Mr. Busse's Classes

Newton's Law of Universal Gravitation

 

Where G is the Universal Gravitational Constant, m and M are the masses of the two objects, and r is the center-to-center distance.

Lord Henry Cavendish was one of the first to calculate G. His apparatus was a torsion pendulum below.

 

Example 10

A man takes his dog for a walk on a deserted beach. Treating people and dogs as point objects for the moment, find the force of gravity between the 105 kg mand and his 11.2 kg dog when they are separated by a distance of (a) 1.00 m and (b) 10.0 m.

 

 

Example 11

The figure shows an arrangement of three particles, particle 1 having mass and particles 2 and 3 having mass and with distance a = 2.0 cm. What is the net gravitational force that acts on particle 1 due to the other particles?

 

 

Example 12

As part of a daring rescue attempt, the Millennium Falcon passes between a pair of twin asteroids, as shown. If the mass of the spaceship is and the mass of each asteroid is , find the net gravitational force exerted on the Millennium Falcon (a) when it is at location A and (b) when it is at location B. Treat the spaceship and the asteroids as if they were point objects.

 

Example 13

The figure shows an arrangement of five particles, with masses , , and with a = 2.0 cm and . What is the net gravitational force on particle 1 due to the other particles?

 

 

Absolute gravitational acceleration at the Earth's surface is:

Acceleration due to gravity for an object above the Earth's surface:

To calculate the orbital speed we set the gravitational force and the centripetal force equal and solve. This leads to the following equation for orbital speed:

 

Example 14

If you climb to the top of Mt. Everest, you will be about 5.50 mi above sea level. What is the acceleration due to gravity at this altitude?

 

 

Example 15

(a) Find the acceleration of gravity on the surface of the Moon.

(b) The lunar rover had a mass of 225 kg. What was its weight on the Earth and on the Moon? (Mass of Moon and its radius is )

 

 

Example 16

Find the mass of Mars, given that its radius is , and that the acceleration of gravity on its surface is .

 

Kepler's Laws of Orbital Motion

Kepler's First Law
The planets move in elliptical orbits with the Sun at one focus. Java

Kepler's Second Law
As a planet oribts the Sun it moves in such a way that a line drawn from the Sun to the planet sweeps out equal areas in equal time intervals. Java

Kepler's Third Law
The ratio of the average distance from the Sun cubed to the period squared is the same constant value for all planet:

Using Newton's Universal Law of Gravitation and algebra we can find a relationship for the period.

 

Example 17

The Earth revolves around the Sun once a year at an average distance of . (a) Use this information to calculate the mass of the Sun. (b) Find the period of revolution for the planet Mercury, whose average distance from the Sun is .

 

 

Example 18

Find the altitude above the Earth's surface where a satellite orbits with a period of one day
(, , )

 

Gravity Simulation