At what distance does a star have an apparent magnitude that is 5 magnitudes brighter (smaller) than its absolute magnitude?
Let's apply the formula
"M=m+5-5 \\lg{(r)}"
Where
"M-" absolute magnitude
"m-" apparent magnitude
where do we write
"M-m=5-5 \\lg{(r)}"
by problem statement
"M-m=5"
then
"5=5-5 \\lg{(r)}"
"5-5=-5 \\lg{(r)}"
"0=-5 \\lg{(r)}"
"0=\\lg{(r)}"
from where
"r=1 pc"
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