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List of multiplanetary systems

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(Redirected fromList of exoplanetary host stars)

List of systems with multiple planets

Further information:Planetary system

Number of extrasolar planet discoveries per year through 2023. Colors indicate method of detection.
  Direct imaging
  Gravitational microlensing
  Pulsar timing
  Radial velocity
  Transit photometry

From the total of 4,490 stars known to haveexoplanets (as of October 2, 2025), there are a total of 1,017 known multiplanetary systems,^[1] or stars with at least two confirmed planets, beyond theSolar System. This list includes systems with at least three confirmed planets or two confirmed planets where additional candidates have been proposed. The stars with the most confirmed planets are theSun (the Solar System's star) andKepler-90, with eight confirmed planets each, followed byTRAPPIST-1 with seven planets.

The 1,013 multiplanetary systems are listed below according to the star's distance from Earth. Proxima Centauri, the closest star to the Solar System, has at least two planets (the confirmedb,d and the disputedc^[2]). The nearest system with four or more confirmed planets isBarnard Star, with four known.^[3] The farthest confirmed system with two or more planets isOGLE-2012-BLG-0026L, at 13,300 light-years (4,100 pc) away.^[4]

The table below contains information about the coordinates, spectral and physical properties, and the number of confirmed (unconfirmed) planets for systems with at least two planets and one not confirmed. The two most importantstellar properties aremass andmetallicity because they determine how theseplanetary systems form. Systems with higher mass and metallicity tend to have more planets and more massive planets. However, although low metallicity stars tend to have fewer massive planets, particularly hot-Jupiters, they also tend to have a larger number of close-in planets, orbiting at less than oneAU.^[5]

Multiplanetary systems

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This is adynamic list and may never be able to satisfy particular standards for completeness. You can help byediting the page to add missing items, with references toreliable sources.

