List of exoplanets discovered in 2025

This list of exoplanets discovered in 2025 is a list of confirmed exoplanets that were first reported in 2025. For exoplanets detected only by radial velocity, the listed value for mass is a lower limit. See Minimum mass for more information.

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
AB Pictoris c 2.5–9 3–5 astrometry + radial vel. 163 0.90±0.10 5188±50 [1]
AT2021uey b 1.34+0.45
−0.50 		4,170+2,910
−1,710 		4.01+1.68
−1.34 		microlensing 3,390+2,410
−1,440 		0.49+0.16
−0.18 		3,680+307
−204 		[2]
Barnard's Star c 0.00105 4.12 0.0274±0.0004 radial vel. 5.96 0.162 3,195 [3]
Barnard's Star d 0.00083 2.34 0.0188±0.0003 radial vel.
Barnard's Star e 0.00061 6.74 0.0381±0.0005 radial vel.
BEBOP-3b 0.558+0.051
−0.048 		547.0+6.2
−7.6 		1.444±0.017 radial vel. 385.13±0.58[4] 1.3445[a] 6,033[b] A circumbinary planet.[5]
BD+05 4868 Ab 0.000063 0.028 1.27187 0.0208±0.0003 1,820±45 transit 142.4±0.1 0.70±0.02 4,596+65
−64 		A disintegrating planet with a comet-like tail.[6]
Cha 1107-7626 8.0±2.0 2.8 1800 imaging 636 Free-floating object of planetary mass. Could also be a sub-brown dwarf.[7]
G 192-15 b 0.00324±0.00057 2.27476+0.00026
−0.00028 		0.01723+0.00038
−0.00039 		453.6+8.8
−8.5 		radial vel. 31.09±0.022 0.132±0.009 Also known as GJ 3380 b.[8]
G 192-15 c 0.0450+0.0050
−0.0047 		1,219+13
−11 		1.137+0.026
−0.027 		55.9±1.1 radial vel. Also known as GJ 3380 c.[8]
G 261-6 b 0.00431+0.00072
−0.00069 		5.4536+0.0031
−0.0032 		0.02971+0.00087
−0.00093 		322.3+9.9
−9.7 		radial vel. 34.66±0.021 0.118±0.011 [8]
G 268-110 b 0.00478±0.00079 1.432630+0.000072
−0.000076 		0.01283+0.00028
−0.00029 		534+12
−11 		radial vel. 31.86 0.137±0.009 [8]
Gliese 251 c 0.01207 53.647±0.044 0.196±0.014 radial vel. 18.21 0.360±0.015 3342±24 Potentially habitable.[9]
Gliese 410 b 0.0249±0.0038 6.02 0.0531±0.0007 radial vel. 38.9 0.55±0.02 3,842±31 Two additional planets in the same system are suspected.[10]
Gliese 536 c 0.01853±0.0022 32.76 0.1617±0.003 290 radial vel. 32.71 0.52±0.05 3685±68 [11]
GJ 2126 b 1.3+0.2
−0.1 		272.7 0.71±0.03 radial vel. 124.3±0.4 0.65+0.09
−0.07 		4,159±130 [12]
GJ 3998 d 0.0191+0.00315
−0.00302 		41.78±0.05 0.189±0.006 radial vel. 58.056±2.283 0.52±0.05 3726±68 [13]
Gliese 508.2 b 1.85 ~5300 4.85 radial vel. 54.3 0.54±0.12 3,720±12 [14]
GJ 9773 b 0.543 2965 2.921±0.045 radial vel. 51.8 0.358±0.011 3,528±25 [14]
HD 85426 c 0.0324+0.0050
−0.0047 		35.73+0.09
−0.10 		0.2118+0.0050
−0.0044 [c] 		640±9 radial vel. 175.3 0.991+0.027
−0.020 		5,746±59 Star also known as TOI-1774. An additional planet is suspected in the system.[15]
HD 87816 b 6.74 484 1.618±0.0003 radial vel. 434.4 2.41±0.1 4,989±46 Host star also known as R Velorum.[16]
HD 87816 c 12.2 7,596+1140
−535 		10.14+1.0
−0.5 		radial vel.
HD 94890 b 2.13 824 2.07±0.001 radial vel. 201.2 1.74±0.20 4,867±38 Host star also known as iota Antliae.[16]
HD 94890 c 8.9 2492 4.33±0.02 radial vel.
HD 102888 b 5.69 252 1.05±0.001 radial vel. 412.6 2.42±0.06 4,990±39 [16]
HD 135344 Ab 10.0+1.4
−1.9 		1.45+0.06
−0.03 		16.5+2.8
−2.0 		1,585+82
−73 		imaging 440 1.5 9,540±100 [17]
HD 143811 (AB)b 5.6±1.1 1.41±0.03 – 1.7 +0.7
−0.4 		117000 +91000
−31000 		63.88 1042 imaging 446.4 2.5 6,575±325 A circumbinary planet.[18]
HD 224018 b 0.0129±0.0025 0.0812+0.0036
−0.033 		10.64 0.0952±0.002 968 transit 346.0±0.7 1.013+0.069
−0.061 		5,784±60 [19]
HD 224018 c 0.0327+0.0041
−0.0035 		0.2159+0.0062
−0.0071 		36.58 0.217±0.005 641 transit
HD 224018 d 0.0132+0.0057
−0.0050 		0.214±0.009 138.1 0.53+0.06
−0.02 		411 transit
HD 224018 e 0.475+0.041
−0.044 		9129±2499 8.6+1.5
−1.6 		102 radial vel.
HIP 54515 b 17.7+7.6
−4.9 		1.08±0.23 32500+15000
−8800 		24.8+7.2
−4.7 		2,348±218 imaging + astrometry 271.4 1.88±0.11 8,100+500
−340 		Host star also known as 66 Leonis.[20]
HIP 99452 Ab 0.00667±0.00088 2.764 0.03608±0.00045 1201 radial vel. 66.67 0.821±0.032 5,185±80 [21]
HIP 99452 Ac 0.016±0.0016 0.2552±0.0161 12.93 0.1009±0.0013 718 transit
HIP 99452 Ad 0.0135±0.0022 29.65 0.175±0.002 545 radial vel.
HIP 99452 Ae 0.0365±0.003 62.98 0.290±0.004 424 radial vel.
J042705.86+261520.3 4.5 imaging 522 Part of a JuMBO along with J042705.86+261520.3 b .[22]
J042705.86+261520.3 b 3.9 imaging 522 Part of a JuMBO along with J042705.86+261520.3.[22]
J041546.22+280811.4 6.0 imaging – Free-floating object of planetary mass. Could also be a sub-brown dwarf.[22]
K2-157 c 0.0969 25.9 0.165±0.0018 587 radial vel. 946.5 0.89 ± 0.029 5,334 ± 64 [23]
K2-157 d 0.0733 66.5 0.309±0.0038 429 radial vel.
