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
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

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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