsito 1174+27
−25 		1.64+0.19
−0.22 		6478+94
−89 		[82] Also known as WASP-179b[83]
NGTS-3Ab 2.38±0.26 1.48±0.37 1.6753728 0.023+0.007
−0.005 		Trânsito 2480±36 1.017±0.093 5600±150 [84]
NGTS-4b 0.0648±0.0094 0.284±0.023 1.3373508±0.0000080 0.019±0.005 1650±400 Trânsito 921.7±5.9 0.75±0.02 5143±100 [85]
OGLE-2011-BLG-0173Lb 0.19+0.18
−0.11 		8 Microlente 20000+4200
−5500 		0.41+0.30
−0.21 		[86] Not the planetary candidate OGLE-2017-BLG-0173Lb!
OGLE-2014-BLG-1722Lb 0.17+0.16
−0.10 		1512+3715
−1029 		1.9+1.3
−0.8 		Microlente 20900+4200
−5900 		0.40+0.36
−0.24 		3500+1490
−470 		[87]
OGLE-2014-BLG-1722Lc 0.26+0.27
−0.16 		2283+7021
−1589 		2.5+2.2
−1.1 		Microlente 20900+4200
−5900 		0.40+0.36
−0.24 		3500+1490
−470 		[87]
OGLE-2015-BLG-1670Lb 0.0563+0.0302
−0.0277 		2.62+0.58
−0.60 		Microlente 22000+3300
−4200 		0.55±0.28 [88]
OGLE-2016-BLG-1067Lb 0.43 1.7 Microlente 12165.633 0.3 [89]
OGLE-2017-BLG-0373Lb 0.40+0.64
−0.26 		2768+3343
−1704 		2.42+0.76
−0.78 		Microlente 19200+4200
−6400 		0.25+0.27
−0.13 		3250+500
−300 		[90]
OGLE-2017-BLG-0482Lb 0.0283+0.028
−0.014 		1972+1306
−2322 		1.8+0.6
−0.7 		Microlente 18900+5900
−6800 		0.20+0.20
−0.10 		3150+350
−300 		[91]
OGLE-2017-BLG-1140Lb 1.59+0.35
−0.26 		819+253
−218 		1.02±0.15 Microlente 11300 0.211+0.032
−0.025 		3170+60
−50 		[92]
OGLE-2017-BLG-1522Lb 0.75+1.26
−0.40 		780+728
−431 		0.59+0.12
−0.11 		Microlente 3200+3000
−1800 		0.045+0.076
−0.024 		1500+1000
−500 		[93]
OGLE-2017-BLG-1434Lb 0.014±0.002 968±69 1.18±0.10 Microlente 2800±290 0.234±0.026 3220+30
−70 		[94] Exoplaneta confirmado em 2021[95]
PDS 70b 8.0±6.0 >1.3 43500 22 Imagem direta 369.96±1.70 0.76±0.02 3972±36 [96]
Pi Mensae c 0.0152+0.0026
−0.0027 		0.1822±0.0045 6.26790±0.00046 0.06839±0.00050 1169.8+2.8
−4.3 		Trânsito 59.62±0.073 1.094±0.039 6037±45 [97]
Qatar-7b 1.88±0.25 1.70±0.03 {2.0320460±0.0000097 0.0352±0.0002 Trânsito 2364.6337 1.409±0.026 6387±38 [98]
TCP J05074264+2447555 b 0.0289±0.0208 0.5 Microlente 1200 0.25±0.18 [99] Also known as Kojima-1Lb[100]
TYC 3318-1333-1 b 3.42±0.35 562.0+4.1
−4.0 		1.414±0.063 Vel. radial 1622±33 1.19±0.14 4776±10 [36]
UKIRT-2017-BLG-001Lb 1.28+0.37
−0.44 		3468+2324
−1300 		4.18+0.96
−0.88 		Microlente 20500+5200
−6800 		0.81+0.21
−0.27 		5100+700
−1300 		[101]
WASP-134b 1.40±0.08 10.1498 0.0956±0.0025 953±22 Trânsito 636±7 0.81±0.04 5700±100 [102]
WASP-134c 0.70±0.07 70.01±0.14 Vel. radial 636±7 0.81±0.04 5700±100 [102]
WASP-137b 0.681±0.054 1.27±0.11 3.9080284±0.0000053 0.0519±0.0018 1601±65 Trânsito 943±13 1.216±0.066 6100±140 [102]
WASP-143b 0.725±0.084 1.234±0.042 3.7788730±0.0000032 0.0490±0.0014 1325±30 Trânsito 1310±20 1.087±0.045 5900±140 [102]
WASP-144b 0.44±0.06 0.85±0.05 2.2783152±0.0000013 0.0316±0.0005 1260±40 Trânsito 1170±34 0.81±0.04 5200±140 [103]
WASP-145Ab 0.89±0.04 0.90±0.40 1.7690381±0.0000008 0.0261±0.0005 1200±60 Trânsito 298±0.8 0.76±0.04 4900±150 [103]
WASP-146b 1.11±0.15 1.228±0.076 3.3969440±0.0000036 0.0451±0.0024 1486±43 Trânsito 1610±90 1.057±0.085 6100±140 [102]
WASP-147b 0.275+0.028
−0.027 		1.115+0.140
−0.093 		4.602730±0.000027 0.0549+0.0012
−0.0013 		1404+69
−43 		Trânsito 1390±46 1.044+0.070
−0.073 		5702±100 [104]
WASP-158b 2.79±0.23 1.07±0.15 3.656333±0.000004 0.0517±0.0018 1590±80 Trânsito 1740±41 1.38±0.14 6350±150 [103]
WASP-159b 0.55±0.08 1.38±0.09 3.840401±0.000007 0.0538±0.0015 1850±50 Trânsito 2382±36 1.41±0.12 6120±140 [103]
WASP-160Bb 0.278+0.044
−0.045 		1.090+0.047
−0.041 		3.7684952±0.0000035 0.0452±0.0012 1119+25
−23 		Trânsito 926±16 9.750±2.280 5298±99 [104]
WASP-161b 2.49±0.21 1.143+0.065
−0.058 		5.4060425±0.0000048 0.0673±0.0023 1557+34
−29 		Trânsito 1130±14 1.39±0.14 6400±100 [105] Nome próprio Isli
WASP-162b 5.2±0.2 1.00±0.05 9.62468±0.00001 0.0871±0.0013 910±20 Trânsito 1023±13 0.95±0.04 5300±100 [103]
