Describing position on an ellipse as a function of angle

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SUMMARY

The discussion centers on deriving the expression for the position on an ellipse as a function of the eccentric anomaly, E, represented by the formula r = a(1 - e cos E). The user references the semi-major axis, a, and the semi-latus rectum, p = a(1 - e²), while seeking clarity on how to connect these concepts. The auxiliary circle method is introduced as a means to visualize the relationship between the ellipse and the eccentric anomaly. The user is looking for guidance on the next steps to complete the derivation.

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  • Understanding of celestial mechanics principles
  • Familiarity with the concepts of eccentricity (e) and eccentric anomaly (E)
  • Knowledge of the geometric properties of ellipses and auxiliary circles
  • Basic trigonometry, specifically the cosine function
NEXT STEPS
  • Study the derivation of the position on an ellipse using the auxiliary circle method
  • Explore the relationship between eccentric anomaly and true anomaly in orbital mechanics
  • Learn about the properties of ellipses, including semi-major and semi-minor axes
  • Investigate the applications of the semi-latus rectum in orbital calculations
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Students and professionals in celestial mechanics, astrophysics, and mathematics who are looking to deepen their understanding of elliptical orbits and their mathematical representations.

tomwilliam2
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My textbook (on celestial mechanics) makes a passing reference to position on an ellipse being expressed as:
##r = a(1 - e \cos E)## before moving on to the substance of the chapter. E is the eccentric anomaly, and r is the distance from the focus to the point on the ellipse.

I'm trying to understand how to derive this expression before moving on. I know that you take the ellipse, with semi-major axis a, and draw an auxiliary circle of radius a around it. Then, the angle opened up as you move around that circle is the eccentric anomaly, E.
Let the foci of the ellipse lie on the x-axis. Now, if ##r_x## is the distance from the centre of the circle to the point on the x-axis which corresponds to the x-component of the position around the auxiliary circle, then:
##\cos E = r_x / a##
because the hypotenuse of the right triangle is the radius, a. I know that ##ae## is the distance from the centre of the circle to the focus of the ellipse. I know that the semi-latus rectum ##p=a(1-e^2)##, and this is the distance from the focus to the ellipse directly above the focus.
Now I'm not sure how to proceed from here.
Can anyone point me in the right direction?
 
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Thanks! That's the kind of review I'm looking for!
 

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