GJ 1061

GJ 1061 is a red dwarf star located 12 light-years (3.7 parsecs) from Earth in the southern constellation of Horologium. Even though it is a relatively nearby star, it has an apparent visual magnitude of about 13, so it can only be seen with at least a moderately-sized telescope.

GJ 1061
GJ 1061
Location of GJ 1061 in the constellation Horologium

Observation data
Epoch J2000      Equinox J2000
Constellation Horologium
Right ascension 03h 35m 59.69916s
Declination −44° 30 45.7308
Apparent magnitude (V) 13.03
Characteristics
Spectral type M5.5 V
Apparent magnitude (J) 7.52 ± 0.02
U−B color index 1.52
B−V color index 1.90
Astrometry
Radial velocity (Rv)1.49±0.23 km/s
Proper motion (μ) RA: 745.654 mas/yr
Dec.: −373.323 mas/yr
Parallax (π)272.1615 ± 0.0316 mas
Distance11.984 ± 0.001 ly
(3.6743 ± 0.0004 pc)
Absolute magnitude (MV)15.26
Details
Mass0.125±0.003 M
Radius0.152±0.007 R
Luminosity (bolometric)0.001641±0.000037 L
Luminosity (visual, LV)0.00007 L
Temperature2,977+72
−69
 K
Metallicity [Fe/H]−0.03±0.09 dex
Rotational velocity (v sin i)≤ 5 km/s
Age>7.0±0.5 Gyr
Other designations
GJ 1061, LHS 1565, LFT 295, LTT 1702, LP 995-46, L 372-58
Database references
SIMBADdata

The proper motion of GJ 1061 has been known since 1974, but it was estimated to be further away: approximately 25 light-years (7.7 parsecs) distant based upon an estimated parallax of 0.130″. The RECONS accurately determined its distance in 1997. At that time, it was the 20th-nearest star system to the Sun. The discovery team noted that many more stars like this are likely to be discovered nearby.

This star is a tiny, dim, red dwarf, close to the lower mass limit. It has an estimated mass of about 12.5% that of the Sun and is only about 0.2% as luminous. The star displays no significant infrared excess due to circumstellar dust.

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