Color indicates number of planets
2 (x)	3	4	5	6	7	8	9

Star	Constellation	Right ascension	Declination	Apparent magnitude	Distance (ly)	Spectral type	Mass (M_☉)	Temperature (K)	Age (Gyr)	Confirmed (unconfirmed) planets	Notes
Sun	N/A	N/A	N/A	−26.74	0.000016	G2V	1	5778	4.572	8 (2)	Has 8 confirmed planets, and 2 unconfirmed ones. Only known system to have life.
Proxima Centauri	Centaurus	14^h 29^m 42.94853^s	−62° 40′ 46.1631″	10.43 to 11.11^[6]	4.244	M5.5Ve^[7]	0.122	3042	4.85	2 (1)	Closest star to the Sun and closest star to the Sun with a multiplanetary system. Planet b is potentially habitable.^[8]^[9]
Barnard's Star	Ophiuchus	17^h 57^m 48.4985^s	+04° 41′ 36.1139″	9.511	5.96	M4.0V^[10]	0.162	3195	10	4	Closest single star to the Sun with a confirmed multiplanetary system.^[3]
Lalande 21185	Ursa Major	11^h 03^m 20.1940^s	+35° 58′ 11.5682″	7.520^[11]	8.3044±0.0007	M2V	0.39	3601±51	8.047	2 (1)	Brightestred dwarf star in the northern celestial hemisphere.^[12]^[13]
Lacaille 9352	Piscis Austrinus	23^h 05^m 52.04^s	−35° 51′ 11.05″	7.34	10.721	M0.5V	0.486	3688±86	4.57	2 (1)	The unconfirmed planet d is potentially habitable.^[14]
Luyten's Star	Canis Minor	07^h 27^m 24.4991^s	05° 13′ 32.827″	9.872	11.20	M3.5V	0.26	3150	unknown	2 (2)	Stellar activity level and rotational rate suggest an age higher than 8 billion years.^[15] Planet b is potentially habitable.^[16]
YZ Ceti	Cetus	01^h 12^m 30.64^s	−16° 59′ 56.3″	12.07	11.74	M4.5V	0.13	3056	4	3 (1)	Flare star.^[17]
Gliese 1061	Horologium	03^h 35^m 59.69^s	−44° 30′ 45.3″	13.03	12.04	M5.5V	0.113	2953	unknown	3	Planets c and d are potentially habitable.^[18]
Teegarden's Star	Aries	02^h 53^m 00.89^s	+16° 52′ 53″	15.13	12.497	M7V	0.097	3034	8	3	Teegarden's Star b and Teegarden's Star c are likely Earth-mass planets that orbit in the habitable zone.^[19]
Wolf 1061	Ophiuchus	16^h 30^m 18.0584^s	−12° 39′ 45.325″	10.07	14.050 ± 0.002	M3.5V	0.294	3342	unknown	3	Planet c is potentially habitable.^[20]^[21]^[22]
Gliese 876	Aquarius	22^h 53^m 16.73^s	−14° 15′ 49.3″	10.17	15.25	M4V	0.334	3348	4.893	4	Planet b is a gas giant which orbits in the habitable zone.^[23]
82 G. Eridani	Eridanus	03^h 19^m 55.65^s	−43° 04′ 11.2″	4.254	19.71	G8V	0.7	5401	5.76	3 (3)	This star also has a dust disk^[24] with a semi-major axis at approximately 19 AU.^[25]
Gliese 581	Libra	15^h 19^m 26.83^s	−07° 43′ 20.2″	10.56	20.56	M3V	0.311	3484	4.326	3 (1)	The disputed planet d is potentially habitable.^[26]
Gliese 667 C	Scorpius	17^h 18^m 57.16^s	−34° 59′ 23.14″	10.20	21	M1.5V	0.31	3700	2	2 (1)	Triple star system - all exoplanets orbit around Star C. Planet c is potentially habitable, There were thought to be up to 5 more planets orbiting the star, Gliese 667 Cd, Ce, Cf, Cg, and Ch but most of them were false positives except for planet d which remains uncomfirmed .^[27]^[28]^[29]
HD 219134	Cassiopeia	23^h 13^m 14.74^s	57° 10′ 03.5″	5.57	21	K3Vvar	0.794	4699	12.66	6	Closest star to the Sun with exactly six^[30] exoplanets, and closestK-type main sequence star to the Sun with a multiplanetary system. One of the oldest stars with a multiplanetary system, although it is still more metal-rich than the Sun. None of the known planets is in the habitable zone.^[31]
61 Virginis	Virgo	13^h 18^m 24.31^s	−18° 18′ 40.3″	4.74	28	G5V	0.954	5531	8.96	2 (1)	Planet d remains unconfirmed,^[32] and a 2021 study found that it was likely a false positive.^[33] 61 Virginis also has a debris disk.
Gliese 433	Hydra	11^h 35^m 26.9485^s	−25° 10′ 08.9″	9.79	29.8±0.1	M1.5V	0.48	3550±100	unknown	3	Aninfrared excess around this star suggests acircumstellar disk.^[34]
Gliese 357	Hydra	09^h 36^m 01.6373^s	−21° 39′ 38.878″	10.906	30.776	M2.5V	0.362	3488	unknown	3	Planet d is a potentially habitable Super-Earth.^[35]^[36]^[37]^[38]
L 98-59	Volans	08^h 18^m 07.62^s	−68° 18′ 46.8″	11.69	34.6	M3V	0.312	3412	unknown	5 (1)	The unconfirmed planet g orbits in closer than b.^[39]
Gliese 414 A	Ursa Major	11^h 11^m 05.88^s	30° 26′ 42.61″	8.31	38.76	K7V	0.65	4120	12.4	2 (0)	^[40]^[41]
Gliese 806	Cygnus	20^h 45^m 04.099^s	+44° 29′ 56.6″	10.79	39.3	M1.5V	0.423	3586	3	2 (1)	-
TRAPPIST-1	Aquarius	23^h 06^m 29.283^s	−05° 02′ 28.59″	18.80	39.5	M8V	0.089	2550	7.6	7 (1)	Planets d, e, f and g are potentially habitable. Only star known with exactly seven confirmed planets. All seven confirmed terrestrial planets lie within only 0.07 AU of the star.
55 Cancri	Cancer	08^h 52^m 35.8111^s	+28° 19′ 50.96″	5.95	41.05	K0IV-V+M4.5V	0.905	5172	8.6	6 (2)	At least 4 planets around primary, and 2 planet around secondary star. Planets55 Cancri Ad and 55 Cancri Ag are unconfirmed. All but55 Cancri Ae (which is asuper-earth) aregiant planets. Two others orbit around star B. First star system known where more than one star has an individual planetary system.
Gliese 180	Eridanus	04^h 53^m 49.9798^s	−17° 46′ 24.294″	10.894	40.3	M2V^[42] or M3V^[43]	0.39	3562	unknown	3	The habitability of planets b and c is disputed.^[44]^[45]
HD 69830	Puppis	08^h 18^m 23.95^s	−12° 37′ 55.8″	5.95	41	K0V	0.856	5385	7.446	3	A debris disk exterior to the three exoplanets was detected by theSpitzer Space Telescope in 2005.^[46]
HD 40307	Pictor	05^h 54^m 04.24^s	−60° 01′ 24.5″	7.17	42	K2.5V	0.752	4977	1.198	4 (2)	The existence of planets e and g are disputed.^[47] If confirmed, planet g is potentially habitable.^[48]
Upsilon Andromedae	Andromeda	01^h 36^m 47.84^s	+41° 24′ 19.7″	4.09	44	F8V	1.27	6107	3.781	3 (1)	NearestF-type main sequence star with a multiplanetary system. Second-brightest star in the night sky with a multiplanetary system after7 Canis Majoris. All exoplanets orbit around star A in the binary system. The existence Of Planet e is disputed.
47 Ursae Majoris	Ursa Major	10^h 59^m 27.97^s	+40° 25′ 48.9″	5.10	46	G0V	1.029	5892	7.434	3	Planet Taphao Thong was discovered in 1996 and was one of the first exoplanets to be discovered.^[49] The planet was the firstlong-period extrasolar planet discovered. The other planets were discovered later.^[50]
Nu² Lupi	Lupus	15^h 21^m 49.57^s	−48° 19′ 01.1″	5.65	47	G2V	0.906	5664	10.36	3	One of the oldest stars in the solar neighbourhood.^[51]^[52]^[53]
LHS 1140	Cetus	00^h 44^m 59.31^s	−15° 16′ 16.7″	14.18	48.9	M4.5V^[54]	0.179	3216±39	5	2 (1)	Planet b is a potentially habitable Super-Earth.^[55]
Gliese 163	Dorado	04^h 09^m 16^s	−53° 22′ 25″	11.8	49	M3.5V	0.4	unknown	3	5	Planet c is possibly a potentially habitable Super-Earth but is probably too hot or massive.^[56]^[57]
Mu Arae	Ara	17^h 44^m 08.70^s	−51° 50′ 02.6″	5.15	51	G3IV-V	1.077	5704	6.413	4	Planet Quijote orbits in thecircumstellar habitable zone. However, it is agas giant, so it itself is uninhabitable although a large moon orbiting around it may behabitable.
GJ 3929	Corona Borealis	15^h 58^m 18.8^s	35° 24′ 24.3″	12.67	51.58	M3.5V	0.313	3384	unknown	2 (0)	^[58]^[59]
Gliese 676 A	Ara	17^h 30^m 11.2042^s	−51° 38′ 13.116″	9.59	53	M0V	0.71	unknown	unknown	4	Held the record for widest range of masses in a planetary system in 2012.^[60]
HD 7924	Cassiopeia	01^h 21^m 59.12^s	+76° 42′ 37.0″	7.19	55	K0V	0.832	5177	unknown	3	These planets may be potentially habitable Super-Earths.^[61]
Pi Mensae	Mensa	05^h 37^m 09.8851^s	−80° 28′ 08.8313″	5.65	59.62±0.07	G0V	1.11	6013	3.4	3	Outer planet is likely abrown dwarf.^[62]
Gliese 3293	Eridanus	04^h 28^m 35.72^s	−25° 10′ 08.9″	11.96	59	M2.5V	0.42	3466±49	unknown	4	Planets b and d orbit in the habitable zone.^[16]
LHS 1678	Caelum	04^h 32^m 43^s	−39° 47′ 21″	12	64.8	M2V	0.345	3490	unknown	3 (0)	^[63]
HD 104067	Corvus	11^h 59^m 10.0^s	−20° 21′ 13.6″	7.92	66.3	K3V	0.82	4942	4.8	2 (1)	The innermost planet, which is unconfirmed, might suffer from significanttidal heating.^[64]
HD 142	Phoenix	00^h 06^m 19.0^s	−49° 04′ 30″	5.70	67	G1 IV	1.1	6180	5.93	3	-
HD 215152	Aquarius	22^h 43^m 21^s	−06° 24′ 03″	8.13	70	G8IV	1.019	5646	7.32	4	A debris disk candidate as it has an infrared excess.^[65]
HD 164922	Hercules	18^h 02^m 30.86^s	+26° 18′ 46.8″	7.01	72	G9V^[66]	0.874	5293	13.4	4	Oldest star with a multiplanetary system. Despite its age, it is more metal-rich than the Sun.^[66]
HD 63433	Gemini	07^h 49^m 55.0^s	+27° 21′ 47.4″	6.92	73	G5V	0.99	5640	0.4	3
HIP 57274	Ursa Major	11^h 44^m 41^s	+30° 57′ 33″	8.96	85	K5V	0.73	4640	7.87	3	-
HD 39194	Mensa	05^h 44^m 32^s	−70° 08′ 37″	8.08	86.2	K0V	unknown	5205	unknown	3	The planets have eccentric orbits.^[67]
LP 791-18	Crater	11^h 02^m 45.95^s	−16° 24′ 22.3″	16.9	86.9	M6V/M7V	0.139	2960	0.5	3	planet d could be volcanically active because its elliptical orbit is periodically stretched and squeezed by the gravitational pull of a larger neighboring planet, LP 791-18 c.
HD 181433	Pavo	19^h 25^m 09.57^s	−66° 28′ 07.7″	8.38	87	K5V	0.777	4962	8.974	3	-
HD 134606	Apus	15^h 15^m 15^s	−70° 31′ 11″	6.85	87	G6IV	unknown	unknown	unknown	5	The planets have moderately eccentric orbits.^[68]
HD 158259	Draco	17^h 25^m 24.0^s	+52° 47′ 26″	6.46	89	G0	1.08	unknown	unknown	5 (1)	A G-type star slightly more massive than the Sun.^[69] Planet g remains unconfirmed.^[69]
HD 82943	Hydra	09^h 34^m 50.74^s	−12° 07′ 46.4″	6.54	90	F9V Fe+0.5^[70]	1.175	5874	3.08	3	Planets b and c are in a 2:1 orbital resonance.^[71] Planet b orbits in the habitable zone, but it and planet c are massive enough to bebrown dwarfs. HD 82943 has an unusuallithium-6 abundance.^[72]
Gliese 3138	Cetus	02^h 09^m 10.90^s	−16° 20′ 22.53″	10.877	92.9		0.681	3717±49	unknown	3
GJ 9827	Pisces	23^h 27^m 04.84^s	−01° 17′ 10.59″	10.10	96.8±0.2	K6V	0.593	4294±52	unknown	3	Also known as K2-135. Planet b is extremely dense, with at least half of its mass being iron.^[73]
Iota Draconis	Draco	15^h 24^m 55.8^s	+58° 57′ 57.3″	3.290	101.2	unknown	1.56	4504	2.49	2	Iota Draconis is already in its red giant phase, both planets have very eccentric orbits.
K2-239	Sextans	10^h 42^m 22.63^s	+04° 26′ 28.86″	14.5	101.5	M3V	0.4	3420	unknown	3
TOI-700	Dorado	06^h 28^m 22.97^s	−65° 34′ 43.01″	13.10	101.61	M2V	0.416	3480	1.5	4	Planets d and e are potentially habitable.^[74]^[75]^[76]
HD 17926	Fornax	02^h 51^m 56.16^s	−30° 48′ 53.2″	6.38	105	F6V	1.145	6201	unknown	3	The star forms a binary with a red dwarf.^[77]
HD 37124	Taurus	05^h 37^m 02.49^s	+20° 43′ 50.8″	7.68	110	G4V	0.83	5606	3.327	3	Planet c orbits at the outer edge of the habitable zone.^[78]
HD 20781	Fornax	03^h 20^m 03^s	−28° 47′ 02″	8.44	115	G9.5V	0.7	5256±29	unknown	4	Located in binary star system.^[79]^[80]
