List of star systems within 60–65 light-years

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This is a list of star systems within 60-65 light years of Earth.

Star system  | Median distance (ly)  | Stars in system  | Spectral type | Apparent magnitude (V)  | Comments and references

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Delta Equulei «Pherasauval» | 60.0 ± 1.0 | 2 | F5V + G0 | 4.49/5.4 | [1]
HD 53143 | 60.0 ± 0.6 | 1 | K9V | 6.80 | [2][3]
15 Leonis Minoris | 60.1 ± 0.8 | 1 | G0V | 5.12 | [4][5]
Gliese 339 | 60.1 ± 1.3 | 2 | KV |  |
Gliese 161 | 60.2 ± 0.9 | 1 | GV |  |
Gliese 2102 | 60.2 ± 1.2 | 1 | KV |  |
Gliese 4134 | 60.4 +9.0−6.9 | 1 | KV |  |
Gliese 315 | 60.4 ± 1.2 | 1 | KV |  |
Gliese 509 | 60.4 ± 2.5 | 2 | KV |  |
HD 156985 | 60.4 ± 0.8 | 1 | KV |  |
G 185-32 | 60.4 +3.5−3.2 | 1 | DA4.0 | 13.00 | [6][7]
Gliese 610 | 60.5 ± 1.5 | 1 | KV |  |
Gliese 106 | 60.5 ± 2.8 | 1 | KV |  |
HR 244 | 60.6 ± 0.7 | 1 | F9V | 4.82 | [8]
Theta Cygni | 60.7 ± 0.5 | 2 | F3V + M3V | 4.490/13.03 | [9][10][11][12]
Gliese 499 | 60.7 ± 2.2 | 2 | KV |  |
WISE 2301+0216 | 60.7 | 1 | T6.5 |  |
Gliese 254 | 60.8 ± 2.0 | 1 | KV |  |
Theta Centauri «Menkent» | 60.9 ± 0.9 | 1 | K0III | 2.06 | [4][13]
Mu Virginis | 60.9 ± 1.1 | 1 | F2IV | 3.88 | [4][5]
HD 152606 | 60.9 ± 1.0 | 1 | KV |  |
Gliese 902.1 | 60.9 ± 1.3 | 1 | KV |  |
Kelu-1 | 60.9 ± 2.3 | 3 | L2 + L4 |  | [14]
Gliese 1094 | 61.0 ± 2.3 | 1 | KV |  |
HR 8061 | 61.1 ± 2.6 | 3 | FV |  |
Tau Piscis Austrini | 61.1 ± 1.0 | 1 | F6V | 4.94 |
HR 8148 | 61.1 ± 1.3 | 2 | GV |  |
HD 206804 | 61.1 ± 1.9 | 2 | KV |  |
Gliese 715 | 61.2 ± 1.2 | 1 | KV |  |
WISE 0150+3827 | 61.3 | 1 | T0 |  |
HD 4747 | 61.4 ± 1.2 | 2 | G8V | 7.30 |
Gliese 249 | 61.4 ± 1.4 | 1 | KV |  |
Gliese 296 | 61.5 ± 9.7 | 1 | KV |  |
HD 170573 | 61.5 ± 9.7 | 1 | KV |  |
Gliese 1054 | 61.55 ± 0.85 | 1 | M1Ve |  |
6 Ceti | 61.6 ± 0.9 | 1 | F8V | 4.89 | [15]
HR 7683 | 61.6 ± 0.6 | 2 | GIV |  |
Gliese 583 | 61.6 ± 1.8 | 1 | KV |  |
Gliese 4287 | 61.6 ± 2.3 | 2 | KV |  |
Gliese 773 | 61.6 ± 1.8 | 2 | KV |  |
WISE 2157+2659 | 61.6 | 1 | T7 |  |
Gliese 100 | 61.7 ± 2.3 | 3 | KV |  |
Eta Serpentis «Tang» | 61.8 ± 0.9 | 1 | K0IV | 3.260 | [16][17]
Gliese 689 | 62.0 ± 0.9 | 1 | KV |  |
WISE 1711+3500 | 62.0 ± 9.8 | 2 | T8 |  |
HD 139477 | 62.2 ± 0.9 | 1 | KV |  |
110 Herculis | 62.3 ± 0.8 | 1 | F6V | 4.20 | [18]
HR 2643 | 62.3 ± 1.0 | 1 | GV |  |
WISE 1721+1117 | 62.3 | 1 | T6 |  |
HR 3625 | 62.4 ± 1.1 | 1 | FV |  |
Gliese 646 | 62.4 ± 2.4 | 3 | KV |  |
Gliese 576 | 62.6 ± 2.5 | 1 | KV |  |
Gliese 1246 | 62.6 ± 1.4 | 1 | KV |  |
ADS 10075 | 62.6 ± 1.4 | 2 | KV |  |
WISE 0049+0441 | 62.6 | 1 | L9 |  |
