List of exoplanets discovered in 2015

Last updated

This is a List of exoplanets discovered in 2015.

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 J02192210-3925225 b 13.9+1.1
1.9
1.44156imaging1290.113064 [2]
2MASS J1119-1137 5-1032872.53.6imaging86 [3] [4] Pair of rogue planets
Kepler-451b 1.94060.92timing1340±200.4829564±106Two additional planets in the system [5] [6]
51 Eridani b 213.2700imaging96±1.01.757331±30 [7]
8 Ursae Minoris b 1.593.40.49radial vel.5191.84847.4 [8] Proper name Halla
BD+49 828 b 1.625904.2radial vel.14601.524943 [9]
COROT-28b 0.4840.9555.208510.0603transit18001.015150 [10]
COROT-29b 0.850.92.850570.0386transit25000.975260 [10]
COROT-33b  [ fr ]59.21.15.8191430.0579transit22700.865225Unusually short period brown dwarf [11]
EPIC 203311200 b 0.51±0.055401.2transit1425±1630.91±0.095200±200Single transit only, true period unknown [12]
Gliese 1132 b 0.00510.1031.62893580transit39.30.183270 [13]
HAT-P-50b 1.351.2883.12201090.04531862transit16201.276280 [14]
HAT-P-51b 0.3091.2934.21802780.050691192transit15000.985449 [14]
HAT-P-52b 0.8181.0092.75359530.036941218transit12600.895131 [14]
HAT-P-53b 1.4841.3181.96162410.031591778transit23501.095956 [14]
HAT-P-55b 0.5821.1823.58524670.046041313transit16001.015808 [15]
HAT-P-56b 2.181.4662.79083270.04231840transit10131.36566 [16]
HAT-P-57b 1.851.4132.4652950.04062200transit9901.477500 [17]
HATS-7b 0.120±0.0120.563+0.046
0.034
3.18530.04012±0.000431084±32transit791±50.849±0.0274985±50 [18]
HATS-8b 0.1380.8733.5838930.046671324transit27001.065679 [19] Intensely blue-colored planet [20]
HATS-9b 0.8371.0651.91530730.030481823transit20301.035366 [21]
HATS-10b 0.5260.9693.3128460.044911407transit16201.15880 [21]
HATS-13b 0.5431.2123.04404990.040571244transit15500.965523 [22]
HATS-14b 1.0711.0392.76676410.03815transit16700.975346 [22]
HATS-15b 2.171.1051.747487530.02712transit22500.875311 [23]
HATS-16b 3.271.32.6865020.03744transit25200.975738 [23]
HATS-17b 1.3380.77716.2546110.1308814transit11101.135846 [24]
HD 1605 b 0.96577.91.48radial vel.2761.314757Subgiant host star [25]
HD 1605 c 3.4821113.52radial vel.2761.314757Subgiant host star [25]
HD 1666 b 6.432700.94radial vel.360.81.56317 [25]
HD 7924 c 0.0247315.2990.1134584radial vel.54.90.835075 [26]
HD 7924 d 0.0202624.4510.1551499radial vel.54.90.835075 [26]
HD 11755 b 6.5433.71.08radial vel.7550.94312.5 [8]
HD 12648 b 2.9133.60.54radial vel.5171.24835.8 [8]
HD 24064 b 9.4535.61.29radial vel.86214052.5 [8]
HD 32963 b 0.723723.41radial vel.114.90.945727 [27]
HD 33844 b  [ ru ]1.96551.41.6radial vel.3291.784861 [28]
HD 33844 c  [ ru ]1.759162.24radial vel.3291.784861 [28]
HD 95127 b 5.014821.28radial vel.10801.24218 [9]
HD 95872 b 4.643755.2radial vel.2360.955312 [29]
HD 145934 b  [ fr ]2.2827304.6radial vel.7481.75 [30]
HD 164595 b 0.05078400.23radial vel.94.40.995790 [31]
HD 175607 b 0.0260±0.003929.03±0.03radial vel.147.70.715392Metal-poor host star, additional planet suspected [32]
HD 216536 b 1.47148.60.609radial vel.12401.364639 [9]
HD 219134 b 0.014910.1433.0929260.03876radial vel.21.40.814699 [33]
HD 219134 c 0.013720.1356.764580.0653radial vel.21.40.814699 [33]
HD 219134 d 0.050880.14446.8590.237radial vel.21.40.814699 [33]
HD 219134 f 0.022970.11722.7170.1463radial vel.21.40.814699 [33]
HD 219134 g 0.03494.20.3753radial vel.21.40.814699 [33]
HD 219134 h 0.308±0.0142100.6±2.93.11radial vel.21.40.814699 [33] [34]
HIP 65891 b 61084.52.81radial vel.4922.55000 [35] Host star also known as HD 117253
HIP 107773 b 1.98144.30.72radial vel.3442.424945 [35] Host star also known as HD 207229
K2-3b 0.19410.054490.0769463transit143.90.63896 [36] [37]
K2-3c 0.16524.643540.1399344transit143.90.63896 [36] [37]
K2-3d 0.13544.559830.2076282transit143.90.63896 [36] [37]
K2-4b 0.21110.003290.0777transit7610.634197 [36]
K2-5b 0.175.735940.0532transit6660.613930 [36]
K2-5c 0.20210.932410.0818transit6660.613930 [36]
K2-6b 0.22330.941910.1898transit10400.975850 [36]
K2-7b 0.23828.679920.1814transit24600.975772 [36]
K2-8b 0.31910.352390.0856transit13300.784870 [36] Unconfirmed in 2016 [38]
K2-9b 0.20118.44980.091transit3600.33390 [36]
K2-10b 0.084950.34319.3044transit8800.925620 [36]
K2-11b 0.67439.937670.2257transit65901.355433 [36]
K2-12b 0.2088.282120.0802transit9601.015800 [36]
K2-13b 0.16939.914880.2114transit9500.85698 [36]
K2-14b 0.4298.368020.0627transit7100.473789 [36]
K2-15b 0.22111.81040.091transit14300.725131 [36]
K2-16b 0.187.61880.0667658transit10600.684742 [36]
K2-16c 0.22719.078630.1229485transit10600.684742 [36]
K2-17b 0.19917.967530.119transit4400.714320 [36]
K2-18b 0.232.944880.1491transit124.20.413503 [36]
K2-19b 0.0900.6917.91940.074854transit9500.935430 [36] [39]
K2-19c 0.0810.43411.907150.0971745transit9500.935430 [36] [39]
K2-21b 0.1429.324140.0731transit2100.644043 [40]
K2-21c 0.17115.50120.1026transit2100.644043 [40]
