A pulsar is a rapidly rotating neutron star that emits a radio beam the way a lighthouse emits a light beam. We receive a radio pulse for each rotation of the star. The period $T$ of rotation is found by measuring the time between pulses. The pulsar in the Crab nebula has a period of rotation of $T=0.033 \mathrm{~s}$ that is increasing at the rate of $1.26 \times 10^{-5} \mathrm{~s} / \mathrm{y}$. (a) What is the pulsar's angular acceleration $\alpha ?$ (b) If $\alpha$ is constant, how many years from now will the pulsar stop rotating? (c) The pulsar originated in a supernova explosion seen in the year $1054 .$ Assuming constant $\alpha,$ find the initial $T$