List of exoplanets discovered in 2026
This list of exoplanets discovered in 2026 is a list of confirmed exoplanets that were first reported in 2026. For exoplanets detected only by radial velocity, the listed value for mass is a lower limit. See Minimum mass for more information. For exoplanets detected only by direct imaging or microlensing without a determined orbit, the listed value for semi-major axis is the projected separation.
| Name | Mass (MJ) | Radius (RJ) | Period (days) | Semi-major axis (AU) | Temp. (K) | Discovery method | Distance (ly) | Host star mass (M☉) | Host star temp. (K) | Remarks |
|---|---|---|---|---|---|---|---|---|---|---|
| Beta Pictoris d | 2.4±0.6 | 1.26±0.03 | 33200+6600 −9900 |
26.0+2.2 −6.1 |
600+45 −60 |
imaging | 63.4 ± 0.1 | 1.789+0.024 −0.027 |
8054±96 | [1][2] |
| DMPP-2c | 0.1629+0.0171 −0.0173 |
0.737 | 3.168+0.355 −0.002 |
0.04789+0.00327 −0.00049 |
radial vel. | 443±1[3] | 1.41±0.04 | 6500±100 | [4] | |
| DMPP-2d | 0.2888+0.0192 −0.0230 |
1.03 | 16.491+0.067 −0.053 |
0.1432+0.0012 −0.0013 |
radial vel. | [4] | ||||
| DMPP-6b | 0.0182+0.0030 −0.0025 |
0.203 | 7.6027+0.0261 −0.0016 |
0.00779+0.0016 −0.0012 |
radial vel. | 177.6±0.1[3] | 1.079±0.045 | 6182+139 −100[5] |
[4] | |
| DMPP-6c | 0.0424+0.0050 −0.0062 |
0.334 | 36.441+0.077 −0.070 |
0.2206+0.0033 −0.0039 |
radial vel. | [4] | ||||
| DMPP-7b | 0.1932+0.0136 −0.0128 |
0.815 | 4.984+0.069 −0.061 |
0.05873+0.00086 −0.00089 |
radial vel. | 333.6±0.6[3] | 1.09±0.04 | 5996+128 −87[5] |
[4] | |
| DMPP-8b | 0.2551±0.0223 | 0.96 | 62.915+0.041 −0.033 |
0.3098+0.0098 −0.0108 |
radial vel. | 248±0.5[3] | 0.99±0.04 | 6009+107 −147[5] |
[4] | |
| DMPP-9b | 0.0454+0.0081 −0.0074 |
0.347 | 12.733+0.584 −0.524 |
0.1097+0.0041 −0.0037 |
radial vel. | 359.1±0.6[3] | 1.10±0.04 | 6092+131 −134[5] |
[4] | |
| Gaia23braL b | 1.630+0.420 −0.378 |
4.847+0.770 −0.808 |
microlensing | 14123+3271 −3300 |
0.774+0.170 −0.146 |
[6] | ||||
| GJ 48 b | 0.0255±0.0051 | 39.6299±0.2900 | 0.1752±0.0011 | 271 | radial vel. | 26.8613±0.0076 | 0.470±0.010 | 3450±50 | [7] | |
| GJ 523 b | 0.0739±0.0104 | 0.2275±0.0134 | 17.745740±0.000045 | 0.1226±0.0015 | 538±13 | transit | 86.8±0.03[3] | 0.781±0.029 | 4660±50 | [8] |
| GJ 887 d | 0.0192±0.0044 | 0.209 | 50.77±0.05 | 0.212+0.007 −0.008 |
241+10 −9 |
radial vel. | 10.7241 ± 0.0007 | 0.495±0.049 | 3688±86 | A super-Earth located in the habitable zone[9] |
| GJ 887 e | 0.0046±0.0006 | 0.102 | 4.4249±0.0001 | 0.0417+0.0014 −0.0015 |
544+21 −20 |
radial vel. | 10.7241 ± 0.0007 | 0.495±0.049 | 3688±86 | [9] |
| GJ 1137 c | 0.0161±0.0022 | 9.6412+0.0012 −0.0011 |
0.0835±0.0008 | radial vel. | 92.91 ± 0.06 | 0.836+0.023 −0.025 |
5033.8+85.7 −77.2 |
[10] | ||
| GJ 3090 c | 0.031±0.004 | 0.28 | 15.9407±0.0058 | 0.0997±0.0008 | 407.2±7.4 | radial vel. | 73.24 | 0.519±0.013 | 3707±32 | [11] |
| GJ 3378 b | 0.0072±0.0013 | 21.45±0.01 | 0.09673±0.00080 | 272±7 | radial vel. | 25.225 ± 0.006 | 0.262±0.021 | 3340±60 | [12] | |
| GJ 4274 b | 0.0093+0.0017 −0.0016 |
0.1394 | 1.6339±0.0001 | 0.0153±0.0008 | radial vel. | 23.60 ± 0.04 | 0.18±0.03 | 3,228±19 | [13] | |
| GJ 4274 c | 0.0264+0.0053 −0.0049 |
0.252 | 69.57+0.32 −1.14 |
0.186±0.010 | radial vel. | 23.60 ± 0.04 | 0.18±0.03 | 3,228±19 | [13] | |
| HD 48265 c | 4.45+0.75 −0.37 |
1.15 | 10418+2451 −1412 |
10.4+1.6 −1.0 |
astrometry + radial vel. | 296.3 ± 0.4 | 1.38±0.06 | 5805±34 | [14] | |
| HD 50554 c | 0.01148±0.00425 | 0.117±0.005 | 5.969362 | 0.066+0.009 −0.018 |
transit | 101.34 ± 0.08 | 1.04±0.05 | 5,968±96 | [15] | |
| HD 50554 d | 0.0211±0.0116 | 0.126+0.013 −0.008 |
28.06940 | 0.168+0.028 −0.065 |
transit | 101.34 ± 0.08 | 1.04±0.05 | 5,968±96 | [15] | |
| HD 60779 b | 0.04465+0.00305 −0.00302 |
0.2896+0.0089 −0.0087 |
29.986175+0.000030 −0.000033 |
0.1922±0.0038 | 650±10 | transit | 115.596+0.1523 −0.1519 |
1.050±0.044 | 6081±60 | [16] |
| HD 60779 c | 0.0890±0.0047 | 104.79±0.23 | radial vel. | 115.596+0.1523 −0.1519 |
1.050±0.044 | 6081±60 | [16] | |||
| HD 68475 b | 5.16+0.53 −0.47 |
1.15 | 7832+463 −323 |
7.27+0.39 −0.36 |
astrometry + radial vel. | 108.7 | 0.83±0.10 | 5022±113 | [14] | |
| HD 100508 b | 1.20+0.30 −0.18 |
1.22 | 5681±42 | 6.11+0.25 −0.28 |
astrometry + radial vel. | 106.9 | 0.94±0.12 | 5419±112 | [14] | |
| HD 114386 c | 0.37±0.03 | 1.2 | 444.00+0.93 −0.88 |
1.05±0.04 | radial vel. | 91.26 | 0.80±0.03 | 4895±62 | [14] | |
| HD 164604 c | 9.5±1.2 or[a] 7.6±1.0 | 1.12 | 5387+120 −127 |
