In this chapter, we will study the motion in two dimensions further. First, we will analyze the path that any object takes when it is thrown in the air. We will see that all falling objects follows the same path. Then, we will analyze the motion that repeats itself, such as the motion of the propeller.
1. Projectile Motion 2. Circular Motion 3. Chapter 6 Quiz
Objects launched are called projectiles. The flight of baseballs and basketballs are some examples of projectile motions. Let's analyze the projectile motion by breaking down the forces acting on the object.
Suppose a ball was thrown horizontally at the velocity of 5 m/s.
Let's think about forces acting on x-direction, or horizontal direction, only. We know that the ball was thrown at the velocity of 5 m/s. Because no other force acts on the ball in the air, we know the velocity will stay constant (because the net force is zero). Therefore, after 5 seconds, the ball is
d = vt = 5 m/s * 5s = 25 m
25 m away. After 10 seconds,
5 m/s * 10 s = 50 m
The ball is 50 m away.
QUESTION: What is the displacement of the ball in y direction after 3 seconds? m
To summarize,
QUESTION: What is the velocity of the ball in y direction when t = 2? m/s
QUESTION: What is the total velocity of the ball when t = 2? m/s
You can see that it moves at constant velocity on x direction, while accelerates on y direction. As a result, the path of the ball will follow the path of parabola.
Motion that repeat itself is called periodic motion. A projectile motion, since it doesn't repeat, is not periodic. The motion of a swinging ball is an example of circular motion. Let's analyze the circular motion.
Consider a planet around the Sun.
When there is no external force, an object will travel in a straight line (Newton's First Law of Motion). In order for an object to travel in a circle, there has to be a force that makes it travel in a circle.
When the centripetal force is too strong, the ball will accelerate toward the center of the circle. When the centripetal force is too weak, the ball will get out of the orbit. An object will maintain a circular motion only when the centripetal force is well balanced.
These formulas can be used to calculate the centripetal force:
Where:
Fc: is the centripetal force (N) m: is the mass (kg) ac: is the centripetal acceleration (m/s2) v: is the speed (m/s) r: is the radius of the circle (m) t: is the period (the length of time required for one complete rotation) (s)
Too complicated? Let's see a concrete example.
You are rotating with Earth, so you are experiencing a circular motion.
Say you have a mass of 50 kg. We know the radius of the circle (6,378,000 m = radius of Earth) and its period (24 hours = 86400 seconds). From this information, you can calculate velocity, acceleration, and centripetal force acting on you.
m/s = 1670 km/h.
To calculate acceleration, use the formula .
m/s2.
You can see that we don't accelerate much (which is obvious).
QUESTION: A ball with a speed of 10 m/s is in a circular motion. If the circle has a radius of 20 m, what would the period of the ball be? s
QUESTION: The Moon's orbit around earth is nearly circular. The orbit has a radius of about 385,000 km and a period of 27.3 days. Determine the acceleration of the moon toward Earth. m/s2
Try Chapter 6 Quiz and see how well you can do!
[Home] - [Ch1] - [Ch2] - [Ch3] - [Ch4] - [Ch5] - [Ch6] - [Ch7]