Kepler-139 f 0.113±0.0315 355±2 radial vel. + timing 1,289.78±13.89 1.08 5,594±100 [24]
Kepler-279 e 0.176+0.0189
−0.0154 		0.310±0.0482 ~98.35 transit 3,487.26±74.07 1.10+0.16
−0.13 		6,363±259 [25]
Kepler-289 e 0.0547+0.00409
−0.00377 		0.286+0.00437
−0.00259 		~330 transit 2,283.09±45.66 1.08±0.02 5,990±38 [25]
Kepler-725 c 0.031 207.5 0.674±0.002 timing 2474±45 0.91 5,293±122 Partially in habitable zone.[26]
KMT-2017-BLG-2197Lb 8.84+8.3
−4.9 		15.9+2.1
−2.7 		microlensing 25,400+3,300
−4,300 		0.36+0.34
−0.2 		[27]
KMT-2019-BLG-0578Lb 1.2+1.2
−0.6 		1.2±0.2 or 2.0±0.3 microlensing 23,810+2,280
−2,610 		0.28+0.28
−0.14 		[28]
KMT-2021-BLG-0736Lb 0.0661+0.0409
−0.0315 		4.0+0.9
−0.8 		microlensing 22,830+2,610
−4,890 		0.60+0.37
−0.29 		[28]
KMT-2022-BLG-1790Lb 1.73+0.95
−0.9 		5.25+0.75
−1.0 		microlensing 21,100+3,000
−4,200 		0.58+0.32
−0.3 		[27]
KMT-2022-BLG-1818Lb 1.5+0.6
−0.3 		1.5+0.3
−0.2 		microlensing 9460+2280
−1300 		0.3+0.12
−0.06 		[29]
KMT-2022-BLG-1818Lc 0.35+0.24
−0.17 		0.4±0.1 microlensing
KMT-2022-BLG-2076Lb 0.88±0.46 5.67±1.58 microlensing 18,200+4,100
−5,000 		0.67±0.35 [27]
KMT-2023-BLG-0119Lb 0.2634+0.16822
−0.14396 		3.14+1.32
−1.33 or 4.01+1.69
−1.70 		microlensing 10,240+5,510
−5,540 		0.71+0.45
−0.39 		[30]
KMT-2023-BLG-1896Lb 0.0515+0.03087
−0.02656 		2.86+1.12
−1.02 or 4.62+1.81
−1.94 		microlensing 17,900+7,000
−7,500 		0.72+0.43
−0.37 		[30]
KMT-2023-BLG-2209Lb 0.80±0.38 5.31+0.95
−1.1 		microlensing 18,200+5,000
−5,700 		0.73±0.35 [27]
KMT-2024-BLG-0176Lb 0.76+1.03
−0.39 		0.75+0.09
−0.10 or 1.32+0.16
−0.18 		microlensing 27201+3294
−3686 		0.103+0.141
−0.054 		[31]
KMT-2024-BLG-0349Lb 11.86+6.56
−6.54 		1.85+0.65
−0.77 or 6.46+2.27
−2.69 		microlensing 18754+6588
−7795 		0.68±0.38 [31]
KMT-2024-BLG-0404Lb 0.0544+0.0802
−0.0277 		0.34±0.05 microlensing 23,510+3,030
−3,160 		0.09+0.133
−0.046 		Also a brown dwarf exists in the system[32]
KMT-2024-BLG-1209Lb 2.64+1.57
−1.16 		2.51+1.50
−1.10 		microlensing 12,800+6,600
−4,600 		0.77+0.46
−0.34 		[33]
KMT-2024-BLG-1870Lb 1.06+0.53
−0.55 		2.57+0.64
−0.97 or 3.15+0.79
−1.19 		microlensing 17873+4468
−6719 		0.67+0.33
−0.34 		[31]
KMT-2024-BLG-2087Lb 4.39+3.07
−2.46 		3.03+0.42
−0.54 		microlensing 23451+3098
−4175 		0.48+0.27
−0.33 		[31]
KOBE-1 b 0.0277±0.0024 8.54 0.07±0.0004 594 radial vel. 77.89±0.04 0.629±0.017 4,135±36 [34]
KOBE-1 c 0.039±0.0035 29.67 0.161±0.001 392 radial vel.
KOI-134 b 1.08±0.2 67.59 0.358 588 transit 3780 1.17 6154±26 [35]
KOI-134 c 0.22 ± 0.01 33.5 timing
KOINTREAU-1 b 10.6±2.5 690±10 imaging 518.6 0.26±0.03 3,551±59 [36]
L 98-59 f 0.00934 23.07 0.1053±0.0024 radial vel. 34.6 0.32±0.03 3,415±135 Potentially habitable[37]
MOA-2022-BLG-033Lb 0.0382+0.0296
−0.0197 		2.15+1.17
−0.75 or 2.31+1.27
−0.81 		microlensing 6,000+3,260
−2,640 		0.51+0.39
−0.26 		[30]
MOA-2022-BLG-091Lb 3.59+2.00
−1.67 		2.67+1.45
−1.24 to 3.63+1.30
−1.31 		microlensing 13,900+4,960
−4,990 		0.75+0.42
−0.35 		[33]
MP Muscae b 5.0 1 – 3 astrometry + disk kinematics 319.3 1.3±0.08 5000 [38]
Mu2 Octantis Ac 0.0318±0.0038 4.60111±0.00024 0.056 radial vel. 130.3 1.330±0.013 6059±52 Also known as HD 196067 c.[39]
OGLE-2016-BLG-0007Lb 0.00415+0.0028
−0.0022 		10.1+3.8
−3.4 		microlensing 14,020+3590
−4570 		0.6+0.4
−0.3 		[40]
OGLE-2023-BLG-0524 0.0293 or 0.182[d] microlensing – Free-floating object of planetary mass.[41]
o005 s41280 8.4 2.3 2,162 imaging 17,300 Free-floating object of planetary mass. Could also be a sub-brown dwarf.[42]
o006 s00089 11.5 1.2 955 imaging 6,520 Free-floating object of planetary mass. Could also be a sub-brown dwarf.[42]
Ross 176 b 0.01438±0.0028 0.1642±0.0071 5.00663±0.00008 0.0464±0.001 682 transit 151.7 0.58±0.02 4,061±70 [43]
TIC 88785435 b 0.449±0.019 10.508843 0.08432±0.00068 635±16 transit 398.2±0.8 0.724±0.017 3,998±95 [44]
TOI-201 c 14.2±2.0 0.99±0.017 2,800+360
−210 		4.28+0.36
−0.2 		timing + transit 372.5 1.316±0.027 6,394±75 [45]
TOI-333 b 0.0632±0.0076 0.3801±0.0098 3.785250±0.000006 0.049±0.001 1445 transit 1132 1.2±0.1 6,241±73 [46]
TOI-375 b 0.745+0.052
−0.053 		0.961+0.044
−0.043 		9.45469±0.00002 0.099±0.002 1,373+47
−45 		transit 1316 1.441+0.076
−0.075 		5,259.9+136.9
−135.3 		The star is a subgiant.[47]
TOI-375 c 2.106+0.223
−0.212 		115.5+2.0
−1.6 		0.524±0.011 596±21 radial vel.
TOI-375 d 1.402+0.311
−0.276 		297.9+28.9
−18.6 		0.984+0.062
−0.044 		434±19 radial vel.
TOI-512 b 0.01123+0.00167
−0.00173 		0.1374±0.0089 7.18886+0.000069
−0.000077 		1,009±29 transit 219.16±0.14 0.74±0.03 5,277±67 [48]
TOI-771 c 0.00903 7.61 0.046±0.002 365 radial vel. 82.45 0.22±0.024 3,201±100 [49]
TOI-1117 b 0.028±0.003 0.219+0.012
−0.011 		2.22816±0.00001 0.0330±0.0002 1,538±21 transit 546.64±2.94 0.97±0.02 5,635±62 [50]
TOI-1117 c 0.0276+0.0037
−0.0038 		4.579±0.004 0.0534±0.0003 1,210±16 radial vel.
TOI-1117 d 0.0337±0.0050 8.665±0.011 0.0817±0.0006 978±13 radial vel.
TOI-1203 b 0.0110±0.0010 0.1356+0.0040
−0.0041 		4.1572888 0.04869+0.00094
−−0.00095 		1361.2+18.8
−18.4 		transit 211.9 0.886±0.036 5,737±62 An old thick disk star. The fourth planet in the system, TOI-1203 d, was already validated in 2020.[51]
TOI-1203 c 0.0172±0.0016 13.0766+0.0079
−0.0072 		radial vel.
TOI-1203 e 0.1325+0.0058
−0.0056 		204.59+0.67
−0.63 		radial vel.
