Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Caelum |
Right ascension | 04h 27m 05.96464s[1] |
Declination | −46° 56′ 50.9697″[1] |
Apparent magnitude (V) | 6.10[2] |
Characteristics | |
Spectral type | F5.5 V[3] |
U−B color index | −0.07[4] |
B−V color index | +0.48[4] |
Astrometry | |
Radial velocity (Rv) | 15±2.4[5] km/s |
Proper motion (μ) | RA: +63.853 mas/yr[1] Dec.: −270.620 mas/yr[1] |
Parallax (π) | 30.6049 ± 0.0259 mas[1] |
Distance | 106.57 ± 0.09 ly (32.67 ± 0.03 pc) |
Absolute magnitude (MV) | +3.5[2] |
Details | |
Mass | 1.24[6] M☉ |
Radius | 1.42±0.06[7] R☉ |
Luminosity | 3.26±0.01[1] L☉ |
Surface gravity (log g) | 4.30 ± 0.14[8] cgs |
Temperature | 6,468±80[9] K |
Metallicity [Fe/H] | −0.25±0.10[10] dex |
Rotational velocity (v sin i) | 8[11] km/s |
Age | 1.61[6] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
HD 28454, also known as HR 1418, is a solitary, yellowish-white hued star located in the southern constellation Caelum, the chisel. It has an apparent magnitude of 6.1,[2] making it faintly visible to the naked eye under ideal conditions. This star is located relatively close at a distance of about 107 light years based on parallax measurements of Gaia DR3 but is receding with a heliocentric radial velocity of 15 km/s.[5]
HD 28454 is an ordinary F-type main sequence star with a stellar classification of F5.5 V.[3] It has 1.21 times the mass of the Sun[6] and 1.42 times its radius.[7] It radiates 3.26 times the luminosity of the Sun[1] from its photosphere at an effective temperature of 6,468 K.[9] HD 28454 is estimated to be 1.61 billion years,[6] and spins modestly with a projected rotational velocity of 8 km/s.[11] The star is metal deficient, having an iron abundance 56% that of the Sun's.[10]
GaiaDR3
was invoked but never defined (see the help page).Anderson2012
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