WASP-163b 1.87±0.21 1.202±0.097 1.6096884±0.0000015 0.0266±0.0014 1638±68 Trânsito 858±12 0.97±0.15 5500±200 [105]
WASP-164b 2.13+0.12
−0.13 		1.128+0.041
−0.043 		1.7771255±0.0000028 0.02818+0.00065
−0.00072 		1610+58
−53 		Trânsito 1050±23 0.9460+0.0670
−0.0710 		5806+190
−200 		[104]
WASP-165b 0.658+0.097
−0.092 		1.26+0.19
−0.17 		3.465509±0.000023 0.04823+0.00091
−0.00092 		1624+93
−89 		Trânsito 1900±110 1.248+0.072
−0.070 		5599±150 [104]
WASP-166 b 0.101±0.005 0.63±0.03 5.443540±0.000004 0.0641±0.0011 1270±30 Trânsito 368.55 1.19±0.06 6050±50 [106][107][108]
WASP-168b 0.42±0.04 1.5+0.5
−0.3 		4.153658±0.000003 0.0519±0.0008 1340±40 Trânsito 1000±6 1.08±0.05 6000±100 [103]
WASP-170b 1.6±0.2 1.096±0.085 2.34478022±0.00000360 0.0337±0.0018 1422±42 Trânsito 1005±12 0.93±0.15 5600±150 [105]
WASP-172b 0.47±0.10 1.57±0.10 5.477433±0.000007 0.0694±0.0011 1740±60 Trânsito 1780±50 1.49±0.07 6900±140 [103]
WASP-173Ab 3.69±0.18 1.20±0.06 1.38665318±0.00000027 0.0248±0.0006 1880±55 Trânsito 235±5.8 1.05±0.08 5800±140 [103]Também conhecido como KELT-22Ab[109]
WASP-174b 1.3+0
−1.3 		1.3 4.233700 0.0559 1490 Trânsito 1350 1.30 6400 [110]
WASP-190b 1.0±0.1 1.15±0.09 5.367753±0.000004 0.0663±0.0008 1500±50 Trânsito 1796.323 1.35±0.05 6400±100 [111]
Wolf 503b 0.020±0.002 0.1811+0.0068
−0.0065 		6.00118+0.00008
−0.00011 		0.0571±0.0020 805±9 Trânsito 145.4±0.3 0.688+0.023
−0.016 		4716±60 [112][113]

Listas específicas de exoplanetas

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Referências

  1. ↑ «NASA Exoplanet Archive». exoplanetarchive.ipac.caltech.edu. California Institute of Technology. Consultado em 27 de março de 2018 
  2. ↑ «The Extrasolar Planets Encyclopaedia». Consultado em 20 de janeiro de 2018 
  3. ↑ a b c Takarada, Takuya; et al. (2018). «Planets around the evolved stars 24 Booties and γ Libra: A 30d-period planet and a double giant-planet system in possible 7:3 MMR». Publications of the Astronomical Society of Japan. 70 (4). arXiv:1804.04008 . doi:10.1093/pasj/psy052 
  4. ↑ Ma, Bo; et al. (2018). «The first super-Earth Detection from the High Cadence and High Radial Velocity Precision Dharma Planet Survey». Monthly Notices of the Royal Astronomical Society. 480 (2). 2411 páginas. Bibcode:2018MNRAS.480.2411M. arXiv:1807.07098 . doi:10.1093/mnras/sty1933 
  5. ↑ Ribas, I.; Tuomi, M.; Reiners, Ansgar; Butler, R. P.; et al. (14 de novembro de 2018). «A candidate super-Earth planet orbiting near the snow line of Barnard's star» (PDF). Omega Space Exploration or OSE. Nature. 563 (7731): 365–368. Bibcode:2018Natur.563..365R. ISSN 0028-0836. OCLC 716177853. PMID 30429552. arXiv:1811.05955 . doi:10.1038/s41586-018-0677-y. hdl:2299/21132. Cópia arquivada (PDF) em 26 de março de 2019 
  6. ↑ Rey, J.; Bouchy, F.; Stalport, M.; Deleuil, M.; Hébrard, G.; Almenara, J. M.; Alonso, R.; Barros, S. C. C.; Bonomo, A. S.; Cazalet, G.; Delisle, J. B.; Díaz, R. F.; Fridlund, M.; Guenther, E. W.; Guillot, T.; Montagnier, G.; Moutou, C.; Lovis, C.; Queloz, D.; Santerne, A.; Udry, S. (2018), «Brown dwarf companion with a period of 4.6 yr interacting with the hot Jupiter CoRoT-20 B», Astronomy & Astrophysics, 619: A115, arXiv:1807.01229 , doi:10.1051/0004-6361/201833180 
  7. ↑ Han, Z.-T.; Qian, S.-B.; Zhu, L.-Y.; Zhi, Q.-J.; Dong, A.-J.; Soonthornthum, B.; Poshyachinda, S.; Sarotsakulchai, T.; Fang, X.-H.; Wang, Q.-S.; Voloshina, Irina (2018). «DE CVn: An Eclipsing Post-common Envelope Binary with a Circumbinary Disk and a Giant Planet». The Astrophysical Journal. 868: 53. doi:10.3847/1538-4357/aae64d  
