Microscopium
Origin
Microscopium is a faint minor constellation in the southern hemisphere sky. It is one of twelve IAU constellations created by Nicolas-Louis de Lacaille in 1751. Lacille cataloged ten thousand stars in the southern hemisphere during a voyage and sabbatical at the Cape of Good Hope from 1750 to 1754. From these stars de Lacaille devised many new constellations which honored the Age of Enlightenment. The constellation was first introduced as the French ‘le Microscope’ and was later latinised to Microscopium by 1763.
Bright Stars
The brightest star in Microscopium is Gamma Microscopii with an apparent brightness of 4.68, which is too faint to be observed through city-level light pollution. Gamma Microscopii is a yellow giant star which likely passed between 1.14 & 3.45 light-years from the Sun approximately 3.9 million years ago; this close encounter might have disturbed the Oort Cloud of the Solar System.
Within Microscopium there are only 43 stars that are bright enough to be seen with the naked eye, all of which are fainter than magnitude 4.5, making them difficult to see against light pollution.


Credit: E. Slawik/NOIRLab/NSF/AURA/M. Zamani
Notable Objects
Most Notable objects are too faint to be seen with the naked eye.
AX Microscopii/Lacaille 8760 is the brightest red dwarf star in the sky (at magnitude 6.68). It is located 12.9 light-years from the Sun.
BO Microscopii, also known as Speedy Mic, is a rapidly rotating star, with a rotation period of 9 hours 7 minutes.
AU Microscopii is a young star in the process of forming planets.
NGC 6925 is a barred spiral galaxy of magnitude 11.3.
The Microscopium Supercluster is a galaxy cluster first observed in the 1990ʻs.
