Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Monoceros |
Right ascension | 06h 51m 33.399s[2] |
Declination | −06° 57′ 59.45″[2] |
Apparent magnitude (V) | 6.58[3] |
Characteristics | |
Spectral type | B6-7III-V[e][4] |
B−V color index | 0.030±0.008[3] |
Variable type | γ Cas[5] or FS CMa[6] |
Astrometry | |
Radial velocity (Rv) | 40.8±0.2[6] km/s |
Proper motion (μ) | RA: −3.678 mas/yr Dec.: 4.178 mas/yr |
Parallax (π) | 2.8487 ± 0.0459 mas[2] |
Distance | 1,140 ± 20 ly (351 ± 6 pc) |
Absolute magnitude (MV) | 0.22[3] |
Details | |
Mass | 6[7] M☉ |
Radius | 7.0±2.1[7] R☉ |
Luminosity | (1.2±0.4)×103[7] L☉ |
Surface gravity (log g) | 4.63±0.16[8] cgs |
Temperature | 6,391±241[8] 13,000[7] K |
Metallicity [Fe/H] | 0.18±0.04[3] dex |
Rotational velocity (v sin i) | 1.81389[8] km/s |
Other designations | |
Database references | |
SIMBAD | data |
HD 50138 is a peculiar star in the equatorial constellation of Monoceros, the unicorn. It has the variable star designation V743 Monocerotis. The typical apparent visual magnitude of this star is 6.58,[3] placing it near the lower limit for visibility to the naked eye.[3] Based on parallax measurements,[2] this star is located at a distance of approximately 1,140 light years. It is drifting further away with a heliocentric radial velocity of 41 km/s.[6] This is an isolated star, being located far from any star forming region and having a low proper motion.[6]
MAST
was invoked but never defined (see the help page).GaiaEDR3
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was invoked but never defined (see the help page).Sandell_et_al_2018
was invoked but never defined (see the help page).Koutoulaki_et_al_2018
was invoked but never defined (see the help page).Jönsson_et_al_2020
was invoked but never defined (see the help page).SIMBAD
was invoked but never defined (see the help page).