Oh no. I'm frightened to say Jim O's explanation is just about exactly what I had envisioned, but it seemed so simple I didn't say it. Must be reading too many of Jorge's posts. On the other hand, I'm proud to say I still don't understand what this has to do with an asymptote to a Mars transfer orbit since it's so highly inclined.
Try this:
The trajectory to Mars leaves Earth in a particular direction.
If the axis of rotation of that orbit were pointed in that direction, the spacecraft would have to make a right angle turn, after killing off all of the orbital velocity. Obviously that won't work.
The idea is to add to the orbital momentum. This works when the trajectory to Mars is in the plane of the orbit. When the plane of the orbit rotates too far from the trajectory, the correction becomes unaffordable from an energy and momentum standpoint.
Or this:
Thing of the Mars departure in reverse. The line to Mars runs back towards the Earth. Wherever it would pass the Earth, the line swings around Earth in a hyperbola. If the collection of these lines is limited to those where the perigee of the hyperbola matches some altitude, you get this hyperbolic cylinder, with the tangent points forming the circle.
The center of the circle is the line along the trajectory through the center of the Earth.
If a satellite passes through that point, it then hits that circle at normal incidence. If it gets a quick boost to escape velocity, plus a specific velocity, it leaves along one of the hyperbolas and is off to Mars.
That circle is fixed in space, or rather, moving very slowly over a period of days. If the orbit normal is regressing around the Earth, it may not intersect the circle, never mind go through the center of it. The energy to force it to the center is the energy for a big plane change, which we know is beyond the S/C capability.
Is that any better?