List of exoplanets discovered in 2011

Last updated

This is a List of exoplanets discovered in 2011. [1]

Contents

For exoplanets detected only by radial velocity, the mass value is actually 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
7 Canis Majoris b 1.85735.11.758radial vel.64.651.344826 [2]
82 G. Eridani b 0.008518.3150.1207660radial vel.19.570.75401 [3]
82 G. Eridani c 0.007640.1140.2036508radial vel.19.570.75401 [3]
82 G. Eridani d 0.01590.3090.3499388radial vel.19.570.75401 [3]
BD+48 738 b 0.91392.61.0radial vel.29100.744414 [4]
CFBDSIR J145829+101343 b 10.510037.52.6370imaging75.340.02580Likely brown dwarf [5]
CoRoT-16b 0.5351.175.352270.06181086transit27401.15650 [6]
CoRoT-17b 2.431.023.76810.04611626transit30011.045740 [7]
CoRoT-18b 3.471.311.90006930.02951550transit28380.955440 [8]
CoRoT-19b 1.111.293.897130.05182000transit25111.216090 [9]
CoRoT-20b 4.30.849.242850.091024transit28191.144947 [10]
COROT-21b 2.26±0.311.30±0.142.72474±0.000140.0417±0.0011transit4560±9301.29±0.096200±100 [11]
CoRoT-23b 2.81.053.63130.0481660transit19571.145900 [12]
Gliese 433 b 0.019017.37050.062radial vel.29.580.483461 [13]
Gliese 667 Cc 0.01228.140.125radial vel.22.180.333350 [13] Potentially habitable exoplanet
Gliese 785 b 0.053274.720.32355radial vel.28.70.85166 [3]
Gliese 785 c 0.076525.81.18185radial vel.28.70.85166 [3]
HAT-P-27b 0.621.023.0395770.04transit665.380.945300 [14]
HAT-P-28b 0.6261.2123.2572150.04341384transit12881.025680 [15]
HAT-P-29b 0.881.175.723190.06671271transit10321.456087 [15] Proper name Surt
HAT-P-30b 0.831.442.81060.04191630transit702.21.556304Independent discoveries [16] [17]
HAT-P-31b 2.271.095.005420.0611450transit11331.316065Additional planet in system suspected. [18]
HAT-P-32b 0.681.982.15000820.033971836transit950.811.136001 [19]
HAT-P-33b 0.921.853.474470.049951782transit13061.826446 [19]
HD 1461 c 0.0175913.50520.1117radial vel.76.51.025765 [20] Planet confirmed in 2015 [21]
HD 1502 b 2.75428.51.262radial vel.626.111.464947 [22] Proper name Indépendance
HD 5891 b 7.63177.110.64radial vel.932.021.934673 [22]
HD 7199 b 0.276151.36radial vel.118.040.775371 [23] Proper name Hairu
HD 7449 A b 0.5081255.52.38radial vel.126.261.056024 [23]
HD 14651 b 47±3.479.4179±0.00210.361±0.013radial vel.1270.96±0.035491±26Brown dwarf or star [24]
HD 18742 b 3.47661.82radial vel.532.861.364940 [22] Proper name Bagan
HD 20003 b 0.0378±0.003111.849±0.0030.0974±0.0016radial vel.136.6±0.20.942±0.0465510+48
137
[20]
HD 20003 c 0.0422±0.004033.823±0.0650.1961±0.0032radial vel.136.6±0.20.942±0.0465510+48
137
[20]
HD 20781 b 0.0334+0.0038
0.0037
29.158+0.0102
0.01
0.1647+0.0076
0.0083
radial vel.115.36±4.40.75256±29 [20]
HD 20781 c 0.0442±0.004985.5073+0.0983
0.0947
0.3374+0.0155
0.017
radial vel.115.36±4.40.75256±29 [20]
HD 21693 b 0.0259+0.0034
0.0033
0.197622.6786+0.0085
0.0087
0.1455+0.0058
0.0063
radial vel.105.61±1.660.85430±26 [20] Confirmed in 2017. [25]
HD 21693 c 0.0547±0.005653.7357+0.0312
0.0309
0.2586+0.0103
0.0113
radial vel.105.61±1.660.85430±26 [20] Confirmed in 2017. [25]
HD 22781 b 13.65528.071.167radial vel.106.430.755027 [24]
HD 28678 b 1.542380.21.18radial vel.622.721.534972 [22] Proper name Tassili
HD 30246 b 55.1+20.3
8.2
990.7±5.62.012±0.069radial vel.1601.05±0.045833±44Brown dwarf or star [24]
HD 30856 b 1.5478471.85radial vel.429.561.174895 [22] Proper name Nakanbé
HD 31527 b 0.0329±0.002816.5535+0.0034
0.0035
