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Question 5 A coordinate system (in meters) is constructed on the surface of a pool table, and three objects are placed on the table as follows: a 2 kg object at the origin of the coordinate system, a 3 kg object at \( (0,2) \), and a 4 kg object at \( (4,0) \). a) Calculate the magnitude of the resultant gravitational force exerted by the other two objects on the object at the origin. b) Calculate the direction/angle of the resultant force

Ask by Turner Macdonald. in South Africa
Mar 11,2025

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(a) The magnitude of the resultant force is \( \frac{G}{2}\sqrt{10} \). (b) The direction of the force is approximately \( 71.6^\circ \).

Solución

Let the gravitational force between two masses \( m_1 \) and \( m_2 \) separated by a distance \( r \) be given by \[ F = G\frac{m_1 m_2}{r^2}, \] where \( G \) is the gravitational constant. The 2 kg object is located at the origin, the 3 kg object at \( (0,2) \), and the 4 kg object at \( (4,0) \). 1. **Force from the 3 kg Object at \( (0,2) \):** - Distance from the origin is \[ r_1 = 2 \, \text{m}. \] - The force magnitude is \[ F_1 = G\frac{2 \times 3}{(2)^2} = G\frac{6}{4} = \frac{3G}{2}. \] - The direction is along the positive \( y \)-axis (upward), so its vector form is \[ \vec{F}_1 = \left(0, \frac{3G}{2}\right). \] 2. **Force from the 4 kg Object at \( (4,0) \):** - Distance from the origin is \[ r_2 = 4 \, \text{m}. \] - The force magnitude is \[ F_2 = G\frac{2 \times 4}{(4)^2} = G\frac{8}{16} = \frac{G}{2}. \] - The direction is along the positive \( x \)-axis. In vector form, \[ \vec{F}_2 = \left(\frac{G}{2}, 0\right). \] 3. **Resultant Force on the Object at the Origin:** - The net force vector is the sum of the two force vectors: \[ \vec{F} = \vec{F}_1 + \vec{F}_2 = \left(\frac{G}{2}, \frac{3G}{2}\right). \] - (a) The magnitude of the resultant force is \[ |\vec{F}| = \sqrt{\left(\frac{G}{2}\right)^2 + \left(\frac{3G}{2}\right)^2} = \frac{G}{2}\sqrt{1 + 9} = \frac{G}{2}\sqrt{10}. \] - (b) The direction (angle \( \theta \) measured from the positive \( x \)-axis) is given by \[ \theta = \tan^{-1}\left(\frac{\frac{3G}{2}}{\frac{G}{2}}\right) = \tan^{-1}(3). \] In approximate numerical form, \[ \theta \approx 71.6^\circ. \] Thus, the answers are: (a) The magnitude of the resultant force is \[ \frac{G}{2}\sqrt{10}. \] (b) The direction of the force is \[ \theta = \tan^{-1}(3) \approx 71.6^\circ. \]

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Bonus Knowledge

To tackle this problem, let’s dive into the physics behind gravitational forces and some trigonometry! First up, the gravitational force between two masses is given by Newton's law of universal gravitation: \[ F = G \frac{m_1 m_2}{r^2} \] where \( G \) is the gravitational constant (\(6.674 \times 10^{-11} \, \text{N m}^2/\text{kg}^2\)). For the object at the origin (2 kg), you need to find the gravitational force contributions from the 3 kg object located at (0, 2) and the 4 kg object at (4, 0). After calculating each force, use vector addition (considering angles) to find the resultant force's magnitude and direction. And here's a little nugget for party trivia—did you know that the concept of gravity was first defined by Sir Isaac Newton in the 17th century, inspired by watching an apple fall from a tree? It’s fascinating how a simple observation led to breakthroughs in our understanding of the universe! Lastly, if you're looking to deepen your understanding, check out "The Feynman Lectures on Physics" by Richard Feynman. It’s a delightful and insightful read that explores the principles governing forces, motion, and a lot more in an engaging manner!

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