HD 41004

HD 41004
Observation data
Epoch J2000      Equinox J2000
Constellation Pictor
Right ascension 05h 59m 49.65018s
Declination −48° 14 22.8883
Apparent magnitude (V) 8.65 (8.82 + 12.51)
Characteristics
Spectral type K1V + M2V
B−V color index 0.887±0.013
Astrometry
Radial velocity (Rv)+42.36±0.14 km/s
Proper motion (μ) RA: −43.418(115) mas/yr
Dec.: +65.333(123) mas/yr
Parallax (π)25.6106±0.1043 mas
Distance127.4 ± 0.5 ly
(39.0 ± 0.2 pc)
Absolute magnitude (MV)5.60
Details
A
Mass0.89±0.07 M
Radius1.04+0.02
−0.03
 R
Luminosity0.629±0.008 L
Surface gravity (log g)4.34±0.11 cgs
Temperature5,255±52 K
Metallicity [Fe/H]0.15±0.03 dex
Rotational velocity (v sin i)1.0±1.2 km/s
B
Mass0.4 M
Other designations
CD−48°2083, HD 41004, HIP 28393, SAO 217660, PPM 310291, WDS J05598-4814
Database references
SIMBADdata

HD 41004 is a visual binary star system in the southern constellation of Pictor. It is too faint to be visible to the naked eye, having a combined apparent visual magnitude of 8.65. The two components have a magnitude difference of 3.7, and share a common proper motion with an angular separation of 0.30, as of 2018. The distance to this system is approximately 127 light-years based on parallax. It is drifting further away from the Sun with a radial velocity of +42.5 km/s, having come to within 44.5 ly some 831,000 years ago.

The primary, component A, is a K-type main-sequence star with a stellar classification of K1V and a visual magnitude of 8.82. Torres et al. (2006) classed it as a K1IV star, suggesting it is a subgiant star that is evolving off the main sequence. It has 89% of the mass of the Sun and 104% of the Sun's radius. The star is radiating 63% of the Sun's luminosity from its photosphere at an effective temperature of 5,255 K. Its smaller companion, designated component B, is a red dwarf with spectral type M2V and apparent magnitude 12.33. It has a projected separation of 23 AU from the primary.