  8. ↑ Pinamonti, M.; Damasso, M.; Marzari, F.; Sozzetti, A.; Desidera, S.; Maldonado, J.; Scandariato, G.; Affer, L.; Lanza, A. F.; Bignamini, A.; Bonomo, A. S.; Borsa, F.; Claudi, R.; Cosentino, R.; Giacobbe, P.; González-Álvarez, E.; González Hernández, J. I.; Gratton, R.; Leto, G.; Malavolta, L.; Martinez Fiorenzano, A.; Micela, G.; Molinari, E.; Pagano, I.; Pedani, M.; Perger, M.; Piotto, G.; Rebolo, R.; Ribas, I.; et al. (2018). «The HADES RV Programme with HARPS-N at TNG. VIII. GJ15A: A multiple wide planetary system sculpted by binary interaction». Astronomy and Astrophysics. 617: A104. Bibcode:2018A&A...617A.104P. arXiv:1804.03476 . doi:10.1051/0004-6361/201732535 
  9. ↑ Hobson, M. J.; et al. (2018), «The SOPHIE search for northern extrasolar planets», Astronomy & Astrophysics, 618: A103, arXiv:1806.10958 , doi:10.1051/0004-6361/201832732 
  10. ↑ a b c Trifonov, Trifon; Rybizki, Jan; Kürster, Martin (2019), «TESS exoplanet candidates validated with HARPS archival data», Astronomy & Astrophysics, 622: L7, arXiv:1812.04501 , doi:10.1051/0004-6361/201834817 
  11. ↑ Bonfils, X.; Almenara, J.-M.; Cloutier, R.; Wünsche, A.; Astudillo-Defru, N.; Berta-Thompson, Z.; Bouchy, F.; Charbonneau, D.; Delfosse, X.; Díaz, R. F.; Dittmann, J.; Doyon, R.; Forveille, T.; Irwin, J.; Lovis, C.; Mayor, M.; Menou, K.; Murgas, F.; Newton, E.; Pepe, F.; Santos, N. C.; Udry, S. (2018), «Radial velocity follow-up of GJ1132 with HARPS», Astronomy & Astrophysics, 618: A142, arXiv:1806.03870 , doi:10.1051/0004-6361/201731884 
  12. ↑ a b Luque, R.; Nowak, G.; Pallé, E.; Kossakowski, D.; Trifonov, T.; Zechmeister, M.; Béjar, V. J. S.; Cardona Guillén, C.; Tal-Or, L.; Hidalgo, D.; Ribas, I.; Reiners, A.; Caballero, J. A.; Amado, P. J.; Quirrenbach, A.; Aceituno, J.; Cortés-Contreras, M.; Díez-Alonso, E.; Dreizler, S.; Guenther, E. W.; Henning, T.; Jeffers, S. V.; Kaminski, A.; Kürster, M.; Lafarga, M.; Montes, D.; Morales, J. C.; Passegger, V. M.; Schmitt, J. H. M. M.; Schweitzer, A. (2018), «The CARMENES search for exoplanets around M dwarfs», Astronomy & Astrophysics, 620: A171, arXiv:1810.07572 , doi:10.1051/0004-6361/201833423 
  13. ↑ Yee, Samuel W.; et al. (2018). «HAT-P-11: Discovery of a Second Planet and a Clue to Understanding Exoplanet Obliquities». The Astronomical Journal. 155 (6). 255. Bibcode:2018AJ....155..255Y . arXiv:1805.09352 . doi:10.3847/1538-3881/aabfec  
  14. ↑ a b c d Bento, J.; Hartman, J. D.; Bakos, G. Á.; Bhatti, W.; Csubry, Z.; Penev, K.; Bayliss, D.; De Val-Borro, M.; Zhou, G.; Brahm, R.; Espinoza, N.; Rabus, M.; Jordán, A.; Suc, V.; Ciceri, S.; Sarkis, P.; Henning, T.; Mancini, L.; Tinney, C. G.; Wright, D. J.; Durkan, S.; Tan, T. G.; Lázár, J.; Papp, I.; Sári, P. (2018), «HATS-39b, HATS-40b, HATS-41b, and HATS-42b: Three inflated hot Jupiters and a super-Jupiter transiting F stars», Monthly Notices of the Royal Astronomical Society, 477 (3): 3406–3423, arXiv:1804.01623 , doi:10.1093/mnras/sty726 
  15. ↑ a b c d e Espinoza, N.; Hartman, J. D.; Bakos, G. Á.; Henning, T.; Bayliss, D.; Bento, J.; Bhatti, W.; Brahm, R.; Csubry, Z.; Suc, V.; Jordán, A.; Mancini, L.; Tan, T. G.; Penev, K.; Rabus, M.; Sarkis, P.; De Val-Borro, M.; Durkan, S.; Lázár, J.; Papp, I.; Sári, P. (2018), «HATS-54b–HATS-58Ab: Five New Transiting Hot Jupiters Including One with a Possible Temperate Companion», The Astronomical Journal, 158 (2): 63, arXiv:1812.07668 , doi:10.3847/1538-3881/ab26bb 
  16. ↑ Jackson, David G.; et al. (2022), «The discovery of three hot Jupiters, NGTS-23b, 24b and 25b, and updated parameters for HATS-54b from the Next Generation Transit Survey», Monthly Notices of the Royal Astronomical Society, 518 (4): 4845–4860, arXiv:2211.01044 , doi:10.1093/mnras/stac3192 
