The penetrating power of the telescope is characterized by the limiting magnitude m of the faintest star that can be seen in this instrument.
If the diameter of the telescope
D=100m=100000mmD=100m=100000mmD=100m=100000mm
then
m=2.1+5⋅lg(D)=2.1+5⋅lg(100000)=2.1+5⋅5=27.1mm=2.1+5\cdot \lg{(D)}=2.1+5\cdot \lg{(100000)}=2.1+5 \cdot 5=27.1^mm=2.1+5⋅lg(D)=2.1+5⋅lg(100000)=2.1+5⋅5=27.1m
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