TOI-1453 Ab 0.00390+0.00208
−0.00204 		0.105+0.00526
−0.00500 		4.3135225+0.0000118
−0.0000092 		transit 257.288±0.209 0.715±0.035 4,975±68 [52]
TOI-1453 Ac 0.00928+0.00261
−0.00264 		0.198±0.00848 6.5886982 transit
TOI-1846 b 0.01385+0.00503
−0.00315 		0.15987+0.00580
−0.00607 		3.931 0.03646+0.00072
−0.00074 		568.1+6.1
−5.9 		transit 154.09±0.11 0.40±0.02 3,568±44 [53]
TOI-2005 b <6.4 1.07+0.06
−0.11 		17.305904+0.000023
−0.000020 		0.16±0.02 transit 1,072.08+15.00
−13.70 		1.59+0.016
−0.017 		7,130±150 [54]
TOI-2015 c 0.02803+0.001196
−0.001259 		5.582796+0.000042
−0.000041 		0.041232±0.000004 448±3 timing 154.34±0.16 0.3041+0.0353
−0.0312 		3,297+14
−28 		[55] Already suspected on discovery of TOI-2015 b in 2023 based on observed TTVs but without clear detection.[56]
TOI-2076 e 0.12089+0.00901
−0.00874 		3.0223445±0.0000033 0.0385+0.0021
−0.0049 		1138 transit 136.7 0.849+0.027
−0.026 		5,200±100 [57]
TOI-2267 b 0.0893 or 0.1089 2.2891 0.0205 or 0.0127 transit 73.5 0.270[e] 3,030±100[f] [58][59]
TOI-2267 c 0.1018 or 0.1214 3.4950 0.0263 or 0.0145 transit
TOI-2267 d 0.0875 or 0.1580 2.0345 0.0174 or 0.0145 transit
TOI-2407 b 0.380±0.023 2.703 0.033±0.001 705±12 transit 300.06 0.548±0.016 3,530±100 [60]
TOI-2427 c 0.02033 5.15±0.01 0.05±0.01 radial vel. 92.95 0.64±0.02 4,072±121 [61]
TOI-2431 b 0.020±0.004 0.137±0.003 0.224196 0.0063±0.0001 2,063±30 transit 117 0.661+0.021
−0.024 		4,109+28
−27 		Has one of the shortest orbital periods of any exoplanet. In just 31 million years the planet will have been destroyed.[62]
TOI-2449 b 0.7±0.04 1.0±0.01 106.1447 0.45±0.01 400 transit 505.5 1.079+0.045
−0.048 		6,021±62 Also known as NGTS-36 b.[63]
TOI-2969 b 1.16±0.04 1.1±0.08 1.8237146±0.0000002 0.0261±0.0002 1186 transit 530.0 0.71±0.02 4738±100 [64]
TOI-2989 b 3.0±0.2 1.12±0.05 3.122832±0.000001 0.0384±0.0003 1000 transit 635.7 0.77±0.02 4672±170 [64]
TOI-3493 b 0.0282+0.00368
−0.00377 		0.287±0.00714 8.1594667+0.0000016
−0.0000017 		1,102+20
−14 		transit 315.59±0.65 1.023±0.041 5,844±42 [65]
TOI-3495 b 0.3631 8.413073±0.000055 902 transit 562.2 1.42±0.17 6,400±230 [66]
TOI-4507 b <0.094 0.7333±0.0071 104.61595±0.00004 0.449±0.003 transit 580.6 1.15±0.07 6,235±100 [67]
TOI-5108 b 0.101±0.0157 0.589±0.00892 6.753 0.073±0.004 1,180±40 transit 427.6±2.0 1.10±0.03 5,808±40 [68]
TOI-5143 c 1.45+0.18
−0.12 		5.2097118+0.0000032
−0.0000039 		0.05602+0.00082
−0.00079 		transit 582.42±1.97 0.864+0.040
−0.033 		5,183±125 [69]
TOI-5300 b 0.6±0.1 0.88±0.08 2.262196±0.000003 0.0295±0.0003 1043 transit 530.6 0.67±0.02 4610±207 [64]
TOI-5349 b 0.40±0.02 0.91±0.02 3.317921 0.0369±0.0004 719±15 transit 620 0.61±0.02 3,751±59 [70]
TOI-5573 b 0.35±0.06 0.87±0.04 8.79759±0.00001 0.0712±0.0008 528 transit 606.0 0.619±0.023 3,790±59 [71]
TOI-5786 b 0.230±0.0283 0.762±0.0116 12.779 0.114±0.007 1,040±40 transit 632.1±1.6 1.23+0.04
−0.03 		6,235±50 [68]
TOI-5795 b 0.0744+0.0129
−0.0145 		0.5014±0.0098 6.140632±0.000005 0.064±0.002 1137 transit 526.7 0.901+0.055
−0.037 		5,715±55 [72]
TOI-5800 b 0.030±0.006 0.218±0.026 2.6279 0.0345±0.0014 1,108±20 transit 139.4±0.1 0.778+0.037
−0.032 		4,850±78 [73]
TOI-5817 b 0.03241+0.00441
−0.00409 		0.275±0.012 15.61 0.1223±0.0060 950+21
−18 		transit 262.0±0.5 0.970+0.072
−0.055 		5,770±50 [73]
TOI-6038 Ab 0.247+0.030
−0.031 		0.572+0.018
−0.014 		5.82673 0.0690+0.0012
−0.0011 		1,439+25
−24 		transit 577.9±2.0 1.291+0.066
−0.060 		6,110±100 The host star is part of a binary system with a K-type companion.[74]
TOI-6041 b <0.03401 0.4059±0.018 26.0494 0.1651±0.002 605 transit 236 0.89±0.04 5,417±50 [75]
TOI-6041 c 0.2451 88.0 0.3721±0.0067 403 radial vel.
TOI-6054 b 0.039±0.0053 0.2364±0.0134 7.501 0.0763±0.0048 1,360+35
−31 		transit 256.7±0.4 1.107±0.040 6,047±50 [76]
TOI-6054 c 0.0289±0.006 0.250±0.016 12.564 0.1077±0.0067 1,144+29
−26 		transit
TOI-6478 b 0.0311 0.411±0.021 34.005019±0.000025 0.1136±0.0060 204.4±4.9 transit 125.93±0.33 0.230±0.007 3,230±75 [77]
TOI-6695 b 0.21 0.85±0.02 80.4 0.402±0.002 599 transit 922 1.338 6,400 [78]
TOI-6695 c 1.45 242 0.838±0.005 415 radial vel.
TOI-6894 b 0.168±0.022 0.855±0.022 3.371 0.02604±0.00045 417.9±8.6 transit 237.96±0.95 0.207±0.011 3007±58 [79]
TOI-7149 b 0.705±0.075 1.180±0.045 2.652 0.026±0.00076 593±21 transit 415.0±2.4 0.344±0.030 3,363±59 [80]
TOI-7166 b 0.1793±0.0054 12.920636±0.000001 0.06191±0.00044 249 transit 114.9 0.19±0.004 3,099±51 Located in habitable zone.[81]
TOI-7510 b 0.0569±0.0053 0.651±0.018 11.5309 0.102±0.002 878 transit 789 1.02±0.03 5,820±80 [82]
TOI-7510 c 0.41±0.04 0.964±0.027 22.5687 0.159±0.003 702 transit
TOI-7510 d 0.56±0.04 0.94±0.03 48.8645 0.267±0.005 542 transit
WASP-154 b 0.626±0.129 0.96±0.06 3.811678±0.000001 0.044±0.003 994±63 transit 702.87±6.40 0.80±0.05 4,774±133 [83]
WASP-188 Ab 1.443+0.296
−0.298 		1.322±0.051 5.748916±0.000003 0.072±0.003 1,666±70 transit 2,202.47±31.55 1.50±0.09 6,850±125 [83]
WASP-195 b 0.104+0.03
−0.031 		0.92±0.05 5.051928±0.000004 0.063±0.003 1,522±71 transit 1,581.38±16.60 1.30±0.08 6,300±125 [83]
WASP-197 b 1.269±0.254 1.289±0.049 5.167228±0.000003 0.065±0.002 1,665±67 transit 1,577.54±40.08 1.36±0.08 6,050±100 [83]
WISPIT 1 b 10.4+0.7
−0.8 		338 imaging 747 4,670+990
−540[g] 		Circumbinary planets.[84]
WISPIT 1 c 5.3+0.8
−0.6 		840 imaging
WISPIT 2 b 5.3±1.0 1.6±0.2 15.0 imaging 435 1.08+0.06
−0.17 		4,400±50 [85][86]

Specific exoplanet lists

Lists of exoplanets

Lists of exoplanets by year of discovery


Notes

  1. ^ Sum of masses of the system
  2. ^ Temperature of component A
  3. ^ Calculated from R★ = 1.1303±0.0069 R☉ and a/R★ = 40.3+0.7
    −0.6    .
