JEE Rotational

A binary star consists of two stars A (mass 2.2 2.2\quad Ms) and B (mass 11 11\quad Ms), where Ms is the mass of the sun. They are separated by distance d and are rotating about their centre of mass, which is stationary. The ratio of the total angular momentum of the binary star to the angular momentum of star B about the centre of mass is...


The answer is 6.

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2 solutions

Anuj Mishra
Jul 17, 2015

A nice problem..

Angular momentum of a body revolving with an angular velocity w = m r 2 w w\, = m*r^2*w

Since they are revolving around a fixed center of mass, their angular velocity must be same. Thus, A n g u l a r m o m e n t u m o f t o t a l s y s t e m A n g u l a r m o m e n t u m o f B = m 1 r 1 2 + m 2 r 2 2 m 2 r 2 2 \frac {Angular\ momentum\ of\ total\ system}{Angular\ momentum\ of\ B} = \frac {m_1*r_1^2+ m_2*r_2^2 }{m_2*r_2^2}

= m 1 r 1 2 m 2 r 2 2 + 1 = \frac {m_1*r_1^2 }{m_2*r_2^2} + 1

= 6 \boxed {= 6 }

Let xd be the distance of 2.2 from center of mass and (1-x)d that of 11. Angler velocity = ω \omega same for both.
Since moments about mass center are equal, 2.2 * xd=11 * (1-x)d.......So x=5/6, and 1-x=1/6.
B m o m e n t u m = ( d 6 ) 2 11 ω . A m o m e n t u m = ( 5 d 6 ) 2 2.2 ω . r e q u i r e d r a t i o = ( d 6 ) 2 11 ω + ( 5 d 6 ) 2 2.2 ω ( d 6 ) 2 11 ω = 6. \therefore\ B_{momentum}=(\dfrac d 6)^2*11*\omega.\\ \therefore\ A_{momentum}=(\dfrac {5d} 6)^2*2.2*\omega.\\ \therefore\ required\ ratio\ =\dfrac{( \dfrac d 6)^2*11*\omega+(\dfrac {5d} 6)^2*2.2*\omega}{( \dfrac d 6)^2*11*\omega}=\large\ \ \color{#D61F06}{6}.

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