List of nearest exoplanets

There are known exoplanets, or planets outside our 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 97 exoplanets listed as confirmed by the NASA Exoplanet Archive. Among the over 400 known stars within 10 parsecs, around 60 have been confirmed to have planetary systems; 51 stars in this range are visible to the naked eye, nine 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 2020 is one around AU Microscopii. The closest exoplanet found is Proxima Centauri b, which was confirmed in 2016 to orbit Proxima Centauri, the closest star to our Solar System. HD 219134 has six exoplanets, the highest number discovered for any star within this range.
Most known nearby exoplanets orbit close to their star and have highly eccentric orbits. A majority are significantly larger than Earth, but a few have similar masses, including two planets which may be less massive than Earth. Several confirmed exoplanets are hypothesized to be potentially habitable, with Proxima Centauri b and three around Gliese 667 C considered the most likely candidates. The International Astronomical Union took a public survey in 2015 about renaming some known extrasolar bodies, including the planets around Epsilon Eridani and Fomalhaut.

Exoplanets within 10 parsecs

Host star system	Host star system	Host star system	Host star system	Companion exoplanet	Companion exoplanet	Companion exoplanet	Companion exoplanet	Companion exoplanet	Companion exoplanet	Companion exoplanet	Companion exoplanet	Notes and additional planetary observations
Name	Distance	Apparent magnitude	Mass	Label	Mass	Radius	Semi-major axis	Orbital period	Eccentricity	Inclination	Discovery year	Notes and additional planetary observations
Sun^°	0		1		'	0.3829	0.387	'	0.205	—		—
Sun^°	0		1		'	1	1	'	0.0167	—		—
Sun^°	0		1		'	'	5.20		0.0488	—		—
Proxima Centauri^#	4.2441	11.13	0.123	b^↑			0.0486		0.109	~133?	2016	1 candidate
Proxima Centauri^#	4.2441	11.13	0.123	c		—	1.489	1,928	0.04	133	2020	1 candidate
Barnard's Star	5.958		0.144	b		—	0.430	232	0.04	—	2018
Wolf 359^#	7.895		0.09	c		—	0.018		0.15	—	2019
Wolf 359^#	7.895		0.09	b		—	1.845		0.04	—	2019
Lalande 21185	8.307		0.46	b		—	0.068		0.04	—	2017
Epsilon Eridani	10.446		0.83			—	3.39		0.50	~25?	2000	1 inferred planet and a disc
Lacaille 9352^#	10.721		0.503	b		—	0.067		0.03	—	2019
Lacaille 9352^#	10.721		0.503	c		—	0.119		0.03	—	2019
Lacaille 9352^#	10.721		0.503	d		—	0.175		0.04	—	2019
Ross 128	11.007		0.168	b^↑			0.0496		0.12	—	2017
Struve 2398 B^#	11.490		0.248	b		—	0.261		0.06	—	2019
Struve 2398 B^#	11.490		0.248	c		—	0.428		0.03	—	2019
Groombridge 34 A^#	11.618		0.38	b		—	0.072		0.094	~61?	2014
Groombridge 34 A^#	11.618		0.38	c		—	5.4	7,600	0.27	~61?	2018
Tau Ceti^#	11.753		0.78			—	0.133		0.06	—	2017	2 retracted and 1 candidate
Tau Ceti^#	11.753		0.78			—	0.243		0.23	—	2017	2 retracted and 1 candidate
Tau Ceti^#	11.753		0.78	^↑			0.538		0.18	—	2017	2 retracted and 1 candidate
Tau Ceti^#	11.753		0.78			—	1.33		0.16	—	2017	2 retracted and 1 candidate
Epsilon Indi A	11.869		0.762	b		—	11.55		0.26	64.25	2002	Not confirmed until 2018
Gliese 1061^#	11.980		0.113	b		—	0.021		<0.31	—	2019	two solutions for d's orbit
Gliese 1061^#	11.980		0.113	c		—	0.035		<0.29	—	2019	two solutions for d's orbit
Gliese 1061^#	11.980		0.113	d		—	0.052		<0.54	—	2019	two solutions for d's orbit
YZ Ceti^#	12.108	12.1	0.130	b		—	0.0156		0.0	—	2017	1 candidate
YZ Ceti^#	12.108	12.1	0.130	c		—	0.0209		0.04	—	2017	1 candidate
YZ Ceti^#	12.108	12.1	0.130	d		—	0.0276		0.03	—	2017	1 candidate
Luyten's Star^#	12.199	11.94	0.29	c		—	0.0365		0.12	—	2017
Luyten's Star^#	12.199	11.94	0.29	b^↑			0.090		0.03	—	2017
Luyten's Star^#	12.199	11.94	0.29	d		—	0.712		0.17	—	2019
Luyten's Star^#	12.199	11.94	0.29	e		—	0.849		0.03	—	2019
Teegarden's Star^#	12.496		0.08	b		—	0.0252		0	—	2019
Teegarden's Star^#	12.496		0.08	c		—	0.0443		0	—	2019
Kapteyn's Star^#	12.829		0.28			—	0.311		0.07	—	2014	1 disputed candidate
Wolf 1061^#	14.046		0.25			—	0.0375		0.03	—	2015
Wolf 1061^#	14.046		0.25	^↑			0.0890		0.03	—	2015
Wolf 1061^#	14.046		0.25			—	0.421		0.02	—	2015
Gliese 83.1^#	14.584		0.14	c		—	0.016		0.09	—	2019
