List of nearest exoplanets

There are 4,301 known exoplanets, or planets outside our solar system that orbit a star, as of August 1, 2020; only a small fraction of these are located in the vicinity of the Solar System.[3] Within 10 parsecs (32.6 light-years), there are 97 exoplanets listed as confirmed by the NASA Exoplanet Archive.^[a][4] Among the over 400 known stars within 10 parsecs,^[b][5] around 60 have been confirmed to have planetary systems; 51 stars in this range are visible to the naked eye,^[c][6] nine of which have planetary systems.

Exoplanet Fomalhaut b (Dagon), 25 light-years away, with its parent star Fomalhaut blacked out, as pictured by Hubble in 2012.[1] In 2020 this object was determined to be an expanding debris cloud from a collision of asteroids rather than a planet.[2]

Distribution of nearest exoplanets

The first report of an exoplanet within this range was in 1998 for a planet orbiting around Gliese 876 (15.3 light-years (ly) away), and the latest as of 2020 is one around AU Microscopii (32 ly). The closest exoplanet found is Proxima Centauri b, which was confirmed in 2016 to orbit Proxima Centauri, the closest star to our Solar System (4.25 ly). HD 219134 (21.6 ly) 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 (around YZ Ceti, 12 ly) 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 (23.6 ly) considered the most likely candidates.[7] The International Astronomical Union took a public survey in 2015 about renaming some known extrasolar bodies, including the planets around Epsilon Eridani (10.5 ly) and Fomalhaut.^[d][8]

Exoplanets within 10 parsecs

Key to colors

^°	Mercury, Earth and Jupiter (for comparison purposes)
^#	Confirmed multiplanetary systems
^↑	Exoplanets believed to be potentially habitable[7]

Confirmed exoplanets[4]

