Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Serpens |
Right ascension | 15h 36m 29.240s[1] |
Declination | +16° 07′ 08.70″[1] |
Apparent magnitude (V) | 5.93[2] |
Characteristics | |
Spectral type | F3V[3] |
U−B color index | +0.04[4] |
B−V color index | +0.354±0.004[2] |
Astrometry | |
Radial velocity (Rv) | −2.0±3.7[5] km/s |
Proper motion (μ) | RA: 72.175 mas/yr[1] Dec.: −5.217 mas/yr[1] |
Parallax (π) | 19.2694 ± 0.0392 mas[1] |
Distance | 169.3 ± 0.3 ly (51.9 ± 0.1 pc) |
Absolute magnitude (MV) | +2.35[2] |
Details | |
Mass | 1.54[5] M☉ |
Luminosity | 10[2] L☉ |
Surface gravity (log g) | 3.96[5] cgs |
Temperature | 6,903±80[5] K |
Metallicity [Fe/H] | −0.20[5] dex |
Rotational velocity (v sin i) | 88±10[6] km/s |
Age | 1.90[5] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Tau5 Serpentis, Latinized from τ5 Serpentis, is a star in the constellation of Serpens. The Flamsteed designation for this star is 18 Serpentis.[3] It has an apparent visual magnitude of 5.93,[2] which is bright enough to be dimly visible to the naked eye. The star is located at a distance of 169 light years from the Sun based on parallax measurements.[1]
The stellar classification of this star is F3V,[3] matching an F-type main-sequence star. It has 1.54 times the mass of the Sun[5] and is radiating 10[2] times the Sun's luminosity from its photosphere at an effective temperature of 6,903 K.[5] The star has an estimated age of 1.9 billion years[5] and is spinning with a projected rotational velocity of about 88 km/s.[6] It is metal poor, which means the abundance of iron in the stellar atmosphere is lower than in the Sun.[5]
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