Keppler's 1st Law: Examining a Proof

In summary, Keppler's 1st Law states that the orbits of planets around the sun are elliptical, with the sun at one of the focal points. This law was proven by Keppler through his observations of the planet Mars and the mathematical calculations of his colleague Tycho Brahe. The law has significant implications for understanding the motion of celestial bodies and has been a cornerstone of modern astronomy.
  • #1
rg057
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Homework Statement


i am examining a proof of kepplers first law for my conics project and I am a bit rusty on the physics, it begins withe the following line


Homework Equations


To begin with, we will start off by applying Newton's law of motion and Newton's law of universal gravitation together to find that

m a = (-G m M/r^2) r

i think there is an extra r in this equation? if no where does it come from??

here is the link if it helps
http://members.kr.inter.net/joo/physics/curriculum/kepler/proof.html

The Attempt at a Solution

 
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  • #2
The r is in bold which indicates its a vector. So the force of gravity has a magnitude of (-G m M/r^2) along the unit vector r.
 
  • #3
thanks, altho the more I am looking at this the more i don't understand it,
can anyone explain where the negative comes from?
 
  • #4
or if anyone knows of a link to a clearer proof, that would be appreciated also
 
  • #5
The negative is there because the force of gravity is attractive.
 

FAQ: Keppler's 1st Law: Examining a Proof

1. What is Keppler's 1st Law?

Keppler's 1st Law, also known as the Law of Ellipses, states that all planets in our solar system orbit the sun in an elliptical shape, with the sun at one of the two foci of the ellipse.

2. How was Keppler's 1st Law proven?

Keppler's 1st Law was proven through observations made by German astronomer Johannes Keppler in the early 17th century. He studied the movement of planets and noticed that their orbits were not circular, but elliptical.

3. What evidence supports Keppler's 1st Law?

The evidence supporting Keppler's 1st Law includes the observations made by Keppler himself, as well as the continued study and observation of planetary orbits by modern astronomers. Additionally, the use of mathematical equations and models have also provided evidence for the elliptical shape of planetary orbits.

4. What is the significance of Keppler's 1st Law?

Keppler's 1st Law is significant because it revolutionized our understanding of planetary motion and paved the way for future discoveries in astronomy. It also helped to disprove the long-standing belief that all celestial bodies must move in perfect circles.

5. How does Keppler's 1st Law impact our understanding of the solar system?

Keppler's 1st Law has greatly impacted our understanding of the solar system by providing a foundation for the study of planetary orbits and their relationships to the sun. It has also helped to explain various phenomena, such as the changing speeds of planets in their orbits and the positioning of planets in relation to each other.

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