Universal Laws of Motion “ If I have seen farther than others, it is because I have stood on the shoulders of giants.” Sir Isaac Newton (1642 – 1727) Physicist.

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Presentation transcript:

Universal Laws of Motion “ If I have seen farther than others, it is because I have stood on the shoulders of giants.” Sir Isaac Newton (1642 – 1727) Physicist

Describing Motion: Examples from Daily Life Distinguish between speed, velocity, and acceleration. What is the acceleration of gravity? How does the acceleration of gravity depend on the mass of a falling object? How do you know when a net force is acting on an object? Have you ever been weightless? Have you ever been massless? Our goals for learning:

Objects in Motion speed – rate at which an object moves, i.e. the distance traveled per unit time [m/s; mi/hr] velocity – an object’s speed in a certain direction, e.g. “10 m/s moving east” acceleration – a change in an object’s velocity, i.e. a change in either speed or direction is an acceleration [m/s 2 ]

The Acceleration of Gravity As objects fall, they accelerate. The acceleration due to Earth’s gravity is 9.8 m/s each second, or g = 9.8 m/s 2. The higher you drop the ball, the greater its velocity will be at impact. © 2004 Pearson Education Inc., publishing as Addison-Wesley

The Acceleration of Gravity (g) Galileo demonstrated that g is the same for all objects, regardless of their mass! This was confirmed by the Apollo astronauts on the Moon, where there is no air resistance. © 2004 Pearson Education Inc., publishing as Addison-Wesley

Forces Forces change the motion of objects. momentum – the (mass x velocity) of an object force – anything that can cause a change in an object’s momentum As long as the object’s mass does not change, the force causes a change in velocity, or an…

Is Mass the Same Thing as Weight? mass – the amount of matter in an object weight – a measurement of the force which acts upon an object When in “free-fall,” you are weightless!!

Free Fall

Recap Distinguish between speed, velocity, and acceleration. Speed is the rate at which an object is moving. Velocity is speed in a certain direction. Acceleration is a change in velocity, meaning a change in either speed or direction What is the acceleration of gravity? The acceleration of an object falling to the ground because of gravity. On Earth’s surface, it is 9.8 m/s 2. How does the acceleration of gravity depend on the mass of a falling object? It does not. All falling objects fall with the same acceleration (on a particular planet).

Newton’s Laws of Motion What are Newton’s three laws of motion? Our goals for learning:

Sir Isaac Newton ( ) Perhaps the greatest genius of all time Invented the reflecting telescope Invented calculus Connected gravity and planetary forces Philosophiae naturalis principia mathematica © 2004 Pearson Education Inc., publishing as Addison-Wesley

Newton’s First Law of Motion A body at rest or in motion at a constant speed along a straight line remains in that state of rest or motion unless acted upon by an outside force.

Newton’s Second Law of Motion The change in a body’s velocity due to an applied force is in the same direction as the force and proportional to it, but is inversely proportional to the body’s mass. F = m a

Newton’s Third Law of Motion 3 For every applied force, a force of equal size but opposite direction arises.

**Newton’s Laws of Motion Find one activity (demonstration) to show each of Newton’s three laws. Write down what you could use for each of the laws below. (Be prepared to show and explain one of your activities in class). First Law: Second Law: Third Law:

What have we learned? How do you know when a net force is acting on an object? A net force must be acting whenever the object’s momentum is changing. Have you ever been weightless? Have you ever been massless? You are weightless every time you jump, because you are in free-fall while in the air. You have never been massless, because mass is a basic property of the matter in your body.

Angular Momentum angular momentum – the momentum involved in spinning /circling = mass x velocity x radius torque – anything that can cause a change in an object’s angular momentum (twisting force)

Conservation of Angular Momentum In the absence of a net torque, the total angular momentum of a system remains constant.

The Force of Gravity What is the universal law of gravitation? How can we determine the mass of distant objects? Our goals for learning:

Newton’s Universal Law of Gravitation Isaac Newton discovered that it is gravity which plays the vital role of determining the motion of the planets - concept of action at a distance

Newton’s Universal Law of Gravitation Between every two objects there is an attractive force, the magnitude is directly proportional to the mass of each object and inversely proportional to the square of the distance between the centers of the objects. ure=fvsr

© 2004 Pearson Education Inc., publishing as Addison-Wesley How does the acceleration of gravity depend on the mass of a falling object? It does not. All falling objects fall with the same acceleration (on a particular planet). Now see why… F = ma and on Earth acceleration due to gravity denoted “g” so F=mg or g=F/m If mass of earth is M 1 then F g =GM 2 /d 2

What have we learned? What is the universal law of gravitation? The force of gravity is directly proportional to the product of the objects’ masses and declines with the square of the distance between their centers. How can we determine the mass of distant objects? Newton’s version of Kepler’s third law allows us to calculate the mass of a distant object if it is orbited by another object, and we can measure the orbital distance and period.

What have we learned? Why are there two high tides on Earth each day? The Moon’s gravity stretches Earth along the Earth-Moon line, so that it bulges both toward and away from the Moon. Why are tides on Earth caused primarily by the Moon rather than by the Sun? Earth’s gravitational attraction to the sun is stronger than its gravitational attraction to the Moon, but tides are caused by the difference between the strength of the gravitational attraction across Earth’s diameter. This difference is greater for the gravitational force due to the Moon, because the Moon is so much closer than the Sun.