Step 1: The formula for the radius of gyration \( K \) of a hollow cylinder about its central axis (the long axis of symmetry) is given by: \[ K = \sqrt{\frac{I}{M}} \] where \( I \) is the moment of inertia and \( M \) is the mass of the hollow cylinder.
Step 2: The moment of inertia \( I \) of a hollow cylinder about its central axis is: \[ I = M R^2 \] where \( R \) is the radius of the hollow cylinder.
Step 3: Substitute the expression for \( I \) into the formula for \( K \): \[ K = \sqrt{\frac{M R^2}{M}} = \sqrt{R^2} = R \] Thus, the radius of gyration \( K \) is equal to the radius \( R \) of the hollow cylinder.
Kepler's second law (law of areas) of planetary motion leads to law of conservation of
Kepler's second law (law of areas) of planetary motion leads to law of conservation of