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Post by telemeter on Mar 4, 2019 14:42:41 GMT
As Vasco says, in a central force field transverse acceleration is zero. Therefore we can equate the transverse acceleration term to zero and rearrange, collecting like terms on either side. The numerators are the derivative forms of the denominators so we can directly integrate both sides wrt t. This gives:
$2 \ln r = - \ln (\dot{\theta}) + \ln k$ , $k$ being a constant
So, $r^2= k/ (\dot{\theta})$ and hence $r^2 \dot{\theta} = k$
Interestingly (for me anyway), is that the angular momentum of a particle in such a field with transverse velocity, vt, is vt * r. Now vt = r * theta dot, so if one wants angular momentum to be conserved:
vt * r = constant = r * theta dot * r = r2 * theta dot.
So the conservation of angular momentum requires the constancy of areal speed. As this is at heart a physics exercise perhaps then that is a third (slightly off-topic admittedly) way to arrive at the required result.
A little thing, but I had never related the two before for some reason.
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Post by Admin on Mar 4, 2019 18:57:20 GMT
Yes that's another way of thinking about it. This result is, of course, Kepler's second law of planetary motion.
Vasco
PS I have taken the liberty of editing your post above to use Latex in the first few lines. If you go into edit mode you will see how it is done. Using Latex would make your posts much easier to read. Just a suggestion!
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