0.1254+0.0041
0.0045
radial vel.125.8±2.90.965898±13 [20] Planet confirmed in 2017 [25]
HD 31527 c 0.0445±0.0040.003951.2053+0.0373
0.0368
0.2663+0.0088
0.0095
radial vel.125.8±2.90.965898±13 [20] Planet confirmed in 2017 [25]
HD 31527 d 0.0372+0.0053
0.0052
271.6737+2.1135
2.2471
0.8098+0.0273
0.0293
radial vel.125.8±2.90.965898±13 [20] Planet confirmed in 2017 [25]
HD 33142 b 1.3853261.07radial vel.397.271.414978 [22]
HD 39194 b 0.01265.630.056±0.001radial vel.71.430.67±0.045205±23 [20] Confirmed in 2017 and 2021. [26] [27]
HD 39194 c 0.019814.030.103±0.002radial vel.71.430.67±0.045205±23 [20] Confirmed in 2017 and 2021. [26] [27]
HD 39194 d 0.012633.910.185±0.033radial vel.71.430.67±0.045205±23 [20] Confirmed in 2017 and 2021. [26] [27]
HD 45184 b 0.0384+0.0033
0.0032
5.8854±0.00030.0644+0.002
0.0021
radial vel.71.36±0.621.035869±14 [20] Confirmed in 2017 [26]
HD 51608 b  [ ru ]0.0402+0.0038
0.0037
14.0726±0.00160.1059+0.0043
0.0046
radial vel.113.6±2.020.85358±22 [20] Confirmed in 2017. [26] [25]
HD 51608 c  [ ru ]0.045+0.0051
0.0048
95.9446+0.1555
0.1366
0.3809+0.0153
0.0164
radial vel.113.6±2.020.85358±22 [20] Confirmed in 2017. [26] [25]
HD 82886 b 2.337051.58radial vel.415.932.534953 [22] Proper name Arber
HD 85512 b 0.0158.430.26298radial vel.36.790.434300 [3]
HD 93385 Ac 0.022313.180.112±0.002radial vel.141.6±0.21.04±0.015823±35 [20] Originally planet HD 93385 b, confirmed in 2017, [26] renamed in 2021 [27]
HD 93385 Ad 0.027445.840.2565±0.0043radial vel.141.6±0.21.04±0.015823±35 [20] Originally planet HD 93385 c, confirmed in 2017, [26] renamed in 2021. [27]
HD 96063 b 1.27362.51.11radial vel.458.661.375020 [22] Proper name Ramajay
HD 96127 b 20.96647.31.42radial vel.194910.943943 [4] Likely not a planet, but a star [28]
HD 96700 b 0.02808.120.0777±0.0013radial vel.84±10.89±0.015845±13 [20] Also unconfirmed planet between orbits b and c [27]
HD 96700 c 0.0400103.50.424±0.007radial vel.84±10.89±0.015845±13 [20] Also unconfirmed planet between orbits b and c [27]
HD 98219 b 1.964433.81.26radial vel.372.061.414925 [22] Proper name Ixbalanqué
HD 99706 b 1.238411.98radial vel.480.151.464862 [22]
HD 100655 b 1.61157.570010.68radial vel.449.22.284891 [29] Proper name Sazum
HD 102329 b 8.16778.11.81radial vel.712.413.214745 [22]
HD 106270 b 10.1318883.34radial vel.306.791.395509 [22]
HD 108863 b 2.414437.71.32radial vel.539.871.594878 [22]
HD 116029 b 1.46701.65radial vel.403.40.834819 [22] One more planet in the system (unconfirmed)
HD 126525 b 0.237±0.002960.41+6.19
6.33
1.837±0.010radial vel.124.1+4.3
4.6
0.90±0.015638±13 [20]
HD 131496 b 1.88962.01radial vel.431.651.344846 [22] Proper name Madriu
HD 132563 Bb 1.4915442.62radial vel.344.011.086073 [30]
HD 134060 b 0.0318+0.0025
0.0024
3.2696±0.00010.0444±0.0007radial vel.78.38±0.071.0955966±14 [20] Eccentric orbit, confirmed in 2017. [25]
HD 134060 c 0.0922+0.0139
0.0133
1292+48
44
2.226±0.051radial vel.78.38±0.071.0955966±14 [20] Confirmed in 2017. [25]
HD 134606 b 0.0292±0.003012.083±0.0100.1023±0.0017radial vel.87.45±0.070.998±0.0245616±34 [20]
HD 134606 c 0.0382±0.005359.52±0.170.2962±0.0049radial vel.87.45±0.070.998±0.0245616±34 [20]
HD 134606 d 0.1212±0.0130459.3±8.31.157±0.024radial vel.87.45±0.070.998±0.0245616±34 [20]
HD 137388 b 0.23300.89radial vel.132.20.685181 [23] Proper name Kererū
HD 142245 b 3.0712992.78radial vel.318.013.54922 [22]
HD 152581 b 1.869686.51.66radial vel.543.21.35027 [22] Proper name Ganja
