Pi Mensae

Pi Mensae (π Men), also known as HD 39091, is a yellow dwarf star in the constellation of Mensa. This star has a high proper motion. The apparent magnitude is 5.67, which can be visible to the naked eye in exceptionally dark, clear skies. It is nearly 60 light-years away. The star is slightly larger than the Sun in terms of mass, size, luminosity, temperature and metallicity, and is about 730 million years younger. It hosts three known planets.

Pi Mensae
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Mensa
Right ascension 05h 37m 09.88684s
Declination −80° 28 08.8346
Apparent magnitude (V) +5.65
Characteristics
Spectral type G0 V
U−B color index 0.11
B−V color index 0.60
V−R color index 0.31
R−I color index 0.29
Variable type none
Astrometry
Radial velocity (Rv)10.71±0.12 km/s
Proper motion (μ) RA: 310.909 mas/yr
Dec.: 1,049.060 mas/yr
Parallax (π)54.6825 ± 0.0354 mas
Distance59.65 ± 0.04 ly
(18.29 ± 0.01 pc)
Absolute magnitude (MV)+4.35±0.01
Details
Mass1.11±0.01 M
Radius1.15±0.01 R
Luminosity1.532±0.004 L
Surface gravity (log g)4.35±0.01 cgs
Temperature6,013±18 K
Metallicity [Fe/H]0.09 dex
Rotational velocity (v sin i)2.96 km/s
Age3.4±0.6 Gyr
Other designations
π Men, CD−80° 195, CPD−80° 161, GJ 9189, HD 39091, HIP 26394, HR 2022, SAO 258421, LFT 429, LHS 208, LTT 2359, TOI-144
Database references
SIMBADdata
ARICNSdata
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