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Tau9 Eridani

τ9 Eridani
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Eridanus
Right ascension 03h 59m 55.48381s
Declination −24° 00′ 58.3798″
Apparent magnitude (V) 4.63
Characteristics
Spectral type B9.5V Si
U−B color index −0.40
B−V color index −0.13
Variable type α2 CVn
Astrometry
Radial velocity (Rv) 25.5±0.5 km/s
Proper motion (μ) RA: +12.12 mas/yr
Dec.: +16.48 mas/yr
Parallax (π) 9.96 ± 0.22mas
Distance 327 ± 7 ly
(100 ± 2 pc)
Absolute magnitude (MV) −0.44
Orbit
Period (P) 5.9537 days
Eccentricity (e) 0.1
Periastron epoch (T) 2417600.95 JD
Argument of periastron (ω)
(secondary)
151°
Semi-amplitude (K1)
(primary)
37.6 km/s
Details
τ9 Eri A
Mass 3.26 M
Radius 3.26 R
Luminosity 166 L
Surface gravity (log g) 4.11±0.11 cgs
Temperature 10,866 K
Rotational velocity (v sin i) 30 km/s
Other designations
τ9 Eridani, τ9 Eri, 36 Eridani, CD−24° 2022, FK5 2287, HD 25267, HIP 18673, HR 1240, SAO 169017.
Database references
SIMBAD data

Tau9 Eridani (τ9 Eri) is a binary star in the constellation Eridanus. It is visible to the naked eye with an apparent visual magnitude of 4.63. The distance to this system can be estimated using the parallax method, which yields a value of roughly 327 light years.

This is a single-lined spectroscopic binary system with an orbital period of 5.9537 days and an eccentricity of 0.1. The primary component, τ9 Eri A, is a magnetic chemically peculiar star with a stellar classification of B9.5V Si, indicating that it is a B-type main sequence star that shows abundance anomalies in its silicon absorption lines. It is an Alpha² Canum Venaticorum variable with a rotational periodicity of 5.954 days. The averaged strength of the stellar effective magnetic field is 240.6±91.0 G.

Tau9 Eridani A has an estimated 326% the mass of the Sun and 3.1 times the Sun's radius. It shines with 166 times the solar luminosity from a outer atmosphere at an effective temperature of 10,866 K. The star is spinning with a projected rotational velocity of 30 km/s.


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