Kepler-444	Lyra	19^h 19^m 01^s	41° 38′ 05″	9.0	117	K0V	0.758	5040	11.23	5	Nearest multiplanetary system where the planets were discovered by theKepler space telescope.
HD 141399	Boötes	15^h 46^m 54.0^s	+46° 59′ 11″	7.2	118	K0V	1.07	5600	unknown	4	Planet c orbits in the habitable zone.^[81]
Kepler-42	Cygnus	19^h 28^m 53^s	+44° 37′ 10″	16.12	126	M5V^[82]	0.13	3068	unknown	3	Host 3 sub earths orbiting it.
HD 31527	Lepus	04^h 55^m 38^s	−23° 14′ 31″	7.48	126	G0V	unknown	unknown	unknown	3	-
HD 10180	Hydrus	01^h 37^m 53.58^s	−60° 30′ 41.5″	7.33	127	G1V	1.055	5911	4.335	6 (3)	Has 6 confirmed planets orbiting around it, Evidence for 3 more planets in the system exist, If these worlds are confirmed, this system would be the largest planetary system found.^[83]
HD 23472	Reticulum	03^h 41^m 50.3988^s	−62° 46′ 01.4772″	9.72	127.48	K3.5V	0.67	4684±99	unknown	5
HR 8799	Pegasus	23^h 07^m 28.72^s	+21° 08′ 03.3″	5.96	129	A5V	1.472	7429	0.064	4 (1)	OnlyA-type main sequence star with a known multiplanetary system, and hottest and most massive single main sequence star with a multiplanetary system. All four planets are massivesuper-Jupiters.
HD 27894	Reticulum	04^h 20^m 47.05^s	−59° 24′ 39.0″	9.42	138	K2V	0.8	4875	3.9	3	-
HD 93385	Vela	10^h 46^m 15.1160^s	−41° 27′ 51.7261″	7.486	141.6	G2V	1.07	5823	4.13	3
K2-3	Leo	11^h 29^m 20.3918^s	−01° 27′ 17.280″	12.168	143.9±0.4	M0V	0.601	3835±70	1	3	The outermost planet orbits in the habitable zone.^[84]
HD 34445	Orion	05^h 17^m 41.0^s	+07° 21′ 12″	7.31	152	G0V	1.07	5836	8.5	1 (5)	Some planets were not detected or inferred to be false positives in a later study.^[33]
HD 204313	Capricornus	21^h 28^m 12.21^s	–21° 43′ 34.5″	7.99	154	G5V	1.045	5767	3.38	3	-
HD 3167	Pisces	00^h 34^m 57.5^s	+04° 22′ 53″	8.97	154.4	K0V	0.852	5300	10.2	4	-
HIP 34269	Puppis	07^h 06^m 13.98^s	−47° 35′ 13.87″	10.59	154.81		0.74	4440±100	unknown	4
HD 133131	Libra	15^h 03^m 35.80651^s	−27° 50′ 27.5520″	8.4	168	G2V+G2V^[85]	0.95	5799±19	6	3	2 planets around primary, and 1 planet around secondary star.^[85]
K2-136	Taurus	04^h 29^m 38.99^s	+22° 52′ 57.80″	11.2	173	K5V	0.71	4364±70	0.7	3
HIP 14810	Aries	03^h 11^m 14.23^s	+21° 05′ 50.5″	8.51	174	G5V	0.989	5485	5.271	3	-
HD 191939	Draco	20^h 08^m 05.75^s	+66° 51′ 2.1″	8.971	175	G9V	0.81	5348	8.7	6	^[86]
HD 125612	Virgo	14^h 20^m 53.51^s	−17° 28′ 53.5″	8.33	177	G3V	1.099	5897	2.15	3	-
TOI-2267	Cepheus	4^h 20^m 14.8^s	+84° 54′ 2.9″	17	190	M5V+M6V	0.171	2930	8	2 (1)	One of the few planetary systems to potential have both stars having planets around them, TOI-2267 b, and c orbit star A, the unconfirmed planet d would orbit star b if it exists.
HD 184010	Vulpecula	19^h 31^m 22.0^s	+26° 37′ 02″	5.9	200	KOIII-IV	1.35	4971	2.76	3	-
HD 109271	Virgo	12^h 33^m 36.0^s	−11° 37′ 19″	8.05	202	G5	1.047	5783	7.3	2 (1)	-
HD 38677	Orion	05^h 47^m 06.0^s	−10° 37′ 49″″	8.0	202	F8V	1.21	6196.0	2.01	4	-
TOI-178	Sculptor	00^h 29^m 12.30^s	30° 27′ 13.46″	11.95	205.16	K7V^[87]	0.65	4316±70	7.1	6	The planets are in anorbital resonance.^[87]
HD 108236	Centaurus	12^h 26^m 17.89^s	−51° 21′ 46.21″	9.24	211	G3V	0.97	5730	5.8	5	-
Kepler-37	Lyra	18^h 58^m 23.1^s	44° 31′ 05″	9.77	215	G8V	0.803	5417	6	3 (1)	The existence of Kepler-37e is dubious.^[88]
K2-72	Aquarius	22^h 18^m 29.2548^s	−09° 36′ 44.3824″	15.04	217	M2V	0.27	3497	unknown	4	2 planets in habitable zone
Kepler-138	Lyra	19^h 21^m 32.0^s	+43° 17′ 35″	13.5	218.5	M1V	0.57	3871	2.3	3 (1)	Planet b is one of the smallest exoplanets known, planets c and d are the first confirmed exoplanets that are likely mostly water.
K2-233	Libra	15^h 21^m 55.2^s	−20° 13′ 54″	10.0	221	K3	0.8	4950	0.36	3
TOI-1260	Ursa Major	10^h 28^m 35.03^s	+65° 51′ 16.38″	11.973	239.5		0.66	4227±85	6.7	3
LP 358-499	Taurus	04^h 40^m 35.64^s	+25° 00′ 36.05″	13.996	245.3		0.46	3655±80	unknown	4	Also known as K2-133
K2-266	Sextans	10^h 31^m 44.5^s	+00° 56′ 15″		252	K	0.69	4285	8.4	4 (2)
K2-155	Taurus	04^h 21^m 52.5^s	+21° 21′ 13″	12.8	267	K7	0.65	4258	unknown	3
K2-384	Cetus	01^h 21^m 59.86^s	00° 45′ 04.41″	16.12	270	M?V	0.33	3623±138	unknown	5
TOI-1136	Draco	12^h 48^m 44.38^s	+64° 51′ 18.99″	9.534	275.8		1.022	5770±50	0.7	6 (1)	The planets are in an orbital resonance.^[89]
TOI-561	Sextans	09^h 52^m 44.44^s	+06° 12′ 57.97″	10.252	279	G9V	0.785	5455	5	4 (1)	-
Kepler-445	Cygnus	19^h 54^m 57.0^s	+46° 29′ 55″	18	294		0.18	3157	unknown	3	-
TOI-763	Centaurus	12^h 57^m 52.45^s	−39° 45′ 27.71″	10.156	311		0.917	5444	6.2	2 (1)	-
K2-229	Virgo	12^h 27^m 29.5848^s	−06° 43′ 18.7660″	10.985	335	K2V	0.837	5185	5.4	3
Kepler-102	Lyra	18^h 45^m 55.9^s	+47° 12′ 29″	11.492	340	K3V^[90]	0.81	4809	1.41	5
V1298 Tauri	Taurus	04^h 05^m 19.5912^s	+20° 09′ 25.5635″	10.31	354	K0-1.5^[91]	1.101	4970	0.023	4	This star is a youngT Tauri variable.^[92]
K2-302	Aquarius	22^h 20^m 22.7764^s	−09° 30′ 34.2934″	11.98	359.3		unknown	3297±73	unknown	3
K2-198	Virgo	13^h 15^m 22.5^s	−06° 27′ 54″	11.0	362		0.8	5213	unknown	3
TOI-125	Hydrus	01^h 34^m 22.73^s	−66° 40′ 32.95″	11.02	363		0.859	5320	unknown	3 (2)
HIP 41378	Cancer	08^h 26^m 28.0^s	+10° 04′ 49″	8.9	378	F8	1.15	6199	unknown	5 (2)	Planet f has an unusually low density, and might have rings or an extended atmosphere.^[93]^[94] More planets are still suspected.^[95]
Kepler-446	Lyra	18^h 49^m 00.0^s	+44° 55′ 16″	16.5	391	M4V	0.22	3359	unknown	3	-
HD 33142	Lepus	05^h 07^m 35.54^s	−13° 59′ 11.34″	7.96	394.3		1.52	5025⁺²⁴ ₋₁₆	unknown	3	Host star is a giant star with spectral type of K0III.^[96]
WASP-132	Lupus	14^h 30^m 26.2^s	−46° 09′ 33″	11.938	403	K4V	0.782	4714	7.2	3
K2-148	Cetus	00^h 58^m 04.28^s	−00° 11′ 35.36″	13.05	407	K7V	0.65	4079±70	unknown	3	A secondary red dwarf is gravitationally bound to K2-148.^[97]
Kepler-68	Cygnus	19^h 24^m 07.76^s	+49° 02′ 25.0″	8.588	440	G1V	1.079	5793	6.3	3 (1)	Planet d, the outermost confirmed planet, is a Jupiter-sized planet which orbits in the habitable zone.^[98] Radial velocity measurements discovered an additional signal, which could be a fourth planet or a stellar companion.^[99]
HD 28109	Hydrus	04^h 20^m 57.13^s	−68° 06′ 09.51″	9.38	457		1.26	6120±50	unknown	3
COROT-7	Monoceros	06^h 43^m 49.47^s	−01° 03′ 46.9″	11.73	489	K0V	0.93	5275	1.5	3
XO-2	Lynx	07^h 48^m 07.4814^s	+50° 13′ 03.2578″	11.18	496±3	K0V+K0V	unknown	unknown	6.3	4	Binary with each star orbited by two planets.^[100]^[101]
Kepler-411	Cygnus	19^h 10^m 25.3^s	+49° 31′ 24″	12.5	499.4	K3V	0.83	4974	unknown	5
K2-381	Sagittarius	19^h 12^m 06.46^s	−21° 00′ 27.51″	13.01	505	K2	0.754	4473±138	unknown	3
K2-285	Pisces	23^h 17^m 32.2^s	+01° 18′ 01″	12.03	508	K2V	0.83	4975	unknown	4
K2-32	Ophiuchus	16^h 49^m 42.2602^s	−19° 32′ 34.151″	12.31	510	G9V	0.856	5275	7.9	4	The planets are likely in a 1:2:5:7 orbital resonance.^[102]
TOI-1246	Draco	16^h 44^m 27.96^s	70° 25′ 46.70″	11.6	558		1.12	5217±50	unknown	4
K2-352	Cancer	09^h 21^m 46.8434^s	+18° 28′ 10.34710″	11.12	577	G2V	0.98	5791	unknown	3
Kepler-398	Lyra	19^h 25^m 52.5^s	+40° 20′ 38″		578	K5V	0.72	4493	unknown	3
Kepler-186	Cygnus	19^h 54^m 36.6^s	+43° 57′ 18″	15.29^[103]	579.23^[104]	M1V^[105]	0.478	3788	unknown	5	Planet f is the first Earth-size exoplanet discovered that orbits in the habitable zone.^[106]
K2-37	Scorpius	16^h 13^m 48.2445^s	−24° 47′ 13.4279″	12.52	590	G3V	0.9	5413	unknown	3
K2-58	Aquarius	22^h 15^m 17.2364^s	−14° 02′ 59.3151″	12.13	596	K2V	0.89	5038	unknown	3
K2-138	Aquarius	23^h 15^m 47.77^s	−10° 50′ 58.91″	12.21	597±55	K1V	0.93	5378±60	2.3	6	Planet g was not fully verified, or could be two long-period planets instead.^[107]
K2-38	Scorpius	16^h 00^m 08.06^s	−23° 11′ 21.33″	11.34	630	G3V	1.03	5731±66	unknown	2 (1)	Dust disk in system
WASP-47	Aquarius	22^h 04^m 49.0^s	−12° 01′ 08″	11.9	652	G9V	1.084	5400	unknown	4	One planet is a gas giant which orbits in the habitable zone.^[108]^[109] WASP-47 is the only planetary system known to have both planets near thehot Jupiter and another planet much further out.^[110]
K2-368	Aquarius	22^h 10^m 32.58^s	−11° 09′ 58.02″	13.54	674	K3	0.746	4663±138	unknown	3 (1)
HAT-P-13	Ursa Major	08^h 39^m 31.81^s	+47° 21′ 07.3″	10.62	698	G4	1.22	5638	5	2 (1)	-
Kepler-19	Cygnus	19^h 21^m 41^s	+37° 51′ 06″	15.178	717	G	0.936	5541	1.9	3	System consists of a thick-envelope Super-Earth and two Neptune-mass planets.^[111]
Kepler-296	Lyra	19^h 06^m 09.6^s	+49° 26′ 14.4″	12.6	737.113	K7V + M1V^[112]	unknown	4249	unknown	5	All planets orbit around the primary star.^[113] Planets e and f are potentially habitable.^[113]
Kepler-454	Lyra	19^h 09^m 55.0^s	+38° 13′ 44″	11.57	753	G	1.028	5687	5.25	3
Kepler-25	Lyra	19^h 06^m 33.0^s	+39° 29′ 16″	11	799	F^[114]	1.22	6190	unknown	3	Two planets were discovered by transit-timing variations,^[115] and the third planet was discovered by follow-up radial velocity measurements.^[116]
Kepler-114	Cygnus	19^h 36^m 29.0^s	+48° 20′ 58″	13.7	846	K	0.71	4450	unknown	3
Kepler-54	Cygnus	19^h 39^m 06.0^s	+43° 03′ 23″	16.3	886	M	0.52	3705	unknown	3
Kepler-20	Lyra	19^h 10^m 47.524^s	42° 20′ 19.30″	12.51	950	G8V	0.912	5466	8.8	5 (1)	Planets e and f were the first Earth-sized planets to be discovered.^[117]
K2-19	Virgo	11^h 39^m 50.4804^s	+00° 36′ 12.8773″	13.002	976	K0V^[118] or G9V^[119]	0.918	5250±70	8	3	-
PSR B1257+12	Virgo	13^h 00^m 03.58^s	+12° 40′ 56.5″	24.31	980	pulsar	1.444	28856	0.797	3	Only pulsar with a multiplanetary system, and first exoplanets and multiplanetary system to be confirmed.^[120]^[121] Star with dimmest apparent magnitude to have a multiplanetary system.
Kepler-62	Lyra	18^h 52^m 51.060^s	+45° 20′ 59.507″	13.75^[122]	990	K2V^[122]	0.69	4925	7	5	Planets e and f orbit in the habitable zone.^[122]^[123]
Kepler-48	Cygnus	19^h 56^m 33.41^s	+40° 56′ 56.47″	13.04	1000	K	0.88	5190	unknown	5
Kepler-100	Lyra	19^h 25^m 32.6^s	+41° 59′ 24″		1011	G1IV	1.109	5825	6.5	4
Kepler-49	Cygnus	19^h 29^m 11.0^s	+40° 35′ 30″	15.5	1015	K	0.55	3974	unknown	4
Kepler-65	Lyra	19^h 14^m 45.3^s	+41° 09′ 04.2″	11.018	1019	F6IV	1.199	6211	unknown	4	-
Kepler-52	Draco	19^h 06^m 57.0^s	+49° 58′ 33″	15.5	1049	K	0.58	4075	unknown	3
K2-314	Libra	15^h 13^m 00.0^s	−16° 43′ 29″	11.4	1059	G8IV/V	1.05	5430	9	3
K2-219	Pisces	00^h 51^m 22.9^s	+08° 52′ 04″	12.09	1071	G2	1.02	5753±50	unknown	3
K2-268	Cancer	08^h 54^m 50.2862^s	+11° 50′ 53.7745″	13.85	1079		unknown	unknown	unknown	5
K2-183	Cancer	08^h 20^m 01.7184^s	14° 01′ 10.0711″	12.85	1083		unknown	5482±50	unknown	3
K2-187	Cancer	08^h 50^m 05.6682^s	23° 11′ 33.3712″	12.864	1090	G?V	0.967	5438±63	unknown	4
Kepler-1542	Lyra	19^h 02^m 54.8^s	+42° 39′ 16″		1096	G5V	0.94	5564	unknown	4 (1)	-
