HD 43587
HD 43587 is a stellar system approximately 63 light-years away in the constellation of Orion, visible to the naked eye. The system comprises four individual stars, with two widely separated binaries forming a quadruple system.
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Orion |
HD 43587 Aab | |
Right ascension | 06h 17m 16.139s ± 3.26 |
Declination | +05° 06′ 00.40″ ± 2.46 |
Apparent magnitude (V) | 5.70 |
HD 43587 BC | |
Right ascension | 06h 17m 10.65s |
Declination | +05° 07′ 02.4″ |
Apparent magnitude (V) | 13.27 (BC total) |
Characteristics | |
Spectral type | G0V / M0V / M3.5V / M5V |
B−V color index | 0.610(system total) |
Astrometry | |
HD 43587 Aa | |
Radial velocity (Rv) | 8.96 ± 0.10 km/s |
Proper motion (μ) | RA: -187.72 ± 0.37 mas/yr Dec.: 170.69 ± 0.28 mas/yr |
Parallax (π) | 51.95 ± 0.40 mas |
Distance | 62.8 ± 0.5 ly (19.2 ± 0.1 pc) |
HD 43587 BC | |
Proper motion (μ) | RA: -198 mas/yr Dec.: 164 mas/yr |
Parallax (π) | 55.2 ± 1.0 mas |
Distance | 59 ± 1 ly (18.1 ± 0.3 pc) |
Absolute magnitude (MV) | 12.07 ± 0.07 / 14.90 ± 0.21 |
Orbit | |
Primary | HD 43587 Aa |
Companion | HD 43587 Ab |
Period (P) | 32.07 years |
Semi-major axis (a) | 0.598″ |
Eccentricity (e) | 0.796 |
Inclination (i) | 35.6° |
Longitude of the node (Ω) | 163.1° |
Periastron epoch (T) | 1998.05 |
Argument of periastron (ω) (secondary) | 75.0° |
Semi-amplitude (K1) (primary) | 4.323 ± 0.009 km/s |
Position (relative to HD 43587 B) | |
Component | HD 43587 C |
Epoch of observation | 2453376.0 |
Angular distance | 366 ± 3 mas |
Position angle | 158 ± 1° |
Details | |
Mass | 1.049 ± 0.016 / 0.67 ± 0.04 / 0.25 ± 0.06 / 0.12 ± 0.02 M☉ |
Radius | 1.15 ± 0.01 R☉ |
Surface gravity (log g) | 4.30 ± 0.01 cgs |
Temperature | 5947 ± 17 K |
Metallicity [Fe/H] | -0.02 ± 0.02 dex |
Age | 4.97 ± 0.52 Gyr |
Other designations | |
HIP 29860, Gliese 231.1, HR 2251 | |
HD 43587 Aab: WDS J06173+0506Aa,Ab, LEP 24A | |
HD 43587 BC: NLTT 16333, WDS J06173+0506E, LEP 24AE | |
Database references | |
SIMBAD | data |
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