మూస:నక్షత్ర్ర వ్యవస్థలు 5 - 10 కాంతి సంవత్సరాల లోపల/doc

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Adopted distance estimates[మార్చు]

Object	Parallax, mas	Distance, pc	Distance, ly	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	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	Benedict et al. (1999)^[2]
Wolf 359	419.1 ± 2.1	2.386 ± 0.012	7.78 ± 0.04	van Altena et al. (1995)^[3]
Lalande 21185	392.64 ± 0.67	2.547 ± 0.004	8.307 ± 0.014	van Leeuwen (2007)^[4]
Luyten 726-8	373.7 ± 2.7	2.676 ± 0.019	8.73 ± 0.06	van Altena et al. (1995)^[5]
Ross 154	336.72 ± 2.03	2.97 ± 0.018	9.69 ± 0.06	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	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	Luhman & Esplin (2014)^[8]

For other distance estimates see articles on these objects.