Geocentric v Heliocentric Models
Famous Astronomers
Eccentricity
Newton's Universal Law of Gravitation
Kepler's Laws of Planetary Motion
100

What does geocentric mean?

Earth in the center

100

Who invented the first telescope?

Galileo

100

An eccentricity of 0 would have what shape?

Perfect circle

100

What is the gravitational constant?

6.67x10-11

100

How many laws of Planetary Motion are there?

Three

200

Who created the original Geocentric Model?

Eudoxus

200

What was the initial reaction to Copernicus's Heliocentric Model?

Rejected by the church and people

200

An eccentricity of 1 would have what shape?

Flat oval/Flat ellipse
200

What unit is Force measured in?

Newtons (N)

200

What is the 1st Law of Planetary Motion?

All planets orbit in ellipses

300

What did Ptolemy change in his Geocentric Model?

Orbit shape: epicycles

300

Why did Ptolemy make his orbits epicycles?

To explain what we know as retrograde

300

Which orbit is less elliptical?
A- 0.6
B- 0.3

B - 0.3

300

Solve for force:
m1 = 300 kg

m2 = 4000 kg

r= 12900 m

4.8 x 10-13 N

300

What is Kepler's 2nd Law of Planetary Motion?

Objects will change speed to cover equal area in equal time

400

How is Kepler's Heliocentric Model different from Copernicus' Heliocentric Model?

Orbits are ellipses

400

What was the evidence that Galileo found with his telescope that helped people believe in Copernicus's model?

Venus has phases, Jupiter has moon

400

Draw an orbit that has an eccentricity of 0.7

Answer may vary

400

Solve for force:

m1= 4.3 x 1012 kg

m2= 4700 kg

r= 3.5 x 108 m

1.1 x 10-11 N

400
Order these objects from shortest to longest orbit: Jupiter, Earth, Venus, Neptune, Mars
Venus, Earth, Mars, Jupiter, Neptune
500

How long was the original Geocentric Model accepted and used?

1500 years

500

Where was Copernicus born? (country)

Poland

500

Order these from most to least elliptical: 0.07, 0.7, 0.2, 0.05

0.7, 0.2, 0.07, 0.05

500

Solve for force:

m1 = 2.9 x 1013 kg

m2= 8.3 x 107 kg

r = 6.7 x 107 m

3.6 x 10-5 N

500

What is Kepler's 3rd Law of Planetary Motion?

The further the object the longer its orbit, the closer the object the shorter the orbit

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