Astronomy:HD 223311

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Short description: Star in the constellation Aquarius
HD 223311
Observation data
Equinox J2000.0]] (ICRS)
Constellation Aquarius
Right ascension  23h 48m 32.47911s[1]
Declination −06° 22′ 49.5328″[1]
Apparent magnitude (V) 6.08[2]
Characteristics
Spectral type K4III[3]
U−B color index +1.71[2]
B−V color index +1.452[3]
Variable type suspected[4]
Astrometry
Radial velocity (Rv)−20.069±0.008[3] km/s
Proper motion (μ) RA: +0.01[5] mas/yr
Dec.: −19.04[5] mas/yr
Parallax (π)3.5950 ± 0.0884[1] mas
Distance910 ± 20 ly
(278 ± 7 pc)
Absolute magnitude (MV)−0.80[6]
Details
Radius40.78+3.27
−7.51
[1] R
Luminosity496±15[1] L
Temperature4,267+457
−162
[1] K
Metallicity [Fe/H]−0.22±0.09[7] dex
Other designations
NSV 14715, BD−07°6086, FK5 3912, HD 223311, HIP 117420, HR 9014, SAO 146919[8]
Database references
SIMBADdata

HD 223311 is a star in the equatorial constellation of Aquarius. It has an orange hue and is visible to the naked eye as a dim star with an apparent visual magnitude of 6.08.[2] Based on parallax measurements, the star is located at a distance of approximately 910 light years from the Sun. It is a radial velocity standard[9] star that is drifting closer to the Sun at the rate of −20 km/s.[3] The star is situated near the ecliptic and thus is subject to lunar occultations.[10]

This is an aging K-type giant star with a stellar classification of K4III.[3] Having exhausted the supply of hydrogen at its core, it has cooled and expanded off the main sequence. At present it has 41[1] times the girth of the Sun. It is a suspected variable star of unknown type that has been measured ranging in brightness from magnitude 5.01 down to 5.26 in the infrared I band.[4] The star is radiating 496 times the luminosity of the Sun from its swollen photosphere at an effective temperature of 4,267 K.[1]

References

  1. 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode2018A&A...616A...1G.  Gaia DR2 record for this source at VizieR.
  2. 2.0 2.1 2.2 Johnson, H. L. et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory 4 (99): 99, Bibcode1966CoLPL...4...99J. 
  3. 3.0 3.1 3.2 3.3 3.4 Soubiran, C. et al. (April 2013), "The catalogue of radial velocity standard stars for Gaia. I. Pre-launch release", Astronomy & Astrophysics 552: 11, doi:10.1051/0004-6361/201220927, A64, Bibcode2013A&A...552A..64S. 
  4. 4.0 4.1 Samus, N. N. et al. (2017), "General Catalogue of Variable Stars", Astronomy Reports, 5.1 61 (1): 80–88, doi:10.1134/S1063772917010085, Bibcode2017ARep...61...80S. 
  5. 5.0 5.1 van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics 474 (2): 653–664, doi:10.1051/0004-6361:20078357, Bibcode2007A&A...474..653V. 
  6. Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode2012AstL...38..331A. 
  7. Taylor, B. J. (February 1999), "Catalogs of temperatures and [Fe/H] averages for evolved G and K stars", Astronomy and Astrophysics Supplement 134 (3): 523–524, doi:10.1051/aas:1999153, Bibcode1999A&AS..134..523T. 
  8. "HD 223311". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+223311. 
  9. Crifo, F. et al. (December 2010), "Towards a new full-sky list of radial velocity standard stars", Astronomy and Astrophysics 524: 8, doi:10.1051/0004-6361/201015315, A10, Bibcode2010A&A...524A..10C. 
  10. Blow, G. L. et al. (November 1982), "Photoelectric observations of lunar occultations. XIII", Astronomical Journal 87: 1571–1584, doi:10.1086/113247, Bibcode1982AJ.....87.1571B. 

External links