HD 27245

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HD 27245
Location of HD 27245 on the map (circled)
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]
Distance
607 ± 10 ly
(186 ± 3 pc)
Absolute magnitude (MV)−0.27[7]
Details
dex
HR 1335, SAO 13113[14]
Database references
SIMBADdata

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

External links