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Weight of a body on the surfaces of two ...

Weight of a body on the surfaces of two planets is the same. If their densities are `d_1 and d_2` then the ratio of their radius

A

`d_1/d_2`

B

`d_2/d_1`

C

`d_1^2/d_2^2`

D

`d_2^2/d_1^2`

Text Solution

AI Generated Solution

The correct Answer is:
To solve the problem, we need to find the ratio of the radii of two planets given that the weight of a body on their surfaces is the same and their densities are \(d_1\) and \(d_2\). ### Step-by-Step Solution: 1. **Understanding the Weight on the Surface of the Planets**: The weight of a body on the surface of a planet is given by the formula: \[ W = mg \] where \(m\) is the mass of the body and \(g\) is the acceleration due to gravity on the surface of the planet. 2. **Acceleration Due to Gravity**: The acceleration due to gravity \(g\) on the surface of a planet can be expressed as: \[ g = \frac{GM}{R^2} \] where \(G\) is the gravitational constant, \(M\) is the mass of the planet, and \(R\) is the radius of the planet. 3. **Relating Mass and Density**: The mass \(M\) of a planet can also be expressed in terms of its density \(d\) and volume \(V\): \[ M = d \cdot V \] The volume of a spherical planet is given by: \[ V = \frac{4}{3} \pi R^3 \] Therefore, we can write: \[ M = d \cdot \frac{4}{3} \pi R^3 \] 4. **Substituting Mass in the Gravity Formula**: Substituting the expression for mass into the formula for \(g\): \[ g = \frac{G \left(d \cdot \frac{4}{3} \pi R^3\right)}{R^2} \] Simplifying this gives: \[ g = \frac{4}{3} \pi G d R \] 5. **Setting Up the Equation for Two Planets**: For two planets with densities \(d_1\) and \(d_2\) and radii \(R_1\) and \(R_2\), we have: \[ g_1 = \frac{4}{3} \pi G d_1 R_1 \quad \text{and} \quad g_2 = \frac{4}{3} \pi G d_2 R_2 \] Since the weight of the body is the same on both planets, we have \(g_1 = g_2\). 6. **Equating the Two Expressions**: Setting the two expressions for \(g\) equal to each other: \[ \frac{4}{3} \pi G d_1 R_1 = \frac{4}{3} \pi G d_2 R_2 \] The constants \(\frac{4}{3} \pi G\) cancel out, leading to: \[ d_1 R_1 = d_2 R_2 \] 7. **Finding the Ratio of the Radii**: Rearranging the equation gives: \[ \frac{R_1}{R_2} = \frac{d_2}{d_1} \] ### Final Answer: The ratio of the radii of the two planets is: \[ \frac{R_1}{R_2} = \frac{d_2}{d_1} \]
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