Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Horologium |
Right ascension | 02h 40m 39.61286s[1] |
Declination | −54° 32′ 59.6836″[1] |
Apparent magnitude (V) | 5.20[2] |
Characteristics | |
Spectral type | F6 V[3] (F2 V + F5 V)[4] |
B−V color index | +0.42[2] |
Astrometry | |
Radial velocity (Rv) | 5.8[3] km/s |
Proper motion (μ) | RA: +32.86[1] mas/yr Dec.: +4.96[1] mas/yr |
Parallax (π) | 20.37 ± 0.21 mas[1] |
Distance | 160 ± 2 ly (49.1 ± 0.5 pc) |
Absolute magnitude (MV) | +1.76[5] |
Orbit[4] | |
Period (P) | 12.9274 d |
Eccentricity (e) | 0.25 |
Periastron epoch (T) | 7.361±0.046 |
Argument of periastron (ω) (secondary) | 78.6±0.13° |
Semi-amplitude (K1) (primary) | 58.1±1.37 km/s |
Semi-amplitude (K2) (secondary) | 66.1±1.56 km/s |
Details | |
ζ Hor A | |
Mass | 1.43[6] M☉ |
Luminosity | 16.7[5] L☉ |
Surface gravity (log g) | 3.74[7] cgs |
Temperature | 6,702[7] K |
Metallicity [Fe/H] | −0.07[7] dex |
Rotational velocity (v sin i) | 8.0±1.2[3] km/s |
Age | 1.50[7] Gyr |
ζ Hor B | |
Mass | 1.26[6] M☉ |
Other designations | |
Database references | |
SIMBAD | data |
Zeta Horologii, Latinized from ζ Horologii, is a yellow-white-hued binary star system in the southern constellation of Horologium. It is visible to the naked eye with a combined apparent visual magnitude of 5.20.[2] Based upon an annual parallax shift of 20.37 mas as seen from Earth,[1] it is located around 160 light-years from the Sun.
This system was determined to be a double-lined spectroscopic binary by J. H. Moore in 1911−12. The first orbital elements were published by J. Sahade and C. A. Hernández in 1964, who found it consisted of two F-type main-sequence stars of probable stellar classifications F2 V and F5 V. The pair orbit each other with a period of 12.9274 days and an eccentricity of 0.25.[4] The system displays an infrared excess at a wavelength of 24 μm but not at 70 μm, yielding a derived temperature of 260 K. This suggests a circumbinary debris disk orbiting at a distance of less than 4.8 AU from the star system.[9]
vanLeeuwen2007
was invoked but never defined (see the help page).Corben1968
was invoked but never defined (see the help page).Torres2006
was invoked but never defined (see the help page).Sahade1964
was invoked but never defined (see the help page).Anderson2012
was invoked but never defined (see the help page).Tokovinin2006
was invoked but never defined (see the help page).Casagrande2011
was invoked but never defined (see the help page).SIMBAD
was invoked but never defined (see the help page).Trilling2007
was invoked but never defined (see the help page).