List of star systems within 30–35 light-years

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 332530.03 ± 0.721M3V
HD 10236530.07 ± 0.062G2V + M4V4.88 + 15has 1 known planet[1][2][3][4]
2MASS 1750-0030.1 ± 0.71L
Gliese 314630.12 ± 1.331M5.0Ve
Gamma Pavonis30.21 ± 0.051F9V4.22[5][1]
Gliese 313530.41 ± 0.151M2.5+V
Gliese 112330.51 ± 0.281M4.5V[6]
Gliese 19030.52 ± 0.181M3.5V
Gliese 22630.60 ± 0.121M2.5V
Gliese 35730.65 ± 0.181M2.5V
Gliese 17630.68 ± 0.171M2.5V9.95has 1 known planet[7]
LHS 19430.69 ± 0.391DQ8
Gliese 36730.82 ± 0.171M1.0V
2MASS J11592743-524718830.9 ± 0.041M9V[8]Brown Dwarf
2MASS 0034+052330.9 +2.4
−2.1		1T
Gliese 69430.92 ± 0.341M2V
Gliese 106530.98 ± 0.981M3V
Gliese 122731.06 ± 1.781M4.0V[9]
HR 445831.18 ± 0.112K0V + DC85.97 + 15[1][10][11]
2MASS J11553952-372735031.2 ± 1.51L
BPS CS 22898-006631.25 ± 7.111M4.2V
61 Ursae Majoris31.35 ± 0.081G8V5.35[12][13]
Gliese 35831.36 ± 0.121M3V
CE Boötis31.49 ± 0.521M3V
TYC 3251-1875-131.51 ± 5.901MV
LHS 616731.57 ± 0.302M4.5V[14]
WISE J140533.32+835030.531.6 ± 5.51L
CFBD J0059-0131.6 ± 0.61T
Gliese 47931.61 ± 0.681M3V(e)
Gliese 113831.70 ± 0.961M5V
Gliese 43631.80 ± 0.101M2.5V10.67has 1 known planet[15]
12 Ophiuchi31.80 ± 0.121K2V5.77[16]
LP 655-4831.96 ± 0.331M7.5Ve
WISE 0811-805132.01T9.5
LHS 14532.04 ± 0.251DA8.1[17]
2MASS J2139+022032.1 ± 0.61T
Gliese 63832.11 ± 0.071K7.5Ve8.11[13]
Gliese 325332.11 ± 0.641M5V
Gliese 49/5132.12 ± 0.502M1.5V + M5V
AU Microscopii32.32 ± 0.333M1Ve8.73[18]
Gliese 311932.36 ± 0.591M4.5Ve
Gliese 68032.37 ± 0.261M3V
WISE 1614+173932.61T919.08
ULAS 1335+1132.6 ± 0.51T
Gliese 112532.61 ± 0.171M3.5Ve[19]
Gliese 397632.71 ± 1.021M5V
Gliese 318232.73 ± 0.101DAZ9.5[20]
Gliese 23932.78 ± 0.171K7V
Gliese 2232.82 ± 0.693M2.5Ve + M3V10.29 + 12.19 + 13.2
HR 525632.83 ± 0.111K3V6.520[21][22]
HR 51132.84 ± 0.181K0V5.63[10][23]
WISE 1150+630232.91T817.72
WISE 1318-175832.91T9
WISE 1217+162632.9 +6.4
−4.6		2T917.83
Gliese 678.1 A33.12 ± 0.101M1.0Ve
Gliese 45333.13 ± 0.191K4+V
Alpha Mensae33.26 ± 0.051G7V5.09[1][10]
Gliese 127733.59 ± 0.331M4.5
Pollux33.78 ± 0.091K0III1.14has 1 known planet[24][25][26]
Gliese 64933.84 ± 0.121M1.5V9.62has 1 known planet[27]
Gliese 339.133.52 ± 0.641DC7P[20]
HD 1792533.76 ± 0.141K1V6.04[10][28]
2MASS 0559-140433.76 ± 0.351T
2MASS 1237+652633.9 ± 1.81T6.5V16.15[29]
WISE 1322-234033.91T817.01
Gliese 59534.01 ± 1.871M3
Gliese 127.1 A34.08 ± 0.621DA3.0[17]
WISE J2030+074934.2 ± 8.51T1.5[30]
Gliese 304934.25 ± 0.501M3[31]
Iota Persei34.38 ± 0.081G0V4.05
2MASS 1047+212434.4 ± 1.41T
WD 0821-66934.44 ± 0.201DA9.8[17]
2MASS J00501994−332240234.5 ± 0.91T
Gliese 653/65434.60 ± 0.351K4/5V + M1.5V
2MASS 2228-431034.7 +2.8
−2.4		1T
2MASS J08251968+211552134.8 ± 0.41L
2MASS 0243-245334.8 ± 1.41T6[29]
