Astronomy: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 |
Distance | 910 ± 20 ly (278 ± 7 pc) |
Absolute magnitude (MV) | −0.80[6] |
Details | |
Radius | 40.78+3.27 −7.51[1] R☉ |
Luminosity | 496±15[1] L☉ |
Temperature | 4,267+457 −162[1] K |
Metallicity [Fe/H] | −0.22±0.09[7] dex |
Other designations | |
Database references | |
SIMBAD | data |
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
- ↑ 1.0 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. Bibcode: 2018A&A...616A...1G. Gaia DR2 record for this source at VizieR.
- ↑ 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, Bibcode: 1966CoLPL...4...99J.
- ↑ 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, Bibcode: 2013A&A...552A..64S.
- ↑ 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, Bibcode: 2017ARep...61...80S.
- ↑ 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, Bibcode: 2007A&A...474..653V.
- ↑ Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A.
- ↑ 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, Bibcode: 1999A&AS..134..523T.
- ↑ "HD 223311". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+223311.
- ↑ 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, Bibcode: 2010A&A...524A..10C.
- ↑ Blow, G. L. et al. (November 1982), "Photoelectric observations of lunar occultations. XIII", Astronomical Journal 87: 1571–1584, doi:10.1086/113247, Bibcode: 1982AJ.....87.1571B.
External links
Original source: https://en.wikipedia.org/wiki/HD 223311.
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