List of star systems within 30–35 light-years

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This is a list of star systems within 30–35 light years of Earth.

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

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Gliese 3325 | 30.03 ± 0.72 | 1 | M3V |  | has 1 known planet[1]
HD 102365 | 30.07 ± 0.06 | 2 | G2V + M4V | 4.88 + 15 | has 1 known planet[2][3][4][5]
2MASS 1750-00 | 30.1 ± 0.7 | 1 | L5.5  |  |
Gliese 3146 | 30.12 ± 1.33 | 1 | M5.0Ve |  |
Gamma Pavonis | 30.21 ± 0.05 | 1 | F9V | 4.22 | [6][2]
Gliese 3135 | 30.41 ± 0.15 | 1 | M2.5+V |  |
Gliese 1123 | 30.51 ± 0.28 | 1 | M4.5V |  | [7]
Gliese 190 | 30.52 ± 0.18 | 1 | M3.5V |  |
Gliese 226 | 30.60 ± 0.12 | 1 | M2.5V |  |
Gliese 357 | 30.65 ± 0.18 | 1 | M2.5V |  | has 3 known planets[8][1]
Gliese 176 | 30.68 ± 0.17 | 1 | M2.5V | 9.95 | has 1 known planet[9]
LHS 194 | 30.69 ± 0.39 | 1 | DQ8 |  |
Gliese 367 | 30.82 ± 0.17 | 1 | M1.0V |  |
2MASS J11592743-5247188 | 30.9 ± 0.04 | 1 | M9V |  | [10]Brown Dwarf
2MASS 0034+0523 | 30.9 +2.4−2.1 | 1 | T6.5 |  |
Gliese 694 | 30.92 ± 0.34 | 1 | M2V |  |
Gliese 3512 | 30.95 ‬± 0.03 | 1 | M5.7 |  | 1 known planet with another suspected[11]
Gliese 1065 | 30.98 ± 0.98 | 1 | M3V |  |
Gliese 1227 | 31.06 ± 1.78 | 1 | M4.0V |  | [12]
HR 4458 | 31.18 ± 0.11 | 2 | K0V + DC8 | 5.97 + 15 | [2][13][14]
2MASS J11553952-3727350 | 31.2 ± 1.5 | 1 | L2.3  |  |
61 Ursae Majoris | 31.35 ± 0.08 | 1 | G8V | 5.35 | [15][16]
Gliese 358 | 31.36 ± 0.12 | 1 | M3V |  |
TYC 3251-1875-1 | 31.51 ± 5.90 | 1 | MV |  |
LHS 6167 | 31.57 ± 0.30 | 2 | M4.5V |  | [17]
WISE J140533.32+835030.5 | 31.6 ± 5.5 | 1 | L8  |  |
CFBD J0059-01 | 31.6 ± 0.6 | 1 | T8.5 |  |
Gliese 479 | 31.61 ± 0.68 | 1 | M3V(e) |  |
Gliese 1138 | 31.70 ± 0.96 | 1 | M5V |  |
Gliese 436 | 31.80 ± 0.10 | 1 | M2.5V | 10.67 | has 1 known planet[18]
12 Ophiuchi | 31.80 ± 0.12 | 1 | K2V | 5.77 | [19]
LP 655-48 | 31.96 ± 0.33 | 1 | M7.5Ve |  |
WISE 0811-8051 | 32.0 | 1 | T9.5 |  |
LHS 145 | 32.04 ± 0.25 | 1 | DA8.1 |  | [20]
2MASS J2139+0220 | 32.1 ± 0.6 | 1 | T1.5 |  |
Gliese 638 | 32.11 ± 0.07 | 1 | K7.5Ve | 8.11 | [16]
Gliese 3253 | 32.11 ± 0.64 | 1 | M5V |  |
Gliese 49/51 | 32.12 ± 0.50 | 2 | M1.5V + M5V |  | has 1 known planet around Gliese 49[21]
AU Microscopii | 32.32 ± 0.33 | 3 | M1Ve | 8.73 | has 2 known planets [22]
Gliese 3119 | 32.36 ± 0.59 | 1 | M4.5Ve |  |
Gliese 680 | 32.37 ± 0.26 | 1 | M3V |  |
Gliese 569 A | 32.466 ± 0.007 | 1 | M3V |  | Orbited by binary brown dwarfs