WISE 0734-715734.91Y020.41[32]
Zeta Herculis34.95 ± 0.182F9IV + G7V2.81[33][34]
Gliese 61734.99 ± 0.142M1-Ve + M3.0Vehas 1 known planet[35]

See also

References

  1. 1 2 3 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, arXiv:astro-ph/0603770, Bibcode:2006AJ....132..161G, doi:10.1086/504637
  2. ↑ 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
  3. ↑ Feinstein, A. (1966), "Photoelectric observations of Southern late-type stars", The Information Bulletin for the Southern Hemisphere, 8: 30, Bibcode:1966IBSH....8...30F
  4. ↑ Raghavan, Deepak; et al. (September 2010), "A Survey of Stellar Families: Multiplicity of Solar-type Stars", The Astrophysical Journal Supplement, 190 (1): 1–42, arXiv:1007.0414, Bibcode:2010ApJS..190....1R, doi:10.1088/0067-0049/190/1/1 For the adopted physical separation, see Table 11 in the appendix.
  5. ↑ Jehin, E.; et al. (January 1999), "Abundance correlations in mildly metal-poor stars", Astronomy and Astrophysics, 341: 241–255, arXiv:astro-ph/9809405, Bibcode:1999A&A...341..241J
  6. ↑ 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. arXiv:1604.05611. Bibcode:2016AJ....152...24W. doi:10.3847/0004-6256/152/1/24. ISSN 1538-3881.
  7. ↑ Forveille, T.; et al. (January 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. arXiv:0809.0750. Bibcode:2009A&A...493..645F. doi:10.1051/0004-6361:200810557.
  8. ↑ http://simbad.u-strasbg.fr/simbad/sim-id?Ident=2MASS+J11592743-5247188
  9. ↑ 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. arXiv:1312.3241. Bibcode:2014ApJ...784..156D. doi:10.1088/0004-637X/784/2/156. ISSN 0004-637X.
  10. 1 2 3 4 Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV data. Bibcode:1986EgUBV........0M.
  11. ↑ 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. arXiv:1307.8047. Bibcode:2013MNRAS.435.2077H. doi:10.1093/mnras/stt1433.
  12. ↑ Cornide, M.; Rego, M. (October 1984). "Iron abundances in G dwarfs". Astrophysics and Space Science. 105 (1): 55–65. Bibcode:1984Ap&SS.105...55C. doi:10.1007/BF00651207.
  13. 1 2 Wilson, O. C. (November 1962). "Relationship Between Colors and Spectra of Late Main-Sequence Stars". Astrophysical Journal. 136: 793. Bibcode:1962ApJ...136..793W. doi:10.1086/147437.
  14. ↑ Bartlett, Jennifer L.; Lurie, John C.; Riedel, Adric; Ianna, Philip A.; Jao, Wei-Chun; Henry, Todd J.; Winters, Jennifer G.; Finch, Charlie T.; Subasavage, John P. (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. Bibcode:2017AJ....154..151B. doi:10.3847/1538-3881/aa8457. ISSN 1538-3881.
  15. ↑ Butler, R. Paul; et al. (2004). "A Neptune-Mass Planet Orbiting the Nearby M Dwarf GJ 436". The Astrophysical Journal. 617 (1): 580–588. arXiv:astro-ph/0408587. Bibcode:2004ApJ...617..580B. doi:10.1086/425173. Retrieved 2009-12-26.