Host star system				Companion exoplanet (in order from star)								Notes and additional planetary observations
Name	Distance (ly)	Apparent magnitude (V)	Mass (M☉)	Label ^[e]	Mass (M⊕)^[f]	Radius (R⊕)	Semi-major axis (AU)	Orbital period (days)	Eccentricity	Inclination (°)	Discovery year
Sun^°	0	−26.7	1	Mercury	0.055	0.3829	0.387	88.0	0.205	—	—	—
				Earth	1	1	1	365.3	0.0167	—	—
				Jupiter	317.8	10.973	5.20	4,333	0.0488	—	—
Proxima Centauri^#	4.2441	11.13	0.123	b^↑	>1.2	~1.1?	0.0486	11.2	0.109	~133?	2016	[9][7][10][11][12] 1 candidate[13]
				c	7	—	1.489	1,928	0.04	133	2020
Barnard's Star	5.958	9.511	0.144	b	>4.2	—	0.430	232	0.04	—	2018	[14][15]
Wolf 359^#	7.895	13.54	0.09	c	>3.8	—	0.018	2.69	0.15	—	2019	[15]
				b	>43.9	—	1.845	2,940	0.04	—	2019
Lalande 21185	8.307	7.52	0.46	b	>2.9	—	0.068	9.87	0.04	—	2017	[15]
Epsilon Eridani	10.446	3.73	0.83	AEgir	248	—	3.39	2,500	0.50	~25?	2000	1 inferred planet and a disc[16][17]
Lacaille 9352^#	10.721	7.34	0.503	b	>4.1	—	0.067	9.26	0.03	—	2019	[15]
				c	>9.0	—	0.119	21.8	0.03	—	2019
				d	>6.5	—	0.175	38.8	0.04	—	2019
Ross 128	11.007	11.1	0.168	b^↑	>1.4	~1.2?	0.0496	9.87	0.12	—	2017	[18]
Struve 2398 B^#	11.490	9.7	0.248	b	>15.7	—	0.261	91.3	0.06	—	2019	[15]
				c	>13.1	—	0.428	192	0.03	—	2019
Groombridge 34 A^#	11.618	8.1	0.38	b	>3.03	—	0.072	11.4	0.094	~61?	2014	[19][20][21]
				c	36	—	5.4	7,600	0.27	~61?	2018
Tau Ceti^#	11.753	3.50	0.78	g	>1.7	—	0.133	20.0	0.06	—	2017	2 retracted and 1 candidate [22][23][7][24][25][26]
				h	>1.8	—	0.243	49.4	0.23	—	2017
				e^↑	>3.9	~1.6?	0.538	163	0.18	—	2017
				f	>3.9	—	1.33	640	0.16	—	2017
Epsilon Indi A	11.869	4.83	0.762	b	1030	—	11.55	16,500	0.26	64.25	2002	Not confirmed until 2018[27] [28][29]
Gliese 1061^#	11.980	7.52	0.113	b	>1.4	—	0.021	3.20	<0.31	—	2019	two solutions for d's orbit[30]
				c	>1.7	—	0.035	6.69	<0.29	—	2019
				d	>1.6	—	0.052	12.4	<0.54	—	2019
YZ Ceti^#	12.108	12.1	0.130	b	>0.75	—	0.0156	1.97	0.0	—	2017	1 candidate [31][32][15]
				c	>1.2	—	0.0209	3.06	0.04	—	2017
				d	>1.1	—	0.0276	4.66	0.03	—	2017
Luyten's Star^#	12.199	11.94	0.29	c	>1.2	—	0.0365	4.72	0.12	—	2017	[7][33][15]
				b^↑	>2.2	~1.4?	0.090	18.6	0.03	—	2017
				d	>10.8	—	0.712	414	0.17	—	2019
				e	>9.3	—	0.849	542	0.03	—	2019
Teegarden's Star^#	12.496	15.40	0.08	b	>1.1	—	0.0252	4.91	0	—	2019	[34]
				c	>1.1	—	0.0443	11.4	0	—	2019
Kapteyn's Star^#	12.829	8.8	0.28	c	>6.9	—	0.311	121	0.07	—	2014	[35] 1 disputed candidate[36][15]
Wolf 1061^#	14.046	10.1	0.25	b	>1.9	—	0.0375	4.89	0.03	—	2015	[7][37][15]
				c^↑	>3.6	~1.5?	0.0890	17.9	0.03	—	2015
				d	>6.5	—	0.421	184	0.02	—	2015
Gliese 83.1^#	14.584	12.30	0.14	c	>4.0	—	0.016	1.93	0.09	—	2019	[15]
				d	>26.0	—	0.406	243	0.15	—	2019
				b	>81.5	—	0.881	773	0.22	—	2019
Gliese 674	14.839	9.38	0.35	b	>11.2	—	0.039	4.69	0.23	—	2007	[38][39][15]
Gliese 687^#	14.840	9.15	0.41	b	>17.3	—	0.163	38.1	0.03	—	2014	[40][15]
				c	>14.5	—	1.193	758	0.03	—	2019
Gliese 876^#	15.250	10.2	0.33	d	6.8	—	0.0208	1.94	0.12	59.5	2005	[41][15]
				c	230	—	0.133	30.2	0.001	59.5	2000
				b	720	—	0.213	61.0	0.001	59.5	1998
				e	15	—	0.342	125	0.18	59.5	2010
Gliese 832^#	16.194	8.67	0.45	c^↑	>5.4	~1.7?	0.164	35.7	0.06	—	2014	[7][42][15]
				b	>206	—	3.67	3,830	0.06	—	2008
AD Leonis	16.197	9.52	0.41	b	>23.1	—	0.025	2.23	0.03	—	2019	[15]
40 Eridani A	16.386	4.4	0.84	b	>8.5	—	0.224	42.4	0.04	~72?	2018	[43]
Gliese 3323^#	17.533	12.2	0.164	b^↑	>2.0	~1.3?	0.0328	5.36	0.2	—	2017	[44]
				c	>2.3	—	0.126	40.5	0.2	—	2017
Gliese 251^#	18.204	9.65	0.372	b	>3.3	—	0.0204	1.74	~0.03	—	2017	[45][15]
				c	>22.2	—	0.974	607	0.03	—	2019
LP 816-60	18.311	11.46	0.23	b	2?	—	—	93.9	—	—	2019	[15]
Gliese 205^#	18.592	7.97	0.63	b	>10.3	—	0.109	16.9	0.11	—	2019	[15]
				c	>13.8	—	0.689	271	0.04	—	2019
Gliese 229 A^#	18.777	8.14	0.58	c	>7.3	—	0.339	122	0.19	—	2020	Ab not confirmed until 2020.[46]
				b	>8.5	—	0.898	526	0.10	—	2014
Gliese 752 A	19.286	9.13	0.46	b	>13.6	—	0.338	106	0.03	—	2018	[47][15]
Gliese 754	19.289	12.23	0.18	b	>9.8	—	0.277	78.4	0.03	—	2019	[15]
Gliese 588^#	19.298	9.31	0.46	b	>2.4	—	0.049	5.81	0.04	—	2019	[15]
				c	>10.3	—	0.530	206	0.06	—	2019
82 G. Eridani^#	19.582	4.26	0.85	b	>2.7	—	0.121	18.3	~0	—	2011	2 candidates [48][49][50]
				c	>2.4	—	0.204	40.1	~0	—	2011
				d	>4.8	—	0.350	90	~0	—	2011
				e	>4.8	—	0.509	147	0.29	—	2017
Gliese 784	20.083	7.97	0.5	b	>9.4	—	0.059	6.66	0.05	—	2019	[15]
Gliese 555	20.370	11.32	0.29	b	>30.1	—	0.727	450	0.04	—	2019	[15]
Gliese 581^#	20.545	10.5	0.31	e	>1.7	—	0.0282	3.15	0.0	~45?	2009	2 disputed candidates and a disc [51][52][53][54]
				b	>16	—	0.0406	5.37	0.0	~45?	2005
				c	>5.5	—	0.072	12.9	0.0	~45?	2007
Gliese 338 B	20.658	7.0	0.64	b	>10.3	—	0.141	24.5	0.11	—	2020	[55]
Gliese 625	21.114	10.2	0.30	b	>2.8	—	0.0784	14.6	~0.1	—	2017	[56]
HD 219134^#	21.306	5.57	0.78	b	4.7	1.60	0.0388	3.09	~0	85.06	2015	1 candidate, 2 dubious planets [57][58]
				c	4.4	1.51	0.065	6.77	0.062	87.28	2015
				d	>16	>1.61	0.235	46.9	0.138	~87?	2015
				h	>110	—	3.11	2,200	0.06	~87?	2015
Gliese 880	22.399	8.64	0.59	b	>8.5	—	0.187	39.4	0.13	—	2019	[15]
LTT 1445 A	22.409	10.53	0.26	b	~2.2	1.35	0.0381	5.36	0.16	89.47	2019	[59]
Gliese 393	22.938	8.65	0.41	b	>1.9	—	0.055	7.03	0.03	—	2019	[15]
Gliese 667 C^#	23.632	10.2	0.33	b	>5.4	—	0.049	7.20	0.13	~52?	2009	5 dubious candidates [60][7][61][62][15]
				c^↑	>3.9	~1.5?	0.1251	28.2	0.03	~52?	2011
Gliese 514	24.851	9.03	0.53	b	>4.3	—	0.097	15.0	0.05	—	2019	[15]
Gliese 300	26.469	12.13	0.26	b	>6.8	—	0.050	8.33	0.29	—	2019	[15]
Gliese 686	26.612	9.58	0.42	b	>7.1	—	0.097	15.5	0.04	—	2019	[63][15]
61 Virginis^#	27.741	4.74	0.95	b	>5.1	—	0.0502	4.22	~0.1	~77?	2009	a debris disc [64]
				c	>18	—	0.218	38.0	0.14	~77?	2009
				d	>23	—	0.476	123	0.35	~77?	2009
CD Ceti	28.080	14.001	0.161	b	>4.0	—	0.0185	2.29	0	—	2020	[65]
Gliese 785^#	28.699	6.13	0.78	b	>17	—	0.32	75	0.13	—	2010	[66]
				c	>24	—	1.18	530	~0.3	—	2011
Gliese 849^#	28.711	10.4	0.49	b	>270	—	2.26	1,910	0.05	—	2006	[67][15]
				c	>300	—	4.82	5,520	0.087	—	2006
Gliese 433^#	29.572	9.79	0.48	b	>6.0	—	0.062	7.37	0.04	—	2009	[68][15][46]
				d	>5.2	—	0.178	36.1	0.07	—	2020
				c	>32	—	4.82	5,090	0.12	—	2012
Gliese 3325	30.109	11.73	0.27	b	>11.8	—	0.071	12.9	0.03	—	2019	[15]
HD 102365 A	30.374	4.89	0.85	b	>16	—	0.46	122	0.34	—	2010	[69]
Gliese 357^#	30.803	10.9	0.34	b	1.6	1.17	0.035	3.93	0.02	88.92	2019	[70][15]
				c	>3.6	—	0.061	9.13	0.04	~89?	2019
				d	>7.7	—	0.204	55.7	0.03	~89?	2019
Gliese 176^#	30.879	10.1	0.45	b	>8.0	—	0.066	8.77	0.08	—	2007	1 dubious planet[71][72][15]
				c	>7.4	—	0.146	28.6	0.02	—	2019
Gliese 479	30.912	10.66	0.43	b	>5.1	—	0.074	11.3	0.03	—	2019	[15]
Gliese 3512^#	30.949	13.11	0.123	b	>147	—	0.338	204	0.44	—	2019	[73]
				c	>54	—	>1.2	>1390	—	—	2019
AU Microscopii	31.719	8.63	0.50	b	<57	4.20	0.066	8.46	0.10	~90	2020	1 candidate[74]
Gliese 436	31.820	10.67	0.41	b	21.4	4.33	0.0280	2.64	0.15	85.8	2004	1 candidate[15]
Gliese 49	32.145	8.9	0.57	b	>16.4	—	0.106	17.3	0.03	—	2019	[15]