Rho Puppis «Tureis» | 62.7 ± 0.8 | 1 | F2mF5IIp | 2.78 | [19][20]
HD 25457 | 62.7 ± 0.9 | 1 | FV |  |
Gliese 292.2 | 62.7 ± 2.3 | 1 | GV |  |
Gliese 825.3 | 62.7 ± 1.5 | 1 | KV |  |
Gliese 3546 | 62.7 +11.4−8.4 | 1 | KV |  |
1 Centauri | 62.8 ± 0.9 | 1 | F3IV | 4.23 |
Gliese 1283 | 62.8 ± 1.4 | 1 | KV |  |
HD 189733 | 62.8 ± 1.1 | 2 | K1.5V + M | 7.676 | has 1 known planet[21][22][23]
Beta Pictoris | 62.9 ± 0.6 | 1 | A6V | 3.861 | has 1 known planet[4][24][25]
WISE 0032-4946 | 62.9 | 1 | T8.5 |  |
HD 43587 | 63.0 ± 1.0 | 4 | G0V + M0V + M3.5V + M5V | 5.70 | [26][27][28]
Gliese 710 | '63.0 ± 1.8 | 1 | K7V | 9.69 | [4][29]
Gliese 900 | '63.0 ± 2.2 | 3 | KV |  |
WD 0806-661 | '63.0 ± 2.0 | 2 | DQ4.2 + Y | 13.71 | [30][31][32]
Gliese 775.1 | 63.1 ± 1.0 | 1 | GV |  |
Gliese 1126 | 63.1 ± 1.1 | 2 | KV |  |
Gliese 45 | 63.1 ± 1.3 | 1 | KV |  |
Gliese 816.1 | 63.2 ± 0.9 | 2 | KV |  |
Omicron Aquilae | 63.3 ± 0.9 | 3 | F8V + M3V | 5.11 | [33][34]
Gliese 790 | 63.3 ± 1.0 | 1 | GV |  |
Gliese 9126 | 63.3 +36.4−16.9 | 1 | KV |  |
HD 274255 | 63.3 +4.9−4.3 | 1 | MV |  |
Alpha Chamaeleontis | 63.5 ± 0.6 | 1 | F5V | 4.066 | [35]
HR 6465 | 63.5 ± 1.1 | 1 | GV |  |
Gliese 894.5 | 63.5 ± 1.6 | 1 | KV |  |
Gliese 59 | 63.6 ± 1.1 | 2 | KV |  |
Gliese 571.1 | 63.6 ± 2.3 | 1 | KV |  |
WISE 0812+4021 | 63.6 | 1 | T8 |  |
HD 130004 | 63.7 ± 1.2 | 1 | KV |  |
c Ursae Majoris | 63.8 ± 0.9 | 2 | G0V | 5.20 | [5][36]
Gliese 204.1 | 63.8 ± 0.6 | 1 | GV |  |
HIP 38594 | 63.8 ± 2.0 | 1 | MV |  |
Gliese 3859 | 63.9 ± 0.7 | 1 | GV |  |
74 Orionis | 64.0 ± 1.1 | 1 | FV |  |
Gliese 3383 | 64.0 +8.5−6.7 | 1 | GV |  |
Alpha Trianguli «Mothallah» | 64.1 ± 1.0 | 2 | F5III-F6IV + M | 3.42 | [13][37][38][39]
Eta Crucis | 64.2 ± 0.6 | 2 | F2III | 4.14 | [40]
Gliese 3867 | 64.2 ± 1.3 | 1 | GV |  |
HD 59747 | 64.2 ± 1.7 | 1 | GV |  |
Gliese 906 | 64.2 ± 2.1 | 1 | KV |  |
45 Boötis | 64.3 ± 1.0 | 2 | F5V | 4.93 | [41]
HD 217107 | 64.3 ± 1.0 | 1 | G8IV | 6.17 | has 2 known planets[42]
Gliese 81.2 | 64.3 ± 1.0 | 1 | KV |  |
HD 220140 | 64.4 ± 0.8 | 1 | GV |  |
Gliese 140.1 | 64.4 ± 2.3 | 2 | KV |  |
Gliese 3678 | 64.4 ± 1.5 | 1 | KV |  |
EQ Virginis | 64.5 ± 1.3 | 1 | K5Ve | 9.31 |
Gliese 3634 | 64.5 +2.0−1.9 | 1 | M2.5 | 11.95 | has 1 known planet[43]
DENIS-P J020529.0-115925 | 64.5 +2.0−1.9 | 3 | L5.5 | 17.3 |
Nu² Canis Majoris | 64.7 ± 0.9 | 1 | K1III | 3.95 | has 1 known planet[44]
Gliese 586 | 64.8 ± 1.5 | 3 | KV |  |
Gliese 1164 | 64.8 +4.4−3.9 | 2 | KV |  |
22 Lyncis | 64.9 ± 1.1 | 2 | FV |  |
HD 192263 | 64.9 ± 1.5 | 1 | K2V | 7.79 | has 1 known planet[45]
HD 35112 | 64.9 ± 2.0 | 1 | KV |  |
WISE 0612-3036 | 64.9 | 1 | T6 |  |
WISE 0929+0409 | 64.9 | 1 | T6.5 |  |
