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The runge-lenz vector, a constant vector in the plane of a two-body problem in celestial mechanics. By expanding the vector product of velocity and angular momentum, we derive the relationship between the position vector, velocity vector, and angular momentum, which is a key result in kepler's laws of planetary motion.
Typology: Exercises
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where x is a fixed vector of integration. We define the Runge–Lenz vector:
A := x k
= q˙^ ×^ J k
− ˆq.
q˙ × J = m[ ˙q × (q × q˙)] = m[| q˙|^2 q − (q · q˙) ˙q].
Thus it follows that
( ˙q × J) · q = m[| q˙|^2 |q|^2 − (q · q˙)^2 ]
and if neither q nor ˙q is zero we have that
( ˙q × J) · q = m| q˙|^2 |q|^2 [1 − cos^2 ϕ] = m| q˙|^2 |q|^2 sin^2 ϕ
where ϕ is the angle between q and ˙q. This last expression is exactly J · J/m so that we have shown:
( ˙q × J) · q = J · J/m (6)
(if either q or q˙ is zero, then J is zero, and the above expression remains valid ). Combining (6) with the definition of A yields:
A · q =
km
− |q|. (7)
|A||q| cos θ =
km
− |q|
which can be solved for |q| to yield:
|q| = J^ ·^ J km
1 + |A| cos θ