Kepler-26	Lyra	18^h 59^m 46^s	+46° 34′ 00″	16	1100	M0V	0.65	4500	unknown	4	Transiting exoplanets^[124] which are low-density planets below the size ofNeptune.^[125]^[126]
Kepler-167	Cygnus	19^h 30^m 38.0^s	+38° 20′ 43″		1119 ± 6		0.76	4796	unknown	4	Planet e is the first transiting Jupiter analog discovered.^[127]^[128]
Kepler-81	Cygnus	19^h 34^m 32.9^s	+42° 49′ 30″	15.56	1136	K?V	0.648	4391	unknown	3
Kepler-132	Lyra	18^h 52^m 56.6^s	+41° 20′ 35″		1140	F9	0.98	6003	unknown	4
Kepler-80	Cygnus	19^h 44^m 27.0^s	+39° 58′ 44″	14.804	1218	M0V^[129]	0.73	4250	unknown	6	Red dwarf star with six confirmed planets.^[130]^[131] Five of them are in anorbital resonance.^[132]^[131]
Kepler-159	Cygnus	19^h 48^m 16.8^s	+40° 52′ 08″		1219	K	0.63	4625	unknown	2 (1)	Star has a very low metallicity.
K2-299	Aquarius	22^h 05^m 06.5342^s	−14° 07′ 18.0135″	13.12	1220		unknown	5724±72	unknown	3
Kepler-88	Lyra	19^h 24^m 35.5431^s	+40° 40′ 09.8098″	13.5	1243	G8IV	1.022	5513±67	2.45	3
Kepler-174	Lyra	19^h 09^m 45.4^s	+43° 49:56′		1269	K	unknown	4880	unknown	3	Planet d may orbit in the habitable zone.
Kepler-83	Lyra	18^h 48^m 55.8^s	+43° 39′ 56″	16.51	1306	K7V	0.664	4164	unknown	3
TOI-1338	Pictor	06^h 08^m 31.97^s	+59° 32′ 28.1″	11.72	1318	F8 M	1.127	6160	4.4	2 (0)
Kepler-271	Lyra	18^h 52^m 00.7^s	+44° 17′ 03″		1319	G7V	0.9	5524	unknown	3	Metal-poor star
Kepler-169		19^h 03^m 60.0^s	+40° 55:10′	12.186	1326	K2V	0.86	4997	unknown	5
Kepler-451	Cygnus	19^h 38^m 32.61^s	46° 03′ 59.1″		1340	sdB M	0.6	29564	6	3	Three circumbinary planets orbit around the Kepler-451 binary pair.^[133]
Kepler-304	Cygnus	19^h 37^m 46.0^s	+40° 33′ 27″		1418	K	0.8	4731	unknown	4
Kepler-18	Cygnus	19^h 52^m 19.06^s	+44° 44′ 46.76″	13.549	1430	G7V	0.97	5345	10	3
Kepler-106	Cygnus	20^h 03^m 27.4^s	+44° 20′ 15″	12.882	1449	G1V	1	5858	4.83	4
Kepler-92	Lyra	19^h 16^m 21.0^s	+41° 33′ 47″	11.6	1463	G1IV	1.209	5871	5.52	3
Kepler-450	Cygnus	19^h 41^m 56.8^s	+51° 00′ 49″	11.684	1487	F	1.19	6152	unknown	3
Kepler-89	Cygnus	19^h 49^m 20.0^s	+41° 53′ 28″	12.4	1580	F8V	1.25	6116	3.9	4	FarthestF-type main sequence star from the Sun with a multiplanetary system. One study found hints of additional planets orbiting Kepler-89.^[134]
Kepler-1388	Lyra	18^h 53^m 20.6^s	+47° 10′ 28″		1604		0.63	4098	unknown	4 (1)	-
K2-282	Pisces	00^h 53^m 43.6833^s	07° 59′ 43.1397″	14.04	1638	G?V	0.94	5499±109	unknown	3
Kepler-107	Cygnus	19^h 48^m 06.8^s	+48° 12′ 31″	12.7	1714	G2V^[135]	1.238	5851	4.29	4	-
Kepler-176	Cygnus	19^h 38^m 40.3^s	+43° 51′ 12″		1746^[136]		unknown	5232	unknown	4
Kepler-1047	Cygnus	19^h 14^m 35.1^s	+50° 47′ 20″		1846	G2V	1.08	5754	unknown	3	-
Kepler-55	Lyra	19^h 00^m 40.0^s	+44° 01′ 35″	16.3	1888	K	0.62	4362	unknown	5	Planet c may orbit in the inner habitable zone.
Kepler-166	Cygnus	19^h 32^m 38.4^s	+48° 52′ 52″		1968	G	0.88	5413	unknown	3
Kepler-11	Cygnus	19^h 48^m 27.62^s	+41° 54′ 32.9″	13.69	2150±20	G6V^[137]	0.954	5681	7.834	6	Farthest star from the Sun with exactly six exoplanets. First system discovered with six transiting planets.^[137] The planets have low densities.^[138]
Kepler-1254	Draco	19^h 34^m 59.3^s	+45° 06′ 26″		2205		0.78	4985	unknown	3	-
Kepler-289	Cygnus	19^h 49^m 51.7^s	+42° 52′ 58″	12.9	2283	G0V	1.08	5990	0.65	3	-
Kepler-85	Cygnus	19^h 23^m 54.0^s	+45° 17′ 25″	15.0	2495	G	0.92	5666	unknown	4
Kepler-157	Lyra	19^h 24^m 23.3^s	+38° 52′ 32″		2523	G2V	1.02	5774	unknown	3
Kepler-342	Cygnus	19^h 24^m 23.3^s	+38° 52′ 32″		2549	F	1.13	6175	unknown	4
Kepler-148	Cygnus	19^h 19^m 08.7^s	+46° 51′ 32″		2580	K?V	0.83	5019.0±122.0	unknown	3
Kepler-51	Cygnus	19^h 45^m 55.0^s	+49° 56′ 16″	15.0	2610	G?V	1	5803	unknown	4	Super-puff planets with some of the lowest densities known.^[139]
Kepler-403	Cygnus	19^h 19^m 41.1^s	+46° 44′ 40″		2741	F9IV-V	1.25	6090	unknown	3
Kepler-9	Lyra	19^h 02^m 17.76^s	+38° 24′ 03.2″	13.91	2754	G2V	0.998	5722	3.008	3	First multiplanetary system to be discovered by the Kepler Space Telescope.^[140]^[141]
Kepler-23	Cygnus	19^h 36^m 52.0^s	+49° 28′ 45″	14	2790	G5V	1.11	5760	unknown	3	-
Kepler-46	Cygnus	19^h 17^m 05.0^s	+42° 36′ 15″	15.3	2795	K?V	0.902	5155	9.9	3	-
Kepler-305	Cygnus	19^h 56^m 53.83^s	+40° 20′ 35.46″	15.812	2833	K	0.85	4918	unknown	3 (1)
Kepler-90	Draco	18^h 57^m 44.0^s	+49° 18′ 19″	14.0	2840 ± 40	F9 IV/V	1.13	5930	2	8	All eight exoplanets are larger than Earth and are within 1.1 AU of the parent star. Only star apart from the Sun with at least eight planets.^[142] AHill stability test shows that the system is stable.^[143] Planet h orbits in the habitable zone.
Kepler-150	Lyra	19^h 12^m 56.2^s	+40° 31′ 15″		2906	G?V	0.97	5560	unknown	5	Planet f orbits in the habitable zone.
Kepler-82	Cygnus	19^h 31^m 29.61^s	+42° 57′ 58.09″	15.158	2949	G?V	0.91	5512	unknown	5
Kepler-154	Cygnus	19^h 19^m 07.3^s	+49° 53′ 48″		2985	G3V	0.98	5690	unknown	5
Kepler-56	Cygnus	19^h 35^m 02.0^s	+41° 52′ 19″	13	3060	K?III	1.32	4840	3.5	3
Kepler-350	Lyra	19^h 01^m 41.0^s	+39° 42′ 22″	13.8	3121	F	1.03	6215	unknown	3
Kepler-603	Cygnus	19^h 37^m 07.4^s	+42° 17′ 27″		3134	G2V	1.01	5808	unknown	3	-
Kepler-160	Lyra	19^h 11^m 05.65^s	+42° 52′ 09.5″	13.101	3140	G2V	unknown	5470	unknown	3 (1)	The unconfirmed planet Kepler-160e (or KOI-456.04) is a potentially habitable planet.^[144]
Kepler-401	Cygnus	19^h 20^m 19.9^s	+50° 51′ 49″		3149	F8V	1.17	6117	unknown	3
Kepler-58	Cygnus	19^h 45^m 26.0^s	+39° 06′ 55″	15.3	3161	G1V	1.04	5843	unknown	3
Kepler-79	Cygnus	20^h 02^m 04.11^s	+44° 22′ 53.69″	13.914	3329	F	1.17	6187	unknown	4
Kepler-60	Cygnus	19^h 15^m 50.70^s	+42° 15′ 54.04″	13.959	3343	G	1.04	5915	unknown	3
Kepler-122		19^h 24^m 26.9^s	+39° 56′ 57″		3351	F	1.08	6050	unknown	5
Kepler-279	Lyra	19^h 09^m 34.0^s	+42° 11′ 42″	13.7	3383	F	1.1	6562	unknown	3
Kepler-255	Cygnus	19^h 44^m 15.4^s	+45° 58′ 37″		3433	G6V	0.9	5573	unknown	3
Kepler-47	Cygnus	19^h 41^m 11.5^s	+46° 55′ 13.69″	15.178	3442	G M	1.043	5636(A) (B is unknown)	4.5	3	Circumbinary planets, with one of the planets orbiting in the habitable zone.^[145]^[146]^[147]
Kepler-292		19^h 43^m 03.84^s	+43° 25′ 27.4″	13.97	3446	K0V	0.85	5299	unknown	5
Kepler-27	Cygnus	19^h 28^m 56.82^s	+41° 05′ 9.15″	15.855	3500	G5V	0.65	5400	unknown	3
Kepler-351	Lyra	19^h 05^m 48.6^s	+42° 39′ 28″		3535	G?V	0.89	5643	unknown	3
Kepler-276	Cygnus	19^h 34^m 16^s	+39° 02′ 11″	15.368	3734	G?V	1.1	5812	unknown	3
Kepler-24	Lyra	19^h 21^m 39.18^s	+38° 20′ 37.51″	14.925	3910	G1V	1.03	5800	unknown	4	-
Kepler-87	Cygnus	19^h 51^m 40.0^s	+46° 57′ 54″	15	4021	G4IV	1.1	5600	7.5	2 (2)	Farthest system from the Sun with an unconfirmed exoplanet candidate.
Kepler-33	Lyra	19^h 16^m 18.61^s	+46° 00′ 18.8″	13.988	4090	G1IV	1.164	5849	4.27	5
Kepler-282	Lyra	18^h 58^m 43.0^s	+44° 47′ 51″	15.2	4363	G?V	0.97	5876	unknown	4
Kepler-758	Cygnus	19^h 32^m 20.3^s	+41° 08′ 08″		4413		1.16	6228	unknown	4	Farthest system from the Sun with exactly four confirmed exoplanets.
Kepler-53	Lyra	19^h 21^m 51.0^s	+40° 33′ 45″	16	4455	G?V	0.98	5858	unknown	3
Kepler-30	Lyra	19^h 01^m 08.07^s	+38° 56′ 50.21″	15.403	4560	G6V	0.99	5498	unknown	3
Kepler-84	Cygnus	19^h 53^m 00.49^s	+40° 29′ 45.87″	14.764	4700	G3IV	1	5755	unknown	5
Kepler-385	Cygnus	19^h 37^m 21.23^s	+50° 20′ 11.55″	15.76	4900	F8V	0.99	5835	unknown	3 (4)
Kepler-31	Cygnus	19^h 36^m 06.0^s	+45° 51′ 11″	15.5	5429	F	1.21	6340	unknown	3	The three planets are in an orbital resonance.^[148]
Kepler-32	Cygnus	19^h 51^m 22.2^s	+46° 34′ 27″			M1V	0.58	3900	unknown	5	Planet f is smaller than Earth.
Kepler-238	Lyra	19^h 11^m 35^s	+40° 38′ 16″	15.084	5867	G5IV	1.06	5614	unknown	5	One of the farthest systems from the Sun with a multiplanetary system, and the farthest system where exoplanets were discovered by theKepler space telescope.
Kepler-245	Cygnus	19^h 26^m 33.4^s	+42° 26′ 11″				0.8	5100	unknown	4
Kepler-218	Cygnus	19^h 41^m 39.1^s	+46° 15′ 59″				unknown	5502	unknown	3
Kepler-217	Cygnus	19^h 32^m 09.1^s	+46° 16′ 39″				unknown	6171	unknown	3
Kepler-192	Lyra	19^h 11^m 40.3^s	+45° 35′ 34″				unknown	5479	unknown	3
Kepler-191	Cygnus	19^h 24^m 44.0^s	+45° 19′ 23″				0.85	5282	unknown	3
Kepler-431	Lyra	18^h 44^m 26.9^s	+43° 13′ 40″				1.071	6004	unknown	3
Kepler-338	Lyra	18^h 51^m 54.9^s	+40° 47′ 04″				1.1	5923	unknown	4
Kepler-197	Cygnus	19^h 40^m 54.3^s	+50° 33′ 32″				unknown	6004	unknown	4
Kepler-247	Lyra	19^h 14^m 34.2^s	+43° 02′ 21″				0.884	5094	unknown	3
Kepler-104	Lyra	19^h 10^m 25.1^s	+42° 10′ 00″				0.81	5711	unknown	3	-
Kepler-126	Cygnus	19^h 17^m 23.4^s	+44° 12′ 31″				unknown	6239	unknown	3	-
Kepler-127	Lyra	19^h 00^m 45.6^s	+46° 01′ 41″				unknown	6106	unknown	3	-
Kepler-130	Lyra	19^h 13^m 48.2^s	+40° 14′ 43″				1	5884	unknown	3	-
Kepler-164	Lyra	19^h 11^m 07.4^s	+47° 37′ 48″				1.11	5888	unknown	3	-
Kepler-171	Cygnus	19^h 47^m 05.3^s	+41° 45′ 20″				unknown	5642	unknown	3	-
Kepler-172	Lyra	19^h 47^m 05.3^s	+41° 45′ 20″				0.86	5526	unknown	4	-
Kepler-149	Lyra	19^h 03^m 24.9^s	+38° 23′ 03″				unknown	5381	unknown	3
Kepler-142	Cygnus	19^h 40^m 28.5^s	+48° 28′ 53″				0.99	5790	unknown	3
Kepler-124	Draco	19^h 07^m 00.7^s	+49° 03′ 54″				unknown	4984	unknown	3
Kepler-402	Lyra	19^h 13^m 28.9^s	+43° 21′ 17″				unknown	6090	unknown	4 (1)
Kepler-399	Cygnus	19^h 58^m 00.4^s	+40° 40′ 15″				unknown	5502	unknown	3
Kepler-374	Cygnus	19^h 36^m 33.1^s	+42° 22′ 14″				0.84	5977	unknown	3
Kepler-372	Cygnus	19^h 25^m 01.5^s	+49° 15′ 32″				1.15	6509	unknown	3
Kepler-363	Lyra	18^h 52^m 46.1^s	+41° 18′ 19″				1.23	5593	unknown	3
Kepler-359	Cygnus	19^h 33^m 10.5^s	+42° 11′ 47″				1.07	6248	unknown	3
Kepler-357	Cygnus	19^h 24^m 58.3^s	+44° 00′ 31″				0.78	5036	unknown	3
Kepler-354	Lyra	19^h 03^m 00.4^s	+41° 20′ 08″				0.65	4648	unknown	3
Kepler-206	Lyra	19^h 26^m 32.3^s	+41° 50′ 02″				0.94	5764	unknown	3
Kepler-203	Cygnus	19^h 01^m 23.3^s	+41° 45′ 43″				0.98	5821	unknown	3
Kepler-194	Cygnus	19^h 27^m 53.1^s	+47° 51′ 51″				unknown	6089	unknown	3
Kepler-184	Lyra	19^h 27^m 48.5^s	+43° 04′ 29″				unknown	5788	unknown	3
Kepler-178	Lyra	19^h 08^m 24.3^s	+46° 53′ 47″				unknown	5676	unknown	3
Kepler-336	Lyra	19^h 20^m 57.0^s	+41° 19′ 53″				0.89	5867	unknown	3
Kepler-334	Lyra	19^h 08^m 33.8^s	+47° 06′ 55″				1	5828	unknown	3
Kepler-332	Lyra	19^h 06^m 39.1^s	+47° 24′ 49″				0.8	4955	unknown	3
Kepler-331	Lyra	19^h 27^m 20.2^s	+39° 18′ 26″				0.51	4347	unknown	3
Kepler-327	Cygnus	19^h 30^m 34.2^s	44° 05′ 16″				0.55	3799	unknown	3
Kepler-326	Cygnus	19^h 37^m 18.1^s	+46° 00′ 08″				0.98	5105	unknown	3
Kepler-325	Cygnus	19^h 19^m 20.5^s	+49° 49′ 32″				0.87	5752	unknown	3

