Conservation of Angular Momentum of Star

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SUMMARY

The discussion focuses on calculating the new angular velocity of a star with a mass of 1.51·1031 kg and an initial angular velocity of 1.50E-7 rad/s after its diameter shrinks to 0.49 times its original size. Using the conservation of angular momentum, the initial angular momentum L(int) is expressed as L(int) = (2/5)M*R2*wint and the final angular momentum L(final) as L(final) = (2/5)M*(0.49R)2*wfinal. The radius cancels out in the equations, allowing for the calculation of the new angular velocity without needing the actual radius value.

PREREQUISITES
  • Understanding of angular momentum (L = Iω)
  • Familiarity with the moment of inertia for a solid sphere (Icm = 2/5 mR2)
  • Basic knowledge of uniform mass distribution
  • Ability to manipulate algebraic equations
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  • Explore the moment of inertia for different shapes and mass distributions
  • Learn about the effects of radius changes on angular velocity
  • Investigate real-world applications of angular momentum conservation in astrophysics
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ganondorf29
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Homework Statement


The mass of a star is 1.51·1031 kg and its angular velocity is 1.50E-7 rad/s. Find its new angular velocity if the diameter suddenly shrinks to 0.49 times its present size. Assume a uniform mass distribution before and after. Icm for a solid sphere of uniform density is 2/5 mr2


Homework Equations



L=Iw

L(int)=L(final)


The Attempt at a Solution



L(int) = [(2/5)M*R^2]*(wint)
L(final) = [(2/5)M*(0.49)*R^2]*(wfinal)

And I got stuck there. I don't know how to find the radius and I think that's holding me back.
 
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Note that it will cancel out when you set them equal since you've expressed the final radius in terms of the initial radius.

Be careful with the 0.49, it should be squared as well.
 

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