5.556+0.093 −0.100 |
astrometry + radial vel. | 128.5 | 0.77±0.02 | 4663±31 | [17] | |
| HD 176986 d | 0.0213±0.0029 | 0.222 | 61.376+0.051 −0.049 |
0.28149±0.0024 | 363±10 | radial vel. | 90.93 | 0.789±0.019 | 4931±77 | [18] |
| HIP 8923 b | 9.98+0.78 −0.16 |
5160+150 −240 |
5.90+0.10 −0.22 |
radial vel. | 215 | 1.01±0.04 | 5980±51 | [19] | ||
| HIP 10090 b | 3.87+0.65 −0.60 |
2960+120 −100 |
3.87+0.19 −0.11 |
radial vel. | 268 | 0.94±0.04 | 5661±72 | Also known as HD 13350 b.[19] | ||
| HIP 10090 c | 0.85+0.03 −0.12 |
321.8+0.3 −0.6 |
0.90±0.01 | radial vel. | Also known as HD 13350 c.[19] | |||||
| HIP 39330 b | 1.67+0.19 −0.08 |
4650+210 −250 |
5.05+0.23 −0.17 |
radial vel. | 119 | 0.96±0.04 | 5748±81 | [19] | ||
| HIP 98599 b | 6.85+0.10 −0.22 |
2656+40 −16 |
3.96+0.07 −0.01 |
radial vel. | 248 | 1.19±0.04 | 5978±300 | [19] | ||
| Kepler-247e | 0.208 | 31.1016590 | TTV | 2205 | 0.840+0.038 −0.042 |
5130+63 −80 |
[20] | |||
| KMT-2016-BLG-1337Lb | 0.54±0.30 | 1.01 | 3945 | 3.97+0.60 −0.92 |
microlensing | 22570+3392 −5251 |
0.54±0.30 0.40±0.22 |
A circumbinary planet.[21] | ||
| KMT-2020-BLG-0202Lb | 12.28+7.37 −5.43 |
1.1 | 3470 | 4.17+1.29 −1.28 |
microlensing | 12518+3879 −3847 |
0.81+0.49 −0.36 |
[22] | ||
| KMT-2021-BLG-0852Lb | 0.49±0.17 | 7.78+0.89 −1.11 |
microlensing | 23581+2707 −3359 |
0.75+0.26 −0.27 |
[23] | ||||
| KMT-2022-BLG-1551Lb | 2.96+1.71 −1.53 |
1.17 | 1717 | 2.29+0.30 −0.44 |
microlensing | 22494+2999 −4336 |
0.54+0.31 −0.28 |
[22] | ||
| KMT-2022-BLG-1818Lb | 4.00+1.24 −2.00 |
2.6±0.9 | microlensing | 17,286 ± 6,197 | 0.30+0.12 −0.06 |
[24] | ||||
| KMT-2022-BLG-1818Lc | 0.36+0.30 −0.21 |
12.6+6.0 −4.7 |
microlensing | 17,286 ± 6,197 | 0.30+0.12 −0.06 |
[24] | ||||
| KMT-2023-BLG-0164Lb | 0.047+0.026 −0.019 |
1.33+0.39 −0.25 |
microlensing | 3390+1663 −880 |
0.32+0.21 −0.13 |
[25] | ||||
| KMT-2023-BLG-0466Lb | 3.25+2.59 −2.03 |
1.17 | 2411 | 2.68+0.45 −0.63 |
microlensing | 22168+3716 −5216 |
0.44+0.36 −0.27 |
[22] | ||
| KMT-2023-BLG-1286Lb | 0.062+0.058 −0.035 |
2.02±0.60 | microlensing | 20049+3227 −4401 |
0.31+0.29 −0.18 |
[25] | ||||
| KMT-2023-BLG-1592Lb | 0.57+0.37 −0.29 |
2.1±0.6 | microlensing | 22820+3586 −7172 |
0.59+0.33 −0.29 |
[26] | ||||
| KMT-2023-BLG-1746Lb | 0.0070+0.0048 −0.0021 |
1.06+0.55 −0.17 |
microlensing | 25363±3064 | 0.11+0.08 −0.03 |
[25] | ||||
| KMT-2024-BLG-0792L | 0.219+0.075 −0.046 |
microlensing | 9948+1892 −1402 |
candidate rogue planet[27] | ||||||
| KMT-2024-BLG-2005Lb | 0.16+0.24 −0.09 |
1.12+0.15 −0.15 |
microlensing | 25179+3262 −3457 |
0.12+0.17 −0.06 |
[23] | ||||
| KMT-2024-BLG-3237L | 0.212+0.325 −0.134 |
microlensing | 23940+3131 −6882 |
candidate rogue planet[28] | ||||||
| KMT-2025-BLG-0121Lb | 7.77+4.08 −4.04 |
1.13 | 2484 | 3.05+0.46 −0.66 |
microlensing | 20212+3032 −4400 |
0.61±0.32 | [22] | ||
| KMT-2025-BLG-0481Lb | 0.59+0.85 −0.34 |
2.18+0.31 −0.39 |
microlensing | 26027+3686 −4697 |
0.22+0.31 −0.13 |
[23] | ||||
| KMT-2025-BLG-0811Lb | 0.02199±0.01466 | 2.47±0.57 | microlensing | 22799+2772 −3457 |
0.49+0.32 −0.23 |
[29] | ||||
| KMT-2025-BLG-1616Lb | 0.1332+0.1278 −0.0694 |
1.6+0.2 −0.3 |
microlensing | 24462+2283 −3262 |
0.26+0.25 −0.14 |
[30] | ||||
| KOINTREAU-1 b | 10.6+2.5 −2.3 |
690±10 | imaging | 517.27+13.79 −13.11 |
0.26±0.03 | 3551±59 | [31] | |||
| KOINTREAU-3b | 3.4±0.7 | 1.17 | 3609839 | 342±4 | imaging | 450 | 3920±70 | [31] | ||
| KOINTREAU-4b | 11.5+1.2 −1.6 or[b] 14.8+1.2 −0.9 |
1.09 | 182±2 | imaging | 463 | [31] | ||||
| LHS 1903 b | 0.01032±0.0013 | 0.1233±0.0041 | 2.1555098+0.0000026 −0.0000029 |
0.02656+0.00055 −0.00058 |
796±20 | transit | 116.3 ± 0.1 | 0.538+0.039 −0.030 |
3664±70 | [32] |
| LHS 1903 c | 0.01432+0.0023 −0.0022 |
0.1825+0.0070 −0.0066 |
6.226185+0.000028 −0.000026 |
0.05387+0.00112 −0.00117 |
559±14 | transit | 116.3 ± 0.1 | 0.538+0.039 −0.030 |
3664±70 | [32] |
| LHS 1903 d | 0.01875±0.0036 | 0.2230+0.0070 −0.0069 |
12.566287+0.000032 −0.000028 |
0.08604+0.00178 −0.00186 |
442±11 | transit | 116.3 ± 0.1 | 0.538+0.039 −0.030 |
3664±70 | [32] |
| LHS 1903 e | 0.01822+0.0050 −0.0051 |
0.1545+0.0053 −0.0052 |
29.31773+0.00028 −0.00025 |
0.15135+0.00314 −0.00338 |
333+9 −8 |
transit | 116.3 ± 0.1 | 0.538+0.039 −0.030 |
3664±70 | [32] |
| OGLE-2023-BLG-0766Lb | 1.20+0.86 −0.60 |
2.2±0.5 | microlensing | 23798+2934 −3586 |
0.45+0.32 −0.22 |
[26] | ||||
| NGTS-38 b | 4.78+0.40 −0.37 |
1.081±0.047 | 180.52797±0.00036 | 0.697±0.035 | 457±11 | transit | 864 | 1.46±0.09 | 6310±129 | Planet also known as TIC 65910228 b[33] |
