List of star systems within 35–40 light-years

This is a list of star systems within 35-40 light years of Earth.

Star system Median distance (ly) Stars in system Spectral type Apparent magnitude (V) Comments and references
TVLM513-4654635.1 ± 0.091M8.5V
Gliese 20335.11 ± 0.921M3.5Ve
Gliese 382035.12 ± 0.321M4.5V
SCR J0838-585535.16 ± 0.222M6.0[1]
HR 903835.2 ± 0.23K3V + M26.40/11.4[2][3][4]
Gliese 48835.2 ± 0.41MV
Delta Trianguli35.4 ± 0.32G0V4.865[5][6]
Beta Virginis «Zavijava»35.6 ± 0.31F9V3.604[7][8]
Gliese 8635.6 ± 0.22K1Vhas 1 known planet[3][9]
SCR J1214-234535.69 ± 0.601M4.5
G 239-2535.77 ± 0.121M3V
HD 16034635.88 ± 0.272K3V
2MASS J19513587-351037535.88 ± 6.521M4
WISE 2313-083735.91T
Gliese 43835.94 ± 0.191MV
2MASS J16452211-131951636.19 ± 0.331L
Denebola36.2 ± 0.41A3V2.113[10][11]
HR 680636.2 ± 0.21K2V6.40[2][3]
54 Piscium36.2 ± 0.32K0V + T7.5V5.88has 1 known planet[12][13][14]
HIP 5705036.2 ± 1.11MVhas 1 known planet [15]
Gamma Serpentis36.3 ± 0.31F6V3.85[16]
HD 7457636.3 ± 0.21KV
HD 8551236.4 ± 0.31K5V7.66has 1 known planet[17]
Gliese 32536.4 +1.5
−1.4		2KV
11 Leonis Minoris36.5 ± 0.32G8V + M5V4.80/12.50[18]
WISE 0325+083136.51T7
Theta Persei36.6 ± 0.32F7V + M1V4.12/10
HD 11540436.6 ± 0.42K2V + M1V6.61
Arcturus36.7 ± 0.31K0III-0.05[3][19]
ADS 4836.7 ± 0.63KV8.83/9.00/9.97[20][21][22]
WISE 0038+276836.91T
Eta Boötis «Muphrid»37.0 ± 0.32G0IV2.680[5][23]
Gliese 20837.1 ± 0.61K7V8.9
Gliese 90237.2 ± 0.31KV
WISE 0627-111437.21T6
WISE 1959-333837.21T8
Gliese 16937.4 ± 0.51KV
WISE 0623-045637.51T8
WISE 2325-410537.51T
HR 555337.6 ± 0.42K0V6.00[2][24]
WISE 2340-074537.81T
Gliese 341737.88 ± 0.961M4.5V
Zeta Doradus38.0 ± 0.22F7V + K7V4.82/9.02[25]
SCR J0640-055238.04 ± 1.271M2[1]
Iota Pegasi38.3 ± 0.32F5V + G8V3.84/6.68[26][27]
Lambda Serpentis38.3 ± 0.41G0V4.43[28][29]
Gliese 773.638.5 ± 5.81KV
Delta Capricorni «Scheddi»38.6 ± 0.42A7mIII2.81[30]
HD 12507238.6 ± 0.41K3IV6.637[3][5]
L 43-7238.66 ± 0.712M4.5[1]
Gamma Virginis «Porrima»38.7 ± 0.42F0V + F0V2.74[31]
L 449-138.7 ± 0.62MV
WISE 0759-490438.81T8
Gliese 41438.9 ± 0.52KV
WISE 0751-763439.11T9
G 180-06039.20 ± 1.191M6V
Zeta Reticuli39.4 ± 0.32G3V + G2V5.22[32][33]
Zeta Trianguli Australis39.5 ± 0.32F9V4.90[2][3]
85 Pegasi39.5 ± 0.43G5Vb + K7V5.75/8.89
Gliese 79839.5 ± 0.61KV
Gliese 18039.5 +1.2
−1.1		1MV10.894has 2 known planets
TRAPPIST-139.5 ± 1.31M8.2V18.80has 7 known planets
WISE 1653+444439.51T8
Gliese 330439.53 ± 1.431M4.5V
HR 338439.7 ± 0.31G9V6.38[3][34]
V538 Aurigae39.9 ± 0.41K1V6.25[2][35]

