List of exoplanets discovered in 2017

Last updated

This is a list of exoplanets discovered in 2017.

For exoplanets detected only by radial velocity, the mass value is actually a lower limit. (See Minimum mass for more information)

Contents

Name Mass (MJ) Radius (RJ) Period (days) Semi-major axis (AU) Temp. (K) [1] Discovery method Distance (ly) Host star mass (M) Host star temp. (K) Remarks
BD+03 2562 b 6.4481.91.3radial vel.85401.144095 [2]
CoRoT-30 b 2.90±0.221.009±0.0769.06005±0.000240.0844±0.0012transit3100±2000.98+0.03
0.05
5650±100 [3]
CoRoT-31 b 0.84±0.341.46±0.304.62941±0.000750.0586±0.0034transit7000±20001.25+0.22
0.21
5700±120 [3]
CoRoT-32 b 0.150.576.718370.071938transit1.085970Host star also known as CoRoT 223977153 [4]
Luyten b 0.0090918.64980.091101259radial vel.120.293382Potentially habitable exoplanet. [5]
Luyten c 0.003714.72340.036467radial vel.120.293382 [5]
Gliese 625 b 0.0088714.6280.078361radial vel.210.303499 [6]
Gliese 1148 c 0.2141532.580.912radial vel.35.980.357±0.013Host star also known as Ross 1003 [7]
Gliese 3138 b 0.00561.220030.0197radial vel.92.90.683717 [5]
Gliese 3138 c 0.013155.9740.057radial vel.92.90.683717 [5]
Gliese 3138 d 0.03304257.80.698radial vel.92.90.683717 [5]
Gliese 3293 d 0.0239148.13450.19394radial vel.51.40.423466 [5]
Gliese 3293 e 0.0103213.25430.08208radial vel.51.40.423466 [5]
Gliese 3323 b 0.006365.36360.03282radial vel.17.40.163159 [5]
Gliese 3323 c 0.0072740.540.1264radial vel.17.40.163159 [5]
Gliese 3942 b 0.02256.9050.0608590radial vel.55.30.633867 [8]
HAT-P-67b0.342.0854.810102500.06505transit10001.6426406 [9]
HATS-36b 2.79±0.401.263±0.0454.1752379±0.00000210.0529±0.00111363±40transit2860±701.135±0.0675970±160Host star also known as K2-145 [10] Host star also known as K2-145
HATS-43b 0.261±0.0541.180±0.0504.38884970.04944±0.000461003±27transit1194.1±7.40.837±0.0235099±61 [11]
HATS-44b 0.56±0.111.067+0.125
0.071
2.74390040.03649±0.000301161±34transit1474±110.860±0.0215080±100 [11]
HATS-45b 0.70±0.151.286±0.0934.18762440.05511±0.000691518±45transit2575±381.272±0.0486450±110 [11]
HATS-46b 0.173±0.0620.903+0.058
0.045
4.74237290.05367±0.000531054±29transit1500±130.917±0.0275495±69 [11]
HATS-50b 0.391.1303.82970150.05046transit23401.175990 [12]
HATS-51b 0.7681.413.34887020.046391553transit15601.175758 [12]
HATS-52b 2.241.3821.366654360.024981834transit20601.116010 [12]
HATS-53b 0.5951.3403.85377680.047531312transit20000.965644 [12]
HD 3167 d 0.02178.5090.07757radial vel.1490.865261 [13]
HD 17674 b 0.87623.81.42radial vel.1450.985904 [14]
HD 20781 d 0.0061+0.0012
0.0011
0.20525.3135±0.0010.0529+0.0024
0.0027
radial vel.115.36±4.40.75256±29 [15]
HD 20781 e 0.0168+0.0022
0.0021
0.218313.8905+0.0033
0.0034
0.1004+0.0046
0.0051
radial vel.115.36±4.40.75256±29 [15]
HD 20794 e 0.0150147.020.509radial vel.19.80.75401 [16]
HD 27894 c 0.16236.070.198radial vel.138.20.84875 [17]
HD 27894 d 5.41551745.448radial vel.138.20.84875 [17]
