Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Orion |
Right ascension | 05h 40m 50.71498s[1] |
Declination | −01° 07′ 43.6366″[1] |
Apparent magnitude (V) | 4.95[2] |
Characteristics | |
primary | |
Spectral type | B2IV-V[3] or B3V[4] |
U−B color index | −0.83[5] |
B−V color index | −0.21[5] |
secondary | |
Spectral type | B1[6] |
Astrometry | |
Radial velocity (Rv) | +26.10[7] km/s |
Proper motion (μ) | RA: −1.50[1] mas/yr Dec.: −0.84[1] mas/yr |
Parallax (π) | 3.63 ± 0.37 mas[1] |
Distance | approx. 900 ly (approx. 280 pc) |
Absolute magnitude (MV) | −2.74[2] |
Orbit[8] | |
Period (P) | 27.154925 d |
Eccentricity (e) | 0.739±0.007 |
Periastron epoch (T) | 2447886.076±0.065 HJD |
Argument of periastron (ω) (secondary) | 81.4±2.4° |
Semi-amplitude (K1) (primary) | 84.7±1.1 km/s |
Details | |
A | |
Mass | 8.6±0.2[9] M☉ |
Radius | 5.3[10] R☉ |
Luminosity | 4,830[11] L☉ |
Surface gravity (log g) | 3.84[10] cgs |
Temperature | 21,150[11] K |
Metallicity [Fe/H] | +0.01[12] dex |
Rotational velocity (v sin i) | 75[13] km/s |
Age | 18.0±3.2[9] Myr |
B | |
Mass | 8.3[6] M☉ |
Other designations | |
Database references | |
SIMBAD | data |
HD 37756 is a binary star system in the equatorial constellation of Orion, positioned less than a degree to the north of the bright star Alnitak.[15] It has a blue-white hue and is faintly visible to the naked eye with an apparent visual magnitude of 4.95.[2] The system is located at a distance of approximately 900 light years from the Sun based on parallax,[1] and is drifting further away with a radial velocity of +26 km/s.[7] It is a member of the OB1b subgroup of the Orion OB1 association.[16]
The binary nature of this system was identified by E. B. Frost in 1904.[17] It is a double-lined spectroscopic binary with an orbital period of 27.15 days and a high eccentricity of 0.74.[8] The spectrum matches a massive B-type main-sequence star with a stellar classification of B3V.[4] The secondary is luminous enough to interfere with measurements of the primary spectrum.[17] It is a suspected Cepheid variable with a period of 0.37968 days and an amplitude of 0.03 magnitude in the B band of the UBV photometric system.[18] The system is a candidate eclipsing binary with a minimum dip of 0.04 in visual magnitude during each orbit.[19]
vanLeeuwen2007
was invoked but never defined (see the help page).XHIP
was invoked but never defined (see the help page).Hoffleit1991
was invoked but never defined (see the help page).Houk1999
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was invoked but never defined (see the help page).Kraicheva1980
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was invoked but never defined (see the help page).Hilditch1991
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was invoked but never defined (see the help page).Hohle2010
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was invoked but never defined (see the help page).Abt2002
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was invoked but never defined (see the help page).Sinnott1997
was invoked but never defined (see the help page).Voss2010
was invoked but never defined (see the help page).Kameswara1990
was invoked but never defined (see the help page).Hill1967
was invoked but never defined (see the help page).Hoffleit1996
was invoked but never defined (see the help page).