HD 94717

From Wikipedia, the free encyclopedia

Right ascension10h 52m 28.63166s[2]
Declination−79° 33 33.9765[2]
HD 94717
Location of HD 94717 on the map (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Chamaeleon[1]
Right ascension 10h 52m 28.63166s[2]
Declination −79° 33 33.9765[2]
Apparent magnitude (V) 6.34±0.01[3]
Characteristics
Evolutionary stage red giant branch[2]
Spectral type K2 II/III[4]
U−B color index +1.57[5]
B−V color index +1.46[5]
Astrometry
Radial velocity (Rv)3.4±0.5[6] km/s
Proper motion (μ) RA: −11.341 mas/yr[2]
Dec.: +1.655 mas/yr[2]
Parallax (π)1.8682±0.021 mas[2]
Distance1,750 ± 20 ly
(535 ± 6 pc)
Absolute magnitude (MV)−2.10[7]
Details
Mass6.3±0.7[8] M
Radius77.8±3.9[9] R
Luminosity1,847+46
49
[2] L
Surface gravity (log g)1.47±0.04[2] cgs
Temperature4,446±122[10] K
Metallicity [Fe/H]−0.01[2] dex
Rotational velocity (v sin i)2.4±1.3[11] km/s
Age63±20[8] Myr
Other designations
28 G. Chamaeleontis[12], CD−78°438, CPD−78°589, GC 14988, HD 94717, HIP 53151, HR 4268, SAO 256768[13]
Database references
SIMBADdata

HD 94717, also known as HR 4268, is a solitary orange hued star located in the southern circumpolar constellation Chamaeleon. It has an apparent magnitude of 6.34,[3] placing it near the limit for naked eye visibility. The object is located relatively far at a distance of 1,750 light years based on Gaia DR3 parallax measurements,[2] but it is receding with a heliocentric radial velocity of 3.4 km/s.[6] At its current distance, HD 94717's brightness is diminished by 0.62 magnitudes due to interstellar dust.[14]

HD 94717 has a stellar classification of K2 II/III,[4] indicating that it is an evolved red giant with the blended luminosity class of a giant star and a bright giant. It is estimated to be 63 million years old,[8] enough time for it to cool and expand to 78 times the Sun's radius.[9] It has 6.3 times the mass of the Sun[8] and radiates 1,847 times the luminosity of the Sun[2] from its photosphere at an effective temperature of 4,446 K.[10] HD 94717 has a solar metallicity[2] and spins modestly with a projected rotational velocity of 2.4 km/s.[11]

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