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HD 63399

Star in the constellation Puppis From Wikipedia, the free encyclopedia

HD 63399 is an orange hued star located in the southern constellation Puppis, the poop deck. It has an apparent magnitude of 6.45,[2] placing it near the limit for naked eye visibility. Based on parallax measurements from Gaia DR3,[1] the object is estimated to be 445 light years distant. It appears to be receding with a spectroscopic radial velocity of 28.5 km/s.[6] At its current distance, HD 63399 is diminished by 0.29 magnitudes due to interstellar dust.[13]

Right ascension07h 47m 14.59403s[1]
Declination−36° 04 24.9619[1]
Quick facts Constellation, Right ascension ...
HD 63399
Observation data
Epoch J2000      Equinox ICRS
Constellation Puppis
Right ascension 07h 47m 14.59403s[1]
Declination −36° 04 24.9619[1]
Apparent magnitude (V) 6.45±0.01[2]
Characteristics
Evolutionary stage red giant branch[3]
Spectral type K1 III[4]
U−B color index +1.13[5]
B−V color index +1.12[5]
Astrometry
Radial velocity (Rv)28.5±0.2[6] km/s
Proper motion (μ) RA: −35.000 mas/yr[1]
Dec.: +26.931 mas/yr[1]
Parallax (π)7.3283±0.0162 mas[1]
Distance445.1 ± 1.0 ly
(136.5 ± 0.3 pc)
Absolute magnitude (MV)+0.78[7]
Details
Mass1.29[8] or 1.7+1.3
0.8
[9] M
Radius10.79[10] R
Luminosity54.8±0.3[6] L
Surface gravity (log g)2.47[8] cgs
Temperature4,761±77[11] K
Metallicity [Fe/H]−0.06[3] dex
Other designations
CD−35°3874, CPD−35°1579, GC 10510, HD 63399, HIP 37996, SAO 198437[12]
Database references
SIMBADdata
Close

HD 63399 is a red giant star that is currently on the red giant branch,[3] fusing hydrogen in a shell around its core. It has a stellar classification of K1 III.[4] At present it has a mass ranging from 1.3 to 1.7 times the mass of the Sun,[8][9] depending on the study. HD 63399 has expanded to 10.8 times its girth[10] and now radiates 54.8 times the luminosity of the Sun[6] from its swollen photosphere at an effective temperature of 4,761 K.[11] The star has an iron abundance 13% below solar levels, making it slightly metal deficient.[3]

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