A Cepheid variable star is a star whose brightness, B , alternately increases and decreases. Suppose that Cephei Joe is a star for which the interval between times of maximum brightness is 6.1 days. Its average brightness is 5 and the brightness changes by +/-0.6. 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) = 5 + 0.6sin ( 2pi(t) / 6.1)
(a) Find the rate of change of the brightness, in units of brightness per day, after t
days.
Rate of change =
(b) Find the rate of change of increase, in units of brightness per day, after one day.
Rate of change of increase =