HD 156279 b 9.88131.050.49radial vel.118.170.955453 [24]
HD 158038 b 1.535211.5radial vel.310.251.34860 [22]
HD 150433 b 0.168±0.0201096±271.930±0.045radial vel.99.36±0.10 [20]
HD 154088 b 0.020818.56±0.010.134±0.002radial vel.58.2±0.50.91±0.025374±43 [20] Confirmed in 2021 [27]
HD 157172 b 0.12104.84±0.130.416±0.007radial vel.107.75±0.22 [20]
HD 163607 b 0.783675.22030.362radial vel.221.531.125522 [31]
HD 163607 c 2.20112722.39radial vel.221.531.125522 [31]
HD 164509 b 0.443280.170.87radial vel.173.491.125922 [31]
HD 189567 b 0.026714.30.111±0.002radial vel.58.43±0.040.83±0.015726±15 [20] Confirmed in 2021, also unconfirmed planet HD 189567 c in the system [27]
HD 192310 c 0.076525.81.18radial vel.28.70.785069 [3]
HD 204313 c 0.055334.9050.2099radial vel.1541.025776 [20] Confirmed in 2015. [21]
HD 215152 c 0.0054+0.0019
0.0023
7.2824+0.0045
0.0083
0.06739+0.00086
0.00089
radial vel.70.48±0.160.770±0.0154935±76 [20] Confirmed in 2018. [32]
HD 215152 d 0.0088+0.0025
0.0029
10.8650+0.0056
0.0061
0.0880+0.0011
0.0012
radial vel.70.48±0.160.770±0.0154935±76 [20] Confirmed in 2018. [32]
HD 204941 b0.26617332.55radial vel.93.740.585026 [23]
HD 215456 b 0.101191.99±0.730.652±0.011radial vel.129.3±0.2 [20]
HD 215456 c 0.2462277±673.394±0.088radial vel.129.3±0.2 [20]
HD 240237 b 15.89745.71.92radial vel.31258.763926 [4]
HIP 5158 c 15.049017.767.7radial vel.168.560.784962 [33]
HIP 57274 b 0.028.13520.07radial vel.84.410.294510 [34]
HIP 57274 c 0.4090232.030.178radial vel.84.410.294510 [34]
HIP 57274 d 0.5267431.71.01radial vel.84.410.294510 [34]
HU Aquarii b 5.923903.6timing626.890.885952Controversial
HU Aquarii c 4.543685.4timing626.890.885952Controversial
Kepler-10b 0.01450.1320.8374910.01722130transit608.30.915708 [35]
Kepler-10c 0.023190.20745.29460.241584transit608.30.915708 [36]
Kepler-11b 0.0060.16110.30390.091transit21480.965663 [37]
Kepler-11c 0.0090.25613.02410.107transit21480.965663 [37]
Kepler-11d 0.0230.27822.68450.155transit21480.965663 [37]
Kepler-11e 0.0250.37431.99960.195transit21480.965663 [37]
Kepler-11f 0.0060.22246.68880.25transit21480.965663 [37]
Kepler-11g 0.0790.297118.38070.466transit21480.965663 [37]
Kepler-12b 0.4321.7544.43796290.05531480transit29501.175947 [38]
Kepler-13b 9.281.5121.7635880.036412550transit13541.727650 [39]
Kepler-14b 8.41.1366.7901230.07711605transit31961.516395 [40]
Kepler-15b 0.660.964.9427820.057141251transit24641.025515 [41]
Kepler-16b 0.3330.754228.7760.7048transit245.440.694450 [42]
Kepler-17b 2.451.311.48571080.025911570transit26091.165781 [43]
Kepler-18b 0.0220.1783.5047250.0447transit14300.975345 [44]
Kepler-18c 0.0540.497.641590.0752transit14300.975345 [44]
Kepler-18d 0.0520.62314.858880.1172transit14300.975345 [44]
Kepler-19b 0.026430.1979.287160.085transit717.40.945544 [45]
Kepler-19c 0.0412228.731timing717.40.945544 [45]
Kepler-20b 0.030520.1673.696115250.04631105transit929.180.955495 [46]
Kepler-20c 0.040120.27210.854090890.0949772transit929.180.955495 [46]
Kepler-20d 0.031680.24577.611300170.3506401transit929.180.955495 [46]
Kepler-20e 0.010.0776.098522810.06391040transit929.180.955495 [46]
Kepler-20f 0.0450.08919.577584780.1396705transit929.180.955495 [46]
Kepler-21b 0.015980.1462.785780.0427172025transit3701.416305 [47]
Kepler-22b 0.1130.212289.86230.849262transit619.720.975518Potentially habitable exoplanet [48]
Kepler-23b 0.80.177.10730.075transit27931.15828 [49]
