List of exoplanets discovered in 2013

Last updated

This is a List of exoplanets discovered in 2013.

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
2MASS J01225093-2439505 b 24.552imaging1200.43530 [2]
BD+15 2940 b 1.11137.480.539radial vel.572.21.14796 [3]
CoRoT-25b 0.271.084.860690.0578transit33001.096040 [4]
CoRoT-26b 0.521.264.204740.0526transit54001.095590 [4]
DENIS-P J082303.1-491201 b 28.5246.360.36astrometry67.70.072150 [5]
Gliese 163 b 0.033358.631820.0607radial vel.48.80.43500 [6]
Gliese 163 c 0.021425.630580.1254radial vel.48.80.43500 [6]
Gliese 163 d 0.0925603.951161.0304radial vel.48.80.43500 [6]
Gliese 221b 0.0273.87280.0428radial vel.660.74324 [7] [8] Disputed [9]
Gliese 221 c 0.17125.940.435radial vel.660.74324 [7] [8]
Gliese 328b 2.341004.5radial vel.65.30.693900 [10]
Gliese 504 b 443.5imaging58.51.226234 [11]
HAT-P-44b 0.3521.2424.3012190.0507transit11800.945295 [12]
HAT-P-44c 4872.21.752radial vel.11800.945295Period is ambiguous [12]
HAT-P-45b 0.8921.4263.1289920.0452transit9901.266330 [12]
HAT-P-46b 0.4931.2844.4631290.0577transit9701.286120 [12]
HATS-2b 1.3451.1681.3541330.023transit12000.885227 [13]
HATS-3b 1.0711.3813.5478510.04851648transit14801.216351 [14]
HD 2952 b  [ ru ]1.6311.61.2radial vel.375.82.544844 [15]
HD 13908 b  [ fr ]0.86519.3820.154radial vel.218.21.296255 [16]
HD 13908 c  [ fr ]5.139312.03radial vel.218.21.296255 [16]
HD 65216c 0.17152.60.54radial vel.116.10.925666 [17] False positive, another planet with same assigned name discovered in 2019. [18]
HD 95086 b 555.7imaging298.71.6 [19]
HD 103774 b 0.3675.88810.07radial vel.173.11.336489 [7]
HD 106906 b 11650imaging299.51.56516 [20]
HD 109271 b 0.0547.85430.079radial vel.185.61.055783 [7]
HD 109271 c 0.07630.930.196radial vel.185.61.055783 [7]
HD 113337 b 2.833240.92radial vel.122.01.46576.6 [21]
HD 120084 b 4.520824.3radial vel.318.52.394892 [15]
HD 159243 b 1.1312.620.11radial vel.223.71.126123 [16]
HD 159243 c  [ fr ]1.9248.40.8radial vel.223.71.126123 [16]
HD 233604 b 6.5751920.747radial vel.2830±901.54791 [3]
HD 285507 b 0.92±0.036.0962±0.0002radial vel.1530.73±0.034503+85
61
member of Hyades (star cluster) [22] [23]
HD 112410 b 9.18124.60.565radial vel.486.81.544830 [24]
HIP 91258 b  [ fr ]1.0685.05050.057radial vel.145.00.955519 [16]
KELT-3b 1.4771.3452.70339040.04122transit5801.286306 [25]
KELT-6b 0.4421.187.84558210.08transit7201.136272 [26]
Kepler-37b 0.031460.02913.3675transit2200.85417 [27]
Kepler-37c 0.037760.06721.302transit2200.85417 [27]
Kepler-37d 0.038390.17339.7922transit2200.85417 [27]
Kepler-61b 0.19259.87756transit1103±160.644017 [28]
Kepler-62b 0.030.1175.7149320.0553transit12000.694925 [29]
Kepler-62c 0.0130.04812.44170.0929transit12000.694925 [29]
Kepler-62d 0.0440.17418.164060.12transit12000.694925 [29]
Kepler-62e 0.1130.144122.38740.427transit12000.694925Potentially habitable exoplanet [29]
Kepler-62f 0.110.126267.2910.718transit12000.694925Potentially habitable exoplanet [29]
Kepler-63b 0.3780.5459.43415050.08transit6500.985576 [30]
Kepler-65b 0.1272.154910.035transit999±81.256211 [31]
Kepler-65c 0.235.8599440.068transit999±81.256211 [31]
Kepler-65d 0.1368.131230.084transit999±81.256211 [31]
Kepler-66b 0.2517.8158150.1352transit36101.045962Belongs to open cluster NGC 6811 [32]
