Tau7 Serpentis
For other stars with this Bayer designation, see Tau Serpentis.
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
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Constellation | Serpens |
Right ascension | 15h 41m 54.7132s[1] |
Declination | +18° 27′ 50.532″[1] |
Apparent magnitude (V) | 5.804[1] |
Characteristics | |
Spectral type | A8Vam[2] |
U−B color index | +0.11[3] |
B−V color index | +0.20[3] |
R−I color index | +0.10[3] |
Astrometry | |
Radial velocity (Rv) | −29.5 ± 2[1] km/s |
Proper motion (μ) | RA: −73.00[1] mas/yr Dec.: 56.85[1] mas/yr |
Parallax (π) | 18.78 ± 0.82[1] mas |
Distance | 174 ± 8 ly (53 ± 2 pc) |
Absolute magnitude (MV) | 2.17[4] |
Details | |
Rotational velocity (v sin i) | 20[3] km/s |
Other designations | |
Database references | |
SIMBAD | data |
Tau7 Serpentis (Tau7 Ser, τ7 Serpentis, τ7 Ser) is an A-type star in the constellation of Serpens, approximately 174 light-years from the Earth.[1] It has an apparent visual magnitude of approximately 5.804.[1]
References
- 1 2 3 4 5 6 7 8 9 10 * 22 Ser -- Star, database entry, SIMBAD. Accessed on line September 19, 2008.
- ↑ Barry, Don C. (1970). "Spectral Classification of a and F Stars". Astrophysical Journal Supplement 19: 281. Bibcode:1970ApJS...19..281B. doi:10.1086/190209.
- 1 2 3 4 HR 5845, 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.
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