Finding out the type of central force given the orbit

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SUMMARY

The discussion centers on determining the type of central force responsible for a spaceship's circular orbit near a gas cloud, as presented in AP French's textbook "Newtonian Mechanics". The key conclusion is that the attractive central force can be described by the equation F ~ -1 / r^5. The problem emphasizes the conservation of angular momentum, expressed as angular momentum = m * r^2 * (dtheta / dt), which remains constant, allowing for the derivation of velocity as a function of radius and subsequently leading to the potential energy associated with the force.

PREREQUISITES
  • Understanding of angular momentum in classical mechanics
  • Familiarity with circular motion and forces
  • Knowledge of potential energy concepts in physics
  • Basic calculus for deriving functions
NEXT STEPS
  • Study the derivation of central force equations in classical mechanics
  • Learn about the implications of angular momentum conservation in orbital mechanics
  • Explore the relationship between force and potential energy in physics
  • Investigate examples of non-standard central forces, such as F ~ -1 / r^n
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Students of physics, particularly those studying classical mechanics, as well as educators and tutors looking to deepen their understanding of orbital dynamics and central forces.

saadhusayn
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Hi,

This is the statement of the problem of AP French's textbook "Newtonian Mechanics".

1. Homework Statement

The commander of a spaceship that has shut down its engines and is
coasting near a strange-appearing gas cloud notes that the ship is
following a circular path that will lead directly into the cloud (see the
figure). He also deduces from the ship's motion that its angular momentum
with respect to the cloud is not changing. What attractive (central)
force could account for such an orbit? (ANSWER : F ~ -1 / r^5)

Homework Equations

The Attempt at a Solution



From the information given, angular momentum = m * r^2 * (dtheta / dt) =
constant.
The acceleration of the ship is a combination of tangential and radial
acceleration, the resultant of which is along the line joining the
spacecraft and the cloud.
[/B]

I don't know where to proceed from here.

Thank you very much for your help.
 

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Physics news on Phys.org
saadhusayn said:
From the information given, angular momentum = m * r^2 * (dtheta / dt) =
constant.
This allows you to find velocity as function of radius, which then leads to the potential.
 

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