Astronomy:HD 221246

From HandWiki
Short description: Star in the open cluster NGC 7686
HD 221246
Observation data
Equinox J2000.0]] (ICRS)
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[2] mas
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

  1. ↑ 1.0 1.1 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A  XHIP record for this object at VizieR.
  2. ↑ 2.0 2.1 2.2 2.3 2.4 2.5 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.
  3. ↑ 3.0 3.1 3.2 3.3 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. ↑ 4.0 4.1 Shenavrin, V. I. et al. (2011). "Search for and study of hot circumstellar dust envelopes". Astronomy Reports 55 (1): 31–81. doi:10.1134/S1063772911010070. Bibcode: 2011ARep...55...31S. 
  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. doi:10.1051/0004-6361:20041272. Bibcode: 2005A&A...430..165F. 
  6. ↑ 6.0 6.1 6.2 6.3 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. doi:10.1051/0004-6361/202141828. Bibcode: 2022A&A...662A.125F. 
  7. ↑ Stassun, Keivan G. et al. (2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal 158 (4): 138. doi:10.3847/1538-3881/ab3467. Bibcode: 2019AJ....158..138S. 
  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. doi:10.1093/mnras/stv503. Bibcode: 2015MNRAS.449.2853R. 



Retrieved from "https://handwiki.org/wiki/index.php?title=Astronomy:HD_221246&oldid=3932059"