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Two masses 'M' and '4M' are at a distanc...

Two masses 'M' and '4M' are at a distance 'r' apart on the line joining them. 'P' is point where the resultant gravitational force is zero (such a point is called as null point). The distance of 'P' from the mass '4M' is

A

`r/5`

B

`r/3`

C

`(2r)/3`

D

`(4r)/5`

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The correct Answer is:
To find the distance of point 'P' from the mass '4M' where the resultant gravitational force is zero, we can follow these steps: ### Step-by-Step Solution 1. **Understanding the Setup**: - We have two masses: \( M \) and \( 4M \) separated by a distance \( r \). - Let point \( P \) be at a distance \( x \) from the mass \( 4M \). Therefore, the distance from mass \( M \) to point \( P \) will be \( r - x \). 2. **Gravitational Forces**: - The gravitational force exerted by mass \( M \) on a mass \( m \) at point \( P \) is given by: \[ F_1 = \frac{G \cdot M \cdot m}{(r - x)^2} \] - The gravitational force exerted by mass \( 4M \) on the mass \( m \) at point \( P \) is given by: \[ F_2 = \frac{G \cdot 4M \cdot m}{x^2} \] 3. **Setting Forces Equal**: - For the gravitational force to be zero at point \( P \), the magnitudes of \( F_1 \) and \( F_2 \) must be equal: \[ F_1 = F_2 \] - This leads to the equation: \[ \frac{G \cdot M \cdot m}{(r - x)^2} = \frac{G \cdot 4M \cdot m}{x^2} \] - We can cancel \( G \) and \( m \) from both sides since they are common factors: \[ \frac{M}{(r - x)^2} = \frac{4M}{x^2} \] 4. **Simplifying the Equation**: - Cancel \( M \) from both sides: \[ \frac{1}{(r - x)^2} = \frac{4}{x^2} \] - Cross-multiplying gives: \[ x^2 = 4(r - x)^2 \] 5. **Expanding and Rearranging**: - Expanding the right side: \[ x^2 = 4(r^2 - 2rx + x^2) \] - This simplifies to: \[ x^2 = 4r^2 - 8rx + 4x^2 \] - Rearranging gives: \[ 0 = 3x^2 - 8rx + 4r^2 \] 6. **Solving the Quadratic Equation**: - Using the quadratic formula \( x = \frac{-b \pm \sqrt{b^2 - 4ac}}{2a} \): - Here, \( a = 3 \), \( b = -8r \), and \( c = 4r^2 \). \[ x = \frac{8r \pm \sqrt{(-8r)^2 - 4 \cdot 3 \cdot 4r^2}}{2 \cdot 3} \] \[ x = \frac{8r \pm \sqrt{64r^2 - 48r^2}}{6} \] \[ x = \frac{8r \pm \sqrt{16r^2}}{6} \] \[ x = \frac{8r \pm 4r}{6} \] - This gives two possible solutions: \[ x = \frac{12r}{6} = 2r \quad \text{or} \quad x = \frac{4r}{6} = \frac{2r}{3} \] 7. **Choosing the Valid Solution**: - Since \( P \) must be between the two masses, the valid solution is: \[ x = \frac{2r}{3} \] 8. **Finding the Distance from Mass \( 4M \)**: - The distance of point \( P \) from mass \( 4M \) is: \[ x = \frac{2r}{3} \] ### Final Answer The distance of point \( P \) from the mass \( 4M \) is \( \frac{2r}{3} \).

To find the distance of point 'P' from the mass '4M' where the resultant gravitational force is zero, we can follow these steps: ### Step-by-Step Solution 1. **Understanding the Setup**: - We have two masses: \( M \) and \( 4M \) separated by a distance \( r \). - Let point \( P \) be at a distance \( x \) from the mass \( 4M \). Therefore, the distance from mass \( M \) to point \( P \) will be \( r - x \). ...
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