Template:Star systems within 5 – 10 light-years/doc

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Adopted distance estimates[edit]

Object Parallax, mas Distance, pc Distance, ly Distance, Pm Source
Systems with an A-type main-sequence star as primary member.
Sirius 379.21 ± 1.58 2.637 ± 0.011 8.6 ± 0.04 81.4 ± 0.3 van Leeuwen (2007)[1]
Systems with an M-type main-sequence star (red dwarf) as primary member.
Barnard's Star 545.4 ± 0.3 1.8335 ± 0.001 5.98 ± 0.003 56.576 ± 0.031 Benedict et al. (1999)[2]
Wolf 359 419.1 ± 2.1 2.386 ± 0.012 7.78 ± 0.04 73.6 ± 0.4 van Altena et al. (1995)[3]
Lalande 21185 392.64 ± 0.67 2.547 ± 0.004 8.307 ± 0.014 78.59 ± 0.13 van Leeuwen (2007)[4]
Luyten 726-8 373.7 ± 2.7 2.676 ± 0.019 8.73 ± 0.06 82.6 ± 0.6 van Altena et al. (1995)[5]
Ross 154 336.72 ± 2.03 2.97 ± 0.018 9.69 ± 0.06 91.6+0.6
−0.5
van Leeuwen (2007)[6]
Systems with an L-type brown dwarf as primary member.
Luhman 16 495 ± 4.6 2.02 ± 0.019 6.59 ± 0.06 62.3 ± 0.6 Boffin et al. (2014)[7]
Systems with a Y-type sub-brown dwarf or a Y-type rogue planet as primary member.
WISE 0855−0714 433 ± 15 2.31 ± 0.08 7.53+0.27
−0.25
71.3+2.6
−2.4
Luhman & Esplin (2014)[8]
For other distance estimates see articles on these objects.

See also[edit]

References[edit]

  1. ^ van Leeuwen F. (2007). "HIP 32349". Validation of the new Hipparcos reduction. Retrieved 2014-06-05. 
  2. ^ Benedict, G. Fritz; McArthur, Barbara; Chappell, D. W.; Nelan, E.; Jefferys, W. H.; Van Altena, W.; Lee, J.; Cornell, D.; Shelus, P. J.; Hemenway, P. D.; Franz, Otto G.; Wasserman, L. H.; Duncombe, R. L.; Story, D.; Whipple, A. L.; Fredrick, L. W. (1999). "Interferometric Astrometry of Proxima Centauri and Barnard's Star Using HUBBLE SPACE TELESCOPE Fine Guidance Sensor 3: Detection Limits for Substellar Companions". The Astronomical Journal 118 (2): 1086–1100. arXiv:astro-ph/9905318. Bibcode:1999AJ....118.1086B. doi:10.1086/300975.  edit
  3. ^ Van Altena W. F., Lee J. T., Hoffleit E. D. (1995). "GCTP 2553". The General Catalogue of Trigonometric Stellar Parallaxes (Fourth ed.). Retrieved 2014-06-04. 
  4. ^ van Leeuwen F. (2007). "HIP 54035". Validation of the new Hipparcos reduction. Retrieved 2014-06-04. 
  5. ^ Van Altena W. F., Lee J. T., Hoffleit E. D. (1995). "GCTP 343.1". The General Catalogue of Trigonometric Stellar Parallaxes (Fourth ed.). Retrieved 2014-06-05. 
  6. ^ van Leeuwen F. (2007). "HIP 92403". Validation of the new Hipparcos reduction. Retrieved 2014-06-05. 
  7. ^ Boffin, Henri M. J.; Pourbaix, D.; Mužić, K.; Ivanov, V.D.; Kurtev, R.; Beletsky, Y.; Mehner, A.; Berger, J. P.; Girard, J. H.; Mawet, D. (January 2014). "Possible astrometric discovery of a substellar companion to the closest binary brown dwarf system WISE J104915.57-531906.1". Astronomy and Astrophysics 561: L4. arXiv:1312.1303. Bibcode:2014A&A...561L...4B. doi:10.1051/0004-6361/201322975.  edit
  8. ^ Luhman, K. L.; Esplin, T. L. (2014). "A New Parallax Measurement for the Coldest Known Brown Dwarf". The Astrophysical Journal 796 (1): 6. arXiv:1409.5899. Bibcode:2014ApJ...796....6L. doi:10.1088/0004-637X/796/1/6.