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.[75] 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 (4.36 ly, two in 2012[76] and 2013[77]), LHS 288 (15.6 ly, in 2007[78]), and Gliese 682 (16.6 ly, two in 2014[7][79][80]). There are also some instances where proposed exoplanets were later disproved by subsequent studies, such as candidates around Teegarden's star (12.6 ly),[81] Van Maanen 2 (13.9 ly),[82] Groombridge 1618 (15.9 ly),[83] and VB 10 (18.7 ly).[84]

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.[85] 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 (12.6 ly),[86] SDSS J1416+1348 B (29.7 ly),[87] and WISE 1217+1626 B (30 ly).[88]

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 (7.3 ly),[89] UGPS 0722-05, (13 ly)[90] WISE 1541−2250 (18.6 ly),[91] and SIMP J01365663+0933473 (20 ly).[92]

Statistics

Planetary systems

Systems by planet count

Exoplanets	№ of systems	Systems
4	5	Tau Ceti, Luyten's Star, Gliese 876, 82 G. Eridani, HD 219134
3	9	Lacaille 9352, Gliese 1061, YZ Ceti, Wolf 1061, L 1159-16, Gliese 581, 61 Virginis, Gliese 433, Gliese 357
2	17	—
1	29	—
Total	60

Distribution of nearby planet-hosting systems

Distance (light-years)	№ of known star systems	№ of known stars	№ of stars hosting known exoplanets	Percentage of stars hosting exoplanets
< 5	1	3	1	33%
5–10	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[93]	60	<14.5%

Systems visible with
the naked eye?^[c][94]

Visible host star?	Systems
Yes (V < 6.5)	9
No (V > 6.5)	51

Exoplanets

Exoplanets by minimum estimated mass

Type	Mass range[95]	№
Terran	0.5–5 M⊕	45
Superterran	5–10 M⊕	24
Neptunian	10–50 M⊕	28
Jovian	50–600 M⊕	9
Superjovian	>600 M⊕	3
Total		109

Exoplanets by orbital radius

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

Exoplanets by orbital period

Orbital period	№	Notes
< 90 days	73	Mercury takes 88 days
90–365 days	17
1–10 years	14	Jupiter takes 11.9 years
> 10 years	5

Exoplanets by orbital eccentricity

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

Exoplanets by discovery year

Year	№
1998	1
2000	2
2002	1
2004	1
2005	2
2006	2
2007	3
2008	1
2009	6
2010	3
2011	5
2012	1
2014	5
2015	7
2016	1
2017	16
2018	4
2019	43
2020	6

See also

• List of nearest stars and brown dwarfs
• List of nearest bright stars
• List of nearest terrestrial exoplanet candidates
• List of nearest free floating planetary mass objects
• Lists of exoplanets
• Lists of planets
• List of planet types
• List of potentially habitable exoplanets

Notes

1. ^{^} Listed values are primarily taken from NASA Exoplanet Archive,[4] but other databases include a few additional exoplanet entries tagged as "Confirmed" that are have yet to be compiled into the NASA archive. Such databases include:

   "Exoplanet Catalog". The Extrasolar Planets Encyclopaedia. Full table.

   "Exoplanets Data Explorer". Exoplanet Orbit Database. California Planet Survey. Click the "+" button to visualize additional parameters.

   "Open Exoplanet Catalogue". Click the "Show options" to visualize additional parameters. Archived from the original on 2017-09-02. Retrieved 2015-02-14.

2. ^{^} For reference, the 104th closest known star system in November 2016 was 82 Eridani (19.7 ly).[96]
3. ^{^} According to the Bortle scale, an astronomical object is visible to the naked eye under "typical" dark-sky conditions in a rural area if it has an apparent magnitude smaller than +6.5. To the unaided eye, the limiting magnitude is +7.6 to +8.0 under "excellent" dark-sky conditions (with effort).[94]
4. ^{^} The star Epsilon Eridani was named Ran (after Rán, the Norse goddess of the sea), and the planet Epsilon Eridani b was named AEgir (after Ægir, Rán's husband),[97] while the planet Fomalhaut b was named Dagon (after Dagon, an ancient Syrian “fish god”[98]).[8]
5. ^{^} Exoplanet naming convention assigns uncapitalized letters starting from b to each planet based on chronological order of their initial report, and in increasing order of distance from the parent star for planets reported at the same time. Omitted letters signify planets that have yet to be confirmed, or planets that have been retracted altogether.
6. ^{^} Most reported exoplanet masses have very large error margins (typically, between 10% and 30%). The mass of an exoplanet has generally been inferred from measurements on changes in the radial velocity of the host star, but this kind of measurement only allows for an estimate on the exoplanet's orbital parameters, but not on their orbital inclination (i). As such, most exoplanets only have an estimated minimum mass (M_real*sin(i)), where their true masses are statistically expected to come close to this minimum, with only about 13% chance for the mass of an exoplanet to be more than double its minimum mass.[99]

