f = L / (4pi'd2), where:
f: apparent brightness
L: luminosity
d: distance of star
(p and i' stay constant between the two stars, so let's make them both equal to 1)
Let's say the closer star has a distance of 1 and the further has a distance of 2, and they both have a luminosity of L.
Apparent brightness of further star:
f = L/(4*2^2) = L/16
Apparent brightness of closer star:
f = L/(4*1^2) = L/4
As you can see here, the apparent brightnesses of the two stars differ by a factor of 4.
Answer: B. four times as great as the second star’s.