List of star systems within 20–25 light-years

Short description: none

This is a list of star systems within 20–25 light years of Earth. So far, 84 such objects have been found, of which only 7 are bright enough to be visible without a telescope.

## List

Key  # | Visible to the unaided eye

|

$  | Bright star (absolute magnitude of +8.5 or brighter)
| White dwarf
§  | Brown dwarf or sub-brown dwarf
* | Nearest in constellation
System←→←→ | Star or
(sub-) brown dwarf | Distance (ly) | Constellation | Coordinates:
RA, Dec
(Ep J2000, Eq J2000) | Stellar
class | Apparent magnitude
(V) | Parallax
(mas) | Notes and additional references

|
|
|
|
|
|
|
|

Gliese 784 (HD 191849) | 20.1062±0.0028 | Telescopium |  20h 13m 53.4s
−45° 09′ 50″ | M0V | 7.97 | 162.2171±0.0225[1] | [2] has 1 candidate planet [3]
WISE J2209+2711§ | 20.17±0.25 | Pegasus* |  22h 09m 05.7s
+27° 11′ 44″ | Y0 |  | 161.7±2.0[4] | [4]
G 240-72 (LHS 455, GJ 1221, EGGR 372) | 20.2588±0.0015  | Draco |  17h 48m 08.2s
+70° 52′ 35″ | DXP9 | 14.22  | 160.9952±0.0119[1] |
Gliese 555 (Wolf 1481, HN Librae, BD-11 3759) | 20.3947±0.0070 | Libra |  14h 34m 16.8s
−12° 31′ 10″ | M4.0V | 10.3–10.33 | 159.9225±0.0546[1] | [5] BY Draconis variable; has 1 known planet, 1 candidate
EQ Pegasi (Gliese 896, BD+19 5116) | A | 20.4277±0.0044 | Pegasus |  23h 31m 52.2s
+19° 56′ 14″ | M3.5V | 10.35 | 159.6634±0.0341[1] | [6] both components are flare stars; has 1 known planet orbiting star A of the binary system [7]
B | M4.5V | 12.4
Gliese 581 (Wolf 562, HO Librae) | 20.5494±0.0039 | Libra |  15h 19m 26.8s
−07° 43′ 20″ | M3.0V | 10.56–10.58 | 158.7183±0.0301[1] | [8][9] BY Draconis variable; has 3 known planets
WISE 1405+5534§  | 20.62±0.34  | Ursa Major |  14h 05m 18.3s
+55° 34′ 21″ | Y0.5  |  | 158.2±2.6[4]
ADS 7251 (HD 79210, Gliese 338, MCC 541) | A | 20.6575±0.0026 | Ursa Major |  09h 14m 22.8s
+52° 41′ 12″ | M0V | 7.64 | 157.8879±0.0197[1] | [10] has 1 known planet orbiting star B of the binary system [11]
B | K7V | 7.70
LHS 2090 (LP 368-128) | 20.7388±0.0071 | Cancer |  09h 00m 23.6s
+21° 50′ 05″ | M6.5V | 16.10 | 157.2686±0.0535[1] | [12]
Furuhjelm 46 (HD 155876, Gliese 661) | A | 20.82±0.18 | Hercules |  17h 12m 07.9s
+45° 39′ 57″ | M3 V | 9.93 | 156.66±1.37[13] | [13]
B | M3.5 V | 10.35
2MASS 1503+2525§ | 20.94±0.10 | Boötes |  15h 03m 19.6s
+25° 25′ 20″ | T5.5 |  | 155.7758±0.7557[1] | [14][4]
LP 944-20§ | 20.9615±0.0070 | Fornax* |  03h 39m 35.2s
–35° 25′ 44″ | M9V | 18.69 | 155.5982±0.0522[1] | [15]
LP 658-2 (EGGR 45) | 21.0102±0.0024 | Orion |  05h 55m 09.5s
−04° 10′ 07″ | DZ11 | 14.45 | 155.2373±0.0175[1] |
GL Virginis (G 12-30) | 21.0832±0.0061 | Virgo |  12h 18m 59.4s
+11° 07′ 34″ | M5Ve | 13.79 | 154.6999±0.0445[1] | flare star
Gliese 625 (AC 54 1646-56, G 202-48) | 21.1309±0.0022 | Draco |  16h 25m 24.6s
+54° 18′ 15″ | M2.0V | 10.17 | 154.3503±0.0161[1] | [16][17] has 1 known planet
V1054 Ophiuchi (HD 152751) | Gliese 644 A | 21.1961±0.0065 | Ophiuchus |  16h 55m 25.2s
