HD 29573

HD 29573 is a binary star system in the constellation Eridanus. It has a combined apparent visual magnitude of 4.99, making it visible to the naked eye. Based upon an annual parallax shift of 14.23 mas, it is located 229 light years from the Sun. The system is moving further away from Earth with a heliocentric radial velocity of +3 km/s.

HD 24160
Observation data
Epoch J2000      Equinox J2000
Constellation Eridanus
Right ascension 04h 38m 53.55015s
Declination −12° 07 23.0681
Apparent magnitude (V) 4.99 (5.19 + 7.22)
Characteristics
Spectral type A0 V (A1 + F2)
B−V color index 0.074±0.003
Astrometry
Radial velocity (Rv)+2.9±0.8 km/s
Proper motion (μ) RA: −60.614 mas/yr
Dec.: −16.417 mas/yr
Parallax (π)14.2348 ± 0.3656 mas
Distance229 ± 6 ly
(70 ± 2 pc)
Absolute magnitude (MV)0.73
Orbit
Period (P)40.9±1.386 yr
Semi-major axis (a)0.2844±0.0055
Eccentricity (e)0.759±0.180
Inclination (i)75.5±2.2°
Longitude of the node (Ω)152.0±1.8°
Periastron epoch (T)2003.805
Argument of periastron (ω)
(secondary)
284.1±11.0°
Details
HD 29573 A
Mass2.28 M
Luminosity51.8+4.6
−4.3
 L
Temperature8,892+103
−102
 K
Rotational velocity (v sin i)27 km/s
HD 29573 B
Mass1.56 M
Other designations
BD−12° 955, GJ 9161, HD 29573, HIP 21644, HR 1483, SAO 149789, WDS J04389-1207AB
Database references
SIMBADdata

The binary nature of this system was discovered through observations made with the Hipparcos spacecraft. The pair orbit each other with a period of 41 years and an eccentricity of 0.8. The magnitude 5.19 primary component has a class of A1, 2.28 times the mass of the Sun, and is a suspected chemically peculiar star. The secondary has magnitude 7.22, 1.56 times the Sun's mass, and a class of F2. The system has a possible infrared excess due to circumstellar dust.

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