  17. ↑ a b Sarkis, P.; Henning, Th.; Hartman, J. D.; Bakos, G. Á.; Brahm, R.; Jordán, A.; Bayliss, D.; Mancini, L.; Espinoza, N.; Rabus, M.; Csubry, Z.; Bhatti, W.; Penev, K.; Zhou, G.; Bento, J.; Tan, T. G.; Arriagada, P.; Butler, R. P.; Crane, J. D.; Shectman, S.; Tinney, C. G.; Wright, D. J.; Addison, B.; Durkan, S.; Suc, V.; Buchhave, L. A.; Val-Borro, M. de; Lázár, J.; Papp, I.; Sári, P. (2018), «HATS-59b,c: A Transiting Hot Jupiter and a Cold Massive Giant Planet around a Sun-like Star», The Astronomical Journal, 156 (5): 216, arXiv:1805.05925 , doi:10.3847/1538-3881/aade54 
  18. ↑ a b c d e f g h i j Hartman, J. D.; Bakos, G. Á.; Bayliss, D.; Bento, J.; Bhatti, W.; Brahm, R.; Csubry, Z.; Espinoza, N.; Henning, Th.; Jordán, A.; Mancini, L.; Penev, K.; Rabus, M.; Sarkis, P.; Suc, V.; Val-Borro, M. de; Zhou, G.; Addison, B.; Arriagada, P.; Butler, R. P.; Crane, J.; Durkan, S.; Shectman, S.; Tan, T. G.; Thompson, I.; Tinney, C. G.; Wright, D. J.; Lázár, J.; Papp, I.; Sári, P. (2018), «HATS-60b–HATS-69b: 10 Transiting Planets from HATSouth», The Astronomical Journal, 157 (2): 55, arXiv:1809.01048 , doi:10.3847/1538-3881/aaf8b6 
  19. ↑ HATS-70b: A 13 Mjup brown dwarf transiting an A star, 2018, arXiv:1811.06925  
  20. ↑ A Jovian planet in an eccentric 11.5 day orbit around HD1397 discovered by TESS, 2018, arXiv:1811.01882  
  21. ↑ HD 1397b: a transiting warm giant planet orbiting a V = 7.8 mag sub-giant star discovered by TESS, 2018, arXiv:1811.02156  
  22. ↑ HD2685 b: A Hot-Jupiter orbiting an early F-type star detected by TESS, 2018, arXiv:1811.05518  
  23. ↑ a b c d e f g h i j k Luhn, Jacob K.; Bastien, Fabienne A.; Wright, Jason T.; Johnson, John A.; Howard, Andrew W.; Isaacson, Howard (2018), «Retired a Stars and Their Companions. VIII. 15 New Planetary Signals around Subgiants and Transit Parameters for California Planet Search Planets with Subgiant Hosts», The Astronomical Journal, 157 (4): 149, arXiv:1811.03043 , doi:10.3847/1538-3881/aaf5d0 
  24. ↑ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al am an ao ap aq Livingston, John H.; et al. (2018). «Sixty Validated Planets from K2 Campaigns 5–8». The Astronomical Journal. 156 (6): 277. Bibcode:2018AJ....156..277L. arXiv:1810.04074 . doi:10.3847/1538-3881/aae778 
  25. ↑ a b Barros, S. C. C.; et al. (2022), «HD 23472: A multi-planetary system with three super-Earths and two potential super-Mercuries», Astronomy & Astrophysics, 665: A154, Bibcode:2022A&A...665A.154B, arXiv:2209.13345 , doi:10.1051/0004-6361/202244293 
  26. ↑ a b c d e f g h Ment, Kristo; Fischer, Debra A.; Bakos, Gaspar; Howard, Andrew W.; Isaacson, Howard (2018), «Radial Velocities from the N2K Project: Six New Cold Gas Giant Planets Orbiting HD 55696, HD 98736, HD 148164, HD 203473, and HD 211810», The Astronomical Journal, 156 (5): 213, arXiv:1809.01228 , doi:10.3847/1538-3881/aae1f5 
  27. ↑ Yu, Liang; Rodriguez, Joseph E.; Eastman, Jason D.; Crossfield, Ian J. M.; Shporer, Avi; Gaudi, B. Scott; Burt, Jennifer; Fulton, Benjamin J.; Sinukoff, Evan; Howard, Andrew W.; Isaacson, Howard; Kosiarek, Molly R.; Ciardi, David R.; Schlieder, Joshua E.; Penev, Kaloyan; Vanderburg, Andrew; Stassun, Keivan G.; Bieryla, Allyson; Butler, R. Paul; Berlind, Perry; Calkins, Michael L.; Esquerdo, Gilbert A.; Latham, David W.; Murawski, Gabriel; Stevens, Daniel J.; Petigura, Erik A.; Kreidberg, Laura; Bristow, Makennah (2018), «Two Warm, Low-density Sub-Jovian Planets Orbiting Bright Stars in K2 Campaigns 13 and 14», The Astronomical Journal, 156 (3): 127, arXiv:1803.02858 , doi:10.3847/1538-3881/aad6e7 
  28. ↑ Van Eylen, V.; et al. (2018), «HD 89345: A bright oscillating star hosting a transiting warm Saturn-sized planet observed by K2», Monthly Notices of the Royal Astronomical Society, 478 (4): 4866–4880, arXiv:1805.01860 , doi:10.1093/mnras/sty1390 
  29. ↑ Bang, Tae-Yang; Lee, Byeong-Cheol; Jeong, Gwang-Hui; Han, Inwoo; Park, Myeong-Gu (2018), «Search for Exoplanets Around Northern Circumpolar Stars III. Long-Period Radial Velocity Variations in Hd 18438 and Hd 158996», Journal of the Korean Astronomical Society, 51 (1), arXiv:1803.07213 , doi:10.5303/JKAS.2018.51.1.17 
