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[editar | editar código-fonte]


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:1804.04008Acessível livremente. 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:1807.07098Acessível livremente. 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:1811.05955Acessível livremente. 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:1807.01229Acessível livremente, 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/aae64dAcessível livremente 
  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:1804.03476Acessível livremente. 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:1806.10958Acessível livremente, 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:1812.04501Acessível livremente, 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:1806.03870Acessível livremente, 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:1810.07572Acessível livremente, 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..255YAcessível livremente. arXiv:1805.09352Acessível livremente. doi:10.3847/1538-3881/aabfecAcessível livremente 
  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:1804.01623Acessível livremente, 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:1812.07668Acessível livremente, 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:2211.01044Acessível livremente, 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:1805.05925Acessível livremente, 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:1809.01048Acessível livremente, doi:10.3847/1538-3881/aaf8b6 
  19. ↑ HATS-70b: A 13 Mjup brown dwarf transiting an A star, 2018, arXiv:1811.06925Acessível livremente 
  20. ↑ A Jovian planet in an eccentric 11.5 day orbit around HD1397 discovered by TESS, 2018, arXiv:1811.01882Acessível livremente 
  21. ↑ HD 1397b: a transiting warm giant planet orbiting a V = 7.8 mag sub-giant star discovered by TESS, 2018, arXiv:1811.02156Acessível livremente 
  22. ↑ HD2685 b: A Hot-Jupiter orbiting an early F-type star detected by TESS, 2018, arXiv:1811.05518Acessível livremente 
  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:1811.03043Acessível livremente, 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:1810.04074Acessível livremente. 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:2209.13345Acessível livremente, 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:1809.01228Acessível livremente, 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:1803.02858Acessível livremente, 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:1805.01860Acessível livremente, 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:1803.07213Acessível livremente, 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:1808.01183Acessível livremente 
  31. ↑ HD 202772A B: A Transiting Hot Jupiter Around A Bright, Mildly Evolved Star In A Visual Binary Discovered By Tess, 2018, arXiv:1810.02341Acessível livremente 
  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:1802.04631Acessível livremente, doi:10.1051/0004-6361/201732529 
  33. ↑ Esposito, M.; Armstrong, D. J.; Gandolfi, D.; Adibekyan, V.; Fridlund, M.; Santos, N. C.; Livingston, J. H.; Mena, E. Delgado; Fossati, L.; Lillo-Box, J.; Barragán, O.; Barrado, D.; Cubillos, P. E.; Cooke, B.; Justesen, A. B. (1 de março de 2019). «HD 219666 b: a hot-Neptune from TESS Sector 1». Astronomy and Astrophysics. 623: A165. ISSN 0004-6361. doi:10.1051/0004-6361/201834853 
  34. ↑ «The Extrasolar Planet Encyclopaedia — HD 219666 b». exoplanet.eu. Consultado em 22 de janeiro de 2023 
  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:1811.07776Acessível livremente 
  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:1801.04379Acessível livremente, doi:10.1051/0004-6361/201732161 
  37. ↑ Leão, I. C.; Canto Martins, B. L.; Alves, S.; Pereira De Oliveira, G.; Cortés, C.; Brucalassi, A.; Melo, C. H. F.; De Freitas, D. B.; Pasquini, L.; De Medeiros, J. R. (2018), «Incidence of planet candidates in open clusters and a planet confirmation», Astronomy & Astrophysics, 620: A139, arXiv:1807.03196Acessível livremente, doi:10.1051/0004-6361/201833123 
