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HD 221246

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HD 221246
Observation data
Epoch J2000      Equinox J2000
Constellation Andromeda[1]
Right ascension 23h 30m 07.4133s[2]
Declination +49° 07′ 59.323″[2]
Apparent magnitude (V) 6.17[3]
Characteristics
Spectral type K3III[4]
U−B color index 1.71[3]
B−V color index 1.46[3]
Astrometry
Radial velocity (Rv)−8.41±0.15[5] km/s
Proper motion (μ) RA: 28.741±0.100[2] mas/yr
Dec.: 3.180±0.087[2] mas/yr
Parallax (π)3.2290±0.0642 mas[2]
Distance1,010 ± 20 ly
(310 ± 6 pc)
Absolute magnitude (MV)−0.97[1]
Details
Mass1.4[6] M☉
Radius44[7] R☉
Luminosity690[6] L☉
Surface gravity (log g)1.20[6] cgs
Temperature4,285[6] K
Metallicity [Fe/H]−0.24±0.10[8] dex
Other designations
BD+48°4070, FK5 3882, HD 221246, HIP 115996, HR 8925, NGC 7686 1, SAO 53088
Database references
SIMBADdata

HD 221246 or NGC 7686 1 is a star in open cluster NGC 7686, and it belongs to the northern constellation of Andromeda. With an apparent visual magnitude of 6.17,[3] it can be viewed by the naked eye only under very favourable conditions. It has a spectral classification of K3III, meaning it is an evolved orange giant star.[4] Parallax measurements place this star about 1,000 light years away from the Solar System.[2]

References

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  1. ^ a b Anderson, 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 at VizieR.
  2. ^ a b c d e f 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 at VizieR.
  3. ^ a b c d 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
  4. ^ a b Shenavrin, V. I.; et al. (2011). "Search for and study of hot circumstellar dust envelopes". Astronomy Reports. 55 (1): 31–81. Bibcode:2011ARep...55...31S. doi:10.1134/S1063772911010070. S2CID 122700080.
  5. ^ Famaey, B.; Jorissen, A.; Luri, X.; Mayor, M.; Udry, S.; Dejonghe, H.; Turon, C. (2005). "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters". Astronomy and Astrophysics. 430: 165–186. arXiv:astro-ph/0409579. Bibcode:2005A&A...430..165F. doi:10.1051/0004-6361:20041272. S2CID 17804304.
  6. ^ a b c d Fouesneau, M.; Andrae, R.; Dharmawardena, T.; Rybizki, J.; Bailer-Jones, C. A. L.; Demleitner, M. (2022). "Astrophysical parameters from Gaia DR2, 2MASS, and AllWISE". Astronomy and Astrophysics. 662: A125. arXiv:2201.03252. Bibcode:2022A&A...662A.125F. doi:10.1051/0004-6361/202141828.
  7. ^ Stassun, Keivan G.; et al. (2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv:1905.10694. Bibcode:2019AJ....158..138S. doi:10.3847/1538-3881/ab3467.
  8. ^ Röck, B.; Vazdekis, A.; Peletier, R. F.; Knapen, J. H.; Falcón-Barroso, J. (2015). "Stellar population synthesis models between 2.5 and 5 μm based on the empirical IRTF stellar library". Monthly Notices of the Royal Astronomical Society. 449 (3): 2853. arXiv:1505.01837. Bibcode:2015MNRAS.449.2853R. doi:10.1093/mnras/stv503.
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