| NGTS-39 b | 1.467±0.081 | 1.088±0.012 | 58.204720+0.000042 −0.000038 |
0.3077±0.0055 | 519+6 −5 |
transit | 907.941+12.988 −12.629 |
1.16±0.05 | 6053+67 −30 |
[34] |
| TIC 77319217 b | 0.27737 | 7.5483 | transit | 868.7 | 1.18±0.05 | 6126±128 | [35] | |||
| TIC 86380416 b | 0.21519 | 6.0409 | transit | 810.2 | 1.07±0.144 | 5889±138.4 | [35] | |||
| TIC 87422071 b | 1.29+0.10 −0.11 |
0.969+0.087 −0.084 |
11.364929 | 0.106±0.005 | 1,110±33 | transit | 1302 | 1.239+0.070 −0.080 |
6150±178 | Star also known as TOI-6752.[36] |
| TIC 117642575 b | 0.25221 | 4.9446 | transit | 615.9 | 1.06±0.13 | 5862±133 | [35] | |||
| TIC 139702105 b | 0.21884 | 6.836 | transit | 301.2 | 0.9±0.11 | 5265±121 | [35] | |||
| TIC 147027702 b | 1.09+0.07 −0.13 |
0.975+0.065 −0.064 |
44.40523 | 0.274+0.014 −0.013 |
863+26 −27 |
transit | 1490 | 1.406+0.074 −0.086 |
6410±183 | [36] |
| TIC 161045582 b | 0.20038 | 8.8558 | transit | 527.9 | 1.04±0.128 | 5806±109.5 | [35] | |||
| TIC 178172313 b | 0.25016 | 4.3732 | transit | 587.6 | 0.91±0.11 | 5300±132 | [35] | |||
| TIC 198190129 b | 0.26077 | 7.948 | transit | 452.4 | 0.638±0.08 | 4075±118 | [35] | |||
| TIC 245076932 b | 0.51+0.04 −0.05 |
0.970±0.048 | 21.613890 | 0.157±0.007 | 845±25 | transit | 1026 | 1.117±0.063 | 6130±178 | [36] |
| TIC 260969020 b | 0.19868 | 8.4858 | transit | 394.2 | 0.75±0.085 | 4685±128 | [35] | |||
| TIC 294329732 b | 0.1853 | 9.7566 | transit | 616.6 | 0.89±0.11 | 5215±119 | [35] | |||
| TIC 423703298 b | 0.2473 | 4.0371 | transit | 442.8 | 0.691±0.08 | 4415±130 | [35] | |||
| TIC 437041147 b | 0.19761 | 3.823 | transit | 812.3 | 0.913±0.11 | 5374±122 | [35] | |||
| TOI-237 c | 0.1076±0.0031 | 1.74486147 | 0.0160+0.0005 −0.0006 |
515+11 −8 |
transit | 124.86 | 0.1698+0.0385 −0.0350 |
3226+47 −48 |
[37] | |
| TOI-791 b | 0.02989++0.00516 −0.00569 |
0.9930±0.0330 | 139.29931++0.00011 −0.00012 |
0.602±0.022 | 434.3±9.7 | transit | 1,097 ± 5 | 1.28±0.08 | 6294±128 | [38] |
| TOI-791 c | 0.05852+0.00705 −0.00658 |
1.155±0.040 | 232.01570+0.00067 −0.00071 |
0.863±0.032 | 362.8±8.2 | transit | 1,097 ± 5 | 1.28±0.08 | 6294±128 | [38] |
| TOI-883 b | 0.123±0.012 | 0.604±0.028 | 10.057716 | 0.0898±0.0023 | 1,086±19 | transit | 336 | 0.956+0.054 −0.051 |
5697±80 | [39] |
| TOI-899 b | 0.213±0.024 | 0.991±0.044 | 12.846185 | 0.1063±0.0026 | 1,040±19 | transit | 1004 | 0.972+0.054 −0.053 |
5696±80 | [39] |
| TOI-1080 b | 0.0055+0.0039 −0.0018[c] |
0.1071±0.0052 | 3.9652482 | 0.0272+0.0015 −0.0016 |
368+12 −10 |
transit | 83.36 | 0.1667±0.0041 | 3065±50 | [40] |
| TOI-1232 b | 0.964±0.06 | 0.975±0.05 | 14.256±0.001 | 0.117±0.001 | transit | 1071.883+7.774 −7.666 |
1.05±0.133 | 5818±134.1 | [41] | |
| TOI-1232 c | 0.18±0.02 | 30.356±0.01 | 0.194±0.002 | radial vel. | 1071.883+7.774 −7.666 |
1.05±0.133 | 5818±134.1 | [41] | ||
| TOI-1243 b | 0.0242±0.0047 | 0.2079±0.0107 | 4.65948 | 0.0437±0.0001 | 450 | transit | 140.6 | 0.515±0.027 | 3515±79 | [42] |
| TOI-1533 b | 0.0884+0.0104 −0.0107 |
0.258±0.005 | 3.6457974±0.0000034 | 0.0445±0.0008 | transit | 326.32+0.98 −0.97 |
0.88±0.04 | 5146±81 | [43] | |
| TOI-1533 c | 0.115+0.013 −0.012 |
>0.67 | 8.0637926±0.0000052 | 0.076±0.002 | transit | 326.32+0.98 −0.97 |
0.88±0.04 | 5146±81 | [43] | |
| TOI-1752 b | 0.01284±0.0057 | 0.1508±0.0062 | 0.9351861+0.0000014 −0.0000015 |
0.01624±0.00056 | 1036±31 | transit | 336.009+1.096 −1.094 |
0.524±0.012 | 3762±77 | [44] |
| TOI-1752 c | 0.0164±0.0069 | 0.1160±0.0125 | 32.71443+0.00041 −0.00035 |
0.1614±0.0069 | 291±17 | transit | 336.009+1.096 −1.094 |
0.524±0.012 | 3762±77 | [44] |
| TOI-2040 b | 0.781±0.036 | 0.921±0.023 | 3.8608576+0.0000045 −0.0000044 |
0.04730±0.00150 | 1070±29 | transit | 472.01+1.61 −1.60 |
0.92±0.03 | 5132±129 | [45] |
| TOI-2049 b | 1.53±0.18 | 1.485+0.071 −0.067 |
5.303468+0.000050 −0.000048 |
0.06919±0.00052 | 1869±128 | transit | 1863.96+29.92 −29.01 |
1.57±0.03 | 6164±202 | [45] |
| TOI-2133 b | 0.026+0.010 −0.008[c] |
0.211±0.008 | 3.8266472 | 0.0410±0.0015 | 798±12 | transit | 245.3 | 0.644±0.019 | 4250±45 | [46] |
| TOI-2147 b | 0.365±0.069 | 0.937±0.027 | 26.20518±0.00003 | 0.172±0.006 | 820±20 | transit | 920.112+8.278 −8.134 |
0.990±0.040 | 5983±50 | [47] |
| TOI-2578 b | 0.526+0.071 −0.068 |
1.754+0.058 −0.057 |
3.4579667±0.0000033 | 0.0495+0.0022 −0.0021 |
1778+75 −74 |
transit | 931.17+11.47 −11.20 |
1.27±0.09 | 6333±244 | [45] |
