a) The relationship is given as
mB - mA = -2.5 log (f1 / f2)
mB - mA = -2.5 log (10)
mB - mA = -2.5
mB - mA = 2.5
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b) we know
flux = luminosity * distance2
for star A and B
flux (A) / flux (B) = luminosity (A) * distance2 (A) / luminosity (B) * distance2 (B)
As distance of both stars is same, we have
flux (A) / flux (B) = luminosity (A) / luminosity (B)
Therefore,
LA / LB = fluxA / fluxB
LA / LB = 1/10
LA / LB = 0.1
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