  30. ↑ The CARMENES search for exoplanets around M dwarfs A Neptune-mass planet traversing the habitable zone around HD 180617, 2018, arXiv:1808.01183  
  31. ↑ HD 202772A B: A Transiting Hot Jupiter Around A Bright, Mildly Evolved Star In A Visual Binary Discovered By Tess, 2018, arXiv:1810.02341  
  32. ↑ a b Delisle, J.-B.; Ségransan, D.; Dumusque, X.; Diaz, R. F.; Bouchy, F.; Lovis, C.; Pepe, F.; Udry, S.; Alonso, R.; Benz, W.; Coffinet, A.; Collier Cameron, A.; Deleuil, M.; Figueira, P.; Gillon, M.; Lo Curto, G.; Mayor, M.; Mordasini, C.; Motalebi, F.; Moutou, C.; Pollacco, D.; Pompei, E.; Queloz, D.; Santos, N. C.; Wyttenbach, A. (2018), «The HARPS search for southern extra-solar planets», Astronomy & Astrophysics, 614: A133, arXiv:1802.04631 , doi:10.1051/0004-6361/201732529 
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  35. ↑ a b The GAPS Programme with HARPS-N at TNG XVIII. Two new giant planets around the metal-poor stars HD 220197 and HD 233832, 2018, arXiv:1811.07776  
  36. ↑ a b Adamów, M.; Niedzielski, A.; Kowalik, K.; Villaver, E.; Wolszczan, A.; MacIejewski, G.; Gromadzki, M. (2018), «Tracking Advanced Planetary Systems (TAPAS) with HARPS-N», Astronomy & Astrophysics, 613: A47, arXiv:1801.04379 , doi:10.1051/0004-6361/201732161 
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  40. ↑ Malavolta, Luca; et al. (2018). «An Ultra-short Period Rocky Super-Earth with a Secondary Eclipse and a Neptune-like Companion around K2-141». The Astronomical Journal. 155 (3). 107. Bibcode:2018AJ....155..107M. arXiv:1801.03502 . doi:10.3847/1538-3881/aaa5b5 
  41. ↑ a b c Diez Alonso, E.; Suarez Gomez, S. L.; Gonzalez Hernandez, J. I.; Suarez Mascareno, A.; Gonzalez Gutierrez, C.; Velasco, S.; Toledo Padron, B.; de Cos Juez, F. J.; Rebolo, R. (2018), A system of three transiting super-Earths in a cool dwarf star, arXiv:1801.06249  
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  73. ↑ Brady, Madison T.; Petigura, Erik A.; Knutson, Heather A.; Sinukoff, Evan; Isaacson, Howard; Hirsch, Lea A.; Fulton, Benjamin J.; Kosiarek, Molly R.; Howard, Andrew W. (2018), «Kepler-1656b: A Dense Sub-Saturn with an Extreme Eccentricity», The Astronomical Journal, 156 (4): 147, arXiv:1809.08436 , doi:10.3847/1538-3881/aad773 
  74. ↑ Hébrard, G.; Bonomo, A. S.; Díaz, R. F.; Santerne, A.; Santos, N. C.; Almenara, J.-M.; Barros, S. C. C.; Boisse, I.; Bouchy, F.; Bruno, G.; Courcol, B.; Deleuil, M.; Demangeon, O.; Guillot, T.; Montagnier, G.; Moutou, C.; Rey, J.; Wilson, P. A. (2019), «SOPHIE velocimetry of Keplertransit candidates», Astronomy & Astrophysics, 623: A104, arXiv:1811.09580 , doi:10.1051/0004-6361/201834333 
  75. ↑ Zang, Weicheng; Hwang, Kyu-Ha; Kim, Hyoun-Woo; Gould, Andrew; Wang, Tianshu; Zhu, Wei; Mao, Shude; Albrow, Michael D.; Chung, Sun-Ju; Han, Cheongho; Jung, Youn Kil; Ryu, Yoon-Hyun; Shin, In-Gu; Shvartzvald, Yossi; Yee, Jennifer C.; Cha, Sang-Mok; Kim, Dong-Jin; Kim, Seung-Lee; Lee, Chung-Uk; Lee, Dong-Joo; Lee, Yongseok; Park, Byeong-Gon; Pogge, Richard W. (2018), «KMT-2016-BLG-1397b: KMTNET-only Discovery of a Microlens Giant Planet», The Astronomical Journal, 156 (5): 236, arXiv:1810.10792 , doi:10.3847/1538-3881/aae537 
  76. ↑ a b Jung, Youn Kil; Hwang, Kyu-Ha; Ryu, Yoon-Hyun; Gould, Andrew; Han, Cheongho; Yee, Jennifer C.; Albrow, Michael D.; Chung, Sun-Ju; Shin, In-Gu; Shvartzvald, Yossi; Zang, Weicheng; Cha, Sang-Mok; Kim, Dong-Jin; Kim, Hyoun-Woo; Kim, Seung-Lee; Lee, Chung-Uk; Lee, Dong-Joo; Lee, Yongseok; Park, Byeong-Gon; Pogge, Richard W. (2018), «KMT-2016-BLG-1820 and KMT-2016-BLG-2142: Two Microlensing Binaries Composed of Planetary-mass Companions and Very-low-mass Primaries», The Astronomical Journal, 156 (5): 208, arXiv:1805.09983 , doi:10.3847/1538-3881/aae319 