  4. ^ The mass of planet depends on its location, which is either galactic disk or galactic bulge
  5. ^ Sum of masses of the system
  6. ^ Temperature of component A
  7. ^ Temperature of component A

References

  1. ^ Lagrange, A.-M.; Kiefer, F.; Rubini, P.; Squicciarini, V.; Chomez, A.; Milli, J.; Zurlo, A.; Bouvier, J.; Delorme, P. (17 January 2025). "Searching for substellar companion candidates with Gaia. III. Search for companions to members of young associations". arXiv:2501.10488 [astro-ph.EP].
  2. ^ Ban, M.; et al. (45) (31 March 2025). "AT2021uey: A planetary microlensing event outside the Galactic bulge". Astronomy & Astrophysics. 697: A57. arXiv:2503.22331. Bibcode:2025A&A...697A..57B. doi:10.1051/0004-6361/202554236.
  3. ^ Basant, Ritvik; Luque, Rafael; et al. (March 2025). "Four Sub-Earth Planets Orbiting Barnard's Star from MAROON-X and ESPRESSO". The Astrophysical Journal Letters. 982 (1): L1. arXiv:2503.08095. Bibcode:2025ApJ...982L...1B. doi:10.3847/2041-8213/adb8d5.
  4. ^ "PPM 6653". SIMBAD. Centre de données astronomiques de Strasbourg.
  5. ^ Baycroft, Thomas A.; Santerne, Alexandre; Triaud, Amaury H. M. J.; Heidari, Neda; Sebastian, Daniel; Davis, Yasmin T.; Correia, Alexandre C. M.; Sairam, Lalitha; Freckelton, Alix V. (17 June 2025). "BEBOP VII. SOPHIE discovery of BEBOP-3b, a circumbinary giant planet on an eccentric orbit". Monthly Notices of the Royal Astronomical Society. 541 (3): 2801–2814. arXiv:2506.14615. Bibcode:2025MNRAS.541.2801B. doi:10.1093/mnras/staf1184.
  6. ^ Hon, Marc; Rappaport, Saul; Shporer, Avi; Vanderburg, Andrew; Collins, Karen A.; Watkins, Cristilyn N.; Schwarz, Richard P.; Barkaoui, Khalid; Yee, Samuel W. (9 January 2025). "A Disintegrating Rocky Planet with Prominent Comet-like Tails Around a Bright Star". The Astrophysical Journal. 984 (1): L3. arXiv:2501.05431. Bibcode:2025ApJ...984L...3H. doi:10.3847/2041-8213/adbf21.
  7. ^ Damian, Belinda; Scholz, Aleks; Jayawardhana, Ray; Almendros-Abad, V.; Flagg, Laura; Mužić, Koraljka; Natta, Antonella; Pinilla, Paola; Testi, Leonardo (2025). "Spectroscopy of Free-Floating Planetary-Mass Objects and their disks with JWST". The Astronomical Journal. 170 (2): 127. arXiv:2507.05155. Bibcode:2025AJ....170..127D. doi:10.3847/1538-3881/adea50.
  8. ^ a b c d Kaminski, A.; Sabotta, S.; Kemmer, J.; Chaturvedi, P.; Burn, R.; Morales, J. C.; Caballero, J. A.; Ribas, I.; Reiners, A.; Quirrenbach, A.; Amado, P. J.; Béjar, V. J. S.; Dreizler, S.; Guenther, E. W.; Hatzes, A. P.; Henning, Th.; Kürster, M.; Montes, D.; Nagel, E.; Pallé, E.; Pinter, V.; Reffert, S.; Schlecker, M.; Shan, Y.; Trifonov, T.; Zapatero Osorio, M. R.; Zechmeister, M. (8 April 2025). "The CARMENES search for exoplanets around M dwarfs". Astronomy & Astrophysics. 696: A101. arXiv:2504.03364. doi:10.1051/0004-6361/202453381.
  9. ^ Beard, Corey; Robertson, Paul; et al. (October 2025). "Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging". The Astronomical Journal. 170 (5): 279. arXiv:2510.19956. Bibcode:2025AJ....170..279B. doi:10.3847/1538-3881/ae0e20.
  10. ^ Carmona, A.; Delfosse, X.; et al. (4 April 2025). "Characterizing planetary systems with SPIRou: Detection of a sub-Neptune in a 6-day period orbit around the M dwarf Gl 410". Astronomy & Astrophysics. 700: A222. arXiv:2504.03572. Bibcode:2025A&A...700A.222C. doi:10.1051/0004-6361/202452513.
  11. ^ Suárez Mascareño, A.; Del Burgo, C.; Delisle, J.-B.; González Hernández, J.I.; Hara, N.C.; Mestre, J.M.; Nari, N.; Rebolo, R.; Stefanov, A.K.; Burt, J.A. (2025). "A second low-mass planet orbiting the nearby M-dwarf GJ 536". Astronomy & Astrophysics. 702: A121. arXiv:2509.03134. Bibcode:2025A&A...702A.121S. doi:10.1051/0004-6361/202555731.
  12. ^ Schorr, A.; Binnenfeld, A.; Zucker, S. (31 January 2025). "GJ 2126 b: A highly eccentric Jovian exoplanet". Astronomy & Astrophysics. 694: A210. arXiv:2502.11139. Bibcode:2025A&A...694A.210S. doi:10.1051/0004-6361/202452563. ISSN 0004-6361.
  13. ^ Stefanov, A. K.; Suárez Mascareño, A.; González Hernández, J. I.; Nari, N.; Rebolo, R.; Affer, L.; Micela, G.; Ribas, I.; Sozzetti, A.; Perger, M.; Pinamonti, M.; Damasso, M.; Maldonado, J.; González Álvarez, E.; Scandariato, G. (11 March 2025). "HADES RV Programme with HARPS-N at TNG XVI. A super-Earth in the habitable zone of the GJ 3998 multi-planet system". Astronomy and Astrophysics. 695. arXiv:2503.08405. Bibcode:2025A&A...695A..62S. doi:10.1051/0004-6361/202452630. Retrieved 13 March 2025.
  14. ^ a b Morales, J. C.; et al. (2025). "The CARMENES search for exoplanets around M dwarfs. Revisiting the GJ 317, GJ 463, and GJ 3512 systems and two newly discovered planets orbiting GJ 9773 and GJ 508.2". Astronomy and Astrophysics. 700. arXiv:2507.15516. Bibcode:2025A&A...700A.242M. doi:10.1051/0004-6361/202554992.
  15. ^ Lienhard, F.; et al. (11 November 2025). "HARPS-N, TESS, and CHEOPS discover a transiting sub-Neptune and two outer companions around the bright solar analogue HD 85426". arXiv:2511.08473 [astro-ph.EP].
  16. ^ a b c Fontanet, E.; Udry, S. (May 2025). "CORALIE radial-velocity search for companions around evolved stars (CASCADES) IV: New planetary systems around HD 87816, HD 94890, and HD 102888 and an update on HD 121056". Astronomy and Astrophysics. 699. arXiv:2505.14317. Bibcode:2025A&A...699A..38F. doi:10.1051/0004-6361/202554137.
  17. ^ Stolker, T.; et al. (2025). "Direct imaging discovery of a young giant planet orbiting on Solar System scales". Astronomy and Astrophysics. 700: A21. arXiv:2507.06206. Bibcode:2025A&A...700A..21S. doi:10.1051/0004-6361/202555064.
  18. ^ Jones, Nathalie K.; et al. (2025). "HD 143811 AB b: A Directly Imaged Planet Orbiting a Spectroscopic Binary in Sco-Cen". The Astrophysical Journal Letters. 995 (2): L41. arXiv:2509.06729. Bibcode:2025ApJ...995L..41J. doi:10.3847/2041-8213/ae2007.
  19. ^ Damasso, M.; Naponiello, L.; Anna John, A.; Egger, J. A.; Cretignier, M.; Mortier, A.; Bonomo, A. S.; Collier Cameron, A.; Dumusque, X.; Wilson, T.; Buchhave, L.; Nicholson, B.; Stalport, M.; Ghedina, A.; Latham, D. W.; Livingston, J.; Malavolta, L.; Sozzetti, A.; Jenkins, J. M.; Mantovan, G.; Martínez Fiorenzano, A. F.; Palethorpe, L.; Tronsgaard, R.; Udry, S.; Watson, C. A. (2025). "Discovery of a multi-planet system orbiting the aged Sun-like star HD 224018". Astronomy & Astrophysics. 702: A118. arXiv:2508.13684. Bibcode:2025A&A...702A.118D. doi:10.1051/0004-6361/202555770.
