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1 Serpentis

From Wikipedia, the free encyclopedia
Red giant star in the constellation Virgo
1 Serpentis
Location of 1 Serpentis (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationVirgo[1]
Right ascension14h 57m 33.251s[2]
Declination−00° 10′ 03.40″[2]
Apparent magnitude (V)5.5[3]
Characteristics
Evolutionary stageRed clump[4]
Spectral typeK1III[5]
Astrometry
Radial velocity (Rv)20.12[6] km/s
Proper motion (μ)RA: +59.929[2]mas/yr
Dec.: −26.500[2]mas/yr
Parallax (π)10.1280±0.1010 mas[2]
Distance322 ± 3 ly
(98.7 ± 1.0 pc)
Absolute magnitude (MV)+0.76[1]
Details
Mass1.37[3] M
Radius13.6[2] R
Luminosity75[2] L
Surface gravity (log g)2.5[6] cgs
Temperature4,581[6] K
Metallicity[Fe/H]−0.07[6] dex
Rotational velocity (v sin i)3.4[6] km/s
Age4.58[4] Gyr
Other designations
1 Ser,BD+00°3277,GJ 3881,HD 132132,HIP 73193,HR 5573,SAO 120758
Database references
SIMBADdata

1 Serpentis (1 Ser) is ared giant in theconstellationVirgo with anapparent magnitude of 5.5. It is ared clump giant, a coolhorizontal branch star that is fusing helium in its core.[4] It has expanded to over 13 times the radius of theSun and although it is cooler at4,581 K it is 77 times more luminous. It is 322 light years away.

TheFlamsteed designation 1 Serpentis was given to the star when the constellationSerpens was combined with the constellationOphiuchus.[7] It was also given theBayer designationM Serpentis. When Ophiuchus and Serpens were separated into distinct constellations, 1 Serpentis was left over the border inLibra. Since then it has moved slightly and is now inVirgo.[8]

A 10th-magnitude companion star discovered byWilliam Herschel is86 away.[9] It is at the same distance as 1 Ser and shares acommon proper motion,[10] It is considered likely to be a physical companion,[11] with the two stars separated by8,600 au.[12] It has a spectral type of G5 IV,[12] and it is slightly smaller and less luminous than the sun.[10]

A much more widely-separated 10th-magnitude star is also listed in multiple star catalogues,[9] but it is an unrelated background object.[13]

References

[edit]
  1. ^abAnderson, 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. XHIP record for this object atVizieR.
  2. ^abcdefgVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  3. ^abLuck, R. Earle; Heiter, Ulrike (2007)."Giants in the Local Region".The Astronomical Journal.133 (6): 2464.Bibcode:2007AJ....133.2464L.doi:10.1086/513194.
  4. ^abcSoubiran, C.; Bienaymé, O.; Mishenina, T. V.; Kovtyukh, V. V. (2008). "Vertical distribution of Galactic disk stars. IV. AMR and AVR from clump giants".Astronomy and Astrophysics.480 (1): 91.arXiv:0712.1370.Bibcode:2008A&A...480...91S.doi:10.1051/0004-6361:20078788.S2CID 16602121.
  5. ^Houk, N.; Swift, C. (1999). "Michigan Catalogue of Two-dimensional Spectral Types for the HD Stars, Vol. 5".Michigan Spectral Survey.5.Bibcode:1999MSS...C05....0H.
  6. ^abcdeMassarotti, Alessandro; Latham, David W.; Stefanik, Robert P.; Fogel, Jeffrey (2008)."Rotational and Radial Velocities for a Sample of 761 HIPPARCOS Giants and the Role of Binarity".The Astronomical Journal.135 (1): 209.Bibcode:2008AJ....135..209M.doi:10.1088/0004-6256/135/1/209.S2CID 121883397.
  7. ^Ian Rdipath."Serpens, the serpent". Retrieved2019-08-28.
  8. ^Hoffleit, Dorrit; Jaschek, Carlos (1991).The Bright star catalogue.Bibcode:1991bsc..book.....H.
  9. ^abMason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (2001)."The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog".The Astronomical Journal.122 (6): 3466.Bibcode:2001AJ....122.3466M.doi:10.1086/323920.
  10. ^abBrown, 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 atVizieR.
  11. ^Eggleton, P. P.; Tokovinin, A. A. (2008)."A catalogue of multiplicity among bright stellar systems".Monthly Notices of the Royal Astronomical Society.389 (2): 869.arXiv:0806.2878.Bibcode:2008MNRAS.389..869E.doi:10.1111/j.1365-2966.2008.13596.x.
  12. ^abStephenson, C. B. (1960). "A study of visual binaries having primaries above the main sequence".The Astronomical Journal.65: 60.Bibcode:1960AJ.....65...60S.doi:10.1086/108191.
  13. ^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 atVizieR.
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