# List of multiplanetary systems

From the total of 5,086 stars known to have exoplanets (as of January 26, 2024), there are a total of 1,033 known multiplanetary systems, or stars with at least two confirmed planets, beyond the Solar 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 the Sun (the Solar System's star) and Kepler-90, with 8 confirmed planets each, followed by TRAPPIST-1 with 7 planets.
The 1,033 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 one confirmed planet (b, along with the candidate d and the disputed c). The nearest system with four or more confirmed planets is Barnard Star, with four known. The farthest confirmed multiplanetary system is OGLE-2012-BLG-0026L, at 13,300 light-years (4,100 pc) away.
The table below contains information about the coordinates, spectral and physical properties, and the number of confirmed (unconfirmed) planets for systems with at least 2 planets and 1 not confirmed. The two most important stellar properties are mass and metallicity because they determine how these planetary 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 1 AU.

## Multiplanetary systems

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 | – | - | - | −26.74 | 0.000016 | G2V | 1 | 5778 | 4.572 | 8 (1) | Pluto was considered a planet before 2006. The hypothesised Planet Nine remains unconfirmed. |
| Proxima Centauri | Centaurus | 14$^h$ 29$^m$ 42.94853$^s$ | −62° 40′ 46.1631″ | 10.43 to 11.11 | 4.244 | M5.5Ve | 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. Planet c initially appeared likely but has since been disputed. |
| Barnard's Star | Ophiuchus | 17$^h$ 57$^m$ 48.4985$^s$ | +04° 41′ 36.1139″ | 9.511 | 5.96 | M4.0V | 0.162 | 3195 | 10 | 4 (0) | Closest single star to the Sun with a confirmed multiplanetary system. |
| Lalande 21185 | Ursa Major | 11$^h$ 03$^m$ 20.1940$^s$ | +35° 58′ 11.5682″ | 7.520 | 8.3044±0.0007 | M2V | 0.39 | 3601±51 | 8.047 | 2 (1) | Brightest red dwarf star in the northern celestial hemisphere. |
| 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. |
| 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. Planet b is potentially habitable. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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 with a semi-major axis at approximately 19 AU. |
| 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. |
| 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, and there are more unconfirmed planets. |
| 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 exoplanets, and closest K-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. |
| 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, and a 2021 study found that it was likely a false positive. 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 | An infrared excess around this star suggests a circumstellar disk. |
| 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. |
| L 98-59 | Volans | 08$^h$ 18$^m$ 07.62$^s$ | −68° 18′ 46.8″ | 11.69 | 34.6 | M3V | 0.312 | 3412 | unknown | 4 (1) | The unconfirmed planet f orbits in the habitable zone. |
| 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) | |
| 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 | Planets d, e, f and g are potentially habitable. Only star known with exactly seven confirmed planets. All seven terrestrial planets lie within only 0.07 AU of the star. |
| 55 Cancri | Cancer | 08$^h$ 52$^m$ 35.81$^s$ | +28° 19′ 50.9″ | 5.95 | 40 | K0IV-V | 1.026 | 5217 | 7.4 | 5 | All five known planets orbit around star A (none are circumbinary or orbit around star B). Closest system with exactly five confirmed planets. |
| Gliese 180 | Eridanus | 04$^h$ 53$^m$ 49.9798$^s$ | −17° 46′ 24.294″ | 10.894 | 40.3 | M2V or M3V | 0.39 | 3562 | unknown | 3 | The habitability of planets b and c is disputed. |
| 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 the Spitzer Space Telescope in 2005. |
| 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. If confirmed, planet g is potentially habitable. |
| Upsilon Andromedae | Andromeda | 01$^h$ 36$^m$ 47.84$^s$ | +41° 24′ 19.7″ | 4.09 | 44 | F8V | 1.27 | 6107 | 3.781 | 3 | Nearest F-type main sequence star with a multiplanetary system. Second-brightest star in the night sky with a multiplanetary system after 7 Canis Majoris. All exoplanets orbit around star A in the binary system. |
| 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. The planet was the first long-period extrasolar planet discovered. The other planets were discovered later. |
| Nu$^2$ 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. |
| LHS 1140 | Cetus | 00$^h$ 44$^m$ 59.31$^s$ | −15° 16′ 16.7″ | 14.18 | 48.9 | M4.5V | 0.179 | 3216±39 | 5 | 2 (1) | Planet b is a potentially habitable Super-Earth. |
| 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. |
| 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 the circumstellar habitable zone. However, it is a gas giant, so it itself is uninhabitable although a large moon orbiting around it may be habitable. |
| 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) | |
| 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. |
| 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. |
| 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 a brown dwarf. |
| 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. |
| LHS 1678 | Caelum | 04$^h$ 32$^m$ 43$^s$ | −39° 47′ 21″ | 12 | 64.8 | M2V | 0.345 | 3490 | unknown | 3 (0) | |
| 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 significant tidal heating. |
| 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. |
| HD 164922 | Hercules | 18$^h$ 02$^m$ 30.86$^s$ | +26° 18′ 46.8″ | 7.01 | 72 | G9V | 0.874 | 5293 | 13.4 | 4 | Oldest star with a multiplanetary system. Despite its age, it is more metal-rich than the Sun. |
| 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. |
| 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 | |
