Predicting orbits and masses of as-yet-unknown bodies

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The discussion explores the relationship between Hamiltonian and Lagrangian dynamics in predicting the orbits and masses of undiscovered celestial bodies based on the orbits of known ones. It highlights that while Hamiltonian mechanics is often considered, there are instances where Lagrangian mechanics may be more beneficial for solving standard problems. The conversation references the historical context of Neptune and Pluto's discoveries, emphasizing the use of perturbation methods and variational techniques in these predictions. Participants also discuss the application of variational methods to find orbits with constraints beyond simple points. Overall, the thread delves into the complexities of celestial mechanics and the methodologies used in astronomical predictions.
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I read an article on Phys.org (The Strange Case of the Missing Dwarf), and as I'm in the middle of reading and studying Hamiltonian Dynamics, the article made me wonder how the unexplained orbits of existing bodies are used to determine the orbits and masses of as-yet-undiscovered bodies. It sounds suspiciously like Hamiltonian Dynamics. Am I right in thinking so?
 
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Has one done Lagrangian mechanics before Hamiltonian mechanics?

Here is an interesting point: there is rarely any benefit from using a Hamiltonian instead of a Lagrangian to solve a standard mechanics problem.
http://www.people.fas.harvard.edu/~djmorin/chap15.pdf

I find examples of both Lagrangian and Hamiltonian dynamics with respect to planetary systems or binary star systems to globular clusters.
 
Thanks for the reply, Astronuc. When I said Hamiltonian Dynamics, I really meant Hamilton's Principle and Lagrangian Dynamics/Mechanics. I'm currently reading through chapter 7 (Hamilton's Principle - Lagrangian and Hamiltonian Dynamics) of Marion & Thornton's "Classical Dynamics of Particles and Systems, 5th Ed." I've also put a dent in Robert Weinstock's "Calculus of Variations: with Applications to Physics and Engineering."

In Weinstock's text, I've already read about the use of Variational methods to find curves that begin or end at points, but end or begin on curves, respectively. It was this indication that Variational methods can be used with more constraints than just points that got me wondering if similar methods can be used to predict orbits (varied functions) of as-yet-undiscovered bodies based on unexplained motions in already-known bodies.
 
Neptune and Pluto were predicted that way, with a nice precision for Neptune and a bit more messy search for Pluto.
 
mfb, I read that Neptune was discovered through the application of perturbation methods. Does this mean a combination of perturbation and variational methods, or did variational methods not enter into the discovery?
 
The prediction is over 150 years old - all those concepts were quite new back then (Hamilton was 41 at the time Neptune was discovered), I don't know how exactly they did the calculations. It looks like the references here have more details.
 
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I am looking at pressure in liquids and I am testing my idea. The vertical tube is 100m, the contraption is filled with water. The vertical tube is very thin(maybe 1mm^2 cross section). The area of the base is ~100m^2. Will he top half be launched in the air if suddenly it cracked?- assuming its light enough. I want to test my idea that if I had a thin long ruber tube that I lifted up, then the pressure at "red lines" will be high and that the $force = pressure * area$ would be massive...
I feel it should be solvable we just need to find a perfect pattern, and there will be a general pattern since the forces acting are based on a single function, so..... you can't actually say it is unsolvable right? Cause imaging 3 bodies actually existed somwhere in this universe then nature isn't gonna wait till we predict it! And yea I have checked in many places that tiny changes cause large changes so it becomes chaos........ but still I just can't accept that it is impossible to solve...
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