Gliese 83.1^#	14.584		0.14	d		—	0.406		0.15	—	2019
Gliese 83.1^#	14.584		0.14	b		—	0.881		0.22	—	2019
Gliese 674	14.839		0.35	b		—	0.039		0.23	—	2007
Gliese 687^#	14.840		0.41	b		—	0.163		0.03	—	2014
Gliese 687^#	14.840		0.41	c		—	1.193		0.03	—	2019
Gliese 876^#	15.250		0.33	d		—	0.0208		0.12	59.5	2005
Gliese 876^#	15.250		0.33	c		—	0.133		0.001	59.5	2000
Gliese 876^#	15.250		0.33	b		—	0.213		0.001	59.5	1998
Gliese 876^#	15.250		0.33	e		—	0.342		0.18	59.5	2010
Gliese 832^#	16.194		0.45	^↑			0.164		0.06	—	2014
Gliese 832^#	16.194		0.45	b		—	3.67		0.06	—	2008
AD Leonis	16.197		0.41	b		—	0.025		0.03	—	2019
40 Eridani A	16.386		0.84	b		—	0.224		0.04	~72?	2018
Gliese 3323^#	17.533	12.2	0.164	b^↑			0.0328			—	2017
Gliese 3323^#	17.533	12.2	0.164	c		—	0.126			—	2017
Gliese 251^#	18.204		0.372	b		—	0.0204			—	2017
Gliese 251^#	18.204		0.372	c		—	0.974	607	0.03	—	2019
LP 816-60	18.311		0.23	b		—	—	93.9	—	—	2019
Gliese 205^#	18.592		0.63	b		—	0.109	16.9	0.11	—	2019
Gliese 205^#	18.592		0.63	c		—	0.689	271	0.04	—	2019
Gliese 229 A^#	18.777		0.58	c		—	0.339		0.19	—	2020	Ab not confirmed until 2020.
Gliese 229 A^#	18.777		0.58	b		—	0.898		0.10	—	2014	Ab not confirmed until 2020.
Gliese 752 A	19.286		0.46	b		—	0.338		0.03	—	2018
Gliese 754	19.289		0.18	b		—	0.277		0.03	—	2019
Gliese 588^#	19.298		0.46	b		—	0.049	5.81	0.04	—	2019
Gliese 588^#	19.298		0.46	c		—	0.530	206	0.06	—	2019
82 G. Eridani^#	19.582		0.85	b		—	0.121			—	2011	2 candidates
82 G. Eridani^#	19.582		0.85	c		—	0.204			—	2011	2 candidates
82 G. Eridani^#	19.582		0.85	d		—	0.350			—	2011	2 candidates
82 G. Eridani^#	19.582		0.85	e		—	0.509			—	2017	2 candidates
Gliese 784	20.083		0.5	b		—	0.059		0.05	—	2019
Gliese 555	20.370		0.29	b		—	0.727		0.04	—	2019
Gliese 581^#	20.545		0.31	e		—	0.0282		0.0	~45?	2009	2 disputed candidates and a disc
Gliese 581^#	20.545		0.31	b		—	0.0406		0.0	~45?	2005	2 disputed candidates and a disc
Gliese 581^#	20.545		0.31	c		—	0.072		0.0	~45?	2007	2 disputed candidates and a disc
Gliese 338 B	20.658	7.0	0.64	b		—	0.141		0.11	—	2020
Gliese 625	21.114	10.2	0.30	b		—	0.0784			—	2017
HD 219134^#	21.306		0.78	b		1.60	0.0388			85.06	2015	1 candidate, 2 dubious planets
HD 219134^#	21.306		0.78			1.51	0.065			87.28	2015	1 candidate, 2 dubious planets
HD 219134^#	21.306		0.78				0.235			~87?	2015	1 candidate, 2 dubious planets
HD 219134^#	21.306		0.78			—	3.11			~87?	2015	1 candidate, 2 dubious planets
Gliese 880	22.399		0.59	b		—	0.187		0.13	—	2019
LTT 1445 A	22.409		0.26	b		1.35	0.0381		0.16	89.47	2019
Gliese 393	22.938		0.41	b		—	0.055		0.03	—	2019
Gliese 667 C^#	23.632		0.33			—	0.049		0.13	~52?	2009	5 dubious candidates
Gliese 667 C^#	23.632		0.33	^↑			0.1251		0.03	~52?	2011	5 dubious candidates
Gliese 514	24.851		0.53	b		—	0.097	15.0	0.05	—	2019
Gliese 300	26.469		0.26	b		—	0.050		0.29	—	2019
Gliese 686	26.612		0.42	b		—	0.097		0.04	—	2019
61 Virginis^#	27.741		0.95	b		—	0.0502			~77?	2009	a debris disc
61 Virginis^#	27.741		0.95	c		—	0.218		0.14	~77?	2009	a debris disc
61 Virginis^#	27.741		0.95	d		—	0.476		0.35	~77?	2009	a debris disc
CD Ceti	28.080		0.161	b		—	0.0185		0	—	2020
Gliese 785^#	28.699		0.78	b		—	0.32		0.13	—	2010
Gliese 785^#	28.699		0.78	c		—	1.18			—	2011
Gliese 849^#	28.711		0.49	b		—	2.26		0.05	—	2006
Gliese 849^#	28.711		0.49	c		—	4.82		0.087	—	2006
Gliese 433^#	29.572		0.48	b		—	0.062		0.04	—	2009
Gliese 433^#	29.572		0.48	d		—	0.178		0.07	—	2020
Gliese 433^#	29.572		0.48	c		—	4.82		0.12	—	2012
Gliese 3325	30.109		0.27	b		—	0.071		0.03	—	2019
HD 102365 A	30.374		0.85	b		—	0.46		0.34	—	2010
Gliese 357^#	30.803		0.34	b		1.17	0.035	3.93	0.02	88.92	2019
Gliese 357^#	30.803		0.34	c		—	0.061	9.13	0.04	~89?	2019
Gliese 357^#	30.803		0.34	d		—	0.204	55.7	0.03	~89?	2019
Gliese 176^#	30.879		0.45	b		—	0.066		0.08	—	2007	1 dubious planet
Gliese 176^#	30.879		0.45	c		—	0.146	28.6	0.02	—	2019	-
Gliese 479	30.912		0.43	b		—	0.074	11.3	0.03	—	2019
Gliese 3512^#	30.949		0.123	b		—	0.338	204	0.44	—	2019
Gliese 3512^#	30.949		0.123	c		—	>1.2	>1390	—	—	2019
AU Microscopii	31.719		0.50	b		4.20	0.066		0.10	~90	2020	1 candidate
Gliese 436	31.820		0.41	b		4.33	0.0280	2.64	0.15	85.8	2004	1 candidate
Gliese 49	32.145		0.57	b		—	0.106	17.3	0.03	—	2019

