From Kepler's law to gravitation force

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Newton derived the theory of gravitation from Kepler's laws, particularly using the relationship (T^2)/(a^3)=const for planets, leading to the conclusion that gravitational force follows an inverse square law, '1/(r^2)'. Although modern approaches use calculus, Newton relied on geometric properties of conic sections to establish his proofs. Richard Feynman later analyzed Newton's work and noted that it depended on non-obvious properties of these conic sections, creating his own accessible proof without calculus. The discussion highlights that Newton's methods were rooted in philosophical and geometric reasoning rather than the calculus techniques developed later. This illustrates the evolution of mathematical tools in understanding gravitational forces.
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"
 
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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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