Gamma2 Normae

Gamma2 Normae
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Norma
Right ascension 16h 19m 50.42231s
Declination 50° 09 19.8216
Apparent magnitude (V) 4.02
Characteristics
Evolutionary stage Red clump
Spectral type K0III
U−B color index +1.16
B−V color index +1.08
Astrometry
Radial velocity (Rv)−29.15±0.42 km/s
Proper motion (μ) RA: −159.666 mas/yr
Dec.: −51.94 mas/yr
Parallax (π)23.5698±0.1272 mas
Distance138.4 ± 0.7 ly
(42.4 ± 0.2 pc)
Absolute magnitude (MV)0.86±0.04
Details
Mass2.06±0.23 M
Radius10.35±0.35 R
Luminosity49.7±2.2 L
Surface gravity (log g)2.750±0.171 cgs
Temperature4,763±63 K
Metallicity [Fe/H]+0.250±0.036 dex
Other designations
γ2 Nor, CD−49°10536, GC 12216, GJ 9554, HD 146686, HIP 80000, HR 6072, SAO 243643
Database references
SIMBADdata
ARICNSdata

Gamma2 Normae, Latinized from γ2 Nor, is the brightest star in the southern constellation of Norma. Its apparent magnitude is 4.02 – making it a faint star but visible to the naked eye. Based upon an annual parallax shift of 23.57 mas as seen from Earth, this star is located roughly 129 light years away. It is moving closer to the Sun with a radial velocity of −29 km/s.

This is an evolved, orange-hued giant of spectral type K0 III. A red clump star, it achieved the fusion of helium at its core and is now in the evolutionary stage known as horizontal branch. The star is around 2.16 times as massive as the Sun and has grown to a diameter 10.35 times that of the Sun. The star is radiating 50 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,763 K.

Gamma2 Normae is a close double, with a magnitude 10 companion. The pair has been previously identified as a binary star system, but parallax measurements the Gaia spacecraft data showed the companion star to be much more distant. A white dwarf located 24.38" away has similar distance and proper motion with Gamma2 Normae.