Triple stellar system in the constellation Orion
HD 39118
Basic layout of the HR 2024 system. |
Observation data Epoch J2000 Equinox J2000
|
Constellation
|
Orion[a]
|
Right ascension
|
05h 50m 30.03s[1]
|
Declination
|
02° 01′ 28.93″[1]
|
Apparent magnitude (V)
|
5.976[1]
|
Characteristics
|
Cool primary
|
Evolutionary stage
|
Red giant branch[2]
|
Spectral type
|
K0II[3]
|
Apparent magnitude (B)
|
6.83±0.015[1]
|
Apparent magnitude (G)
|
5.64[1]
|
Apparent magnitude (J)
|
4.193±0.238[1]
|
Apparent magnitude (H)
|
3.502±0.194[1]
|
Apparent magnitude (K)
|
3.337±0.19[1]
|
B−V color index
|
1.12[3]
|
Hot secondary
|
Evolutionary stage
|
B-type main-sequence star + A-type main-sequence star
|
Spectral type
|
B7V/B8V + A0V[3]
|
B−V color index
|
-0.09[3]
|
Astrometry |
---|
|
---|
Radial velocity (Rv) | 4.24[3] km/s |
Proper motion (μ) | RA: 1.097 mas/yr[1] Dec.: -5.161 mas/yr[1] |
Parallax (π) | 1.47 ± 0.23 mas[4] |
Distance | 2300+350 −270 ly (707.6+107 −83.3 pc)[4] |
Absolute magnitude (MV) | –2.53 (–2.3 (primary) + –0.75 (secondary))[3] |
|
Orbit |
---|
Primary | Cool primary |
Companion | Hot secondary |
Period (P) | 2570±13 d 7.04±0.04 year[5] |
Semi-major axis (a) | 4.7×108 km 3.14 AU[5] |
Eccentricity (e) | 0.3±0.007[5] |
Details |
---|
K-type giant |
---|
Mass | 3.3+0.3 −0.27[2] M☉ |
Radius | 23.5+3.7 −1.9[2] R☉ |
Luminosity | 535[6] L☉ |
Surface gravity (log g) | 1.52[7] cgs |
Temperature | 4,550[7] K |
Metallicity [Fe/H] | -0.34[7] dex |
Rotational velocity (v sin i) | 4.19[8] km/s |
Age | 257[2] Myr |
B-type star |
---|
Temperature | 11,300[9] K |
Other designations |
---|
BD+01 1148, Gaia DR2 3316078695157768448, Gaia DR3 3316078695157768448, HD 39118/39119, HIP 27588, HR 2024, SAO 113198, PPM 149543, TIC 158867386, TYC 120-877-1, GSC 00120-00877, IRAS 05478+0200, 2MASS J05503003+0201290 |
Database references |
---|
SIMBAD | data |
HD 39118 (HD 39119, HR 2024) is a spectroscopic binary star in the constellation Orion, close to the celestial equator. It is made up from three stars: a cool primary (a K-type giant star) and a hot secondary, which is a binary star formed from a B-type main-sequence star and an A-type main-sequence star. A 2021 estimate derive a distance of 708 parsecs (2,310 ly) to HD 39118, and it is moving away from Earth at a speed of 4.24 km/s. The apparent magnitude is 5.976, making it visible to the naked eye only from dark skies.
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