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Question
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 $m = -2.78(\log p) - 1.35$, where $m$ is the absolute magnitude, or brightness, of the star, and $p$ is the number of days required for the star to complete one cycle. use a calculator to solve each problem. round your answers to the nearest hundredth. what is the absolute magnitude of a star that has a period of 62 days? what is the absolute magnitude of a star that has a period of 50 days?
Step1: Calculate $\log(62)$
$\log(62) \approx 1.7924$
Step2: Substitute into the formula for $P=62$
$M = -2.78\times1.7924 - 1.35$
$M \approx -5.0829 - 1.35$
$M \approx -6.43$
Step3: Calculate $\log(50)$
$\log(50) \approx 1.6990$
Step4: Substitute into the formula for $P=50$
$M = -2.78\times1.6990 - 1.35$
$M \approx -4.7232 - 1.35$
$M \approx -6.07$
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For a period of 62 days: $-6.43$
For a period of 50 days: $-6.07$