List of nearest exoplanets


There are known exoplanets, or planets outside the Solar System that orbit a star, as of ; only a small fraction of these are located in the vicinity of the Solar System. Within, there are 106 exoplanets listed as confirmed by the NASA Exoplanet Archive. Among the over 500 known stars and brown dwarfs within 10 parsecs, around 60 have been confirmed to have planetary systems; 51 stars in this range are visible to the naked eye, eight of which have planetary systems.
The first report of an exoplanet within this range was in 1998 for a planet orbiting around Gliese 876, and the latest as of 2025 is a system around Barnard's Star. The closest exoplanets are those found orbiting the star closest to the Solar System, which is Proxima Centauri 4.25 light-years away. The first confirmed exoplanet discovered in the Proxima Centauri system was Proxima Centauri b, in 2016. HD 219134 has six exoplanets, the highest number discovered for any star within this range.
Most known nearby exoplanets orbit close to their stars. A majority are significantly larger than Earth, but a few have similar masses, including planets around YZ Ceti, Gliese 367, Proxima Centauri, and Barnard's Star which may be less massive than Earth. Several confirmed exoplanets are hypothesized to be potentially habitable, with Proxima Centauri b and GJ 1002 b considered among the most likely candidates. The International Astronomical Union has assigned proper names to some known extrasolar bodies, including nearby exoplanets, through the NameExoWorlds project. Planets named in the 2015 event include the planets around Epsilon Eridani and Fomalhaut, while planets named in the 2022 event include those around Gliese 436, Gliese 486, and Gliese 367.

Exoplanets within 10 parsecs

Host star systemHost star systemHost star systemHost star systemCompanion exoplanet Companion exoplanet Companion exoplanet Companion exoplanet Companion exoplanet Companion exoplanet Companion exoplanet Companion exoplanet Companion exoplanet Notes and additional planetary observations
NameDistance