−08° 19′ 21″ | M3 V | 9.74 | 153.8754±0.0474[1] | [18] components Ab and Ac are flare stars
Gliese 644 Ba | M4 Ve | 10.34
Gliese 644 Bb | M4 Ve | 10.84
Gliese 643 | M3.5 V | 11.74
vB 8 (Gliese 644 C) | M7.0 V | 16.80
GJ 1128 (L 100-115) | 21.2121±0.0034 | Carina |  09h 42m 46.3s
−68° 53′ 06″ | M4.0V | 12.78 | 153.7593±0.0249[1] | [15]
HD 219134 (HR 8832, Gliese 892)$ | 21.3364±0.0069 | Cassiopeia |  23h 13m 17.0s
+57° 10′ 06″ | K3V | 5.574# | 152.8640±0.0494[1] | [19] has 6 known planets
WISE 0825+2805§  | 21.37±0.28  | Cancer |  08h 25m 07.4s
+28° 05′ 49″ | Y0.5  |  | 152.6±2.0[4] | [20][4]
WISE 0410+1502§ | 21.56±0.29 | Taurus* |  04h 10m 22.8s
+15° 02′ 47″ | Y0 |  | 151.3±2.0[4] | [21][4]
WISE J0521+1025§  | 21.71±0.44  | Orion |  05h 21m 26.4s
+10° 25′ 27″ | T7.5  |  | 150.2±3.0[4] | [4]
GJ 3737 (LHS 337, L 471-42) | 21.7324±0.0047 | Centaurus |  12h 38m 49.1s
−38° 22′ 53″ | M4.5V: | 12.74 | 150.0781±0.0322[1] | [12]
Gliese 408 (Ross 104) | 22.0081±0.0038 | Leo |  11h 00m 04.3s
+22° 49′ 59″ | M3.0V | 10.02 | 148.1986±0.0253[1] |
Xi Boötis | A$ | 22.0109±0.0081 | Boötes |  14h 51m 23.4s
+19° 06′ 02″ | G8Ve | 4.70# | 148.1793±0.0546[1] | BY Draconis variable
B$ | K4Ve | 6.97
Gliese 299 (Ross 619) | 22.079±0.014 | Cancer |  08h 11m 57.6s
+08° 46′ 22″ | M4.5V | 12.83 | 147.7218±0.0950[1] |
GJ 3522 (G 41-14) | A | 22.08±0.30 | Cancer |  08h 58m 56.3s
+08° 28′ 26″ | M3.5V | 10.92 | 147.66±1.98[12] |
B | M
C | M
Gliese 829 (Ross 775) | A | 22.1129±0.0039 | Pegasus |  21h 29m 36.8s
+17° 38′ 36″ | M3+M | 10.30 | 147.4958±0.0257[1] |
B | M
Scholz's Star | A  | 22.17±0.18  | Monoceros |  07h 20m 03.3s
−08° 46′ 50″ | M9.5  | 18.3  | 147.1±1.2[22] | passed through the Solar System's Oort Cloud 70,000 years ago
B§  | T5.5  |
WISE 1928+2356§ | 22.28±0.18 | Vulpecula* |  19h 28m 41.5s
+23° 56′ 02″ | T6 |  | 146.4067±1.2001[1] | [4]
WISE J0254+0223§  | 22.32±0.23  | Cetus  |  02h 54m 09.6s
+02° 23′ 59″ | T8  |  | 146.1±1.5[23] | [4]
LTT 1445 (BD-17 588) | A | 22.3867±0.0037 | Eridanus |  03h 01m 51.4s
−16° 35′ 36″ | M3.0 | 11.22 | 145.6922±0.0244[1] | has 2-3 known planets orbiting star A[24][25]
B | M3.5 | 11.37
C | M
Gliese 880 (HD 216899) | 22.3973±0.0039 | Pegasus |  22h 56m 34.8s
+16° 33′ 12″ | M2.0V | 8.64 | 145.6234±0.0254[1] | has 1 candidate planet [3]
CWISE J1055+5443§  | 22.5+2.6−2.0 | Ursa Major |  10h 55m 12.1s
+54° 43′ 28″ | Y0 (pec)  |  | 145.0±14.7[4] | possibly a young low mass object (4−6 MJ)[26]
Gliese 402 (EE Leonis, Wolf 358) | 22.7225±0.0045 | Leo |  10h 50m 52.0s
+06° 48′ 29.2″ | M5.0V | 11.68 | 143.5391±0.0286[1] | BY Draconis variable; member of the Hercules-Lyra association
Gliese 393 (BD+01 2447) | 22.9534±0.0034 | Sextans |  10h 28m 55.6s
+00° 50′ 28″ | M2.5V | 9.65 | 142.0951±0.0212[1] | Member of the AB Doradus moving group; has 1 known planet
Gliese 809 (HD 199305) | 22.9600±0.0026 | Cepheus |  20h 53m 19.8s
+62° 09′ 16″ | M2.0V | 8.60 | 142.0543±0.0160[1] |
LSPM J2146+3813 (UCAC4 642-113039) | 22.9858±0.0034 | Cygnus |  21h 46m 22.1s
+38° 13′ 05″ | M5V |  | 141.8946±0.0212[1] |