References

1. Harrington, J. D.; Villard, Ray (2013-08-01). "NASA's Hubble Reveals Rogue Planetary Orbit For Fomalhaut". NASA. Archived from the original on 2015-11-06. Retrieved 2015-09-18.
2. Gáspár, András; Rieke, George H. (April 20, 2020). "New HST data and modeling reveal a massive planetesimal collision around Fomalhaut". PNAS. arXiv:2004.08736. doi:10.1073/pnas.1912506117. Retrieved April 21, 2020.
3. Schneider, Jean. "Interactive Extra-solar Planets Catalog". The Extrasolar Planets Encyclopaedia. Exoplanet.eu. Archived from the original on 2012-02-08. Retrieved 2018-03-20.
4. "NASA Exoplanet Archive—Confirmed Planets". NASA Exoplanet Science Institute. California Institute of Technology. Retrieved 2018-03-22.
5. "Stars within 10 parsecs". Solstation.com. 2014-04-25. Archived from the original on 2017-10-26. Retrieved 2018-03-22.
6. Powell, Richard (2006). "Stars within 50 light years". An Atlas of the Universe. Archived from the original on 2014-06-27. Retrieved 2014-05-17.
7. "The Habitable Exoplanets Catalog". Planetary Habitability Laboratory. University of Puerto Rico in Arecibo. 2015-09-01. Archived from the original on 2016-01-09. Retrieved 2015-09-17.
8. "Final Results of NameExoWorlds Public Vote Released" (Press release). International Astronomical Union. 2015-12-15. Archived from the original on 2018-05-15. Retrieved 2018-03-17.
9. Anglada-Escudé, Guillem; Amado, Pedro J.; Barnes, John; Berdiñas, Zaira M.; Butler, R. Paul; Coleman, Gavin A. L.; de la Cueva, Ignacio; Dreizler, Stefan; Endl, Michael; Giesers, Benjamin; Jeffers, Sandra V.; Jenkins, James S.; Jones, Hugh R. A.; Kiraga, Marcin; Kürster, Martin; López-González, Marίa J.; Marvin, Christopher J.; Morales, Nicolás; Morin, Julien; Nelson, Richard P.; Ortiz, José L.; Ofir, Aviv; Paardekooper, Sijme-Jan; Reiners, Ansgar; Rodríguez, Eloy; Rodrίguez-López, Cristina; Sarmiento, Luis F.; Strachan, John P.; Tsapras, Yiannis; Tuomi, Mikko; Zechmeister, Mathias (August 25, 2016). "A terrestrial planet candidate in a temperate orbit around Proxima Centauri" (PDF). Nature. 536 (7617): 437–440. arXiv:1609.03449. Bibcode:2016Natur.536..437A. doi:10.1038/nature19106. PMID 27558064.
10. Damasso, Mario; Del Sordo, Fabio; Anglada-Escudé, Guillem; et al. (15 January 2020). "A low-mass planet candidate orbiting Proxima Centauri at a distance of 1.5 AU". Science Advances. 6 (3). eaax7467. Bibcode:2020SciA....6.7467D. doi:10.1126/sciadv.aax7467. PMC 6962037. PMID 31998838.
11. Kervella, Pierre; Arenou, Frédéric; Schneider, Jean (2020). "Orbital inclination and mass of the exoplanet candidate Proxima c". Astronomy & Astrophysics. 635: L14. arXiv:2003.13106. Bibcode:2020A&A...635L..14K. doi:10.1051/0004-6361/202037551. ISSN 0004-6361.
12. Benedict, G. Fritz; McArthur, Barbara E. (16 June 2020). "A Moving Target—Revising the Mass of Proxima Centauri c". Research Notes of the AAS. 4 (6). doi:10.3847/2515-5172/ab9ca9. Retrieved 17 June 2020.
13. Suárez Mascareño, A.; Faria, J. P.; et al. (2020). "Revisiting Proxima with ESPRESSO". Astronomy & Astrophysics. arXiv:2005.12114. doi:10.1051/0004-6361/202037745. ISSN 0004-6361.
14. Ribas, I.; Tuomi, M.; Reiners, A.; Butler, R. P.; Morales, J. C.; Perger, M.; Dreizler, S.; Rodríguez-López, C.; González Hernández, J. I.; Rosich, A.; Feng, F.; Trifonov, T.; Vogt, S. S.; Caballero, J. A.; Hatzes, A.; Herrero, E.; Jeffers, S. V.; Lafarga, M.; Murgas, F.; Nelson, R. P.; Rodríguez, E.; Strachan, J. B. P.; Tal-Or, L.; Teske, J.; Toledo-Padrón, B.; Zechmeister, M.; Quirrenbach, A.; Amado, P. J.; Azzaro, M.; Béjar, V. J. S.; Barnes, J. R.; Berdiñas, Z. M.; Burt, J.; Coleman, G.; Cortés-Contreras, M.; Crane, J.; Engle, S. G.; Guinan, E. F.; Haswell, C. A.; Henning, Th.; Holden, B.; Jenkins, J.; Jones, H. R. A.; Kaminski, A.; Kiraga, M.; Kürster, M.; Lee, M. H.; López-González, M. J.; Montes, D.; Morin, J.; Ofir, A.; Pallé, E.; Rebolo, R.; Reffert, S.; Schweitzer, A.; Seifert, W.; Shectman, S. A.; Staab, D.; Street, R. A.; Suárez Mascareño, A.; Tsapras, Y.; Wang, S. X.; Anglada-Escudé, G. (2018). "A candidate super-Earth planet orbiting near the snow line of Barnard's star" (PDF). Nature. 563 (7731): 365–368. arXiv:1811.05955. Bibcode:2018Natur.563..365R. doi:10.1038/s41586-018-0677-y. hdl:2299/21132. ISSN 0028-0836. OCLC 716177853. PMID 30429552.
15. Barnes, J. R.; Kiraga, M.; Diaz, M.; Berdiñas, Z.; Jenkins, J. S.; Keiser, S.; Thompson, I.; Crane, J. D.; Shectman, S. A.; Teske, J. K.; Holden, B.; Laughlin, G.; Burt, J.; Vogt, S. S.; Arriagada, P.; Butler, R. P.; Anglada-Escudé, G.; Jones, H. R. A.; Tuomi, M. (11 June 2019). "Frequency of planets orbiting M dwarfs in the Solar neighbourhood". arXiv:1906.04644 [astro-ph.EP].
16. "eps Eri". NASA Exoplanet Science Institute. California Institute of Technology. Retrieved 2016-04-23.
17. "eps Eridani c". The Extrasolar Planet Encyclopaedia. Exoplanet.eu. Archived from the original on 2014-02-23. Retrieved 2014-05-17.
18. "Ross 128". NASA Exoplanet Science Institute. California Institute of Technology. Retrieved 2018-03-22.
