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A planet has a mass of eight time the ma...

A planet has a mass of eight time the mass of earth and denisity is also equal to eight times a the average density of the earth. If g be the acceleration due to earth's gravity on its surface, then acceleration due to gravity on planet's surface will be

A

2g

B

4g

C

8g

D

16g

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The correct Answer is:
To find the acceleration due to gravity on the surface of a planet that has a mass and density both eight times that of Earth, we can follow these steps: ### Step 1: Define Given Values Let: - \( M_e \) = Mass of Earth - \( D_e \) = Density of Earth - \( M_p = 8M_e \) = Mass of the planet - \( D_p = 8D_e \) = Density of the planet ### Step 2: Relate Density to Mass and Volume The density \( D \) is defined as: \[ D = \frac{M}{V} \] For a spherical object, the volume \( V \) is given by: \[ V = \frac{4}{3} \pi r^3 \] Thus, we can express the densities as: \[ D_p = \frac{M_p}{V_p} \quad \text{and} \quad D_e = \frac{M_e}{V_e} \] ### Step 3: Write the Volume in Terms of Radius For the planet and Earth, we can write: \[ D_p = \frac{M_p}{\frac{4}{3} \pi r_p^3} \quad \text{and} \quad D_e = \frac{M_e}{\frac{4}{3} \pi r_e^3} \] ### Step 4: Substitute Known Values Substituting the values for \( M_p \) and \( D_p \): \[ 8D_e = \frac{8M_e}{\frac{4}{3} \pi r_p^3} \] And for Earth: \[ D_e = \frac{M_e}{\frac{4}{3} \pi r_e^3} \] ### Step 5: Set Up the Equation Equating the two expressions for density: \[ \frac{8M_e}{\frac{4}{3} \pi r_p^3} = 8 \cdot \frac{M_e}{\frac{4}{3} \pi r_e^3} \] ### Step 6: Simplify the Equation Cancel out common terms: \[ \frac{8M_e}{r_p^3} = \frac{8M_e}{r_e^3} \] This implies: \[ r_p^3 = r_e^3 \implies r_p = r_e \] ### Step 7: Use the Formula for Acceleration due to Gravity The formula for acceleration due to gravity \( g \) is given by: \[ g = \frac{GM}{r^2} \] For Earth: \[ g_e = \frac{GM_e}{r_e^2} \] For the planet: \[ g_p = \frac{GM_p}{r_p^2} \] ### Step 8: Substitute Known Values Substituting \( M_p = 8M_e \) and \( r_p = r_e \): \[ g_p = \frac{G(8M_e)}{(r_e)^2} = 8 \cdot \frac{GM_e}{r_e^2} = 8g_e \] ### Conclusion Thus, the acceleration due to gravity on the surface of the planet is: \[ g_p = 8g \]
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