A Cepheid variable star is a star whose brightness alternately increases and decreases. For a certain star, the interval between times of maximum brightness is 6.2 days. The average brightness of this star is 3.0 and its brightness changes by ±0.25. In view of these data, the brightness of the star at time t, where t is measured in days, has been modeled by the function B(t)=4.2 +0.45sin(2pit/4.4)

(a) Find the rate of change of the brightness after t days.
(b) Find the rate of increase after one day.

Respuesta :

Answer:

a)

[tex]B'(t) = \dfrac{0.9\pi}{4.4}\cos\bigg(\dfrac{2\pi t}{4.4}\bigg)[/tex]

b) 0.09

Step-by-step explanation:

We are given the following in the question:

[tex]B(t) = 4.2 +0.45\sin\bigg(\dfrac{2\pi t}{4.4}\bigg)[/tex]

where B(t) gives the brightness of the star at time t, where t is measured in days.

a) rate of change of the brightness after t days.

[tex]B(t) = 4.2 +0.45\sin\bigg(\dfrac{2\pi t}{4.4}\bigg)\\\\B'(t) = 0.45\cos\bigg(\dfrac{2\pi t}{4.4}\bigg)\times \dfrac{2\pi}{4.4}\\\\B'(t) = \dfrac{0.9\pi}{4.4}\cos\bigg(\dfrac{2\pi t}{4.4}\bigg)[/tex]

b) rate of increase after one day.

We put t = 1

[tex]B'(t) = \dfrac{0.9\pi}{4.4}\cos\bigg(\dfrac{2\pi t}{4.4}\bigg)\\\\B'(1) = \dfrac{0.9\pi}{4.4}\bigg(\cos(\dfrac{2\pi (1)}{4.4}\bigg)\\\\B'(t) = 0.09145\\B'(t) \approx 0.09[/tex]

The rate of increase after 1 day is 0.09