HR 3430 | 65.0 ± 1.3 | 2 | GV |  |
Gliese 530 | 65.0 ± 1.1 | 1 | GV |  |
HD 216520 | 65.0 ± 0.8 | 1 | KV |  |

## See also

* Lists of stars
* List of star systems within 55-60 light-years
* List of star systems within 65-70 light-years
* List of nearest stars and brown dwarfs

## References

1. ↑ "Delta Equulei". University of Illinois Astronomy department. http://www.astro.uiuc.edu/~kaler/sow/deltaequ.html.
2. ↑ Torres, C. A. O. et al. (December 2006), "Search for associations containing young stars (SACY). I. Sample and searching method", Astronomy and Astrophysics 460 (3): 695–708, doi:10.1051/0004-6361:20065602, Bibcode: 2006A&A...460..695T
3. ↑ Cousins, A. W. J. (1973), "UBV photometry of some southern stars", Monthly Notes of the Astronomical Society of Southern Africa 32: 11, Bibcode: 1973MNSSA..32...11C
4. ↑ 4.0 4.1 4.2 4.3 4.4 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, doi:10.1086/504637, Bibcode: 2006AJ....132..161G.
5. ↑ 5.0 5.1 5.2 Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", SIMBAD Astronomical Database, Bibcode: 1986EgUBV........0M.
6. ↑ Gianninas, A.; Bergeron, P.; Ruiz, M. T. (2011). "A Spectroscopic Survey and Analysis of Bright, Hydrogen-Rich White Dwarfs". The Astrophysical Journal 743 (2): 138. doi:10.1088/0004-637X/743/2/138. Bibcode: 2011ApJ...743..138G.
7. ↑ VSX (4 January 2010). "PY Vulpeculae". AAVSO Website. American Association of Variable Star Observers. http://www.aavso.org/vsx/index.php?view=detail.top&oid=38498.
8. ↑ "HR 244". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-id?Ident=HR+244&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id.
9. ↑ Eggen, O. J. (1962), "Space-velocity vectors for 3483 stars with proper motion and radial velocity", Royal Observatory Bulletin 51: 79, Bibcode: 1962RGOB...51...79E
10. ↑ Haas, Michael Robert et al. (January 2011), "Public Kepler Data on the Bright Star Theta Cygni", Bulletin of the American Astronomical Society 43: 140.07, Bibcode: 2011AAS...21714007H
11. ↑ Holmberg, J.; Nordstrom, B.; Andersen, J. (July 2009), "The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics", Astronomy and Astrophysics 501 (3): 941–947, doi:10.1051/0004-6361/200811191, Bibcode: 2009A&A...501..941H
12. ↑ Lépine, Sébastien; Shara, Michael M. (March 2005), "A Catalog of Northern Stars with Annual Proper Motions Larger than 0.15" (LSPM-NORTH Catalog)", The Astronomical Journal 129 (3): 1483–1522, doi:10.1086/427854, Bibcode: 2005AJ....129.1483L
13. ↑ 13.0 13.1 Johnson, H. L. et al. (1966). "UBVRIJKL photometry of the bright stars". Communications of the Lunar and Planetary Laboratory 4 (99): 99. Bibcode: 1966CoLPL...4...99J.