| TOI-3862 b | 0.1688+0.0087 −0.0090 |
0.493±0.016 | 1.55745774 | 0.02539+0.00064 −0.00068 |
1,539 | transit | 801.2 | 0.90±0.07 | 5300±50 | [48] |
| TOI-4336 A c | 0.114 | 0.1039+0.0054 −0.0052 |
7.587270 | 0.0481±0.0027 | 378±12 | transit | 73.23 | 0.2853+0.0438 −0.0356 |
3369+51 −57 |
[37] |
| TOI-4427 b | 0.276+0.039 −0.041 |
1.168±0.028 | 4.6182621±0.0000017 | 0.05389+0.00520 −0.00350 |
1040+46 −50 |
transit | 646.52+3.03 −3.00 |
0.90±0.03 | 5347±135 | [45] |
| TOI-4458 b | 1.737±0.095 | 1.107±0.023 | 3.9393792±0.0000018 | 0.0522+0.0016 −0.0015 |
1759+30 −31 |
transit | 1648.35+16.63 −16.31 |
1.47±0.04 | 6151±160 | [45] |
| TOI-4495 b | 0.024+0.004 −0.05 |
0.221+0.012 −0.008 |
2.56699 | 0.03957±0.00047 | 1735 | transit | 801.2 | 1.247±0.045 | 6210±70 | [49] |
| TOI-4529 b | 0.0154 | 0.1579±0.008 | 5.87958 | 0.04997±0.0008 | 511 | transit | 92.6 | 0.482±0.023 | 3697±71 | [42] |
| TOI-4552 b | 0.00576±0.0016 | 0.099±0.0036 | 0.30110032±0.00000014 | 0.0056255±0.0000003 | 1122 | transit | 89.3 | 0.2619±0.0063 | 3258±115 | [50] |
| TOI-4602 b | 0.01948±0.0028 | 0.2195±0.02025 | 3.9812997±0.0000050 | 0.04746±0.00035 | 1321±78 | transit | 204.2 | 0.90±0.02 | 5966±50 | [51] |
| TOI-4616 b | 0.00708±0.00236 | 0.1088 | 1.55382±0.00001 | 0.0150±0.00001[d] | 525 | transit | 91.9 | 0.1881±0.0094 | 3150±75 | [52] |
| TOI-5007 b | 0.664+0.043 −0.042 |
0.9880±0.0310 | 2.543371±0.000001 | 0.0307±0.0012 | 774±19 | transit | 663.26+4.05 −4.00 |
0.632±0.013 | 3793±80 | [53] |
| TOI-5292 Ab | 1.299+0.081 −0.074 |
1.128+0.039 −0.037 |
2.021910±0.000003 | 0.0279±0.0013 | 809+22 −21 |
transit | 1099.13 ± 26.63 | 0.596±0.013 | 3919±80 | [53] |
| TOI-5624 b | 0.0296±0.0044 | 0.20644±0.00312 | 3.3903473±0.0000054 | 0.04201+0.00041 −0.00043 |
1136±15 | transit | 330.7±0.5 | 0.858+0.033 −0.029 |
5327±64 | [54] |
| TOI-5624 c | 0.0151±0.006 | 0.22072±0.00375 | 7.885385±0.000018 | 0.07374+0.00072 −0.00075 |
857±11 | transit | 330.7±0.5 | 0.858+0.033 −0.029 |
5327±64 | [54] |
| TOI-5624 d | 0.0154±0.0069 | 0.31975+0.00455 −0.0045 |
13.731468+0.000042 −0.000041 |
0.1067+0.0010 −0.0011 |
712.6+9.5 −9.4 |
transit | 330.7±0.5 | 0.858+0.033 −0.029 |
5327±64 | [54] |
| TOI-5624 e | 0.028+0.0091 −0.009 |
0.28968+0.00375 −0.00384 |
21.489936±0.000029 | 0.1439+0.0014 −0.0015 |
613.8+8.2 −8.1 |
transit | 330.7±0.5 | 0.858+0.033 −0.029 |
5327±64 | [54] |
| TOI-5624 f | 0.0409±0.0116 | 45.37+0.74 −0.90 |
0.2366+0.0040 −0.0041 |
478.5+7.1 −7.0 |
TTV | 330.7±0.5 | 0.858+0.033 −0.029 |
5327±64 | [54] | |
| TOI-5734 b | 0.0286±0.0082 | 0.187±0.011 | 6.1841876+0.0000080 −0.0000094 |
0.05921±0.00024 | 688±23 | transit | 106.034+0.255 −0.254 |
0.724±0.009 | 4750±100 | [55] |
| TOI-5628 Ab | 0.090±0.040 | 0.74±0.04 | 4.3416612±0.0000015 | 0.0368±0.0210 | 492±15 | transit | 358.87+2.987 −2.937 |
0.36±0.02 | 3310±100 | [56] |
| TOI-5788 b | 0.0117±0.0030 | 0.1365±0.0067 | 6.340758 | 0.0640±0.0011 | transit | 317.6 ± 0.4 | 0.87±0.04 | 5615±25 | [57] | |
| TOI-5788 c | 0.0201±0.0038 | 0.2025±0.0036 | 16.213358 | 0.1197±0.0020 | transit | 317.6 ± 0.4 | 0.87±0.04 | 5615±25 | [57] | |
| TOI-5789 b | 0.00667±0.00088 | 2.76369±0.00096 | 0.03608±0.00045 | 1201±26 | radial vel. | 66.726+0.124 −0.123 |
0.821+0.032 −0.027 |
5185±80 | [58] | |
| TOI-5789 c | 0.0157±0.0016 | 0.255+0.016 −0.013 |
12.927748±0.000016 | 0.1009±0.0013 | 718±15 | transit | 66.726+0.124 −0.123 |
0.821+0.032 −0.027 |
5185±80 | [58] |
| TOI-5789 d | 0.0135±0.0021 | 29.65±0.12 | 0.1756±0.0023 | 545±10 | radial vel. | 66.726+0.124 −0.123 |
0.821+0.032 −0.027 |
5185±80 | [58] | |
| TOI-5789 e | 0.03653±0.00305 | 62.98±0.22 | 0.2901±0.0037 | 424±8 | radial vel. | 66.726+0.124 −0.123 |
0.821+0.032 −0.027 |
5185±80 | [58] | |
| TOI-5916 b | 0.713+0.241 −0.114 |
1.013+0.032 −0.033 |
2.367128±0.000001 | 0.0262+0.0021 −0.0029 |
683+43 −29 |
transit | 651.43+11.10 −10.75 |
0.477±0.011 | 3613±80 | [53] |
| TOI-5938 b | 0.049+0.025 −0.022[c] |
0.341±0.010 | 2.2604240 | 0.0308±0.0010 | 1077+16 −15 |
transit | 371.9 | 0.744±0.016 | 4650±50 | [46] |
| TOI-6692 b | 0.620+0.080 −0.065 |
1.042+0.050 −0.049 |
131.125±0.012 | 0.512+0.014 −0.012 |
467.0+9.3 −9.5 |
transit | 1013 | 1.047+0.089 −0.071 |
5890+170 −180 |
[59] |
| TOI-6019 b | 0.469±0.047 | 1.10±0.03 | 14.547952+0.000036 −0.000035 |
0.1212±0.0033 | 1095±30 | transit | 849.047+7.718 −7.581 |
1.13±0.04 | 5561±70 | [47] |
| TOI-6716 b | 0.00287 | 0.0874±0.0062 | 4.71859 | 0.032±0.003 | 369 | transit | 61.6 | 0.223±0.011 | 3110±80 | [60] |