WISE 1614+1739 | 32.6 | 1 | T9 | 19.08 |
ULAS 1335+11 | 32.6 ± 0.5 | 1 | T9 |  |
Gliese 239 (ja) | 32.608 ± 0.007 | 1 | M0V |  | has 2 known planets[23]
Gliese 1125 | 32.61 ± 0.17 | 1 | M3.5Ve |  | [24]
Gliese 3976 | 32.71 ± 1.02 | 1 | M5V |  |
Gliese 3182 | 32.73 ± 0.10 | 1 | DAZ9.5 |  | [25]
Gliese 22 | 32.82 ± 0.69 | 3 | M2.5Ve + M3V | 10.29 + 12.19 + 13.2 |
HR 5256 | 32.83 ± 0.11 | 1 | K3V | 6.520 | [26][27]
HR 511 | 32.84 ± 0.18 | 1 | K0V | 5.63 | [13][28]
WISE 1150+6302 | 32.9 | 1 | T8 | 17.72 |
WISE 1318-1758 | 32.9 | 1 | T9 |  |
Gliese 678.1 A | 33.12 ± 0.10 | 1 | M1.0Ve |  |
Gliese 453 | 33.13 ± 0.19 | 1 | K4+V |  |
Alpha Mensae | 33.26 ± 0.05 | 1 | G7V | 5.09 | [2][13]
Gliese 1277 | 33.59 ± 0.33 | 1 | M4.5 |  |
Pollux | 33.78 ± 0.09 | 1 | K0III | 1.14 | has 1 known planet[29][30][31]
Gliese 649 | 33.84 ± 0.12 | 1 | M1.5V | 9.62 | has 1 known planet[32]
Gliese 339.1 | 33.52 ± 0.64 | 1 | DC7P |  | [25]
SCR J0533-4257 | 33.75 ± 0.64 | 1 | M4.5V |  |
HD 17925 | 33.76 ± 0.14 | 1 | K1V | 6.04 | [13][33]
2MASS 0559-1404 | 33.76 ± 0.35 | 1 | T4.5 |  |
2MASS 1237+6526 | 33.9 ± 1.8 | 1 | T6.5V | 16.15 | [34]
WISE 1322-2340 | 33.9 | 1 | T8 | 17.01 |
Gliese 595 | 34.01 ± 1.87 | 1 | M3 |  |
Gliese 127.1 | 34.08 ± 0.62 | 1 | DA3.0 |  | [20]
WISE J2030+0749 | 34.2 ± 8.5 | 1 | T1.5 |  | [35]
Gliese 3049 | 34.25 ± 0.50 | 1 | M3 |  | has 1 known planet [36]
Iota Persei | 34.38 ± 0.08 | 1 | G0V | 4.05 |
2MASS 1047+2124 | 34.4 ± 1.4 | 1 | T6.5 |  |
WD 0821-669 | 34.44 ± 0.20 | 1 | DA9.8 |  | [20]
2MASS J00501994−3322402 | 34.5 ± 0.9 | 1 | T7 |  |
Gliese 653/654 | 34.60 ± 0.35 | 2 | K4/5V + M1.5V |  |
L 98-59 | 34.6 | 1 | M3V |  | has 4 known planets and 1 unconfirmed
2MASS 2228-4310 | 34.7 +2.8−2.4 | 1 | T6.5 |  |
2MASS J08251968+2115521 | 34.8 ± 0.4 | 1 | L7.5  |  |
2MASS 0243-2453 | 34.8 ± 1.4 | 1 | T6 |  | [34]
WISE 0734-7157 | 34.9 | 1 | Y0 | 20.41 | [37]
Zeta Herculis | 34.95 ± 0.18 | 2 | F9IV + G7V | 2.81 | [38][39]
Gliese 617 | 34.99 ± 0.14 | 2 | M1-Ve + M3.0Ve |  | has 1 known planet[40]

## See also

* Lists of stars
* List of star systems within 25-30 light-years
* List of star systems within 35-40 light-years
* List of nearest stars and brown dwarfs

## References

1. ↑ 1.0 1.1 Barnes, J. R.; Kiraga, M.; Diaz, M.; Berdiñas, Z.; Jenkins, J. S.; Keiser, S.; Thompson, I.; Crane, J. D.; Shectman, S. A. (2019-06-11). "Frequency of planets orbiting M dwarfs in the Solar neighbourhood". arXiv:1906.04644 [astro-ph.EP].
