Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Camelopardalis |
Right ascension | 05h 20m 22.61066s[1] |
Declination | +62° 39′ 13.3608″[1] |
Apparent magnitude (V) | 5.60±0.01[2] |
Characteristics | |
Spectral type | K4 I[3] |
U−B color index | +2.00[4] |
B−V color index | +1.75[4] |
Astrometry | |
Radial velocity (Rv) | −7.7±0.15[5] km/s |
Proper motion (μ) | RA: −3.105 mas/yr[1] Dec.: −2.373 mas/yr[1] |
Parallax (π) | 1.9726 ± 0.0788 mas[1] |
Distance | 1,650 ± 70 ly (510 ± 20 pc) |
Absolute bolometric magnitude (Mbol) | −4.40±0.24[6] |
Details | |
Mass | 6.9±0.9[7] M☉ |
Radius | 145[6] R☉ |
Luminosity | 6,101[8] L☉ |
Surface gravity (log g) | 1.14[9] cgs |
Temperature | 3,927±170[6] K |
Metallicity [Fe/H] | −0.01±0.05[9] dex |
Age | 46±6[7] Myr |
Other designations | |
Database references | |
SIMBAD | data |
HD 34255, also known HR 1720, is a star located in the northern circumpolar constellation Camelopardalis, the giraffe. It has an apparent magnitude of 5.60,[2] allowing it to be faintly visible to the naked eye. The object is located relatively far at a distance of about 1.65 kly[1] but is approaching the Solar System with a heliocentric radial velocity of −7.7 km/s.[5]
This is a solitary,[11] evolved red supergiant with a stellar classification of K4 I.[3] It has 6.9 times the mass of the Sun and is said to be 46 million years old.[7] Despite the young age, it has already ceased hydrogen fusion at its core and now has an enlarged radius of 145 R☉.[6] HD 34255 radiates a bolometric luminosity over 6,000 times that of the Sun[8] from its photosphere at an effective temperature of 3,927 K,[6] giving it an orange glow. The star's metallicity – what astronomers dub as elements heavier than helium – is around solar level.[9]
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