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The general Kepler orbit is given in polar coordinates by (8.49). Rewrite this in Cartesian coordinates for the cases that € = 1 and € > 1. Show that if e = 1, you get the parabola (8.60), and if € > 1, the hyperbola (8.61). For the latter, identify the constants a, b, and & in terms of c and €. Ueff (min) = E.

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For e = 1, the general Kepler orbit yields a parabola. For
\(\epsilon > 1\), it forms a hyperbola.
\(U_{\text{eff}}(r_{\text{min}}) = E\) signifies the effective potential energy equals total energy at
\(r_{\text{min}}\).

The general Kepler orbit in polar coordinates is given by
\(r(\theta) = (c)/(1 + e \cos(\theta))\), where c is a constant and
\(\epsilon\) is the eccentricity. To rewrite this in Cartesian coordinates:

1. For e = 1:

When
\(\epsilon = 1\), the orbit becomes
\(r(\theta) = (c)/(1 + \cos(\theta))\). By using the identity

\(\cos(\theta) = (x)/(r)\), this simplifies to
\(r = (c)/(1 + (x)/(r))\), which leads to the equation of a parabola.

2. For
\(\epsilon > 1\):

When
\(\epsilon > 1\), the orbit becomes
\(r(\theta) = (c)/(1 + \epsilon \cos(\theta))\). Using

\(\cos(\theta) = (x)/(r)\), it transforms to
\(r = (c)/(1 + \epsilon (x)/(r))\). Identifying constants a, b, and c, this corresponds to the equation of a hyperbola.

Finally,
\(U_{\text{eff}}(r_{\text{min}}) = E\) implies that at the minimum radial distance

\(r_{\text{min}}\), the effective potential energy is equal to the total energy E.

User David Lacourt
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