B(t) = 4.0 + 0.35 sin(2mt/5.4)

Algebra & Trigonometry with Analytic Geometry
13th Edition
ISBN:9781133382119
Author:Swokowski
Publisher:Swokowski
Chapter7: Analytic Trigonometry
Section7.2: Trigonometric Equations
Problem 104E
icon
Related questions
Topic Video
Question

A Cepheid variable star is a star whose brightness alternately
increases and decreases. The most easily visible such
star is Delta Cephei, for which the interval between times of
maxi mum brightness is 5.4 days. The average brightness of
this star is 4.0 and its brightness changes by ± 0.35 . In view
of these data, the brightness of Delta Cephei at time t , where
t is measured in days, has been modeled by the function given below

(a) Find the rate of change of the brightness after days.
(b) Find, correct to two decimal places, the rate of increase
after one day.

B(t) = 4.0 + 0.35 sin(2mt/5.4)
Transcribed Image Text:B(t) = 4.0 + 0.35 sin(2mt/5.4)
Expert Solution
trending now

Trending now

This is a popular solution!

steps

Step by step

Solved in 2 steps with 2 images

Blurred answer
Knowledge Booster
Discrete Probability Distributions
Learn more about
Need a deep-dive on the concept behind this application? Look no further. Learn more about this topic, calculus and related others by exploring similar questions and additional content below.
Recommended textbooks for you
Algebra & Trigonometry with Analytic Geometry
Algebra & Trigonometry with Analytic Geometry
Algebra
ISBN:
9781133382119
Author:
Swokowski
Publisher:
Cengage