  20. ^ Currie, Thayne; Li, Yiting; et al. (1 December 2025). "SCExAO/CHARIS and Gaia Direct Imaging and Astrometric Discovery of a Superjovian Planet 3─4 λ/D from the Accelerating Star HIP 54515". arXiv:2512.02159 [astro-ph.EP].
  21. ^ Bonomo, A. S.; et al. (2025). "The GAPS programme at TNG XYZ. A sub-Neptune suitable for atmospheric characterization in a multiplanet and mutually inclined system orbiting the bright K dwarf TOI-5789 (HIP 99452)". arXiv:2510.11490 [astro-ph.EP].
  22. ^ a b c Bouy, H.; Duchêne, G.; Strampelli, G.; Aguilar, J.; Olivares, J.; Barrado, D.; Raymond, S. N.; Huélamo, N.; Tamura, M.; Bertin, E.; Brandner, W.; Cuillandre, J. -C.; Galli, P. A. B.; Miret-Roig, N. (2025). "Multiplicity of young isolated planetary mass objects in Taurus and Upper Scorpius". arXiv:2506.14380 [astro-ph.SR].
  23. ^ Castro-González, A.; et al. (2025). "Two neighbours of the ultra-short-period Earth-sized planet K2-157 b in the warm Neptunian savanna". Astronomy & Astrophysics. 699: A344. arXiv:2504.20999. Bibcode:2025A&A...699A.344C. doi:10.1051/0004-6361/202554736.
  24. ^ Lammers, Caleb; Winn, Joshua N. (17 April 2025). "Discovery and Dynamics of the Nontransiting Planet Kepler-139f". The Astrophysical Journal. 984 (2): L39. arXiv:2504.13160. Bibcode:2025ApJ...984L..39L. doi:10.3847/2041-8213/adce01.
  25. ^ a b Ofir, Aviv; Yoffe, Gideon; Aharonson, Oded (21 January 2025). "Planetary Mass Determinations from a Simplified Photodynamical Model—Application to the Complete Kepler Dataset". The Astronomical Journal. 169 (2): 90. arXiv:2410.11401. Bibcode:2025AJ....169...90O. doi:10.3847/1538-3881/ad91a7.
  26. ^ Sun, L.; Gu, S.; Wang, X.; Schmitt, J. H. M. M.; Ioannidis, P.; Kouwenhoven, M. B. N.; Dou, J.; Zhao, G. (June 2025). "A temperate 10-Earth-mass exoplanet around the Sun-like star Kepler-725". nature. 9 (8): 1184–1194. Bibcode:2025NatAs...9.1184S. doi:10.1038/s41550-025-02565-z.
  27. ^ a b c d Han, Cheongho; Albrow, Michael D. (2 May 2025). "Four Planets Found through Microlensing Events Involving Faint Source Stars". The Astronomical Journal. 169 (6): 288. Bibcode:2025AJ....169..288H. doi:10.3847/1538-3881/adc5e7. ISSN 0004-6256.
  28. ^ a b Yang, Hongjing; Yee, Jennifer C.; Zhang, Jiyuan; Lee, Chung-Uk; Kim, Dong-Jin; Bond, Ian A.; Udalski, Andrzej; Hwang, Kyu-Ha; Zang, Weicheng; Qian, Qiyue; Gould, Andrew; Mao, Shude (26 March 2025). "Systematic Reanalysis of KMTNet Microlensing Events. II. Two New Planets in Giant-source Events". The Astronomical Journal. 169 (6): 295. arXiv:2503.19471. Bibcode:2025AJ....169..295Y. doi:10.3847/1538-3881/adc73e.
  29. ^ Li, Hongyu; et al. (2025). "KMT-2022-BLG-1818Lb,c: A Cold Super-Jupiter with a Saturn Sibling". The Astronomical Journal. 171 (1): 41. arXiv:2505.05093. Bibcode:2026AJ....171...41L. doi:10.3847/1538-3881/ae1b8f.
  30. ^ a b c Han, Cheongho; Bond, Ian A.; Jung, Youn Kil; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew; Hwang, Kyu-Ha; Lee, Chung-Uk; Ryu, Yoon-Hyun (4 January 2025). "MOA-2022-BLG-033Lb, KMT-2023-BLG-0119Lb, and KMT-2023-BLG-1896Lb: Three low mass-ratio microlensing planets detected through dip signals". Astronomy and Astrophysics. 694: A90. arXiv:2501.02193. Bibcode:2025A&A...694A..90H. doi:10.1051/0004-6361/202452027.
  31. ^ a b c d Han, Cheongho; Udalski, Andrzej; Bond, Ian A.; Lee, Chung-Uk; Zhang, Jiyuan; et al. (10 December 2025). "Four Giant Planets from 2024 KMTNet Microlensing Campaign". arXiv:2512.09325 [astro-ph.EP].
  32. ^ Han, Cheongho; et al. (9 July 2025). "KMT-2024-BLG-0404L: A triple microlensing system consisting of a star, a brown dwarf, and a planet". Astronomy and Astrophysics. 700: A181. arXiv:2507.07326. Bibcode:2025A&A...700A.181H. doi:10.1051/0004-6361/202452760.
  33. ^ a b Han, Cheongho; Lee, Chung-Uk; Udalski, Andrzej; Bond, Ian A.; Yang, Hongjing; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew; Jung, Youn Kil (29 May 2025), "MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals", Astronomy and Astrophysics, 699: A91, arXiv:2505.22951, Bibcode:2025A&A...699A..91H, doi:10.1051/0004-6361/202554182
  34. ^ Balsalobre-Ruza, O.; Lillo-Box, J.; Silva, A. M.; Grouffal, S.; Aceituno, J.; Castro-González, A.; Cifuentes, C.; Standing, M. R.; Faria, J. P. (3 February 2025), "KOBE-1: The first planetary system from the KOBE survey", Astronomy & Astrophysics, 694: A15, arXiv:2502.01249, doi:10.1051/0004-6361/202452631
  35. ^ Nabbie, Emma; Huang, Chelsea X.; Korth, Judith; Parviainen, Hannu; Wang, Su; Venner, Alexander; Wittenmyer, Robert; Bieryla, Allyson; Latham, David W.; Li, Gongjie; Lin, Douglas N. C.; Zhou, George (27 June 2025). "A high mutual inclination system around KOI-134 revealed by transit timing variations". Nature Astronomy. 9 (9): 1317–1325. arXiv:2507.02238. Bibcode:2025NatAs...9.1317N. doi:10.1038/s41550-025-02594-8. ISSN 2397-3366.
  36. ^ Walker, Samuel A. U.; Liu, Michael C.; Mawet, Dimitri; Bond, Charlotte; Chun, Mark; Martinez, Raquel A.; Phillips, Mark W.; Williams, Jonathan P.; Zhang, Zhoujian; Ren, Bin B.; Stapelfeldt, Karl; Uyama, Taichi; Wallack, Nicole (2026). "Keck Observations in the INfrared of Taurus and ρ Oph Exoplanets and Ultracool Dwarfs (KOINTREAU) I: A Planetary-mass Companion and a Disk-obscured Stellar Companion Discovered in Taurus". The Astronomical Journal. 171 (2): 80. arXiv:2512.05191. Bibcode:2026AJ....171...80W. doi:10.3847/1538-3881/ae267f.
  37. ^ Schwarz, Paul; Dreizler, Stefan; Heller, René (8 July 2025). "Confirmation of a non-transiting planet in the habitable zone of the nearby M dwarf L 98-59". arXiv:2507.06413 [astro-ph.EP].
  38. ^ Ribas, Álvaro; Vioque, Miguel; Zagaria, Francesco; Longarini, Cristiano; MacÍas, Enrique; Clarke, Cathie J.; Pérez, Sebastián; Carpenter, John; Cuello, Nicolás; De Gregorio-Monsalvo, Itziar (2025). "A young gas giant and hidden substructures in a protoplanetary disk". Nature Astronomy. 9 (8): 1176–1183. arXiv:2507.11612. Bibcode:2025NatAs...9.1176R. doi:10.1038/s41550-025-02576-w. PMC 12360948. PMID 40837857.
