Chapter 13

Universal Gravitation

The Big Idea

• Everything pulls

everything else.

• There is a force that pulls all objects together. It is gravity.

What Newton Knew

Newton understood

the concept of inertia

developed earlier by Galileo.

•Without an outside force, moving objects continueto move at constant speed in a straight line.

•If an object undergoes a change in speed or direction,then a force is responsible.

Newton’s 1st LawThe Law of Inertia

• What is it?– An object in equilibrium will remain in

equilibrium unless acted on by a non zero net force.

• Equilibrium – Zero Net Force.– No Acceleration.

• Static - Object at rest.• Dynamic - Object moving

at a constant speed in a straight line.

The Apple and the Moon

• Newton saw apples falling to Earth and wondered if the moon fell towards the Earth just like the apple fell towards the Earth.

•Was he correct?•What makes things fall towards the center of the Earth?•What is different about the moon and the apple?

The Moon Falls?

• If something is moving and

no force acts on it, how does it

Keep moving?

• What is needed for circular

motion?

Newton realized that if the moon did not fall, it would move off in a straight line and leave its orbit.

His idea was that the moon must be falling around the Earth.

Cannonball being shot off a Very Tall Mountain

• If I could climb a mountain tall enough, could I shoot a cannonball so that it would never land back on Earth.

• We call this putting an object into orbit.

Nev nThought aExperiment.

vton’s

From hypothesisto theory

• Newton thought the apple, the orbiting cannonball, and the motion of the moon were all caused by a force now called gravity.

• He needed to test this hypothesis.

I need to test my hypothesis

The moon and the apple.

• Newton knew the apple fell 5m in one second.

• He wondered how far the moon fell in one second.

• The moon was 60 times away from the Earth than the apple was.

• The force of Gravity must dilute the farther away something is.

Using geometry, Newton calculated how far the circle of the moon’s orbit lies below the straight-line distance the moon otherwise would travel in one second. His value turned out to be about the 1.4-mm distance accepted today.

But he was unsure of the exact Earth moon distance, and whether or not the correct distance to use was the distance between their centers. At this time he hadn’t proved mathematically that the gravity of the spherical Earth (and moon) is the same as if all its mass were concentrated at its center.

Because of this uncertainty, and also because of criticisms he had experienced in publishing earlier findings in optics, he placed his papers in a drawer, where they remained for nearly 20 years.

During this period he laid the foundation and developed the field of geometrical optics for which he first became famous.

Newton finally returned to the moon problem at the prodding of his astronomer friend Edmund Halley (of Halley’s comet fame). It wasn’t until after Newton invented a new branch of mathematics, calculus, to prove his center-of-gravity hypothesis, that he published what is one of the greatest achievements of the humankind, the law of universal gravitation.

Law of Universal Gravitation

• The force between two objects is equal to the gravitational constant G times the product of the two masses divided by the distance squared.

inverse-square law

Measuring G

• G was first measured 150 years after Newton’s discovery of universal gravitation by an English physicist, Henry Cavendish.

How Cavendish Measured G

• 1st - Balance F and little m

• 2nd- Move Big M under little m

• 3rd- Rebalance scale by adding mass to big F.

Examples of how the force of gravity changes.

1.If both masses are doubled, what happens to the force?

2.If the masses are not changed, but the distance of separation is reduced to half the original distance, what happens to the force?

3.If the masses are not changed, but the distance of separation is reduced to one fourth the original distance, what happens to the force?

4.If both masses are doubled, and the distance of separation is doubled, show what happens to the force.