Orbital Motion © Simon Porter 2007. How far could you kick a dog? From a table, medium kick.

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Orbital Motion© Simon Porter 2007

Even bigger cannon?

Even bigger cannon

GravityGravity

Gravity

VERY big cannon?

VERY big cannon

Gravity

Humungous cannon?

Dog in orbit!

The dog is now in orbit! (assuming no air resistance of course)

Dog in orbit!

The dog is falling towards the earth, but never gets there!

Dogs in orbit!

The force that keeps an object moving in a circle is called the centripetal force (here provided by gravity)

Gravity

Uniform Circular Motion

Remember we have already looked at circular motion

Centripetal force = mv2/r

velocity

Centripetal acceleration = v2/r

© Simon Porter 2007

Uniform Circular Motion

For orbital motion, the centripetal force is provided by gravity

Earth’s gravitational attraction on moon

© Simon Porter 2007

Uniform Circular Motion

centripetal force = force of gravity

Mmv2/r = GMeMm/r2

v2 = GMe/r

Earth’s gravitational attraction on moon

© Simon Porter 2007

Period of orbit

v2 = GMe/r

Distance travelled in one orbit = 2πr

Speed = distance/time = 2πr/T

Earth’s gravitational attraction on moon

© Simon Porter 2007

(T = period of orbit)

Period of orbit

v2 = GMe/r(2πr/T)2 = GM/rT2 = 4π2r3/GM

T2 α r3

This is known as Kepler’s third law of planetary motion.

© Simon Porter 2007

Energy of a satellite

A satellite has kinetic energy and gravitational potential energy.

Total energy = ½mv2 - GMm/r

v2 = GM/r so Ek = GMm/2r

Total energy = GMm/2r – GMm/r = -GMm/2r

Total energy = -½mv2

© Simon Porter 2007

from slide 4

Energy of a satellite

Total energy of satellite = -GMm/2r

Kinetic energy = GMm/2r

Potential energy = - GMm/r

© Simon Porter 2007

Energy of a satellite© Simon Porter 2007

Ep

Ek

ET

energy

distance

Weightlessness

Consider an astronaut in a space ship orbiting the earth

© Simon Porter 2007

Weightlessness

Remember both the ship and astronaut are falling towards the earth (centripetal acceleration)

© Simon Porter 2007

v

mv2/r

acceleration = v2/r

Weightlessness

Because they are both falling together, the astronaut feels no reaction force from the floor of the space craft so she feels “weightless” (you get a small feeling of this as a lift (elevator) starts to descend).

© Simon Porter 2007

Weightlessness

There is a mathematical way to look at this.

© Simon Porter 2007

Weightlessness

The forces on the astronaut are gravity from the earth (GMm/r2) and the normal reaction force (N) of the floor of the spacecraft.

The net force must be equal to mv2/r if he is in orbit.

GMm/r2 – N = mv2/r

© Simon Porter 2007

Weightlessness

GMm/r2 – N = mv2/r

N = GMm/r2 – mv2/r

N = (m/r)(GM/r – v2)

since v2 = GM/r, N = zero

© Simon Porter 2007

More questions!© Simon Porter 2007

I hate physics.

Page 152 Questions 1, 3, 4, 15, 24.

Page 153 Q7, 13

Pages 307 Questions 2, 4, 5, 6, 11, 12.

You can have some time to finish them in this lesson, and then you can finish the rest for homework, due in Wednesday 30th September

TEST on 6th October