From Kepler's law to gravitation force

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Discussion Overview

The discussion centers on the historical development of Newton's gravitational theory, particularly how he derived the gravitational force from Kepler's laws of planetary motion. Participants explore the mathematical and conceptual frameworks involved, including the role of calculus and geometric properties of conic sections.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • Some participants suggest that Newton deduced the gravitational force relationship of '1/(r^2)' from Kepler's laws, specifically the relationship (T^2)/(a^3)=const.
  • Others argue that while deriving the gravitational force for circular orbits is straightforward, working backward from Kepler's laws to establish the force relationship is less clear.
  • A participant mentions that Newton did not use calculus in his derivation of Kepler's laws, relying instead on properties of conic sections.
  • Another participant notes that Newton invented calculus for physics, implying that it may have been used in his reasoning, despite earlier claims.
  • Some participants reference Feynman's examination of Newton's proof, highlighting its reliance on non-obvious geometric properties and the existence of an "elementary" proof that does not use calculus.
  • There is a question raised about whether Newton's derivation was based on philosophical reasoning and geometry rather than calculus.

Areas of Agreement / Disagreement

Participants express differing views on the role of calculus in Newton's derivation of gravitational laws. While some acknowledge its invention by Newton, others emphasize his reliance on geometric properties without calculus. The discussion remains unresolved regarding the exact methods Newton employed.

Contextual Notes

Participants note the historical context of calculus and its development, as well as the complexities involved in deriving gravitational laws from Kepler's observations. There are references to specific mathematical relationships and proofs that may not be universally agreed upon.

Mesmerized
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Hi all! It is often said that Newton deduced from Kepler's laws the theory of gravitation. Particularly from (T^2)/(a^3)=const for differnet planets he deduced that gravitational force must look like '1/(r^2)'. I can also do that by writing F=ma and integrating it in spherical coordinates, but back when Newton lived there was nothing like integrals and differentials as I know.

Any ideas or info about how Newton came to that conclusion?
 
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Mesmerized said:
Hi all! It is often said that Newton deduced from Kepler's laws the theory of gravitation. Particularly from (T^2)/(a^3)=const for differnet planets he deduced that gravitational force must look like '1/(r^2)'. I can also do that by writing F=ma and integrating it in spherical coordinates, but back when Newton lived there was nothing like integrals and differentials as I know.

Any ideas or info about how Newton came to that conclusion?

For a circular orbit it's fairly trivial to show that the gravitational force produces a T^2/r^3 relationship. I'm not sure about working it the other way, though. In general, the procedure is as follows:
F=\frac{Gm_1 m_2}{r^2}=m_2 a
\frac{Gm_1}{r^2}=\frac{v^2}{r}
\frac{Gm_1}{r^2}=\frac{(\frac{2 \pi r}{T})^2}{r}=\frac{4 \pi ^2 r}{T^2}
\frac{Gm_1}{4\pi^2}=\frac{r^3}{T^2}

For ellipses the derivation is similar, but a bit more complicated. I imagine you could work backward from the above finding and work out that the force should be a 1/r^2 relationship with a bit of imagination.
 
Mesmerized said:
I can also do that by writing F=ma and integrating it in spherical coordinates, but back when Newton lived there was nothing like integrals and differentials as I know.
Ah, but Newton invented them for the purpose of doing physics. (For all I know, it may have been for this exact problem :wink:)
 
Mesmerized said:
but back when Newton lived there was nothing like integrals and differentials as I know.

You might want to look up who invented them. :wink:
 
LOL! thanks, just checked and was surprised that actually he was one of the founders of infinitesimal calculus, I was sure it was developed not until 19th century, thanks for pointing that! And thanks to 'Nabeshin' too for detailed formulas
 
Nabeshin, your argument works the other way too.

For a circular orbit, a = v^2/r (that's universal, nothing to do with gravitation). Plug in

v=\omega r = \frac{2\pi r}{T}

and obtain

a = \frac{4 \pi^2 r}{T^2}

On the other hand, from Kepler's law, T^2 ~ r^3, so

F = ma \propto \frac{4 \pi^2 }{r^2}

Generalizing from this is just a matter of induction (and courage!).

-----
Assaf
http://www.physicallyincorrect.com"
 
Last edited by a moderator:
Newton did not use calculus to derive Kepler's laws from his own. He relied on what we today would consider very arcane properties of conic sections in his proof. Feynman examined Newton's proof and found it took for granted these properties that were not at all obvious. So, Feynman created his own "elementary" proof, which is a bit more accessible, but still does not use calculus. This is the famous "lost lecture" on gravitation. http://en.wikipedia.org/wiki/Feynman’s_Lost_Lecture If you can find the audio for this lecture, it's worth a listen.
 
Cantab Morgan said:
Newton did not use calculus to derive Kepler's laws from his own. He relied on what we today would consider very arcane properties of conic sections in his proof. Feynman examined Newton's proof and found it took for granted these properties that were not at all obvious. So, Feynman created his own "elementary" proof, which is a bit more accessible, but still does not use calculus. This is the famous "lost lecture" on gravitation. http://en.wikipedia.org/wiki/Feynman’s_Lost_Lecture If you can find the audio for this lecture, it's worth a listen.
wow, so does that mean he derived those laws based on some philosophical thinking and geometry, or did I untderstand wrongly the phrase 'did not use calculus'?
 

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