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If a planet gets inflated, keeping its d...

If a planet gets inflated, keeping its density constant, then g will increase.

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To solve the problem, we need to analyze how the acceleration due to gravity (g) changes when a planet is inflated while keeping its density constant. We will use the formula for gravitational acceleration and the relationship between mass, density, and volume. ### Step-by-Step Solution: 1. **Understanding the Formula for Gravitational Acceleration**: The acceleration due to gravity (g) at the surface of a planet is given by the formula: \[ g = \frac{G \cdot M}{R^2} \] where: - \( G \) is the gravitational constant, - \( M \) is the mass of the planet, - \( R \) is the radius of the planet. 2. **Relating Mass and Density**: The mass \( M \) of the planet can be expressed in terms of its density \( \rho \) and volume \( V \): \[ M = \rho \cdot V \] For a spherical planet, the volume \( V \) is given by: \[ V = \frac{4}{3} \pi R^3 \] Therefore, we can substitute this into the mass equation: \[ M = \rho \cdot \frac{4}{3} \pi R^3 \] 3. **Substituting Mass into the Gravitational Formula**: Now, substituting the expression for mass \( M \) into the formula for \( g \): \[ g = \frac{G \cdot \left( \rho \cdot \frac{4}{3} \pi R^3 \right)}{R^2} \] Simplifying this gives: \[ g = \frac{G \cdot \rho \cdot \frac{4}{3} \pi R^3}{R^2} = \frac{4}{3} \pi G \rho R \] 4. **Analyzing the Effect of Increasing Radius**: From the derived formula, we see that \( g \) is directly proportional to the radius \( R \) of the planet when density \( \rho \) is constant: \[ g \propto R \] Therefore, if the radius \( R \) increases (as the planet gets inflated), the acceleration due to gravity \( g \) will also increase. 5. **Conclusion**: Since we have established that increasing the radius of the planet while keeping the density constant results in an increase in \( g \), the statement "If a planet gets inflated, keeping its density constant, then g will increase" is **true**. ### Final Answer: The statement is **true**. ---
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