Verified for the 2025 AP Physics 2 exam•Citation:
The AP Physics 2 writers really want us to review forces and get a deep understanding of dynamics. So let's walk through the famous Newtonian Laws again briefly and remind ourselves of what forces are and how they work.
Sir Isaac Newton's three laws of motion, also known as Newton's laws, are fundamental principles that describe the relationship between a body and the forces acting upon it. These laws form the basis of classical mechanics, which is the study of how objects move and behave under the influence of forces.
Here are brief overviews of each of Newton's laws:
These laws are useful in predicting the motion of objects under the influence of forces, and they can be applied to a wide range of physical situations, from the motion of objects on Earth to the orbits of planets and other celestial bodies.
This law deals with two main concepts in physics: the principle of inertia and the principle of frames of reference. Newton’s First Law is sometimes known as the Law of Inertia because it explains the concept that objects have the tendency to resist a change in motion.
Example Problem #1:
A car is driving down the road at a constant speed of 50 km/h. The driver suddenly slams on the brakes, causing the car to come to a stop in 5 seconds. What is the acceleration of the car during this time?
Solution:
To solve this problem, we can use Newton's second law, which states that the acceleration of an object is directly proportional to the force applied to it and inversely proportional to its mass. We know that the car starts at a constant speed of 50 km/h and comes to a stop in 5 seconds, so it must have experienced a negative acceleration. We can set up the equation as follows: a = F/m. If we let m be the mass of the car and F be the force applied by the brakes, we can solve for a by rearranging the equation: a = (-50 km/h)/5 s = -10 km/h/s. This means that the car's acceleration was -10 km/h/s, or a deceleration of 10 km/h/s.
Example Problem #2:
A ball is thrown straight up into the air with an initial velocity of 20 m/s. How high does the ball go before it reaches its maximum height and begins to fall back down?
Solution:
To solve this problem, we can use Newton's first law, which states that an object will remain at rest or in motion at a constant velocity unless acted upon by an external force. We know that the ball is initially thrown upward with an initial velocity of 20 m/s, and that it reaches its maximum height before starting to fall back down. Since the ball is not being acted upon by any external forces while it is in the air, it must have a constant velocity of 0 m/s while it is at its maximum height. We can use the equation v^2 = u^2 + 2as to solve for the height of the ball, where v is the final velocity (0 m/s), u is the initial velocity (20 m/s), and a is the acceleration due to gravity (-9.8 m/s^2). Plugging these values into the equation, we get: 0 = 400 + (-19.6)s. Solving for s, we find that s = 20.4 m, which is the height of the ball.
After Newton had done his groundbreaking work regarding gravity, charges and electricity were the next big thing. Scientific celebrities like Daniel Bernoulli and Benjamin Franklin worked on finding out more about electric charges and fields as well. Franklin shared his findings with his teacher, John Priestley.
Priestley agreed with the commonly held belief among scientists that the force between charges followed an inverse square pattern just like Gravity. This means that if the distance between charges was decreased by a factor of 2, the force between them would increase by a factor of 4. Priestley's entire theory did have some flaws. Many scientists continued to solve this entangled puzzle about the electric force. Charles Augustin de Coulomb would be the man who would publish a definitive study that electrical force between two point-charges varied inversely with the square of their separation.
The study of electric forces has a long and fascinating history that dates back to ancient civilizations. Here is a brief summary of the key events and milestones in the development of our understanding of electric forces: