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69 Virginis

From Wikipedia, the free encyclopedia
Star in the constellation Virgo
69 Virginis
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationVirgo
Right ascension13h 27m 27.16348s[1]
Declination−15° 58′ 24.8980″[1]
Apparent magnitude (V)4.76[2]
Characteristics
Evolutionary stagehorizontal branch
Spectral typeK0 III-IIIb CN1.5 CH0.5[3]
U−Bcolor index+1.06[4]
B−Vcolor index+1.09[4]
Astrometry
Radial velocity (Rv)−12.9±0.5[5] km/s
Proper motion (μ)RA: −121.016[1]mas/yr
Dec.: +21.197[1]mas/yr
Parallax (π)12.5871±0.2367 mas[1]
Distance259 ± 5 ly
(79 ± 1 pc)
Absolute magnitude (MV)0.09[2]
Details[6]
Mass3.51±0.94 M
Radius15[7] R
Luminosity87.1[7] L
Surface gravity (log g)2.70±0.11 cgs
Temperature4,909±92 K
Metallicity[Fe/H]0.11[8] dex
Rotational velocity (v sin i)4.3[7] km/s
Age288+343
−156
 Myr
Other designations
16 Vir,NSV 6253,BD+04°2604,GJ 9444,HD 116976,HIP 65639,HR 5068,SAO 157946[9]
Database references
SIMBADdata

69 Virginis is a single[10]star in thezodiacconstellation ofVirgo, located about 259 light years away. It is visible to the naked eye as a faint orange-hued star with anapparent visual magnitude of 4.76,[2] although it is a suspectedvariable that may range in magnitude from 4.75 down to 4.79.[11] This object is moving closer to the Earth with a heliocentricradial velocity of −13 km/s.[5] The light from this star ispolarized due to interveninginterstellar dust.[12]

This is anevolvedK-typegiant star with astellar classification ofK0 III-IIIb CN1.5 CH0.5,[3] showing overabundances of CN and CH molecules in thespectrum. It is ared clump giant, which indicates is on thehorizontal branch generating energy viahelium fusion at its core.[13] The star is about 288 million years old with 3.5[6] times themass of the Sun and 15[7] times theSun's radius. It is radiating 87[7] times theSun's luminosity from its enlargedphotosphere at aneffective temperature of 4,909 K.[6]

References

[edit]
  1. ^abcdeBrown, 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.
  2. ^abcAnderson, 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.
  3. ^abKeenan, 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. ^abHoffleit, Dorrit; Jaschek, Carlos (1991), "The Bright star catalogue",New Haven,Bibcode:1991bsc..book.....H
  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. ^abcFeuillet, Diane K.; et al. (2016), "Determining Ages of APOGEE Giants with Known Distances",The Astrophysical Journal,817 (1): 40,arXiv:1511.04088,Bibcode:2016ApJ...817...40F,doi:10.3847/0004-637x/817/1/40,S2CID 118675933.
  7. ^abcdeMassarotti, 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.
  8. ^Meléndez, J.; et al. (June 2008), "Chemical similarities between Galactic bulge and local thick disk red giant stars",Astronomy and Astrophysics,484 (3):L21 –L25,arXiv:0804.4124,Bibcode:2008A&A...484L..21M,doi:10.1051/0004-6361:200809398,S2CID 3201679.
  9. ^"69 Vir".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-02-10.
  10. ^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.
  11. ^Samus, N. N.; et al. (2017), "General Catalogue of Variable Stars",Astronomy Reports, 5.1,61 (1):80–88,Bibcode:2017ARep...61...80S,doi:10.1134/s1063772917010085,S2CID 125853869.
  12. ^Leroy, J. L. (July 1993), "A Polarimetric Investigation on Interstellar Dust Within 50-PARSECS from the Sun",Astronomy and Astrophysics,274 (1): 203,Bibcode:1993A&A...274..203L.
  13. ^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.
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