LHS 3003 (GJ 3877, LP 914-54) | 23.003±0.010 | Hydra |  14h 56m 38.3s
−28° 09′ 47″ | M7.0V | 17.14 | 141.7891±0.0617[1] | [27]
WISE 2056+1459§ | 23.16±0.33 | Delphinus* |  20h 56m 28.9s
+14° 59′ 54″ | Y0 |  | 140.8±2.0[4] | [4]
GJ 1068 (L 230-188) | 23.1816±0.0035 | Dorado* |  04h 10m 28.1s
−53° 36′ 08″ | M4.5 | 13.58 | 140.6961±0.0214[1] |
WISE J004945.61+215120.0§ | 23.23±0.35 | Andromeda |  00h 49m 45.6s
+21° 51′ 20″ | T8.5 |  | 140.4±2.1[4] | [4]
GJ 1286 (G 157-77) | 23.4074±0.0074 | Pisces |  23h 35m 10.5s
−02° 23′ 21″ | M5.5V | 14.69 | 139.3389±0.0441[1] |
Gliese 105 (268 G. Ceti, HD 16160) | A$ | 23.5599±0.0071 | Cetus |  02h 36m 04.9s
+06° 53′ 13″ | K3V | 5.82# | 138.4371±0.0420[1] | star B is a BY Draconis variable
B | M4.5V | 11.66
C | M6V | 16.9
2MASS J08354256-0819237§  | 23.581±0.037  | Hydra |  08h 35m 42.6s
−08° 19′ 24″ | L5  |  | 138.3147±0.2145[1] | [4]
GJ 4274 (L 788-34) | 23.5955±0.0082 | Aquarius |  22h 23m 07.0s
−17° 36′ 26″ | M4.5Ve | 13.30 | 138.2280±0.0482[1] | [28]
Gliese 667 (142 G. Scorpii) | A$ | 23.6232±0.0048 | Scorpius |  17h 18m 57.2s
−34° 59′ 23″ | K3V | 7.07 | 138.0663±0.0283[1] | star C has 2 known planets
B$ | K5V | 8.02
C | M1.5V | 11.03
WISE 0607+2429§ | 23.624±0.089 | Gemini |  06h 07m 38.7s
+24° 29′ 54″ | L8 | 14.22 ± 0.03 (J) | 138.0616±0.5185[1] | [1]
WISE 0313+7807§ | 24.05±0.51 | Cepheus |  03h 13m 26.0s
+78° 07′ 44″ | T8.5 |  | 135.6±2.8[4] | [4]
2MASS 1507-1627§ | 24.169±0.047 | Libra |  15h 07m 47.7s
−16° 27′ 389″ | L5.5 | 22.14 | 134.9474±0.2611[1] | [4]
HD 4628 (96 G. Piscium, Gliese 33)$ | 24.250±0.010 | Pisces |  00h 48m 23.0s
+05° 16′ 50″ | K2.5V | 5.75# | 134.4948±0.0578[1] |
Beta Hydri$ | 24.327±0.020 | Hydrus* |  00h 25m 45.1s
–77° 15′ 15″ | G2IV | 2.79# | 134.07±0.11[29] |
WISE J2000+3629§  | 24.45±0.41  | Cygnus |  20h 00m 50.2s
+36° 29′ 50″ | T8  |  | 133.4±2.2[4] | [4]
GJ 3991 (G 203-47) | A | 24.784±0.081 | Hercules |  17h 09m 32.0s
+43° 40′ 49″ | M3.5V | 13.671 | 131.5996±0.4285[1] |
B | D? |
Alpha Piscis Austrini | B (TW PsA)$ | 24.7929±0.0052 | Piscis Austrinus |  22h 56m 24.17s
−31° 33′ 56″ | K5Vp | 6.48# | 131.5525±0.0275[1] | component B of triple system
107 Piscium$ | 24.805±0.029 | Pisces |  01h 42m 29.8s
+20° 16′ 07″ | K1V | 5.24# | 131.4903±0.1515[30] |
G 141-36 | 24.8445±0.0075 | Aquila |  18h 48m 17.5s
+07° 41′ 21″ | M6V |  | 131.2790±0.0398[1] |
Gliese 514 (BD+11 2576) | 24.8782±0.0051 | Virgo |  13h 29m 59.8s
+10° 22′ 38″ | M1.0V | 9.02 | 131.1013±0.0270[1] | has 1 known planet
WISE 1738+2732§  | 24.92±0.41  | Hercules |  17h 38m 35.5s
+27° 32′ 59″ | Y0  |  | 130.9±2.1[4] | [4]
GJ 4053 (G 258-33) | 24.9254±0.0041 | Draco |  18h 18m 57.2s
+66° 11′ 33″ | M4.5V | 13.46 | 130.8531±0.0217[1] |
WISE J2354+0240§  | 24.97±0.65  | Pisces |  23h 54m 02.8s
+02° 40′ 14″ | Y1  |  | 130.6±3.3[4] | [4]
System  | Star or
(sub-) brown dwarf | Distance (ly) | Constellation | Coordinates:
RA, Dec
(Ep J2000, Eq J2000) | Stellar
class | Apparent magnitude
(V) | Parallax
(mas) | Notes and additional references