  77. ↑ Burdanov, Artem; Benni, Paul; Sokov, Eugene; Krushinsky, Vadim; Popov, Alexander; Delrez, Laetitia; Gillon, Michael; Hébrard, Guillaume; Deleuil, Magali; Wilson, Paul A.; Demangeon, Olivier; Baştürk, Özgür; Pakštiene, Erika; Sokova, Iraida; Rusov, Sergei A.; Dyachenko, Vladimir V.; Rastegaev, Denis A.; Beskakotov, Anatoliy; Marchini, Alessandro; Bretton, Marc; Shadick, Stan; Ivanov, Kirill (2018), «KPS-1b: The First Transiting Exoplanet Discovered Using an Amateur Astronomer's Wide-field CCD Data», Publications of the Astronomical Society of the Pacific, 130 (989): 074401, arXiv:1804.05551 , doi:10.1088/1538-3873/aabde2 
  78. ↑ Kristo Ment, Jason A. Dittmann, Nicola Astudillo-Defru, David Charbonneau, Jonathan Irwin, Xavier Bonfils, Felipe Murgas, Jose-Manuel Almenara, Thierry Forveille, Eric Agol, Sarah Ballard, Zachory K. Berta-Thompson, Franc¸ois Bouchy, Ryan Cloutier, Xavier Delfosse, Rene Doyon, Courtney D. Dressing, Gilbert A. Esquerdo, Raphaelle D. Haywood, David M. Kipping, David W. Latham, Christophe Lovis, Elisabeth R. Newton, Francesco Pepe, Joseph E. Rodriguez, Nuno C. Santos, Thiam-Guan Tan, Stephane Udry, Jennifer G. Winters, and Anael Wunsche (3 de agosto de 2018). «A Second Terrestrial Planet Orbiting the Nearby M Dwarf LHS 1140». The Astronomical Journal. 157: 32. arXiv:1808.00485 . doi:10.3847/1538-3881/aaf1b1 
  79. ↑ A Planetary Microlensing Event with an Unusually Red Source Star: MOA-2011-BLG-291
  80. ↑ Miyazaki, S.; et al. (24 de julho de 2018). «MOA-2015-BLG-337: A Planetary System with a Low-mass Brown Dwarf/Planetary Boundary Host, or a Brown Dwarf Binary». The Astronomical Journal. 156 (3). 136 páginas. Bibcode:2018AJ....156..136M. arXiv:1804.00830 . doi:10.3847/1538-3881/aad5ee 
  81. ↑ Han, Cheongho; et al. (2018), «MOA-2016-BLG-319Lb: Microlensing Planet Subject to Rare Minor-image Perturbation Degeneracy in Determining Planet Parameters», The Astronomical Journal, 156 (5): 226, arXiv:1809.07898 , doi:10.3847/1538-3881/aae38e 
  82. ↑ Raynard, Liam; et al. (2018), «NGTS-2b: An inflated hot-Jupiter transiting a bright F-dwarf», Monthly Notices of the Royal Astronomical Society, 481 (4): 4960–4970, arXiv:1805.10449 , doi:10.1093/mnras/sty2581 
  83. ↑ Anderson, D. R.; Bouchy, F.; Brown, D. J. A.; Burdanov, A.; Collier Cameron, A.; Delrez, L.; Gillon, M.; Hellier, C.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Nielsen, L. D.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, B.; Temple, L. Y.; Triaud, A. H. M. J.; Udry, S.; West, R. G. (2018), A low-density hot Jupiter in a near-aligned, 4.5-day orbit around a V = 10.8, F5V star, arXiv:1809.07709  
  84. ↑ Günther, Maximilian N.; Queloz, Didier; Gillen, Edward; Delrez, Laetitia; Bouchy, Francois; McCormac, James; Smalley, Barry; Almleaky, Yaseen; Armstrong, David J. (21 de agosto de 2018). «Unmasking the hidden NGTS-3Ab: a hot Jupiter in an unresolved binary system». Monthly Notices of the Royal Astronomical Society. 478 (4): 4720–4737. Bibcode:2018MNRAS.478.4720G. ISSN 0035-8711. arXiv:1805.01378 . doi:10.1093/mnras/sty1193 
  85. ↑ West, Richard G.; et al. (2018), «NGTS-4b: A sub-Neptune transiting in the desert», Monthly Notices of the Royal Astronomical Society, 486 (4): 5094–5103, arXiv:1809.00678 , doi:10.1093/mnras/stz1084 
  86. ↑ Poleski, Radosław; Gaudi, B. S.; Udalski, A.; Szymański, M. K.; Soszyński, I.; Pietrukowicz, P.; Kozłowski, S.; Skowron, J.; Wyrzykowski, Ł.; Ulaczyk, K. (2018), «An Ice Giant Exoplanet Interpretation of the Anomaly in Microlensing Event OGLE-2011-BLG-0173», The Astronomical Journal, 156 (3): 104, arXiv:1805.00049 , doi:10.3847/1538-3881/aad45e 
