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Tau6 Serpentis
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τ6 Serpentis
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Serpens[1]
Right ascension 15h 40m 59.1008s[2]
Declination +16° 01′ 28.517″[2]
Apparent magnitude (V) 6.000[2]
Characteristics
Spectral type G8III[2]
U−B color index +0.61[3]
B−V color index +0.90[3]
R−I color index +0.46[3]
Astrometry
Radial velocity (Rv)3.4±0.9[2] km/s
Proper motion (μ) RA: 22.16[2] mas/yr
Dec.: −16.80[2] mas/yr
Parallax (π)7.24±0.79 mas[2]
Distanceapprox. 450 ly
(approx. 140 pc)
Absolute magnitude (MV)−0.33[1]
Details
Mass3.2[4] M
Radius15[4] R
Luminosity137[4] L
Surface gravity (log g)2.64[4] cgs
Temperature5,126[4] K
Metallicity [Fe/H]−0.01[4] dex
Rotational velocity (v sin i)4,5[5] km/s
Age310[4] Myr
Other designations
τ6 Ser, 19 Serpentis, BD+16°2816, GC 21089, HD 140027, HIP 76810, HR 5840, SAO 101678, PPM 131601 τ6 Ser, Tau6 Serpentis, Tau6 Ser, 19 Serpentis, 19 Ser, BD+16 2816, GC 21089, HD 140027, HIP 76810, HR 5840, PPM 131601, SAO 101678.[2]
Database references
SIMBADdata

Tau6 Serpentis, Latinized from τ6 Serpentis, is a G-type giant star in the constellation of Serpens, approximately 450 light-years from the Earth.[2] It has an apparent visual magnitude of approximately 6.000,[2] and is a member of the Ursa Major Stream.[3]

References

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