Runge-Lenz Vector: Calculating Magnitude & Direction

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In summary, the conversation revolves around finding the magnitude and direction of the Runge-Lenz vector, which is a constant of motion for a particle. The first part of the question shows that the vector is indeed a constant of motion by differentiating it with respect to time. The second part involves calculating the vector's magnitude and direction explicitly, which can be done by dotting the vector with the particle's position vector and using the initial conditions of the particle. The relation between this and the motion of the particle in circular, elliptical, or other types of orbits is not explicitly mentioned.
  • #1
samjohnny
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Homework Statement



Please find it attached.

Homework Equations



95de2fe45c8ce9deef85438d31928c57.png

233599c315ed09e65711c7f9410eab4f.png

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The Attempt at a Solution



For the first part of the question I managed to show that the vector is a constant of the motion by differentiating it with respect to time and showing that it yields a value of zero.

As for the second part where I need to calculate the magnitude and direction of the vector then I'm not sure how to go about doing that explicitly. I know that the way vector is defined is such that it is equivalent to the eccentricity vector and so for the circle part it would necessarily be equal to zero. But to show that explicitly I'm not to sure. Any ideas?
 

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  • #2
samjohnny said:

Homework Statement



Please find it attached.

Homework Equations



95de2fe45c8ce9deef85438d31928c57.png

233599c315ed09e65711c7f9410eab4f.png

676dc21daca293b822638428a5ea3c2e.png


The Attempt at a Solution



For the first part of the question I managed to show that the vector is a constant of the motion by differentiating it with respect to time and showing that it yields a value of zero.

As for the second part where I need to calculate the magnitude and direction of the vector then I'm not sure how to go about doing that explicitly. I know that the way vector is defined is such that it is equivalent to the eccentricity vector and so for the circle part it would necessarily be equal to zero. But to show that explicitly I'm not to sure. Any ideas?
Hi,

First of all, notice that the Rung-Lenz Vector could be written by velocity of the particle, because momentum divided my mass is equal to velocity, and K is a constant. Obviously, it is necessary to know initial conditions of the particle, so assume that we know the initial distance and initial velocity, and therefore, the Runge-Lenz Vector (I show this with A). Let me show the particle position vector's with R. Now, calculate Dot Product of A and R in two different ways; in the first path, consider the A has its initial value, but in the second way, put its definition expression. Hence, by some calculation, you can find the R in terms of angle (from a specific axis.)
 
  • #3
Kiarash said:
Hi,

First of all, notice that the Rung-Lenz Vector could be written by velocity of the particle, because momentum divided my mass is equal to velocity, and K is a constant. Obviously, it is necessary to know initial conditions of the particle, so assume that we know the initial distance and initial velocity, and therefore, the Runge-Lenz Vector (I show this with A). Let me show the particle position vector's with R. Now, calculate Dot Product of A and R in two different ways; in the first path, consider the A has its initial value, but in the second way, put its definition expression. Hence, by some calculation, you can find the R in terms of angle (from a specific axis.)

Thank you for the reply. Would it not be the case that, by dotting the Runge Lenz vector with R, the resultant expression would describe motion of the object? I'm not clear on what relation this would have to finding the magnitude/direction of the vector in the case of circular, elliptical etc orbits.
 
  • #4
samjohnny said:
Thank you for the reply. Would it not be the case that, by dotting the Runge Lenz vector with R, the resultant expression would describe motion of the object? I'm not clear on what relation this would have to finding the magnitude/direction of the vector in the case of circular, elliptical etc orbits.
 

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FAQ: Runge-Lenz Vector: Calculating Magnitude & Direction

What is the Runge-Lenz vector?

The Runge-Lenz vector is a mathematical concept used in classical mechanics to describe the orbital behavior of a particle under the influence of a central force, such as gravity. It is named after the two scientists who independently discovered it: Carl Runge and Wilhelm Lenz.

How is the magnitude of the Runge-Lenz vector calculated?

The magnitude of the Runge-Lenz vector is calculated using the formula: |A| = mvr, where m is the mass of the particle, v is its velocity, and r is the distance from the particle to the center of the force. This formula represents the angular momentum of the particle.

What is the direction of the Runge-Lenz vector?

The direction of the Runge-Lenz vector is always perpendicular to both the orbital plane of the particle and the direction of its angular momentum. This means that it points in the direction of the eccentricity vector, which describes the shape of the particle's orbit.

Why is the Runge-Lenz vector important?

The Runge-Lenz vector is important because it is a conserved quantity in a central force system, meaning that its magnitude and direction remain constant over time. This allows us to make predictions about the orbital behavior of a particle without having to constantly calculate its position and velocity.

How is the Runge-Lenz vector used in physics?

The Runge-Lenz vector is used in many areas of physics, including classical mechanics, celestial mechanics, and quantum mechanics. In classical mechanics, it is used to describe the motion of planets and other celestial bodies. In quantum mechanics, it is used to describe the energy levels of an atom and the behavior of electrons around a nucleus.

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