4. Newton's Laws
Overview
Newton's Laws are fundamental concepts in classical physics. They help us predict the motion and behavior of everyday objects.Slides
Skills and Understanding
- Apply Newton's Laws to analyze physical behaviors and interactions of objects.
- Draw Free Body Diagrams (FBDs) and analyze forces in 2D.
- Apply Newton's 2nd Law, \(F=ma\), to solve for force, mass, and acceleration.
- Identify when an object is in equilibrium, and solve equilibrium equations.
Equations
\[ \begin{array}{cc} F = ma \quad \quad \quad \quad F_{f} = \mu F_{N} \quad \quad \quad \quad F_{g} = G \frac{m_{1} m_{2}}{d^{2}} \\ \end{array} \]Vocabulary
- Acceleration is the rate at which velocity changes.
- Equilibrium describes when the forces on an object add to zero, resulting in no acceleration.
- Force is an influence on mass that can change its velocity. \(F=ma\).
- Friction is a force that opposes sliding motion due to the interaction of two surfaces. It acts parallel to the surfaces in contact.
- Inertia is the tendency of an object to continue in its state of motion. An object at rest stays at rest unless acted upon by a force. An object in motion maintains that motion unless acted upon by a force.
- Mass is a measure of the amount of matter in an object, measured in kilograms (kg).
- Weight is a measure of the force exerted on an object due to gravity.
4.1 Newton's Laws
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Newton's First Law (Inertia)
An object at rest will stay at rest, and an object in motion will stay in motion, unless acted upon by a force. -
Newton's Second Law
The acceleration of an object is directly proportional to the force applied to it, and inversely proportional to its mass. \[F=ma\] -
Newton's Third Law
For every action, there is an equal and opposite reaction. This means that if an object A exerts a force on object B, then object B exerts an equal force in the opposition direction on object A.
4.2 Forces
There are several types of forces we will consider, including:
- \(F_{g}\) Force of Gravity - The weight of a mass.
- \(F_{a}\) Applied Force - A force that is applied to a mass, for example from pushing or pulling on it.
- \(F_{f}\) Frictional Force - A force that results from the friction between two surfaces.
- \(F_{N}\) Normal Force - The force that results from solid objects interacting. \(F_{n}\) is always perpendicular to the surface.
- \(F_{T}\) Tension Force - A force applied from a non-rigitd object like a rope, string, or cable.
4.3 Free Body Diagrams
Here are examples with Free Body Diagrams.
- A 3.2 kg bag of toys is sitting on the ground.

- A 0.325 kg book is sitting on a shelf.

- A 41.5 kg crate is sitting on the ground and someone is pushing with 5 N of force to the right.
- A 41.5 kg crate is sitting on the ground and someone is pushing with 5 N of force to the right but the crate is being held in place by friction.

- A sled with mass 35 kg is being pulled by a rope. The rope has a tension of 18 N and is pulled at an angle \(22^{\circ}\) above the horizontal.

- A 2 kg block is on a frictionless ramp of incline \(14^{\circ}\).

4.4 Analyzing Forces
4.5 Gravity
The force of gravity \(F_{g}\) between two masses is given by \[ F_{g} = G \frac{m_{1}m_{2}}{d^{2}} \] where \(m_{1}\) and \(m_{2}\) are the two masses, \(d\) is the distance between the masses, and \(G\) is Newton's gravitational constant, \[G \approx 6.67 \times 10^{-11} \text{ Nm^2/kg^2} \]
Find the force of gravity between the Earth and Moon.
↓
The masses of Earth and the Moon are:
\(M_{earth} = 5.972 \times 10^{24} \) kg
\(M_{moon} = 7.348 \times 10^{22} \) kg
and the distance between the two is \(384,400\) km. Plugging this into our formula for \(F_{g}\), we have \[ F_{g} = G \frac{m_{1}m_{2}}{d^{2}} \] \[ F_{g} = \left( 6.67 \times 10^{-11} \right) \frac{ \left( 5.972 \times 10^{24} \right) \left( 7.348 \times 10^{22} \right) }{\left( 384,400,000 \right)^{2}} \] \[ F_{g} = 1.98 \times 10^{20} \text{ N} \]
\(M_{earth} = 5.972 \times 10^{24} \) kg
\(M_{moon} = 7.348 \times 10^{22} \) kg
and the distance between the two is \(384,400\) km. Plugging this into our formula for \(F_{g}\), we have \[ F_{g} = G \frac{m_{1}m_{2}}{d^{2}} \] \[ F_{g} = \left( 6.67 \times 10^{-11} \right) \frac{ \left( 5.972 \times 10^{24} \right) \left( 7.348 \times 10^{22} \right) }{\left( 384,400,000 \right)^{2}} \] \[ F_{g} = 1.98 \times 10^{20} \text{ N} \]
1. Simple Motion
2. Accelerated Motion
3. Projectile Motion
4. Newton's Laws
5. Momentum
6. Energy
7. Heat
8. Electrostatics
9. Circuits
10. Magnetism
11. Waves