19. Howard, Andrew W.; et al. (October 2014), "The NASA-UC-UH ETA-Earth Program. IV. A Low-mass Planet Orbiting an M Dwarf 3.6 PC from Earth", The Astrophysical Journal, 794 (1): 9, arXiv:1408.5645, Bibcode:2014ApJ...794...51H, doi:10.1088/0004-637X/794/1/51, 51.
20. Trifonov, T; Kürster, M; Zechmeister, M; et al. (2018). "The CARMENES search for exoplanets around M dwarfs". Astronomy & Astrophysics. 609 (117): A117. arXiv:1710.01595. Bibcode:2018A&A...609A.117T. doi:10.1051/0004-6361/201731442.
21. Pinamonti, M.; Damasso, M.; Marzari, F.; Sozzetti, A.; Desidera, S.; Maldonado, J.; Scandariato, G.; Affer, L.; Lanza, A. F.; Bignamini, A.; Bonomo, A. S.; Borsa, F.; Claudi, R.; Cosentino, R.; Giacobbe, P.; González-Álvarez, E.; González Hernández, J. I.; Gratton, R.; Leto, G.; Malavolta, L.; Martinez Fiorenzano, A.; Micela, G.; Molinari, E.; Pagano, I.; Pedani, M.; Perger, M.; Piotto, G.; Rebolo, R.; Ribas, I.; et al. (2018). "The HADES RV Programme with HARPS-N at TNG. VIII. GJ15A: A multiple wide planetary system sculpted by binary interaction". Astronomy and Astrophysics. 617: A104. arXiv:1804.03476. Bibcode:2018A&A...617A.104P. doi:10.1051/0004-6361/201732535.
22. "tau Cet". NASA Exoplanet Science Institute. California Institute of Technology. Retrieved 2018-03-22.
23. "tau Ceti". Open Exoplanet Catalogue. Archived from the original on 2014-03-14. Retrieved 2014-05-17.
24. "tau Cet b". The Extrasolar Planet Encyclopaedia. Exoplanet.eu. Archived from the original on 2017-11-07. Retrieved 2018-03-22.
25. "tau Cet c". The Extrasolar Planet Encyclopaedia. Exoplanet.eu. Archived from the original on 2017-12-01. Retrieved 2018-03-22.
26. "tau Cet d". The Extrasolar Planet Encyclopaedia. Exoplanet.eu. Archived from the original on 2017-12-01. Retrieved 2018-03-22.
27. Endl, M.; Kürster, M.; Els, S.; Hatzes, A. P.; Cochran, W. D.; Dennerl, K.; Döbereiner, S. (2002). "The planet search program at the ESO Coudé Echelle spectrometer. III. The complete Long Camera survey results". Astronomy and Astrophysics. 392 (2): 671–690. arXiv:astro-ph/0207512. Bibcode:2002A&A...392..671E. doi:10.1051/0004-6361:20020937.
28. Feng, Fabo; Tuomi, Mikko; Jones, Hugh R. A. (23 March 2018). "Detection of the closest Jovian exoplanet in the Epsilon Indi triple system". arXiv:1803.08163 [astro-ph.EP].
29. Feng, Fabo; Anglada-Escudé, Guillem; Tuomi, Mikko; Jones, Hugh R. A.; Chanamé, Julio; Butler, Paul R.; Janson, Markus (14 October 2019). "Detection of the nearest Jupiter analog in radial velocity and astrometry data". Monthly Notices of the Royal Astronomical Society. 490 (4): 5002–5016. arXiv:1910.06804. Bibcode:2019MNRAS.490.5002F. doi:10.1093/mnras/stz2912.
30. Anglada-Escudé, G.; Reiners, A.; Pallé, E.; Ribas, I.; Berdiñas, Z. M.; Rodríguez López, C.; Morales, N.; López-González, M. J.; Hambsch, F-J; Strachan, J B P.; Hidalgo Soto, D.; Lalitha, S.; Coleman, G A L.; Haswell, C. A.; Barnes, J. R.; Zechmeister, M.; Rodríguez, E.; Jeffers, S. V.; Dreizler, S.; Anglada-Escudé, G. (2020). "RedDots: A temperate 1.5 Earth-mass planet candidate in a compact multiterrestrial planet system around GJ 1061". Monthly Notices of the Royal Astronomical Society. 493 (1): 536–550. arXiv:1908.04717. Bibcode:2020MNRAS.493..536D. doi:10.1093/mnras/staa248.
31. "YZ Cet". NASA Exoplanet Science Institute. California Institute of Technology. Retrieved 2018-03-22.
32. "YZ Cet e". The Extrasolar Planet Encyclopaedia. Exoplanet.eu. 2017-08-15. Archived from the original on 2018-03-19. Retrieved 2018-03-22.
33. "GJ 273". NASA Exoplanet Science Institute. California Institute of Technology. Retrieved 2018-03-22.
34. Caballero, J. A.; Reiners, A.; Ribas, I.; Dreizler, S.; Zechmeister, M.; et al. (12 June 2019). "The CARMENES search for exoplanets around M dwarfs. Two temperate Earth-mass planet candidates around Teegarden's Star" (PDF). Astronomy & Astrophysics. 627: A49. arXiv:1906.07196. Bibcode:2019A&A...627A..49Z. doi:10.1051/0004-6361/201935460. ISSN 0004-6361.
35. "Kapteyn". NASA Exoplanet Science Institute. California Institute of Technology. Retrieved 2018-03-22.
36. "Kapteyn's b". The Extrasolar Planet Encyclopaedia. Exoplanet.eu. 2015-05-13. Archived from the original on 2017-12-01. Retrieved 2018-03-22.
37. "Wolf 1061". NASA Exoplanet Science Institute. California Institute of Technology. Retrieved 2018-03-22.
38. "GJ 674". NASA Exoplanet Science Institute. California Institute of Technology. Retrieved 2018-03-22.
39. "GJ 674 b". The Extrasolar Planet Encyclopaedia. Exoplanet.eu. 2007-04-25. Archived from the original on 2014-02-10. Retrieved 2014-05-17.
40. "GJ 687". NASA Exoplanet Science Institute. California Institute of Technology. Retrieved 2018-03-22.
41. "GJ 876". NASA Exoplanet Science Institute. California Institute of Technology. Retrieved 2018-03-22.
42. "GJ 832". NASA Exoplanet Science Institute. California Institute of Technology. Retrieved 2018-03-22.