HD 29021 b 2.41362.32.28radial vel.1000.855560 [14]
HD 40956 b 2.7578.61.4radial vel.3852.004869 [18]
HD 42012 b 1.6857.51.67radial vel.1210.835405 [14]
HD 45184 c 0.0277+0.0034
0.0032
13.1354+0.0026
0.0025
0.11+0.0034
0.0036
radial vel.71.36±0.621.035869±14 [19]
HD 76920 b 3.93415.891+0.043
0.039
1.149radial vel.602.71.174698Extremely eccentric orbit around an evolved red giant [20] [21] [22]
HD 93385 Ab 0.0125±0.00157.3422±0.00140.0749±0.00171129±19radial vel.141.6±0.21.04±0.015823±35 [19] Confirmed in 2021, renamed from HD 93385 d [23]
HD 106315 b 0.02550.2079.558040.09051046transit3581.086277Host star also known as K2-109 [24]
HD 106315 c 0.05600.38521.057880.1533804transit3581.086277Host star also known as K2-109 [24]
HD 111591 b 4.41056.42.5radial vel.3521.944884 [18]
HD 113996 b 6.3610.21.6radial vel.331.41.494181 [18]
HD 147379 b 0.077786.540.3193radial vel.35.010.584090 [25]
HD 176986 b 0.01816.489800.06296radial vel.86.10.794931 [26]
HD 176986 c 0.0288816.81910.11878radial vel.86.10.794931 [26]
HD 177565 b 0.0475144.5050.246radial vel.561.0 [27]
HD 208897 b 1.40352.71.05radial vel.2111.254860 [28]
HIP 65426 b 9.0±3.01.5±0.1230,400921500+100
200
imaging363.3±12.31.96±0.058840±200Gas giant orbiting the host star also known as HD 116434 [29] [30]
K2-18c 0.02368.9620.060363radial vel.1100.363547 [31]
K2-105b 0.094390.3698.2669020.081transit7601.015434 [32]
K2-106b 0.02630.1360.5712920.01162333transit7980.955470 [33] Host star also known as EPIC 220674823
K2-106c 0.22613.341245transit8300.935590 [33] Host star also known as EPIC 220674823
K2-108b 0.186890.4714.734010.05731446transit15301.125474 [34]
K2-111b 0.02710.175.351170.06211309transit6800.885730 [35]
K2-114b 1.850.94211.391090.09309719transit15700.835027 [36]
K2-115b 0.841.11520.2730340.1367682transit13600.835560 [36]
K2-116b  [ ru ]0.0624.6554110.048transit183.10.694348 [37] Host star also known as BD-12 6259
K2-117b 0.1751.2915050.019transit333.50.583842 [38]
K2-117c 0.1815.4448200.051transit333.50.583842 [38]
K2-118b 0.22750.920920.245transit10570.764726 [37]
K2-119b 0.2047.7285780.070transit11800.764753 [37]
K2-120b 0.1799.5627420.078transit9500.694350 [37]
K2-121b 0.8145.1857540.052transit5520.714471 [37]
K2-122b 0.1142.2194050.029transit2360.633993 [37] [38]
K2-123b 0.23630.9567630.167transit5290.654076 [37] [38]
K2-124b 0.2366.4135390.051transit4480.443561 [37]
K2-125b 0.19421.7502640.121transit4150.493654 [37]
K2-126b 0.1647.3870730.066transit3320.704368 [37]
K2-127b 0.7733.5881650.041transit23700.704388 [37]
K2-128b 0.1275.6758190.056transit3730.714470 [37]
K2-129b 0.09288.2394930.057transit90.19±0.070.363459 [37] Host star also known as LP 868-19
K2-130b 0.1122.4941200.032transit384.4±0.60.704356 [37]
K2-131b 0.0170.1520.369310.0095002062transit5010.845245 [39]
K2-132b 1.309.1751transit5681.08±0.084840±90 [40]
K2-133b  [ ru ]0.1173.07120.033transit245.3±0.70.46±0.013655±80Host star also known as LP 358–499, 4 planets in system [41]
