T Microscopii is a
semiregular variable
In astronomy, a semiregular variable star, a type of variable star, is a giant or supergiant of intermediate and late (cooler) spectral type showing considerable periodicity in its light changes, accompanied or sometimes interrupted by various irre ...
star in the constellation
Microscopium. It ranges from magnitude 6.74 to 8.11 over a period of 352 days.
Located around 700 light-years distant, it shines with a
bolometric luminosity 7,509 times that of the Sun and has a surface temperature of .
References
Microscopium
Microscopii, T
Semiregular variable stars
M-type giants
100935
194676
Durchmusterung objects
Emission-line stars
{{var-star-stub