| TOI-7009 b | 0.047+0.023 −0.021[c] |
0.331±0.013 | 2.3206612 | 0.0287±0.0010 | 872+11 −10 |
transit | 600.5 | 0.583±0.014 | 4080±25 | [46] |
| TOI-7169 b | 0.41±0.14 | 1.475±0.029 | 3.4373125+0.0000020 −0.0000019 |
0.04280+0.00016 −0.00017 |
1631+19 −20 |
transit | 1524.303+22.931 −22.274 |
0.885 ±0.01 | 5714±42 | Orbits a metal-poor star.[61] |
| TOI-7384 b | 0.039 | 0.3176±0.0187 | 6.23403 | 0.0439±0.004 | 378 | transit | 218 | 0.318±0.016 | 3185±75 | [60] |
| WISPIT 2 c | 10±2 | 1.6+0.6 −0.7 |
14 | 2050±550 | imaging | 437 ± 1 | 1.08+0.06 −0.17 |
4400±50 | [62] | |
| TOI-201 d | 0.018±0.006 | 0.124±0.006 | 5.84889±0.00009 | 0.0698±0.0005 | transit | 365.9 ± 0.6 | 1.32+0.02 −0.04 |
6423+86 −90 |
[63] | |
| TOI-159 b | 3.49±0.26 | 1.622±0.015 | 3.7628396±0.0000003 | 0.0560±0.0007 | 1891±23 | transit | 1133.688+8.275 −8.157 |
1.661+0.017 −0.019 |
7287+69 −73 |
[64] |
| TIC 183374187 b | 0.56±0.19 | 1.252±0.070 | 5.05907±0.00059 | 1379±23 | transit | 3952.89+150.23 −139.82 |
0.853±0.048 | 5768±58 | [65] | |
| TOI-4311 b | 0.014+0.005 −0.004 |
0.1228+0.0069 −0.0071 |
0.9902738+0.0000029 −0.0000030 |
0.01817+0.00036 −0.00037 |
1664±28 | transit | 440.311+3.04 −3.00 |
0.816+0.047 −0.049 |
5063±66 | [66] |
| TOI-4311 c | <0.04273 | 0.220+0.011 −0.010 |
15.070425+0.000081 −0.000075 |
0.1116+0.0022 −0.0023 |
671±11 | transit | 440.311+3.04 −3.00 |
0.816+0.047 −0.049 |
5063±66 | [66] |
| TOI-3457 b | <2.51 | 0.949±0.022 | 32.600268+0.000028 −0.000030 |
0.2001±0.0064 | 824.2+10.3 −9.9 |
transit | 1209.118+10.033 −9.873 |
1.04±0.06 | 6300±120 | [67] |
| TOI-707 b | 0.2155±0.0087 | 52.79918+0.00021 −0.00016 |
0.275±0.010 | 491.7+7.9 −7.4 |
transit | 427.142+1.357 −1.347 |
0.990±0.060 | 5424±61 | [67] | |
| TOI-3664 b | 0.36±0.12 | 1.222±0.030 | 3.2974839±0.0000041 | 0.0431±0.0010 | 1232±12 | transit | 1516.122+15.885 −15.566 |
0.980±0.030 | 5593±32 | [68] |
| TOI-4034 b | 0.870±0.160 | 1.580±0.020 | 1.8020932±0.0000012 | 0.03289±0.00071 | 1907±22 | transit | 2431.015+29.237 −28.561 |
1.19+0.13 −0.03 |
5891±40 | [68] |
| TOI-6564 b | 0.699±0.066 | 1.463±0.019 | 3.985413±0.000011 | 0.0542±0.0012 | 1445±21 | transit | 624.237+4.534 −4.472 |
1.18+0.16 −0.03 |
5943±64 | [68] |
| HD 190360 d | 0.0322±0.0025 | 88.690+0.051 −0.049 |
0.3886±0.0046 | radial vel. | 52.2 ± 0.3 | 0.9960+0.0360 −0.0350 |
5560±100 | Star also known as Gliese 777[69] | ||
| HD 127195 b | 0.67±0.02 | 534.50+2.85 −2.92 |
radial vel. | 276.307 ± 1.871 | 1.34±0.06 | 4981±26 | [70] | |||
| HD 127195 c | 0.65±0.02 | 836.99+9.35 −9.67 |
radial vel. | 276.307 ± 1.871 | 1.34±0.06 | 4981±26 | [70] | |||
| HD 125136 b | 2.26±0.08 | 849.77+4.61 −4.73 |
radial vel. | 395.488 ± 1.438 | 1.55±0.08 | 4959±34 | [70] | |||
| HD 126105 b | 1.67+0.19 −0.17 |
524.0±2.9 | 1.36+0.05 −0.06 |
radial vel. | 270.329+1.079 −1.071 |
1.20+0.14 −0.21 |
4875+45 −40 |
[71] | ||
| TIC 150070085 b | 0.323+0.019 −0.018 |
10.474230+0.000045 −0.000044 |
945.06+62.73 −42.89 |
transit | 666.729+7.573 −7.407 |
1.16±0.06 | 5999±50 | [72] | ||
| Gl 725 B c | 0.011±0.002 | 37.90±0.17 | 0.139±0.004 | 215±4 | radial vel. | 11.491 ± 0.001 | 0.25±0.02 | 3379±31 | [73] | |
| HD 202206 b | 3.09±0.14 | 1299.22+3.21 −2.76 |
2.39+0.04 −0.05 |
radial vel. | 148.7 ± 0.2 | 1.06+0.07 −0.06 |
5764.23+64 −58 |
[74] | ||
| HIP 81991 b | 9.50+5.40 −2.20 |
5860±603 | 6.4+0.6 −0.3 |
radial vel. | 143.189 ± 0.233 | 1.09+0.07 −0.13 |
5100+40 −70 |
[75] | ||
| MOA-2020-BLG-108L b | 10.67+4.75 −5.41 |
3.69+0.98 −1.11 |
microlensing | 15492+4631 −5871 |
0.58+0.26 −0.30 |
[76] | ||||
| TOI-603 b | 0.104+0.020 −0.020 |
0.658±0.021 | 16.179846+0.000019 −0.000017 |
0.1282+0.0046 −0.0049 |
899±17 | transit | 671.706+5.192 −5.117 |
1.240±0.092 | 6027±93 | [77] |
| TOI-2114 b | 1.02+0.15 −0.14 |
1.298±0.060 | 6.2099590+0.0000045 −0.0000047 |
0.0760+0.0050 −0.0049 |
1472+57 −55 |
transit | 1036.800+8.043 −7.918 |
1.309±0.052 | 6400±170 | [77] |
| TOI-4492 b | 5.92+0.67 −0.64 |
1.051±0.055 | 4.4331824+0.0000015 −0.0000014 |
0.0535+0.0029 −0.0030 |
1207±34 | transit | 467.047+2.939 −2.900 |
1.067±0.055 | 5711±83 | [77] |
| TOI-5806 b | 2.27+0.26 −0.25 |
1.35+0.17 −0.11 |
3.1856381±0.0000010 | 0.0484±0.0025 | 1621+56 −52 |
transit | 388.814+2.711 −2.679 |
1.333±0.099 | 6730±190 | [77] |
| TOI-5811 B b | 0.81+0.11 −0.10 |
1.96±0.18 | 6.25663±0.00012 | 0.0731+0.0048 −0.0047 |
1530+50 −54 |
transit | 554.998+4.980 −4.896 |
1.08±0.32 | 4840±110 | [77] |
| TOI-6158 b | 0.425+0.060 −0.058 |
