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Three spherical shells of masses M, 2M a...

Three spherical shells of masses `M`, `2M` and `3M` have radii `R`, `3R` and `4R` as shows in figure. Find net potential at point `P`,

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To find the net gravitational potential at point P due to the three spherical shells, we can use the formula for the gravitational potential \( V \) due to a spherical shell, which is given by: \[ V = -\frac{G M}{r} \] where \( G \) is the gravitational constant, \( M \) is the mass of the shell, and \( r \) is the distance from the center of the shell to the point where the potential is being calculated. ### Step-by-step Solution: 1. **Identify the masses and radii of the shells**: - Mass of shell 1: \( M_1 = M \), Radius: \( R_1 = R \) - Mass of shell 2: \( M_2 = 2M \), Radius: \( R_2 = 3R \) - Mass of shell 3: \( M_3 = 3M \), Radius: \( R_3 = 4R \) 2. **Calculate the distance from point P to the center of each shell**: - For shell 1 (mass \( M \)): - Distance \( r_1 = 2R \) (since point P is outside the shell) - For shell 2 (mass \( 2M \)): - Distance \( r_2 = 3R \) - For shell 3 (mass \( 3M \)): - Distance \( r_3 = 4R \) 3. **Calculate the potential at point P due to each shell**: - Potential due to shell 1: \[ V_1 = -\frac{G M}{r_1} = -\frac{G M}{2R} \] - Potential due to shell 2: \[ V_2 = -\frac{G (2M)}{r_2} = -\frac{2G M}{3R} \] - Potential due to shell 3: \[ V_3 = -\frac{G (3M)}{r_3} = -\frac{3G M}{4R} \] 4. **Calculate the net potential at point P**: - The net potential \( V \) at point P is the sum of the potentials due to each shell: \[ V = V_1 + V_2 + V_3 \] \[ V = -\frac{G M}{2R} - \frac{2G M}{3R} - \frac{3G M}{4R} \] 5. **Finding a common denominator**: - The common denominator for \( 2R, 3R, \) and \( 4R \) is \( 12R \). - Rewriting each term: \[ V = -\left(\frac{6G M}{12R} + \frac{8G M}{12R} + \frac{9G M}{12R}\right) \] \[ V = -\frac{(6G M + 8G M + 9G M)}{12R} = -\frac{23G M}{12R} \] ### Final Result: The net gravitational potential at point P is: \[ V = -\frac{23G M}{12R} \]

To find the net gravitational potential at point P due to the three spherical shells, we can use the formula for the gravitational potential \( V \) due to a spherical shell, which is given by: \[ V = -\frac{G M}{r} \] where \( G \) is the gravitational constant, \( M \) is the mass of the shell, and \( r \) is the distance from the center of the shell to the point where the potential is being calculated. ...
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