HD 82741

Star in the constellation Lynx From Wikipedia, the free encyclopedia

HD 82741 is a single[10] star in the northern constellation of Lynx. It is visible to the naked eye with an apparent visual magnitude of 4.81.[1] The distance to HD 82741 is 223 light years, as determined from its annual parallax shift of 14.6 mas.[2] It is moving further from the Earth with a heliocentric radial velocity of 1 km/s.[1]

Right ascension09h 35m 03.83005s[2]
Declination+39° 37 17.3743[2]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
HD 82741
Observation data
Epoch J2000      Equinox J2000
Constellation Lynx[1]
Right ascension 09h 35m 03.83005s[2]
Declination +39° 37 17.3743[2]
Apparent magnitude (V) 4.81[1]
Characteristics
Evolutionary stage red clump[3]
Spectral type G9.5 IIIb Fe-1[4]
B−V color index 0.980[5]
Astrometry
Radial velocity (Rv)0.992±0.002[1] km/s
Proper motion (μ) RA: −30.124[2] mas/yr
Dec.: +20.155[2] mas/yr
Parallax (π)14.6281±0.2230 mas[2]
Distance223 ± 3 ly
(68 ± 1 pc)
Absolute magnitude (MV)0.573[5]
Details
Mass1.62[6] M
Radius8.78±0.61[7] R
Luminosity58.9[6] L
Surface gravity (log g)2.6[8] cgs
Temperature4,809±51[6] K
Metallicity [Fe/H]−0.18[5] dex
Rotational velocity (v sin i)1.0[8] km/s
Age2.74[6] Gyr
Other designations
BD+40°2224, FK5 2762, HD 82741, HIP 47029, HR 3809, SAO 61578[9]
Database references
SIMBADdata
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At the age of 2.74[6] billion years, this is an evolved giant star with a stellar classification of G9.5 IIIb Fe-1,[4] where the suffix notation indicates an underabundance of iron in its atmosphere. It belongs to a sub-category of giants called the red clump, indicating that it is on the horizontal branch and is generating energy through the fusion of helium at its core.[3] With 1.62 times the mass of the Sun,[6] it has expanded to 9 times the Sun's radius.[7] It is radiating 58.9 times the Sun's luminosity[6] from its enlarged photosphere at an effective temperature of 4,809 K.[6]

References

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