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6 Serpentis

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Star in the constellation Serpens
6 Serpentis
Observation data
Epoch J2000      Equinox J2000
Constellation Serpens
Right ascension 15 21 01.99609
Declination +00° 42′ 55.2213″
Apparent magnitude (V) 5.382 (5.54 + 9.42)
Characteristics
Spectral type K3 III
B−V color index 1.224
Astrometry
Radial velocity (Rv)+9.7±0.3 km/s
Proper motion (μ) RA: −42.36 mas/yr
Dec.: −103.14 mas/yr
Parallax (π)13.63 ± 0.73 mas
Distance240 ± 10 ly
(73 ± 4 pc)
Absolute magnitude (MV)1.03
Details
6 Ser A
Mass1.27 M
Radius12 R
Luminosity55 L
Surface gravity (log g)2.4 cgs
Temperature4,417±17 K
Metallicity −0.02 dex
Rotational velocity (v sin i)2.4 km/s
Age6.03 Gyr
Other designations
6 Ser, BD+01° 3067, HD 136514, HIP 75119, HR 5710, SAO 120955, ADS 9596, WDS J15210+0043
Database references
SIMBADdata

6 Serpentis is a binary star system in the constellation Serpens. It has a combined apparent visual magnitude of 5.382, which is bright enough to be faintly visible to the naked eye. The distance to this system, based upon an annual parallax shift of 13.63±0.73 mas, is about 240 light years. It is moving further from the Sun with a heliocentric radial velocity of +10 km/s.

The primary, component A, is an evolved red giant of spectral type K3III, a star that has used up its core hydrogen and has expanded. At the age of around six billion years it is a red clump star, indicating it is on the horizontal branch and is generating energy through helium fusion at its core. The star has 1.27 times the mass of the Sun and has expanded to 12 times the Sun's radius. It is radiating 55 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,417 K.

As of 2005, the magnitude 9.42 secondary, component B, was at an angular separation of 3.329″±0.017″ along a position angle of 21.8°±0.3°.

References

  1. ^ van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357, S2CID 18759600.
  2. ^ Luck, R. Earle (September 2015), "Abundances in the Local Region. I. G and K Giants", The Astronomical Journal, 150 (3): 23, arXiv:1507.01466, Bibcode:2015AJ....150...88L, doi:10.1088/0004-6256/150/3/88, S2CID 118505114, 88.
  3. ^ Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society, 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
  4. ^ de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics, 546: 14, arXiv:1208.3048, Bibcode:2012A&A...546A..61D, doi:10.1051/0004-6361/201219219, S2CID 59451347, A61.
  5. 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.
  6. ^ Massarotti, Alessandro; et al. (January 2008), "Rotational and Radial Velocities for a Sample of 761 Hipparcos Giants and the Role of Binarity", The Astronomical Journal, 135 (1): 209–231, Bibcode:2008AJ....135..209M, doi:10.1088/0004-6256/135/1/209, S2CID 121883397.
  7. ^ Laney, C. D.; et al. (2012), "A new Large Magellanic Cloud K-band distance from precision measurements of nearby red clump stars", Monthly Notices of the Royal Astronomical Society, 419 (2): 1637, arXiv:1109.4800, Bibcode:2012MNRAS.419.1637L, doi:10.1111/j.1365-2966.2011.19826.x, S2CID 117788450.
  8. "6 Ser". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-03-19.
  9. Alves, David R. (August 2000), "K-Band Calibration of the Red Clump Luminosity", The Astrophysical Journal, 539 (2): 732–741, arXiv:astro-ph/0003329, Bibcode:2000ApJ...539..732A, doi:10.1086/309278, S2CID 16673121.
  10. Scardia, M.; et al. (January 2007), "Speckle observations with PISCO in Merate - III. Astrometric measurements of visual binaries in 2005 and scale calibration with a grating mask" (PDF), Monthly Notices of the Royal Astronomical Society, 374 (3): 965–978, Bibcode:2007MNRAS.374..965S, doi:10.1111/j.1365-2966.2006.11206.x.
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