## See also

* List of nearest stars
* List of star systems within 25–30 light-years
* Lists of stars
* List of nearest bright stars

## References

1. ↑ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 1.10 1.11 1.12 1.13 1.14 1.15 1.16 1.17 1.18 1.19 1.20 1.21 1.22 1.23 1.24 1.25 1.26 1.27 1.28 1.29 1.30 1.31 1.32 1.33 1.34 1.35 1.36 1.37 1.38 1.39 1.40 1.41 1.42 Brown, A. G. A. (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics 649: A1. doi:10.1051/0004-6361/202039657. Bibcode: 2021A&A...649A...1G.
2. ↑ van Leeuwen, F. (2007). "HIP 99701". Validation of the new Hipparcos reduction. http://webviz.u-strasbg.fr/viz-bin/VizieR-5?-source=I/311&HIP=99701.
3. ↑ 3.0 3.1 Barnes, J. R.; et al. (2019-06-11). "Frequency of planets orbiting M dwarfs in the Solar neighbourhood". arXiv:1906.04644 [astro-ph.EP].
4. ↑ 4.00 4.01 4.02 4.03 4.04 4.05 4.06 4.07 4.08 4.09 4.10 4.11 4.12 4.13 4.14 4.15 4.16 4.17 4.18 4.19 4.20 4.21 4.22 4.23 4.24 4.25 4.26 Cite error: Invalid `<ref>` tag; no text was provided for refs named `:0`
5. ↑ Jao, Wei-Chun; Henry, Todd J.; Subasavage, John P.; Brown, Misty A.; Ianna, Philip A.; Bartlett, Jennifer L.; Costa, Edgardo; Méndez, René A. (April 2005). "The Solar Neighborhood. XIII. Parallax Results from the CTIOPI 0.9 Meter Program: Stars with μ ≥ 1."0 yr (MOTION Sample)". The Astronomical Journal 129 (4): 1954–1967. doi:10.1086/428489. Bibcode: 2005AJ....129.1954J.
6. ↑ van Leeuwen, F. (2007). "HIP 116132". Validation of the new Hipparcos reduction. http://webviz.u-strasbg.fr/viz-bin/VizieR-5?-source=I/311&HIP=116132.
7. ↑ Curiel, Salvador; Ortiz-León, Gisela N.; Mioduszewski, Amy J.; Sanchez-Bermudez, Joel (31 May 2022). "3D Orbital Architecture of a Dwarf Binary System and Its Planetary Companion". The Astronomical Journal 164:93 (3): 23pp. 1 September 2022. doi:10.3847/1538-3881/ac7c66. Bibcode: 2022AJ....164...93C.
8. ↑ von Braun, Kaspar; Boyajian, Tabetha S.; Kane, Stephen R.; van Belle, Gerard T.; Ciardi, David R.; López-Morales, Mercedes; McAlister, Harold A.; Henry, Todd J. et al. (10 March 2011). "Astrophysical Parameters and Habitable Zone of the Exoplanet Hosting Star Gj 581". The Astrophysical Journal 729 (2): L26. doi:10.1088/2041-8205/729/2/L26. Bibcode: 2011ApJ...729L..26V.
9. ↑ Robertson, Paul et al. (3 July 2014). "Stellar activity masquerading as planets in the habitable zone of the M dwarf Gliese 581". Science 345 (6195): 440–444. doi:10.1126/science.1253253. PMID 24993348. Bibcode: 2014Sci...345..440R.
10. ↑ Gliese, W.; Jahreiß, H. (1991). "GI 338". Preliminary Version of the Third Catalogue of Nearby Stars. http://webviz.u-strasbg.fr/viz-bin/VizieR-5?-source=V/70A&Name=Gl 338.
