Nu Microscopii

ν Microscopii
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Microscopium
Right ascension 20h 33m 55.07257s
Declination −44° 30 57.7642
Apparent magnitude (V) 5.12
Characteristics
Evolutionary stage red giant branch
Spectral type K0 III
U−B color index +1.009
B−V color index +0.999±0.002
Astrometry
Radial velocity (Rv)8.7±2 km/s
Proper motion (μ) RA: +11.560 mas/yr
Dec.: −35.355 mas/yr
Parallax (π)12.9361±0.0955 mas
Distance252 ± 2 ly
(77.3 ± 0.6 pc)
Absolute magnitude (MV)+0.84
Details
Mass2.46 M
Radius11 R
Luminosity59 L
Surface gravity (log g)2.78 cgs
Temperature4,832 K
Metallicity [Fe/H]+0.05±0.10 dex
Rotational velocity (v sin i)2.02 km/s
Age377 Myr
Other designations
ν Mic, ν Ind, CD−44°14020, FK5 3643, HD 195569, HIP 101477, HR 7846, SAO 230276
Database references
SIMBADdata

ν Microscopii, Latinized as Nu Microscopii, is a star in the constellation Microscopium. It is an orange-hued star that is visible to the naked eye as a faint point of light with an apparent visual magnitude of 5.12. It is located at a distance of around 252 light-years from the Sun, based on parallax, and is drifting further away with a radial velocity of about +9 km/s.

ν Microscopii is an aging giant star with a stellar classification of K0 III. It has expanded to 11 times the girth of the Sun after exhausting the supply of hydrogen at its core and evolving off the main sequence. The star has 2.46 times the mass of the Sun. It is radiating 59 times the Sun's luminosity from its swollen photosphere at an effective temperature of 4,832 K.

ν Microscopii was first catalogued as Nu Indi by the French explorer and astronomer Nicolas Louis de Lacaille in 1756, before being reclassified in Microscopium and given its current Bayer designation of Nu Microscopii by Gould. Despite this, most recent studies and the SIMBAD database use the designation Nu Indi for the star HD 211998.