  39. ^ Delisle, J. -B.; Faria, J. P.; Ségransan, D.; Fontanet, E.; Ceva, W.; Barbato, D.; Sousa, S. G.; Unger, N.; Leleu, A.; Bouchy, F.; Cretignier, M.; Díaz, R. F.; Dumusque, X.; Frensch, Y. G. C.; Hara, N. C.; Laughlin, G.; Lo Curto, G.; Lovis, C.; Marmier, M.; Mayor, M.; Mignon, L.; Mordasini, C.; Pepe, F.; Santos, N. C.; Udry, S. (2025). "Architecture of planetary systems with and without outer giant planets I. Inner planet detections around HD 23079, HD 196067, and HD 86226". Astronomy and Astrophysics. 703. arXiv:2509.26232. Bibcode:2025A&A...703A..78D. doi:10.1051/0004-6361/202555445.
  40. ^ Weicheng, Zang; Youn Kil, Jung (2025). "Microlensing events indicate that super-Earth exoplanets are common in Jupiter-like orbits". Science. 388 (6745): 400–404. arXiv:2504.20158. Bibcode:2025Sci...388..400Z. doi:10.1126/science.adn6088. PMID 40273242.
  41. ^ Kapusta, Mateusz; et al. (2025). "HST pre-imaging of a free-floating planet candidate microlensing event". arXiv:2507.01109 [astro-ph.EP].
  42. ^ a b Tu, Zhijun; Wang, Shu; Chen, Xiaodian; Liu, Jifeng (2025). "Three Brown Dwarfs Masquerading as High-Redshift Galaxies in JWST Observations". The Astrophysical Journal. 980 (2): 230. arXiv:2501.16648. Bibcode:2025ApJ...980..230T. doi:10.3847/1538-4357/adaf9f.
  43. ^ Geraldía-González, S.; et al. (2025). "Discovery of a transiting hot water-world candidate orbiting Ross 176 with TESS and CARMENES". Astronomy & Astrophysics. 700: A216. arXiv:2507.15763. Bibcode:2025A&A...700A.216G. doi:10.1051/0004-6361/202553719.
  44. ^ Vach, Sydney; et al. (1 February 2025). "A 16 Myr super-Neptune in Upper-Centaurus Lupus and a preliminary survey of transiting planets in Sco-Cen with TESS". The Astronomical Journal. 170 (2): 131. arXiv:2502.00576. Bibcode:2025AJ....170..131V. doi:10.3847/1538-3881/ade67f.
  45. ^ Maciejewski, Gracjan; Łoboda, Weronika (2025). "A Transiting Giant on a 7.7 yr Orbit Revealed by Transit Timing Variations in the TOI-201 System". The Astrophysical Journal Letters. 988 (2): L63. arXiv:2507.11504. Bibcode:2025ApJ...988L..63M. doi:10.3847/2041-8213/adefe5.
  46. ^ Alves, Douglas R.; et al. (2026). "TOI-333b: A Neptune-desert planet around an F7V star". Astronomy & Astrophysics. 705: A210. arXiv:2511.13832. Bibcode:2026A&A...705A.210A. doi:10.1051/0004-6361/202557014.
  47. ^ Reinarz, Y.; et al. (February 2026). "A transiting hot Jupiter with two outer siblings orbiting an intermediate-mass post-main-sequence star". Astronomy & Astrophysics. 706 A20. arXiv:2509.26430. Bibcode:2026A&A...706A..20R. doi:10.1051/0004-6361/202557200.
  48. ^ Rodrigues, J.; et al. (20 February 2025). "TOI-512: Super-Earth transiting a K-type star discovered by TESS and ESPRESSO". Astronomy and Astrophysics. 695: A237. arXiv:2502.14472. Bibcode:2025A&A...695A.237R. doi:10.1051/0004-6361/202452887.
  49. ^ Lacedelli, G.; Pallé, E.; Davis, Y. T.; Luque, R.; Morello, G.; Tabernero, H. M.; Zapatero Osorio, M. R.; Pozuelos, F. J.; Jankowski, D.; Nowak, G.; Murgas, F.; Orell-Miquel, J.; Akana Murphy, J. M.; Barkaoui, K.; Charbonneau, D.; Dransfield, G.; Ducrot, E.; Geraldía-González, S.; Irwin, J.; Jehin, E.; Osborne, H. L. M.; Pedersen, P. P.; Rackham, B. V.; Scott, M. G.; Timmermans, M.; Triaud, A.; Van Eylen, V. (2025). "A transiting rocky super-Earth and a non-transiting sub-Neptune orbiting the M dwarf TOI-771". Astronomy & Astrophysics. 698: A223. arXiv:2504.18223. Bibcode:2025A&A...698A.223L. doi:10.1051/0004-6361/202554161.
  50. ^ Lockley, Isobel S.; Armstrong, David J.; Fernández, Jorge Fernández; Millholland, Sarah; Knierim, Henrik; Mena, Elisa Delgado; Sousa, Sergio; Collins, Karen A.; Watkins, Cristilyn N.; Howell, Steve B.; Adibekyan, Vardan; Helled, Ravit; Ziegler, Carl; Bayliss, Daniel; Briceño, César (June 2025). "The TOI-1117 Multi-planetary System: 3 sub-Neptunes, 1 in both the Neptunian Desert and Radius Valley". Monthly Notices of the Royal Astronomical Society. 541 (2): 919–938. arXiv:2506.05521. Bibcode:2025MNRAS.541..919L. doi:10.1093/mnras/staf939. ISSN 0035-8711.
  51. ^ Gandolfi, D.; et al. (12 September 2025). "A four-planet system orbiting the old thick disk star TOI-1203". arXiv:2509.10136 [astro-ph.EP].
  52. ^ Stalport, M.; Mortier, A.; Cretignier, M.; Egger, J. A.; Malavolta, L.; Latham, D. W.; Collins, K. A.; Watkins, C. N.; Murgas, F.; Buchhave, L. A.; López-Morales, M.; Udry, S.; Quinn, S. N.; Silva, A. M.; Andreuzzi, G.; Baker, D.; Boschin, W.; Ciardi, D. R.; Damasso, M.; Di Fabrizio, L.; Dumusque, X.; Fukui, A.; Haywood, R.; Howell, S. B.; Jenkins, J. M.; Leleu, A.; Lewin, P.; Lillo-Box, J.; Martínez-Fiorenzano, A. F.; Narita, N.; Pedani, M.; Pinamonti, M.; Poretti, E.; Schwarz, R. P.; Seager, S.; Sozzetti, A.; Ting, E. B.; Vanderburg, A.; Winn, J. N.; Ziegler, C. (10 March 2025). "TESS and HARPS-N unveil two planets transiting TOI-1453. A super-Earth and one of the lowest mass sub-Neptunes". Astronomy & Astrophysics. 696. arXiv:2503.07529. Bibcode:2025A&A...696A..86S. doi:10.1051/0004-6361/202452969.
  53. ^ Soubkiou, Abderahmane; Barkaoui, Khalid; Benkhaldoun, Zouhair; Ghachoui, Mourad; Chouqar, Jamila; Rackham, Benjamin V.; Burgasser, Adam; Softich, Emma; Pallé, Enric (23 June 2025). "TOI-1846b: A super-Earth in the radius valley orbiting a nearby M dwarf". Monthly Notices of the Royal Astronomical Society. 541 (4): 3249–3268. arXiv:2506.18550. Bibcode:2025MNRAS.541.3249S. doi:10.1093/mnras/staf1030.
  54. ^ Bieryla, Allyson; et al. (39) (27 March 2025). "TOI-2005b: An Eccentric Warm Jupiter in Spin-orbit Alignment". The Astronomical Journal. 169 (5): 273. arXiv:2503.20069. Bibcode:2025AJ....169..273B. doi:10.3847/1538-3881/adc441.