11. ↑ González-Álvarez, E.; Osorio, M. R. Zapatero; Caballero, J. A.; Sanz-Forcada, J.; Béjar, V. J. S.; González-Cuesta, L.; Dreizler, S.; Bauer, F. F. et al. (May 2020). "The CARMENES search for exoplanets around M dwarfs. A super-Earth planet orbiting HD 79211 (GJ 338 B)". Astronomy & Astrophysics 637: A93. doi:10.1051/0004-6361/201937050. ISSN 0004-6361. Bibcode: 2020A&A...637A..93G.
12. ↑ 12.0 12.1 12.2 Henry, Todd J.; Jao, Wei-Chun; Subasavage, John P.; Beaulieu, Thomas D.; Ianna, Philip A.; Costa, Edgardo; Méndez, René A. (January 2006). "The Solar Neighborhood. XVII. Parallax Results from the CTIOPI 0.9 m Program: 20 New Members of the RECONS 10 Parsec Sample". The Astronomical Journal 132 (6): 2360–2371. doi:10.1086/508233. Bibcode: 2006AJ....132.2360H. http://repositorio.uchile.cl/bitstream/2250/126230/1/Henry_Todd.pdf.
13. ↑ 13.0 13.1 Söderhjelm, Staffan (1999). "HIP 84140". Visual binary orbits and masses post Hipparcos. http://webviz.u-strasbg.fr/viz-bin/VizieR-5?-source=J/A+A/341/121&HIP=84140.
14. ↑ Dupuy, Trent J.; Liu, Michael C. (1 August 2012). "The Hawaii Infrared Parallax Program. I. Ultracool Binaries and the L/T Transition". The Astrophysical Journal Supplement Series 201 (2): 19. doi:10.1088/0067-0049/201/2/19. Bibcode: 2012ApJS..201...19D.
15. ↑ 15.0 15.1 Lurie, John C.; Henry, Todd J.; Jao, Wei-Chun; Quinn, Samuel N.; Winters, Jennifer G.; Ianna, Philip A.; Koerner, David W.; Riedel, Adric R. et al. (13 October 2014). "The Solar Neighborhood. XXXIV. A Search for Planets Orbiting Nearby M Dwarfs Using Astrometry". The Astronomical Journal 148 (5): 91. doi:10.1088/0004-6256/148/5/91. Bibcode: 2014AJ....148...91L.
16. ↑ van Leeuwen, F. (2007). "HIP 80459". Validation of the new Hipparcos reduction. http://webviz.u-strasbg.fr/viz-bin/VizieR-5?-source=I/311&HIP=80459.
17. ↑ Suárez Mascareño, A.; González Hernández, J. I.; Rebolo, R.; Velasco, S.; Toledo-Padrón, B.; Affer, L.; Perger, M.; Micela, G. et al. (2017). "HADES RV Programme with HARPS-N at TNG". Astronomy & Astrophysics 605: A92. doi:10.1051/0004-6361/201730957. Bibcode: 2017A&A...605A..92S.
18. ↑ VizieR, Yale Trigonometric Parallaxes, Fourth Edition (van Altena+ 1995)
19. ↑ HD 219134 PLANET HOST OVERVIEW PAGE
20. ↑ Schneider, Adam C.; Cushing, Michael C.; Kirkpatrick, J. Davy; Gelino, Christopher R.; Mace, Gregory N.; Wright, Edward L.; Eisenhardt, Peter R.; Skrutskie, M. F. et al. (2015-05-01). "Hubble Space Telescope Spectroscopy of Brown Dwarfs Discovered with the Wide-field Infrared Survey Explorer". The Astrophysical Journal 804 (2): 92. doi:10.1088/0004-637X/804/2/92. ISSN 0004-637X. Bibcode: 2015ApJ...804...92S.
