Binary Stars: Moment of Inertia & Angular Momentum

AI Thread Summary
The discussion focuses on calculating the moment of inertia and angular momentum of a binary star system with stars A and B in circular orbits around their common center of mass. The moment of inertia is expressed as the sum of the individual moments, calculated using the formula I = m1r1^2 + m2r2^2. For angular momentum, it can be derived by multiplying the moment of inertia by the angular velocity, which is given by 2π/T. It's emphasized that both stars must rotate in the same direction to correctly sum their angular momenta. The calculations and concepts presented are confirmed to be accurate.
lucifer
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two stars, A and B, are in circular orbit of radii r1 and r2, respectively, about their common center of mass. each star has the same period of revolution T.

Determine expressions for the following two quantities in terms of the stars' masses, radii and T.

1- the moment of inertia of the two star system about it's center of mass
2- the angular momentum of the system about teh center of mass

for the moi, i highly doubt it but... would it just be m1r1^2 + m2r2^2 ?

and then to find the angular momentum i can just multiply the I i got before with 2pi/T... ?

thanks. :-)
 
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Consider the centre of mass of the system to be the rotational axis. The moment of inertia is simply the sum of the individual moments. Each moment is given as mr^2. What does that make the moment of inertia?
 
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The answers look fine to me.
Be sure to convince yourself that the planets are rotating in the same direction (both clockwise or both counterclockwise), so you can add the angular momenta of the two instead of subtracting them.
 
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