HD 24160

Star in the constellation Eridanus From Wikipedia, the free encyclopedia

HD 24160 is a single[10] star in the equatorial constellation of Eridanus. It has the Bayer designation g Eridani. It is visible to the naked eye with an apparent visual magnitude of 4.17.[1] The distance to HD 24160 can be estimated from its annual parallax shift of 14.98 mas,[2] yielding a separation of 218 light years. It is moving further from the Earth with a heliocentric radial velocity of +2 km/s.[5] This object is a coronal member of the Ursa Major Moving Group of stars that share a common motion through space.[11]

Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
HD 24160
Location of HD 24160 (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Eridanus[1]
Right ascension 03h 49m 27.24527s[2]
Declination −36° 12 34.8771[2]
Apparent magnitude (V) 4.17[1]
Characteristics
Evolutionary stage red clump[3]
Spectral type G7 III[4]
B−V color index 0.927±0.045[1]
Astrometry
Radial velocity (Rv)+2.0±0.7[5] km/s
Proper motion (μ) RA: −45.547(77) mas/yr[2]
Dec.: −49.503(108) mas/yr[2]
Parallax (π)14.9781±0.0915 mas[2]
Distance218 ± 1 ly
(66.8 ± 0.4 pc)
Absolute magnitude (MV)0.13[1]
Details
Mass2.33[6] M
Radius11[7] R
Luminosity81.3[6] L
Surface gravity (log g)2.85±0.08[8] cgs
Temperature4,948±45[6] K
Metallicity [Fe/H]+0.08±0.02[8] dex
Age1.76[6] Gyr
Other designations
g Eri, CD−36°1467, FK5 143, HD 24160, HIP 17874, HR 1195, SAO 194559[9]
Database references
SIMBADdata
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At the age of 1.76 billion years old, HD 24160 is an evolved G-type giant with a stellar classification of G7 III,[4] having consumed the hydrogen at its core and tracked away from the main sequence. It has 2.33[6] times the mass of the Sun and has expanded to about 11[7] times the Sun's radius. The star is radiating 81.3[6] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,948 K.[6]

References

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