  16. ↑ Fuhrmann, Klaus (February 2008), "Nearby stars of the Galactic disc and halo - IV", Monthly Notices of the Royal Astronomical Society, 384 (1): 173–224, Bibcode:2008MNRAS.384..173F, doi:10.1111/j.1365-2966.2007.12671.x
  17. 1 2 3 Subasavage, John P.; Jao, Wei-Chun; Henry, Todd J.; Harris, Hugh C.; Dahn, Conard C.; Bergeron, P.; Dufour, P.; Dunlap, Bart H.; Barlow, Brad N.; Ianna, Philip A.; Lépine, Sébastien; Margheim, Steven J. (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. arXiv:1706.00709. Bibcode:2017AJ....154...32S. doi:10.3847/1538-3881/aa76e0. ISSN 1538-3881.
  18. ↑ 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, arXiv:astro-ph/0609258, Bibcode:2006A&A...460..695T, doi:10.1051/0004-6361:20065602
  19. ↑ 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. arXiv:1611.00656. Bibcode:2016ApJ...832L..18J. doi:10.3847/2041-8205/832/1/L18. ISSN 2041-8213.
  20. 1 2 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. arXiv:1606.01236. Bibcode:2016MNRAS.462.2295H. doi:10.1093/mnras/stw1357. ISSN 0035-8711.
  21. ↑ 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.
  22. ↑ 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. Bibcode:2003A&A...406..995M. doi:10.1051/0004-6361:20030647.
  23. ↑ 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, arXiv:0706.0542, Bibcode:2007AJ....133.2524W, doi:10.1086/514336.
  24. ↑ 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.
  25. ↑ Morgan, W. W.; Keenan, P. C. (1973), "Spectral Classification", Annual Review of Astronomy and Astrophysics, 11: 29, Bibcode:1973ARA&A..11...29M, doi:10.1146/annurev.aa.11.090173.000333
  26. ↑ 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: 335–341, arXiv:astro-ph/0606517, Bibcode:2006A&A...457..335H, doi:10.1051/0004-6361:20065445
  27. ↑ 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. arXiv:0912.2730. Bibcode:2010PASP..122..149J. doi:10.1086/651007. JSTOR 10.1086/651007.
  28. ↑ 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, arXiv:astro-ph/0106537, Bibcode:2001MNRAS.328...45M, doi:10.1046/j.1365-8711.2001.04781.x.
  29. 1 2 Vrba, F. J.; Henden, A. A.; Luginbuhl, C. B.; Guetter, H. H.; Munn, J. A.; Canzian, B.; Burgasser, A. J.; Kirkpatrick, J. Davy; Fan, X.; Geballe, T. R.; Golimowski, D. A.; Knapp, G. R.; Leggett, S. K.; Schneider, D. P.; Brinkman, J. (2004). "Preliminary Parallaxes of 40 L and T Dwarfs from the U.S. Naval Observatory Infrared Astrometry Program". The Astronomical Journal. 127: 2948–2968. arXiv:astro-ph/0402272. Bibcode:2004AJ....127.2948V. doi:10.1086/383554.
  30. ↑ 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. arXiv:1307.2722. Bibcode:2013A&A...557A..43B. doi:10.1051/0004-6361/201322141.
  31. ↑ Winters, Jennifer G.; Sevrinsky, R. Andrew; Jao, Wei-Chun; Henry, Todd J.; Riedel, Adric R.; Subasavage, John P.; Lurie, John C.; Ianna, Philip A.; Finch, Charlie T. (2016). "THE SOLAR NEIGHBORHOOD. XXXVIII. RESULTS FROM THE CTIO/SMARTS 0.9 m: TRIGONOMETRIC PARALLAXES FOR 151 NEARBY M DWARF SYSTEMS". The Astronomical Journal. 153 (1): 14. arXiv:1610.07552. Bibcode:2017AJ....153...14W. doi:10.3847/1538-3881/153/1/14. ISSN 1538-3881.
  32. ↑ Kirkpatrick, J. D.; Gelino, C. R.; Cushing, M. C.; Mace, G. N.; Griffith, R. L.; Skrutskie, M. F.; Marsh, K. A.; Wright, E. L.; Eisenhardt, P. R.; McLean, I. S.; Mainzer, A. K.; Burgasser, A. J.; Tinney, C. G.; Parker, S.; Salter, G. (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:1205.2122. Bibcode:2012ApJ...753..156K. doi:10.1088/0004-637X/753/2/156.
