Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Ursa Major |
Right ascension | 08h 41m 20.12866s[1] |
Declination | +59° 29′ 50.4441″[1] |
Apparent magnitude (V) | +15.05[2] |
Characteristics | |
Evolutionary stage | Main sequence |
Spectral type | dM5.5[3] |
Astrometry | |
Radial velocity (Rv) | +7.13±2.45[1] km/s |
Proper motion (μ) | RA: −260.276 mas/yr[1] Dec.: −1,279.562 mas/yr[1] |
Parallax (π) | 105.2935 ± 0.0313 mas[1] |
Distance | 30.976 ± 0.009 ly (9.497 ± 0.003 pc) |
Details[3] | |
Mass | 0.1254±0.0031 M☉ |
Radius | 0.1636±0.0023 R☉ |
Luminosity | 0.001574±0.000018 L☉ |
Surface gravity (log g) | 5.240±0.044 cgs |
Temperature | 3,081±51 K |
Metallicity [Fe/H] | −0.07±0.16 dex |
Rotation | 87±5 d[4] |
Rotational velocity (v sin i) | 2.0[5] km/s |
Age | 3–8[6] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
GJ 3512 is a nearby star in the northern circumpolar constellation of Ursa Major. It is invisible to the naked eye but can be observed using a telescope, having an apparent visual magnitude of +15.05.[2] The star is located at a distance of 31 light-years from the Sun based on parallax.[1] It has a high proper motion,[6] traversing the celestial sphere at the rate of 1.311″ yr−1.[8] The measurement of the star's radial velocity is poorly constrained, but it appears to be drifting further away at a rate of ~8 km/s.[9]
The stellar classification of GJ 3512 is dM5.5,[3] which determines this to be a small red dwarf star that is generating energy through core hydrogen fusion. It displays a moderate amount of magnetic activity with a Sun-like cycle lasting 14 years. A low-level variability lasting ~87 d matches the approximate rotation period.[4] The star has 12.5% of the mass of the Sun and 16% of the Sun's radius. It is radiating 1.6% of the luminosity of the Sun from its photosphere at an effective temperature of 3,081 K.[3]
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