List of exoplanets with Bayer designations

Last updated

This is a list of confirmed exoplanets with Bayer designations.

Star Exoplanet Mass
(MJ)
Semimajor axis
(AU)
Orbital period DiscoveredDiscovery methodReference
α Arietis b 1.8±0.21.2380.8±0.3 d 2011 Radial velocity [1]
α Tauri b 5.8±0.71.46±0.27628.96±0.9 d 2015 Radial velocity [2]
β Cancri b 7.8±0.81.7±0.1605.2±4 d 2014 Radial velocity [3]
β Pictoris b 11.729+1.175
−2.135
10.018+0.082
−0.076
23.593+0.248
−0.209
d
2008 Infrared [4]
β Pictoris c 10.139+1.175
−1.031
2.680+0.016
−0.015
3.266+0.015
−0.012
d
2020 Direct imaging [5]
β Ursae Minoris b 6.1±1.01.4±0.1522.3±2.7 d 2014 Radial velocity [6]
γ Cephei A b 9.4+0.7
−1.1
2.05±0.06903.3±1.5 d 2002 Doppler spectroscopy [7]
γ1 Leonis b  ?1.19429 d 2009 Radial velocity [8]
γ Librae b 1.021.24415.2 d 2018 Radial velocity [9]
γ Librae c 4.582.17964.6±3.1 d 2018 Radial velocity [10]
γ Piscium b 1.34+0.02
−0.31
1.32+0.05
−0.08
555.1+6.0
−2.5
d
2021 Radial velocity [11]
ε Coronae Borealis b 6.7±0.31.3417.9±0.5 d 2012 Radial velocity [12]
ε Eridani b 0.63+0.12
−0.04
3.52±0.042775±5 d 2000 Doppler spectroscopy [13]
ε Indi A b 3.0±0.18.8+0.2
−0.1
10932+266
−228
d
2018 Radial velocity [14]
ε Tauri b 7.6±0.21.93±0.03645.5±5.3 d 2007 Doppler spectroscopy [15]
ι Draconis b 16.4+9.3
−4
1.453±0.026510.854±0.013 d 2002 Doppler spectroscopy [16]
ι Draconis c 17.0+13
−5.4
19.4+10
−7.7
68+60
−36
d
2021 Radial velocity [17]
κ Andromedae b 13+12
−2
57±133242±900 y 2012 Direct imaging [18]
κ Coronae Borealis b 1.811±0.0572.65±0.131285±142012 Radial velocity [19]
μ Arae b 1.65±0.0091.522±0.001643.25±0.90 d 2000 Doppler spectroscopy [20]
μ Arae c 0.032±0.0020.09094±0.0000059.6386±0.0015 d 2004 Radial velocity [21]
μ Arae d 0.448±0.0110.9210±0.00151310.55±0.83 d 2006 Doppler spectroscopy [22]
μ Arae e 5.2354205.8±758.9 d 2002 Radial velocity [23]
μ Leonis b 2.4±0.41.1±0.1357.8±1.2 d 2014 Radial velocity [24]
μ2 Scorpii b 14.4±0.8242.4+114.5
−52.1
 ?2022 Direct imaging [25]
ν Octantis A b 2.10591.276414.8 d 2021 Radial velocity [26]
ν Ophiuchi b 81.7±22.21.803530.73±0.10 d 2012 Radial velocity [27]
ν Ophiuchi c 92±24.76.0223188.95±6.26 d 2012 Radial velocity [28]
ξ Aquilae b 2.80.68136.75±0.252008 Radial velocity [29]
ο Coronae Borealis b 1.50.83187.83±0.54 d 2012 Radial velocity [30]
ο Ursae Majoris b 4.13.91630±35 d 2012 Radial velocity [31]
π Mensae b 12.325+1.192
−1.384
3.311+0.134
−0.148
5.719±0.001 y 2001 Doppler spectroscopy [32]
π Mensae c 3.63±0.380.06839±0.00056.267852±0.000016 d 2014 Transit [33]
π Mensae d 3.63±0.38 ?124.64+0.48
−0.52
d
2023 Radial velocity [34]
ρ1 Cancri b 0.824±0.0070.115±0.000001114.65162±0.0007 d 1996 Radial velocity [35]
ρ1 Cancri c 51.2±1.30.240±0.0000544.3446±0.007 d 2002 Radial velocity [36]
ρ1 Cancri d 3.12±0.15.77±0.115218±230 d 2002 Radial velocity [37]
ρ1 Cancri e 7.99+0.32
−0.33
0.01544±0.0000517.67711 h 2004 Radial velocity [38]
ρ1 Cancri f 7.70±0.080.781±0.007260±1.1 d 2005 Doppler spectroscopy [39]
ρ Coronae Borealis b 1.093±0.0230.2245+0.0023
−0.0024
39.8438±0.0027 d 1997 Radial velocity [40]
ρ Coronae Borealis c 28.2±1.50.4206+0.0044
−0.0024
102.19+0.27
−0.22
d
2016 Radial velocity [41]
ρ Coronae Borealis d 21.6±2.50.827±0.011282.2+2.2
−3.7
d
2023 Radial velocity [42]
ρ Coronae Borealis e 3.79+0.53
−0.54
0.1061±0.001112.949±0.014 d 2023 Radial velocity [43]
τ Boötis b 5.5±60.04813.312463±0.000014 d 1996 Radial velocity [44]
τ Ceti e 3.93+0.83
−0.64
0.538±0.006162.87+1.08
−0.46
d
2012 Radial velocity [45]
τ Ceti f 3.93+1.05
−1.37
1.334+0.017
−0.044
636.13+11.70
−47.69
d
2012 Direct imaging [46]
τ Ceti g 1.75+0.25
−0.40
0.133+0.001
−0.002
20+0.02
−0.01
d
2017 Radial velocity [47]
τ Ceti h 1.83+0.68
−0.26
0.243±0.00349.41+0.08
−0.10
d
2017 Radial velocity [48]
τ Geminorum b 20.61.17305.5±0.1 d 2004 Radial velocity [49]
υ Andromedae b 1.7+0.33
−0.24
0.0594±0.00034.61711±0.000014 d 1996 Radial velocity [50]
υ Andromedae c 13.98+2.3
−5.3
0.829±0.043241.26±0.64 d 1999 Radial velocity [51]
υ Andromedae d 10.25+0.7
−3.3
0.1061±0.00111.27646±0.57 d 1999 Radial velocity [52]
υ Leonis b 0.51+0.06
−0.26
1.18+0.11
−0.32
385.2+2.8
−1.3
d
2021 Radial velocity [53]
ψ1 Aquarii b 3.20.7181.4±0.1 d 2013 Radial velocity [54]
ω Serpentis b 1.71.q277.02+0.52
−0.51
d
2013 Radial velocity [55]