14. ↑ Dupuy, Trent J.; Liu, Michael C. (2012). "The Hawaii Infrared Parallax Program. I. Ultracool Binaries and the L/T Transition". The Astrophysical Journal Supplement 201 (2): 19. doi:10.1088/0067-0049/201/2/19. Bibcode: 2012ApJS..201...19D.
15. ↑ SIMBAD, LTT 75 (accessed 7 September 2012)
16. ↑ Frasca, A. et al. (December 2009), "REM near-IR and optical photometric monitoring of pre-main sequence stars in Orion. Rotation periods and starspot parameters", Astronomy and Astrophysics 508 (3): 1313–1330, doi:10.1051/0004-6361/200913327, Bibcode: 2009A&A...508.1313F
17. ↑ Cousins, A. W. J. (1984), "Standardization of Broadband Photometry of Equatorial Standards", South African Astronomical Observatory Circulars 8: 59, Bibcode: 1984SAAOC...8...59C
18. ↑ SIMBAD, 110 Herculis (accessed 22 September 2012)
19. ↑ Rhee, Joseph H. et al. (May 2007), "Characterization of Dusty Debris Disks: The IRAS and Hipparcos Catalogs", The Astrophysical Journal 660 (2): 1556–1571, doi:10.1086/509912, Bibcode: 2007ApJ...660.1556R
20. ↑ Bookmeyer, B. B. et al. (August 1977), "Photoelectric UBV observations of RR Lyrae variable stars. Second list", Revista Mexicana de Astronomía y Astrofísica 2: 235–258, Bibcode: 1977RMxAA...2..235B
21. ↑ "HD 189733". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+189733.
22. ↑ Bakos, Gáspár Á. et al. (2006). "A Stellar Companion in the HD 189733 System with a Known Transiting Extrasolar Planet". The Astrophysical Journal Letters 641 (1): L57–L60. doi:10.1086/503671. Bibcode: 2006ApJ...641L..57B.
23. ↑ "Water vapour found on exoplanet". BBC News. 2007-07-11. http://news.bbc.co.uk/1/hi/sci/tech/6292076.stm.
24. ↑ "* bet Pic—Star". SIMBAD. http://simbad.u-strasbg.fr/simbad/sim-id?protocol=html&Ident=bet+pic.
25. ↑ "Exoplanet Caught on the Move". 2010-06-10. http://www.eso.org/public/news/eso1024/.
26. ↑ A Modern Mean Stellar Color and Effective Temperatures (Teff) # Sequence for O9V-Y0V Dwarf Stars, E. Mamajek, 2011, website
27. ↑ Catala, C. (2006). "Adaptive Optics Observations of the Binary Star HD 43587". The Astronomical Journal 132 (6): 2318–2325. doi:10.1086/508374. Bibcode: 2006AJ....132.2318C.
28. ↑ Pravdo, Stephen H. (2006). "Masses of Astrometrically Discovered and Imaged Binaries: G78-28AB and GJ 231.1BC". The Astrophysical Journal 649 (1): 389–398. doi:10.1086/506192. Bibcode: 2006ApJ...649..389P.
29. ↑ "Gliese 710". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Gliese+710.
30. ↑ Holberg, J. B.; Sion, E. M.; Oswalt, T.; McCook, G. P.; Foran, S.; Subasavage, John P. (2008). "A New Look at the Local White Dwarf Population". The Astronomical Journal 135 (4): 1225–1238. doi:10.1088/0004-6256/135/4/1225. Bibcode: 2008AJ....135.1225H. https://commons.erau.edu/cgi/viewcontent.cgi?article=1948&context=publication.
