Eta Normae

G-type star in the constellation Norma From Wikipedia, the free encyclopedia

Eta Normae, Latinized from η Normae, is a single[8] star in the southern constellation of Norma. It is visible to the naked eye as a faint, yellow-hued star with an apparent visual magnitude of 4.65.[2] The distance to this star is about 219 light years, based on parallax.[1] The Gamma Normids radiate from a position near this star.[9]

Right ascension16h 03m 12.89783s[1]
Declination49° 13 46.9151[1]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
Eta Normae
Location of η Normae (circled in red)
Observation data
Epoch J2000      Equinox J2000
Constellation Norma
Right ascension 16h 03m 12.89783s[1]
Declination 49° 13 46.9151[1]
Apparent magnitude (V) 4.65[2]
Characteristics
Evolutionary stage red clump[3]
Spectral type G8III[4]
U−B color index +0.64[2]
B−V color index +0.92[2]
Astrometry
Radial velocity (Rv)−0.3±2.8[5] km/s
Proper motion (μ) RA: 42.05[1] mas/yr
Dec.: 9.14[1] mas/yr
Parallax (π)14.86±0.25 mas[1]
Distance219 ± 4 ly
(67 ± 1 pc)
Absolute magnitude (MV)0.524[3]
Details
Mass2.78[3] M
Radius11.07+0.23
−0.09
[6] R
Luminosity71.9±3.1[6] L
Surface gravity (log g)2.84[3] cgs
Temperature5052+16
−51
[6] K
Metallicity [Fe/H]−0.05[3] dex
Other designations
η Nor, CD−48°10512, HD 143546, HIP 78639, HR 5962, SAO 226466[7]
Database references
SIMBADdata
Close

This is an aging giant star with a stellar classification of G8III,[4] having exhausted the supply of hydrogen at its core then swollen and cooled off the main sequence. At present it has a diameter of 11[6] times that of the Sun. It is a red clump[3] giant, meaning it is on the horizontal branch and is generating energy through core helium fusion. The star has 2.78[3] times the mass of the Sun and is radiating 72[6] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 5,052 K.[6] It is a source for X-ray emission.[10]

References

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