2. ↑ 2.0 2.1 2.2 2.3 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
3. ↑ Poveda, A. et al. (April 1994), "Statistical studies of visual double and multiple stars. II. A catalogue of nearby wide binary and multiple systems", Revista Mexicana de Astronomía y Astrofísica 28 (1): 43–89, Bibcode: 1994RMxAA..28...43P
4. ↑ Feinstein, A. (1966), "Photoelectric observations of Southern late-type stars", The Information Bulletin for the Southern Hemisphere 8: 30, Bibcode: 1966IBSH....8...30F
5. ↑ 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 For the adopted physical separation, see Table 11 in the appendix.
6. ↑ Jehin, E. et al. (January 1999), "Abundance correlations in mildly metal-poor stars", Astronomy and Astrophysics 341: 241–255, Bibcode: 1999A&A...341..241J
7. ↑ Weinberger, Alycia J.; Boss, Alan P.; Keiser, Sandra A.; Anglada-Escudé, Guillem; Thompson, Ian B.; Burley, Gregory (2016). "Trigonometric Parallaxes and Proper Motions of 134 Southern Late M, L, and T Dwarfs from the Carnegie Astrometric Planet Search Program". The Astronomical Journal 152 (1): 24. doi:10.3847/0004-6256/152/1/24. ISSN 1538-3881. Bibcode: 2016AJ....152...24W.
8. ↑ Wohler, B.; Winn, J. W.; Wang, S. X.; Twicken, J. D.; Teske, J.; Tamura, M.; Shectman, S. A.; Rowden, P. et al. (2019-04-29). "A planetary system around the nearby M dwarf Gl 357 including a transiting hot Earth-sized planet optimal for atmospheric characterisation" (in en). Astronomy & Astrophysics 628: A39. doi:10.1051/0004-6361/201935801. Bibcode: 2019A&A...628A..39L.
9. ↑ Forveille, Thierry; Bonfils, Xavier; Delfosse, Xavier; Gillon, Michaël; Udry, Stéphane; Bouchy, François; Lovis, Christophe; Mayor, Michel et al. (2009). "The HARPS search for southern extra-solar planets. XIV. Gl 176b, a super-Earth rather than a Neptune, and at a different period". Astronomy and Astrophysics 493 (2): 645–650. doi:10.1051/0004-6361:200810557. Bibcode: 2009A&A...493..645F. https://www.aanda.org/articles/aa/full/2009/02/aa10557-08/aa10557-08.html.
10. ↑ "2Mass J11592743-5247188". http://simbad.u-strasbg.fr/simbad/sim-id?Ident=2MASS+J11592743-5247188.
11. ↑ Morales, J. C. et al. (2019). "A giant exoplanet orbiting a very-low-mass star challenges planet formation models". Science 365 (6460): 1441–1445. doi:10.1126/science.aax3198. ISSN 0036-8075. PMID 31604272. Bibcode: 2019Sci...365.1441M.
12. ↑ Dittmann, Jason A.; Irwin, Jonathan M.; Charbonneau, David; Berta-Thompson, Zachory K. (2014). "Trigonometric Parallaxes for 1507 Nearby Mid-To-Late M Dwarfs". The Astrophysical Journal 784 (2): 156. doi:10.1088/0004-637X/784/2/156. ISSN 0004-637X. Bibcode: 2014ApJ...784..156D.
13. ↑ 13.0 13.1 13.2 13.3 Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data. Bibcode: 1986EgUBV........0M.
14. ↑ Holberg, J. B. et al. (November 2013). "Where are all the Sirius-like binary systems?". Monthly Notices of the Royal Astronomical Society 435 (3): 2077–2091. doi:10.1093/mnras/stt1433. Bibcode: 2013MNRAS.435.2077H.