21. ↑ Beichman, C.; Gelino, Christopher R.; Kirkpatrick, J. Davy; Cushing, Michael C.; Dodson-Robinson, Sally; Marley, Mark S.; Morley, Caroline V.; Wright, E. L. (10 March 2014). "Wisey Dwarfs as Probes of the Brown Dwarf-Exoplanet Connection". The Astrophysical Journal 783 (2): 68. doi:10.1088/0004-637X/783/2/68. Bibcode: 2014ApJ...783...68B.
22. ↑ Wizinowich, Peter; Wetherell, Ed; Ragland, Sam; Mawet, Dimitri; Lilley, Scott; Jovanovic, Nemanja; Delorme, Jacques-Robert; Chun, Mark et al. (19 August 2019). "WISE J072003.20-084651.2B Is A Massive T Dwarf" (in en). The Astronomical Journal 158 (5): 174. doi:10.3847/1538-3881/ab3cd1. Bibcode: 2019AJ....158..174D.
23. ↑ Kirkpatrick, J. Davy et al. (February 2019). "Preliminary Trigonometric Parallaxes of 184 Late-T and Y Dwarfs and an Analysis of the Field Substellar Mass Function into the "Planetary" Mass Regime". The Astrophysical Journal Supplement Series 240 (2): 69. doi:10.3847/1538-4365/aaf6af. 19. Bibcode: 2019ApJS..240...19K.
24. ↑ Almenara, Jose-Manuel et al. (2019-06-24). "Three Red Suns in the Sky: A Transiting, Terrestrial Planet in a Triple M Dwarf System at 6.9 Parsecs" (in en). The Astronomical Journal 158 (152). doi:10.3847/1538-3881/ab364d. Bibcode: 2019AJ....158..152W.
25. ↑ "Gj 3192". http://simbad.u-strasbg.fr/simbad/sim-id?Ident=GJ+3192&submit=submit+id.
26. ↑ Robbins, Grady; Meisner, Aaron M.; Schneider, Adam C.; Burgasser, Adam J.; Kirkpatrick, J. Davy; Gagné, Jonathan; Hsu, Chih-Chun; Moranta, Leslie et al. (2023-11-01). "CWISE J105512.11+544328.3: A Nearby Y Dwarf Spectroscopically Confirmed with Keck/NIRES". The Astrophysical Journal 958 (1): 94. doi:10.3847/1538-4357/ad0043. ISSN 0004-637X. Bibcode: 2023ApJ...958...94R.
27. ↑ Dahn, Conard C.; Harris, Hugh C.; Vrba, Frederick J.; Guetter, Harry H.; Canzian, Blaise; Henden, Arne A.; Levine, Stephen E.; Luginbuhl, Christian B. et al. (August 2002). "Astrometry and Photometry for Cool Dwarfs and Brown Dwarfs". The Astronomical Journal 124 (2): 1170–1189. doi:10.1086/341646. Bibcode: 2002AJ....124.1170D.
28. ↑ Bobylev, V. V. (2017). "Search for close stellar encounters with the solar system from data on nearby dwarfs". Astronomy Reports 61 (10): 883–890. doi:10.1134/S106377291710002X. ISSN 1063-7729. Bibcode: 2017ARep...61..883B.
29. ↑ van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics 474 (2): 653–664, doi:10.1051/0004-6361:20078357, Bibcode: 2007A&A...474..653V
30. ↑ Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G.