43. Ma, Bo; Ge, Jian; Muterspaugh, Matthew; Singer, Michael A; Henry, Gregory W; González Hernández, Jonay I; Sithajan, Sirinrat; Jeram, Sarik; Williamson, Michael; Stassun, Keivan; Kimock, Benjamin; Varosi, Frank; Schofield, Sidney; Liu, Jian; Powell, Scott; Cassette, Anthony; Jakeman, Hali; Avner, Louis; Grieves, Nolan; Barnes, Rory; Zhao, Bo; Gilda, Sankalp; Grantham, Jim; Stafford, Greg; Savage, David; Bland, Steve; Ealey, Brent (October 2018). "The first super-Earth detection from the high cadence and high radial velocity precision Dharma Planet Survey". Monthly Notices of the Royal Astronomical Society. 480 (2): 2411–2422. arXiv:1807.07098. Bibcode:2018MNRAS.480.2411M. doi:10.1093/mnras/sty1933.
44. "GJ 3323". NASA Exoplanet Science Institute. California Institute of Technology. Retrieved 2018-03-22.
45. Butler, R. Paul; Vogt, Steven S.; Laughlin, Gregory; Burt, Jennifer A.; Rivera, Eugenio J.; Tuomi, Mikko; Teske, Johanna; Arriagada, Pamela; Diaz, Matias; Holden, Brad; Keiser, Sandy (12 April 2017). "The LCES HIRES/Keck Precision Radial Velocity Exoplanet Survey". The Astronomical Journal. 153 (5): 208. arXiv:1702.03571. Bibcode:2017AJ....153..208B. doi:10.3847/1538-3881/aa66ca. ISSN 1538-3881.
46. Feng, Fabo; Butler, R. Paul; Shectman, Stephen A.; Crane, Jeffrey D.; Vogt, Steve; Chambers, John; Jones, Hugh R. A.; Wang, Sharon Xuesong; Teske, Johanna K.; Burt, Jenn; Díaz, Matías R.; Thompson, Ian B. (8 January 2020). "Search for Nearby Earth Analogs. II. Detection of Five New Planets, Eight Planet Candidates, and Confirmation of Three Planets around Nine Nearby M Dwarfs". The Astrophysical Journal Supplement Series. 246 (1): 11. arXiv:2001.02577. Bibcode:2020ApJS..246...11F. doi:10.3847/1538-4365/ab5e7c.
47. Kaminski, A.; Trifonov, T.; Caballero, J. A.; Quirrenbach, A.; Ribas, I.; Reiners, A.; Amado, P. J.; Zechmeister, M.; Dreizler, S.; Perger, M.; Tal-Or, L.; Bonfils, X.; Mayor, M.; Astudillo-Defru, N.; Bauer, F. F.; Béjar, V. J. S.; Cifuentes, C.; Colomé, J.; Cortés-Contreras, M.; Delfosse, X.; Díez-Alonso, E.; Forveille, T.; Guenther, E. W.; Hatzes, A. P.; Henning, Th; Jeffers, S. V.; Kürster, M.; Lafarga, M.; Luque, R.; Mandel, H.; Montes, D.; Morales, J. C.; Passegger, V. M.; Pedraz, S.; Reffert, S.; Sadegi, S.; Schweitzer, A.; Seifert, W.; Stahl, O.; Udry, S. (3 August 2018). "The CARMENES search for exoplanets around M dwarfs. A Neptune-mass planet traversing the habitable zone around HD 180617". Astronomy & Astrophysics. 618: A115. arXiv:1808.01183. Bibcode:2018A&A...618A.115K. doi:10.1051/0004-6361/201833354.
48. "HD 20794". NASA Exoplanet Science Institute. California Institute of Technology. Retrieved 2018-03-22.
49. "HD 20794 f". The Extrasolar Planet Encyclopaedia. Exoplanet.eu. Archived from the original on 2018-03-20. Retrieved 2018-03-22.
50. "HD 20794 g". The Extrasolar Planet Encyclopaedia. Exoplanet.eu. Archived from the original on 2018-03-20. Retrieved 2018-03-22.
51. "GJ 581". NASA Exoplanet Science Institute. California Institute of Technology. Retrieved 2018-03-22.
52. "GJ 581 d". The Extrasolar Planet Encyclopaedia. Exoplanet.eu. Archived from the original on 2017-12-01. Retrieved 2018-03-22.
53. "GJ 581 f". The Extrasolar Planet Encyclopaedia. Exoplanet.eu. Archived from the original on 2018-03-20. Retrieved 2018-03-22.
54. "GJ 581 g". The Extrasolar Planet Encyclopaedia. Exoplanet.eu. Archived from the original on 2018-03-24. Retrieved 2018-03-22.
55. González-Álvarez, E.; Osorio, M. R. Zapatero; Caballero, J. A.; Sanz-Forcada, J.; Béjar, V. J. S.; González-Cuesta, L.; Dreizler, S.; Bauer, F. F.; Rodríguez, E.; Tal-Or, L.; Zechmeister, M.; Montes, D.; López-González, M. J.; Ribas, I.; Reiners, A.; Quirrenbach, A.; Amado, P. J.; Anglada-Escudé, G.; Azzaro, M.; Cortés-Contreras, M.; Hatzes, A. P.; Henning, T.; Jeffers, S. V.; Kaminski, A.; Kürster, M.; Lafarga, M.; Morales, J. C.; Pallé, E.; Perger, M.; Schmitt, J. H. M. M. (29 March 2020). "The CARMENES search for exoplanets around M dwarfs. A super-Earth planet orbiting HD 79211 (GJ 338 B)". arXiv:2003.13052 [astro-ph.EP].
56. "GJ 625". NASA Exoplanet Science Institute. California Institute of Technology. Retrieved 2018-03-22.
57. "HD 219134". NASA Exoplanet Science Institute. California Institute of Technology. Retrieved 2018-03-22.
58. "HD 219134 e". The Extrasolar Planet Encyclopaedia. Exoplanet.eu. Archived from the original on 2017-12-01. Retrieved 2018-03-22.
59. Almenara, Jose-Manuel; Berlind, Perry; Bouchy, Franois; Burke, Chris J.; Delfosse, Xavier; D'iaz, Rodrigo F.; Dressing, Courtney D.; Esquerdo, Gilbert A.; Figueira, Pedro; Forveille, Thierry; Fur'esz, G'abor; Henze, Christopher E.; Jao, Wei-Chun; L'epine, S'ebastien; Levine, Alan M.; Lovis, Christophe; Mink, Jessica; Muirhead, Philip S.; Murgas, Felipe; Pepe, Francesco; Tenenbaum, Peter; Teske, Johanna K.; Twicken, Dr Joseph D.; Udry, St'ephane; Jenkins, Jon M.; Winn, Joshua N.; Seager, Sara; Latham, David W.; Vanderspek, Roland; Ricker, George R.; Bonfils, Xavier; Winston, Elaine; Diamond-Lowe, Hannah; Henry, Todd J.; Vrijmoet, Eliot; Eastman, Jason D.; Horch, Elliott P.; Astudillo-Defru, Nicola; Charbonneau, David; Irwin, Jonathan M.; Medina, Amber A.; Winters, Jennifer G. (24 June 2019). "Three Red Suns in the Sky: A Transiting, Terrestrial Planet in a Triple M Dwarf System at 6.9 Parsecs". arXiv:1906.10147. doi:10.3847/1538-3881/ab364d. Cite journal requires |journal= (help)