Kepler-67b 0.26215.72590.1171transit36100.865331Belongs to open cluster NGC 6811 [32]
Kepler-68b 0.018780.2085.398751280transit4401.085793 [33]
Kepler-68c 0.022650.0899.60504transit4401.085793 [33]
Kepler-68d 0.84007625radial vel.4401.085793 [33]
Kepler-69b 0.213.7223410.094transit2430±300.815638 [34]
Kepler-69c 0.153242.46130.64transit2430±300.815638 [34] [35]
Kepler-74b  [ es ]0.630.967.3407110.0781transit43001.186000 [36]
Kepler-75b  [ es ]10.11.058.88491160.0818transit37000.915200 [36]
Kepler-76b 2.011.361.54492980.0274orbital brightness modulation2750±301.26409 [37]
Kepler-77b  [ es ]0.430.963.578780870.04501transit19000.955520 [38]
Kepler-78b 0.0060.1050.3552330transit407.1±1.10.765058 [39]
Kepler-87b 1.021.204114.736350.481478transit4170±901.15600Two more unconfirmed planets in the system [40]
Kepler-87c 0.020.548191.23180.676403transit4170±901.15600Two more unconfirmed planets in the system [40]
Kepler-88b 0.0270.33710.95416transit11100.965471 [41]
Kepler-88c 0.62622.33950.15525timing11100.965471 [41] [42]
Kepler-89b 0.0330.1533.7432080.05119transit1577±161.286182 [43]
Kepler-89c 0.0490.38510.4236480.1013transit1577±161.286182 [43]
Kepler-89d 0.3341.00522.3429890.1684transit1577±161.286182 [43]
Kepler-89e 0.110.58554.320310.3046transit1577±161.286182 [43]
Kepler-90b 0.1177.0081510.0741056transit25001.26080 [44]
Kepler-90c 0.1068.7193750.089981transit25001.26080 [44]
Kepler-90d 0.25659.736670.32518transit25001.26080 [44]
Kepler-90e 0.23791.939130.42448transit25001.26080 [44]
Kepler-90f 0.257124.91440.48592transit25001.26080 [44]
Kepler-90g 0.723210.606970.71340transit25001.26080 [44]
Kepler-90h 1.008331.600591.01292transit25001.26080 [44]
Kepler-91b 0.811.3676.246580.0731transit34001.314550 [45]
Kepler-92b 0.2020.31313.749transit1580±171.215883 [46]
Kepler-92c 0.0190.23226.723transit1580±171.215883 [46]
Kepler-102e 0.0280.19816.1457579transit352.7±0.70.814909 [47]
Kepler-105b 0.4295.41220.066transit1517±180.965827 [47]
Kepler-114c 0.0090.1438.041623transit852±40.564605 [46]
Kepler-114d 0.0120.22611.776549transit852±40.564605 [46]
Kepler-128b 0.0970.10115.09transit1307±121.186090 [46]
Kepler-128c 0.1050.10122.804transit1307±121.186090 [46]
Kepler-130b 0.0918.4574580.079transit1042±715884 [47]
Kepler-145b 0.1170.23622.951transit1880±301.326022 [46]
Kepler-145c 0.250.38542.882transit1880±301.326022 [46]
Kepler-177b 0.0060.25936.855transit4880±1401.075942 [46]
Kepler-177c 0.0240.63349.412transit4880±1401.075942 [46]
Kepler-238e 0.5340.523.654transit6200±3001.065751 [46]
Kepler-238f 0.0420.17850.447transit6200±3001.065751 [46]
Kepler-276c 0.0520.25931.884transit3850±1501.16105 [46]
Kepler-276d 0.0510.2548.648transit3850±1501.16105 [46]
Kepler-277b 0.2750.26117.324transit3280±501.125946 [46]
Kepler-277c 0.2020.333.006transit3280±501.125946 [46]
Kepler-279b 0.32312.3096810.112transit3480±701.16363KOI-1236.01 [48]
Kepler-279c 0.1550.38435.736transit3490±701.16363KOI-1236.02 [48] [46]
Kepler-279d 0.1180.27754.414transit3490±701.16363 [46]
Kepler-282d 0.1920.21924.806transit4540±1500.975602 [46]
Kepler-282e 0.1770.27744.347transit4540±1500.975602 [46]
Kepler-305b 0.0330.3215.487transit2900±900.765100 [46] KOI-1563.01 [48]
Kepler-305c 0.0190.2948.291transit2900±900.765100 [46] KOI-1563.02 [48]
Kepler-307b 0.023410.21710.4208transit1908±170.915367 [46]
Kepler-307c 0.011450.19613.0729transit1908±170.915367 [46]