See also

References

  1. 1 2 3 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.
  2. 1 2 3 4 5 Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV data. SIMBAD, Bibcode:1986EgUBV........0M.
  3. 1 2 3 4 5 6 7 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.
  4. ↑ Malkov, O. Yu.; et al. (2012), "Dynamical masses of a selected sample of orbital binaries", Astronomy & Astrophysics, 546: 5, Bibcode:2012A&A...546A..69M, doi:10.1051/0004-6361/201219774, A69.
  5. 1 2 3 Holmberg, J.; Nordström, 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, arXiv:0811.3982, Bibcode:2009A&A...501..941H, doi:10.1051/0004-6361/200811191
  6. ↑ Kim, Jinyoung Serena; et al. (October 2005), "Formation and Evolution of Planetary Systems: Cold Outer Disks Associated with Sun-like Stars", The Astrophysical Journal, 632 (1): 659–669, arXiv:astro-ph/0506434, Bibcode:2005ApJ...632..659K, doi:10.1086/432863
  7. ↑ Gutierrez-Moreno, Adelina; Moreno, Hugo (June 1968), "A photometric investigation of the Scorpio-Centaurus association", Astrophysical Journal Supplement, 15: 459, Bibcode:1968ApJS...15..459G, doi:10.1086/190168
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  11. ↑ Gutierrez-Moreno, Adelina; et al. (1966), "A System of photometric standards", Publ. Dept. Astron. Univ. Chile, Publicaciones Universidad de Chile, Department de Astronomy, 1: 1–17, Bibcode:1966PDAUC...1....1G
  12. ↑ van Belle, Gerard T.; von Braun, Kaspar (2009). "Directly Determined Linear Radii and Effective Temperatures of Exoplanet Host Stars". The Astrophysical Journal (abstract). 694 (2): 1085–1098. arXiv:0901.1206. Bibcode:2009ApJ...694.1085V. doi:10.1088/0004-637X/694/2/1085.
  13. ↑ 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.
  14. ↑ Fischer, Debra A.; et al. (2003). "A Sub-Saturn Mass Planet Orbiting HD 3651". The Astrophysical Journal. 590 (2): 1081–1087. Bibcode:2003ApJ...590.1081F. CiteSeerX 10.1.1.582.3920. doi:10.1086/375027.
  15. ↑ Haghighipour, Nader; Vogt, Steven S.; Paul Butler, R.; Rivera, Eugenio J.; Laughlin, Greg; Meschiari, Stefano; Henry, Gregory W. (20 May 2010). "The Lick-Carnegie Exoplanet Survey: A Saturn-Mass Planet In The Habitable Zone Of The Nearby M4v Star Hip 57050". The Astrophysical Journal. 715 (1): 271–276. arXiv:1004.4608. Bibcode:2010ApJ...715..271H. doi:10.1088/0004-637X/715/1/271.
  16. ↑ 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
  17. ↑ Pepe, F.; et al. (2011). "The HARPS search for Earth-like planets in the habitable zone. I. Very low-mass planets around HD 20794, HD 85512, and HD 192310". Astronomy and Astrophysics. 534. A58. arXiv:1108.3447. Bibcode:2011A&A...534A..58P. doi:10.1051/0004-6361/201117055.
  18. ↑ Malkov, O. Yu.; et al. (2012), "Dynamical masses of a selected sample of orbital binaries", Astronomy & Astrophysics, 546: 5, Bibcode:2012A&A...546A..69M, doi:10.1051/0004-6361/201219774, A69
  19. ↑ 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.
  20. ↑ GJ 4 A – Star in double system, database entry, SIMBAD. Accessed 13 July 2013
  21. ↑ GJ 4 B – Star in double system, database entry, SIMBAD. Accessed 13 July 2013
  22. ↑ GJ 2 – Star in double system, database entry, SIMBAD. Accessed 13 July 2013.
  23. ↑ Thévenin, F.; et al. (June 2005), "VLTI/VINCI diameter constraints on the evolutionary status of δ Eri, ξ Hya, η Boo", Astronomy and Astrophysics, 436 (1): 253–262, arXiv:astro-ph/0501420, Bibcode:2005A&A...436..253T, doi:10.1051/0004-6361:20042075
  24. ↑ Kennedy, Grant M. (February 2015), "Nature or nurture of coplanar Tatooines: the aligned circumbinary Kuiper belt analogue around HD 131511", Monthly Notices of the Royal Astronomical Society: Letters, 447 (1): L75–L79, arXiv:1412.0674, Bibcode:2015MNRAS.447L..75K, doi:10.1093/mnrasl/slu190.
  25. ↑ van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. Archived from the original on 2016-04-02.
  26. ↑ Konacki, Maciej; et al. (2010). "High-precision Orbital and Physical Parameters of Double-lined Spectroscopic Binary Stars—HD78418, HD123999, HD160922, HD200077, and HD210027". The Astrophysical Journal. 719 (2): 1293–1314. arXiv:0910.4482. Bibcode:2010ApJ...719.1293K. doi:10.1088/0004-637X/719/2/1293.
  27. ↑ 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
  28. ↑ "lam Ser -- Spectroscopic binary". SIMBAD. Centre de Données astronomiques de Strasbourg. Retrieved 2010-12-15.
  29. ↑ Johnson, H. L.; Morgan, W. W. (1953). "Fundamental stellar photometry for standards of spectral type on the revised system of the Yerkes spectral atlas". Astrophysical Journal. 117: 313–352. Bibcode:1953ApJ...117..313J. doi:10.1086/145697.
  30. ↑ Malkov, O. Yu.; et al. (February 2006), "A catalogue of eclipsing variables", Astronomy and Astrophysics, 446 (2): 785–789, Bibcode:2006A&A...446..785M, doi:10.1051/0004-6361:20053137
  31. ↑ Cayrel de Strobel, G.; Soubiran, C.; Ralite, N. (July 2001), "Catalogue of [Fe/H] determinations for FGK stars: 2001 edition", Astronomy and Astrophysics, 373: 159–163, arXiv:astro-ph/0106438, Bibcode:2001A&A...373..159C, doi:10.1051/0004-6361:20010525
  32. ↑ del Peloso, E. F.; da Silva, L.; Porto de Mello, G. F. (June 2000). "zeta1 and zeta2 Reticuli and the existence of the zeta Herculis group". Astronomy and Astrophysics. 358: 233–241. Bibcode:2000A&A...358..233D.
  33. ↑ Feinstein, A. (1966), "Photoelectric observations of Southern late-type stars", Informational Bulletin of the Southern Hemisphere, 8: 30, Bibcode:1966IBSH....8...30F
  34. ↑ Mamajek, Eric E.; Hillenbrand, Lynne A. (November 2008), "Improved Age Estimation for Solar-Type Dwarfs Using Activity-Rotation Diagnostics", The Astrophysical Journal, 687 (2): 1264–1293, arXiv:0807.1686, Bibcode:2008ApJ...687.1264M, doi:10.1086/591785
  35. ↑ Montes, D.; et al. (November 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.
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