List of star systems within 20–25 light-years

This is a list of star systems within 20–25 light years of Earth.

Star system Median distance (ly) Parallax (mas) Stars in system Spectral type Apparent magnitude (V) Comments and references
ADS 7251 20.09 162.5±2.00 2 M0V+K7V 6.92 [1]
EQ Pegasi 20.16 161.76±1.66 2 M3.5V+M4.5V 10.17 (10.35/12.4) [2] both components are flare stars
Gliese 784 20.21 161.34±1.00 1 M0V 7.97 [3]
Gliese 581 20.22 160.12±1.33 1 M5.0V 10.56–10.58 [4] BY Draconis variable; has 4 known planets
WISE 0410+1502 20.4 160±9 1 Y0 [5]
WISE 0146+4234 20.5 1 Y0 [6]
HN Librae 20.60 158.46±2.62 1 M4.0V 10.3–10.33 [7] BY Draconis variable
2MASS 1503+2525 20.74 157.2±2.2 1 T5.5 [8]
LHS 3003 20.76 157.0±3.0 1 M7.0V 17.14 [9]
LHS 2090 20.78 156.87±2.68 1 M6.5V 16.10 [10]
LHS 337 20.79 156.78±1.99 1 M4.5V: 12.74 [10]
Furuhjelm 46 20.82 156.66±1.37 2 M3V+M 9.35 [11]
LP 658-2 20.88 156.13±0.84 1 DZ11 14.45
SIMP J013656.5+093347 20.9 1 T2.5 [12]
LP 944-20 20.91 155.89±1.03 1 M9V 18.69 [13]
V1054 Ophiuchi 21.07 154.8±0.6 5 M3.5Ve+M4.5Ve+M4.5Ve
+M4VI+M7V 		9.02/11.76/16.92 [14] components Ab and Ac are flare stars
GJ 1128 21.13 154.27±0.76 1 M4.0V 12.78 [13]
LP 71-82 21.2 1 M6.1V 13.51 [6]
AC 54 1646-56 21.24 153.46±0.99 1 M2.0V 10.17 [15]
G 161-71 21.3 1 M5 13.65 [6]
WISE 0313+7807 21.3 1 T8.5
G 12-30 21.32 152.9±2 1 M5Ve 13.79 flare star
HR 8832 21.35 152.76±0.29 1 K3V 5.574 [16] has 4 known planets
Ross 775 21.72 15.010±1.70 2 M3.0V+M 10.02
LSPM J2146+3813 21.80 1 M5V
Xi Boötis 21.89 148.98±0.48 2 G8Ve+K4Ve 4.52–4.67 BY Draconis variable
Ross 775 21.86 149.15±1.81 2 M3+M 10.30
SCR J1546−5534 21.9 1 M7.5
Gliese 299 22.0 148±2.6 1 M4.5V 12.83
EE Leonis 22.04 147.92±3.52 1 M5.0V 11.68 BY Draconis variable; member of the Hercules-Lyra association
G 41-14 22.08 147.66±1.98 3 M3.5V+M+M 10.92
WISE J2209+2711 22.2 147±11 1 Y0
Gliese 880 22.31 146.09±1.00 2 M2.0V+M 8.64
BD-17 588 22.7 3 M3.0+M3.5+M 10.40
GJ 1068 22.7 1 M4.5 13.58
L 369-44 22.8 2 M5+M 12.67
2MASS J18522528-3730363 22.8 1 M4.5
G 161-7 22.8 2 M5+M5 13.76
WISE 1928+2356 22.8 2 T6
HD 199305 22.98 141.87±0.65 2 M2.0V+M 8.60
Gliese 393 23.04 141.50±2.22 1 M2.5V 9.65 Member of the AB Doradus moving group
WISE 0713−2917 23.2 1 Y0
WISE J000517.48+373720.5 23.2 1 T9
WISE 2056+1459 23.3 140±9 1 Y0
G 141-36 23.4 1 M6V
Gliese 105 23.42 139.27±0.45 3 K3V+M4.5V+M6V 5.82/11.66/16.9 star B is a BY Draconis variable
SCR J0740−4257 23[17] 1 M4.5 13.81
L 43-72 23.5 1 M4.5
GJ 1286 23.57 138.3±3.5 1 M5.5V 14.69
Gliese 667 23.62 146.29±9.03 3 K3V+K5V+M1.5V 5.89 star C has 2 known planets
GJ 4063 23.6 138±40 1 M4V 11.75
GJ 4053 23.74 137.3±5.3 1 M4.5V 13.46
2MASS 1507-1627 23.90 136.40±0.60 1 L5.5 22.14
WISE J004945.61+215120.0 24.1 1 T8.5
GJ 3991 24.27 134.31±1.99 2 M3.5V+M 11.78
GJ 4248 24.28 134.29±1.31 1 M3.5 11.80
HD 4628 24.31 134.14±0.51 1 K2.5V 5.75
GJ 4274 24.31 134.1±5.6 1 M4 13.30
Beta Hydri 24.32 134.07±0.11 1 G2IV 2.79
VX Arietis 24.48 133.16±2.26 1 M3.5V 10.56 flare star
107 Piscium 24.57 132.76±0.50 1 K1V 5.24
GJ 1224 24.59 132.6±3.7 1 M4.5V 13.48
Mu Cassiopeiae 24.63 132.38±0.82 2 G5VIp+M5V 5.17
Gliese 514 24.96 130.62±1.05 1 M1.0V 9.02