K2-22b 1.40.2230.3810780.0088transit7300.63830 [41]
K2-25b 0.3063.484552transit1490.293180Parent star, also known as EPIC 210490365, belongs to Hyades [42]
K2-28b 0.2072.2604550.0214transit1700.263214 [43]
KELT-4Ab 0.9021.6992.98959320.043171827transit6801.26206 [44]
KELT-6c 3.7112762.39radial vel.7201.136272 [45]
KELT-7b 1.28±0.171.496±0.0352.73477490.0434±0.00122028±17transit442±21.517±0.0226699±24 [46] [47]
KELT-8b 0.8671.863.244060.045711675transit7701.215754 [48]
KELT-10b 0.6791.3994.16627390.05251377transit6001.115948 [49]
KELT-14b 1.2841.7431.71005660.03005transit8701.245720Host star also known as WASP-122 [50] [51]
KELT-15b 0.911.4433.3294410.04613transit9501.186003 [50]
Kepler-455b 0.6161322.3transit41000.986175 [52] Host star also known as KIC 3558849
Kepler-460b 0.571440.7813transit43301.076340 [52] Host star also known as KIC 5437945
Kepler-456b 0.5891320.1transit24800.986258 [52] Host star also known as KIC 5951458
Kepler-458b 0.41572.3847transit55000.986065 [52] Host star also known as KIC 9663113
Kepler-459b 0.491854.083transit50001.016091 [52] Host star also known as KIC 10525077
Kepler-457b 0.36631.8099transit36101.046474 [52] Host star also known as KIC 8540376
Kepler-457c 0.21475.2transit36101.046474 [52] Host star also known as KIC 8540376
KOI-12b 101.4317.85523330.151transit13901.456820Host star also known as Kepler-448 [53]
KOI-4427.01 0.208147.66060.42transit7830.5263813Potentially habitable exoplanet, false positive probability 0.8%. [54] Also a red dwarf in the system. [55]
Kepler-92d 0.18449.3568transit1580±171.215883 [56]
Kepler-433b 2.821.455.334083840.0679transit61001.466360Host star also known as KOI-206 [57]
Kepler-434b 2.861.1312.87470990.1143transit40001.25977Host star also known as KOI-614 [57]
Kepler-435b 0.841.998.60015360.0948transit68001.546161Host star also known as KOI-680 [57]
Kepler-436b 0.2464.002050.339transit20200.734651Host star also known as KOI-2529 [54]
Kepler-437b 0.1966.650620.288transit13600.714551Host star also known as KOI-3255 [54]
Kepler-438b 0.135.233190.166transit4700.543748Host star also known as KOI-3284 [54]
Kepler-439b 0.2178.13960.563transit22600.885431Host star also known as KOI-4005 [54]
Kepler-440b 0.17101.111410.242transit8500.574134Host star also known as KOI-4087 [54]
Kepler-441b 0.15207.24820.64transit9300.574340Host star also known as KOI-4622 [54]
Kepler-442b 0.12112.30530.409transit11200.614402Potentially habitable exoplanet, host star also known as KOI-4742 [54]
Kepler-443b 0.21177.66930.495transit25400.744723Host star also known as KOI-4745 [54]
Kepler-444b 0.0363.60010530.04178transit1160.765046 [56]
Kepler-444c 0.0444.54588410.04881transit1160.765046 [56]
Kepler-444d 0.0476.1893920.06transit1160.765046 [56]
Kepler-444e 0.0497.7434930.0696transit1160.765046 [56]
Kepler-444f 0.0669.7404860.0811transit1160.765046 [56]
Kepler-445b 0.142.984151transit2900.183157 [58]
Kepler-445c 0.224.871229transit2900.183157 [58]
Kepler-445d 0.118.15275transit2900.183157 [58]
Kepler-446b 0.131.565409transit3900.223359 [58]
Kepler-446c 0.13.036179transit3900.223359 [58]
Kepler-446d 0.125.148921transit3900.223359 [58]
Kepler-447b 1.371.657.794301320.0769transit881±615493 [59]
Kepler-449b 0.18312.58242transit8480.97 [56] Stellar companion in system [60]
Kepler-449c 0.24733.6727transit8480.97 [56] Stellar companion in system [60]
Kepler-450b 0.54828.454851transit1506±171.35 [56]
Kepler-450c 0.23415.413135transit1506±171.35 [56]
Kepler-450d 0.0757.51464transit1506±171.35 [56]
Kepler-454b 0.021520.21110.573753390.0954transit758±41.035701 [61]
Kepler-454c 4.46523.9radial vel.758±41.035701 [61]
MOA-2010-BLG-353Lb 0.271.72microlensing210000.18 [62]
MOA-2011-BLG-028Lb 0.094394.14microlensing241000.75 [63]
MOA-2013-BLG-605Lb 0.010070.94microlensing0.03 [64]
OGLE-2012-BLG-0563Lb 0.390.9microlensing42000.34 [65]
OGLE-2015-BLG-0966Lb 0.066072.1microlensing82000.38 [66] [67]
Psi1 Draconis Bb 1.5331174.43radial vel.72.31.196212 [29]
VHS 1256-1257 b 11.8±0.26,200,000+2,900,000
4,000,000
360+110
150
imaging69.0±0.70.089+0.010
0.010
2620±140 [68] [69]
WASP-41c 3.184211.07241radial vel.5900.935545 [70]
WASP-47c 1.57580.71.41247radial vel.6501.115576 [70]
WASP-47d 0.052860.3319.0950.088transit6501.115576 [71] [70]
WASP-47e 0.028630.1620.7896360.0173transit6501.115576 [71] [70]
WASP-120b 4.851.4733.61127060.05141890transit14301.396450 [51]
WASP-121b 1.183+0.064
0.062
1.865±0.0441.2749255+0.00000020
0.00000025
0.02544+0.00049
0.00050
2358±52timing858±21.353+0.080
0.079
6459±140 [72]
WASP-123b 0.8991.3182.97764120.042631510transit7001.175740 [51]
WASP-135b 1.90±0.081.30±0.091.4013794±0.00000080.0243±0.0005transit980±1500.98±0.065675±60 [73]
Wolf 1061b 0.006014.88690.0375radial vel.14.04±0.030.293342 [74]
Wolf 1061c 0.0107317.87190.089radial vel.14.04±0.030.293342Potentially habitable exoplanet [74]
Wolf 1061d 0.02423217.210.47radial vel.14.04±0.030.293342 [74]