See also

Related Research Articles

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<span class="mw-page-title-main">Rho Coronae Borealis</span> Star in the constellation Corona Borealis

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<span class="mw-page-title-main">Tau Boötis b</span> Hot Jupiter orbiting Tau Boötis A

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<span class="mw-page-title-main">55 Cancri b</span> Extrasolar planet in the constellation Cancer

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<span class="mw-page-title-main">55 Cancri c</span> Extrasolar planet in the constellation Cancer

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<span class="mw-page-title-main">Upsilon Andromedae b</span> Extrasolar planet in the Andromeda constellation

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<span class="mw-page-title-main">Upsilon Andromedae c</span> Extrasolar planet in the Andromeda constellation

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<span class="mw-page-title-main">55 Cancri f</span> Extrasolar planet in the constellation Cancer

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<span class="mw-page-title-main">14 Andromedae b</span> Extrasolar planet in Andromeda constellation

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<span class="mw-page-title-main">Discoveries of exoplanets</span> Detecting planets located outside the Solar System

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The exoplanet naming convention is an extension of the system used for naming multiple-star systems as adopted by the International Astronomical Union (IAU). For exoplanets orbiting a single star, the name is normally formed by taking the name of its parent star and adding a lowercase letter. A provisional IAU-sanctioned standard exists to accommodate the naming of planets that orbit two stars, which are known as circumbinary planets. A limited number of exoplanets have IAU-sanctioned proper names. Other naming systems exist.

References

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