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=100000mm"
then
"m=2.1+5\\cdot \\lg{(D)}=2.1+5\\cdot \\lg{(100000)}=2.1+5 \\cdot 5=27.1^m"
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