Stars orbited by both planets and brown dwarfs

[edit]

These are stars orbited by objects on both sides of the ~13Jupiter mass dividing line.

Notes

[edit]

References

[edit]

^Schneider, Jean (6 December 2016)."Interactive Extra-solar Planets Catalog".Extrasolar Planets Encyclopaedia.Archived from the original on 2016-12-09. Retrieved2016-12-06.
^Artigau, Étienne; Cadieux, Charles; Cook, Neil J.; Doyon, René; Vandal, Thomas; et al. (June 23, 2022)."Line-by-line velocity measurements, an outlier-resistant method for precision velocimetry".The Astronomical Journal. 164:84 (3) (published August 8, 2022): 18pp.arXiv:2207.13524.Bibcode:2022AJ....164...84A.doi:10.3847/1538-3881/ac7ce6.
^^a ^bBasant, Ritvik; Luque, Rafael; et al. (March 2025)."Four Sub-Earth Planets Orbiting Barnard's Star from MAROON-X and ESPRESSO".The Astrophysical Journal Letters.982 (1): L1.arXiv:2503.08095.Bibcode:2025ApJ...982L...1B.doi:10.3847/2041-8213/adb8d5.
^Beaulieu, Jean-Philippe; Bennett, D. P.; Batista, Virginie; Fukui, A. (January 2016)."Revisiting the microlensing event OGLE 2012-BLG-0026: A solar mass star with two cold giant planets".researchgate.net.
^Brewer, John M.; Wang, Songhu; Fischer, Debra A.; Foreman-Mackey, Daniel (2018-10-24)."Compact multi-planet systems are more common around metal poor hosts".The Astrophysical Journal.867 (1). L3.arXiv:1810.10009.Bibcode:2018ApJ...867L...3B.doi:10.3847/2041-8213/aae710.S2CID 67832557.
^Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR online data catalog: General catalogue of variable stars (Samus+ 2007–2013)".VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S.1.Bibcode:2009yCat....102025S.
^Bessell, M. S. (1991)."The late-M dwarfs".The Astronomical Journal.101: 662.Bibcode:1991AJ....101..662B.doi:10.1086/115714.
^Mascareño, A. Suárez; Faria, J. P.; Figueira, P.; Lovis, C.; Damasso, M.; Hernández, J. I. González; Rebolo, R.; Cristiani, S.; Pepe, F.; Santos, N. C.; Osorio, M. R. Zapatero; Adibekyan, V.; Hojjatpanah, S.; Sozzetti, A.; Murgas, F.; Abreu, M.; Affolter, M.; Alibert, Y.; Aliverti, M.; Allart, R.; Prieto, C. Allende; Alves, D.; Amate, M.; Avila, G.; Baldini, V.; Bandi, T.; Barros, S. C. C.; Bianco, A.; Benz, W.; Bouchy, F.; Broeng, C.; Cabral, A.; Calderone, G.; Cirami, R.; Coelho, J.; Conconi, P.; Coretti, I.; Cumani, C.; Cupani, G.; D’Odorico, V.; Deiries, S.; Delabre, B.; Marcantonio, P. Di; Dumusque, X.; Ehrenreich, D.; Fragoso, A.; Genolet, L.; Genoni, M.; Santos, R. Génova; Hughes, I.; Iwert, O.; Kerber, F.; Knusdstrup, J.; Landoni, M.; Lavie, B.; Lillo-Box, J.; Lizon, J.; Curto, G. Lo; Maire, C.; Manescau, A.; Martins, C. J. a. P.; Mégevand, D.; Mehner, A.; Micela, G.; Modigliani, A.; Molaro, P.; Monteiro, M. A.; Monteiro, M. J. P. F. G.; Moschetti, M.; Mueller, E.; Nunes, N. J.; Oggioni, L.; Oliveira, A.; Pallé, E.; Pariani, G.; Pasquini, L.; Poretti, E.; Rasilla, J. L.; Redaelli, E.; Riva, M.; Tschudi, S. Santana; Santin, P.; Santos, P.; Segovia, A.; Sosnowska, D.; Sousa, S.; Spanò, P.; Tenegi, F.; Udry, S.; Zanutta, A.; Zerbi, F. (1 July 2020)."Revisiting Proxima with ESPRESSO".Astronomy & Astrophysics.639: A77.arXiv:2005.12114.Bibcode:2020A&A...639A..77S.doi:10.1051/0004-6361/202037745.ISSN 0004-6361.S2CID 218869742.Archived from the original on 27 June 2022. Retrieved9 May 2022.
^Del Genio, Anthony D.; Way, Michael J.; Amundsen, David S.; Aleinov, Igor; Kelley, Maxwell; Kiang, Nancy Y.; Clune, Thomas L. (January 2019)."Habitable Climate Scenarios for Proxima Centauri b with a Dynamic Ocean".Astrobiology.19 (1):99–125.arXiv:1709.02051.Bibcode:2019AsBio..19...99D.doi:10.1089/ast.2017.1760.ISSN 1531-1074.PMID 30183335.S2CID 52165056.
^Gizis, John E. (February 1997). "M-Subdwarfs: Spectroscopic Classification and the Metallicity Scale".The Astronomical Journal.113 (2):806–822.arXiv:astro-ph/9611222.Bibcode:1997AJ....113..806G.doi:10.1086/118302.S2CID 16863021.
^Oja, T. (August 1985), "Photoelectric photometry of stars near the north Galactic pole. II",Astronomy and Astrophysics Supplement Series,61:331–339,Bibcode:1985A&AS...61..331O
^Dickinson, David (2015-12-23)."14 Red Dwarf Stars to View with Backyard Telescopes". Universe Today.Archived from the original on 2021-02-11. Retrieved2016-12-04.
^Croswell, Ken (July 2002)."The Brightest Red Dwarf".KenCroswell.com.Archived from the original on 2018-10-20. Retrieved2016-12-04.
^Jeffers, S. V.; Dreizler, S.; Barnes, J. R.; Haswell, C. A.; Nelson, R. P.; Rodríguez, E.; López-González, M. J.; Morales, N.; Luque, R.; et al. (2020), "A multiple planet system of super-Earths orbiting the brightest red dwarf star GJ887",Science,368 (6498):1477–1481,arXiv:2006.16372,Bibcode:2020Sci...368.1477J,doi:10.1126/science.aaz0795,PMID 32587019,S2CID 220075207
^Pozuelos, Francisco J.; Suárez, Juan C.; de Elía, Gonzalo C.; Berdiñas, Zaira M.; Bonfanti, Andrea; Dugaro, Agustín; et al. (2020). "GJ 273: On the formation, dynamical evolution, and habitability of a planetary system hosted by an M dwarf at 3.75 parsec".Astronomy & Astrophysics.641: A23.arXiv:2006.09403.Bibcode:2020A&A...641A..23P.doi:10.1051/0004-6361/202038047.S2CID 219721292.GJ 273 is a planetary system orbiting an M dwarf only 3.75 pc away, composed of two confirmed planets, GJ 273b and GJ 273c, and two promising candidates, GJ 273d and GJ 273e ... the system remained stable only for values of inclinations ranging from 90◦ to ~72◦
^^a ^bAstudillo-Defru, Nicola; Forveille, Thierry; Bonfils, Xavier; Ségransan, Damien; Bouchy, François; Delfosse, Xavier; et al. (2017)."The HARPS search for southern extra-solar planets. XLI. A dozen planets around the M dwarfs GJ 3138, GJ 3323, GJ 273, GJ 628, and GJ 3293".Astronomy and Astrophysics.602. A88.arXiv:1703.05386.Bibcode:2017A&A...602A..88A.doi:10.1051/0004-6361/201630153.S2CID 119418595.Archived from the original on 2022-09-28. Retrieved2022-02-25.
^Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)".VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S.1.Bibcode:2009yCat....102025S.
^Dreizler, S.; Jeffers, S. V.; Rodríguez, E.; Zechmeister, M.; Barnes, J.R.; Haswell, C.A.; Coleman, G. A. L.; Lalitha, S.; Hidalgo Soto, D.; Strachan, J.B.P.; Hambsch, F-J.; López-González, M. J.; Morales, N.; Rodríguez López, C.; Berdiñas, Z. M.; Ribas, I.; Pallé, E.; Reiners, Ansgar; Anglada-Escudé, G. (2019-08-13)."Red Dots: A temperate 1.5 Earth-mass planet in a compact multi-terrestrial planet system around GJ1061".Monthly Notices of the Royal Astronomical Society.493 (1):536–550.arXiv:1908.04717.doi:10.1093/mnras/staa248.S2CID 199551874.
^Caballero, J. A.; Reiners, Ansgar; 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".Astronomy & Astrophysics.627: A49.arXiv:1906.07196.Bibcode:2019A&A...627A..49Z.doi:10.1051/0004-6361/201935460.ISSN 0004-6361.S2CID 189999121.
^Davison, Cassy L.; White, Russel J.; Henry, Todd J.; Riedel, Adric R.; Jao, Wei-Chun; Bailey III, John I.; Quinn, Samuel N.; Justin R., Cantrell; John P., Subasavage; Jen G., Winters (2015). "A 3D Search for Companions to 12 Nearby M-Dwarfs".The Astronomical Journal.149 (3): 106.arXiv:1501.05012.Bibcode:2015AJ....149..106D.doi:10.1088/0004-6256/149/3/106.S2CID 9719725.
^Stuart Gary (17 December 2015)."Potentially habitable super-Earth discovered orbiting star 14 light years from Earth". ABC News (Australia).Archived from the original on 2017-06-09. Retrieved2022-05-10.
^Kane, Stephen R.; et al. (February 2017), "Characterization of the Wolf 1061 Planetary System",The Astrophysical Journal,835 (2): 9,arXiv:1612.09324,Bibcode:2017ApJ...835..200K,doi:10.3847/1538-4357/835/2/200,S2CID 30738573, 200.
^Jones, Barrie W.; et al. (2005)."Prospects for Habitable "Earths" in Known Exoplanetary Systems".The Astrophysical Journal.622 (2):1091–1101.arXiv:astro-ph/0503178.Bibcode:2005ApJ...622.1091J.doi:10.1086/428108.
^Wyatt, M. C.; et al. (2012)."Herschel imaging of 61 Vir: implications for the prevalence of debris in low-mass planetary systems".Monthly Notices of the Royal Astronomical Society.424 (2): 1206.arXiv:1206.2370.Bibcode:2012MNRAS.424.1206W.doi:10.1111/j.1365-2966.2012.21298.x.S2CID 54056835.
^Kennedy, G. M.; Matra, L.; Marmier, M.; Greaves, J. S.; Wyatt, M. C.; Bryden, G.; Holland, W.; Lovis, C.; Matthews, B. C.; Pepe, F.; Sibthorpe, B.; Udry, S. (2015)."Kuiper belt structure around nearby super-Earth host stars".Monthly Notices of the Royal Astronomical Society.449 (3): 3121.arXiv:1503.02073.Bibcode:2015MNRAS.449.3121K.doi:10.1093/mnras/stv511.S2CID 53638901.
^"Reanalysis of data suggests 'habitable' planet GJ 581d really could exist".Astronomy Now. 9 March 2015.Archived from the original on 20 May 2015. Retrieved27 May 2015.
^Anglada-Escudé, Guillem; Arriagada, Pamela; Vogt, Steven S.; Rivera, Eugenio J.; Butler, R. Paul; Crane, Jeffrey D.; Shectman, Stephen A.; Thompson, Ian B.; Minniti, Dante; Haghighipour, Nader; Carter, Brad D.; Tinney, C. G.; Wittenmyer, Robert A.; Bailey, Jeremy A.; O'Toole, Simon J.; Jones, Hugh R. A.; Jenkins, James S. (2012). "A Planetary System around the nearby M Dwarf GJ 667C with At Least One Super-Earth in Its Habitable Zone".The Astrophysical Journal Letters.751 (1). L16.arXiv:1202.0446.Bibcode:2012ApJ...751L..16A.doi:10.1088/2041-8205/751/1/L16.S2CID 16531923.
^Anglada-Escudé, Guillem; et al. (2013-06-07)."A dynamically-packed planetary system around GJ 667C with three super-Earths in its habitable zone"(PDF).Astronomy & Astrophysics.556: A126.arXiv:1306.6074.Bibcode:2013A&A...556A.126A.doi:10.1051/0004-6361/201321331.S2CID 14559800. Archived fromthe original(PDF) on 2013-06-30. Retrieved2013-06-25.
^Makarov, Valeri V.; Berghea, Ciprian (2013). "Dynamical Evolution and Spin-Orbit Resonances of Potentially Habitable Exoplanets. The Case of Gj 667C".The Astrophysical Journal.780 (2): 124.arXiv:1311.4831.doi:10.1088/0004-637X/780/2/124.S2CID 118700510.
^Vogt, Steven S.; et al. (November 2015). "Six Planets Orbiting HD 219134".The Astrophysical Journal.814 (1): 12.arXiv:1509.07912.Bibcode:2015ApJ...814...12V.doi:10.1088/0004-637X/814/1/12.S2CID 45438051.
^Dietrich, Jeremy; Apai, Dániel; Malhotra, Renu (2022)."An Integrative Analysis of the HD 219134 Planetary System and the Inner solar system: Extending DYNAMITE with Enhanced Orbital Dynamical Stability Criteria".The Astronomical Journal.163 (2): 88.arXiv:2112.05337.Bibcode:2022AJ....163...88D.doi:10.3847/1538-3881/ac4166.S2CID 245117944.
^Wyatt, M. C.; et al. (2012)."Herschel imaging of 61 Vir: implications for the prevalence of debris in low-mass planetary systems".MNRAS.424 (2):1206–1223.arXiv:1206.2370.Bibcode:2012MNRAS.424.1206W.doi:10.1111/j.1365-2966.2012.21298.x.S2CID 54056835.
^^a ^bRosenthal, Lee J.; Fulton, Benjamin J.; Hirsch, Lea A.; Isaacson, Howard T.; Howard, Andrew W.; Dedrick, Cayla M.; Sherstyuk, Ilya A.; Blunt, Sarah C.; Petigura, Erik A.; Knutson, Heather A.; Behmard, Aida; Chontos, Ashley; Crepp, Justin R.; Crossfield, Ian J. M.; Dalba, Paul A.; Fischer, Debra A.; Henry, Gregory W.; Kane, Stephen R.; Kosiarek, Molly; Marcy, Geoffrey W.; Rubenzahl, Ryan A.; Weiss, Lauren M.; Wright, Jason T. (2021)."The California Legacy Survey. I. A Catalog of 178 Planets from Precision Radial Velocity Monitoring of 719 Nearby Stars over Three Decades".The Astrophysical Journal Supplement Series.255 (1): 8.arXiv:2105.11583.Bibcode:2021ApJS..255....8R.doi:10.3847/1538-4365/abe23c.S2CID 235186973.
^Kennedy, G. M.; et al. (June 2018)."Kuiper belt analogues in nearby M-type planet-host systems".Monthly Notices of the Royal Astronomical Society.476 (4):4584–4591.arXiv:1803.02832.Bibcode:2018MNRAS.476.4584K.doi:10.1093/mnras/sty492.
^Falconer, Rebecca,Newly uncovered super-Earth 31 light-years away may be habitable Archived 2019-12-18 at theWayback Machine, Axios, August 1, 2019
^Reddy, Francis; Center, NASA’s Goddard Space Flight (2019-07-31)."TESS Discovers Habitable Zone Planet in GJ 357 System".SciTechDaily.Archived from the original on 2019-08-01. Retrieved2019-08-01.
^"Potentially habitable 'super-Earth' discovered just 31 light-years away".NBC News. 31 July 2019.Archived from the original on 2019-07-31. Retrieved2019-08-01.
^Garner, Rob (2019-07-30)."NASA's TESS Helps Find Intriguing New World".NASA.Archived from the original on 2019-08-01. Retrieved2019-08-01.
^Demangeon, Oliver D. S.; Zapatero Osorio, M. R.; Alibert, Y.; Barros, S. C. C.; Adibekyan, V.; Tabernero, H. M.; et al. (July 2021)."A warm terrestrial planet with half the mass of Venus transiting a nearby star"(PDF).Astronomy & Astrophysics.653: 38.arXiv:2108.03323.Bibcode:2021A&A...653A..41D.doi:10.1051/0004-6361/202140728.S2CID 236957385.Archived(PDF) from the original on 2021-11-13. Retrieved2022-03-03.
^Dedrick, Cayla M.; Fulton, Benjamin J.; Knutson, Heather A.; Howard, Andrew W.; Beatty, Thomas G.; Cargile, Phillip A.; Gaudi, B. Scott; Hirsch, Lea A.; Kuhn, Rudolf B.; Lund, Michael B.; James, David J.; Kosiarek, Molly R.; Pepper, Joshua; Petigura, Erik A.; Rodriguez, Joseph E. (January 2021)."Two Planets Straddling the Habitable Zone of the Nearby K Dwarf Gl 414A".The Astronomical Journal.161 (2): 86.arXiv:2009.06503.Bibcode:2021AJ....161...86D.doi:10.3847/1538-3881/abd0ef.ISSN 1538-3881.
^"GJ 414 Overview".NASA Exoplanet Archive.Archived from the original on December 9, 2023. RetrievedJanuary 4, 2024.
