Eccentricity of Elliptical Orbit

In summary, the eccentricity of an elliptical orbit is proportional to the square root of the ratio of the maximum angular velocity to the minimum angular velocity of the particle in its orbit.
  • #1
cscott
782
1
A particle moves in an elliptical orbit in an inverse-square law central force field. If the
ratio of the maximum angular velocity to the minimum angular velocity of the particle
in its orbit is n, then show that the eccentricity of the orbit is

[tex]
\epsilon = \frac{\sqrt{n}-1}{\sqrt{n}+1}[/tex]

Not sure where to go with this. I tried finding total energy and angular momentum in terms of max/min angular velocity and radius but can't get anywhere
 
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  • #2
At what points in the orbit are the maximal and minimum angular (or, for that matter, linear) velocities attained? At what distances from the "massive body" (what the particle is orbiting around -- assumed to be "infinitely massive" here) is the particle at those moments? (You don't need values here -- just identify those places on the orbit and label them appropriately.)

Now for the critical part. Angular momentum is conserved. What angle does the velocity makes to the radial vector from the massive body at those moments (and no others)? Express the angular momentum in terms of radial distance and velocities for those two moments and set them equal. What is the relationship between these two angular (or linear) velocities and the two distances from the massive body?

Having found how the ratio of angular velocities, called n here, relates to those distances, how do those distances fit into the expression for the eccentricity of an ellipse?

That would be the full derivation of the answer. If you already know how n relates to the ratio of distances, it's a short step to getting to the eccentricity expression...
 
  • #3
Thanks, got it. Silly of me for starting with eccentricity in terms of energy and angular momentum instead of geometry.
 
  • #4
… geometry …

Hi cscott! :smile:

Consider it geometrically …

Hint: if F is a focus of the ellipse, and P and Q are the ends of the major axis, what is PF/QF as a function of e?

And then what is n as a function of PF/QF? :smile:
 

1. What is eccentricity of orbit?

Eccentricity of orbit refers to the shape of an object's path around another object in space. It is a measure of how circular or elongated the orbit is, with a value ranging from 0 (perfectly circular) to 1 (highly elongated).

2. How is eccentricity of orbit calculated?

Eccentricity of orbit is calculated by dividing the distance between the foci of the ellipse (the two points where the orbiting object is closest and farthest from the object it is orbiting) by the length of the major axis of the ellipse (the longest diameter).

3. What factors affect the eccentricity of orbit?

The eccentricity of orbit is primarily affected by the amount of gravitational force between the two objects, as well as the initial velocity and direction of the orbiting object. Other factors such as the shape and mass of the two objects can also play a role.

4. How does eccentricity of orbit impact a planet's climate?

The eccentricity of orbit can impact a planet's climate by affecting the amount of sunlight it receives at different points in its orbit. A more eccentric orbit can result in more extreme seasonal changes, while a less eccentric orbit can lead to more consistent temperatures throughout the year.

5. How does eccentricity of orbit impact the stability of a system?

The eccentricity of orbit can impact the stability of a system by influencing the gravitational forces between the two objects. A high eccentricity can result in a more unstable orbit, while a low eccentricity can lead to a more stable and predictable orbit.

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