HD 27245
Appearance
Observation data 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] |
Absolute magnitude (MV) | −0.27[7] |
Details | |
dex | |
Database references | |
SIMBAD | data |
HD 27245, also known as HR 1335 or rarely 25 H. Camelopardalis is a solitary red-hued
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]
HD 27245 is an aging
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]
References
- ^ .
- ^ ISSN 0004-6361.
- ^ ISSN 0004-6280.
- Bibcode:1970Priv.........0H.
- ^ S2CID 125853869.
- ^ S2CID 17804304.
- ^ S2CID 119257644.
- ^ ISSN 0004-6361.
- ISSN 0004-6361.
- ^ .
- ^ ISSN 0035-8711.
- ^ S2CID 166227927.
- ISSN 0004-6361.
- ^ "HD 27245". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-06-05.
- S2CID 14878976.
- ISSN 0035-8711.
- Bibcode:1930PWasO..15..140S.
- ISSN 0067-0049.
- ISSN 0374-0676.