Motion and Free Fall Physics 113 Goderya Chapter(s): 5 Learning Outcomes: All.

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Presentation transcript:

Motion and Free Fall Physics 113 Goderya Chapter(s): 5 Learning Outcomes: All

Motion  Motion is one of the most necessary functions of all living things. Exactly what is motion and what law’s govern its behavior has been the most crucial question ever since man began to reason. a v

Speed  Speed: The most simple definition is called speed. S=distance/time Example A friend takes 2.0 hours to drive from his house in Stephenville to DFW airport at an average speed of 65 mi/h. How far is the airport from the friends house. Answer: 130 mi

Velocity  Velocity (v): For speed we did not put any importance to the direction of motion. The friend would travel the same distance from DFW to Stephenville. When we associate direction with a number then the speed changes its name from speed to velocity.

How is velocity different from speed? –Example : A runner makes one lap around a 200 m track in a time of 25 seconds. What is the runner’s average speed and average velocity.

What happens when velocity changes with times?  Acceleration (a): We define a quantity called acceleration (a).  acceleration ( m /s 2 ) = change in velocity (m/s) / time interval (s)  i.e. how fast is velocity changing. A very common experience is when you step on a car’s accelerator.

Galileo and the Law of Falling Body Galileo found that the distance that the objects fall from rest is proportional to the square of the time the object is in motion. This is written in the language of mathematics as d = constant x t 2 Galileo found that this constant is the same for all freely falling bodies on earth. This acceleration is called acceleration due to gravity and is given the symbol g for its use in equations.

Acceleration of Gravity Acceleration of gravity is independent of the mass (weight) of the falling object! Iron ball Wood ball

Acceleration due to Gravity (g) The value of g is different for different planets, and on the same planet its value varies from one place to another. In case of planet Earth, for the purpose of computations we approximate the value of g to 9.8 m /s 2.