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+5−5lg(r)M=m+5-5 \lg{(r)}M=m+5−5lg(r)
Where
M−M-M− absolute magnitude
m−m-m− apparent magnitude
where do we write
M−m=5−5lg(r)M-m=5-5 \lg{(r)}M−m=5−5lg(r)
by problem statement
M−m=5M-m=5M−m=5
then
5=5−5lg(r)5=5-5 \lg{(r)}5=5−5lg(r)
5−5=−5lg(r)5-5=-5 \lg{(r)}5−5=−5lg(r)
0=−5lg(r)0=-5 \lg{(r)}0=−5lg(r)
0=lg(r)0=\lg{(r)}0=lg(r)
from where
r=1pcr=1 pcr=1pc
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