Kepler-328b 0.090.20534.921transit7700±5001.155914 [46]
Kepler-328c 0.1240.48271.312transit7700±5001.155914 [46]
Kepler-350c 0.0190.27717.849transit3210±7016186 [46]
Kepler-350d 0.0470.2526.136transit3210±7016186 [46]
Kepler-396b 0.2380.31242.994transit734±50.855384 [46] KOI-2672.01 [48]
Kepler-396c 0.0560.47388.505transit734±50.855384 [46] KOI-2672.02 [48]
Kepler-410Ab 0.25317.8336480.1226transit4301.216273 [49]
Kepler-411b 0.1683.005160.0381040transit503.5±1.50.834974 [47]
Kepler-1359c0.3711+0.12
0.06
505.46+0.05
0.04
1.143±0.018transit2182+81
82
0.78+0.03
0.04
4709+46
56
[44] Also called KIC 6436029 c, discovery retracted in 2015 after 3rd transit was proven to be false. [50]
MOA-2008-BLG-379Lb 4.13.3microlensing110000.56 [51]
MOA-2010-BLG-328Lb 0.028950.92microlensing26000.11 [52]
MOA-2011-BLG-262Lb 0.0566340.3831microlensing228300.13300Host star may be a rogue planet, planet may be an exomoon [53]
MOA-2011-BLG-262L 4 N/A microlensing228303300Host star may be a rogue planet, planet may be an exomoon [53]
MOA-2011-BLG-293Lb 4.81.1microlensing252000.86 [54]
MOA-2011-BLG-322Lb 11.64.3microlensing247000.39 [55]
OGLE-2011-BLG-0251Lb 0.532.72microlensing84000.26 [56]
OGLE-2012-BLG-358Lb 1.850.87microlensing57000.02Orbiting a brown dwarf [57]
OGLE-2012-BLG-406Lb 2.733.45microlensing162000.44 [58]
Omega Serpentis b 1.7277.021.1radial vel.263.02.174770 [15]
PH2b 0.903282.52550.828281transit1130±100.945629 [59] Also called Kepler-86b
POTS-1b 2.310.9413.16062960.03734transit39000.694400 [60]
PSO J318.5−22 6.51.53 N/A N/A 1160imaging80 N/A N/A Rogue planet [61]
ROXs 12b 16210imaging3900.873850 [62]
ROXs 42Bb 9157imaging4401 [62]
WASP-8c 9.4543235.28radial vel.2801.035600 [63]
WASP-65b 1.551.1122.31142430.0334transit10000.935600 [64]
WASP-68b 0.951.245.0842980.06206transit962±81.245911 [65]
WASP-69b 0.261.0573.86813820.04525963transit1600.834715 [66]
WASP-70Ab 0.591.1643.71302030.048531387transit8001.115763 [66]
WASP-73b 1.881.164.087220.055121790transit1042±91.346036 [65]
WASP-75b 1.071.272.4841930.0375transit8501.146100 [64] [67]
WASP-76b 0.921.831.8098860.0332190transit3901.466250 [68]
WASP-80b 0.5380.9993.067852340.0344transit2000.584143 [69] Proper name Wadirum
WASP-82b  [ fr ]1.241.672.7057820.04472190transit6501.636490 [68]
WASP-84b 0.6940.9428.52348650.0771797transit4100.845314 [66]
WASP-88b 0.561.74.9540.064311775transit1730±301.456431 [65]
WASP-90b 0.63±0.071.63±0.093.916243±0.0000030.0562±0.00121840±50transit1100±2001.55±0.106440±130 [68]
WASP-95b 1.13+0.1
0.04
1.21±0.062.184673±0.00000140.03416±0.000831570±50transit450±21.11±0.095630±130 [70]
WASP-96b 0.48±0.031.2±0.063.4252602±0.00000270.0453±0.00131285±40transit1161±151.06±0.095540±140 [70]
WASP-97b 1.32±0.051.13±0.062.07276±0.0000010.03303±0.000561555±40transit494.9±1.71.12±0.065640±100 [70]
WASP-98b 0.83±0.071.10±0.042.96264036±0.00000130.03762±0.0011180±30transit926±50.69±0.065525±130 [70]
WASP-99b 2.78±0.131.10+0.08
0.05
5.75251±0.000040.0717±0.00161480±40transit519±21.48±0.106180±100 [70]
WASP-100b 2.03±0.121.69±0.292.849375±0.0000080.0457±0.00102190±140transit1201±91.57±0.106900±120 [70]
WASP-101b 0.50±0.041.41±0.053.585722±0.0000040.0506±0.00091560±35transit660±31.34±0.076400±110 [70]
WTS-2b 1.121.3631.01870680.018552000transit33000.825000 [71] [72]