^Schweitzer, A.; et al. (May 2019). "The CARMENES search for exoplanets around M dwarfs. Different roads to radii and masses of the target stars".Astronomy & Astrophysics.625: 16.arXiv:1904.03231.Bibcode:2019A&A...625A..68S.doi:10.1051/0004-6361/201834965.S2CID 102351979. A68.
^Stephenson, C. B. (July 1986), "Dwarf K and M stars of high proper motion found in a hemispheric survey",The Astronomical Journal,92:139–165,Bibcode:1986AJ.....92..139S,doi:10.1086/114146.
^Sutherland, Paul (March 5, 2014)."Habitable planets common around red dwarf stars".Sen. Sen Corporation Ltd.Archived from the original on November 12, 2020. RetrievedJuly 28, 2022.
^Tuomi, Mikko; et al. (2014), "Bayesian search for low-mass planets around nearby M dwarfs – estimates for occurrence rate based on global detectability statistics",Monthly Notices of the Royal Astronomical Society,441 (2):1545–1569,arXiv:1403.0430,Bibcode:2014MNRAS.441.1545T,doi:10.1093/mnras/stu358,S2CID 32965505.
^Lovis, Christophe; et al. (2006)."An extrasolar planetary system with three Neptune-mass planets"(PDF).Nature.441 (7091):305–309.arXiv:astro-ph/0703024.Bibcode:2006Natur.441..305L.doi:10.1038/nature04828.PMID 16710412.S2CID 4343578. Archived fromthe original(PDF) on 2016-03-03. Retrieved2022-02-24.
^Díaz, R. F.; et al. (2016)."The HARPS search for southern extra-solar planets. XXXVIII. Bayesian re-analysis of three systems. New super-Earths, unconfirmed signals, and magnetic cycles".Astronomy and Astrophysics.585. A134.arXiv:1510.06446.Bibcode:2016A&A...585A.134D.doi:10.1051/0004-6361/201526729.S2CID 118531921.Archived from the original on 2021-02-24. Retrieved2022-02-24.
^Tuomi, Mikko; Anglada-Escudé, Guillem; Gerlach, Enrico; Jones, Hugh R. A.; Reiners, Ansgar; Rivera, Eugenio J.; Vogt, Steven S.; Butler, R. Paul (17 December 2012). "Habitable-zone super-Earth candidate in a six-planet system around the K2.5V star HD 40307".Astronomy & Astrophysics.549: A48.arXiv:1211.1617.Bibcode:2013A&A...549A..48T.doi:10.1051/0004-6361/201220268.S2CID 7424216.
^R. P. Butler; Marcy, Geoffrey W. (1996)."A Planet Orbiting 47 Ursae Majoris".Astrophysical Journal Letters.464 (2):L153 –L156.Bibcode:1996ApJ...464L.153B.doi:10.1086/310102.
^P. C. Gregory; D. A. Fischer (2010)."A Bayesian periodogram finds evidence for three planets in 47 Ursae Majoris".Monthly Notices of the Royal Astronomical Society.403 (2):731–747.arXiv:1003.5549.Bibcode:2010MNRAS.403..731G.doi:10.1111/j.1365-2966.2009.16233.x.S2CID 16722873.
^Takeda, Genya; et al. (2007). "Structure and Evolution of Nearby Stars with Planets. II. Physical Properties of ~1000 Cool Stars from the SPOCS Catalog".The Astrophysical Journal Supplement Series.168 (2):297–318.arXiv:astro-ph/0607235.Bibcode:2007ApJS..168..297T.doi:10.1086/509763.S2CID 18775378.
^Sousa, S. G.; et al. (August 2008). "Spectroscopic parameters for 451 stars in the HARPS GTO planet search program. Stellar [Fe/H] and the frequency of exo-Neptunes".Astronomy and Astrophysics.487 (1):373–381.arXiv:0805.4826.Bibcode:2008A&A...487..373S.doi:10.1051/0004-6361:200809698.S2CID 18173201.
^Lovis, C.; et al. (2011). "The HARPS search for southern extra-solar planets. XXXI. Magnetic activity cycles in solar-type stars: statistics and impact on precise radial velocities".arXiv:1107.5325 [astro-ph.SR].
^Dittmann, Jason A.; Irwin, Jonathan M.; Charbonneau, David; Bonfils, Xavier; Astudillo-Defru, Nicola; Haywood, Raphaëlle D.; et al. (2017). "A temperate rocky super-Earth transiting a nearby cool star".Nature.544 (7650):333–336.arXiv:1704.05556.Bibcode:2017Natur.544..333D.doi:10.1038/nature22055.PMID 28426003.S2CID 2718408.
^Overbye, Dennis (19 April 2017)."A new exoplanet may be most promising yet in search for life".New York Times.Archived from the original on 11 November 2020. Retrieved20 April 2017.
^Méndez, Abel (August 29, 2012)."A Hot Potential Habitable Exoplanet around Gliese 163".University of Puerto Rico at Arecibo (Planetary Habitability Laboratory). Archived fromthe original on October 21, 2019. RetrievedSeptember 20, 2012.
^Redd, Nola Taylor (September 20, 2012)."Newfound Alien Planet a Top Contender to Host Life".Space.com.Archived from the original on December 26, 2019. RetrievedSeptember 20, 2012.
^"Simbad - Object view".simbad.cds.unistra.fr. Retrieved2024-01-04.
^Beard, Corey; Robertson, Paul; Kanodia, Shubham; Lubin, Jack; Cañas, Caleb I.; Gupta, Arvind F.; Holcomb, Rae; Jones, Sinclaire; Libby-Roberts, Jessica E.; Lin, Andrea S. J.; Mahadevan, Suvrath; Stefánsson, Guđmundur; Bender, Chad F.; Blake, Cullen H.; Cochran, William D. (2022-08-30)."GJ 3929: High-precision Photometric and Doppler Characterization of an Exo-Venus and Its Hot, Mini-Neptune-mass Companion".The Astrophysical Journal.936 (1): 55.arXiv:2207.10672.Bibcode:2022ApJ...936...55B.doi:10.3847/1538-4357/ac8480.ISSN 0004-637X.
^Anglada-Escudé, Guillem; Tuomi, Mikko (2012)."A planetary system with gas giants and super-Earths around the nearby M dwarf GJ 676A. Optimizing data analysis techniques for the detection of multi-planetary systems"(PDF).Astronomy.548: A58.arXiv:1206.7118.Bibcode:2012A&A...548A..58A.doi:10.1051/0004-6361/201219910.S2CID 17115882.^{[permanent dead link]}
^Fulton, Benjamin J.; et al. (2015). "Three Super-Earths Orbiting HD 7924".The Astrophysical Journal.805 (2): 175.arXiv:1504.06629.Bibcode:2015ApJ...805..175F.doi:10.1088/0004-637X/805/2/175.S2CID 7969255.
^Damasso, M.; et al. (2020), "A precise architecture characterization of the π Mensae planetary system",Astronomy & Astrophysics,642: A31,arXiv:2007.06410,Bibcode:2020A&A...642A..31D,doi:10.1051/0004-6361/202038416,S2CID 220496034
^"Planet LHS 1678 D". 2024.
^Kane, Stephen R.; Fetherolf, Tara; et al. (March 2024)."A Perfect Tidal Storm: HD 104067 Planetary Architecture Creating an Incandescent World".The Astronomical Journal.167 (5): 239.arXiv:2403.17062.Bibcode:2024AJ....167..239K.doi:10.3847/1538-3881/ad3820.
^Koerner, D. W.; et al. (February 2010),"New Debris Disk Candidates Around 49 Nearby Stars"(PDF),The Astrophysical Journal Letters,710 (1):L26 –L29,Bibcode:2010ApJ...710L..26K,doi:10.1088/2041-8205/710/1/L26,S2CID 122844702,archived(PDF) from the original on 2020-09-15, retrieved2022-02-25.
^^a ^bFulton, Benjamin J.; Howard, Andrew W.; Weiss, Lauren M.; Sinukoff, Evan; Petigura, Erik A.; Isaacson, Howard; Hirsch, Lea; Marcy, Geoffrey W.; Henry, Gregory W.; Grunblatt, Samuel K.; Huber, Daniel; Kaspar von Braun; Boyajian, Tabetha S.; Kane, Stephen R.; Wittrock, Justin; Horch, Elliott P.; Ciardi, David R.; Howell, Steve B.; Wright, Jason T.; Ford, Eric B. (2016)."Three Temperate Neptunes Orbiting Nearby Stars".The Astrophysical Journal.830 (1): 46.arXiv:1607.00007.Bibcode:2016ApJ...830...46F.doi:10.3847/0004-637X/830/1/46.S2CID 36666883.
^Unger, N.; et al. (October 2021)."The HARPS search for southern extra-solar planets".Astronomy & Astrophysics.654: A104.arXiv:2108.10198.Bibcode:2021A&A...654A.104U.doi:10.1051/0004-6361/202141351.eISSN 1432-0746.ISSN 0004-6361.
^Mayor, M.; Marmier, M.; Lovis, C.; Udry, S.; Ségransan, D.; Pepe, F.; Benz, W.; Bertaux, J.-L.; Bouchy, F.; Dumusque, X.; Lo Curto, G.; Mordasini, C.; Queloz, D.; Santos, N. C. (September 13, 2011),The HARPS search for southern extra-solar planets XXXIV. Occurrence, mass distribution and orbital properties of super-Earths and Neptune-mass planets,arXiv:1109.2497
^^a ^bHara, N. C.; Bouchy, F.; Stalport, M.; Boisse, I.; Rodrigues, J.; Delisle, J. B.; Santerne, A.; Henry, G. W.; Arnold, L.; Astudillo-Defru, N.; Borgniet, S.; Bonfils, X.; Bourrier, V.; Brugger, B.; Courcol, B.; Dalal, S.; Deleuil, M.; Delfosse, X.; Demangeon, O.; Díaz, R. F.; Dumusque, X.; Forveille, T.; Hébrard, G.; Hobson, M. J.; Kiefer, F.; Lopez, T.; Mignon, L.; Mousis, O.; Moutou, C.; Pepe, F.; Rey, J.; Santos, N. C.; Ségransan, D.; Udry, S.; Wilson, P. A. (March 10, 2020). "The SOPHIE search for northern extrasolar planets XVI. HD 158259: A compact planetary system in a near-3:2 mean motion resonance chain".Astronomy & Astrophysics.636 (1): L6.arXiv:1911.13296.Bibcode:2020A&A...636L...6H.doi:10.1051/0004-6361/201937254.S2CID 208512859.
^Gray, R. O.; et al. (July 2006), "Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample",The Astronomical Journal,132 (1):161–170,arXiv:astro-ph/0603770,Bibcode:2006AJ....132..161G,doi:10.1086/504637,S2CID 119476992
^Lee, Man Hoi; et al. (2006). "On the 2:1 Orbital Resonance in the HD 82943 Planetary System".The Astrophysical Journal.641 (2):1178–1187.arXiv:astro-ph/0512551.Bibcode:2006ApJ...641.1178L.doi:10.1086/500566.S2CID 119432579.
^"The Harsh Destiny of a Planet?" (Press release). Garching, Germany:European Southern Observatory. May 9, 2001.Archived from the original on September 21, 2020. RetrievedDecember 30, 2012.
^Rodriguez, Joseph E; Vanderburg, Andrew; Eastman, Jason D; Mann, Andrew W; Crossfield, Ian J. M; Ciardi, David R; Latham, David W; Quinn, Samuel N (2018)."A System of Three Super Earths Transiting the Late K-Dwarf GJ 9827 at 30 pc".The Astronomical Journal.155 (2): 72.arXiv:1709.01957.Bibcode:2018AJ....155...72R.doi:10.3847/1538-3881/aaa292.S2CID 55459523.
^Andreolo, Claire; Cofield, Calla; Kazmierczak, Jeanette (6 January 2020)."NASA Planet Hunter Finds Earth-Size Habitable-Zone World".NASA.Archived from the original on 14 April 2020. Retrieved6 January 2020.
^Garner, Rob (6 January 2020)."NASA Planet Hunter Finds Earth-Size Habitable-Zone World".NASA.Archived from the original on 5 April 2020. Retrieved6 January 2020.
^Wall, Mike (6 January 2020)."NASA's TESS Planet Hunter Finds Its 1st Earth-Size World in 'Habitable Zone'".Space.com.Archived from the original on 8 April 2020. Retrieved6 January 2020.
^Vanderburg, Andrew; et al. (2019)."TESS Spots a Compact System of Super-Earths around the Naked-Eye Star HR 858".The Astrophysical Journal.881 (1): L19.arXiv:1905.05193.Bibcode:2019ApJ...881L..19V.doi:10.3847/2041-8213/ab322d.S2CID 153311715.
^Vogt, Steven S.; et al. (2005)."Five New Multicomponent Planetary Systems"(PDF).The Astrophysical Journal.632 (1):638–658.Bibcode:2005ApJ...632..638V.doi:10.1086/432901.S2CID 16509245.Archived(PDF) from the original on 2018-07-22. Retrieved2020-12-11.
^Udry, S.; Dumusque, X.; Lovis, C.; Segransan, D.; Diaz, R. F.; Benz, W.; Bouchy, F.; Coffinet, A.; Lo Curto, G.; Mayor, M.; Mordasini, C.; Motalebi, F.; Pepe, F.; Queloz, D.; Santos, N. C.; Wyttenbach, A.; Alonso, R.; Collier Cameron, A.; Deleuil, M.; Figueira, P.; Gillon, M.; Moutou, C.; Pollacco, D.; Pompei, E. (2019), "The HARPS search for southern extra-solar planets. XLII. Eight HARPS multi-planet systems hosting 20 super-Earth and Neptune-mass companions",Astronomy & Astrophysics,A37: 622,arXiv:1705.05153,Bibcode:2019A&A...622A..37U,doi:10.1051/0004-6361/201731173,S2CID 119095511
^Mayor, M.; Marmier, M.; Lovis, C.; Udry, S.; Ségransan, D.; Pepe, F.; Benz, W.; Bertaux, J.-L.; Bouchy, F.; Dumusque, G.; Curto, Lo; Mordasini, C.; Queloz, D.; Santos, N. C.; et al. (2011). "The HARPS search for southern extra-solar planets XXXIV. Occurrence, mass distribution and orbital properties of super-Earths and Neptune-mass planets".arXiv:1109.2497 [astro-ph].
^Hébrard, Guillaume; Arnold, Luc; Forveille, Thierry; Correia, Alexandre C. M.; Laskar, Jacques; Bonfils, Xavier; Boisse, Isabelle; Díaz, Rodrigo F.; Hagelberg, Janis; Sahlmann, Johannes; Santos, Nuno C.; et al. (2016-04-01)."The SOPHIE search for northern extrasolar planets. X. Detection and characterization of giant planets by the dozen".Astronomy and Astrophysics.588: A145.arXiv:1602.04622.Bibcode:2016A&A...588A.145H.doi:10.1051/0004-6361/201527585.ISSN 0004-6361.S2CID 55138055.Archived from the original on 2019-04-10. Retrieved2022-02-26.
^Philip S. Muirhead; John Asher Johnson; Kevin Apps; Joshua A. Carter; Timothy D. Morton; Daniel C. Fabrycky; J. Sebastian Pineda; Michael Bottom; Barbara Rojas-Ayala; Everett Schlawin; Katherine Hamren; Kevin R. Covey; Justin R. Crepp; Keivan G. Stassun; Joshua Pepper; Leslie Hebb; Evan N. Kirby; Andrew W. Howard; Howard T. Isaacson; Geoffrey W. Marcy; David Levitan; Tanio Diaz-Santos; Lee Armus; James P. Lloyd (2012). "Characterizing the Cool KOIs III. KOI-961: A Small Star with Large Proper Motion and Three Small Planets".The Astrophysical Journal.747 (2): 144.arXiv:1201.2189.Bibcode:2012ApJ...747..144M.doi:10.1088/0004-637X/747/2/144.S2CID 14889361.
^Tuomi, Mikko (6 April 2012). "Evidence for 9 planets in the 10180 system".Astronomy & Astrophysics.543: A52.arXiv:1204.1254v1.Bibcode:2012A&A...543A..52T.doi:10.1051/0004-6361/201118518.S2CID 15876919.
^"Three Super-Earths Found Circling Nearby Red Dwarf".Archived from the original on 2019-01-02. Retrieved2022-02-27.
^^a ^bTeske, Johanna K; Shectman, Stephen A; Vogt, Steve S; Díaz, Matías; Butler, R. Paul; Crane, Jeffrey D; Thompson, Ian B; Arriagada, Pamela (2016)."The Magellan PFS Planet Search Program: Radial Velocity and Stellar Abundance Analyses of the 360 AU, Metal-Poor Binary "Twins" HD 133131A & B".The Astronomical Journal.152 (6): 167.arXiv:1608.06216.Bibcode:2016AJ....152..167T.doi:10.3847/0004-6256/152/6/167.S2CID 118852162.
