List of exoplanets discovered in 2026
Appearance
This list of exoplanets discovered in 2026 is a list of confirmed exoplanets and exoplanet candidates 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 | Planet status | Distance (ly) | Host star mass (M☉) | Host star temp. (K) | Remarks |
|---|---|---|---|---|---|---|---|---|---|---|---|
| AB Aurigae d | 20 | 65 | 550 | imaging | Candidate | 508.6 | 2.4 | 25 | Candidate into planet.[1] | ||
| DMPP-2c | 0.1629+0.0171 −0.0173 |
0.737 | 3.168+0.355 −0.002 |
0.04789+0.00327 −0.00049 |
radial vel. | Confirmed | 443 | 1.41±0.04 | 6,500±100 | [2] | |
| DMPP-2d | 0.2888+0.0192 −0.0230 |
1.03 | 16.491+0.067 −0.053 |
0.1432+0.0012 −0.0013 |
radial vel. | Confirmed | [2] | ||||
| DMPP-6b | 0.0182+0.0030 −0.0025 |
0.203 | 7.6027+0.0261 −0.0016 |
0.00779+0.0016 −0.0012 |
radial vel. | Confirmed | 178 | 1.079±0.045 | [2] | ||
| DMPP-6c | 0.0424+0.0050 −0.0062 |
0.334 | 36.441+0.077 −0.070 |
0.2206+0.0033 −0.0039 |
radial vel. | Confirmed | [2] | ||||
| DMPP-7b | 0.1932+0.0136 −0.0128 |
0.815 | 4.984+0.069 −0.061 |
0.05873+0.00086 −0.00089 |
radial vel. | Confirmed | 333 | 1.09±0.04 | [2] | ||
| DMPP-8b | 0.2551±0.0223 | 0.96 | 62.915+0.041 −0.033 |
0.3098+0.0098 −0.0108 |
radial vel. | Confirmed | 248 | 0.99±0.04 | [2] | ||
| DMPP-9b | 0.0454+0.0081 −0.0074 |
0.347 | 12.733+0.584 −0.524 |
0.1097+0.0041 −0.0037 |
radial vel. | Confirmed | 359 | 1.10±0.04 | [2] | ||
| DO Tauri b | 2.8±0.6 | 21.14±0.2 | 10.12±0.01 | radial vel. | Candidate | 1451.8 | 10.54±0.07 | 3450±50 | Candidate into planet.[3] | ||
| GJ 523 b | 0.0739±0.0104 | 0.2275±0.0134 | 17.745740±0.000045 | 0.1226±0.0015 | 538±13 | transit | Confirmed | 86.8 | 0.781±0.029 | [4] | |
| GJ 887 d | 0.0192±0.0044 | 50.77±0.05 | 0.212+0.007 −0.008 |
241+10 −9 |
radial vel. | Confirmed | 10.724 | 0.495±0.049 | 3,688±86 | A super-Earth located in the habitable zone[5] | |
| GJ 887 e | 0.0046±0.0006 | 4.4249±0.0001 | 0.0417+0.0014 −0.0015 |
544+21 −20 |
radial vel. | Confirmed | [5] | ||||
| GJ 887 f | ~≥0.00157 | ~2.21661±0.0001 | ~0.0263 | ~685 | radial.vel | Candidate | Candidate into planet.[5] | ||||
| GJ 1137 c | 0.0161±0.0022 | 9.6412+0.0012 −0.0011 |
0.0835±0.0008 | radial vel. | Confirmed | 92.83 | 0.836+0.023 −0.025 |
5,033.8+85.7 −77.2 |
[6] | ||
| GJ 3090 c | 0.031±0.004 | 0.28 | 15.9407±0.0058 | 0.0997±0.0008 | 407.2±7.4 | radial vel. | Confirmed | 73.24 | 0.519±0.013 | 3,707±32 | [7] |
| GJ 3410 | ~6.8 | ~11.8 | ~261±9 | imaging | Candidate | 159 | 10.95 | 16943±68 | Candidate into planet.Orbits a white dwarf.[8] | ||
| GJ 4274 b | 0.0093+0.0017 −0.0016 |
0.1394 | 1.6339±0.0001 | 0.0153±0.0008 | radial vel. | Confirmed | 23.595 | 0.18±0.03 | 3,228±19 | [9] | |