0.930+0.240 −0.100 |
3.04468990+0.00000551 −0.00000534 |
0.03275±0.00040 | 636±13 | transit | 590.679+12.068 −11.602 |
0.503+0.022 −0.023 |
3467±59 | [78] |
| TOI-7189 b | 0.50±0.09 | 0.980±0.050 | 2.89055000+0.00000612 −0.00000610 |
0.03294+0.00037 −0.00038 |
738±32 | transit | 626.601+5.255 −5.171 |
0.612+0.024 −0.023 |
3775±59 | [79] |
| TOI-7265 B b | 0.71±0.09 | 0.95±0.04 | 4.17232000+0.00000256 −0.00000257 |
0.04007+0.00052 −0.00054 |
571±27 | transit | 469.624+3.451 −3.400 |
0.521±0.023 | 3503±59 | [79] |
| TOI-7393 b | 0.61±0.07 | 1.01±0.06 | 3.33708000+0.00000095 −0.00000094 |
0.03664±0.00041 | 747±32 | transit | 616.561 ± 2.101 | 0.600±0.021 | 3927±59 | [79] |
| TOI-7394 B b | 2.10+0.13 −0.15 |
1.02±0.06 | 1.25299500±0.00000031 | 0.01913±0.00021 | 986.0±42.0 | transit | 619.682+3.131 −3.102 |
0.624±0.022 | 3717±59 | [79] |
| TOI-4468 b | 0.535+0.031 −0.028 |
1.01 ± ~0.03 | 2.77085931 ± 0.00000036 | 0.03592+0.0006 −0.00057 |
1153+26 −22 |
radial vel. | 1,233 ± 6 | 0.805+0.042 −0.038 |
5170+120 −110 |
[80] |
| TOI-2195 A b | 0.079±0.017 | 0.793+0.024 −0.022 |
4.16451307±0.00000054 | 0.04901+0.00065 −0.00052 |
1,098 ± 10 | transit | 174.67±0.3 | 0.905+0.036 −0.028 |
5266+72 −76 |
[81] |
Specific exoplanet lists
- List of directly imaged exoplanets
- List of exoplanet extremes
- List of exoplanet firsts
- List of exoplanets discovered by the Kepler space telescope
- List of exoplanets observed during Kepler's K2 mission
- List of exoplanets discovered by the TESS mission
- List of extrasolar candidates for liquid water
- List of terrestrial exoplanet candidates for atmosphere detection
- List of hottest exoplanets
- List of coldest exoplanets
- List of multiplanetary systems
- List of circumbinary planets
- List of nearest exoplanets
- List of nearest terrestrial exoplanet candidates
- List of potentially habitable exoplanets
- List of proper names of exoplanets
- List of largest exoplanets
- List of smallest exoplanets
- List of transiting exoplanets
- List of exoplanets and planetary debris around giant stars
- List of exoplanets and planetary debris around white dwarfs
- List of extrasolar planetary collisions
Lists of exoplanets by year of discovery
- List of exoplanets discovered before 2000 (31)
- List of exoplanets discovered between 2000–2009 (375)
- List of exoplanets discovered in 2010 (109)
- List of exoplanets discovered in 2011 (179)
- List of exoplanets discovered in 2012 (149)
- List of exoplanets discovered in 2013 (149)
- List of exoplanets discovered in 2014 (869)
- List of exoplanets discovered in 2015 (144)
- List of exoplanets discovered in 2016 (1498)
- List of exoplanets discovered in 2017 (152)
- List of exoplanets discovered in 2018 (300)
- List of exoplanets discovered in 2019 (169)
- List of exoplanets discovered in 2020 (256)
- List of exoplanets discovered in 2021 (253)
- List of exoplanets discovered in 2022 (312)
- List of exoplanets discovered in 2023 (304)
- List of exoplanets discovered in 2024 (284)
- List of exoplanets discovered in 2025 (138)
- List of exoplanets discovered in 2026 (159)
Notes
- ↑ Mass determination depends on whether the orbit is prograde or retrograde.
- ↑ Mass determination depends on whether the star is an Ophiuchus or Upper Scorpius association member.
- 1 2 3 4 Estimated using theoretical mass–radius relations.
- ↑ Converted from orbital period.
References
- ↑ Sutlieff, Ben J.; Bonse, Markus J.; Christiaens, Valentin; Fontanive, Clémence; Matthews, Elisabeth C.; et al. (15 July 2026). "Direct Imaging Discovery of Giant Exoplanet β Pictoris d: A Decade-long Game of Hide-and-seek". The Astrophysical Journal Letters. 1006 (1): L10. arXiv:2606.23801. Bibcode:2026ApJ..1006L..10S. doi:10.3847/2041-8213/ae80a0. ISSN 2041-8205.
- ↑ Gibbs, Aidan; Ruffio, Jean-Baptiste; Bidot, Alexis; Barman, Travis S.; Do Ó, Clarissa R.; et al. (15 July 2026). "Discovery of an Exterior Third Planet Orbiting β Pictoris". The Astrophysical Journal Letters. 1006 (1): L11. arXiv:2606.23789. Bibcode:2026ApJ..1006L..11G. doi:10.3847/2041-8213/ae801b. ISSN 2041-8205.
- 1 2 3 4 5 6 Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875.
- 1 2 3 4 5 6 7 Standing, Matthew R.; Barnes, John R.; et al. (2026). "The Dispersed Matter Planet Project Sample - Detection limits, Occurrence Rates and New Planets". Monthly Notices of the Royal Astronomical Society. stag370 (3) stag370. arXiv:2602.18207. doi:10.1093/mnras/stag370. S2CID 285872137.
