Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Serpens |
Right ascension | 18h 19m 50.8412s[1] |
Declination | −01° 56′ 19.005″[1] |
Apparent magnitude (V) | 9.66[2] (9.65–9.69)[3] |
Characteristics | |
Spectral type | K7 Vk[4] |
U−B color index | +1.26[2] |
B−V color index | +1.37[2] |
Variable type | Suspected[3] |
Astrometry | |
Radial velocity (Rv) | −14.53±0.44[5] km/s |
Proper motion (μ) | RA: −0.414±0.019[5] mas/yr Dec.: −0.108±0.017[5] mas/yr |
Parallax (π) | 52.3963 ± 0.0171 mas[5] |
Distance | 62.25 ± 0.02 ly (19.085 ± 0.006 pc) |
Absolute magnitude (MV) | 8.20[6] (8.19–8.23)[note 1] |
Details | |
Mass | 0.57[7] M☉ |
Radius | 0.58[7] R☉ |
Luminosity (bolometric) | 0.091[7] L☉ |
Luminosity (visual, LV) | 0.045[note 2] L☉ |
Surface gravity (log g) | 4.66[7] cgs |
Temperature | 4,143[7] K |
Metallicity [Fe/H] | −0.11[7] dex |
Rotational velocity (v sin i) | 6.42±0.78[8] km/s |
Age | 300[9] Myr |
Other designations | |
Database references | |
SIMBAD | data |
ARICNS | data |
Gliese 710, or HIP 89825, is an orange 0.6 M☉ star in the constellation Serpens Cauda. It is projected to pass near the Sun in about 1.29 million years at a predicted minimum distance of 0.051 parsecs—0.1663 light-years (10,520 astronomical units)[5] (about 1.6 trillion km)—about 1/25th of the current distance to Proxima Centauri.[10] Such a distance would make for a similar brightness to the brightest planets, optimally reaching an apparent visual magnitude of about −2.7. The star's proper motion will peak around one arcminute per year,[11][12] a rate of apparent motion that would be noticeable over a human lifespan. This is a timeframe, based on data from Gaia DR3, well within the parameters of current models which cover the next 15 million years.
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