Misplaced Pages

16 Serpentis

Article snapshot taken from[REDACTED] with creative commons attribution-sharealike license. Give it a read and then ask your questions in the chat. We can research this topic together.
Binary star system in the constellation Serpens
16 Serpentis
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Serpens
Right ascension 15 36 29.57498
Declination 10° 00′ 36.5574″
Apparent magnitude (V) 5.261
Characteristics
Spectral type K0III: CN1 Ba0.7 Sr2
U−B color index +0.66
B−V color index +0.937
Astrometry
Radial velocity (Rv)+2.94±0.13 km/s
Proper motion (μ) RA: 41.881 mas/yr
Dec.: −125.722 mas/yr
Parallax (π)14.3226 ± 0.1100 mas
Distance228 ± 2 ly
(69.8 ± 0.5 pc)
Orbit
Period (P)5,324±19 d
Eccentricity (e)0.345±0.024
Periastron epoch (T)44,090±53
Argument of periastron (ω)
(secondary)
358±4°
Semi-amplitude (K1)
(primary)
3.86±0.09 km/s
Details
16 Ser A
Mass1.70 M
RadiusR
Luminosity42.7 L
Surface gravity (log g)2.64±0.12 cgs
Temperature4,946±51 K
Metallicity −0.13±0.06 dex
Rotational velocity (v sin i)1.4 km/s
Age2.40 Gyr
Other designations
16 Ser, BD+10°2884, FK5 3226, GC 20981, HD 139195, HIP 76425, HR 5802, SAO 101640
Database references
SIMBADdata

16 Serpentis is a binary star system in the Serpens Caput portion of the equatorial constellation of Serpens, located 228 light years from the Sun. It is visible to the naked eye as a fain, orange-hued star with an apparent visual magnitude of 5.261. The system is moving further from the Earth with a heliocentric radial velocity of +3 km/s.

The variable radial velocity of this star was discovered at Lick Observatory and was announced by J. H. Moore in 1924. It is a single-lined spectroscopic binary with an orbital period of 14.58 years and an eccentricity of 0.345. The visible component is an evolved giant star with a stellar classification of K0III: CN1 Ba0.7 Sr2. This is a mild barium star with the suffix notation above indicating associated abundance anomalies. The companion is a presumed white dwarf star that has already passed through its giant stage, during which time it enhanced the envelope of the companion with s-process elements. The pair form one of the widest barium star binaries known, which may account for the mildness of the barium anomaly.

References

  1. ^ Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  2. ^ Luck, R. Earle (2015). "Abundances in the Local Region. I. G and K Giants". Astronomical Journal. 150 (3). 88. arXiv:1507.01466. Bibcode:2015AJ....150...88L. doi:10.1088/0004-6256/150/3/88. S2CID 118505114.]
  3. ^ Keenan, Philip C.; McNeil, Raymond C. (1989). "The Perkins catalog of revised MK types for the cooler stars". Astrophysical Journal Supplement Series. 71: 245. Bibcode:1989ApJS...71..245K. doi:10.1086/191373.
  4. Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data. Bibcode:1986EgUBV........0M.
  5. ^ Griffin, R. F. (February 1991). "Spectroscopic binary orbits from photoelectric radial velocities. Paper 96: 16 Serpentis". The Observatory. 111: 29–37. Bibcode:1991Obs...111...29G.
  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.
  7. ^ Prugniel, Ph.; et al. (July 2011). "The atmospheric parameters and spectral interpolator for the MILES stars". Astronomy & Astrophysics. 531: A165. arXiv:1104.4952. Bibcode:2011A&A...531A.165P. doi:10.1051/0004-6361/201116769. S2CID 54940439.
  8. ^ "16 Ser". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-03-22.
  9. Tomkin, J.; Lambert, D. L. (1986). "Heavy-element abundances in the mild barium stars Omicron Virginis and 16 Serpentis". The Astrophysical Journal. 311: 819. Bibcode:1986ApJ...311..819T. doi:10.1086/164821.
Constellation of Serpens
Stars
Bayer
Flamsteed
Variable
HR
HD
Other
Exoplanets
Star
clusters
NGC
Other
Nebulae
Other
Galaxies
NGC
Other
Galaxy clusters
Astronomical events
Category
Categories:
16 Serpentis Add topic