13 Monocerotis

Star in the constellation Monoceros From Wikipedia, the free encyclopedia

13 Monocerotis (13 Mon) is a class A0 Ib (white supergiant) star in the constellation Monoceros. Its apparent magnitude is 4.5 and it is approximately 780 parsecs (2,500 ly) away.

Right ascension06h 32m 54.22948s[1]
Declination07° 19′ 58.6942″[1]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
13 Monocerotis
Location of 13 Monocerotis (circled red)
Observation data
Epoch J2000      Equinox J2000
Constellation Monoceros
Right ascension 06h 32m 54.22948s[1]
Declination 07° 19′ 58.6942″[1]
Apparent magnitude (V) 4.498[2]
Characteristics
Spectral type A0 Ib[2]
U−B color index −0.217[2]
B−V color index +0.007[2]
Variable type suspected[3]
Astrometry
Radial velocity (Rv)+11.80[4] km/s
Proper motion (μ) RA: -0.20[1] mas/yr
Dec.: -3.48[1] mas/yr
Parallax (π)0.83±0.46 mas[1]
Distance780[5] pc
Absolute magnitude (MV)−4.80[6]
Details
Mass12.0[7] M☉
Radius38 ± 4[8][a] R☉
Luminosity14,100+2,900
−2,400
[8] L☉
Surface gravity (log g)2.15[2] cgs
Temperature10,250±200[8] K
Metallicity [Fe/H]−0.18[9] dex
Rotational velocity (v sin i)0[2] km/s
Age16[7] Myr
Other designations
BD+07 1337, FK5 1174, GC 8506, HIP 31216, HR 2385, HD 46300, NSV 16904, SAO 114034
Database references
SIMBADdata
Close

13 Mon lies within the Monoceros OB1 stellar association,[6] halfway between the Rosette Nebula and NGC 2264, at a distance of about 780 parsecs.[5] It is surrounded by a small reflection nebula listed as Van den Bergh 81 (VdB 81).[10]

13 Monocerotis has been used as a standard star for the A0 Ib spectral class.[11]

Extended photometry of 13 Monocerotis from 1997 to 2000 shows irregular variation of up to 0.04 magnitudes and also a slight trend to become fainter over the period.[12] All the bright A0 - A5 supergiants analysed using Hipparcos satellite data were found to be variable, but 13 Mon was the least variable.[13]

Notes

  1. Applying the Stefan–Boltzmann law with a nominal solar effective temperature of 5,772 K:
    .

References

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