Mass rotating on ellipse track

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Homework Help Overview

The problem involves a mass moving on an elliptical track under the influence of a homogeneous gravitational field. The original poster attempts to find the equilibrium position and frequency of oscillation using Lagrangian mechanics, with the generalized coordinate defined as an angle related to the ellipse's parametric equations.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning, Assumption checking

Approaches and Questions Raised

  • Participants discuss the appropriateness of the chosen generalized coordinate and its implications for the kinetic and potential energy expressions. There is an exploration of the relationship between the angle α and the polar coordinates, as well as attempts to derive the equations of motion.

Discussion Status

Some participants have offered guidance on the need to approximate energies for small oscillations and have pointed out potential misinterpretations of the coordinate system. Multiple interpretations of the coordinate definitions and their effects on the equations are being explored, but there is no explicit consensus on the correct approach yet.

Contextual Notes

Participants are navigating the complexities of using polar versus Cartesian coordinates and are questioning the assumptions underlying their formulations. There is a noted concern regarding the expected outcomes when the ellipse becomes a circle.

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Homework Statement


A body with mass ##m## can move without any friction on ellipse that ##(x/a)^2+(y/b)^2=1## describe. In ##y## direction homogeneous gravity field ##g## is present. For generalized coordinate we take angle ##\alpha ## defined with ##x=acos\alpha ##, ##y=bsin\alpha ##. Find equilibrium position and frequency of oscillation around that position.

Homework Equations


The Attempt at a Solution



##L=T-V##

##T=\frac{1}{2}m(\dot{r}^2+r^2\dot{\alpha }^2)## and ##V=mgsin\alpha ##.

##L=\frac{1}{2}m(\dot{r}^2+r^2\dot{\alpha }^2)-mgsin\alpha ##

##\frac{\partial L}{\partial \alpha }-\frac{\mathrm{d} }{\mathrm{d} t}\frac{\partial L}{\partial \dot{\alpha }}=0=-mgbcos\alpha -2mr\dot{r}\dot{\alpha }-mr^2\ddot{\alpha }=0##

So finally

##\ddot{\alpha }+\frac{2\dot{r}}{r}\dot{\alpha }+\frac{gb}{r^2}cos\alpha =0##.

For equilibrium position:

##cos\alpha =0## so ##\alpha =-\frac{\pi}{2}##

Now for frequency, I am guessing I can write:

##\ddot{\alpha }+\frac{2\dot{r}}{r}\dot{\alpha }+\frac{gb}{r^2}\alpha =0##

But this will be like horrible to calculate, since ##r=\sqrt{a^2cos^2\alpha +b^2sin^2\alpha }##...

Hmmm, is that ok? :/
 
Last edited:
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Your generalized coordinate is not the polar angle, don't mix them.

At some point you'll have to approximate the kinetic and potential energy for small oscillations, otherwise you won't find a meaningful solution.
 
Note that the parameter t (called the eccentric anomaly in astronomy) is not the angle of (X(t),Y(t)) with the X-axis.

You can use the more general form described above that (and simplify it), but then you need a different variable and you don't use the one the problem statement suggested.
 
hmmm...

##\vec{r}=(acos\alpha ,bsin\alpha )## and ##r^2=a^2cos^2\alpha +b^2sin^2\alpha ##

##\dot{\vec{r}}=\dot{\alpha }(-asin\alpha ,bcos\alpha )## and ##\dot{r}^2=\dot{\alpha }^2(a^2sin^2\alpha +b^2cos^2\alpha )##.

Than ##L=T-V=\frac{1}{2}m(\dot{r}^2+r^2\dot{\alpha }^2)-mgbsin\alpha ##

##L=\frac{1}{2}m(\dot{\alpha }^2(a^2sin^2\alpha +b^2cos^2\alpha )+\dot{\alpha }^2(a^2cos^2\alpha +b^2sin^2\alpha ))-mgbsin\alpha ##

which leaves me with ##L=\frac{1}{2}m\dot{\alpha }^2(a^2+b^2)-mgbsin\alpha ##

Now ##\frac{\mathrm{d} }{\mathrm{d} t}\frac{\partial L}{\partial \dot{\alpha }}-\frac{\partial L}{\partial \alpha }=m\ddot{\alpha }(a^2+b^2)+mgcos\alpha=0##

and finally ##\ddot{\alpha }+\frac{gb}{a^2+b^2}cos\alpha=0##.

Which leaves me with equilibrium position at ##\pi/2## and therefore frequency ## \omega ^2=\frac{gb}{a^2+b^2}##

However, this has to be wrong (don't ask me why), but if ##a=b##, than the track would be a simple circle and I would expect frequency something like ##\omega ^2=\frac{g}{R}##... Hmmm?
 
One more question, I would expect that ##T## is independent of cartesian or polar coordinates, but obviously this is not the case:

##T=\frac{1}{2}m(\dot{x}^2+\dot{y}^2)=\frac{1}{2}m\dot{\alpha }^2(a^2sin^2\alpha + b^2cos^2\alpha )## and

##T=\frac{1}{2}m(\dot{r}^2+r^2\dot{\alpha }^2)=\frac{1}{2}m\dot{\alpha }^2(a^2+b^2)##.How is that so?
 
Your second equation is wrong because, as explained, α is NOT the polar coordinate.
 
Last edited:
Aaaaaaaaaaaaaaaaaaaaaaaaa,

Now I can see what the problem is! Aha! HA! Ok! I can't believe it took me so long.

Well than let's forget about polar coordinates and do everything in cartesian.

This brings me to ##\omega ^2=\frac{gb}{a^2}##
 

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