60. "GJ 667 C". NASA Exoplanet Science Institute. California Institute of Technology. Retrieved 2018-03-22.
61. "GJ 667 C d". The Extrasolar Planet Encyclopaedia. Exoplanet.eu. Archived from the original on 2017-12-01. Retrieved 2018-03-22.
62. "GJ 667 C h". The Extrasolar Planet Encyclopaedia. Exoplanet.eu. 2016-02-23. Archived from the original on 2017-12-01. Retrieved 2018-03-22.
63. Affer, L.; Damasso, M.; Micela, G.; Poretti, E.; Scandariato, G.; Maldonado, J.; Lanza, A. F.; Covino, E.; Rubio, A. Garrido; Hernandez, J. I. Gonzalez; Gratton, R.; Leto, G.; Maggio, A.; Perger, M.; Sozzetti, A.; Mascareno, A. Suarez; Bonomo, A. S.; Borsa, F.; Claudi, R.; Cosentino, R.; Desidera, S.; Molinari, E.; Pedani, M.; Pinamonti, M.; Rebolo, R.; Ribas, I.; Toledo-Padron, B. (16 January 2019). "HADES RV programme with HARPS-N at TNG. X. A super-Earth around the M dwarf Gl686". Astronomy & Astrophysics. A193: 622. arXiv:1901.05338. doi:10.1051/0004-6361/201834868.
64. "61 Vir". NASA Exoplanet Science Institute. California Institute of Technology. Retrieved 2018-03-22.
65. Bauer, F. F.; Zechmeister, M.; Kaminski, A.; López, C. Rodríguez; Caballero, J. A.; Azzaro, M.; Stahl, O.; Kossakowski, D.; Quirrenbach, A.; Jarque, S. Becerril; Rodríguez, E.; Amado, P. J.; Seifert, W.; Reiners, A.; Schäfer, S.; Ribas, I.; Béjar, V. J. S.; Cortés-Contreras, M.; Dreizler, S.; Hatzes, A.; Henning, T.; Jeffers, S. V.; Kürster, M.; Lafarga, M.; Montes, D.; Morales, J. C.; Schmitt, J. H. M. M.; Schweitzer, A.; Solano, E. (2 June 2020). "The CARMENES search for exoplanets around M dwarfs. Measuring precise radial velocities in the near infrared: the example of the super-Earth CD Cet b". arXiv:2006.01684 [astro-ph]. Retrieved 3 June 2020.
66. "HD 192310". NASA Exoplanet Science Institute. California Institute of Technology. Retrieved 2018-03-22.
67. "GJ 849". NASA Exoplanet Science Institute. California Institute of Technology. Retrieved 2018-03-22.
68. "GJ 433". NASA Exoplanet Science Institute. California Institute of Technology. Retrieved 2018-03-22.
69. "HD 102365". NASA Exoplanet Science Institute. California Institute of Technology. Retrieved 2018-03-22.
70. Wohler, B.; Winn, J. W.; Wang, S. X.; Twicken, J. D.; Teske, J.; Tamura, M.; Shectman, S. A.; Rowden, P.; Ricker, G. R.; Ribas, I.; Pedraz, S.; Nagel, E.; Murgas, F.; Morales, J. C.; Montañés-Rodríguez, P.; McDermott, S.; Latham, D. W.; Lafarga, M.; Kotani, T.; Klahr, H.; Kaminski, A.; Jenkins, J. M.; Feng, F.; Dynes, S.; Dressing, C. D.; Crane, J. D.; Collins, K. I.; Collins, K. A.; Chen, G.; Caldwell, D. A.; Butler, R. P.; Burt, J.; Burke, C. J.; Bluhm, P.; Bauer, F. F.; Batalha, N. E.; Anderson, D. R.; Amado, P. J.; Zechmeister, M.; Osorio, M. R. Zapatero; Trifonov, T.; Stock, S.; Schlecker, M.; Rodríguez-López, C.; Reiners, A.; Reffert, S.; Quirrenbach, A.; Parviainen, H.; Oshagh, M.; Ofir, A.; Nowak, G.; Narita, N.; Montes, D.; Molaverdikhani, K.; Kürster, M.; Kaltenegger, L.; Jeffers, S. V.; Henning, T.; Hellier, C.; Hatzes, A.; Díez-Alonso, E.; Cortés-Contreras, M.; Caballero, J. A.; Béjar, V. J. S.; Anglada-Escudé, G.; Espinoza, N.; Kemmer, J.; Dreizler, S.; Kossakowski, D.; Pallé, E.; Luque, R. (29 April 2019). "A planetary system around the nearby M dwarf Gl 357 including a transiting hot Earth-sized planet optimal for atmospheric characterisation". Astronomy & Astrophysics. A39: 628. arXiv:1904.12818. doi:10.1051/0004-6361/201935801.
71. "HD 285968". NASA Exoplanet Science Institute. California Institute of Technology. Retrieved 2018-03-22.
72. "GJ 176 c". The Extrasolar Planet Encyclopaedia. Exoplanet.eu. 2010-12-17. Archived from the original on 2014-02-23. Retrieved 2014-05-20.
73. Morales, J. C.; Mustill, A. J.; Ribas, I.; Davies, M. B.; Reiners, A.; Bauer, F. F.; Kossakowski, D.; Herrero, E.; Rodríguez, E.; López-González, M. J.; Rodríguez-López, C.; Béjar, V. J. S.; González-Cuesta, L.; Luque, R.; Pallé, E.; Perger, M.; Baroch, D.; Johansen, A.; Klahr, H.; Mordasini, C.; Anglada-Escudé, G.; Caballero, J. A.; Cortés-Contreras, M.; Dreizler, S.; Lafarga, M.; Nagel, E.; Passegger, V. M.; Reffert, S.; Rosich, A.; et al. (27 September 2019). "A giant exoplanet orbiting a very-low-mass star challenges planet formation models". Science. 365 (6460): 1441–1445. arXiv:1909.12174. Bibcode:2019Sci...365.1441M. doi:10.1126/science.aax3198. ISSN 0036-8075. PMID 31604272.
74. Plavchan, Peter; Barclay, Thomas; Gagné, Jonathan; et al. (2020). "A planet within the debris disk around the pre-main-sequence star AU Microscopii". Nature. 582: 497–500. arXiv:2006.13248. doi:10.1038/s41586-020-2400-z.
75. Lee, Rhodi (2015-09-18). "Want To Name An Exoplanet? Here's Your Chance". Tech Times. Archived from the original on 2015-09-07. Retrieved 2015-09-17.
76. "alf Cen B b". The Extrasolar Planet Encyclopaedia. Exoplanet.eu. 2011-05-27. Archived from the original on 2014-06-25. Retrieved 2014-05-17.