  55. ^ Barkaoui, K.; et al. (10 February 2025). "TOI-2015b: a sub-Neptune in strong gravitational interaction with an outer non-transiting planet". Astronomy and Astrophysics. 695: A281. arXiv:2502.07074. Bibcode:2025A&A...695A.281B. doi:10.1051/0004-6361/202452916.
  56. ^ Jones, Sinclaire E.; et al. (9 May 2024). "TOI-2015b: A Warm Neptune with Transit Timing Variations Orbiting an Active mid M Dwarf". arXiv:2310.11775 [astro-ph.EP].
  57. ^ Barber, Madyson G.; Mann, Andrew W.; Vanderburg, Andrew; Boyle, Andrew W.; Ana Isabel Lopez Murillo (2025). "TESS Investigation -- Demographics of Young Exoplanets (TI-DYE) III: an inner super-Earth in TOI-2076". The Astronomical Journal. 170 (1): 32. arXiv:2505.06358. Bibcode:2025AJ....170...32B. doi:10.3847/1538-3881/add7db.
  58. ^ Zúñiga-Fernández, S.; et al. (2025). "Two warm Earth-sized exoplanets and an Earth-sized candidate in the M5V-M6V binary system TOI-2267". Astronomy & Astrophysics. 702: A85. arXiv:2508.14176. Bibcode:2025A&A...702A..85Z. doi:10.1051/0004-6361/202554419.
  59. ^ Greklek-McKeon, Michael; Jonathan Gomez Barrientos; Knutson, Heather A.; Zúñiga-Fernández, Sebastián; Pozuelos, Francisco J.; Saidel, Morgan; Garrett Levine, W.; Hu, Renyu; Dai, Fei; Daylan, Tansu; Doty, John P.; Rodriguez, David R.; Twicken, Joseph D.; Latham, David W.; Jenkins, Jon M.; Schwarz, Richard P. (2025). "Validation of a Third Earth-sized Planet in the TOI-2267 Binary System". The Astronomical Journal. 171 (2): 97. arXiv:2512.10007. Bibcode:2026AJ....171...97G. doi:10.3847/1538-3881/ae2be9.
  60. ^ Janó Muñoz, C.; Hooton, M. J.; Pedersen, P. P.; Barkaoui, K.; Rackham, B. V.; Burgasser, A. J.; Pozuelos, F. J.; Stassun, K. G.; Queloz, D.; Triaud, A. H. M. J.; Ziegler, C.; Almenara, J. M.; Timmermans, M.; Bonfils, X.; Collins, K. A. (June 2025). "TOI-2407 b: a warm Neptune in the desert". Monthly Notices of the Royal Astronomical Society. 541 (1): 630–641. arXiv:2506.05521. Bibcode:2025MNRAS.541..630J. doi:10.1093/mnras/staf946. ISSN 0035-8711.
  61. ^ Schmerling, H.; Goffo, E.; Grziwa, S.; Persson, C. M.; Gandolfi, D.; Pätzold, M.; Hatzes, A.; Hellier, C.; Livingston, J.; Acuña, L.; Aguichine, A.; Costanza, E.; Deeg, H. J.; Masseron, T.; Palle, E.; Cochran, W.; Nowak, G.; Jankowski, D.; Goździewski, K.; Luque, R.; Mathur, S.; Palakkatharappil, D. B.; García, R. A. (2025). "The TOI-2427 system: Two close-in planets orbiting a late K-dwarf star". Astronomy & Astrophysics. 699: A185. Bibcode:2025A&A...699A.185S. doi:10.1051/0004-6361/202452620.
  62. ^ Kaya Han Taş; Stefansson, Gudmundur; Fariz, Syarief N. M.; Garg, Esha; Espinoza-Retamal, Juan I.; Koo, Elise; Bruijne, David; Luhn, Jacob; Ford, Eric B.; Mahadevan, Suvrath; Logsdon, Sarah E.; Cañas, Caleb I.; Han, Te; Everett, Mark E.; Alvarado-Montes, Jaime A.; Blake, Cullen; Cochran, William D.; Dong, Jiayin; Fernandes, Rachel B.; Giovinazzi, Mark R.; Halverson, Samuel; Kanodia, Shubham; Krolikowski, Daniel; McElwain, Michael; Ninan, Joe; Paredes, Leonardo A.; Robertson, Paul; Schwab, Christian (2025). "An Earth-Sized Planet in a 5.4h Orbit Around a Nearby K dwarf". arXiv:2507.08464 [astro-ph.EP].
  63. ^ Ulmer-Moll, S.; et al. (2025). "Detection and characterisation of a 106-day transiting Jupiter: TOI-2449 b/NGTS-36 B". Astronomy & Astrophysics. 703: A258. arXiv:2509.15424. Bibcode:2025A&A...703A.258U. doi:10.1051/0004-6361/202555168.
  64. ^ a b c Frensch, Y. G. C.; et al. (2025). "Three hot Jupiters transiting K-dwarfs with significant heavy element masses". Astronomy & Astrophysics. 700: A118. arXiv:2506.04923. Bibcode:2025A&A...700A.118F. doi:10.1051/0004-6361/202553879.
  65. ^ Chaturvedi, P.; Goffo, E.; Gandolfi, D.; Persson, C. M.; Hatzes, A. P.; Nowak, G.; Bonfanti, A.; Bieryla, A.; Cochran, W. D.; Collins, K. A.; Fajardo-Acosta, S. B.; Howell, S. B.; Jenkins, J. M.; Korth, J.; Livingston, J.; Pallé, E.; Quinn, S. N.; Schwarz, R. P.; Seager, S.; Shporer, A.; Stassun, K. G.; Striegel, S.; Van Eylen, V.; Watkins, C. N.; Winn, J. N.; Ziegler, C. (17 April 2025). "TOI-3493 b: A planet with a Neptune-like density transiting a bright G0-type star". Astronomy and Astrophysics. 697: A169. arXiv:2504.12884. Bibcode:2025A&A...697A.169C. doi:10.1051/0004-6361/202453511.
  66. ^ Fairnington, Tyler R.; et al. (2025). "The Eccentricity Distribution of Warm Sub-Saturns in TESS". Monthly Notices of the Royal Astronomical Society. 540 (1): 1144. arXiv:2505.04106. Bibcode:2025MNRAS.540.1144F. doi:10.1093/mnras/staf759.
  67. ^ Espinoza-Retamal, Juan I.; et al. (2026). "A Cold and Superpuffy Planet on a Prograde Orbit". The Astrophysical Journal Letters. 996 (1): L13. arXiv:2510.00102. Bibcode:2026ApJ...996L..13E. doi:10.3847/2041-8213/ae2bfa.
  68. ^ a b Thomas, Luis; et al. (47) (7 January 2025). "TOI-5108 b and TOI 5786 b: Two transiting sub-Saturns detected and characterized with TESS, MaHPS, and SOPHIE". Astronomy & Astrophysics. 694: A143. arXiv:2501.03803. Bibcode:2025A&A...694A.143T. doi:10.1051/0004-6361/202451676.
  69. ^ Radzom, Brandon T.; Dong, Jiayin; Rice, Malena; Wang, Xian-Yu; Hixenbaugh, Kyle; Zhou, George; Huang, Chelsea X.; Wang, Songhu (3 March 2025). "Evidence for Primordial Alignment II: Insights from Stellar Obliquity Measurements for Hot Jupiters in Compact Multiplanet Systems". The Astronomical Journal. 169 (3): 189. arXiv:2503.03745. Bibcode:2025AJ....169..189R. doi:10.3847/1538-3881/ad9dd5.
  70. ^ Sandoval, Angeli; et al. (23 September 2025). "Searching for GEMS: TOI-5349b is a Saturn-like planet orbiting a metal-rich early M-dwarf". arXiv:2509.19492 [astro-ph.EP].
  71. ^ Rachel B Fernandes; et al. (2025). "Searching for GEMS: Confirmation of TOI-5573b, a Cool, Saturn-like Planet Orbiting An M-dwarf". The Astronomical Journal. 170 (1): 55. arXiv:2505.08947. Bibcode:2025AJ....170...55F. doi:10.3847/1538-3881/addc51.
  72. ^ Manni, F.; et al. (2025). "The Hot Neptune Initiative (HONEI) II. TOI-5795 b: A hot super-Neptune orbiting a metal-poor star". Astronomy and Astrophysics. 701. arXiv:2507.23413. Bibcode:2025A&A...701A.230M. doi:10.1051/0004-6361/202556081.
