13 Monocerotis
Star in the constellation Monoceros
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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.
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Monoceros |
| Right ascension | 06h 32m 54.22948s[1] |
| Declination | 07° 19â² 58.6942â³[1] |
| Apparent magnitude (V) | 4.498[2] |
| Characteristics | |
| Spectral type | A0 Ib[2] |
| UâB color index | â0.217[2] |
| BâV 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 (Ï) | 0.83±0.46 mas[1] |
| Distance | 780[5] pc |
| Absolute magnitude (MV) | â4.80[6] |
| Details | |
| Mass | 12.0[7] Mâ |
| Radius | 38 ± 4[8][a] Râ |
| Luminosity | 14,100+2,900 â2,400[8] Lâ |
| Surface gravity (log g) | 2.15[2] cgs |
| Temperature | 10,250±200[8] K |
| Metallicity [Fe/H] | â0.18[9] dex |
| Rotational velocity (v sin i) | 0[2] km/s |
| Age | 16[7] Myr |
| Other designations | |
| BD+07 1337, FK5 1174, GC 8506, HIP 31216, HR 2385, HD 46300, NSV 16904, SAO 114034 | |
| Database references | |
| SIMBAD | data |
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
- Applying the StefanâBoltzmann law with a nominal solar effective temperature of 5,772 K:
- .