| GJ 4274 c | 0.0264+0.0053 −0.0049 |
0.252 | 69.57+0.32 −1.14 |
0.186±0.010 | radial vel. | Confirmed | |||||
| HD 2134 b | 32.3 | radial vel. | Candidate | 233 | 1.01±0.128 | 5672±129 | Candidate into planet.[10] | ||||
| HD 48265 c | 4.45+0.75 −0.37 |
1.15 | 10418+2451 −1412 |
10.4+1.6 −1.0 |
astrometry + radial vel. | Confirmed | 296.2 | 1.38±0.06 | 5,805±34 | [11] | |
| HD 50554 c | 0.01148±0.00425 | 0.117±0.005 | 5.969362 | 0.066+0.009 −0.018 |
transit | Confirmed | 101.34 | 1.04±0.05 | 5,968±96 | [12] | |
| HD 50554 d | 0.0211±0.0116 | 0.126+0.013 −0.008 |
28.06940 | 0.168+0.028 −0.065 |
transit | Confirmed | |||||
| HD 68475 b | 5.16+0.53 −0.47 |
1.15 | 7832+463 −323 |
7.27+0.39 −0.36 |
astrometry + radial vel. | Confirmed | 108.7 | 0.83±0.10 | 5,022±113 | [11] | |
| HD 100508 b | 1.20+0.30 −0.18 |
1.22 | 5681±42 | 6.11+0.25 −0.28 |
astrometry + radial vel. | Confirmed | 106.9 | 0.94±0.12 | 5,419±112 | [11] | |
| HD 114386 c | 0.37±0.03 | 1.2 | 444.00+0.93 −0.88 |
1.05±0.04 | radial vel. | Confirmed | 91.26 | 0.80±0.03 | 4,895±62 | [11] | |
| HD 137010 b | 0.0946±0.0054 | 355.0+200.0 −59.0 |
0.88+0.3 −0.1 |
205.0±25.0 | transit | Candidate | 146.3 | 0.726±0.017 | 4,770±90 | сandidate Earth-sized planet at the edge of the habitable zone[13] | |
| 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. | Confirmed | 128.5 | 0.77±0.02 | 4,663±31 | [14] | |
| HD 176986 d | 0.0213±0.0029 | 0.222 | 61.376+0.051 −0.049 |
0.28149±0.0024 | 363±10 | radial vel. | Confirmed | 90.93 | 0.789±0.019 | 4,931±77 | [15] |
| KMT-2016-BLG-1337Lb | 0.54±0.30 | 1.01 | 3945 | 3.97+0.60 −0.92 |
microlensing | Confirmed | 22570+3392 −5251 |
0.54±0.30 0.40±0.22 |
A circumbinary planet.[16] | ||
| KMT-2020-BLG-0202Lb | 12.28+7.37 −5.43 |
1.1 | 3470 | 4.17+1.29 −1.28 |
microlensing | Confirmed | 12518+3879 −3847 |
0.81+0.49 −0.36 |
[17] | ||
| KMT-2021-BLG-0852Lb | 0.49+0.17 −0.17 |
7.78+0.89 −1.11 |
microlensing | Confirmed | 23581+2707 −3359 |
0.75+0.26 −0.27 |
[18] | ||||
| KMT-2022-BLG-1551Lb | 2.96+1.71 −1.53 |
1.17 | 1717 | 2.29+0.30 −0.44 |
microlensing | Confirmed | 22494+2999 −4336 |
0.54+0.31 −0.28 |
[17] | ||
| KMT-2023-BLG-0164Lb | 0.047+0.026 −0.019 |
1.33+0.39 −0.25 |
microlensing | Confirmed | 3390+1663 −880 |
0.32+0.21 −0.13 |
[19] | ||||
| KMT-2023-BLG-0466Lb | 3.25+2.59 −2.03 |
1.17 | 2411 | 2.68+0.45 −0.63 |
microlensing | Confirmed | 22168+3716 −5216 |
0.44+0.36 −0.27 |
[17] | ||
| KMT-2023-BLG-1286Lb | 0.062+0.058 −0.035 |
2.02±0.60 | microlensing | Confirmed | 20049+3227 −4401 |
0.31+0.29 −0.18 |
[19] | ||||
| KMT-2023-BLG-1746Lb | 0.0070+0.0048 −0.0021 |
1.06+0.55 −0.17 |
