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# Kepler's 3rd Law

Extracts from this document...

Introduction

Confirming Kepler’s 3rd Law Lab                Adnan Masood

7/28/2009

Introduction:

Johannes Kepler was a German astronomer who is best known for his three laws on planetary motion. He lived from 1571-1630, and his works all took place during the scientific revolution (Johannes Kepler).

He was most famous for coming up with his three laws of planetary motion. His first law states that all planets move in an elliptical orbit with two foci, one of those foci being a star. His second law states that if one was to connect a line from a star to a planet, at equal times,

Middle

1.94E+20

Venus

0.38

1.26E+24

Earth

1.00

3.38E+24

Mars

3.53

1.19E+25

Jupiter

141.61

4.71E+26

Saturn

870.25

2.92E+27

Uranus

7056.00

2.36E+28

Neptune

27225.00

9.11E+28

Sample Calculations (Mercury):

Graph 2-Transformiong

Conclusion

and , which verifies that Kepler’s 3rd law is indeed true.

Works Cited

"Johannes Kepler." Wikipedia, the free encyclopedia. Web. 28 July 2009.

<http://en.wikipedia.org/wiki/Johannes_Kepler>.

"Kepler's Laws." Test Page for Apache Installation. Web. 28 July 2009.

<http://hyperphysics.phy-astr.gsu.edu/HBASE/Kepler.html>.

"Lesson 34: Kepler's Three Laws of Planetary Motion." Mr. Clintberg's Studyphysics!

Web. 29 July 2009.

<http://www.studyphysics.ca/newnotes/20/unit02_circulargravitation/chp08_s

pace/lesson34.htm>.

This student written piece of work is one of many that can be found in our International Baccalaureate Physics section.

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