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Whathat will be the acceleration due to gravity on a planet whose mass is 4 times that of earth and identical in size ?

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To find the acceleration due to gravity on a planet whose mass is 4 times that of Earth and has the same radius as Earth, we can follow these steps: ### Step 1: Understand the formula for acceleration due to gravity 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 universal gravitational constant, - \( M \) is the mass of the planet, - \( R \) is the radius of the planet. ### Step 2: Define the parameters for Earth and the new planet Let: - \( M_e \) be the mass of Earth, - \( R_e \) be the radius of Earth. For the new planet: - The mass \( M_p = 4 \cdot M_e \) (since the mass of the planet is 4 times that of Earth), - The radius \( R_p = R_e \) (since the planet is identical in size to Earth). ### Step 3: Substitute the values into the formula for the new planet Using the formula for acceleration due to gravity for the new planet: \[ g_p = \frac{G \cdot M_p}{R_p^2} \] Substituting the values we defined: \[ g_p = \frac{G \cdot (4 \cdot M_e)}{(R_e)^2} \] ### Step 4: Factor out the constants We can factor out the constants: \[ g_p = 4 \cdot \frac{G \cdot M_e}{R_e^2} \] Notice that \( \frac{G \cdot M_e}{R_e^2} \) is the acceleration due to gravity on Earth, denoted as \( g_e \): \[ g_e = \frac{G \cdot M_e}{R_e^2} \] ### Step 5: Relate the acceleration due to gravity on the new planet to that on Earth Thus, we can express \( g_p \) in terms of \( g_e \): \[ g_p = 4 \cdot g_e \] ### Final Answer The acceleration due to gravity on the planet is \( 4g_e \), where \( g_e \) is the acceleration due to gravity on Earth.

To find the acceleration due to gravity on a planet whose mass is 4 times that of Earth and has the same radius as Earth, we can follow these steps: ### Step 1: Understand the formula for acceleration due to gravity 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: ...
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