Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Camelopardalis |
Right ascension | 03h 53m 43.28625s[1] |
Declination | +57° 58′ 30.5263″[1] |
Apparent magnitude (V) | 5.79±0.01[2] |
Characteristics | |
Spectral type | kA3hF0mF0[3] or A7 V[4] |
U−B color index | +0.11[5] |
B−V color index | +0.18[5] |
Astrometry | |
Radial velocity (Rv) | −0.2±0.6[6] km/s |
Proper motion (μ) | RA: +86.826 mas/yr[1] Dec.: −91.295 mas/yr[1] |
Parallax (π) | 18.5633 ± 0.0352 mas[1] |
Distance | 175.7 ± 0.3 ly (53.9 ± 0.1 pc) |
Absolute magnitude (MV) | +2.28[7] |
Position (relative to HD 24141A) | |
Component | HD 24141B |
Epoch of observation | J2000.0 |
Angular distance | 1.02″ [8] |
Position angle | 69° [9] |
Projected separation | 52.3 AU [8] |
Details | |
A | |
Mass | 1.92[10] M☉ |
Radius | 1.72±0.09[11] R☉ |
Luminosity | 10.66±0.04[1] L☉ |
Surface gravity (log g) | 4.28+0.08 −0.07[12] cgs |
Temperature | 8,518±290[10] K |
Metallicity [Fe/H] | −0.02[13] dex |
Rotational velocity (v sin i) | 53±10[14] km/s |
Age | 15[10] Myr |
B | |
Mass | 0.77[8] M☉ |
Other designations | |
Database references | |
SIMBAD | data |
HD 24141, also known as HR 1192, is a star located in the northern constellation Camelopardalis, the giraffe. It is faintly visible to the naked eye as a white-hued point of light with an apparent magnitude of 5.79.[2] The object is located relatively close at a distance of 176 light-years based on Gaia DR3 parallax measurements[1] and it is slowly drifting closer with a heliocentric radial velocity of −0.2 km/s.[6] At its current distance, HD 24141's brightness is diminished by 0.17 magnitudes due to interstellar extinction[16] and it has an absolute magnitude of +2.28.[7]
It is not entirely certain whether HD 24141 is an Am star or not.[17] One stellar classification is kA3hF0mF0,[3] which indicates that it is an Am star with the calcium K-lines of an A3 star and the hydrogen and metallic lines of a F0 star. However, Abt & Levy (1985) gave a class of A7 V,[4] indicating that it is instead an ordinary A-type main-sequence star. HD 24141 has 1.92 times the mass of the Sun and it is estimated to be only 15 million years old.[10] It radiates 10.66 times the luminosity of the Sun[1] from its photosphere at an effective temperature of 8,518 K.[10] These parameters correspond to a radius that is 72% larger than the Sun's.[11] HD 24141 has a near-solar metallicity at [Fe/H] = −0.02[13] and it spins modestly with a projected rotational velocity of 53 km/s.[14]
Most sources generally agree that HD 24141 is a solitary star.[18][4][19] A 2014 multiplicity survey found a 7th magnitude companion with a mass of 0.77 M☉[8] located 1.02" away from the star[8] along a position angle of 69°. Another 15th magnitude companion designated as C is located 1216″ away along a position angle of 187°.[20] The object appears to share the same proper motion as HD 24141,[9] but the Gaia DR3 parallax is different and it is considered very unlikely that the two are physically associated.[21]
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