A Cepheid star is a type of variable star, which means that its brightness is not constant.
The relationship between the brightness of a Cepheid star and its period, or length of its pulse, is given by:
[tex]\[ M = -2.78(\log P) - 1.35 \][/tex]
where [tex]\( M \)[/tex] is the absolute magnitude, or brightness, of the star, and [tex]\( P \)[/tex] is the number of days required for the star to complete one cycle.
Use a calculator to solve the problem. Round your answer to the nearest hundredth.
What is the absolute magnitude of a star that has a period of 62 days?
[tex]\[ \boxed{} \][/tex]