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Thursday, 4 August 2011

Physics GRE - #3

In Kepler's problem of planetary motion, various values of the eccentricity and hence the energy E classify orbits according to conic sections. What value of the eccentricity \epsilon and the energy E belongs to a parabolic orbit?

  • \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
Choice number 5 is the answer. Recall that the eccentricity is defined by \epsilon = \sqrt{1+\frac{E}{V_{min}}}. Additionally, we also have the corresponding trajectory equation: \frac{p}{r}=1+\epsilon \cos{\phi} where p is the radius of the circular orbit (when \epsilon = 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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[hide] Alemi said...

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

on 4 August 2011 at 20:46
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