A Cepheid variable star is a star whose brightness alternately increases and decreases. Suppose that Cephei Joe is a star for which the interval between times of maximum brightness is 5.3 days. Its average brightness is 3.1 and the brightness changes by +/-0.25. Using this data, we can construct a mathematical model for the brightness of Ceph Joe at time t, where t is measured in days: B(t) = 3.1 + 0.25 sin(2nt/5.3) (a) Find the rate of change of the brightness after t days. Rate of change = !! (b) Find the rate of increase after one day. Rate of increase =

Algebra & Trigonometry with Analytic Geometry
13th Edition
ISBN:9781133382119
Author:Swokowski
Publisher:Swokowski
Chapter5: Inverse, Exponential, And Logarithmic Functions
Section5.6: Exponential And Logarithmic Equations
Problem 64E
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A Cepheid variable star is a star whose brightness alternately increases and decreases. Suppose that Cephei Joe is a
star for which the interval between times of maximum brightness is 5.3 days. Its average brightness is 3.1 and the
brightness changes by +/-0.25. Using this data, we can construct a mathematical model for the brightness of Cephei
Joe at time t, where t is measured in days:
B(t) = 3.1 + 0.25 sin(2nt/5.3)
(a) Find the rate of change of the brightness after t days.
Rate of change =
(b) Find the rate of increase after one day.
Rate of increase
%3D
Transcribed Image Text:A Cepheid variable star is a star whose brightness alternately increases and decreases. Suppose that Cephei Joe is a star for which the interval between times of maximum brightness is 5.3 days. Its average brightness is 3.1 and the brightness changes by +/-0.25. Using this data, we can construct a mathematical model for the brightness of Cephei Joe at time t, where t is measured in days: B(t) = 3.1 + 0.25 sin(2nt/5.3) (a) Find the rate of change of the brightness after t days. Rate of change = (b) Find the rate of increase after one day. Rate of increase %3D
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