Lambda2 Sculptoris

Lambda2 Sculptoris
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Sculptor
Right ascension 00h 44m 12.09903s
Declination −38° 25 18.0542
Apparent magnitude (V) +5.90
Characteristics
Evolutionary stage Horizontal branch
Spectral type K1 III
B−V color index +1.15
Astrometry
Radial velocity (Rv)+28.22±0.13 km/s
Proper motion (μ) RA: +245.567 mas/yr
Dec.: +119.038 mas/yr
Parallax (π)9.8530±0.0458 mas
Distance331 ± 2 ly
(101.5 ± 0.5 pc)
Absolute magnitude (MV)+0.82
Details
Mass1.26±0.09 or 1.12±0.06 M
Radius12.01±0.14 R
Luminosity56.7±1.4 L
Surface gravity (log g)2.34±0.10 cgs
Temperature4,572±35 K
Metallicity [Fe/H]+0.01±0.08 dex
Age4.64±1.01 or 6.50±1.22 Gyr
Other designations
λ2 Scl, CD−39°181, FK5 26, HD 4211, HIP 3456, HR 195, SAO 192703
Database references
SIMBADdata

Lambda2 Sculptoris is an orange-hued star in the southern constellation of Sculptor. On dark nights it is faintly visible to the naked eye, having an apparent visual magnitude of +5.90. Based upon an annual parallax shift of 9.63 mas as measured from Earth, it is located at a distance of 331 light-years. It has a relatively large proper motion, advancing 0.273 arcsecond per year across the sky.

The spectrum of this star matches a spectral class of K1III, with the luminosity class III indicating it is a giant star that has exhausted the hydrogen at its core. It is now fusing helium, being in the evolutionary stage known as the horizontal branch. Estimates of its mass and age give two different values: 1.12 or 1.26 solar masses and 4.64 or 6.50 billion years. It has expanded to 12.01 times the Sun's radius and radiates 56.7 times the solar luminosity from its photosphere at an effective temperature of 4,572 K.