Lambda Normae

Lambda Normae
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Norma
Right ascension 16h 19m 17.64660s
Declination −42° 40 26.3014
Apparent magnitude (V) 5.44 (5.83 + 6.86)
Characteristics
Spectral type A0V + A3V
B−V color index 0.099±0.004
Astrometry
Radial velocity (Rv)−15.0±3.7 km/s
Proper motion (μ) RA: +7.59 mas/yr
Dec.: −13.30 mas/yr
Parallax (π)9.35±0.76 mas
Distance350 ± 30 ly
(107 ± 9 pc)
Absolute magnitude (MV)0.31
Orbit
Period (P)67.50 yr
Semi-major axis (a)0.293″
Eccentricity (e)0.788
Inclination (i)45.8°
Longitude of the node (Ω)215.2°
Periastron epoch (T)2049.59 B
Argument of periastron (ω)
(secondary)
82.5°
Details
Luminosity64 L
λ Nor A
Mass2.53–2.57 M
λ Nor B
Mass2.00–2.13 M
Other designations
λ Nor, CD−42°11188, HD 146667, HIP 79963, HR 6071, SAO 226650, WDS J16193-4240
Database references
SIMBADdata

λ Normae, Latinised as Lambda Normae, is a binary star system in the southern constellation of Norma, located near the northern constellation boundary with Scorpius. It is visible to the naked eye as a dim, white-hued point of light that shines with a combined apparent visual magnitude of 5.44. The system is located approximately 350 light years distant from the Sun based on parallax, but is drifting closer with a radial velocity of about −15 km/s.

The pair have an orbital period of 67.5 years with a high eccentricity of 0.788. Both components are A-type main-sequence stars that are generating energy through core hydrogen fusion. The primary component has a visual magnitude of 5.83, and is of class A0V. The fainter secondary is class A3V with a magnitude 6.86.