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A pulsar is a rapidly rotating neutron star. The Crab nebula pulsar in the constellation Taurus has a period of 33.5\times 10^{-3}~\text{s}33.5×10 ​−3 ​​ s, radius 10.0 km, and mass 2.8\times 10^{30}~\text{kg}2.8×10 ​30 ​​ kg. The pulsar’s rotational period will increase over time due to the release of electromagnetic radiation, which doesn’t change its radius but reduces its rotational energy. What is the angular momentum of the pulsar?

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Answer:


5.25\cdot 10^(40) kg m^2/s

Step-by-step explanation:

The angular momentum of the pulsar is given by:


L=m\omega r^2

where


m=2.8\cdot 10^(30) kg is the mass of the pulsar


r = 10.0 km = 1\cdot 10^4 m is the radius


\omega is the angular speed

Given the period of the pulsar,
T=33.5\cdot 10^(-3) s, the angular speed is given by


\omega=(2\pi)/(T)=(2 \pi)/(33.5\cdot 10^(-3)s)=187.5 rad/s

And so, the angular momentum is


L=m\omega r^2=(2.8\cdot 10^(30)kg)(187.5 rad/s)(1\cdot 10^4 m)^2=5.25\cdot 10^(40) kg m^2/s

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