- 1 2 3 4 Stassun, Keivan G.; Oelkers, Ryan J.; Paegert, Martin; Torres, Guillermo; Pepper, Joshua; De Lee, Nathan; Collins, Kevin; Latham, David W.; Muirhead, Philip S.; Chittidi, Jay; Rojas-Ayala, Bárbara; Fleming, Scott W.; Rose, Mark E.; Tenenbaum, Peter; Ting, Eric B. (1 October 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv:1905.10694. Bibcode:2019AJ....158..138S. doi:10.3847/1538-3881/ab3467. ISSN 0004-6256. S2CID 166227927.
- ↑ Harris, Mallory; Dragomir, Diana; Bachelet, Etienne; Fausnaugh, Michael; Johnson, Samson (10 July 2026). "TESS's First Bound Microlensing Planet—A Binary Microlensing Event Revealing a Planetary Companion toward the Galactic Plane". The Astrophysical Journal Letters. 1005 (2): L33. arXiv:2607.01853. Bibcode:2026ApJ..1005L..33H. doi:10.3847/2041-8213/ae7a50. ISSN 2041-8205.
- ↑ Conzo, G.; Moriconi, M.; CorrêaJr., S. A. (2026). "Detection and Characterization of the Temperate Super-Earth Gliese 48 B" (PDF). Open European Journal on Variable Stars. 273 (273): 1–18. arXiv:2605.11123. Bibcode:2026OEJV..273....1C. doi:10.5817/OEJV2026-0273.
- ↑ Kroft, Maxwell A.; Beatty, Thomas G.; Salzer, Joseph M.; Zwicker, Claire; Triantafillides, Anastasia; Becker, Juliette; Soares-Furtado, Melinda; Cisewski-Kehe, Jessi; Lissauer, Jack J. (25 March 2026), GJ 523b is a Massive, 170 Myr-old Mega-Earth, Likely on a Polar Orbit, arXiv:2603.24682
- 1 2 Hartogh, C.; Jeffers, S. V.; et al. (January 2026). "RedDots: Multiplanet system around M dwarf GJ 887 in the solar neighborhood". Astronomy & Astrophysics. 707: A93. arXiv:2602.08929. Bibcode:2026A&A...707A..93H. doi:10.1051/0004-6361/202554984. S2CID 284940885.
- ↑ Stoeva, Denitza; Stefanov, Atanas K.; et al. (March 2026). "Long-period magnetic activity in the K dwarf GJ 1137 and a new super-Earth on a 9-day orbit". Astronomy & Astrophysics. 708: A232. arXiv:2603.04919. doi:10.1051/0004-6361/202557806.
- ↑ Lamontagne, Pierrot; et al. (14 January 2026). "NIRPS tightens the mass estimate of GJ 3090 b and detects a planet near the stellar rotation period". Astronomy & Astrophysics. 706: A278. arXiv:2601.09330. Bibcode:2026A&A...706A.278L. doi:10.1051/0004-6361/202556887.
- ↑ Robertson, Paul; Endl, Michael; Cochran, William D.; Stefansson, Gudmundur; Mahadevan, Suvrath; Cañas, Caleb I.; James, Gogod; Arendtsz, Roan; Terrien, Ryan C.; Bender, Chad F.; Diddams, Scott A.; Giovinazzi, Mark R.; Gupta, Arvind F.; Halverson, Samuel; Kanodia, Shubham (30 June 2026). "A Revised Mass and Period for the Habitable Zone super-Earth GJ 3378 b: A Planet Straddling the Cosmic Shoreline". The Astrophysical Journal. 1005 (1): 32. arXiv:2605.16499. Bibcode:2026ApJ..1005...32R. doi:10.3847/1538-4357/ae732b. ISSN 0004-637X.
- 1 2 Charpentier, Paul; Moutou, Claire; Donati, Jean-François; Larue, Pierre; Delfosse, Xavier; Cortés-Zuleta, Pía; Ould-Elhkim, Merwan; Artigau, Étienne; Cadieux, Charles; Hebrard, Guillaume; L’Heureux, Alexandrine; Carmona, Andres; Debras, Florian; Boisse, Isabelle; Cook, Neil James (23 January 2026). "SPIRou detects two planets around the nearby M4.5V star GJ 4274". Astronomy & Astrophysics. 705: A243. Bibcode:2026A&A...705A.243C. doi:10.1051/0004-6361/202557666. ISSN 0004-6361.
- 1 2 3 4 Wu, Yiyun; Xiao, Guang-Yao; Butler, R. Paul; Feng, Fabo; Shectman, Stephen A.; Crane, Jeffrey D.; Teske, Johanna K.; Wang, Sharon X.; Beletsky, Yuri; Burt, Jennifer A.; Daylan, Tansu; Diaz, Matias; Dragomir, Diana; Flowers, Erin; Jenkins, Sydney; Kanodia, Shubham; Nandakumar, Sangeetha; Rice, Malena; Shporer, Avi; Yee, Sam; Zhou, George; Lin, Zitao (2026). "Detection of four cold Jupiters through combined analyses of radial velocity and astrometry data". The Astronomical Journal. 171 (3): 189. arXiv:2601.11280. Bibcode:2026AJ....171..189W. doi:10.3847/1538-3881/ae40f5.
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- 1 2 Rea, Erika; Günther, Maximilian N.; Dransfield, George; Guillot, Tristan; Triaud, Amaury H. M. J.; Stassun, Keivan G.; Espinoza-Retamal, Juan I.; Brahm, Rafael; Ulmer-Moll, Solène; Beltrame, Matteo; Deloupy, Vincent; Timmermans, Mathilde; Abe, Lyu; Agabi, Karim; Bendjoya, Philippe (14 July 2026). "High five from ASTEP: Three validated planets and two eclipsing binaries in a diverse set of long-period candidates". Astronomy & Astrophysics. 711: A86. arXiv:2510.01725. Bibcode:2026A&A...711A..86R. doi:10.1051/0004-6361/202557498. ISSN 0004-6361.
- 1 2 3 Battley, Matthew P; Lafarga, Marina; Gillen, Edward; Lendl, Monika; Ulmer-Moll, Solène; Ho, Cynthia S K; Marfil, Emilio; Sousa, Sergio; Frensch, Yolanda; Veras, Dimitri; Bouchy, François; Carteret, Yann; Crossfield, Ian J M; Fairnington, Tyler; Houelle, Mathilde (11 July 2026). "TOI-3664 b, TOI-4034 b, and TOI-6564 b: three new hot Jupiters around stars approaching the terminal age main sequence". Monthly Notices of the Royal Astronomical Society. 549 (4) stag1053. arXiv:2606.05295. doi:10.1093/mnras/stag1053. ISSN 0035-8711.
- ↑ Giovinazzi, Mark R.; Fitzmaurice, Evan; Gupta, Arvind F.; Robertson, Paul; Mahadevan, Suvrath; Ford, Eric B.; Alvarado-Montes, Jaime A.; Bender, Chad F.; Blake, Cullen H.; Dong, Jiayin; Fernandes, Rachel B.; Halverson, Samuel; Han, Te; Kanodia, Shubham; Krolikowski, Daniel M. (1 May 2026). "The NEID Earth Twin Survey. IV. Confirming an 89 days, m sin i = 10 M ⊕ Planet Orbiting a Nearby Sun-like Star". The Astronomical Journal. 171 (5): 286. doi:10.3847/1538-3881/ae48f1. ISSN 0004-6256.