* v
* t
* e

Stars

Formation|

* Accretion
* Molecular cloud
* Bok globule
* Young stellar object
* Protostar
* Pre-main-sequence
* Herbig Ae/Be
* T Tauri
* FU Orionis
* Herbig–Haro object
* Hayashi track
* Henyey track

Evolution|

* Main sequence
* Red-giant branch
* Horizontal branch
* Red clump
* Asymptotic giant branch
* Blue loop
* Protoplanetary nebula
* Planetary nebula
* PG1159
* Dredge-up
* Instability strip
* Luminous blue variable
* Blue straggler
* Stellar population
* Supernova
* Superluminous supernova / Hypernova

Spectral
classification|

* Early
* Late
* Main sequence
* O
* B
* A
* F
* G
* K
* M
* Brown dwarf
* WR
* OB
* Subdwarf
* O
* B
* Subgiant
* Giant
* Blue
* Red
* Yellow
* Bright giant
* Supergiant
* Blue
* Red
* Yellow
* Hypergiant
* Yellow
* Carbon
* S
* CN
* CH
* White dwarf
* Chemically peculiar
* Am
* Ap/Bp
* HgMn
* Helium-weak
* Barium
* Extreme helium
* Lambda Boötis
* Lead
* Technetium
* Be
* Shell
* B[e]

Remnants|

* White dwarf
* Helium planet
* Black dwarf
* Neutron
* Radio-quiet
* Pulsar
* Binary
* X-ray
* Magnetar
* Stellar black hole
* X-ray binary
* Burster

Hypothetical|

* Blue dwarf
* Green
* Black dwarf
* Exotic
* Boson
* Electroweak
* Strange
* Preon
* Planck
* Dark
* Dark-energy
* Quark
* Q
* Black
* Gravastar
* Frozen
* Quasi-star
* Thorne–Żytkow object
* Iron
* Blitzar

Stellar
nucleosynthesis|

* Deuterium burning
* Lithium burning
* Proton–proton chain
* CNO cycle
* Helium flash
* Triple-alpha process
* Alpha process
* Carbon burning
* Neon burning
* Oxygen burning
* Silicon burning
* S-process
* R-process
* Fusor
* Nova
* Symbiotic
* Remnant
* Luminous red nova

Structure|

* Core
* Convection zone
* Microturbulence
* Oscillations
* Radiation zone
* Atmosphere
* Photosphere
* Starspot
* Chromosphere
* Corona
* Stellar wind
* Bubble
* Bipolar outflow
* Accretion disk
* Asteroseismology
* Helioseismology
* Eddington luminosity
* Kelvin–Helmholtz mechanism

Properties|

* Designation
* Dynamics
* Effective temperature
* Luminosity
* Kinematics
* Magnetic field
* Absolute magnitude
* Mass
* Metallicity
* Rotation
* Starlight
* Variable
* Photometric system
* Color index
* Hertzsprung–Russell diagram
* Color–color diagram

Star systems|

* Binary
* Contact
* Common envelope
* Eclipsing
* Symbiotic
* Multiple
* Cluster
* Open
* Globular
* Super
* Planetary system

Earth-centric
observations|

* Sun
* Solar System
* Sunlight
* Pole star
* Circumpolar
* Constellation
* Asterism
* Magnitude
* Apparent
* Extinction
* Photographic
* Radial velocity
* Proper motion
* Parallax
* Photometric-standard

Lists|

* Proper names
* Arabic
* Chinese
* Extremes
* Most massive
* Highest temperature
* Largest volume
* Smallest volume
* Brightest
* Historical
* Most luminous
* Nearest
* Nearest bright
* With exoplanets
* Brown dwarfs
* White dwarfs
* Milky Way novae
* Supernovae
* Candidates
* Remnants
* Planetary nebulae
* Timeline of stellar astronomy

Related articles|

* Substellar object
* Brown dwarf
* Sub-brown dwarf
* Planet
* Galactic year
* Galaxy
* Guest
* Gravity
* Intergalactic
* Starfield
* Tidal disruption event

'Category:Stars * '

* v
* t
* e

List of star systems within 500 light-years

* 0–20
* 20–25
* 25–30
* 30–35
* 35–40
* 40–45
* 45–50
* 50–55
* 55–60
* 60–65
* 65–70
* 70–75
* 75–80
* 80–85
* 85–90
* 90–95
* 95–100
* 100–150
* 150–200
* 200–250
* 250–300
* 300–350
* 350–400
* 400–450
* 450–500

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Original source: https://en.wikipedia.org/wiki/List of star systems within 20–25 light-years. Read more

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