^Orell-Miquel, J.; Nowak, G.; Murgas, F.; Palle, E.; Morello, G.; Luque, R.; Badenas-Agusti, M.; Ribas, I.; Lafarga, M.; Espinoza, N.; Morales, J. C.; Zechmeister, M.; Alqasim, A.; Cochran, W. D.; Gandolfi, D.; Goffo, E.; Kabáth, P.; Korth, J.; Livingston, J.; Lam, K. W. F.; Muresan, A.; Persson, C. M.; Van Eylen, V. (2023). "HD 191939 revisited: New and refined planet mass determinations, and a new planet in the habitable zone".Astronomy & Astrophysics.669: A40.arXiv:2211.00667.Bibcode:2023A&A...669A..40O.doi:10.1051/0004-6361/202244120.S2CID 253197272.
^^a ^bLeleu, A.; Alibert, Y.; Hara, N. C.; Hooton, M. J.; Wilson, T. G.; Robutel, P.; Delisle, J.-B.; Laskar, J.; Hoyer, S.; Lovis, C.; Bryant, E. M.; Ducrot, E.; Cabrera, J.; Delrez, L.; Acton, J. S.; Adibekyan, V.; Allart, R.; Prieto, Allende; Alonso, R.; Alves, D.; et al. (2021-01-20). "Six transiting planets and a chain of Laplace resonances in TOI-178".Astronomy & Astrophysics.649: A26.arXiv:2101.09260.Bibcode:2021A&A...649A..26L.doi:10.1051/0004-6361/202039767.ISSN 0004-6361.S2CID 231693292.
^Rajpaul, V. M.; Buchhave, L. A.; Lacedelli, G.; Rice, K.; Mortier, A.; Malavolta, L.; Aigrain, S.; Borsato, L.; Mayo, A. W.; Charbonneau, D.; Damasso, M.; Dumusque, X.; Ghedina, A.; Latham, D. W.; López-Morales, M.; Magazzù, A.; Micela, G.; Molinari, E.; Pepe, F.; Piotto, G.; Poretti, E.; Rowther, S.; Sozzetti, A.; Udry, S.; Watson, C. A. (2021), "A HARPS-N mass for the elusive Kepler-37d: A case study in disentangling stellar activity and planetary signals",Monthly Notices of the Royal Astronomical Society,507 (2):1847–1868,arXiv:2107.13900,Bibcode:2021MNRAS.507.1847R,doi:10.1093/mnras/stab2192 Kepler-37e is discussed in sections 2.2.2 & 6.4.
^Dai, Fei; Masuda, Kento; et al. (February 2023)."TOI-1136 is a Young, Coplanar, Aligned Planetary System in a Pristine Resonant Chain".The Astronomical Journal.165 (2): 33.arXiv:2210.09283.Bibcode:2023AJ....165...33D.doi:10.3847/1538-3881/aca327.
^"KOI-82".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved20 March 2022.
^David, Trevor J.; Cody, Ann Marie; Hedges, Christina L.; Mamajek, Eric E.; Hillenbrand, Lynne A.; Ciardi, David R.; Beichman, Charles A.; Petigura, Erik A.; Fulton, Benjamin J.; Isaacson, Howard T.; Howard, Andrew W. (August 2019)."A Warm Jupiter-sized Planet Transiting the Pre-main-sequence Star V1298 Tau".The Astronomical Journal.158 (2): 79.arXiv:1902.09670.Bibcode:2019AJ....158...79D.doi:10.3847/1538-3881/ab290f.ISSN 0004-6256.S2CID 119003936.
^David, Trevor J.; Petigura, Erik A.; Luger, Rodrigo; Foreman-Mackey, Daniel; Livingston, John H.; Mamajek, Eric E.; Hillenbrand, Lynne A. (2019-10-29)."Four Newborn Planets Transiting the Young Solar Analog V1298 Tau".The Astrophysical Journal.885 (1): L12.arXiv:1910.04563.Bibcode:2019ApJ...885L..12D.doi:10.3847/2041-8213/ab4c99.ISSN 2041-8213.S2CID 204008446.
^Akinsanmi, B.; Santos, N. C.; Faria, J. P.; Oshagh, M.; Barros, S. C. C.; Santerne, A.; Charnoz, S. (2020-03-01)."Can planetary rings explain the extremely low density of HIP 41378 𝑓?".Astronomy & Astrophysics.635: L8.arXiv:2002.11422.doi:10.1051/0004-6361/202037618.ISSN 0004-6361.Archived from the original on 2021-10-28. Retrieved2022-03-19.
^Santerne, A.; Malavolta, L.; Kosiarek, M. R.; Dai, F.; Dressing, C. D.; Dumusque, X.; Hara, N. C.; Lopez, T. A.; Mortier, A.; Vanderburg, A.; Adibekyan, V.; Armstrong, D. J.; Barrado, D.; Barros, S. C. C.; Bayliss, D.; Berardo, D.; Boisse, I.; Bonomo, A. S.; Bouchy, F.; Brown, D. J. A.; Buchhave, L. A.; Butler, R. P.; Collier Cameron, A.; Cosentino, R.; Crane, J. D.; Crossfield, I. J. M.; Damasso, M.; Deleuil, M. R.; Delgado Mena, E.; et al. (2019). "An extremely low-density and temperate giant exoplanet".arXiv:1911.07355 [astro-ph.EP].
^Andrew Vanderburg; et al. (2016)."Five Planets Transiting a Ninth Magnitude Star".The Astrophysical Journal.827 (1): L10.arXiv:1606.08441.Bibcode:2016ApJ...827L..10V.doi:10.3847/2041-8205/827/1/L10.S2CID 8794583.
^Martin, Pierre-Yves (2022)."Planet HD 33142 c".exoplanet.eu.Archived from the original on 2024-02-03. Retrieved2024-02-03.
^Hirano, Teruyuki; Dai, Fei; Gandolfi, Davide; Fukui, Akihiko; Livingston, John H.; Miyakawa, Kohei; Endl, Michael; Cochran, William D.; Alonso-Floriano, Francisco J.; Kuzuhara, Masayuki; Montes, David; Ryu, Tsuguru; Albrecht, Simon; Barragan, Oscar; Cabrera, Juan; Csizmadia, Szilard; Deeg, Hans; Eigmüller, Philipp; Erikson, Anders; Fridlund, Malcolm; Grziwa, Sascha; Guenther, Eike W.; Hatzes, Artie P.; Korth, Judith; Kudo, Tomoyuki; Kusakabe, Nobuhiko; Narita, Norio; Nespral, David; Nowak, Grzegorz; et al. (2018)."Exoplanets around Low-mass Stars Unveiled by K2".The Astronomical Journal.155 (3): 127.arXiv:1710.03239.Bibcode:2018AJ....155..127H.doi:10.3847/1538-3881/aaa9c1.S2CID 54590874.
^Gilliland, Ronald L.; et al. (2013)."Kepler-68: Three Planets, One with a Density Between That of Earth and Ice Giants".The Astrophysical Journal.766 (1). 40.arXiv:1302.2596.Bibcode:2013ApJ...766...40G.doi:10.1088/0004-637X/766/1/40.
^Mills, Sean M.; et al. (2019)."Long-period Giant Companions to Three Compact, Multiplanet Systems".The Astronomical Journal.157 (4). 145.arXiv:1903.07186.Bibcode:2019AJ....157..145M.doi:10.3847/1538-3881/ab0899.S2CID 119197547.
^Desidera, S.; et al. (2014)."The GAPS programme with HARPS-N at TNG. IV. A planetary system around XO-2S".Astronomy and Astrophysics.567 (6). L6.arXiv:1407.0251.Bibcode:2014A&A...567L...6D.doi:10.1051/0004-6361/201424339.S2CID 118567085.Archived from the original on 2021-05-11. Retrieved2022-06-25.
^Damasso, M.; et al. (2015)."A comprehensive analysis of the XO-2 stellar and planetary systems".Astronomy & Astrophysics.575. A111.arXiv:1501.01424.doi:10.1051/0004-6361/201425332.
^Heller, René; Rodenbeck, Kai; Hippke, Michael (2019)."Transit least-squares survey. I. Discovery and validation of an Earth-sized planet in the four-planet system K2-32 near the 1:2:5:7 resonance".Astronomy and Astrophysics.625. A31.arXiv:1904.00651.Bibcode:2019A&A...625A..31H.doi:10.1051/0004-6361/201935276.Archived from the original on 2022-01-25. Retrieved2022-03-04.
^Souto, Diogo; et al. (2017)."Chemical Abundances of M-dwarfs from the APOGEE Survey. I. The Exoplanet Hosting Stars Kepler-138 and Kepler-186".The Astrophysical Journal.835 (2): 239.arXiv:1612.01598.Bibcode:2017ApJ...835..239S.doi:10.3847/1538-4357/835/2/239.S2CID 73634716.
^Bailer-Jones, C. A. L.; et al. (August 2018)."Estimating distances from parallaxes IV: Distances to 1.33 billion stars in Gaia Data Release 2".The Astronomical Journal.156 (2): 58.arXiv:1804.10121.Bibcode:2018AJ....156...58B.doi:10.3847/1538-3881/aacb21.S2CID 119289017. Distance to Kepler 186, after taking into account light extinction Archived 2022-05-11 at theWayback Machine
^"Kepler-186 f".NASA Exoplanet Archive.Archived from the original on 18 March 2022. Retrieved19 July 2016.
^Quintana, E. V.; Barclay, T.; Raymond, S. N.; Rowe, J. F.; Bolmont, E.; Caldwell, D. A.; Howell, S. B.; Kane, S. R.; Huber, D.; Crepp, J. R.;Lissauer, J. J.; Ciardi, D. R.; Coughlin, J. L.; Everett, M. E.; Henze, C. E.; Horch, E.; Isaacson, H.; Ford, E. B.; Adams, F. C.; Still, M.; Hunter, R. C.; Quarles, B.; Selsis, F. (2014-04-18). "An Earth-Sized Planet in the Habitable Zone of a Cool Star".Science.344 (6181):277–280.arXiv:1404.5667.Bibcode:2014Sci...344..277Q.doi:10.1126/science.1249403.PMID 24744370.S2CID 1892595. free version =http://www.nasa.gov/sites/default/files/files/kepler186_main_final.pdf Archived 2014-04-18 at theWayback Machine
^Christiansen, Jessie L.; Crossfield, Ian J. M.; Barentsen, Geert; Lintott, Chris J.; Barclay, Thomas; Simmons, Brooke D.; Petigura, Erik; Schlieder, Joshua E.; Dressing, Courtney D.; Vanderburg, Andrew; Ciardi, David R.; Allen, Campbell; McMaster, Adam; Miller, Grant; Veldthuis, Martin; Allen, Sarah; Wolfenbarger, Zach; Cox, Brian; Zemiro, Julia; Howard, Andrew W.; Livingston, John; Sinukoff, Evan; Catron, Timothy; Grey, Andrew; Kusch, Joshua J. E.; Terentev, Ivan; Vales, Martin; Kristiansen, Martti H. (2018-01-11)."The K2-138 System: A Near-resonant Chain of Five Sub-Neptune Planets Discovered by Citizen Scientists".The Astronomical Journal.155 (2): 57.arXiv:1801.03874.Bibcode:2018AJ....155...57C.doi:10.3847/1538-3881/aa9be0.ISSN 1538-3881.S2CID 52971376.
^Becker, Juliette C.; Vanderburg, Andrew; Adams, Fred C.; Rappaport, Saul A.; Schwengeler, Hans Martin (2015-10-12). "Wasp-47: A Hot Jupiter System with Two Additional Planets Discovered by K2".The Astrophysical Journal.812 (2): L18.arXiv:1508.02411.Bibcode:2015ApJ...812L..18B.doi:10.1088/2041-8205/812/2/L18.ISSN 2041-8213.S2CID 14681933.
^Neveu-VanMalle, M.; et al. (2016)."Hot Jupiters with relatives: Discovery of additional planets in orbit around WASP-41 and WASP-47".Astronomy and Astrophysics.586. A93.arXiv:1509.07750.Bibcode:2016A&A...586A..93N.doi:10.1051/0004-6361/201526965.S2CID 53354547.Archived from the original on 2022-02-28. Retrieved2022-05-08.
^"WASP-47".exoplanetarchive.ipac.caltech.edu.Archived from the original on 2022-05-08. Retrieved2022-05-08.
^Malavolta, Luca; et al. (2017)."The Kepler-19 System: A Thick-envelope Super-Earth with Two Neptune-mass Companions Characterized Using Radial Velocities and Transit Timing Variations".The Astronomical Journal.153 (5). 224.arXiv:1703.06885.Bibcode:2017AJ....153..224M.doi:10.3847/1538-3881/aa6897.
^Lissauer, Jack J; Marcy, Geoffrey W; Bryson, Stephen T; Rowe, Jason F; Jontof-Hutter, Daniel; Agol, Eric; Borucki, William J; Carter, Joshua A; Ford, Eric B; Gilliland, Ronald L; Kolbl, Rea; Star, Kimberly M; Steffen, Jason H; Torres, Guillermo (2014). "Validation Of Kepler's Multiple Planet Candidates. Ii. Refined Statistical Framework and Descriptions of Systems of Special Interest".The Astrophysical Journal.784 (1): 44.arXiv:1402.6352.Bibcode:2014ApJ...784...44L.doi:10.1088/0004-637X/784/1/44.S2CID 119108651.
^^a ^bBarclay, Thomas; Quintana, Elisa V; Adams, Fred C; Ciardi, David R; Huber, Daniel; Foreman-Mackey, Daniel; Montet, Benjamin T; Caldwell, Douglas (2015). "The Five Planets in the Kepler-296 Binary System All Orbit the Primary: A Statistical and Analytical Analysis".The Astrophysical Journal.809 (1): 7.arXiv:1505.01845.Bibcode:2015ApJ...809....7B.doi:10.1088/0004-637X/809/1/7.S2CID 37742564.
^Schneider, Jean,"Star: Kepler-25",Extrasolar Planets Encyclopaedia, archived fromthe original on 2012-06-16, retrieved2013-12-18
^Steffen, Jason H.; et al. (2012)."Transit timing observations from Kepler - III. Confirmation of four multiple planet systems by a Fourier-domain study of anticorrelated transit timing variations".Monthly Notices of the Royal Astronomical Society.421 (3):2342–2354.arXiv:1201.5412.Bibcode:2012MNRAS.421.2342S.doi:10.1111/j.1365-2966.2012.20467.x.
^Marcy, Geoffrey W.; et al. (2014)."Masses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets".The Astrophysical Journal Supplement Series.210 (2). 20.arXiv:1401.4195.Bibcode:2014ApJS..210...20M.doi:10.1088/0067-0049/210/2/20.
^Hand, Eric (20 December 2011). "Kepler discovers first Earth-sized exoplanets".Nature.doi:10.1038/nature.2011.9688.S2CID 122575277.
^Nespral, D.; et al. (2017)."Mass determination of K2-19b and K2-19c from radial velocities and transit timing variations".Astronomy and Astrophysics.601. A128.arXiv:1604.01265.Bibcode:2017A&A...601A.128N.doi:10.1051/0004-6361/201628639.S2CID 55978628.Archived from the original on 2022-05-04. Retrieved2022-03-18.
^Sinukoff, Evan; et al. (2016)."Eleven Multiplanet Systems From K2 Campaigns 1 and 2 and the Masses of Two Hot Super-Earths".The Astrophysical Journal.827 (1). 78.arXiv:1511.09213.Bibcode:2016ApJ...827...78S.doi:10.3847/0004-637X/827/1/78.
^"Pulsar Planets". Archived fromthe original on 30 December 2005.
^Wolszczan, A.; Frail, D. (1992). "A planetary system around the millisecond pulsar PSR1257 + 12".Nature.355 (6356):145–147.Bibcode:1992Natur.355..145W.doi:10.1038/355145a0.S2CID 4260368.
^^a ^b ^cBorucki, William J.; et al. (18 April 2013)."Kepler-62: A Five-Planet System with Planets of 1.4 and 1.6 Earth Radii in the Habitable Zone".Science Express.340 (6132):587–90.arXiv:1304.7387.Bibcode:2013Sci...340..587B.doi:10.1126/science.1234702.hdl:1721.1/89668.PMID 23599262.S2CID 21029755.Archived from the original on 2 May 2022. Retrieved18 March 2022.
^Johnson, Michele; Harrington, J.D. (18 April 2013)."NASA's Kepler Discovers Its Smallest 'Habitable Zone' Planets to Date".NASA. Archived fromthe original on 8 May 2020. Retrieved18 March 2022.
^Steffen, Jason H.; Fabrycky, Daniel C.; Ford, Eric B.; Carter, Joshua A.; Desert, Jean-Michel; Fressin, Francois; Holman, Matthew J.; Lissauer, Jack J.; Moorhead, Althea V.; Rowe, Jason F.; Ragozzine, Darin; Welsh, William F.; Batalha, Natalie M.; Borucki, William J.; Buchhave, Lars A.; Bryson, Steve; Caldwell, Douglas A.; Charbonneau, David; Ciardi, David R.; Cochran, William D.; Endl, Michael; Everett, Mark E.; Gautier III, Thomas N.; Gilliland, Ron L.; Girouard, Forrest R.; Jenkins, Jon M.; Horch, Elliott; Howell, Steve B.; Isaacson, Howard; et al. (2012), "Transit Timing Observations from Kepler: III. Confirmation of 4 Multiple Planet Systems by a Fourier-Domain Study of Anti-correlated Transit Timing Variations",Monthly Notices of the Royal Astronomical Society,421 (3),arXiv:1201.5412,Bibcode:2012MNRAS.421.2342S,doi:10.1111/j.1365-2966.2012.20467.x,S2CID 11898578