  87. ↑ a b Suzuki, D.; et al. (2018), «A Likely Detection of a Two-planet System in a Low-magnification Microlensing Event», The Astronomical Journal, 155 (6): 263, arXiv:1803.05238 , doi:10.3847/1538-3881/aabd7a 
  88. ↑ OGLE-2015-BLG-1670Lb: A Cold Neptune beyond the Snow Line in the Provisional WFIRST Microlensing Survey Field, 2018, arXiv:1810.00014  
  89. ↑ Calchi Novati, S.; et al. (2018), «Spitzer Microlensing Parallax for OGLE-2016-BLG-1067: A Sub-Jupiter Orbiting an M Dwarf in the Disk», The Astronomical Journal, 157 (3): 121, arXiv:1801.05806 , doi:10.3847/1538-3881/ab0106 
  90. ↑ Skowron, J.; et al. (2018), «OGLE-2017-BLG-0373Lb: A Jovian Mass-Ratio Planet Exposes a New Accidental Microlensing Degeneracy», Acta Astronomica, 68 (1), arXiv:1802.10067 , doi:10.32023/0001-5237/68.1.2 
  91. ↑ Han, C.; et al. (2018), «OGLE-2017-BLG-0482Lb: A Microlensing Super-Earth Orbiting a Low-mass Host Star», The Astronomical Journal, 155 (5): 211, arXiv:1803.10830 , doi:10.3847/1538-3881/aabad2 
  92. ↑ Novati, S. Calchi; et al. (2018), «Spitzer Opens New Path to Break Classic Degeneracy for Jupiter-mass Microlensing Planet OGLE-2017-BLG-1140Lb», The Astronomical Journal, 155 (6): 261, arXiv:1803.04437 , doi:10.3847/1538-3881/aac21c 
  93. ↑ Jung, Y. K; Udalski, A; Gould, A; Ryu, Y.-H; Yee, J. C; Han, C; Albrow, M. D; Lee, C.-U; Kim, S.-L; Hwang, K.-H; Chung, S.-J; Shin, I.-G; Zhu, W; Cha, S.-M; Kim, D.-J; Lee, Y; Park, B.-G; Lee, D.-J; Kim, H.-W; Pogge, R. W; Szymański, M. K; Mróz, P; Poleski, R; Skowron, J; Pietrukowicz, P; Soszyński, I; Kozłowski, S; Ulaczyk, K; Pawlak, M; Rybicki, K (2018). «OGLE-2017-BLG-1522: A Giant Planet around a Brown Dwarf Located in the Galactic Bulge». The Astronomical Journal. 155 (5). 219 páginas. Bibcode:2018AJ....155..219J. arXiv:1803.05095 . doi:10.3847/1538-3881/aabb51 
  94. ↑ Udalski, A.; et al. (2018). «OGLE-2017-BLG-1434Lb: Eighth q<1×10-4 Mass-Ratio Microlens Planet Confirms Turnover in Planet Mass-Ratio Function». Acta Astronomica. 68 (1): 1. Bibcode:2018AcA....68....1U. arXiv:1802.02582 . doi:10.32023/0001-5237/68.1.1 
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  96. ↑ Keppler, M; et al. (2018). «Discovery of a planetary-mass companion within the gap of the transition disk around PDS 70». Astronomy & Astrophysics. 617: A44. Bibcode:2018A&A...617A..44K. arXiv:1806.11568 . doi:10.1051/0004-6361/201832957 
  97. ↑ Huang, Chelsea Xu; et al. (2018). «TESS Discovery of a Transiting Super-Earth in the π Mensae System». The Astrophysical Journal Letters. 868 (2): L39. PMC 6662726 . PMID 31360431. arXiv:1809.05967 . doi:10.3847/2041-8213/aaef91 
  98. ↑ Qatar Exoplanet Survey: Qatar-7b -- A Very Hot Jupiter Orbiting a Metal Rich F-Star, 2018, arXiv:1812.05601  
  99. ↑ Nucita, A. A.; Licchelli, D.; De Paolis, F.; Ingrosso, G.; Strafella, F.; Katysheva, N.; Shugarov, S. (2018), «Discovery of a bright microlensing event with planetary features towards the Taurus region: A super-Earth planet», Monthly Notices of the Royal Astronomical Society, 476 (3): 2962–2967, arXiv:1802.06659 , doi:10.1093/mnras/sty448 
  100. ↑ Fukui, A.; et al. (2019), «Kojima-1Lb is a Mildly Cold Neptune around the Brightest Microlensing Host Star», The Astronomical Journal, 158 (5): 206, arXiv:1909.11802 , doi:10.3847/1538-3881/ab487f 
  101. ↑ Shvartzvald, Y.; Novati, S. Calchi; Gaudi, B. S.; Bryden, G.; Nataf, D. M.; Penny, M. T.; Beichman, C.; Henderson, C. B.; Jacklin, S.; Schlafly, E. F.; Huston, M. J. (2018), «UKIRT-2017-BLG-001Lb: A Giant Planet Detected through the Dust», The Astrophysical Journal, 857: L8, arXiv:1802.06795 , doi:10.3847/2041-8213/aab71b 