K2-133c  [ ru ]0.1324.86820.045transit245.3±0.70.46±0.013655±80Host star also known as LP 358–499, 4 planets in system [41]
K2-133d  [ ru ]0.18011.02340.077transit245.3±0.70.46±0.013655±80Host star also known as LP 358–499, 4 planets in system [41]
K2-135b 0.1561.2089570.0201043.5transit98.80.664255 [42]
K2-135c 0.1213.648020.042721.9transit98.80.664255 [42]
K2-135d 0.1876.201410.060604.9transit98.80.664255 [42]
K2-136b  [ ru ]0.08837.975292553transit0.744499 [43]
K2-136c  [ ru ]0.057±0.0060.26017.3071370.11728425transit0.744499 [43] [44]
K2-136d  [ ru ]0.12925.575065373transit0.744499 [43]
K2-137b 0.50.0790.1797150.00581471transit0.463492 [45]
K2-139b 0.3870.80828.382360.179565transit4961.85340 [46]
K2-140b 0.2111.0936.569180.0687957transit11101.005705 [47]
K2-141b 0.0160±0.00130.135±0.0040.28032260.00716+0.00055
0.00065
2039+87
48
transit202.16±0.540.708±0.0284599±79 [48] [49]
K2-146b 0.196±0.0212.6446460.0266±0.0010transit259.2±1.50.358±0.0423385±70 [38]
K2-147b 0.123+0.015
0.013
0.9619170.0159±0.0005transit296.10±0.900.583±0.0593672±70 [38] Also called EPIC 213715787 [50]
K2-148b 0.119+0.017
0.016
4.38395±0.000800.0454±0.0014transit407.4±2.00.650±0.0614079±70 [38]
K2-148c 0.154+0.021
0.019
6.92260±0.000700.0616±0.0019transit407.4±2.00.650±0.0614079±70 [38]
K2-148d 0.146+0.021
0.019
9.7579±0.00100.0774±0.0024transit407.4±2.00.650±0.0614079±70 [38]
K2-149b 0.146+0.018
0.016
11.3320±0.00130.0830±0.0027transit404.8±1.80.595±0.0593745±70 [38]
K2-150b 0.178+0.024
0.019
10.59357±0.000840.0727±0.0027transit335.2±2.60.457±0.0513499±70 [38]
K2-151b 0.120+0.014
0.012
3.8355920.0365±0.0014transit227.07±0.490.440±0.0503585±70 [38]
K2-152b 0.204+0.022
0.021
32.6527±0.00350.1716±0.0012337±3transit354.8±1.30.63±0.014044+34
35
[38]
K2-153b 0.178+0.019
0.016
7.515540.0614±0.0004497±6transit468.7±3.00.55±0.013845±37 [38]
K2-154b 0.178+0.019
0.010
3.676350.0405±0.0003715+9
8
transit423.5±1.50.65+0.02
0.01
4097+40
45
[38]
K2-154c 0.185+0.016
0.012
7.954780.0677±0.0005552±7transit423.5±1.50.65+0.02
0.01
4097+40
45
[38]
KELT-9b 2.881.8911.48112350.034624050transit615.52.5210170Hottest confirmed exoplanet [51]
KELT-18b 1.181.5702.87175180.045502085transit1.526670 [52]
KELT-19Ab <4.071.914.61170930.06371935transit9501.627500 [53]
KELT-20b 1.7413.47410850.05422262transit455.61.768720 [54] Also known as MASCARA-2b [55]
KELT-21b 3.91+0
3.91
1.586+0.039
0.040
3.61276470.05224+0.00035
0.00034
2051+29
30
transit1557±211.458+0.029
0.028
7598+81
84
[56]
Kepler-19d 0.070862.95radial vel.69100.945541 [57]
Kepler-80g 0.10114.64558418transit11600.734540 [58]
Kepler-90i 0.11814.44912709transit25401.26080 [58]
Kepler-150 f 0.325637.20931.24transit2980±505560 [59]
Kepler-1649b 0.09648.6890900.0514transit0.223240 [60]
Kepler-1650b 0.08561.53818001transit3930.333410 [61]
Kepler-1651b 0.1649.87863917transit2260.523713 [61]
Kepler-1652b 0.14338.097220.1654268transit8220.403638 [62]
Kepler-1653b  [ it ]0.194140.25240.4706284transit24600.724807 [62]