  33. ↑ Edwards, T. W. (April 1976), "MK classification for visual binary components", Astronomical Journal, 81: 245–249, Bibcode:1976AJ.....81..245E, doi:10.1086/111879
  34. ↑ Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory, 4 (99), Bibcode:1966CoLPL...4...99J
  35. ↑ "The CARMENES search for exoplanets around M dwarfs HD 147379 b: A nearby Neptune in the temperate zone of an early-M dwarf". A. Reiners , I. Ribas , M. Zechmeister , J.A. Caballero , T. Trifonov , S. Dreizler , J.C. Morales , L. Tal-Or , M. Lafarga , A. Quirrenbach , P.J. Amado , A. Kaminski , S.V. Jeffers , J. Aceituno , V.J.S. Béjar , J. Guàrdia , E.W. Guenther , H.-J. Hagen , D. Montes , V.M. Passegger , W. Seifert , A. Schweitzer , M. Cortés-Contreras , M. Abril , F.J. Alonso-Floriano , M. Ammler-von Eiff , R. Antona , G. Anglada-Escudé , H. Anwand-Heerwart , B. Arroyo-Torres , M. Azzaro , D. Baroch , D. Barrado , F.F. Bauer , S. Becerril , D. Benítez , Z.M. Berdiñas6 , G. Bergond7 , M. Blümcke, M. Brinkmöller , C. del Burgo , J. Cano, M.C. Cárdenas Vázquez, E. Casal , C. Cifuentes, A. Claret , J. Colomé , S. Czesla, E. Díez-Alonso, C. Feiz , M. Fernández , I.M. Ferro , B. Fuhrmeister, D. Galadí-Enríquez , A. Garcia-Piquer , M.L. García Vargas, L. Gesa , V. Gómez Galera , J.I. González Hernández , R. González-Peinado, U. Grözinger , S. Grohnert , A. Guijarro , E. de Guindos , J. Gutiérrez-Soto , A.P. Hatzes , P.H. Hauschildt, R.P. Hedrosa , J. Helmling , Th. Henning , I. Hermelo , R. Hernández Arabí , L. Hernández Castaño , F. Hernández Hernando , E. Herrero , A. Huber , P. Huke , E.N. Johnson , E. de Juan , M. Kim, R. Klein , J. Klüter , A. Klutsch, M. Kürster , F. Labarga, A. Lamert , M. Lampón , L.M. Lara , W. Laun , U. Lemke , R. Lenzen , R. Launhardt , M. López del Fresno , M.J. López-González , M. López-Puertas , J.F. López Salas , J. López-Santiago, R. Luque , H. Magán Madinabeitia , U. Mall , L. Mancini, H. Mande , E. Marfil, J.A. Marín Molina , D. Maroto Fernández , E.L. Martín , S. Martín-Ruiz , C.J. Marvin1 , R.J. Mathar Manduro , J. Pascual , A. Pavlov , S. Pedraz , A. Pérez-Calpena, D. Pérez Medialdea , M. Perger , M.A.C. Perryman, M. Pluto , O. Rabaza, A. Ramón , R. Rebolo , P. Redondo , S. Reffert , S. Reinhart , P. Rhode , H.-W. Rix , F. Rodler, E. Rodríguez , C. Rodríguez-López , A. Rodríguez Trinidad , R.-R. Rohloff , A. Rosich , S. Sadegi , E. Sánchez-Blanco , M.A. Sánchez Carrasco , A. Sánchez-López , J. Sanz-Forcada , P. Sarkis , L.F. Sarmiento , S. Schäfer1 , J.H.M.M. Schmitt, J. Schiller , P. Schöfer , E. Solano , O. Stahl , J.B.P. Strachan, J. Stürmer, J.C. Suárez , H.M. Tabernero, M. Tala , S.M. Tulloch , R.-G. Ulbrich , G. Veredas , J.I. Vico Linares , F. Vilardell , K. Wagner , J. Winkler , V. Wolthoff , W. Xu , F. Yan , and M.R. Zapatero Osorio (Dec 15, 2017).
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