The Kepler Orbits (algebra manipulation)

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SUMMARY

The discussion focuses on transforming the Kepler orbit equation, represented as r(φ) = c / (1 + ε * cos(φ)), into rectangular coordinates (x, y) to demonstrate that it conforms to the standard ellipse equation (8.51). The constants a, b, and d are defined in equation 8.52, where a = c / (1 - ε²), b = c / √(1 - ε²), and d = aε. The participant successfully simplifies the left-hand side to r² but struggles to manipulate the right-hand side to match the ellipse form, indicating a need for further algebraic manipulation.

PREREQUISITES
  • Understanding of Keplerian orbits and their mathematical representation.
  • Familiarity with polar and rectangular coordinate transformations.
  • Knowledge of algebraic manipulation techniques, particularly with quadratic equations.
  • Proficiency in interpreting and applying mathematical equations from textbooks.
NEXT STEPS
  • Study the derivation of the standard ellipse equation from polar coordinates.
  • Practice algebraic manipulation of equations involving square roots and perfect squares.
  • Explore the geometric interpretation of ellipses in rectangular coordinates.
  • Review the properties of conic sections, focusing on ellipses and their parameters.
USEFUL FOR

Students studying advanced algebra, physics enthusiasts exploring orbital mechanics, and educators seeking to enhance their understanding of conic sections and their applications in celestial mechanics.

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Homework Statement



We have proved that any Kepler orbit can be written in the form of r(\phi) = \frac{c}{1+\epsilon*cos(\phi)} where c>0 \epsilon\geq 0. for the case that 0 \leq \epsilon < 1, rewrite this equation in rectangular coordinates (x,y) and prove that the equation can be cast in the form 8.51 which is the equation of an ellipse. Verify the values of the constants given in 8.52

Homework Equations



8.51: 1 = \frac{(x+d)^{2}}{a^{2}} + \frac{y^{2}}{b^{2}}

8.52: a = \frac{c}{1-\epsilon^{2}} ; b = \frac{c}{\sqrt{1-\epsilon^{2}}} ; d = a\epsilon or d = \frac{c\epsilon}{1-\epsilon^{2}}

The Attempt at a Solution



i plugged in equation 8.52 into 8.51 and started simplifying stuff... I ended up with x^{2}+y^{2} = c^{2} + \epsilon^{2}x^{2} - 2xc\epsilon

i know the left hand side is correct because it equals r^{2}. So i know i have to eventually take the square root of each side, however, I have no idea how to get the right hand side of my equation to look like the right hand side of the equation listed in the problem.

any ideas?
 
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i just simplified it down more so that

\sqrt{x^{2}+y^{2}} = c - \epsilonx

because the right hand side was a perfect square and could be made into (c-\epsilonx)^{2}
 

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