Motion in a Central Gravitational Force

In summary, the conversation discusses the motion of a particle in a central inverse-square-law force field with a superimposed force that is inversely proportional to the cube of the distance from the particle to the force center. The equation F(r) = -k/r2 - λ/r3 is used, where k and λ are positive constants. The goal is to show that the motion is described by a precessing ellipse. The suggested approach is to use the equation (d2/dθ2)(1/r) + (1/r) = -μr2F(r)/l2, but the individual is unsure of how to proceed with the left hand side. The response suggests solving the differential equation and understanding the motivation behind the equation
  • #1
Macykc2
13
1

Homework Statement


Discuss the motion of a particle in a central inverse-square-law force field for a superimposed force whose magnitude is inversely proportional to the cube of the distance from the particle to the force center, that is:
F(r) = -k/r2 - λ/r3 and k,λ>0​
Show that the motion is described by a precessing ellipse.

Homework Equations


The one given in the question

The Attempt at a Solution


I honestly don't know where to begin, we derived an equation in class that we could find the force law if a particular known orbit r=r(θ), and I was thinking of using it:
(d2/dθ2)(1/r) + (1/r) = -μr2F(r)/l2
but I don't know what to do with the left hand side, but again it's just a guess as to what to start with.
Sorry for not using the math commands, they didn't want to work for some reason.
 
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  • #2
You need to solve the differential equation.

For equations, you can type out LaTeX markup directly.

You may want to back up a bit and make sure you understand the motivation for deriving the equation you used in the first place... see if the same approach still applies here.
 

What is motion in a central gravitational force?

Motion in a central gravitational force refers to the movement of an object under the influence of a central force, such as gravity, acting towards a fixed point. This type of motion follows the laws of classical mechanics and can be described using equations such as Newton's laws of motion and Kepler's laws of planetary motion.

What factors affect motion in a central gravitational force?

The main factors that affect motion in a central gravitational force are the mass of the object and the distance from the center of the gravitational force. The greater the mass of the object, the stronger the gravitational force, and the closer the object is to the center of the force, the stronger the force will be.

What is the relationship between velocity and distance in motion in a central gravitational force?

In motion in a central gravitational force, the velocity of an object is inversely proportional to the distance from the center of the force. This means that as the object moves closer to the center, its velocity will increase, and as it moves further away, its velocity will decrease.

How does motion in a central gravitational force differ from motion in a non-central force?

The main difference between motion in a central gravitational force and motion in a non-central force is the direction of the force. In a central force, the force always acts towards a fixed point, while in a non-central force, the force can act in any direction.

How is motion in a central gravitational force used in real-life applications?

Motion in a central gravitational force is used in many real-life applications, such as space travel, satellite orbiting, and planetary motion. Understanding and calculating the motion in these scenarios is crucial for predicting and controlling the movement of objects in space.

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