31. ↑ Rodriguez, David R.; Zuckerman, B.; Melis, Carl; Song, Inseok (2011). "The Ultra Cool Brown Dwarf Companion of WD 0806-661B: Age, Mass, and Formation Mechanism". The Astrophysical Journal Letters 732 (2): L29. doi:10.1088/2041-8205/732/2/L29. Bibcode: 2011ApJ...732L..29R.
32. ↑ Giammichele, N.; Bergeron, P.; Dufour, P. (2012). "Know Your Neighborhood: A Detailed Model Atmosphere Analysis of Nearby White Dwarfs". The Astrophysical Journal Supplement 199 (2): 29. doi:10.1088/0067-0049/199/2/29. Bibcode: 2012ApJS..199...29G.
33. ↑ Raghavan, Deepak et al. (September 2010), "A Survey of Stellar Families: Multiplicity of Solar-type Stars", The Astrophysical Journal Supplement 190 (1): 1–42, doi:10.1088/0067-0049/190/1/1, Bibcode: 2010ApJS..190....1R.
34. ↑ Nicolet, B. (1978), "Photoelectric photometric Catalogue of homogeneous measurements in the UBV System", Astronomy and Astrophysics Supplement Series 34: 1–49, Bibcode: 1978A&AS...34....1N.
35. ↑ "Alf Cha". http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=alf+Cha&submit=SIMBAD+search.
36. ↑ Francis C., Fekel et al. (February 2015), "New Precision Orbits of Bright Double-Lined Spectroscopic Binaries. IX. HD 54371, HR 2692, and 16 Ursa Majoris", The Astronomical Journal 149 (2): 13, doi:10.1088/0004-6256/149/2/63, 63, Bibcode: 2015AJ....149...63F.
37. ↑ Abt, Helmut A. (January 2009), "MK Classifications of Spectroscopic Binaries", The Astrophysical Journal Supplement 180 (1): 117–118, doi:10.1088/0067-0049/180/1/117, Bibcode: 2009ApJS..180..117A
38. ↑ Fekel, Francis C.; Warner, Phillip B.; Kaye, Anthony B. (April 2003), "Spectroscopy of Early F Stars: γ Doradus Candidates and Possible Metallic Shell Stars", The Astronomical Journal 125 (4): 2196–2214, doi:10.1086/368239, Bibcode: 2003AJ....125.2196F
39. ↑ Fuhrmann, Klaus (February 2008), "Nearby stars of the Galactic disc and halo - IV", Monthly Notices of the Royal Astronomical Society 384 (1): 173–224, doi:10.1111/j.1365-2966.2007.12671.x, Bibcode: 2008MNRAS.384..173F
40. ↑ "SIMBAD Astronomical Database". Centre de Données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/.
41. ↑ Malagnini, M. L.; Morossi, C. (November 1990), "Accurate absolute luminosities, effective temperatures, radii, masses and surface gravities for a selected sample of field stars", Astronomy and Astrophysics Supplement Series 85 (3): 1015–1019, Bibcode: 1990A&AS...85.1015M
42. ↑ Vogt, Steven S. et al. (2005). "Five New Multicomponent Planetary Systems". The Astrophysical Journal 632 (1): 638–658. doi:10.1086/432901. Bibcode: 2005ApJ...632..638V. https://resolver.caltech.edu/CaltechAUTHORS:20130108-151615622.
43. ↑ Bonfils, Xavier; Gillon, Michael (2011). "A short-period super-Earth orbiting the M2.5 dwarf GJ 3634: Detection with Harps velocimetry and transit search with Spitzer photometry". Astronomy and Astrophysics (European Southern Observatory). doi:10.1051/0004-6361/201015981. Bibcode: 2011yCat..35280111B.
44. ↑ Wittenmyer et al. (2011). "The Pan-Pacific Planet Search. I. A Giant Planet Orbiting 7 CMa". The Astrophysical Journal 743 (2): 184. doi:10.1088/0004-637X/743/2/184. Bibcode: 2011ApJ...743..184W.
45. ↑ Dragomir, Diana et al. (2012). "The HD 192263 System: Planetary Orbital Period and Stellar Variability Disentangled". The Astrophysical Journal 754 (1): 37. doi:10.1088/0004-637X/754/1/37. Bibcode: 2012ApJ...754...37D.

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