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Ch 13: Newton's Theory of Gravity
Chapter 13, Problem 13

You have been visiting a distant planet. Your measurements have determined that the planet's mass is twice that of earth but the free-fall acceleration at the surface is only one-fourth as large. (a) What is the planet's radius?

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Identify the given values: the mass of the planet (M) is twice that of Earth (2M_E), and the acceleration due to gravity (g) on the planet is one-fourth that of Earth (0.25g_E).
Recall the formula for gravitational force, which is also used to calculate the acceleration due to gravity: F = G \frac{Mm}{r^2}, where G is the gravitational constant, M is the mass of the planet, m is the mass of the object, and r is the radius of the planet.
Since the force is directly proportional to the mass and inversely proportional to the square of the radius, set up the equation for the acceleration due to gravity on the planet in terms of Earth's gravity: 0.25g_E = G \frac{2M_E}{r^2}.
Use Earth's gravity equation g_E = G \frac{M_E}{R_E^2} to eliminate G and express in terms of Earth's radius R_E: 0.25 \left( G \frac{M_E}{R_E^2} \right) = G \frac{2M_E}{r^2}.
Solve for r by isolating r on one side of the equation and simplifying, using algebraic manipulation: r = 2R_E.

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Key Concepts

Here are the essential concepts you must grasp in order to answer the question correctly.

Gravitational Force

The gravitational force between two objects is determined by their masses and the distance between their centers, as described by Newton's law of universal gravitation. The formula is F = G(m1*m2)/r^2, where G is the gravitational constant, m1 and m2 are the masses, and r is the distance. This concept is crucial for understanding how mass and distance affect gravitational acceleration.
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Free-Fall Acceleration

Free-fall acceleration is the acceleration of an object due solely to the influence of gravity, typically denoted as 'g'. On Earth, this value is approximately 9.81 m/s². For other celestial bodies, free-fall acceleration can be calculated using the formula g = G*M/r^2, where M is the mass of the planet and r is its radius, highlighting the relationship between mass, radius, and gravitational pull.
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Planetary Radius Calculation

To find the radius of a planet based on its mass and free-fall acceleration, we can rearrange the formula for gravitational acceleration. Given that g = G*M/r^2, we can solve for r, leading to r = sqrt(G*M/g). This relationship allows us to determine the radius when we know the mass of the planet and its surface gravitational acceleration.
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