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

What is the net gravitational force on the 20.0 kg mass in FIGURE P13.36? Give your answer using unit vectors.

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1
Identify the masses involved and their respective positions. In this problem, you need to consider the 20.0 kg mass and any other masses that exert a gravitational force on it.
Calculate the distance vectors between the 20.0 kg mass and each of the other masses. These vectors are crucial as they determine the direction of the gravitational force exerted by each mass.
Use Newton's Law of Universal Gravitation to calculate the gravitational force exerted by each mass on the 20.0 kg mass. The formula is $F = G \frac{m_1 m_2}{r^2}$, where $G$ is the gravitational constant, $m_1$ and $m_2$ are the masses, and $r$ is the distance between the centers of the two masses.
Express each gravitational force as a vector in unit vector notation. This involves dividing the force vector by its magnitude and then multiplying by the respective unit vectors in the x, y, and z directions as applicable.
Sum up all the gravitational force vectors to find the net gravitational force on the 20.0 kg mass. This is done by adding together the corresponding components of all the force vectors.

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Key Concepts

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

Gravitational Force

Gravitational force is the attractive force between two masses, described by Newton's law of universal gravitation. It is directly proportional to the product of the masses and inversely proportional to the square of the distance between their centers. The formula is F = G(m1*m2)/r^2, where G is the gravitational constant. This force acts downward towards the center of the Earth or any other massive body.
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Unit Vectors

Unit vectors are vectors with a magnitude of one, used to indicate direction. In physics, they are often represented as i, j, and k for the x, y, and z axes, respectively. When calculating forces, expressing them in terms of unit vectors allows for easier addition and subtraction of vector quantities, as well as clearer representation of direction in a coordinate system.
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Net Force

The net force is the vector sum of all individual forces acting on an object. It determines the object's acceleration according to Newton's second law, F_net = m*a. In the context of gravitational forces, calculating the net force involves summing the gravitational forces from all other masses acting on the object in question, taking into account their directions and magnitudes.
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Related Practice
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Hint: The minimum speed is not the escape speed. You need to analyze a three-body system.

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