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HD 212710
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cepheus[1]
Right ascension 22h 13m 10.6136s[2]
Declination +86° 6′ 28.6366″[2]
Apparent magnitude (V) 5.258±0.009[3]
Characteristics
Spectral type B9.5 Vn[4]
U−B color index -0.11[5]
B−V color index -0.03[5]
Astrometry
Radial velocity (Rv)-6±5[6] km/s
Proper motion (μ) RA: 60.554±0.202[7] mas/yr
Dec.: 39.468±0.193[7] mas/yr
Parallax (π)12.8648 ± 0.1662 mas[7]
Distance254 ± 3 ly
(78 ± 1 pc)
Absolute magnitude (MV)0.79[8]
Details
Mass2.61+0.438
−0.254
[9] M
Radius2.387+0.086
−0.052
[9] R
Luminosity53.79±1.38[7] L
Surface gravity (log g)4.0991±0.0652[9] cgs
Temperature10162+164.7
−134
[9] K
Other designations
HIP 109693, HR 8546, AG+85 372, BD+85 383, HD 212710, SAO 3721, 2MASS J22131056+8606287, FK5 1648
Database references
SIMBADdata

HD 212710, also known as BD+85 383, SAO 3721, HR 8546, HIP 109693 is a star in Cepheus[1] with an apparent magnitude of 5.258[3] and a spectral type of B9.5 Vn,[4] indicating that it is a B-type main sequence star, giving it a blue hue. It's about 254 light-years far away from the solar system. It has about 2.61 times the mass of sun, 2.387 times the radius of sun and 53.79 times as luminous as sun.

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Transcription

Nomenclature

This star doesn't have a Bayer or Flamsteed designation.

It has a Chinese name, "Great Tianhuang Emperor" (Chinese: 天皇大帝, tiānhuángdàdì) which means "The Emperor of Heaven". It is an independent constellation in the system of Chinese constellations, belonging to the Purple Forbidden enclosure.[citation needed]

References

  1. ^ a b Roman, Nancy G. (1987). "Identification of a constellation from a position". Publications of the Astronomical Society of the Pacific. 99: 695. Bibcode:1987PASP...99..695R. doi:10.1086/132034. S2CID 120559848.
  2. ^ a b van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID 18759600.
  3. ^ a b Høg, E.; Fabricius, C.; Makarov, V. V.; Urdan, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 335: L27–L30. Bibcode:2000A&A...355L..27H.
  4. ^ a b Egret, D.; Didelon, P.; McLean, B. J.; Russell, J. L.; Turon, C. (1992). "The TYCHO Input Catalogue. Cross- matching the Guide Star Catalog with the HIPPARCOS INCA Data Base". Astronomy and Astrophysics. 258: 217–222. Bibcode:1992A&A...258..217E.
  5. ^ a b Mallama, A. (2018). "Erratum: Sloan Magnitudes for the Brightest Stars". The Journal of the American Association of Variable Star Observers. 46 (1): 90. arXiv:1805.09324. Bibcode:2018JAVSO..46...90M.
  6. ^ Gontcharov, G. A. (2006). "Pulkovo compilation of radial velocities for 35495 stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv:1606.08053. Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065. S2CID 119231169.
  7. ^ a b c d Gaia Collaboration (2022). "VizieR Online Data Catalog: Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022)". Astronomy and Astrophysics. Bibcode:2022yCat.1355....0G.
  8. ^ Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331–346. arXiv:1108.4971. Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. S2CID 255204555.
  9. ^ a b c d Paegert, Martin; Stassun, Keivan G.; Collins, Karen A.; Pepper, Joshua; Torres, Guillermo; Jenkins, Jon; Twicken, Joseph D.; Latham, David W. (2021). "TESS Input Catalog versions 8.1 and 8.2: Phantoms in the 8.0 Catalog and How to Handle Them". arXiv:2108.04778 [astro-ph.EP].
This page was last edited on 11 September 2023, at 08:44
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