Polar Form of the Equation of a Conic

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SUMMARY

The polar equation of an elliptical orbit with the sun as a focus is established as r = (1 - e²)a / (1 - e cos θ, where 'a' represents half the length of the major axis and 'e' is the eccentricity defined as e = √(1 - b²/a²). The discussion outlines the conversion process from the rectangular form of an ellipse, x²/a² + y²/b² = 1, to its polar form, emphasizing the relationship between the coordinates and the parameters of the ellipse. Key properties such as the distance from the focus to the center of the ellipse, f = ae, are also highlighted as essential for understanding the transformation.

PREREQUISITES
  • Understanding of polar coordinates and their relationship to rectangular coordinates.
  • Familiarity with the standard form of an ellipse in rectangular coordinates.
  • Knowledge of eccentricity and its calculation in the context of ellipses.
  • Basic algebraic manipulation skills for converting equations between forms.
NEXT STEPS
  • Study the derivation of the polar equation of conics, focusing on ellipses.
  • Learn about the properties of ellipses, including foci and directrices.
  • Explore the application of polar coordinates in physics, particularly in orbital mechanics.
  • Investigate the relationship between eccentricity and the shape of conic sections.
USEFUL FOR

Students studying conic sections, mathematicians interested in polar coordinates, and anyone involved in physics or astronomy focusing on orbital mechanics.

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Homework Statement


The planets travel in an elliptical orbit with the sun as a focus. Assume that the focus is at the pole, the major axis lies on the polar axis and the length of the major axis is 2a. Show that the polar equation of orbit is given by [tex]r=\frac{(1-e^2)a}{1-e\cos\theta}[/tex]

here's a diagram they give:
attachment.php?attachmentid=27172&stc=1&d=1280061444.jpg



Homework Equations



The Attempt at a Solution



Ok, I have converted the equation of an ellipse in rectangular form: [tex]\frac{x^2}{a^2}+\frac{y^2}{b^2}=1[/tex]

to polar form before, yielding [tex]r^2=\frac{b^2}{1-e^2\cos^2\theta}[/tex]

this seems like it would be a similar process.


On the standard form of the ellipse in rectangular form, I believe you would have (x+c)2 because with one focus at the origin the center is going to be c away from the focus (I know It's plus c because they give a diagram showing the center in the positive x axis; rather than negative which would be minus c)

so would you be converting

[tex]\frac{(x+c)^2}{a^2}+\frac{y^2}{b^2}=1[/tex]

to polar form to yield the equation given?

[tex]\frac{(r\cos\theta+c)^2}{a^2}+\frac{(r\sin\theta)^2}{b^2}=1[/tex]

[tex]a^2(r^2\cos^2\theta+2cr\cos\theta+c^2)+b^2(r^2\sin^2\theta)=a^2b^2[/tex]

Before I go any deeper am I on the right path? Thanks.
 

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it may help to know some useful properties of ellipses, the eccentcity is defined as
[tex]e = \sqrt{1-\frac{b^2}{a^2}}[/tex]

and the distance from the focus to the centre of the ellipse is
[tex]f = ae[/tex]

these should help you remove b&c from your equation...

see here for more
http://en.wikipedia.org/wiki/Ellipse
 

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