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- ↑ Wittenmyer, Robert A; Venner, Alexander; Fairnington, Tyler; Zhou, George; Wright, Duncan J; Curtin, Evan; Bedding, Timothy R; Crawford, Courtney L; Li, Yaguang; Stello, Dennis; Hon, Marc; Huber, Daniel; Grundahl, Frank; Skakke.Fredslund, M; Palle, Pere L (21 July 2026). "The Pan-Pacific Planet Search–IX. A menagerie of companions orbiting evolved stars". Monthly Notices of the Royal Astronomical Society. 550 (1) stag1038. doi:10.1093/mnras/stag1038. ISSN 0035-8711.
- ↑ Barber, Madyson G.; Mann, Andrew W.; Vach, Sydney; Boff, Leah J.; Boyle, Andrew W.; Vanderburg, Andrew; Kraus, Adam L.; Tofflemire, Benjamin M.; Johnson, Marshall C.; Bieryla, Allyson; Latham, David W.; Collins, Karen A.; Howell, Steve B.; Schwarz, Richard P.; Srdoc, Gregorg (3 August 2026). "Stellar Obliquities of Young Systems, Atmospheres Undergoing Contraction and Escape (SOYSAUCE). II. A 135 Myr Planet on an Aligned Orbit with Transit Timing Variations". The Astronomical Journal. 172 (2): 73. arXiv:2606.09973. Bibcode:2026AJ....172...73B. doi:10.3847/1538-3881/ae78d0. ISSN 0004-6256.
- ↑ Ould-Elhkim, M.; Moutou, C.; Donati, J.-F.; Cortés-Zuleta, P.; Delfosse, X.; Artigau, é.; Cadieux, C.; Charpentier, P.; Carmona, A.; Boisse, I.; Reylé, C.; Gaidos, E.; Cloutier, R.; Hébrard, G.; Arnold, L. (26 January 2026). "The SPIRou Legacy Survey: Detection of a nearby world orbiting in the habitable zone of Gl 725B achieved by correcting strong telluric contamination in near-infrared radial velocities with wapiti". Astronomy & Astrophysics. 705: A234. arXiv:2601.22815. Bibcode:2026A&A...705A.234O. doi:10.1051/0004-6361/202555469. ISSN 0004-6361.
- ↑ Cao, Yingyi; Lee, Man Hoi; Reffert, Sabine; Trifonov, Trifon; Stefanov, Stefan (17 July 2026). "Dynamical analysis of the 5:1 mean-motion resonance of the HD202206 system". Astronomy & Astrophysics. 711: A229. arXiv:2607.04396. Bibcode:2026A&A...711A.229C. doi:10.1051/0004-6361/202660788. ISSN 0004-6361.
- ↑ Van Zandt, Judah; Bowler, Brendan P.; Petigura, Erik A.; Franson, Kyle; Xuan, Jerry W.; Morgan, Marvin; Biddle, Lauren I.; Kiman, Rocio; Zhang, Jingwen; Isaacson, Howard; Fulton, Benjamin; Howard, Andrew W.; Crepp, Justin R.; Thompson, William; Blakely, Dori (1 August 2026). "Gaia Exoplanet Orbits, Demographics, and Evolution Survey (GEODES). I. Characteristics of Three Long-period Companions Accelerating their Host Stars". The Astrophysical Journal. 1006 (2): 222. arXiv:2605.23018. Bibcode:2026ApJ..1006..222V. doi:10.3847/1538-4357/ae74cd. ISSN 0004-637X.
- ↑ Satoh, Yuki K; Bennett, David P; Sumi, Takahiro; Bond, Ian; Rattenbury, Nicholas; Suzuki, Daisuke; Koshimoto, Naoki; Miyazaki, Shota; Kirikawa, Rintaro; Abe, Fumio; Bhattacharya, Aparna; Hamada, Ryusei; Ishitani, Stela; Hirao, Yuki; Matsubara, Yutaka (28 July 2026). "MOA-2020-BLG-108Lb: A giant planet beyond the snow line of a low-mass lens near the lower boundary of the mass-ratio desert". Publications of the Astronomical Society of Japan psag091. arXiv:2607.12081. doi:10.1093/pasj/psag091. ISSN 2053-051X.
- 1 2 3 4 5 Lillo-Box, J.; Cifuentes, C.; Balsalobre-Ruza, O.; Montesinos, B.; Latham, D.; Collins, K. A.; Ciardi, D.; Hébrard, G.; Yee, S. W. (22 July 2026), CAFE follow-up of TESS hot Jupiter candidates left behind: I. Five newly confirmed planets and a false positive, arXiv:2607.19756
- ↑ O’Brien, Shane; Wong, Amber; Han, Te; Robertson, Paul; Kanodia, Shubham; Cañas, Caleb I.; Gupta, Arvind F.; Swaby, Tera; Kobulnicky, Henry A.; Morrell, Nidia; Rodruck, Michael; Lin, Andrea S. J.; Monson, Andrew; Cochran, William D.; Bender, Chad F. (3 August 2026). "Searching for GEMS: TOI-5916 b & TOI-6158 b are Two Saturn-density Planets Orbiting M2 Dwarfs". The Astronomical Journal. 172 (2): 117. arXiv:2510.11798. Bibcode:2026AJ....172..117O. doi:10.3847/1538-3881/ae844e. ISSN 0004-6256.
- 1 2 3 4 Premnath, Pranav H.; Robertson, Paul; Kanodia, Shubham; Cañas, Caleb I.; Gupta, Arvind F.; Rodruck, Michael; Han, Te; Kobulnicky, Henry A.; Lin, Andrea S.J.; Monson, Andrew; Allely, Libby; Bailey, Cooper; Birkholz, Alexina; Beagle, Zack; Choi, Philip (3 August 2026). "Searching for GEMS: Three Warm Saturns and a Super-Jupiter Orbiting Four Early M Dwarfs*". The Astronomical Journal. 172 (2): 92. arXiv:2604.27064. Bibcode:2026AJ....172...92P. doi:10.3847/1538-3881/ae82d3. ISSN 0004-6256.
- ↑ Livesey, Joseph R.; Hord, Benjamin J.; Becker, Juliette; Vanderburg, Andrew; Rodriguez, Joseph E.; Koo, Elise; Huang, Chelsea X.; Stefánsson, Gudmundur; Collins, Karen A. (25 August 2026). "Discovery and Characterization of the TOI-4468 Planetary System: A Transiting Hot Jupiter With a Lone Nearby Outer Companion". arXiv.org. Retrieved 29 August 2026.
- ↑ Weldon, Grant C.; Yee, Samuel W.; Hansen, Bradley M. S.; Naoz, Smadar; Hartman, Joel D.; Winn, Joshua N.; Butler, R. Paul; Crane, Jeffrey D.; Evans, Phil (1 July 2026). "Discovery of an Inflated Hot Neptune and Its Formation from Jovian Mass Loss". arXiv.org. Retrieved 29 August 2026.


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