Relationships: Runge-Lenz Vector, Kepler's Laws, Position, Velocity, and Angular Momentum, Exercises of Classical and Relativistic Mechanics

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.

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2011/2012

Uploaded on 07/19/2012

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where xis a fixed vector of integration. We define the Runge–Lenz vector:
A:= x
k=˙q×J
kˆq.
4. Let’s expand ˙q×Jusing the vector identity given in Exercise 1:
˙q×J=m[ ˙q×(q×˙q)] = m[|˙q|2q(q·˙q) ˙q].
Thus it follows that
( ˙q×J)·q=m[|˙q|2|q|2(q·˙q)2]
and if neither qnor ˙qis zero we have that
( ˙q×J)·q=m|˙q|2|q|2[1 cos2ϕ] = m|˙q|2|q|2sin2ϕ
where ϕis the angle between qand ˙q. This last expression is exactly J·J/m so that we have shown:
( ˙q×J)·q=J·J/m (6)
(if either qor ˙qis zero, then Jis zero, and the above expression remains valid ). Combining (6)
with the definition of Ayields:
A·q=J·J
km |q|.(7)
5. If we write A·qas |A||q|cos θwhere θis the angle between Aand qwe see that (7) gives:
|A||q|cos θ=J·J
km |q|
which can be solved for |q|to yield:
|q|=J·J
km
1
1 + |A|cos θ.(8)
2
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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.

  1. Let’s expand ˙q × J using the vector identity given in Exercise 1:

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 =

J · J

km

− |q|. (7)

  1. If we write A · q as |A||q| cos θ where θ is the angle between A and q we see that (7) gives:

|A||q| cos θ =

J · J

km

− |q|

which can be solved for |q| to yield:

|q| = J^ ·^ J km

1 + |A| cos θ

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