microlensing | Confirmed | 25363±3064 | 0.11+0.08 −0.03 |
[19] | ||||
| KMT-2024-BLG-0792L | 0.219+0.075 −0.046 |
microlensing | Candidate | 9948+1892 −1402 |
candidate rogue planet[20] | ||||||
| KMT-2024-BLG-2005Lb | 0.16+0.24 −0.09 |
1.12+0.15 −0.15 |
microlensing | Confirmed | 25179+3262 −3457 |
0.12+0.17 −0.06 |
[18] | ||||
| KMT-2024-BLG-3237L | 0.212+0.325 −0.134 |
microlensing | Candidate | 23940+3131 −6882 |
candidate rogue planet[21] | ||||||
| KMT-2025-BLG-0121Lb | 7.77+4.08 −4.04 |
1.13 | 2484 | 3.05+0.46 −0.66 |
microlensing | Confirmed | 20212+3032 −4400 |
0.61±0.32 | [17] | ||
| KMT-2025-BLG-0481Lb | 0.59+0.85 −0.34 |
2.18+0.31 −0.39 |
microlensing | Confirmed | 26027+3686 −4697 |
0.22+0.31 −0.13 |
[18] | ||||
| KMT-2025-BLG-0811Lb | 0.02199±0.01466 | 2.47±0.57 | microlensing | Confirmed | 22799+2772 −3457 |
0.49+0.32 −0.23 |
[22] | ||||
| KMT-2025-BLG-1616Lb | 0.1332+0.1278 −0.0694 |
1.6+0.2 −0.3 |
microlensing | Confirmed | 24462+2283 −3262 |
0.26+0.25 −0.14 |
[23] | ||||
| KOINTREAU-3b | 3.4±0.7 | 1.17 | 3609839 | 342±4 | imaging | Confirmed | 450 | 3,920±70 | [24] | ||
| KOINTREAU-4b | 11.5+1.2 −1.6 or[b] 14.8+1.2 −0.9 |
1.09 | 182±2 | imaging | Confirmed | 463 | [24] | ||||
| LHS 1903 b | 0.01032±0.0013 | 0.1233±0.0041 | 2.1555098 | 0.02656+0.00055 −0.00058 |
796±20 | transit | Confirmed | 116.3 | 0.538+0.039 −0.030 |
3,664±70 | [25] |
| LHS 1903 c | 0.01432+0.0023 −0.0022 |
0.1825+0.0070 −0.0066 |
6.226185 | 0.05387+0.00112 −0.00117 |
559±14 | transit | Confirmed | ||||
| LHS 1903 d | 0.01875±0.0036 | 0.2230+0.0070 −0.0069 |
12.566287 | 0.08604+0.00178 −0.00186 |
442±11 | transit | Confirmed | ||||
| LHS 1903 e | 0.01822+0.0050 −0.0051 |
0.1545+0.0053 −0.0052 |
29.31773 | 0.15135+0.00314 −0.00338 |
333+9 −8 |
transit | Confirmed | ||||
| MP mus g | ~0.003+0.028 −0.0028 |
~60 | imaging | Candidate | 319.3 | 1.3±0.08 | 5000 | Candidate into planet.[26] | |||
| TIC 259230140 b | ~0.5692±0.0348 | ~14.31708±0.00016 | transit | Candidate | 904.8 | 7500-10000 | Candidate into planet.Also known as HD 130599.[27] | ||||
| TIC 65910228 b | 4.78+0.40 −0.37 |
1.081±0.047 | 180.52791 | 0.695±0.036 | 458±11 | transit | Confirmed | 864 | 1.46±0.09 | 6,310±129 | Planet also known as NGTS-38 b.[28][29] |
| 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 | Confirmed | 1302 | 1.239+0.070 −0.080 |
6,150±178 | Star also known as TOI-6752.[30] |
| 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 | Confirmed | 1490 | 1.406+0.074 −0.086 |
6,410±183 | [30] |
| TIC 245076932 b | 0.51+0.04 −0.05 |
0.970±0.048 | 21.613890 | 0.157±0.007 | 845±25 | transit | Confirmed | 1026 | 1.117±0.063 | 6,130±178 | [30] |