See also

References

  1. ↑ Gliese, W.; Jahreiß, H. (1991). "GI 338". Preliminary Version of the Third Catalogue of Nearby Stars.
  2. ↑ van Leeuwen, F. (2007). "HIP 116132". Validation of the new Hipparcos reduction.
  3. ↑ van Leeuwen, F. (2007). "HIP 99701". Validation of the new Hipparcos reduction.
  4. ↑ 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.; Jao, Wei-Chun; Riedel, Adric R.; Subasavage, John P.; Schaefer, Gail; ten Brummelaar, Theo A.; Ridgway, Stephen; Sturmann, Laszlo; Sturmann, Judit; Mazingue, Jude; Turner, Nils H.; Farrington, Chris; Goldfinger, P. J.; Boden, Andrew F. (10 March 2011). "ASTROPHYSICAL PARAMETERS AND HABITABLE ZONE OF THE EXOPLANET HOSTING STAR GJ 581". The Astrophysical Journal. 729 (2): L26. arXiv:1102.0237Freely accessible. Bibcode:2011ApJ...729L..26V. doi:10.1088/2041-8205/729/2/L26.
  5. ↑ 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). "Y DWARFS AS PROBES OF THE BROWN DWARF-EXOPLANET CONNECTION". The Astrophysical Journal. 783 (2): 68. arXiv:1401.1194Freely accessible. Bibcode:2014ApJ...783...68B. doi:10.1088/0004-637X/783/2/68.
  6. 1 2 3 Davy Kirkpatrick, J.; Gelino, Christopher R.; Cushing, Michael C.; Mace, Gregory N.; Griffith, Roger L.; Skrutskie, Michael F.; Marsh, Kenneth A.; Wright, Edward L.; Eisenhardt, Peter R.; McLean, Ian S.; Mainzer, Amanda K.; Burgasser, Adam J.; Tinney, C. G.; Parker, Stephen; Salter, Graeme (10 July 2012). "FURTHER DEFINING SPECTRAL TYPE "Y" AND EXPLORING THE LOW-MASS END OF THE FIELD BROWN DWARF MASS FUNCTION". The Astrophysical Journal. 753 (2): 156. arXiv:1205.2122Freely accessible. Bibcode:2012ApJ...753..156K. doi:10.1088/0004-637X/753/2/156.
  7. ↑ 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. arXiv:astro-ph/0502167Freely accessible. Bibcode:2005AJ....129.1954J. doi:10.1086/428489.
  8. ↑ 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. arXiv:1201.2465Freely accessible. Bibcode:2012ApJS..201...19D. doi:10.1088/0067-0049/201/2/19.
  9. ↑ Dahn, Conard C.; Harris, Hugh C.; Vrba, Frederick J.; Guetter, Harry H.; Canzian, Blaise; Henden, Arne A.; Levine, Stephen E.; Luginbuhl, Christian B.; Monet, Alice K. B.; Monet, David G.; Pier, Jeffrey R.; Stone, Ronald C.; Walker, Richard L.; Burgasser, Adam J.; Gizis, John E.; Kirkpatrick, J. Davy; Liebert, James; Reid, I. Neill (August 2002). "Astrometry and Photometry for Cool Dwarfs and Brown Dwarfs". The Astronomical Journal. 124 (2): 1170–1189. arXiv:astro-ph/0205050Freely accessible. Bibcode:2002AJ....124.1170D. doi:10.1086/341646.
  10. 1 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. arXiv:astro-ph/0608230Freely accessible. Bibcode:2006AJ....132.2360H. doi:10.1086/508233.
  11. ↑ Söderhjelm, Staffan (1999). "HIP 84140". Visual binary orbits and masses post Hipparcos.
  12. ↑ Artigau et al.: "Discovery of the Brightest T Dwarf in the Northern Hemisphere"; in: The Astrophysical Journal, Bd. 651, Nr. 1, S. L57-L60 (2006)
  13. 1 2 Lurie, John C.; Henry, Todd J.; Jao, Wei-Chun; Quinn, Samuel N.; Winters, Jennifer G.; Ianna, Philip A.; Koerner, David W.; Riedel, Adric R.; Subasavage, John P. (13 October 2014). "THE SOLAR NEIGHBORHOOD. XXXIV. A SEARCH FOR PLANETS ORBITING NEARBY M DWARFS USING ASTROMETRY". The Astronomical Journal. 148 (5): 91. arXiv:1407.4820Freely accessible. Bibcode:2014AJ....148...91L. doi:10.1088/0004-6256/148/5/91.
  14. ↑ VizieR, Yale Trigonometric Parallaxes, Fourth Edition (van Altena+ 1995)
  15. ↑ van Leeuwen, F. (2007). "HIP 80459". Validation of the new Hipparcos reduction.
  16. ↑ HD 219134 PLANET HOST OVERVIEW PAGE
  17. ↑ The AstraLux Large M-dwarf Multiplicity Survey
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