Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Camelopardalis [1] |
A | |
Right ascension | 06h 46m 14.1500s [2] |
Declination | +79° 33′ 53.319″ [2] |
Apparent magnitude (V) | +5.44 [1] |
B | |
Right ascension | 06h 46m 27.5604s [3] |
Declination | +79° 35′ 04.513″ [3] |
Characteristics | |
Spectral type | F7 V [4] + L9 [5] |
U−B color index | −0.02 [6] |
B−V color index | +0.53 [6] |
Astrometry | |
A | |
Radial velocity (Rv) | 15.30±0.13 [2] km/s |
Proper motion (μ) | RA: −99.163 mas/yr [2] Dec.: −604.042 mas/yr [2] |
Parallax (π) | 54.9380±0.0595 mas [2] |
Distance | 59.37 ± 0.06 ly (18.20 ± 0.02 pc) |
Absolute magnitude (MV) | +4.18 [1] |
Details | |
A | |
Mass | 1.13+0.03 −0.02 [7] M☉ |
Radius | 1.16±0.04 [8] R☉ |
Luminosity | 1.82 [9] L☉ |
Surface gravity (log g) | 4.40±0.02 [7] cgs |
Temperature | 6,273±91 [7] K |
Metallicity [Fe/H] | −0.12±0.06 [7] dex |
Rotation | 10.3 d [8] |
Rotational velocity (v sin i) | 2.50±1.74 [8] km/s |
Age | 1.27+1.65 −0.22 [7] Gyr |
B | |
Mass | 0.064+0.008 −0.019 M☉ |
Temperature | 1360+50 −80 K |
Other designations | |
23 H. Camelopardalis, AG+79°200, BD+79°212, GC 8711, GJ 240.1, HD 46588, HIP 32439, HR 2401, SAO 5946, WDS J06462+7934 [10] | |
Database references | |
SIMBAD | A |
B |
HD 46588 (HR 2401; Gliese 240.1) is a star with a brown dwarf companion in the northern circumpolar constellation Camelopardalis. It has an apparent magnitude of 5.44, [1] allowing it to be faintly seen with the naked eye. The object is relatively close at a distance of only 59 light-years [2] but is receding with a heliocentric radial velocity of 15 km/s . [11]
HD 46588 is an ordinary F-type main-sequence star with a spectral classification of F7 V. [4] It has 113% the mass of the Sun [7] and 119% its radius. [9] It shines at 182% the luminosity of the Sun [9] from its photosphere at an effective temperature of 6,273 K, [7] giving it a yellow white glow. Isochronic measurements place HD 46588's age at 1.27 billion years, [7] but it is poorly constrained. The star's metallicity is 76% that of the Sun [7] and spins modestly with a projected rotational velocity of 6.63 km/s . [12]
Due to the star's close proximity to Earth and similarity to the Sun, it has been well studied by astronomers. [5] A brown dwarf companion, HD 46588 B, was discovered in a WISE survey in 2011, at a distance of 1420 AU from the primary. It has a mass of 67+8
−20 Jupiter masses and a temperature of 1360+50
−80 K. [5] An infrared excess has been discovered around HD 46588, indicating a cold debris disk with a temperature of 60 K. [13] In addition, a 2022 study detected a candidate planet around the star using the radial velocity method. [8]
Companion (in order from star) | Mass | Semimajor axis (AU) | Orbital period (days) | Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b(unconfirmed) | ≥0.25+0.06 −0.04 MJ | — | 223±3 | 0.42+0.19 −0.14 | — | — |
dust disk | 26.34 AU | — | — |