Kepler-23c 2.70.28510.74210.099transit27931.15828 [49]
Kepler-24b 1.60.2148.14530.08transit39010.985897 [49]
Kepler-24c 1.60.2512.33350.106transit39010.985897 [49]
Kepler-25b 0.02750.2456.2382970.068transit798.981.196270 [50]
Kepler-25c 0.04790.46512.72070.11transit798.981.196270 [50]
Kepler-26b 0.016110.24812.280.08551427transit11040.543914 [50]
Kepler-26c 0.019510.24317.25590.10725381transit11040.543914 [50]
Kepler-27b 9.110.35715.33480.118transit35070.655400 [50]
Kepler-27c 13.80.43731.33090.191transit35070.655400 [50]
Kepler-28b 1.510.3215.91230.062583transit14480.754590 [50]
Kepler-28c 1.360.3038.98580.081507transit14480.754590 [50]
Kepler-29b 0.014190.29910.33840.09transit27790.985701 [51]
Kepler-29c 0.012590.2813.28840.11transit27790.985701 [51]
Kepler-31b 0.49120.86130.16transit57001.216340 [52]
Kepler-31c 4.70.47342.63180.26transit57001.216340 [52]
Kepler-32b 4.10.1965.901240.05530transit10660.583900 [52]
Kepler-32c 0.50.1788.75220.09470transit10660.583900 [52]
Kepler-33b 0.1555.667930.0677transit40861.295904 [53]
Kepler-33c 0.001230.28513.175620.1189transit40861.295904 [53]
Kepler-33d 0.01230.47721.775960.1662transit40861.295904 [53]
Kepler-33e 0.017530.35931.78440.2138transit40861.295904 [53]
Kepler-39b 20.11.2421.087210.164897transit35571.296350 [54] brown dwarf
Kepler-41b 0.561.291.85555820.031011790transit36801.155750 [55]
Kepler-42b 0.071.21376720.0116519transit126.230.133068 [36]
Kepler-42c 0.0650.453285090.006720transit126.230.133068 [36]
Kepler-42d 0.0511.8651690.0154450transit126.230.133068 [36]
Kepler-43 b 3.231.2193.02409490.0461620transit33791.326041 [43]
Kepler-44b 1.01.093.24672930.04461544transit40091.125800 [43]
Kepler-45b 0.5050.962.4552390.031000transit10860.593820 [53]
Kepler-70b 0.00140.0680.2401040.006orbital brightness modulation38490.527730Controversial [56]
Kepler-70c 0.00210.0770.3428870.0076orbital brightness modulation38490.527730Controversial [56]
MOA-2009-BLG-266Lb 0.03327743.2microlensing99000.56 [57]
Nu2 Lupi b 0.01450.13211.57779+0.00091
0.0011
0.0969+0.0019
0.0017
radial vel.47.85±0.070.87±0.045664±61 [20]
Nu2 Lupi c 0.03550.23327.5909+0.0028
0.0031
0.1729+0.0034
0.0030
radial vel.47.85±0.070.87±0.045664±61 [20]
Nu2 Lupi d 0.02780.229107.245±0.0500.425±0.012radial vel.47.85±0.070.87±0.045664±61 [20]
NY Vir (AB) b 2.331603.3timing18000.633000Circumbinary planet [58]
NY Vir (AB) c 4.499861.757.54timing18000.633000Circumbinary planet [59]
PSR J1719-1438 b 1.20.090706290.0044timing39141.44500Shortest orbital period of any known exoplanet [60]
Qatar-2 b 2.4941.2541.337116470.021531344transit594.670.744645 [61]
TrES-5 1.791.1941.482246860.024591480transit11880.95171 [62]
UZ Fornacis b 6.358405.9timing781.50.75286false positive
UZ Fornacis c 7.71916.252.8timing781.50.75286unconfirmed as in 2020
WASP-35b 0.72±0.061.32±0.033.161580.04317transit663.391.055990 [16]
WASP-39b 0.281.274.0552590.04861166transit750.180.935400 [63] Proper name Bocaprins
WASP-43b 1.780.930.8134750.01421427transit260.930.584400 [64]
WASP-44b 0.871.12.4238040.034531337transit12010.945420 [65]
WASP-45b 0.9640.9463.1260890.039631153transit693.040.855150 [65]
WASP-46b 1.911.1741.430367630.023351636transit12370.835600 [65]
WASP-48b 0.81.52.143630.034442035transit15010.885920 [16]
WASP-50 b 1.46881.1661.95510.02931395transit606.080.895400 [66] Proper name Maeping
WD 0806-661 b 7.52500323imaging62.620.629552Y-type sub-brown dwarf [67]

