HD 44120

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HD 44120
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Pictor
Right ascension 06h 16m 18.786s[1]
Declination −59° 12′ 48.61″[1]
Apparent magnitude (V) 6.44[2] + 14.03[3]
Characteristics
Spectral type F9.5V[4] + DB3.2[3]
B−V color index 0.593±0.015[2]
Distance
117.51 ± 0.07 ly
(36.03 ± 0.02 pc)
Absolute magnitude (MV)3.57[2]
Details
A
Gyr
C
Mass0.67±0.10[10] M
Radius0.0130±0.0003[10] R
Surface gravity (log g)8.04±0.06[10] cgs
Temperature15,746±238[10] K
L 182-61, WD 0615-591[3]
Database references
SIMBADA
C

HD 44120 is a wide

light years from the Sun based on parallax, but it is drifting closer with a radial velocity of −2 km/s.[5] It has an absolute magnitude of 3.57.[2]

The primary member, designated component A of this system, is an

The faint secondary companion, component C, is a magnitude 14.03

semimajor axis of 1,702.6 AU and an orbital period of 51,100 years.[3]

A magnitude 7.61

along a position angle of 234° from component A, as of 2015. It was discovered as a double star by the Scottish astronomer James Dunlop and announced in 1829.[15] The parallax for this star indicates a distance of approximately 215 ly (66 pc) from the Sun.[16]

References