HD 64307

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HD 64307
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Camelopardalis[1]
Right ascension 08h 00m 11.7385s[2]
Declination +73° 55 04.5036[2]
Apparent magnitude (V) 5.35±0.01[3]
Characteristics
Evolutionary stage red giant branch[4]
Spectral type K3 III[5]
U−B color index +1.64[6]
B−V color index +1.43[6]
Astrometry
Radial velocity (Rv)33.54±0.19[7] km/s
Proper motion (μ) RA: −8.194 mas/yr[2]
Dec.: −37.514 mas/yr[2]
Parallax (π)4.7407±0.0741 mas[2]
Distance690 ± 10 ly
(211 ± 3 pc)
Absolute magnitude (MV)−1.77[1]
Details
Mass1.19[8] M
Radius49.9[9] R
Luminosity (bolometric)892[10] L
Surface gravity (log g)1.18[8] cgs
Temperature4,264±122[11] K
Metallicity [Fe/H]−0.1[12] dex
Rotational velocity (v sin i)<2[13] km/s
Other designations
AG+74°195, BD+74°338, FK5 300, GC 10745, HD 64307, HIP 39117, HR 3075, SAO 6378
Database references
SIMBADdata

HD 64307, also known as HR 3075, is a solitary,[14] orange hued star located in the northern circumpolar constellation Camelopardalis. It has an apparent magnitude of 5.35,[3] allowing it to be faintly seen with the naked eye. Based on parallax measurements from the Gaia spacecraft, The object is estimated to be 690 light years[2] distant. It appears to be receding from the Sun, having a heliocentric radial velocity of 34 km/s.[7]

HD 64307 is an evolved star with a stellar classification of K3 III.[5] Gaia DR3 stellar evolution models place it on the red giant branch.[4] It has a mass comparable to the Sun[8] but due to its evolved state, it has an enlarged radius of 49.9 R. It shines with a bolometric luminosity of 892 L from its photosphere at an effective temperature of 4,264 K.[11] HD 64307 has an iron abundance 80% that of the Sun, and is also lithium enriched.[12] Like most giant stars, the object spins slowly, having a projected rotational velocity lower than 2 km/s.[13]

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