The ratio of brightness of two stars can be determined by a constant of 2.512 raised to the power of the magnitude difference. The formula
b1

b2
= 2.512(m2 − m1) where b1 and b2 represent the brightness and m1 and m2 refer to the magnitudes of the stars being compared. One star has a magnitude of 0.2, and another star has a magnitude of 2.2. What is the ratio of brightness of these two stars?