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Universal Gravitation

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Universal Gravitation. A space station revolves around the earth as a satellite, 100 km above Earth’s surface. What is the net force on an astronaut at rest inside the space station?. Equal to her weight on Earth. Zero (she is weightless). Less than her weight on Earth. - PowerPoint PPT Presentation
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Universal Gravitation
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Page 1: Universal  Gravitation

Universal

Gravitation

Page 2: Universal  Gravitation

A space station revolves around the earth as a satellite, 100 km above Earth’s surface. What is the net force on an astronaut at rest inside the

space station?

A. Equal to her weight on Earth.B. Zero (she is weightless).C. Less than her weight on Earth.D. Somewhat larger than her weight on Earth.

Page 3: Universal  Gravitation

What is Gravity?Fundamental Forces:

Strong Nuclear Force – The force that is involved in holding the nucleus of an atom together

Electromagnetic Force – The force that exists between charged particles

Weak Nuclear Force – The force involved in nuclear decay

Gravity – The force that exists between any two objects that have mass.

- Always attractive

Page 4: Universal  Gravitation

Newton’s Law of Universal GravitationIf the force of gravity is being exerted on objects on Earth, what is the origin of that force?

Newton’s realization was that the force must come from the Earth.

He further realized that this force must be what keeps the Moon in its orbit.

Page 5: Universal  Gravitation

Newton’s Law of Universal GravitationThe gravitational force on you is one-half of a Newton’s Third Law pair (the action force):

When there is such a difference in masses, the reaction force is undetectable,

The Earth exerts a downward force on you, and you exert an upward force on the Earth.

but for bodies more equal in mass it can be significant.

Page 6: Universal  Gravitation

Newton’s Law of Universal Gravitation

Therefore, the gravitational force must be proportional to both masses.

By observing planetary orbits, Newton also concluded that the gravitational force must decrease as the inverse of the square of the distance between the masses. (This is called the inverse square law)

In its final form, the law of universal gravitation reads:

Where:

Page 7: Universal  Gravitation

Inverse Square Law for universal gravitation:

As the distance decreases, the strength of Fg increases by the square of the number the distance went up by.

If d is halved (1/2) the force will be 4 times what it was.

Review of Scientific Notation.

Page 8: Universal  Gravitation

Newton’s Law of Universal Gravitation

The magnitude of the gravitational constant G can be measured in the

laboratory.This is the Cavendish experiment.

Page 9: Universal  Gravitation

Gravitational Attraction of Spherical Bodies

Gravitational force between a point mass and a sphere: the force is the same as if all the mass of the sphere were concentrated at its center.

Page 10: Universal  Gravitation

Gravitational Attraction of Spherical Bodies

The acceleration of gravity decreases slowly with altitude:

Page 11: Universal  Gravitation

Gravitational Attraction of Spherical Bodies

Once the altitude becomes comparable to the radius of the Earth, the decrease in the acceleration of gravity is much larger:

Page 12: Universal  Gravitation

Tides

Usually we can treat planets, moons, and stars as though they were point objects, but in fact they are not.

When two large objects exert gravitational forces on each other, the force on the near side is larger than the force on the far side, because the near side is closer to the other object.

This difference in gravitational force across an object due to its size is called a tidal force.

Page 13: Universal  Gravitation

TidesThis figure illustrates a general tidal force on the left, and the result of lunar tidal forces on the Earth on the right.

Gravity of moon

Moon’s pull is greatest here because it is closer. Highest tide

Second high tide (smaller then the other)

Page 14: Universal  Gravitation

Tides

Tidal forces can result in orbital locking, where the moon always has the same face towards the planet – as does Earth’s Moon.

If a moon gets too close to a large planet, the tidal forces can be strong enough to tear the moon apart. This occurs inside the Roche limit; closer to the planet we have rings, not moons.

Page 15: Universal  Gravitation

Tidal lockingTidal lockingThis is what allows only one side of the moon to face the Earth

It can even keep moons from forming!

Page 16: Universal  Gravitation

Newton’s Law of Universal Gravitation

Example 6-1: Can you attract another person gravitationally?

A 50-kg person and a 70-kg person are sitting on a bench close to each other. Estimate the magnitude of the gravitational force each exerts on the other.

Page 17: Universal  Gravitation

Newton’s Law of Universal Gravitation

Example 6-2: Spacecraft at 2rE.

What is the force of gravity acting on a 2000-kg spacecraft when it orbits two Earth radii from the Earth’s center (one earth radius is: rE = 6380 km)? The mass of the Earth is mE = 5.98 x 1024 kg.

Page 18: Universal  Gravitation

Newton’s Law of Universal Gravitation

Example 6-3: Force on the Moon.

Find the net force on the Moon (mM = 7.35 x 1022 kg) due to the gravitational attraction of both the Earth (mE = 5.98 x 1024 kg) and the Sun (mS = 1.99 x 1030 kg), assuming they are at right angles to each other.

Page 19: Universal  Gravitation

So…If gravity is always present and goes on for ever and ever, why hasn’t the Moon crashed into the Earth?

Since the Moon is not only falling toward Earth, but also moving “tangentially,” the tangential velocity keeps the Moon from crashing into Earth.

Page 20: Universal  Gravitation

Newton’s Thought Experiment

To make something orbit the Earth, all you need to do is shoot it at a tangential velocity that will make it fall along with the curve of the Earth.

As a satellite or the Moon falls towards Earth, the earth also falls (or curves) away from the satellite at the same rate!

Page 21: Universal  Gravitation

Gravity and Orbits• Centripetal acceleration

– The acceleration towards the center if something going in a circle

– ac= v2/r

• Centripetal Force–The force in circular motion that is directed towards the center – “centripetal”–This is the force that causes centripetal acceleration –Fc= mac

Page 22: Universal  Gravitation

Try This:What is the centripetal acceleration on the moon if it travels around Earth with a tangential velocity of 1023m/s and its average distance from the Earth is 384,000,000m?

What is the centripetal force on the moon?

What is the force due to gravity on the moon from the Earth?

Page 23: Universal  Gravitation

All of the planets as a system.

The deviation of a planet from its normal orbit is called a perturbation. It is caused by other planets.

Page 24: Universal  Gravitation

Some more facts about angles and planetary motion

Page 25: Universal  Gravitation

Angular Velocity

Just like how velocity is the rate at which an object covers a distance, Angular Velocity is the rate at which an angle (or an amount of degrees) is covered.

Page 26: Universal  Gravitation

Moment of Inertia and Angular Momentum

Moment of Inertia: The further mass is from it’s rotation axis, the greater the “moment of inertia”

- The greater the moment of inertia, the greater the torque required to alter the angular motion.

Inertia is_____________________?

Angular Momentum is the product of the moment of inertia and the angular velocity.

Page 27: Universal  Gravitation

Gyroscopic MotionA device used to both measure and maintain its orientation while it is spinning.

Works based on the principles of conservation of angular momentum.

Bicycles

Airplanes

Hubble space telescope

Yo Yos

Frisbees

Page 28: Universal  Gravitation

Precession

The motion of the axis of a spinning body, such as the wobble of a spinning top, when there is an external force acting on the axis.

Page 29: Universal  Gravitation

Conservation of Angular Momentum and the seasons

of Earth


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