HD 30442

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HD 30442
Observation data
Epoch J2000      Equinox J2000
Constellation Camelopardalis[1]
Right ascension 04h 52m 05.2195s[2]
Declination +63° 30 19.5173[2]
Apparent magnitude (V) 5.47±0.01[3]
Characteristics
Evolutionary stage AGB[4]
Spectral type M3 IIIab[5]
U−B color index +1.76[6]
B−V color index +1.55[6]
Astrometry
Radial velocity (Rv)−37±0.3[7] km/s
Proper motion (μ) RA: +38.424 mas/yr[2]
Dec.: −94.026 mas/yr[2]
Parallax (π)8.098±0.1027 mas[2]
Distance403 ± 5 ly
(123 ± 2 pc)
Absolute magnitude (MV)−0.44[1]
Details
Mass1.09[8] M
Radius70.85[9] R
Luminosity1,096+106
96
[10] L
Surface gravity (log g)0.92[8] cgs
Temperature3,500±150[10] K
Metallicity [Fe/H]0.00[10] dex
Other designations
BD+63°543, FK5 2362, GC 5881, HD 30442, HIP 22626, HR 1527, SAO 13291, WDS J04521+6330A[11]
Database references
SIMBADdata

HD 30442 (HR 1527) is a solitary[12] star in the northern circumpolar constellation Camelopardalis. It is faintly visible to the naked eye with an apparent magnitude of 5.47[3] and is estimated to be 403 light years away from the Solar System.[2] The object has a heliocentric radial velocity of −37 km/s, indicating that it is drifting closer.[7]

HD 30442 has a stellar classification of M3 IIIab,[5] indicating that it is a red giant. It is an asymptotic giant branch[4] star currently generating energy using hydrogen and helium shells around an inert carbon core. It has 109% the mass of the Sun[8] and has an enlarged radius of 70.8 R[9] due to its evolved state. It radiates at almost 1,100 times the luminosity of the Sun from its photosphere at an effective temperature of 3,500 K,[10] giving a red hue. HD 30442 is estimated to have a solar metallicity,[8] with an abundance of iron equivalent to that of the Sun.

HD 30442 has a companion 120 away along a position angle of 350°.[13] It shares a common proper motion with HD 30442, suggesting physical relation, but its parallax indicates otherwise.[14]

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