  38. ↑ Delgado Mena, E.; Lovis, C.; Santos, N. C.; Gomes Da Silva, J.; Mortier, A.; Tsantaki, M.; Sousa, S. G.; Figueira, P.; Cunha, M. S.; Campante, T. L.; Adibekyan, V.; Faria, J. P.; Montalto, M. (2018), «Planets around evolved intermediate-mass stars», Astronomy & Astrophysics, 619: A2, arXiv:1807.09608Acessível livremente, doi:10.1051/0004-6361/201833152 
  39. ↑ a b c d e Christiansen, Jessie L.; Crossfield, Ian J. M.; Barentsen, Geert; Lintott, Chris J.; Barclay, Thomas; Simmons, Brooke D.; Petigura, Erik; Schlieder, Joshua E.; Dressing, Courtney D.; Vanderburg, Andrew; Ciardi, David R.; Allen, Campbell; McMaster, Adam; Miller, Grant; Veldthuis, Martin; Allen, Sarah; Wolfenbarger, Zach; Cox, Brian; Zemiro, Julia; Howard, Andrew W.; Livingston, John; Sinukoff, Evan; Catron, Timothy; Grey, Andrew; Kusch, Joshua J. E.; Terentev, Ivan; Vales, Martin; Kristiansen, Martti H. (11 de janeiro de 2018). «The K2-138 System: A Near-resonant Chain of Five Sub-Neptune Planets Discovered by Citizen Scientists». The Astronomical Journal (em inglês). 155 (2). 57 páginas. Bibcode:2018AJ....155...57C. ISSN 1538-3881. arXiv:1801.03874Acessível livremente. doi:10.3847/1538-3881/aa9be0 
  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:1801.03502Acessível livremente. 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:1801.06249Acessível livremente 
  42. ↑ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al am an ao ap aq ar as at au av aw ax ay az ba bb bc bd be bf bg bh bi bj bk bl bm bn bo bp bq br bs bt bu bv bw bx by bz ca cb cc cd ce cf cg ch ci cj ck cl cm cn co cp cq Mayo, Andrew W.; et al. (2018). «275 Candidates and 149 Validated Planets Orbiting Bright Stars inK2 Campaigns 0–10». The Astronomical Journal. 155 (3): 136. Bibcode:2018AJ....155..136M. arXiv:1802.05277Acessível livremente. doi:10.3847/1538-3881/aaadff 
  43. ↑ a b c d e f g Adams, Elisabeth R.; et al. (2020). «Ultra Short Period Planets in K2 III: Neighbors are Common with 13 New Multi-Planet Systems and 10 Newly Validated Planets in Campaigns 0-8, 10». The Planetary Science Journal. 2 (4): 152. Bibcode:2021PSJ.....2..152A. arXiv:2011.11698Acessível livremente. doi:10.3847/PSJ/ac0ea0 
  44. ↑ a b c d e f g h i j k l m n o p q r s t u v w x Livingston, John H.; et al. (2018), «44 Validated Planets from K2 Campaign 10», The Astronomical Journal, 156 (2): 78, arXiv:1806.11504Acessível livremente, doi:10.3847/1538-3881/aaccde 
  45. ↑ a b c Akana Murphy, Joseph M.; Kosiarek, Molly R.; Batalha, Natalie M.; Gonzales, Erica J.; Isaacson, Howard; Petigura, Erik A.; Weiss, Lauren M.; Grunblatt, Samuel K.; Ciardi, David R.; Fulton, Benjamin; Hirsch, Lea A.; Behmard, Aida; Rosenthal, Lee J. (2021), «Another Superdense Sub-Neptune in K2-182 b and Refined Mass Measurements for K2-199 b and C», The Astronomical Journal, 162 (6): 294, Bibcode:2021AJ....162..294A, arXiv:2110.05502Acessível livremente, doi:10.3847/1538-3881/ac2830 
  46. ↑ Nava, Chantanelle; et al. (2021), «K2-79b and K2-222b: Mass measurements of two small exoplanets with periods beyond 10 days that overlap with periodic magnetic activity signals», The Astronomical Journal, 163 (2): 41, Bibcode:2022AJ....163...41N, arXiv:2111.02608Acessível livremente, doi:10.3847/1538-3881/ac3141 
  47. ↑ Curtis, Jason Lee; Vanderburg, Andrew; Torres, Guillermo; Kraus, Adam L.; Huber, Daniel; Mann, Andrew W.; Rizzuto, Aaron C.; Isaacson, Howard; Howard, Andrew W.; Henze, Christopher E.; Fulton, Benjamin J.; Wright, Jason T. (2018), «K2-231 b: A Sub-Neptune Exoplanet Transiting a Solar Twin in Ruprecht 147», The Astronomical Journal, 155 (4): 173, arXiv:1803.07430Acessível livremente, doi:10.3847/1538-3881/aab49c 
  48. ↑ K2-232 b: a transiting warm Saturn on an eccentric P = 11.2  d orbit around a V = 9.9 star
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