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Tau8 Serpentis

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Star in the constellation Serpens For other stars with this Bayer designation, see Tau Serpentis.
Tau8 Serpentis
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Serpens
Right ascension 15 44 42.1323
Declination +17° 15′ 51.197″
Apparent magnitude (V) 6.144
Characteristics
Spectral type A0V
U−B color index −0.03
B−V color index 0.00
Astrometry
Radial velocity (Rv)−5.2 ± 5 km/s
Proper motion (μ) RA: −30.44 mas/yr
Dec.: 6.59 mas/yr
Parallax (π)10.16 ± 0.79 mas
Distance320 ± 20 ly
(98 ± 8 pc)
Absolute magnitude (MV)0.88
Details
Radius2.0 R
Rotational velocity (v sin i)76 km/s
Other designations
τ Ser, Tau Ser, 26 Serpentis, BD+17° 2906, GC 21164, HD 140729, HIP 77111, HR 5858, SAO 101712, PPM 131656
Database references
SIMBADdata

Tau Serpentis, Latinized from τ Serpentis, is an A-type main sequence star in the constellation of Serpens, approximately 320 light-years from the Earth. It has an apparent visual magnitude of approximately 6.144. Although it was observed to be binary by speckle interferometry in 1985, subsequent observations show no sign of binarity, and the detection appears to have been spurious.

References

  1. ^ * 26 Ser -- Star, database entry, SIMBAD. Accessed on line September 19, 2008.
  2. ^ HR 5858, 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.
  3. Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv:1108.4971, Bibcode:2012AstL...38..331A, doi:10.1134/S1063773712050015, S2CID 119257644.
  4. HD 140729, database entry, Catalog of Apparent Diameters and Absolute Radii of Stars (CADARS), 3rd edition, L. E. Pasinetti-Fracassini, L. Pastori, S. Covino, and A. Pozzi, CDS ID II/224. Accessed on line September 19, 2008.
  5. ICCD speckle observations of binary stars. X - A further survey for duplicity among the bright stars, Harold A. McAlister, Brian D. Mason, William I. Hartkopf, and Michael M. Shara, Astronomical Journal 106, #4 (October 1993), pp. 1639–1655, doi:10.1086/116753, Bibcode:1993AJ....106.1639M.
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