LHS 1140 b 0.02090.12824.737120.0875254transit40.70.183216Potentially habitable exoplanet [63]
MASCARA-1b 3.71.52.1487800.0432570transit615.51.727554 [64]
MOA-2010-BLG-117Lb 0.54±0.102369+835
2717
2.9+1.6
0.6
microlensing11400±13000.58±0.114000+450
350
[65]
MOA-2012-BLG-006Lb 8.4010.2microlensing170000.49 [66]
MOA-2012-BLG-505Lb 0.021080.900microlensing235000.10 [67]
MOA-2016-BLG-227Lb 2.81.67microlensing210000.29 [68]
MXB 1658-298 b 23.77601.613timing1.98Circumbinary planet [69]
NGTS-1b 0.8121.332.6472980.0326790transit7310.6173916Largest exoplanet in relation to its star [70]
OGLE-2013-BLG-0132Lb 0.293.6microlensing130000.54 [71]
OGLE-2013-BLG-1721Lb 0.642.6microlensing210000.46 [71]
OGLE-2013-BLG-1761Lb 2.7+2.5
1.5
1.8±0.5microlensing23000+3300
3900
0.33+0.32
0.19
[72]
OGLE-2016-BLG-0263Lb 4.105.4microlensing210000.13 [73]
OGLE-2016-BLG-0613(AB)b 4.186.40microlensing111000.72 [74]
OGLE-2016-BLG-1190Lb 13.3812242.17microlensing221000.88Extremely massive; possible brown dwarf [75]
OGLE-2016-BLG-1195Lb 0.0312.62±0.28microlensing22000±20000.57±0.06 [76] [77]
OGLE-2017-BLG-0173Lb 0.0103+0.0121
0.0063
4493+3090
7055
3.9±1.6microlensing15700+4900
5900
0.40+0.39
0.23
3500+1500
500
Atypical lensing event [78] Not an OGLE-2011-BLG-0173Lb!
PSR J2322-2650 b 0.79490.3229639970.0102timing7501.4 [79]
Qatar-6b 0.6681.0623.5061950.0423transit3300.8225052 [80]
Ross 128 b 0.004409.86580.0496301radial vel.11.030.173192 [81]
SAND978 b 2.18511.21radial vel.2051.31.374200 [82] Red giant host star, belonging to M67, is also known as NGC 2682 108
TAP 26 b 1.6610.790.0968radial vel.4801.044620Host star also known as V1069 Tauri [83]
Tau Ceti g 0.0055120.000.133radial vel.120.78 [84]
Tau Ceti h 0.0057649.410.243radial vel.120.78 [84]
TRAPPIST-1e 0.001950.0826.0996150.02817251transit390.082559Potentially habitable exoplanet [85]
TRAPPIST-1f 0.002140.0939.206690.0371219transit390.082559Potentially habitable exoplanet [85]
TRAPPIST-1g 0.004220.10112.352940.0451199transit390.082559Potentially habitable exoplanet [85]
TRAPPIST-1h 0.067200.063168transit390.082559 [85]
TYC 4282-605-1 b 10.78101.540.422radial vel.23000.974300 [86]
WASP-91b 1.341.032.7985810.0371160transit4900.844920 [87]
WASP-105b 1.80.967.872880.075900transit0.895070 [87]
WASP-107b 0.120.945.7214900.055770transit0.694430 [87]
WASP-151b 0.311.134.5334710.0551290transit15701.015871 [88] Host star also known as K2-134
WASP-153b 0.391.553.3326090.0481700transit14001.345914 [88]
WASP-156b 0.1280.513.8361690.0453970transit4600.844910 [88] Host star also known as TOI-465
WASP-167b 1.582.02195960.03652329transit12401.597000Host star also known as KELT-13 [89]
YZ Ceti b 0.00241.968760.01634+0.00035
0.00041
radial vel.12.122±0.0020.130±0.0133056±60 [90]
YZ Ceti c 0.003083.060080.02156+0.00046
0.00054
radial vel.12.122±0.0020.130±0.0133056±60 [90]
YZ Ceti d 0.003594.656270.02851+0.00061
0.00071
radial vel.12.122±0.0020.130±0.0133056±60 [90]