77. LePage, Andrew (2015-03-28). "Has Another Planet Been Found Orbiting Alpha Centauri B?". Drew Ex Machina. Archived from the original on 2015-09-29. Retrieved 2015-09-17.
78. Bartlett, Jennifer L; Ianna, Philip A; Begam, Michael C (2009). "A Search for Astrometric Companions to Stars in the Southern Hemisphere". Publications of the Astronomical Society of the Pacific. 121 (878): 365. Bibcode:2009PASP..121..365B. doi:10.1086/599044.
79. "GJ 682 b". The Extrasolar Planet Encyclopaedia. Exoplanet.eu. Archived from the original on 2015-04-02. Retrieved 2015-03-30.
80. "GJ 682 c". The Extrasolar Planet Encyclopaedia. Exoplanet.eu. Archived from the original on 2015-04-02. Retrieved 2015-03-30.
81. Barnes, J.R.; Jenkins, J. S.; Jones, H. R. A.; et al. (July 2012). "ROPS: A New Search for Habitable Earths in the Southern Sky". Monthly Notices of the Royal Astronomical Society. 424 (1): 591–604. arXiv:1204.6283. Bibcode:2012MNRAS.424..591B. doi:10.1111/j.1365-2966.2012.21236.x.
82. Farihi, J.; Becklin, E. E.; Macintosh, B. A. (June 2004). "Mid-Infrared Observations of van Maanen 2: No Substellar Companion". Astrophysical Journal Letters. 608 (2): L109–L112. arXiv:astro-ph/0405245. Bibcode:2004ApJ...608L.109F. doi:10.1086/422502.
83. Heinze, A. N.; Hinz, Philip M.; Sivanandam, Suresh; et al. (May 2010). "Constraints on Long-period Planets from an L'- and M-band Survey of Nearby Sun-like Stars: Observations". The Astrophysical Journal. 714 (2): 1551–1569. arXiv:1003.5340. Bibcode:2010ApJ...714.1551H. doi:10.1088/0004-637X/714/2/1551.
84. "VB 10 b". The Extrasolar Planet Encyclopaedia. Exoplanet.eu. Archived from the original on 2015-09-29. Retrieved 2015-09-17.
85. Boss, Alan P.; Butler, R. Paul; Hubbard, William B.; et al. (2007). "Working Group on Extrasolar Planets". Proceedings of the International Astronomical Union. 1 (T26A): 183. Bibcode:2007IAUTA..26..183B. doi:10.1017/S1743921306004509.
86. "SCR 1845 b". The Extrasolar Planet Encyclopaedia. Exoplanet.eu. 2012-04-13. Archived from the original on 2015-10-01. Retrieved 2015-09-17.
87. "SDSS 141624 b". The Extrasolar Planet Encyclopaedia. Exoplanet.eu. 2010-01-18. Archived from the original on 2014-02-23. Retrieved 2014-05-20.
88. "WISE 1217+16A b". The Extrasolar Planet Encyclopaedia. Exoplanet.eu. Archived from the original on 2017-06-12. Retrieved 2014-05-17.
89. Clavin, Whitney; Harrington, J. D. (2014-04-25). "NASA's Spitzer and WISE Telescopes Find Close, Cold Neighbor of Sun". NASA. Archived from the original on 2014-04-26. Retrieved 2015-09-17.
90. Lucas, P. W.; Tinney, C. G.; Burningham, B.; et al. (2010). "The discovery of a very cool, very nearby brown dwarf in the Galactic plane". Monthly Notices of the Royal Astronomical Society. 408 (1): L56–L60. arXiv:1004.0317. Bibcode:2010MNRAS.408L..56L. doi:10.1111/j.1745-3933.2010.00927.x.
91. Cushing, Michael C.; Kirkpatrick, J. Davy; Gelino, Christopher R.; et al. (2011). "The Discovery of Y Dwarfs using Data from the Wide-field Infrared Survey Explorer (WISE)". The Astrophysical Journal. 743 (1): 50. arXiv:1108.4678. Bibcode:2011ApJ...743...50C. doi:10.1088/0004-637X/743/1/50.
92. "Astronomers discover a nearby free-range planet with incredible magne".
93. "Stars within 10 parsecs".
94. Bortle, John E. (2001). "Light Pollution And Astronomy: The Bortle Dark-Sky Scale". Sky & Telescope. Archived from the original on 2009-03-23. Retrieved 2014-05-20.
95. "HEC: Periodic Table of Exoplanets". Planetary Habitability Laboratory. University of Puerto Rico at Arecibo. 2014-04-17. Archived from the original on 2014-07-03. Retrieved 2014-05-17.
96. Johnston, Robert (2014-11-02). "List of Nearby Stars: To 21 light years". Johnstonsarchive.net. Archived from the original on 2015-10-16. Retrieved 2015-09-17.
97. "epsilon Eridani". NameExoWorlds. International Astronomical Union. Archived from the original on 2018-02-15. Retrieved 2018-05-14.
98. "Fomalhaut (alpha Piscis Austrini)". Nameexoworlds. International Astronomical Union. Archived from the original on 2017-04-30. Retrieved 2018-05-14.
99. Cumming, Andrew; Butler, R. Paul; Marcy, Geoffrey W.; et al. (2008). "The Keck Planet Search: Detectability and the Minimum Mass and Orbital Period Distribution of Extrasolar Planets". Publications of the Astronomical Society of the Pacific. 120 (867): 531–554. arXiv:0803.3357. Bibcode:2008PASP..120..531C. doi:10.1086/588487.

External links

• "Extrasolar Planets". The Planetary Society. Planetary.org.
• "Extrasolar Planets News". Science Daily.
• "Exoplanet Exploration: Planets Beyond our Solar System". Exoplanet Exploration Program and Jet Propulsion Laboratory. NASA. 2015-12-16.
• "Universe - Exoplanets (pictures, video, facts & news)". BBC. Archived from the original on 2018-02-13. Retrieved 2018-03-23.
• "PHL's Exoplanets Catalog". Planetary Habitability Laboratory. UPR Arecibo. 2018-03-02.
• Onsi Fakhouri. "Exoplanet Orbit Database". Exoplanet Data Explorer. Exoplanets.org.
• "NASA Exoplanet Archive". Caltech.
• "Stars Within 20 Light Years". Atlas of the Universe.