Tau5 Serpentis
For other stars with this Bayer designation, see Tau Serpentis.
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Serpens |
Right ascension | 15h 36m 29.2391s[1] |
Declination | +16° 07′ 08.705″[1] |
Apparent magnitude (V) | 5.938[1] |
Characteristics | |
Spectral type | F3V[1] |
U−B color index | +0.04[2] |
B−V color index | +0.29[2] |
Astrometry | |
Radial velocity (Rv) | −2 ± 5[1] km/s |
Proper motion (μ) | RA: 71.54[1] mas/yr Dec.: −5.54[1] mas/yr |
Parallax (π) | 20.40 ± 0.81[1] mas |
Distance | 160 ± 6 ly (49 ± 2 pc) |
Absolute magnitude (MV) | 2.49[3] |
Details | |
Mass | 1.52 (1.47 to 1.58)[4] M☉ |
Temperature | 6900[4] K |
Metallicity | [Fe/H] = −0.20[4] |
Age | (1.6 ± 0.1) × 109 [4] years |
Other designations | |
Database references | |
SIMBAD | data |
Tau5 Serpentis (Tau5 Ser, τ5 Serpentis, τ5 Ser) is a F-type main sequence star in the constellation of Serpens, approximately 160 light-years from Earth.[1] It has an apparent visual magnitude of approximately 5.938.[1]
References
- 1 2 3 4 5 6 7 8 9 10 11 * 18 Ser -- Star, database entry, SIMBAD. Accessed on line September 19, 2008.
- 1 2 HR 5804, database entry, The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version), D. Hoffleit and W. H. Warren, Jr., CDS ID V/50. Accessed on line September 19, 2008.
- ↑ From apparent magnitude and parallax.
- 1 2 3 4 HD 139225, database entry, Geneva-Copenhagen Survey of the Solar neighbourhood, J. Holmberg et al., 2007, CDS ID V/117A. Accessed on line November 19, 2008.
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