15. ↑ Cornide, M.; Rego, M. (October 1984). "Iron abundances in G dwarfs". Astrophysics and Space Science 105 (1): 55–65. doi:10.1007/BF00651207. Bibcode: 1984Ap&SS.105...55C.
16. ↑ 16.0 16.1 Wilson, O. C. (November 1962). "Relationship Between Colors and Spectra of Late Main-Sequence Stars". Astrophysical Journal 136: 793. doi:10.1086/147437. Bibcode: 1962ApJ...136..793W.
17. ↑ Bartlett, Jennifer L.; Lurie, John C.; Riedel, Adric; Ianna, Philip A.; Jao, Wei-Chun; Henry, Todd J.; Winters, Jennifer G.; Finch, Charlie T. et al. (2017). "The Solar Neighborhood. XXXX. Parallax Results from the CTIOPI 0.9 m Program: New Young Stars Near the Sun". The Astronomical Journal 154 (4): 151. doi:10.3847/1538-3881/aa8457. ISSN 1538-3881. Bibcode: 2017AJ....154..151B.
18. ↑ Butler, R. Paul et al. (2004). "A Neptune-Mass Planet Orbiting the Nearby M Dwarf GJ 436". The Astrophysical Journal 617 (1): 580–588. doi:10.1086/425173. Bibcode: 2004ApJ...617..580B.
19. ↑ 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
20. ↑ 20.0 20.1 20.2 Subasavage, John P.; Jao, Wei-Chun; Henry, Todd J.; Harris, Hugh C.; Dahn, Conard C.; Bergeron, P.; Dufour, P.; Dunlap, Bart H. et al. (2017). "The Solar Neighborhood. XXXIX. Parallax Results from the CTIOPI and NOFS Programs: 50 New Members of the 25 parsec White Dwarf Sample". The Astronomical Journal 154 (1): 32. doi:10.3847/1538-3881/aa76e0. ISSN 1538-3881. Bibcode: 2017AJ....154...32S.
21. ↑ Zechmeister, M.; Osorio, M. R. Zapatero; Sánchez, R. Zanmar; Toledo-Padrón, B.; Mascareño, A. Suárez; Sozzetti, A.; Schmitt, J. H. M. M.; Rodríguez-López, C. et al. (2019-03-12). "Gliese 49: Activity evolution and detection of a super-Earth" (in en). Astronomy & Astrophysics 624: A123. doi:10.1051/0004-6361/201935192.
22. ↑ 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
23. ↑ Luque, R.; Fulton, B. J. et al. (2022-04-21). "The HD 260655 system: Two rocky worlds transiting a bright M dwarf at 10 pc". Astronomy & Astrophysics 664: A199. doi:10.1051/0004-6361/202243834. Bibcode: 2022A&A...664A.199L.
24. ↑ Jao (饒惟君), Wei-Chun; Henry, Todd J.; Riedel, Adric R.; Winters, Jennifer G.; Slatten, Kenneth J.; Gies, Douglas R. (2016). "Distance-Dependent Offsets Between Parallaxes for Nearby Stars Andgaiadr1 Parallaxes". The Astrophysical Journal 832 (1): L18. doi:10.3847/2041-8205/832/1/L18. ISSN 2041-8213. Bibcode: 2016ApJ...832L..18J.
25. ↑ 25.0 25.1 Holberg, J. B.; Oswalt, T. D.; Sion, E. M.; McCook, G. P. (2016). "The 25 parsec local white dwarf population". Monthly Notices of the Royal Astronomical Society 462 (3): 2295–2318. doi:10.1093/mnras/stw1357. ISSN 0035-8711. Bibcode: 2016MNRAS.462.2295H.
26. ↑ Oja, T. (August 1991). "UBV photometry of stars whose positions are accurately known. VI". Astronomy and Astrophysics Supplement Series 89 (2): 415–419. Bibcode: 1991A&AS...89..415O.
27. ↑ Marrese, P. M.; Boschi, F.; Munari, U. (August 2003). "High resolution spectroscopy over lambda lambda 8500-8750 Å for GAIA. IV. Extending the cool MK stars sample". Astronomy and Astrophysics 406: 995–999. doi:10.1051/0004-6361:20030647. Bibcode: 2003A&A...406..995M.