Apparent
magnitude
Mass

Label
Mass
Radius

Semi-major axis

Orbital period

Eccentricity
Inclination

Discovery
method
Discovery yearNotes and additional planetary observations
Sun°0.0000161'0.38290.387'0.2053.38For comparison purposes. One candidate planet
Sun°0.0000161'11'0.01677.25For comparison purposes. One candidate planet
Sun°0.0000161''5.200.04886.09For comparison purposes. One candidate planet
Proxima Centauri#4.24650.123d~0.81 ± 0.080.02895.1220.04RV2025one disputed candidate
Proxima Centauri#4.24650.123b0.941.40.048611.190.02RV2016one disputed candidate
Barnard's Star#5.96299.510.162d0.01882.3400.04RV2025
Barnard's Star#5.96299.510.162b0.02293.1540.03RV2024
Barnard's Star#5.96299.510.162c0.02744.1240.08RV2025
Barnard's Star#5.96299.510.162e0.03816.7390.04RV2025
Lalande 21185#8.3040.46b0.078812.940.06RV20191 candidate
Lalande 21185#8.3040.46c2.940.13RV20211 candidate
Epsilon Eridani10.5010.823183.532,6800.0640RV20001 inferred planet, 1 or possibly 2 inner debris discs, and an outer disc
Lacaille 9352#10.7240.489b0.0689.2620.03RV20191 candidate
Lacaille 9352#10.7240.489c0.12021.790.03RV20191 candidate
Ross 12811.0070.168b0.04969.8660.12RV2017
Gliese 725 A11.4918.940.330b≥2.780.06811.22010.0RV2024
Gliese 725 B11.4919.700.25c≥3.40.13937.90RV2025
Groombridge 34 A#11.6190.38b0.07211.440.09~54?RV2014
Groombridge 34 A#11.6190.38c5.40.27~54?RV2018
Epsilon Indi A11.8670.762b200528.40.40103.7RV2018nearest exoplanet directly imaged
GJ 1061#11.9840.113b0.0213.204<0.31RV2019two solutions for d's orbit
GJ 1061#11.9840.113c0.0356.689<0.29RV2019two solutions for d's orbit
GJ 1061#11.9840.113d0.05413.03<0.53RV2019two solutions for d's orbit
YZ Ceti#12.1220.130b0.01632.0210.06RV2017
YZ Ceti#12.1220.130c0.02163.0600.0RV2017
YZ Ceti#12.1220.130d0.02854.6560.07RV2017
Luyten's Star#12.3480.29c0.03654.7230.10RV20172 candidates
Luyten's Star#12.3480.29b0.091118.650.17RV20172 candidates
Teegarden's Star#12.4970.08b0.02594.9060.03RV2019
Teegarden's Star#12.4970.08c0.045511.420.04RV2019
Teegarden's Star#12.4970.08d0.079126.130.07RV2024
Wolf 1061#14.0500.25b0.03754.8870.15RV2015
Wolf 1061#14.0500.25c0.089017.870.11RV2015
Wolf 1061#14.0500.25d0.4702170.55RV2015
TZ Arietis14.5780.14b0.887710.46RV20192 refuted candidates
Gliese 687#14.8390.41b0.16338.140.17RV2014
Gliese 687#14.8390.41c1.1657280.40RV2019
Gliese 67414.8490.35b0.0394.6940.20RV2007
Gliese 876#15.2380.33d6.680.02101.9380.0456.7RV2005
Gliese 876#15.2380.33c2350.130930.100.2656.7RV2000
Gliese 876#15.2380.33b7490.209861.100.0356.7RV1998
Gliese 876#15.2380.33e160.3355123.60.0556.7RV2010
GJ 1002#15.8060.12b0.045710.35RV2022
GJ 1002#15.8060.12c0.073821.2RV2022
Gliese 83216.2000.45b3153.70.0551 or 134RV20081 refuted candidate
GJ 3323#17.5310.164b0.0328RV2017
GJ 3323#17.5310.164c0.126RV2017
Gliese 251#18.2150.372b0.0808RV2020
Gliese 251#18.2150.372c0.196RV2025
Gliese 752 A19.2920.46b0.3430.10RV2018
82 G. Eridani#19.7040.79b0.1260.06RV2011
82 G. Eridani#19.7040.79c0.3630.08RV2011
82 G. Eridani#19.7040.79d1.3540.45RV2023
HN Librae20.3950.29b0.1420.08RV20231 candidate
EQ Pegasi A20.4000.436b0.6430.3569.2Astrometry2022
Gliese 581#20.5490.295e0.02800.0147RV20093 refuted candidates and a disc
Gliese 581#20.5490.295b0.03990.0347RV20053 refuted candidates and a disc
Gliese 581#20.5490.295c0.07180.0347RV20073 refuted candidates and a disc
Gliese 338 B20.6580.64b0.1410.11RV2020
Gliese 62521.1310.30b0.0784RV2017
HD 219134#21.3360.78b1.600.038885.05RV2015Has 1 candidate planet
HD 219134#21.3360.781.510.06587.28RV2015Has 1 candidate planet
HD 219134#21.3360.780.146~87?RV2015Has 1 candidate planet
HD 219134#21.3360.780.237~87?RV2015Has 1 candidate planet
HD 219134#21.3360.783.11~87?RV2015Has 1 candidate planet
LTT 1445 A#22.3870.26c1.150.0266<0.2287.43Transit20211 candidate
LTT 1445 A#22.3870.26b1.300.0381<0.1189.68Transit20191 candidate
Gliese 39322.9530.41b0.05400.00RV2019
Gliese 667 C#23.6230.330.0490.13~52?RV20095 dubious candidates
Gliese 667 C#23.6230.330.12510.03~52?RV20115 dubious candidates
Gliese 51424.8780.53b0.4211400.45RV2022
GJ 115126.2310.164c0.571390RV20231 refuted candidate
Gliese 48626.3510.321.310.017388.4Transit2021
Gliese 68626.6130.42b0.0970.04RV2019
GJ 128927.27512.670.21b0.271120RV2024
61 Virginis#27.8360.95b0.050.05~77?RV2009a debris disc
61 Virginis#27.8360.95c0.220.06~77?RV2009a debris disc
61 Virginis#27.8360.95d0.470.12~77?RV2009a debris disc
CD Ceti28.0520.161b0.01850RV2020
Gliese 785#28.7390.78b0.320.13RV2010
Gliese 785#28.7390.78c1.18RV2011
Gliese 849#28.7500.49b2.260.05RV2006
Gliese 849#28.7500.49c4.820.087RV2006
Gliese 433#29.6050.48b0.0620.04RV2009
Gliese 433#29.6050.48d0.1780.07RV2020
Gliese 433#29.6050.48c4.820.12RV2012
Gliese 367#30.7190.450.700.00710.0679.89Transit2021
Gliese 367#30.7190.45c0.07711.50.09~80?RV2023
Gliese 367#30.7190.45d0.15934.40.14~80?RV2023
Gliese 357#30.7760.34b1.170.0353.930.0288.92Transit2019
Gliese 357#30.7760.34c0.0619.130.04~89?RV2019
Gliese 357#30.7760.34d0.20455.70.03~89?RV2019
Gliese 17630.9370.45b0.0660.08RV20071 disputed candidate
GJ 3512#30.9760.123b0.3382040.44RV2019
GJ 3512#30.9760.123c1.722RV2020
G 192-15#31.0750.132b0.01722.2750RV2025
G 192-15#31.0750.132c1.1370.68RV2025
Wolf 106931.2290.167b0.067215.56RV2023
AU Microscopii#31.6830.50b4.380.06450.1089.03Transit20202 candidates
AU Microscopii#31.6830.50c3.510.1101088.62Transit20202 candidates
Gliese 43631.8820.414.330.02802.640.1585.8RV2004One dubious candidate
G 268-11031.8880.137b0.01281.4330RV2025
Gliese 4932.1580.57b0.10617.30.03RV2019
GJ 398832.3160.184b0.04056.9440RV2023
HD 260655#32.6080.439b1.2400.02930.03987.35Transit2022
HD 260655#32.6080.439c1.5330.04750.03887.79Transit2022