Specific exoplanet lists

Lists of exoplanets

Lists of exoplanet by year of discovery

Related Research Articles

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-11, also designated GSC 03561-02092 and Kepler-3, is an orange dwarf metal rich star about 123 light-years away in the constellation Cygnus. This star is notable for its relatively large rate of proper motion. The magnitude of this star is about 9, which means it is not visible to the naked eye but can be seen with a medium-sized amateur telescope on a clear dark night. The age of this star is about 6.5 billion years.

Kepler-17 is a main-sequence yellow dwarf star that is much more active than the Sun with starspots covering roughly 6% of its surface. Starspots are long-lived, with at least one persisting for 1400 days.

Kepler-39 is an F-type main sequence star located in the constellation Cygnus. It is located about 3,560 light-years away. One known substellar companion orbits it, Kepler-39b.

Kepler-31 is a star in the northern constellation of Cygnus, the swan. It is orbited by three known exoplanets. It is located at the celestial coordinates: Right Ascension 19h 36m 05.5270s, Declination +45° 51′ 11.106″. With an apparent visual magnitude of 14.0, this star is too faint to be seen with the naked eye.

<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.

Kepler-13 or KOI-13 is a stellar triple star system consisting of Kepler-13A, around which an orbiting hot Jupiter exoplanet was discovered with the Kepler spacecraft in 2011, and Kepler-13B a common proper motion companion star which has an additional star orbiting it.

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-30, also known as WASP-51, is the primary of a binary star system about 700 light-years away. It is a G-type main-sequence star. HAT-P-30 has a similar concentration of heavy elements compared to the Sun.

References

  1. "NASA Exoplanet Archive" . Retrieved 20 December 2019.
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