Gliese 1061

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Coordinates: Sky map 03h 35m 59.69s, −44° 30′ 45.3″

Gliese 1061
Observation data
Epoch J2000      Equinox J2000
Constellation Horologium
Right ascension 03h 35m 59.69s[1]
Declination −44° 30′ 45.3″[1]
Apparent magnitude (V) 13.03[2]
Characteristics
Spectral type M5.5 V[2]
Apparent magnitude (J) 7.52 ± 0.02[3]
U−B color index 1.52[3]
B−V color index 1.90[3]
Astrometry
Radial velocity (Rv)−8 km/s
Proper motion (μ) RA: 750.01[4] mas/yr
Dec.: -349.98[5] mas/yr
Parallax (π)272.1615 ± 0.0316[6] mas
Distance11.984 ± 0.001 ly
(3.6743 ± 0.0004 pc)
Absolute magnitude (MV)15.26[4]
Details
Mass0.113[5] M
Radius0.156±0.005 − 0.19[7] R
Luminosity (bolometric)0.0017±0.0001 − 0.003[7] L
Luminosity (visual, LV)0.00007[nb 1] L
Temperature2953±982999±41[7] K
Metallicity [Fe/H]−0.09±0.09[8] dex
Rotational velocity (v sin i)≤ 5[9] km/s
Age>7.0±0.5[7] Gyr
Other designations
GJ 1061, LHS 1565, LFT 295, LTT 1702, LP 995-46, L 372-58[3]
Database references
SIMBADdata
Gliese 1061 is located in the constellation Horologium.
Gliese 1061 is located in the constellation Horologium.
Gliese 1061
Location of Gliese 1061 in the constellation Horologium

Gliese 1061 is a red dwarf star located approximately 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,[2] so it can only be seen with at least a moderately-sized telescope.

The proper motion of Gliese 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.[2]

This star is a tiny, dim, red dwarf, close to the lower mass limit. It has an estimated mass of about 11.3% of the Sun and is only about 0.2% as luminous.[5][7] The star displays no significant infrared excess due to circumstellar dust.[10]

Planetary system[]

Orbits of the exoplanets in the Gliese 1061 system compared to the HZ. Gliese 1061 b has the innermost orbit, Gliese 1061 c the intermediate one, and Gliese 1061 d the outermost.

On August 13, 2019, a planetary system was announced orbiting the star Gliese 1061 by the Red Dots project of detecting terrestrial planets around nearby red dwarf stars.[7] The planet Gliese 1061 d orbits in the conservative circumstellar habitable zone of its star and the planet Gliese 1061 c orbits in the inner edge of the habitable zone.[7] Gliese 1061 is a non-variable star that does not suffer flares, so there is a greater probability that the exoplanets still conserve their atmosphere if they had one.[11]

The Gliese 1061 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 1.38+0.16
−0.15
 M
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