HD 36780

Star in the constellation Orion From Wikipedia, the free encyclopedia

HD 36780 is a star located in Orion's Belt, within the equatorial constellation of Orion. It has an orange hue and is dimly visible to the naked eye with an apparent visual magnitude of +5.92.[1] The distance to this object is approximately 525 light years based on parallax.[2] It is drifting away from the Sun with a radial velocity of 82 km/s,[2] having come to within 185.6 light-years some 2.1 million years ago.[1]

Right ascension05h 34m 04.04753s[2]
Declination−01° 28 12.8726[2]
Quick facts Constellation, Right ascension ...
HD 36780
Location of HD 36780 (circled) in the Orion's Belt region
Credit: Martin Mutti
Observation data
Epoch J2000      Equinox J2000
Constellation Orion[1]
Right ascension 05h 34m 04.04753s[2]
Declination −01° 28 12.8726[2]
Apparent magnitude (V) +5.92[1]
Characteristics
Evolutionary stage giant
Spectral type K4 III[3]
U−B color index +1.87[4]
B−V color index +1.535±0.008[1]
Astrometry
Radial velocity (Rv)82.45±0.21[2] km/s
Proper motion (μ) RA: −8.295[2] mas/yr
Dec.: −31.553[2] mas/yr
Parallax (π)6.2074±0.0975 mas[2]
Distance525 ± 8 ly
(161 ± 3 pc)
Absolute magnitude (MV)−0.65[1]
Details
Mass1.2[5] M
Radius33.8[6] R
Luminosity279[6] L
Surface gravity (log g)1.43[7] cgs
Temperature4,058[6] K
Rotational velocity (v sin i)2.1[8] km/s
Age12.4[7] Gyr
Other designations
BD−01°950, GC 6894, HD 36780, HIP 26108, HR 1874, SAO 132270[9]
Database references
SIMBADdata
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This is an aging giant star with a stellar classification of K4 III.[3] After exhausting the supply of hydrogen at its core, the star cooled and expanded off the main sequence. At present it has around 34 times the girth of the Sun. It is radiating 279 times the luminosity of the Sun from its swollen photosphere at an effective temperature of 4,058 K.[6]

References

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