12 Canis Majoris

12 Canis Majoris

A visual band light curve for HK Canis Majoris (2020)[1]
Observation data
Epoch J2000      Equinox J2000
Constellation Canis Major
Right ascension 06h 47m 01.48353s[2]
Declination −21° 00′ 55.4517″[2]
Apparent magnitude (V) +6.07[3]
Characteristics
Spectral type B7 II/III[4] or B5 V[5]
B−V color index −0.159±0.004[3]
Variable type SX Ari[6]
Astrometry
Radial velocity (Rv)+16.4±2.5[3] km/s
Proper motion (μ) RA: −14.568[2] mas/yr
Dec.: +5.778[2] mas/yr
Parallax (π)4.6155 ± 0.0543 mas
Distance707 ± 8 ly
(217 ± 3 pc)
Absolute magnitude (MV)−0.81[3]
Details
Mass4.8[7] M
Radius2.73[8] R
Luminosity537[9] L
Surface gravity (log g)4.23[5] cgs
Temperature15,830±60[9] K
Metallicity [Fe/H]−0.37[10] dex
Rotation2.18045 d[7]
Rotational velocity (v sin i)65[7] km/s
Age134[11] Myr
Other designations
12 Cep, HK CMa, BD−20°1576, FK5 817, GC 8884, HD 49333, HIP 32504, HR 2509, SAO 172318[12]
Database references
SIMBADdata

12 Canis Majoris is a variable star located about 707 light years away from the Sun in the southern constellation of Canis Major.[12] It has the variable star designation HK Canis Majoris; 12 Canis Majoris is the Flamsteed designation. This body is just barely visible to the naked eye as a dim, blue-white hued star with a baseline apparent visual magnitude of +6.07.[3] It is moving away from the Earth with a heliocentric radial velocity of +16 km/s.[3] This is the brightest star in the vicinity of the open cluster NGC 2287,[13] although it is probably not a member based on its proper motion.[14]

This star has a stellar classification of B7 II/III,[4] matching the spectrum of a B-type star intermediate between a giant and bright giant.[4] (Cidale et al. (2007) show a class of B5 V,[5] which would indicate it is instead a B-type main-sequence star.) It is a magnetic Bp star[15] of the helium–weak variety (CP4), with the spectrum displaying evidence for vertical stratification of helium in the atmosphere.[16] Samus et al. (2017) classify it as an SX Arietis variable that varies in brightness by about 0.05 magnitudes over a period of 2.18045 days.[6] It has 4.8 times the mass of the Sun and 2.73[8] times the Sun's radius. The star is radiating 537 times the Sun's luminosity from its photosphere at an effective temperature of 15,830 K.

  1. ^ Cite error: The named reference Bernhard was invoked but never defined (see the help page).
  2. ^ a b c d Cite error: The named reference GaiaDR3 was invoked but never defined (see the help page).
  3. ^ a b c d e f Cite error: The named reference Anderson2012 was invoked but never defined (see the help page).
  4. ^ a b c Cite error: The named reference houk1978 was invoked but never defined (see the help page).
  5. ^ a b c Cite error: The named reference Cidale2007 was invoked but never defined (see the help page).
  6. ^ a b Cite error: The named reference Samus2017 was invoked but never defined (see the help page).
  7. ^ a b c Cite error: The named reference schultz2022 was invoked but never defined (see the help page).
  8. ^ a b Cite error: The named reference Shulyak2014 was invoked but never defined (see the help page).
  9. ^ a b Cite error: The named reference Netopil2008 was invoked but never defined (see the help page).
  10. ^ Cite error: The named reference Mosser2005 was invoked but never defined (see the help page).
  11. ^ Cite error: The named reference gontcharov2012 was invoked but never defined (see the help page).
  12. ^ a b Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
  13. ^ Cite error: The named reference Feinstein1979 was invoked but never defined (see the help page).
  14. ^ Cite error: The named reference Levato1984 was invoked but never defined (see the help page).
  15. ^ Cite error: The named reference Bailey2013 was invoked but never defined (see the help page).
  16. ^ Cite error: The named reference Farthmann1994 was invoked but never defined (see the help page).

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