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6 Persei

From Wikipedia, the free encyclopedia
Star in the constellation Andromeda
6 Persei
Location of 6 Persei (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationAndromeda[1]
Right ascension02h 13m 36.34084s[2]
Declination+51° 03′ 56.8222″[2]
Apparent magnitude (V)5.29[3]
Characteristics
Spectral typeG8.5 IIIb Fe-2[3]
B−Vcolor index0.926[4]
Astrometry
Radial velocity (Rv)+41.82±0.27[5] km/s
Proper motion (μ)RA: +344.397[2]mas/yr
Dec.: −164.853[2]mas/yr
Parallax (π)17.8901±0.0943 mas[2]
Distance182.3 ± 1.0 ly
(55.9 ± 0.3 pc)
Absolute magnitude (MV)+1.25±0.07[6]
Orbit[6]
Period (P)1,576.23±0.04 d
Eccentricity (e)0.8828±0.0007
Inclination (i)104°
Periastronepoch (T)2,450,307.31±0.12 JD
Argument of periastron (ω)
(secondary)
266.4±0.3°
Semi-amplitude (K1)
(primary)
19.82±0.06 km/s
Details[4]
Mass1.5 M
RadiusR
Luminosity26.3 L
Surface gravity (log g)3.0 cgs
Temperature4,920 K
Metallicity[Fe/H]−0.60 dex
Rotational velocity (v sin i)0.0 km/s
Other designations
NSV 747,AG+50°249,BD+50°481,FK5 77,HD 13530,HIP 10366,HR 645,SAO 23047,PPM 27263,WDS J02136+5104A[7]
Database references
SIMBADdata

6 Persei is abinary star[8] system in the northernconstellation ofAndromeda.[9] It is faintly visible to the naked eye with anapparent visual magnitude of 5.29.[3] The system is located 182 light years from Earth, as determined from its annualparallax shift of17.9 mas.[2] It is moving further away with a heliocentricradial velocity of +42 km/s.[5] The system has a relatively high rate ofproper motion, traversing thecelestial sphere at the rate of0.386 arcsecond/year.[10]

This is a single-linedspectroscopic binary with anorbital period of 4.3155 yr and aneccentricity of 0.88. Thea sini value for the primary is201.8±0.9 Gm, wherea is thesemimajor axis andi is theorbital inclination. The inclination is estimated to be 104°.[6]

The visible component is anevolvedgiant star with astellar classification ofG8.5 IIIb Fe-2,[3] where the suffix notation indicates an underabundance of iron in thespectrum. It has 1.5 times themass of the Sun and has expanded to 7 times theSun's radius. The star is radiating 26 times theSun's luminosity from its enlargedphotosphere at aneffective temperature of 4,920 K.[4] It has a magnitude 10.49 visual companion at anangular separation of108.9 along aposition angle of 57°, as of 2004.[11]

References

[edit]
  1. ^Roman, Nancy G. (1987)."Identification of a constellation from a position".Publications of the Astronomical Society of the Pacific.99 (617): 695.Bibcode:1987PASP...99..695R.doi:10.1086/132034. Constellation record for this object atVizieR.
  2. ^abcdefBrown, 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.
  3. ^abcdKeenan, 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. ^abcMassarotti, 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.
  5. ^abde 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.
  6. ^abcScarfe, C. D. (October 2017), "Spectroscopic Orbits of Three Binaries",Revista Mexicana de Astronomía y Astrofísica,53:333–347,Bibcode:2017RMxAA..53..333S.
  7. ^"HD 13530".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved20 August 2018.
  8. ^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.
  9. ^Sinnott, Roger W.; Perryman, Michael A. C. (1997),Millennium Star Atlas, vol. 1, Sky Publishing Corporation and the European Space Agency, p. 81,ISBN 0-933346-82-4.
  10. ^Lépine, Sébastien; Shara, Michael M. (March 2005), "A Catalog of Northern Stars with Annual Proper Motions Larger than 0.15" (LSPM-NORTH Catalog)",The Astronomical Journal,129 (3):1483–1522,arXiv:astro-ph/0412070,Bibcode:2005AJ....129.1483L,doi:10.1086/427854,S2CID 2603568.
  11. ^Mason, Brian D.; et al. (December 2001), "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog",The Astronomical Journal,122 (6):3466–3471,Bibcode:2017yCat....102026M,doi:10.1086/323920.
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