Beta Microscopii

β Microscopii
Location of β Microscopii (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Microscopium
Right ascension 20h 51m 58.7618s
Declination −33° 10 40.705
Apparent magnitude (V) 6.05±0.01
Characteristics
Spectral type A1 IV
B−V color index +0.03
Astrometry
Radial velocity (Rv)−12±4.3 km/s
Proper motion (μ) RA: +7.712 mas/yr
Dec.: −5.568 mas/yr
Parallax (π)6.5022±0.0451 mas
Distance502 ± 3 ly
(154 ± 1 pc)
Absolute magnitude (MV)+0.22
Details
Mass2.96 M
Radius3.5±0.1 R
Luminosity77.25 L
Surface gravity (log g)3.58 cgs
Temperature8,942 K
Metallicity [Fe/H]0.00 dex
Rotational velocity (v sin i)275±3 km/s
Age337 Myr
Other designations
β Mic, 32 Microscopii, CD−33°15245, HD 198529, HIP 102989, HR 7979, SAO 212499
Database references
SIMBADdata

Beta Microscopii (Beta Mic), Latinized from β Microscopii, is a solitary star in the constellation Microscopium. It is close to the lower limit of stars that are visible to the naked eye having an apparent visual magnitude of 6.05 Based upon an annual parallax shift of 6.5022 mas as seen from Earth, this star is located 502 light years away from the Sun. At that distance, the visual magnitude is diminished by an extinction factor of 0.19 due to interstellar dust.

Beta Mic has a stellar classification of A1 IV, indicating that it is an evolved A-type subgiant. Older sources give it a class of A2 Vn, suggesting that it is an A-type main-sequence star with nebulous absorption lines due to rapid rotation. Consistent with the older classification, the star is spinning rapidly with a projected rotational velocity of 275 km/s. The star has 2.96 times the mass of the Sun and due to its evolved status, has a radius of 3.5 R. It radiates at 77.2 times the luminosity of the Sun from its photosphere at an effective temperature of 8,942 K, giving a white hue. Beta Mic has a solar metallicity and is estimated to be around 340 million years old.