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

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

4.1 Newton's Laws

  1. 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.
  2. Newton's Second Law

    The acceleration of an object is directly proportional to the force applied to it, and inversely proportional to its mass. \[F=ma\]
  3. 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:

4.3 Free Body Diagrams

Here are examples with Free Body Diagrams.

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 \[ F_{g} = G \frac{m_{1}m_{2}}{d^{2}} \] \[ F_{g} = \left( 6.67 \times 10^{-11} \right) \frac{ \left( 5.972 \times 10^{24} \right) \left( 7.348 \times 10^{22} \right) }{\left( 384,400,000 \right)^{2}} \] \[ F_{g} = 1.98 \times 10^{20} \text{ N} \]