Specific exoplanet lists

Lists of exoplanets

Lists of exoplanets by year of discovery

Related Research Articles

BD−10°3166 is a K-type main sequence star approximately 268 light-years away in the constellation of Crater. It was inconspicuous enough not be included in the Draper catalog (HD). The Hipparcos satellite also did not study it, so its true distance is poorly known. The distance measured by the Gaia spacecraft of 268 light years rules out a suggested companion star, LP 731-076, being its true binary star companion.

<span class="mw-page-title-main">WASP-4b</span> Extrasolar planet in the constellation Phoenix

WASP-4b is an exoplanet, specifically a hot Jupiter, approximately 891 light-years away in the constellation of Phoenix.

HD 222155 is a star in the northern constellation of Andromeda. It is a yellow star that can be viewed with binoculars or a small telescope, but is too faint to be seen with the naked eye at an apparent visual magnitude of 7.1. The imaging survey in 2017 did not detect any stellar companions to HD 222155.

GJ 9827 is a star in the constellation of Pisces. It is a K-type main-sequence star with an apparent magnitude of 10.250. It is 97 light-years away, based on parallax.

HD 3167 is a single, orange-hued star in the zodiac constellation of Pisces that hosts a system with three exoplanets. The star is too faint to be seen with the naked eye, having an apparent visual magnitude of 8.97. The distance to HD 3167 can be determined from its annual parallax shift of 21.1363 mas as measured by the Gaia space observatory, yielding a range of 154 light years. It has a relatively high proper motion, traversing the celestial sphere at the rate of 0.204″ per year. Since it was first photographed during the Palomar observatory sky survey in 1953, it had moved over 12.5″ by 2017. The star is moving away from the Earth with an average heliocentric radial velocity of +19.5 km/s.

K2-32 is a G9-type main sequence star slightly smaller and less massive than the sun. Four confirmed transiting exoplanets are known to orbit this star. A study of atmospheric escape from the planet K2-32b caused by high-energy stellar irradiation indicates that the star has always been a very slow rotator.

HD 197037 is a binary star system. Its primary or visible star, HD 197037 A, is a F-type main-sequence star. Its surface temperature is 6150±34 K. HD 197037 A is depleted in heavy elements compared to the Sun, with a metallicity Fe/H index of −0.16±0.03, but is younger at an age of 3.408±0.924 billion years.

HAT-P-41 is a binary star system. Its primary is a F-type main-sequence star. Its surface temperature is 6390±100 K. compared to the Sun, HAT-P-41 is enriched in heavy elements, with a metallicity Fe/H index of 0.21±0.10, but is much younger at an age of 2.2±0.4 billion years.

HD 106315, or K2-109, is a single star with a pair of close-orbiting exoplanets, located in the constellation of Virgo. Based on parallax measurements, this system lies at a distance of 356 light years from the Sun. At that range, the star is too faint to be seen with the naked eye, as it has an apparent visual magnitude of 8.95. But it is slowly drifting closer with a radial velocity of −3 km/s. As of 2020, multiplicity surveys have not detected any stellar companions to HD 106315.

References

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