- \epsilon > 1 and E > 0
- 0 < \epsilon < 1 and V_{min} < E < 0
- \epsilon = 0 and E = V_{min}
- \epsilon < 0 and E < V_{min}
- \epsilon = 1 and E = 0
Thus, we can determine the orbit type by looking at the eccentricity alone (but we must also check the energy to make sure its non-sensical). If you use the trajectory equation, you can determine the cartesian equation form of the orbit by converting the polar form given above. The choices above correspond to the following orbits:
- \epsilon > 1 and E > 0 - hyperbola
- 0 < \epsilon < 1 and V_{min} < E < 0 - ellipse
- \epsilon = 0 and E = V_{min} - circle
- \epsilon < 0 and E < V_{min} - impossible. \epsilon is always positive (because of the square root)
- \epsilon = 1 and E = 0 - parabola
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We've forgotten the definition of eccentricity, but being good physicists, we know that Kepler's equations have three types of solutions, bound solutions ( ellipses ), unbound ( hyperbolas) and parabolas, which are a special case at the turning point.
So, we know that if E < 0 we are bound, if E> 0 we are unbound, so the special case at the turning point must have E= 0, neither bound nor unbound. Answer is E
Thinking on your feet:
We've forgotten the definition of eccentricity, but being good physicists, we know that Kepler's equations have three types of solutions, bound solutions ( ellipses ), unbound ( hyperbolas) and parabolas, which are a special case at the turning point.
So, we know that if E < 0 we are bound, if E> 0 we are unbound, so the special case at the turning point must have E= 0, neither bound nor unbound. Answer is E
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