Showing that planets follow elliptical orbits

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Discussion Overview

The discussion revolves around the challenge of demonstrating that planets follow elliptical orbits around the sun using Newton's theory. Participants explore the relationship between Newton's laws and Kepler's laws of planetary motion, particularly focusing on the derivation of elliptical orbits.

Discussion Character

  • Technical explanation
  • Conceptual clarification
  • Debate/contested
  • Homework-related

Main Points Raised

  • One participant questions the difficulty of showing that planets follow elliptical orbits using only Newton's theory.
  • Another participant references Wikipedia and a German version of the page for detailed explanations of Kepler's laws, suggesting that these resources could aid in understanding the derivation.
  • It is proposed that Newton's laws should allow for the derivation of the elliptical orbit equation, as stated in the linked Wikipedia page.
  • Concerns are raised about the initial conditions necessary for applying Newton's laws, indicating that while orbits could be elliptical or nearly circular, these conditions are not determined by Newton's laws alone.
  • A historical context is provided regarding Johannes Kepler's work with Tycho Brahe's observations, leading to the formulation of his laws of planetary motion.
  • One participant asserts that deriving Kepler's laws from Newton's theory is standard material in introductory mechanics courses and suggests looking for textbooks or online resources for guidance.

Areas of Agreement / Disagreement

Participants express differing views on the ease of deriving elliptical orbits using Newton's laws. While some believe it is straightforward and standard in textbooks, others highlight the limitations regarding initial conditions and the historical context of Kepler's work.

Contextual Notes

The discussion touches on the dependence on initial conditions for applying Newton's laws, which remains unresolved. There is also a mention of the historical development of the laws of planetary motion, indicating a potential gap in understanding the transition from observational data to theoretical formulation.

kent davidge
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Is it difficult to show that planets follow elliptic orbits around the sun, using Newton's theory?

I have seen the equations showing it, but from General Relativity, considering the Newtonian limit.

How to arrive at them using only Newton?
 
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fresh_42 said:
Wikipedia has it
The part of the Wiki page you linked to shows the three Keplers laws, one of which, namely the first law, states that the planets follow elliptic orbits. Newtons laws should let us see why that happens.

So one should be able to arrive at the equation of the ellipse presented in the Wiki page, by means of Newtons laws.
 
kent davidge said:
Newtons laws should let us see why that happens.
I haven't checked the English version, the German does exactly this. Try the second alternative, either by reading just the formulas or translate the page. It worked reasonably well here (translated by Google chrome). A few sentences remained untouched, but it worked sufficiently.
 
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kent davidge said:
So one should be able to arrive at the equation of the ellipse presented in the Wiki page, by means of Newtons laws.

There is one thing you can't get from Newton's Laws; the initial conditions. I mean the position, and momentum at the time you start applying Newton's Laws.

With Newton's Laws, an orbit could be elliptical or (nearly) circular. Kepler predated Newton,

https://en.wikipedia.org/wiki/Kepler_orbit#Johannes_Kepler said:
n 1601, Johannes Kepler acquired the extensive, meticulous observations of the planets made by Tycho Brahe. Kepler would spend the next five years trying to fit the observations of the planet Mars to various curves. In 1609, Kepler published the first two of his three laws of planetary motion. The first law states:

"The orbit of every planet is an ellipse with the sun at a focus."
 
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kent davidge said:
Is it difficult to show that planets follow elliptic orbits around the sun, using Newton's theory?
That's standard fare in the first-semester mechanics class. It's in Kleppner and Kolenkow; and I'd expect to find it any comparable textbook. Googling for "derive Kepler's" brings up many promising-looking links.
 
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