Delta Mensae

Delta Mensae
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Mensa
Right ascension 04h 17m 59.27258s
Declination −80° 12 50.5073
Apparent magnitude (V) 5.69
Characteristics
Spectral type K2/3 III + A9
U−B color index +0.53
B−V color index +0.84
Astrometry
Radial velocity (Rv)−20.0±4.3 km/s
Proper motion (μ) RA: +27.719 mas/yr
Dec.: +61.679 mas/yr
Parallax (π)6.9662±0.1168 mas
Distance468 ± 8 ly
(144 ± 2 pc)
Absolute magnitude (MV)0.34
Details
δ Men A
Radius13.12+0.52
−0.46
 R
Luminosity111.7±2.2 L
Temperature5,180+94
−99
 K
Rotational velocity (v sin i)< 4.7±0.2 km/s
Other designations
δ Men, CPD−80°116, FK5 166, HD 28525, HIP 20049, HR 1426, SAO 258372
Database references
SIMBADdata

Delta Mensae, Latinized from δ Mensae, is a binary star system in the southern constellation of Mensa. It is faintly visible to the naked eye, having an apparent visual magnitude of 5.69. Based upon an annual parallax shift of 7.70 mas as seen from the Earth, it is 420 light years from the Sun.

The primary, designated component A, is a K-type giant star with a stellar classification of K2/3 III. With the supply of hydrogen at its core exhausted, it has cooled and expanded to 13 times the radius of the Sun. The star is radiating 112 times the Sun's luminosity from its photosphere at an effective temperature of 5,180 K. Its companion, component B, is an A-type star about 0.9 magnitudes fainter than the primary.