Excluded objects

Unlike for bodies within our Solar System, there is no clearly established method for officially recognizing an exoplanet. According to the International Astronomical Union, an exoplanet should be considered confirmed if it has not been disputed for five years after its discovery. There have been examples where the existence of exoplanets has been proposed, but even after follow-up studies their existence is still considered doubtful by some astronomers. Such cases include: Alpha Centauri, LHS 288, and Gliese 682. There are also some instances where proposed exoplanets were later disproved by subsequent studies, such as candidates around Teegarden's star, Van Maanen 2, Groombridge 1618, and VB 10.
The Working Group on Extrasolar Planets of the International Astronomical Union adopted in 2003 a working definition on the upper limit for what constitutes a planet: not being massive enough to sustain thermonuclear fusion of deuterium. Some studies have calculated this to be somewhere around 13 times the mass of Jupiter, and therefore objects more massive than this are usually classified as brown dwarfs. Some proposed candidate exoplanets were later shown to be massive enough to fall above the threshold, and are likely brown dwarfs, as was the case for: SCR 1845-6357 B, SDSS J1416+1348 B, and WISE 1217+1626 B.
Excluded from the current list are known examples of potential free-floating sub-brown dwarfs, or "rogue planets", which are bodies that are too small to undergo fusion yet they do not revolve around a star. Known such examples include: WISE 0855–0714, UGPS 0722-05, WISE 1541−2250, and SIMP J01365663+0933473.

Statistics

Planetary systems

Distance	№ of known star systems	№ of known stars	№ of stars hosting known exoplanets	Percentage of stars hosting exoplanets
	1	3	1	33%
	8	11	3	27%
10–15	31	43	16	37%
15–20	57	77	13	17%
20–25	55	78	11	14%
25–32.6	?	~200	16	~8%
Total		>413	60	<14.5%

Exoplanets

Orbital radius	№	Notes
	80	Mercury orbits at 0.39 AU
0.4–1.0 AU	16	Earth orbits at 1.0 AU
1.0–5 AU	11	Earth orbits at 1.0 AU
	2	Jupiter orbits at 5.2 AU

Orbital eccentricity	№	Notes
	15	Earth's is 0.0167
0.02–0.20	78	Earth's is 0.0167
0.02–0.20	78	Mercury's is 0.205
	14	Mercury's is 0.205

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