| TOI-237 c | 0.1076±0.0031 | 1.74486147 | 0.0160+0.0005 −0.0006 |
515+11 −8 |
transit | Confirmed | 124.86 | 0.1698+0.0385 −0.0350 |
3,226+47 −48 |
[31] | |
| TOI-883 b | 0.123±0.012 | 0.604±0.028 | 10.057716 | 0.0898±0.0023 | 1,086±19 | transit | Confirmed | 336 | 0.956+0.054 −0.051 |
5,697±80 | [32] |
| TOI-899 b | 0.213±0.024 | 0.991±0.044 | 12.846185 | 0.1063±0.0026 | 1,040±19 | transit | Confirmed | 1004 | 0.972+0.054 −0.053 |
5,696±80 | [32] |
| 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 | Confirmed | 83.36 | 0.1667±0.0041 | 3,065±50 | [33] |
| TOI-1232 b | 0.964±0.06 | 0.975±0.05 | 14.256±0.001 | 0.117±0.001 | transit | Confirmed | 1068 | 1.05±0.133 | 5818±134.1 | [34] | |
| TOI-1232 c | 0.18±0.02 | 30.356±0.01 | 0.194±0.002 | radial vel. | Confirmed | ||||||
| TOI-1243 b | 0.0242±0.0047 | 0.2079±0.0107 | 4.65948 | 0.0437±0.0001 | 450 | transit | Confirmed | 140.6 | 0.515±0.027 | 3,515±79 | [35] |
| TOI-2133 b | 0.026+0.010 −0.008[c] |
0.211±0.008 | 3.8266472 | 0.0410±0.0015 | 798±12 | transit | Confirmed | 245.3 | 0.644±0.019 | 4,250±45 | [36] |
| TOI-3862 b | 0.1688+0.0087 −0.0090 |
0.493±0.016 | 1.55745774 | 0.02539+0.00064 −0.00068 |
1,539 | transit | Confirmed | 801.2 | 0.90±0.07 | 5,300±50 | [37] |
| TOI-4336 A c | 0.114 | 0.1039+0.0054 −0.0052 |
7.587270 | 0.0481±0.0027 | 378±12 | transit | Confirmed | 73.23 | 0.2853+0.0438 −0.0356 |
3,369+51 −57 |
[31] |
| TOI-4495 b | 0.024+0.004 −0.05 |
0.221+0.012 −0.008 |
2.56699 | 0.03957±0.00047 | 1735 | transit | Confirmed | 801.2 | 1.247±0.045 | 6,210±70 | [38] |
| TOI-4529 b | 0.0154 | 0.1579±0.008 | 5.87958 | 0.04997±0.0008 | 511 | transit | Confirmed | 92.6 | 0.482±0.023 | 3,697±71 | [35] |
| TOI-4552 b | 0.00576±0.0016 | 0.099±0.0036 | 0.30110032±0.00000014 | 0.0056255±0.0000003 | 1122 | transit | Confirmed | 89.3 | 0.2619±0.0063 | 3,258±115 | [39] |
| TOI-4616 b | 0.00708±0.00236 | 0.1088 | 1.55382±0.00001 | 0.0150±0.00001[d] | 525 | transit | Confirmed | 91.9 | 0.1881±0.0094 | 3,150±75 | [40] |
| TOI-5734 b | 0.0286±0.0082 | 0.187±0.011 | 6.1841876 | 0.05921±0.00024 | 688±23 | transit | Confirmed | 100.1 | 0.724±0.009 | 4,750±100 | [36][41] |
| TOI-5788 b | 0.0117±0.0030 | 0.1365±0.0067 | 6.340758 | 0.0640±0.0011 | transit | Confirmed | 318.2 | 0.87±0.04 | 5,615±25 | [42] | |
| TOI-5788 c | 0.0201±0.0038 | 0.2025±0.0036 | 16.213358 | 0.1197±0.0020 | transit | Confirmed | |||||
| 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 | Confirmed | 1013 | 1.047+0.089 −0.071 |
5,890+170 −180 |
[43] |
| TOI-5938 b | 0.049+0.025 −0.022[c] |
0.341±0.010 | 2.2604240 | 0.0308±0.0010 | 1077+16 −15 |
transit | Confirmed | 371.9 | 0.744±0.016 | 4,650±50 | [36] |
