Hi Marlsda,<br /><br />I enjoyed your website, I found it quite interesting, and it was fun to go back and look at some mechanics stuff that I haven't thought about in a long while. I must confess though, that I had skepticism reading the website for the following reason: Bertrand proved in 1873 that the only central power-law forces that give closed orbits are the 1/r^2 law, and Hooke's law (force is propotional to r, used for springs). Check out "Classical Dynamics" by Jose and Saletan (page 88-92) for a proof. So it seems impossible to me that you could conclude that the planets orbit in ellipses using only the assumption that they are moving in a central force. It seems that you would either have to assume elliptical orbits, or you would have to assume a 1/r^2 law. Reading through your website, I think I agree with what you have written until chapter 11. In that chapter you show that the distance and tangential velocities can be plotted using a hotodyne. It seems to me, though, that you are implicitely assuming that the angle CGA would correspond to the orbital angle of the planet when it is at a distance GA. That assumption would not be valid in a general central force law, to get the angle as a function of distance you would have to integrate the force equations. To put it another way, while you can use the hotodyne to plot the radius and the tangential velocities in what looks like an ellipse, the orbit of a general object will not be on that ellipse. I still think the hotodyne is a neat way to visualize the orbit of a planet - but only if you specify before-hand that the force law is 1/r^2, in which case the angle CGA will work out to be the orbital angle of the planet. Also, as a point that you may have already appreciated, chapter 5 is essentially a proof that angular momentum is conserved in a central-force law (angular momentum is just radius times the tangential velocity). <div class="Discussion_UserSignature"> </div>