Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Camelopardalis |
Right ascension | 07h 30m 52.66467s[1] |
Declination | +68° 27′ 56.3270″[1] |
Apparent magnitude (V) | 5.64±0.01[2] |
Characteristics | |
Evolutionary stage | red giant branch[1] |
Spectral type | K2 III[3] |
B−V color index | +1.11[4] |
Astrometry | |
Radial velocity (Rv) | 58.6±0.2[5] km/s |
Proper motion (μ) | RA: −2.031 mas/yr[1] Dec.: −42.687 mas/yr[1] |
Parallax (π) | 6.9858 ± 0.2644 mas[1] |
Distance | 470 ± 20 ly (143 ± 5 pc) |
Absolute magnitude (MV) | −0.05[6] |
Details | |
Mass | 1.74±0.52[7] M☉ |
Radius | 24.7[8] R☉ |
Luminosity | 199+24 −22[9] L☉ |
Surface gravity (log g) | 2.4±0.1[10] cgs |
Temperature | 4,479±62[8] K |
Metallicity [Fe/H] | −0.42±0.04[10] dex |
Age | 3.55+0.52 −0.46[7] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
HD 58425, also known as HR 2830, is an astrometric binary[13] (100% chance[14]) located in the northern circumpolar constellation Camelopardalis. It is faintly visible to the naked eye as an orang point of light at an apparent magnitude of 5.64.[2] Based on parallax measurements from Gaia DR3, the system is estimated to be 470 light years away from Earth.[1] It appears to be rapidly receding from the Sun, having a heliocentric radial velocity of 58.6 km/s.[5] HD 58425 is listed as 54 Ursae Majoris in Johann Hevelius' catalogue,[11] but this was dropped after the official IAU's official constellation borders were drawn.
The visible component is an evolved, RGB star with a stellar classification of K2 III.[3] It has 1.74 times the mass of the Sun and is said to be 3.55 billion years old.[7] At this age, the object has expanded to 24.7 times the radius of the Sun[8] and now radiates nearly 200 times the luminosity of the Sun[9] from its enlarged photosphere at an effective temperature of 4,479 K.[8] HD 58425 A has an iron abundance only 38% that of the Sun's,[10] making it metal deficient.
GaiaDR3
was invoked but never defined (see the help page).Tycho2000
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