^Cubillos, Patricio; Erkaev, Nikolai V.; Juvan, Ines; Fossati, Luca; Johnstone, Colin P.; Lammer, Helmut; Lendl, Monika; Odert, Petra; Kislyakova, Kristina G. (2016), "An overabundance of low-density Neptune-like planets",Monthly Notices of the Royal Astronomical Society,466 (2):1868–1879,arXiv:1611.09236,doi:10.1093/mnras/stw3103,S2CID 119408956
^Jontof-Hutter, Daniel; Ford, Eric B.; Rowe, Jason F.; Lissauer, Jack J.; Fabrycky, Daniel C.; Christa Van Laerhoven; Agol, Eric; Deck, Katherine M.; Holczer, Tomer; Mazeh, Tsevi (2015), "Secure TTV Mass Measurements: Ten Kepler Exoplanets between 3 and 8 M_🜨 with Diverse Densities and Incident Fluxes",The Astrophysical Journal,820 (1): 39,arXiv:1512.02003,doi:10.3847/0004-637X/820/1/39,S2CID 11322397
^Kipping, David M.; Torres, Guillermo; et al. (April 2016)."A Transiting Jupiter Analog".The Astrophysical Journal.820 (2): 112.arXiv:1603.00042.Bibcode:2016ApJ...820..112K.doi:10.3847/0004-637X/820/2/112.S2CID 1892262.
^Chachan, Yayaati; Dalba, Paul A.; et al. (February 2022)."Kepler-167e as a Probe of the Formation Histories of Cold Giants with Inner Super-Earths".The Astrophysical Journal.926 (1): 62.arXiv:2112.00747.Bibcode:2022ApJ...926...62C.doi:10.3847/1538-4357/ac3ed6.S2CID 244799213.
^"Kepler-80".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved10 January 2017.
^Xie, J.-W. (2013). "Transit timing variation of near-resonance planetary pairs: confirmation of 12 multiple-planet systems".Astrophysical Journal Supplement Series.208 (2): 22.arXiv:1208.3312.Bibcode:2013ApJS..208...22X.doi:10.1088/0067-0049/208/2/22.S2CID 17160267.
^^a ^bShallue, C. J.; Vanderburg, A. (2017)."Identifying Exoplanets With Deep Learning: A Five Planet Resonant Chain Around Kepler-80 And An Eighth Planet Around Kepler-90"(PDF).The Astrophysical Journal.155 (2): 94.arXiv:1712.05044.Bibcode:2018AJ....155...94S.doi:10.3847/1538-3881/aa9e09.S2CID 4535051.Archived(PDF) from the original on 2017-12-24. Retrieved2017-12-15.
^MacDonald, Mariah G.; Ragozzine, Darin; Fabrycky, Daniel C.; Ford, Eric B.; Holman, Matthew J.; Isaacson, Howard T.; Lissauer, Jack J.; Lopez, Eric D.; Mazeh, Tsevi (2016-01-01)."A Dynamical Analysis of the Kepler-80 System of Five Transiting Planets".The Astronomical Journal.152 (4): 105.arXiv:1607.07540.Bibcode:2016AJ....152..105M.doi:10.3847/0004-6256/152/4/105.S2CID 119265122.
^Ekrem Murat Esmer; Baştürk, Özgür; Selim Osman Selam; Aliş, Sinan (2022), "Detection of two additional circumbinary planets around Kepler-451",Monthly Notices of the Royal Astronomical Society,511 (4):5207–5216,arXiv:2202.02118,Bibcode:2022MNRAS.511.5207E,doi:10.1093/mnras/stac357
^Masuda, Kento; Hirano, Teruyuki; Taruya, Atsushi; Nagasawa, Makiko; Suto, Yasushi (2013). "Characterization of the KOI-94 System with Transit Timing Variation Analysis: Implication for the Planet-Planet Eclipse".The Astrophysical Journal.778 (2):185–200.arXiv:1310.5771.Bibcode:2013ApJ...778..185M.doi:10.1088/0004-637X/778/2/185.S2CID 119264400.
^Bonomo, Aldo S.; Zeng, Li; Damasso, Mario; Leinhardt, Zoë M.; Justesen, Anders B.; Lopez, Eric; Lund, Mikkel N.; Malavolta, Luca; Silva Aguirre, Victor; Buchhave, Lars A.; Corsaro, Enrico; Denman, Thomas; Lopez-Morales, Mercedes; Mills, Sean M.; Mortier, Annelies; Rice, Ken; Sozzetti, Alessandro; Vanderburg, Andrew; Affer, Laura; Arentoft, Torben; Benbakoura, Mansour; Bouchy, François; Christensen-Dalsgaard, Jørgen; Collier Cameron, Andrew; Cosentino, Rosario; Dressing, Courtney D.; Dumusque, Xavier; Figueira, Pedro; Fiorenzano, Aldo F. M.; García, Rafael A.; Handberg, Rasmus; Harutyunyan, Avet; Johnson, John A.; Kjeldsen, Hans; Latham, David W.; Lovis, Christophe; Lundkvist, Mia S.; Mathur, Savita; Mayor, Michel; Micela, Giusi; Molinari, Emilio; Motalebi, Fatemeh; Nascimbeni, Valerio; Nava, Chantanelle; Pepe, Francesco; Phillips, David F.; Piotto, Giampaolo; Poretti, Ennio; Sasselov, Dimitar; Ségransan, Damien; Udry, Stéphane; Watson, Chris (May 2019). "A giant impact as the likely origin of different twins in the Kepler-107 exoplanet system".Nature Astronomy.3 (5):416–423.arXiv:1902.01316.Bibcode:2019NatAs...3..416B.doi:10.1038/s41550-018-0684-9.S2CID 89604609.
^"The Extrasolar Planet Encyclopaedia — Kepler-176 b.".Extrasolar Planets Encyclopaedia. 2025.
^^a ^bLissauer, Jack J.; et al. (2011). "A closely packed system of low-mass, low-density planets transiting Kepler-11".Nature.470 (7332):53–58.arXiv:1102.0291.Bibcode:2011Natur.470...53L.doi:10.1038/nature09760.PMID 21293371.S2CID 4388001.
^Lissauer, Jack J.; et al. (2013)."All Six Planets Known to Orbit Kepler-11 Have Low Densities".The Astrophysical Journal.770 (2). 131.arXiv:1303.0227.Bibcode:2013ApJ...770..131L.doi:10.1088/0004-637X/770/2/131.
^Libby-Roberts, Jessica E.; et al. (2020)."The Featureless Transmission Spectra of Two Super-puff Planets".The Astronomical Journal.159 (2): 57.arXiv:1910.12988.Bibcode:2020AJ....159...57L.doi:10.3847/1538-3881/ab5d36.S2CID 204950000.
^Nancy Atkinson (26 August 2010)."Kepler Discovers Multi-Planet System". Universe Today.Archived from the original on 24 February 2012. Retrieved13 January 2011.
^Holman, M. J.; et al. (2010)."Kepler-9: A System of Multiple Planets Transiting a Sun-Like Star, Confirmed by Timing Variations"(PDF).Science.330 (6000):51–54.Bibcode:2010Sci...330...51H.doi:10.1126/science.1195778.PMID 20798283.S2CID 8141085.Archived(PDF) from the original on 2022-12-07. Retrieved2022-06-17.
^Chou, Felicia; Hawkes, Alison; Landau, Elizabeth (14 December 2017)."Artificial Intelligence, NASA Data Used to Discover Eighth Planet Circling Distant Star".NASA.Archived from the original on 5 May 2020. Retrieved15 December 2017.
^Schmitt, J. R.; Wang, J.; Fischer, D. A.; Jek, K. J.; Moriarty, J. C.; Boyajian, T. S.; Schwamb, M. E.; Lintott, C.; Lynn, S.; Smith, A. M.; Parrish, M.; Schawinski, K.; Simpson, R.; LaCourse, D.; Omohundro, M. R.; Winarski, T.; Goodman, S. J.; Jebson, T.; Schwengeler, H. M.; Paterson, D. A.; Sejpka, J.; Terentev, I.; Jacobs, T.; Alsaadi, N.; Bailey, R. C.; Ginman, T.; Granado, P.; Guttormsen, K. V.; Mallia, F.; Papillon, A. L.; Rossi, F.; Socolovsky, M.; Stiak, L. (2014-06-26). "Planet Hunters. VI. An Independent Characterization of KOI-351 and Several Long Period Planet Candidates From the Kepler Archival Data".The Astronomical Journal.148 (28): 28.arXiv:1310.5912.Bibcode:2014AJ....148...28S.doi:10.1088/0004-6256/148/2/28.S2CID 119238163.
^Patel, Neel V. (2020-06-05)."Astronomers have found a planet like Earth orbiting a star like the sun".MIT Technology Review.Archived from the original on 2023-05-25. Retrieved2020-06-07.
^Orosz, Jerome A.; Welsh, William F.; Carter, Joshua A.; Fabrycky, Daniel C.; Cochran, William D.; Endl, Michael; Ford, Eric B.; Haghighipour, Nader; MacQueen, Phillip J.; Mazeh, Tsevi; Sanchis-Ojeda, Roberto; Short, Donald R.; Torres, Guillermo; Agol, Eric; Buchhave, Lars A.; Doyle, Laurance R.; Isaacson, Howard; Lissauer, Jack J.; Marcy, Geoffrey W.; Shporer, Avi; Windmiller, Gur; Barclay, Thomas; Boss, Alan P.; Clarke, Bruce D.; Fortney, Jonathan; Geary, John C.; Holman, Matthew J.; Huber, Daniel; Jenkins, Jon M.; et al. (2012). "Kepler-47: A Transiting Circumbinary Multi-Planet System".Science.337 (6101):1511–4.arXiv:1208.5489.Bibcode:2012Sci...337.1511O.doi:10.1126/science.1228380.PMID 22933522.S2CID 44970411.
^"NASA's Kepler Discovers Multiple Planets Orbiting a Pair of Stars".exoplanets.nasa.gov.NASA. 28 August 2012. Archived fromthe original on 31 October 2012. Retrieved2 September 2012.Kepler mission has discovered multiple transiting planets orbiting two suns for the first time
^Orosz, Jerome A.; Welsh, William F.; Carter, Joshua A.; Fabrycky, Daniel C.; Cochran, William D.; Endl, Michael; Ford, Eric B.; Haghighipour, Nader; MacQueen, Phillip J.; Mazeh, Tsevi; Sanchis-Ojeda, Roberto; Short, Donald R.; Torres, Guillermo; Agol, Eric; Buchhave, Lars A.; Doyle, Laurance R.; Isaacson, Howard; Lissauer, Jack J.; Marcy, Geoffrey W.; Shporer, Avi; Windmiller, Gur; Barclay, Thomas; Boss, Alan P.; Clarke, Bruce D.; Fortney, Jonathan; Geary, John C.; Holman, Matthew J.; Huber, Daniel; Jenkins, Jon M.; et al. (28 August 2012)."NASA's Kepler discovers multiple planets orbiting a pair of stars".Science.337 (6101).Sciencedaily.com:1511–4.arXiv:1208.5489.Bibcode:2012Sci...337.1511O.doi:10.1126/science.1228380.hdl:1721.1/89172.PMID 22933522.S2CID 44970411.Archived from the original on 21 September 2022. Retrieved4 November 2012.
^Pichierri, Gabriele; Batygin, Konstantin; Morbidelli, Alessandro (2019), "The role of dissipative evolution for three-planet, near-resonant extrasolar systems",Astronomy & Astrophysics,625: A7,arXiv:1903.09474,Bibcode:2019A&A...625A...7P,doi:10.1051/0004-6361/201935259,S2CID 85459759
^Mugrauer, M.; et al. (2006)."HD 3651 B: the first directly imaged brown dwarf companion of an exoplanet host star".Monthly Notices of the Royal Astronomical Society: Letters (abstract).373 (1):L31 –L35.arXiv:astro-ph/0608484.Bibcode:2006MNRAS.373L..31M.doi:10.1111/j.1745-3933.2006.00237.x.S2CID 15608344.
^Marcy, Geoffrey W.; et al. (1999). "Two New Planets in Eccentric Orbits".The Astrophysical Journal.520 (1):239–247.arXiv:astro-ph/9904275.Bibcode:1999ApJ...520..239M.doi:10.1086/307451.S2CID 16827678.
^Marcy, Geoffrey W.; et al. (2001)."Two Substellar Companions Orbiting HD 168443".The Astrophysical Journal.555 (1):418–425.Bibcode:2001ApJ...555..418M.doi:10.1086/321445.
^Cheetham, A.; et al. (June 2018). "Direct imaging of an ultracool substellar companion to the exoplanet host star HD 4113 A".Astronomy & Astrophysics.614: 19.arXiv:1712.05217.Bibcode:2018A&A...614A..16C.doi:10.1051/0004-6361/201630136.S2CID 119084543. A16.
^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,S2CID 204575783
^Scholz, Ralf-Dieter; McCaughrean, Mark (2003-01-13)."Discovery of Nearest Known Brown Dwarf: Bright Southern Star Epsilon Indi Has Cool, Substellar Companion". European Southern Observatory. Archived fromthe original on October 14, 2007. Retrieved2006-05-24.
^Scholz, R.-D.; McCaughrean, M. J.; Lodieu, N.; Kuhlbrodt, B. (February 2003). "ε Indi B: A new benchmark T dwarf".Astronomy and Astrophysics.398 (3):L29 –L33.arXiv:astro-ph/0212487.Bibcode:2003A&A...398L..29S.doi:10.1051/0004-6361:20021847.S2CID 119474823.
^Butler, R. P.; et al. (2006). "Catalog of Nearby Exoplanets".The Astrophysical Journal.646 (1):505–522.arXiv:astro-ph/0607493.Bibcode:2006ApJ...646..505B.doi:10.1086/504701.S2CID 119067572.
^Feng, Fabo; Butler, R. Paul; et al. (August 2022)."3D Selection of 167 Substellar Companions to Nearby Stars".The Astrophysical Journal Supplement Series.262 (21): 21.arXiv:2208.12720.Bibcode:2022ApJS..262...21F.doi:10.3847/1538-4365/ac7e57.S2CID 251864022.
^Hatzes, Artie P.; et al. (2022)."A Radial Velocity Study of the Planetary System of π Mensae: Improved Planet Parameters for π Mensae c and a Third Planet on a 125 Day Orbit".The Astronomical Journal.163 (5): 223.arXiv:2203.01018.Bibcode:2022AJ....163..223H.doi:10.3847/1538-3881/ac5dcb.S2CID 247218413.
^Fischer, Debra A.; et al. (2003)."A Planetary Companion to HD 40979 and Additional Planets Orbiting HD 12661 and HD 38529".The Astrophysical Journal.586 (2):1394–1408.Bibcode:2003ApJ...586.1394F.doi:10.1086/367889.
^Khandelwal, Akanksha; Sharma, Rishikesh; Chakraborty, Abhijit; Chaturvedi, Priyanka; Ulmer-Moll, Solène; Ciardi, David R.; Boyle, Andrew W.; Baliwal, Sanjay; Bieryla, Allyson; Latham, David W.; Prasad, Neelam J. S. S. V.; Nayak, Ashirbad; Lendl, Monika; Mordasini, Christoph (2023-04-01)."Discovery of a massive giant planet with extreme density around the sub-giant star TOI-4603".Astronomy & Astrophysics.672: L7.arXiv:2303.11841.Bibcode:2023A&A...672L...7K.doi:10.1051/0004-6361/202245608.ISSN 0004-6361.Archived from the original on 2024-02-28. Retrieved2023-12-15.
^Zhang, Keming; Zang, Weicheng; El-Badry, Kareem; Lu, Jessica R.; et al. (September 2024). "An Earth-mass planet and a brown dwarf in orbit around a white dwarf".Nature Astronomy.8 (12):1575–1582.arXiv:2409.02157.Bibcode:2024NatAs...8.1575Z.doi:10.1038/s41550-024-02375-9.
^Han, Cheongho; Udalski, Andrzej; Lee, Chung-Uk; Ryu, Yoon-Hyun; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew; Hwang, Kyu-Ha; Jung, Youn Kil (2025-07-09). "KMT-2024-BLG-0404L: A triple microlensing system consisting of a star, a brown dwarf, and a planet".Astronomy and Astrophysics.700: A181.arXiv:2507.07326.Bibcode:2025A&A...700A.181H.doi:10.1051/0004-6361/202452760.

Exoplanets

Main topics

Sizes
and
types

Terrestrial	Carbon planet Catastrophically evaporating planet Coreless planet Desert planet Dwarf planet Hycean planet Ice planet Iron planet (Super-Mercury) Lava planet Ocean world Mega-Earth Steam world Sub-Earth Super-Earth
Gaseous	Cold Jupiter Eccentric Jupiter Mini-Neptune (Gas dwarf) Helium planet Hot Jupiter Hot Neptune Gas giant Ice giant Neptunian Jupiter analogue Super-Jupiter Super-Neptune Super-puff Ultra-hot Jupiter Ultra-hot Neptune Warm Jupiter
Other types	Blanet Brown dwarf Chthonian planet Circumbinary planet Circumtriple planet Disrupted planet Double planet Ecumenopolis Eyeball planet Giant planet Mesoplanet Planemo Planet/Brown dwarf boundary Planetesimal Protoplanet Pulsar planet Sub-brown dwarf Sub-Neptune Toroidal planet Ultra-cool dwarf Ultra-short period planet (USP)