Specific exoplanet lists

Lists of exoplanets

Lists of exoplanet by year of discovery

Related Research Articles

HAT-P-7 is a F-type main sequence star located about 1088 light-years away in the constellation Cygnus. The apparent magnitude of this star is 10.5, which means it is not visible to the naked eye but can be seen with a small telescope on a clear dark night.

Kepler-18 is a star with almost the same mass as the Sun in the Cygnus constellation.

HAT-P-17 is a K-type main-sequence star about 92.6 parsecs (302 ly) away. It has a mass of about 0.857 ± 0.039 M. It is the host of two planets, HAT-P-17b and HAT-P-17c, both discovered in 2010. A search for a binary companion star using adaptive optics at the MMT Observatory was negative. A candidate companion was detected by a spectroscopic search of high-resolution K band infrared spectra taken at the Keck observatory.

Kepler-80, also known as KOI-500, is a red dwarf star of the spectral type M0V. This stellar classification places Kepler-80 among the very common, cool, class M stars that are still within their main evolutionary stage, known as the main sequence. Kepler-80, like other red dwarf stars, is smaller than the Sun, and it has both radius, mass, temperatures, and luminosity lower than that of our own star. Kepler-80 is found approximately 1,223 light years from the Solar System, in the stellar constellation Cygnus, also known as the Swan.

Kepler-32 is an M-type main sequence star located about 1070 light years from Earth, in the constellation of Cygnus. Discovered in January 2012 by the Kepler spacecraft, it shows a 0.58 ± 0.05 solar mass (M), a 0.53 ± 0.04 solar radius (R), and temperature of 3900.0 K, making it half the mass and radius of the Sun, two-thirds its temperature and 5% its luminosity.

Kepler-65 is a subgiant star slightly more massive than the Sun and has at least four planets.

Kepler-88 is a Sun-like star in the constellation of Lyra, with three confirmed planets. In April 2012, scientists discovered that a Kepler candidate known as KOI-142.01 (Kepler-88b) exhibited very significant transit-timing variations caused by a non-transiting planet. Timing variations were large enough to cause changes to transit durations to Kepler-88b as well. Large transit-timing variations helped to put tight constraints to masses of both planets. The non-transiting planet was further confirmed through the radial velocity method in November 2013.

<span class="mw-page-title-main">Kepler-25</span> Yellow-white hued star in the constellation Lyra

Kepler-25 is a star in the northern constellation of Lyra. It is slightly larger and more massive than the sun with a luminosity 212 times that of the sun. With an apparent visual magnitude of 10.6, this star is too faint to be seen with the naked eye.

Kepler-30 is a star in the northern constellation of Lyra. It is located at the celestial coordinates: Right Ascension 19h 01m 08.0747s Declination +38° 56′ 50.219″. With an apparent visual magnitude of 15.5, this star is too faint to be seen with the naked eye. Kepler-30 is exhibiting a strong starspot activity.

<span class="mw-page-title-main">KOI-256</span> Double star in the constellation Cygnus

KOI-256 is a double star located in the constellation Cygnus approximately 575 light-years (176 pc) from Earth. While observations by the Kepler spacecraft suggested the system contained a gas giant exoplanet orbiting a red dwarf, later studies determined that KOI-256 was a binary system composed of the red dwarf orbiting a white dwarf.

<span class="mw-page-title-main">GJ 3470 b</span> Hot Neptune orbiting GJ 3470

GJ 3470 b is an exoplanet orbiting the star GJ 3470, located in the constellation Cancer. With a mass of just under 14 Earth-masses and a radius approximately 4.3 times that of Earth's, it is likely something akin to Neptune despite the initially strong belief that the planet was not covered in clouds like the gas giants in the Solar System.

HAT-P-16 is a F-type main-sequence star about 740 light-years away. The star has a concentration of heavy elements slightly higher than solar abundance, and low starspot activity. The survey in 2015 have failed to find any stellar companions to it. The spectral analysis in 2014 have discovered the HAT-P-16 has a carbon to oxygen molar ratio of 0.58±0.08, close to Sun`s value of 0.55.

HAT-P-15 is a G-type main-sequence star about 630 light-years away. The star is older than Sun yet has a concentration of heavy elements roughly 190% of solar abundance. The star has no noticeable starspot activity.

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