  73. ^ a b Naponiello, L.; Vissapragada, S.; Bonomo, A. S.; Steinmeyer, M.-L.; Filomeno, S.; D'Orazi, V.; Dorn, C.; Sozzetti, A.; Mancini, L. (15 May 2025). "The Hot-Neptune Initiative (HONEI). I. Two hot sub-Neptunes on a close-in eccentric orbit (TOI-5800b) and a farther-out circular orbit (TOI-5817b)". Astronomy & Astrophysics. 701: A79. arXiv:2505.10123. Bibcode:2025A&A...701A..79N. doi:10.1051/0004-6361/202555523.
  74. ^ Baliwal, Sanjay; Sharma, Rishikesh; Chakraborty, Abhijit; Nikitha, K. J.; Castro-González, A.; Bhaskar, Hareesh G.; Khandelwal, Akanksha; Latham, David W.; Bieryla, Allyson (4 January 2025). "TOI-6038 A b: A dense sub-Saturn in the transition regime between the Neptunian ridge and savanna". The Astronomical Journal. 169 (3): 147. arXiv:2501.02272. Bibcode:2025AJ....169..147B. doi:10.3847/1538-3881/ada959.
  75. ^ Heidari, N.; et al. (December 2025). "Giant Outer Transiting Exoplanet Mass (GOTEM) Survey.VII. TOI-6041: a multi-planet system including a warm Neptune exhibiting strong TTVs". arXiv:2512.01911 [astro-ph.EP].
  76. ^ Kroft, Maxwell; Beatty, Thomas G.; Crossfield, Ian J. M.; Livesey, Joseph R.; Becker, Juliette; Luhn, Jacob K.; Robertson, Paul; Bieryla, Allyson; Ciardi, David R. (15 January 2025). "A Pair of Dynamically Interacting Sub-Neptunes Around TOI-6054". The Astronomical Journal. 170 (3): 150. arXiv:2501.09095. Bibcode:2025AJ....170..150K. doi:10.3847/1538-3881/adee24.
  77. ^ Scott, Madison G.; Triaud, Amaury H. M. J.; Barkaoui, Khalid; Sebastian, Daniel; Burgasser, Adam J.; Collins, Karen A.; Dransfield, Georgina; Hellier, Coel; Howell, Steve B.; Piette, Anjali A. A.; Rackham, Benjamin V.; Stassun, Keivan G.; Stokholm, Amalie; Timmermans, Mathilde; Watkins, Cristilyn N.; Fausnaugh, Michael; Fukui, Akihiko; Jenkins, Jon M.; Narita, Norio; Ricker, George; Softich, Emma; Schwarz, Richard P.; Seager, Sara; Shporer, Avi; Theissen, Christopher; Twicken, Joseph D.; Winn, Joshua N.; Watanabe, David (9 April 2025). "TOI-6478 b: a cold under-dense Neptune transiting a fully convective M dwarf from the thick disc". Monthly Notices of the Royal Astronomical Society. 540 (2): 1909–1927. arXiv:2504.06848. Bibcode:2025MNRAS.540.1909S. doi:10.1093/mnras/staf684.
  78. ^ Eberhardt, Jan; Trifonov, Trifon (2025). "TOI-6695: A Pair of Near-resonant Massive Planets Observed with TESS from the WINE Survey". The Astronomical Journal. 169 (6): 298. arXiv:2504.20999. Bibcode:2025AJ....169..298E. doi:10.3847/1538-3881/adc44e.
  79. ^ Bryant, Edward M.; Jordán, Andrés; Hartman, Joel D.; Bayliss, Daniel; Sedaghati, Elyar; Barkaoui, Khalid; Chouqar, Jamila; Pozuelos, Francisco J.; Thorngren, Daniel P.; Timmermans, Mathilde; Almenara, Jose Manuel; Chilingarian, Igor V.; Collins, Karen A.; Gan, Tianjun; Howell, Steve B. (June 2025). "A transiting giant planet in orbit around a 0.2-solar-mass host star". Nature Astronomy. 9 (7): 1031–1044. arXiv:2506.07931. Bibcode:2025NatAs...9.1031B. doi:10.1038/s41550-025-02552-4. ISSN 2397-3366. PMC 12274134. PMID 40687772.
  80. ^ Kanodia, Shubham; Cañas, Caleb I.; Mahadevan, Suvrath; Lin, Andrea S. J.; Kobulnicky, Henry A.; Karfs, Ian; Birkholz, Alexina; Gupta, Arvind; Everett, Mark (2025). "Searching for GEMS: TOI-7149~b an Inflated Giant Planet causing a 12% Transit of a Fully Convective M-dwarf". The Astronomical Journal. 170 (4): 203. arXiv:2506.17861. Bibcode:2025AJ....170..203K. doi:10.3847/1538-3881/adf6db.
  81. ^ Barkaoui, Khalid; et al. (2025). "TOI-7166 b: A Habitable Zone mini-Neptune planet around a nearby low-mass star". Monthly Notices of the Royal Astronomical Society. 544 (2): 2637–2652. arXiv:2512.06841. doi:10.1093/mnras/staf1807.
  82. ^ Almenara, J.M.; Leleu, A.; Guillot, T.; Mardling, R.; Bouchy, F.; Forveille, T.; Winn, J.; Abe, L.; Beltrame, M.; Bendjoya, P.; Bonfils, X.; Deline, A.; Delisle, J.-B.; Díaz, R.F.; Fridén, E.; Hobson, M.; Hoogenboom, R.M.; Jenkins, J.M.; Korth, J.; Lendl, M.; Mékarnia, D.; Petit, A.C.; Rosenqvist, M.; Suárez, O.; Triaud, A.H.M.J.; Udry, S. (2025). "TOI-7510: A solar-analog system of three transiting giant planets near a Laplace resonance chain". Astronomy & Astrophysics. 704: L16. arXiv:2511.20074. Bibcode:2025A&A...704L..16A. doi:10.1051/0004-6361/202557359.
  83. ^ a b c d Schanche, N.; et al. (55) (10 April 2025). "A Swarm of WASP Planets: Nine giant planets identified by the WASP survey". The Astronomical Journal. 169 (6): 334. arXiv:2504.08091. Bibcode:2025AJ....169..334S. doi:10.3847/1538-3881/adccc6.
  84. ^ van Capelleveen, Richelle F.; et al. (December 2025). "WIde Separation Planets In Time (WISPIT): Two directly imaged exoplanets around the Sun-like stellar binary WISPIT 1". Astronomy and Astrophysics. 704 A221. arXiv:2508.18456. Bibcode:2025A&A...704A.221V. doi:10.1051/0004-6361/202556584. S2CID 280870673.
  85. ^ Close, Laird M.; et al. (2025). "Wide Separation Planets In Time (WISPIT): Discovery of a Gap Hα Protoplanet WISPIT 2b with MagAO-X". The Astrophysical Journal. 990 (1): L9. arXiv:2508.19046. Bibcode:2025ApJ...990L...9C. doi:10.3847/2041-8213/adf7a5.
  86. ^ Van Capelleveen, Richelle F.; Ginski, Christian; Kenworthy, Matthew A.; Byrne, Jake; Lawlor, Chloe; McLachlan, Dan; Mamajek, Eric E.; Stolker, Tomas; Benisty, Myriam; Bohn, Alexander J.; Close, Laird M.; Dominik, Carsten; Haffert, Sebastiaan; Landman, Rico; Ma, Jie; Snellen, Ignas; Tazaki, Ryo; Van Der Marel, Nienke; Welzel, Lukas; Zhang, Yapeng (2025). "WIde Separation Planets in Time (WISPIT): A Gap-clearing Planet in a Multi-ringed Disk around the Young Solar-type Star WISPIT 2". The Astrophysical Journal Letters. 990 (1): L8. arXiv:2508.19053. Bibcode:2025ApJ...990L...8V. doi:10.3847/2041-8213/adf721.
This article is issued from Wikipedia. The text is available under Creative Commons Attribution-Share Alike 4.0 unless otherwise noted. Additional terms may apply for the media files.