Specific exoplanet lists

Lists of exoplanets

Lists of exoplanets by year of discovery

Related Research Articles

<span class="mw-page-title-main">Hot Jupiter</span> Class of high-mass planets orbiting close to a star

Hot Jupiters are a class of gas giant exoplanets that are inferred to be physically similar to Jupiter but that have very short orbital periods. The close proximity to their stars and high surface-atmosphere temperatures resulted in their informal name "hot Jupiters".

The Hungarian Automated Telescope Network (HATNet) project is a network of six small fully automated "HAT" telescopes. The scientific goal of the project is to detect and characterize extrasolar planets using the transit method. This network is used also to find and follow bright variable stars. The network is maintained by the Center for Astrophysics | Harvard & Smithsonian.

WASP-11/HAT-P-10 is a binary star. It is a primary main-sequence orange dwarf star. Secondary is M-dwarf with a projected separation of 42 AU. The system is located about 424 light-years away in the constellation Aries.

HAT-P-27, also known as WASP-40, is the primary of a binary star system about 659 light-years away. It is a G-type main-sequence star. The star's age is similar to the Sun's at 4.4 billion years. HAT-P-27 is enriched in heavy elements, having a 195% concentration of iron compared to the Sun.

<span class="mw-page-title-main">Mini-Neptune</span> Planet smaller than Neptune with a gas atmosphere

A Mini-Neptune is a planet less massive than Neptune but resembling Neptune in that it has a thick hydrogen-helium atmosphere, probably with deep layers of ice, rock or liquid oceans.

K2-19 is an early K-type or late G-type main sequence star that is magnetically active, and has a light curve that exhibits variations in brightness of ~1%. It is located approximately 976 light-years away in the constellation Virgo. Three confirmed transiting exoplanets are known to orbit this star.

WASP-37 is a yellow main sequence star in the constellation of Virgo.

HAT-P-18 is a K-type main-sequence star about 530 light-years away. The star is very old and has a concentration of heavy elements similar to solar abundance. A survey in 2015 detected very strong starspot activity on HAT-P-18.

HAT-P-16 is a F-type main-sequence star about 725 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.

References

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