| TOI-6716 b | 0.00287 | 0.0874±0.0062 | 4.71859 | 0.032±0.003 | 369 | transit | Confirmed | 61.6 | 0.223±0.011 | 3,110±80 | [44] |
| TOI-7009 b | 0.047+0.023 −0.021[c] |
0.331±0.013 | 2.3206612 | 0.0287±0.0010 | 872+11 −10 |
transit | Confirmed | 600.5 | 0.583±0.014 | 4,080±25 | [36] |
| TOI-7169 b | 0.41±0.014v | 1.475±0.029 | 3.4373125 | transit | Confirmed | 0.885 ±0.01 | 1,477 | Orbits a metal-poor star.[45][46] | |||
| TOI-7384 b | 0.039 | 0.3176±0.0187 | 6.23403 | 0.0439±0.004 | 378 | transit | Confirmed | 218 | 0.318±0.016 | 3,185±75 | [44] |
Specific exoplanet lists
[edit]- 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
[edit]- 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 (254)
- List of exoplanets discovered in 2022 (313)
- 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 (79)
Notes
[edit]- ^ 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.
- ^ a b c d Estimated using theoretical mass–radius relations.
- ^ Converted from orbital period.
References
[edit]- ^ Kozdon, Janus; Fung, Jeffrey; et al. (27 February 2026). "AB Aurigae: 12CO Ro-vibrational Spectroscopy of AB Aurigae -- A Potential Point Source is Present". arXiv:2603.00250 [astro-ph.EP].
- ^ a b c d e f g 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. Bibcode:2026MNRAS.tmp..387S. doi:10.1093/mnras/stag370.
{{cite journal}}: CS1 maint: bibcode (link) - ^ Donati, J.-F.; Cristofari, P.I.; et al. (27 February 2026). "Monitoring the magnetospherie accretion of the classical T Tauri star DO Tau with SPIRou". arXiv:2602.24078 [astro-ph.EP].
- ^ Kroft, Maxwell A.; Beatty, Thomas G.; Salzer, Joseph M.; Zwicker, Claire; Becker, Juliette; Dou, Jingyao; et al. (25 March 2026). "GJ 523b is a Massive, 170 Myr-old Mega-Earth, Likely on a Polar Orbit". Astronomical Journal. forthcoming. arXiv:2603.24682.
- ^ a b c 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.
- ^ 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. 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.
- ^ Poulsen, Sabrina; Debes, John; et al. (26 January 2026). "The MIRI Excess around Degenerates (MEAD) Survey II: A Probable Planet detected via IR Excess around WD 0644+025". The Astronomical Journal. 171 (3): 183. arXiv:2601.18965. Bibcode:2026AJ....171..183P. doi:10.3847/1538-3881/ae3c0e.
- ^ Charpentier, Paul; et al. (The SPIRou science Consortium) (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.
- ^ 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. 547 (3). arXiv:2602.18207. Bibcode:2026MNRAS.547.4527H. doi:10.1093/mnras/stag370.
- ^ a b c d 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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