Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Eridanus |
Right ascension | 03h 38m 15.69799s[1] |
Declination | −11° 29′ 13.5050″[1] |
Apparent magnitude (V) | +13.010[2] |
Characteristics | |
Spectral type | M2.5VI[3] |
U−B color index | +1.385[4] |
B−V color index | +1.605[4] |
R−I color index | 1.184[2] |
Astrometry | |
Radial velocity (Rv) | −84.88±0.56[1] km/s |
Proper motion (μ) | RA: 1,458.201 mas/yr[1] Dec.: −2,696.545 mas/yr[1] |
Parallax (π) | 61.8861 ± 0.0220 mas[1] |
Distance | 52.70 ± 0.02 ly (16.159 ± 0.006 pc) |
Absolute magnitude (MV) | 10.608[5] |
Details | |
Mass | 0.255[6] M☉ |
Radius | 0.411±0.051 R☉[2] 0.372±0.076 R☉[5] 0.202±0.012[7] R☉ |
Luminosity | 0.0055[2] L☉ |
Temperature | 3,488±50[2] K |
Metallicity [Fe/H] | −0.28±0.15[7] dex |
Rotational velocity (v sin i) | 9.80[2] km/s |
Other designations | |
Database references | |
SIMBAD | data |
ARICNS | data |
GJ 1062 is a single[6] red dwarf star in the constellation Eridanus, positioned about two degrees to the SSE of Epsilon Eridani.[9] It is also known as LHS 20 and Ross 578. The star is invisible to the naked eye with an apparent visual magnitude of +13.0,[2] requiring a telescope with at least a 25 cm (10 in) aperture to view.[10] It is located at a distance of 52.7 light years from the Sun based on parallax, but is drifting closer with a radial velocity of −85 km/s.[1] The star has a high proper motion, traversing the sky at the rate of 3.033 arcseconds per year.[11]
This is an M-type subdwarf star with a stellar classification of M2.5VI.[3] It was one of the first three subdwarfs to be definitively identified by G. Kuiper in 1940, the other two being Kapteyn's Star and Wolf 1106.[12] GJ 1062 is considered a likely member of the halo population, and thus is a MACHO.[13]
GaiaDR3
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