28. ↑ White, Russel J.; Gabor, Jared M.; Hillenbrand, Lynne A. (June 2007), "High-Dispersion Optical Spectra of Nearby Stars Younger Than the Sun", The Astronomical Journal 133 (6): 2524–2536, doi:10.1086/514336, Bibcode: 2007AJ....133.2524W.
29. ↑ Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues 2237: 0. Bibcode: 2002yCat.2237....0D.
30. ↑ Morgan, W. W.; Keenan, P. C. (1973), "Spectral Classification", Annual Review of Astronomy and Astrophysics 11: 29, doi:10.1146/annurev.aa.11.090173.000333, Bibcode: 1973ARA&A..11...29M
31. ↑ Hatzes, A. P. et al. (2006), "Confirmation of the planet hypothesis for the long-period radial velocity variations of β Geminorum", Astronomy and Astrophysics 457 (1): 335–341, doi:10.1051/0004-6361:20065445, Bibcode: 2006A&A...457..335H
32. ↑ Johnson, John Asher et al. (2010). "The California Planet Survey II. A Saturn-Mass Planet Orbiting the M Dwarf Gl649". The Publications of the Astronomical Society of the Pacific 122 (888): 149–155. doi:10.1086/651007. Bibcode: 2010PASP..122..149J.
33. ↑ Montes, D. et al. (2001), "Late-type members of young stellar kinematic groups - I. Single stars", Monthly Notices of the Royal Astronomical Society 328 (1): 45–63, doi:10.1046/j.1365-8711.2001.04781.x, Bibcode: 2001MNRAS.328...45M, http://eprints.ucm.es/30941/1/castrorubio18libre.pdf.
34. ↑ 34.0 34.1 Vrba, F. J.; Henden, A. A.; Luginbuhl, C. B.; Guetter, H. H.; Munn, J. A.; Canzian, B.; Burgasser, Adam J.; Kirkpatrick, J. Davy et al. (2004). "Preliminary Parallaxes of 40 L and T Dwarfs from the U.S. Naval Observatory Infrared Astrometry Program". The Astronomical Journal 127 (5): 2948–2968. doi:10.1086/383554. Bibcode: 2004AJ....127.2948V.
35. ↑ Bihain, Gabriel; Scholz, Ralf-Dieter; Storm, Jesper; Schnurr, Olivier (2013). "An overlooked brown dwarf neighbour (T7.5 at d~5pc) of the Sun and two additional T dwarfs at about 10pc". Astronomy & Astrophysics 557: A43. doi:10.1051/0004-6361/201322141. Bibcode: 2013A&A...557A..43B.
36. ↑ Sartori, Lia F.; Lovis, Christophe; Delisle, Jean-Baptiste; Lendl, Monika; Cugno, Gabriele; Boehle, Anna; Dannert, Felix; Krenn, Andreas et al. (2023), "L 363-38 b: A planet newly discovered with ESPRESSO orbiting a nearby M dwarf star", Astronomy & Astrophysics 670: A42, doi:10.1051/0004-6361/202244347, Bibcode: 2023A&A...670A..42S
37. ↑ Kirkpatrick, J. Davy; Gelino, Christopher R.; Cushing, Michael C.; Mace, Gregory N.; Griffith, Roger L.; Skrutskie, Michael F.; Marsh, Kenneth A.; Wright, Edward L. et al. (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. doi:10.1088/0004-637X/753/2/156. Bibcode: 2012ApJ...753..156K.
38. ↑ Edwards, T. W. (April 1976), "MK classification for visual binary components", Astronomical Journal 81: 245–249, doi:10.1086/111879, Bibcode: 1976AJ.....81..245E
39. ↑ 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
40. ↑ Reiners, Ansgar; Ribas, Ignasi et al. (2018). "The CARMENES search for exoplanets around M dwarfs. HD147379 b: A nearby Neptune in the temperate zone of an early-M dwarf". Astronomy & Astrophysics 609: L5. doi:10.1051/0004-6361/201732165. ISSN 0004-6361. Bibcode: 2018A&A...609L...5R.

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