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If a satellites is revolving close to a planet of density `rho` with period `T`, show that the quantity `rho T_(2)` is a universal constant.

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To show that the quantity \( \rho T^2 \) is a universal constant for a satellite revolving close to a planet of density \( \rho \) with period \( T \), we will follow these steps: ### Step 1: Understand the relationship between gravitational force and circular motion For a satellite of mass \( m \) revolving around a planet of mass \( M \) at a distance \( r \), the gravitational force provides the necessary centripetal force for circular motion. This can be expressed as: \[ \frac{GMm}{r^2} = m \omega^2 r \] where \( G \) is the gravitational constant and \( \omega \) is the angular velocity of the satellite. ### Step 2: Simplify the equation We can cancel \( m \) from both sides (assuming \( m \neq 0 \)): \[ \frac{GM}{r^2} = \omega^2 r \] Rearranging gives: \[ \omega^2 = \frac{GM}{r^3} \] ### Step 3: Relate angular velocity to the period The angular velocity \( \omega \) is related to the period \( T \) by the formula: \[ \omega = \frac{2\pi}{T} \] Substituting this into our equation gives: \[ \left(\frac{2\pi}{T}\right)^2 = \frac{GM}{r^3} \] which simplifies to: \[ \frac{4\pi^2}{T^2} = \frac{GM}{r^3} \] Rearranging this gives us: \[ T^2 = \frac{4\pi^2 r^3}{GM} \] ### Step 4: Express mass in terms of density The mass \( M \) of the planet can be expressed in terms of its density \( \rho \) and volume \( V \): \[ M = \rho V = \rho \left(\frac{4}{3} \pi r^3\right) \] Substituting this expression for \( M \) into our equation for \( T^2 \): \[ T^2 = \frac{4\pi^2 r^3}{G \left(\rho \frac{4}{3} \pi r^3\right)} \] This simplifies to: \[ T^2 = \frac{3\pi}{G\rho} \] ### Step 5: Show that \( \rho T^2 \) is a constant Now, multiplying both sides by \( \rho \): \[ \rho T^2 = \rho \cdot \frac{3\pi}{G\rho} = \frac{3\pi}{G} \] This shows that \( \rho T^2 \) is indeed a constant, specifically \( \frac{3\pi}{G} \), which is a universal constant. ### Conclusion Thus, we have shown that the quantity \( \rho T^2 \) is a universal constant. ---

To show that the quantity \( \rho T^2 \) is a universal constant for a satellite revolving close to a planet of density \( \rho \) with period \( T \), we will follow these steps: ### Step 1: Understand the relationship between gravitational force and circular motion For a satellite of mass \( m \) revolving around a planet of mass \( M \) at a distance \( r \), the gravitational force provides the necessary centripetal force for circular motion. This can be expressed as: \[ \frac{GMm}{r^2} = m \omega^2 r \] where \( G \) is the gravitational constant and \( \omega \) is the angular velocity of the satellite. ...
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