| 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. |
| 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. Planet g remains unconfirmed. |
| HD 82943 | Hydra | 09$^h$ 34$^m$ 50.74$^s$ | −12° 07′ 46.4″ | 6.54 | 90 | F9V Fe+0.5 | 1.175 | 5874 | 3.08 | 3 | Planets b and c are in a 2:1 orbital resonance. Planet b orbits in the habitable zone, but it and planet c are massive enough to be brown dwarfs. HD 82943 has an unusual lithium-6 abundance. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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. |
| 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 the Kepler 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. |
| Kepler-42 | Cygnus | 19$^h$ 28$^m$ 53$^s$ | +44° 37′ 10″ | 16.12 | 126 | M5V | 0.13 | 3068 | unknown | 3 | - |
| 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 three unconfirmed candidates. If these candidate exoplanets were confirmed, HD 10180 would have the largest planetary system of any star. |
| 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) | Only A-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 massive super-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. |
| 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. |
| 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 | 0.95 | 5799±19 | 6 | 3 | 2 planets around primary, and 1 planet around secondary star. |
| 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 | |
| HD 125612 | Virgo | 14$^h$ 20$^m$ 53.51$^s$ | −17° 28′ 53.5″ | 8.33 | 177 | G3V | 1.099 | 5897 | 2.15 | 3 | - |
| 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 | 0.65 | 4316±70 | 7.1 | 6 | The planets are in an orbital resonance. |
| 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. |
| 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 | unknown | 3 (1) | |
| 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. |
| 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 | 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 | 1.101 | 4970 | 0.023 | 4 | This star is a young T Tauri variable. |
| 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. More planets are still suspected. |
| 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. |
| 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. |
| 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. Radial velocity measurements discovered an additional signal, which could be a fourth planet or a stellar companion. |
| 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. |
| 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. |
| 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 | 579.23 | M1V | 0.478 | 3788 | unknown | 5 | Planet f is the first Earth-size exoplanet discovered that orbits in the habitable zone. |
| 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. |
| 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. WASP-47 is the only planetary system known to have both planets near the hot Jupiter and another planet much further out. |
| 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. |
| Kepler-296 | Lyra | 19$^h$ 06$^m$ 09.6$^s$ | +49° 26′ 14.4″ | 12.6 | 737.113 | K7V + M1V | unknown | 4249 | unknown | 5 | All planets orbit around the primary star. Planets e and f are potentially habitable. |
| 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 | 1.22 | 6190 | unknown | 3 | Two planets were discovered by transit-timing variations, and the third planet was discovered by follow-up radial velocity measurements. |
| 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 | 6 | Planets e and f were the first Earth-sized planets to be discovered. |
| K2-19 | Virgo | 11$^h$ 39$^m$ 50.4804$^s$ | +00° 36′ 12.8773″ | 13.002 | 976 | K0V or G9V | 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. 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 | 990 | K2V | 0.69 | 4925 | 7 | 5 | Planets e and f orbit in the habitable zone. |
| 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 which are low-density planets below the size of Neptune. |
| 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. |
| 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 | 0.73 | 4250 | unknown | 6 | Red dwarf star with six confirmed planets. Five of them are in an orbital resonance. |
| 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-32 | Cygnus | 19$^h$ 51$^m$ 22.0$^s$ | +46° 34′ 27″ | 16 | 1301.1 | M1V | 0.58 | 3900 | unknown | 3 (2) | - |
| 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. |
| 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 | Farthest F-type main sequence star from the Sun with a multiplanetary system. One study found hints of additional planets orbiting Kepler-89. |
| 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 | 1.238 | 5851 | 4.29 | 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 | 0.954 | 5681 | 7.834 | 6 | Farthest star from the Sun with exactly six exoplanets. First system discovered with six transiting planets. The planets have low densities. |
| 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. |
| 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. |
| 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 | G0V | 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. A Hill stability test shows that the system is stable. 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. |
| 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. |
| 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. |
| 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 the Kepler 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-176 | Cygnus | 19$^h$ 38$^m$ 40.3$^s$ | +43° 51′ 12″ | | | | unknown | 5232 | unknown | 4 | |
| 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

Stars orbited by objects on both sides of the ~13 Jupiter mass dividing line.
* 54 Piscium (HD 3651)
* HD 168443
* HD 4113 A
* Gliese 229 A
* Epsilon Indi A
* HD 82943
* Pi Mensae
* HD 38529
* HD 245134
* KMT-2020-BLG-0414L