HD 27245, also known as HR 1335 or rarely 25 H. Camelopardalis is a solitary red-hued star[15] located in the northern circumpolar constellation Camelopardalis. It has an apparent magnitude of 5.4,[2] making it faintly visible to the naked eye. Gaia DR3 Parallax measurements place it approximately 607 light years[1] away from it the Solar System and is drifting further away with a heliocentric radial velocity of 25.2 km/s.[6] At its current distance, HD 27245's brightness is diminished by 0.36 magnitudes due to extinction from interstellar dust.[16] It has an absolute magnitude of −0.27.[7]
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Camelopardalis |
Right ascension | 04h 21m 47.64917s[1] |
Declination | +60° 44′ 08.2461″[1] |
Apparent magnitude (V) | 5.40±0.01[2] |
Characteristics | |
Spectral type | M0 III[3] |
B−V color index | +1.50[4] |
Variable type | suspected[5] |
Astrometry | |
Radial velocity (Rv) | +25.2±0.3[6] km/s |
Proper motion (μ) | RA: +55.890 mas/yr[1] Dec.: −114.046 mas/yr[1] |
Parallax (π) | 5.3716 ± 0.0848 mas[1] |
Distance | 607 ± 10 ly (186 ± 3 pc) |
Absolute magnitude (MV) | −0.27[7] |
Details | |
Mass | 1.18[8] M☉ |
Radius | 52.8±2.7[9] R☉ |
Luminosity | 570±16[10] L☉ |
Surface gravity (log g) | 1.29[11] cgs |
Temperature | 4,033±122[12] K |
Metallicity [Fe/H] | +0.11[8] dex |
Other designations | |
Database references | |
SIMBAD | data |
HD 27245 is an aging red giant with a stellar classification of M0 III.[3] It has 118% the mass of the Sun[8] but has expanded to a radius of 52.8 R☉.[11] It radiates 570 times the luminosity of the Sun[10] from its enlarged photosphere at an effective temperature of 4,033 K.[12] HD 27245's iron abundance is 129% that of the Sun's,[8] making it metal enriched.
HD 27245 is a suspected variable star with an amplitude of 0.05 magnitudes.[5] Its variability was first observed in 1930 by Joel Stebbins.[17] However, Eggen (1967) instead lists it as an ordinary M-type giant and used the object for comparison.[18] In 1978-9, HD 28245 was again listed as a variable star but did not provide further insight.[19] As of 2017, the star has not been confirmed to be variable.[5]