  102. ↑ a b c d e Anderson, D. R.; et al. (2018). «The discovery of WASP-134b, WASP-134c, WASP-137b, WASP-143b and WASP-146b: three hot Jupiters and a pair of warm Jupiters orbiting Solar-type stars». arXiv:1812.09264  [astro-ph.EP] 
  103. ↑ a b c d e f g h Hellier, Coel; et al. (2019). «New transiting hot Jupiters discovered by WASP-South, Euler/CORALIE, and TRAPPIST-South». Monthly Notices of the Royal Astronomical Society. 482: 1379–1391. arXiv:1803.02224 . doi:10.1093/mnras/sty2741 
  104. ↑ a b c d Lendl, M.; et al. (2019). «WASP-147b, 160Bb, 164b, and 165b: Two hot Saturns and two Jupiters, including two planets with metal-rich hosts». Monthly Notices of the Royal Astronomical Society. 482: 301–312. arXiv:1807.06973 . doi:10.1093/mnras/sty2667 
  105. ↑ a b c Barkaoui, K.; et al. (2018), «Discovery of Three New Transiting Hot Jupiters: WASP-161 b, WASP-163 b, and WASP-170 B», The Astronomical Journal, 157 (2): 43, arXiv:1807.06548 , doi:10.3847/1538-3881/aaf422 
  106. ↑ Wyttenbach, A.; West, R. G.; Udry, S.; Temple, L. Y.; Spake, J. J.; Smalley, B.; Ségransan, D.; Queloz, D.; Pollacco, D.; Pepe, F.; Maxted, P F L.; Nielsen, L. D.; Linder, E.; Lendl, M.; Jehin, E.; Gillon, M.; Ehrenreich, D.; Delrez, L.; Collier Cameron, A.; Burdanov, A.; Bouchy, F.; Triaud, A H M J.; Anderson, D. R.; Hellier, Coel (2018), «WASP-166b: A bloated super-Neptune transiting a V = 9 star», Monthly Notices of the Royal Astronomical Society, 488 (3): 3067–3075, arXiv:1811.05292 , doi:10.1093/mnras/stz1903 
  107. ↑ Seidel, J. V.; Cegla, H. M.; Doyle, L.; Lafarga, M.; Brogi, M.; Gandhi, S.; Anderson, D. R.; Allart, R.; Buchschacher, N.; Lovis, C.; Sosnowska, D. (2022), «The hot Neptune WASP-166 b with ESPRESSO II: Confirmation of atmospheric sodium», Monthly Notices of the Royal Astronomical Society: Letters, 513: L15–L19, arXiv:2203.04494 , doi:10.1093/mnrasl/slac027 
  108. ↑ Doyle, L.; Cegla, H. M.; Bryant, E.; Bayliss, D.; Lafarga, M.; Anderson, D. R.; Allart, R.; Bourrier, V.; Brogi, M.; Buchschacher, N.; Kunovac, V.; Lendl, M.; Lovis, C.; Moyano, M.; Roguet-Kern, N.; Seidel, J. V.; Sosnowska, D.; Wheatley, P. J.; Acton, J. S.; Burleigh, M. R.; Casewell, S. L.; Gill, S.; Goad, M. R.; Henderson, B. A.; Jenkins, J. S.; Tilbrook, R. H.; West, R. G. (2022), «The Hot Neptune WASP-166 b with ESPRESSO – I. Refining the planetary architecture and stellar variability», Monthly Notices of the Royal Astronomical Society, 516: 298–315, arXiv:2207.10127 , doi:10.1093/mnras/stac2178 
  109. ↑ Labadie-Bartz, Jonathan; et al. (2018), «KELT-22Ab: A Massive, Short-Period Hot Jupiter Transiting a Near-solar Twin», The Astrophysical Journal Supplement Series, 240: 13, arXiv:1803.07559 , doi:10.3847/1538-4365/aaee7e 
  110. ↑ Temple, L. Y.; Hellier, C.; Almleaky, Y.; Anderson, D. R.; Bouchy, F.; Brown, D J A.; Burdanov, A.; Cameron, Collier; Delrez, L.; Gillon, M.; Hall, R.; Jehin, E.; Lendl, M.; Maxted, P F L.; Nielsen, L. D.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, B.; Sohy, S.; Thompson, S.; Triaud, A H M J.; Turner, O. D.; Udry, S.; West, R. G. (2018), «Discovery of WASP-174b: Doppler tomography of a near-grazing transit», Monthly Notices of the Royal Astronomical Society, 480 (4): 5307–5313, arXiv:1802.00766 , doi:10.1093/mnras/sty2197 
  111. ↑ WASP-190b: Tomographic discovery of a transiting hot Jupiter, 2018, arXiv:1811.05742  
  112. ↑ Peterson, Merrin S.; et al. (2018). «A 2 R ⊕ Planet Orbiting the Bright Nearby K Dwarf Wolf 503». The Astronomical Journal. 156 (5): 188. Bibcode:2018AJ....156..188P. arXiv:1806.03494 . doi:10.3847/1538-3881/aaddfe 
  113. ↑ Polanski, Alex S.; et al. (2021). «Wolf 503 b: Characterization of a Sub-Neptune Orbiting a Metal-poor K Dwarf». The Astronomical Journal. 162 (6): 238. Bibcode:2021AJ....162..238P. arXiv:2107.08092 . doi:10.3847/1538-3881/ac1590 
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