Acceleration only due to conservation of angular momentum

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SUMMARY

The discussion centers on the relationship between conservation of angular momentum and acceleration in planetary motion, specifically addressing the case where no external force is present. It is established that the angular momentum \(\vec{L}\) of planets, defined as \(\mid \vec{L} \mid = mr^2 \dot{\theta} = mrv_{\theta}\), remains constant. The acceleration in polar coordinates reveals that while the tangential acceleration \(a_{\theta}\) is zero due to the conservation of angular momentum, the velocity \(v_{\theta}\) must increase as the radial distance \(r\) decreases to maintain constant angular momentum. This phenomenon occurs without an external force acting in the tangential direction.

PREREQUISITES
  • Understanding of angular momentum and its conservation principles
  • Familiarity with polar coordinate systems in physics
  • Knowledge of basic kinematics, particularly acceleration and velocity
  • Concept of central forces, particularly gravitational forces
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  • Study the implications of conservation of angular momentum in non-inertial reference frames
  • Explore the mathematical derivation of acceleration in polar coordinates
  • Investigate the role of central forces in orbital mechanics
  • Learn about the dynamics of planetary motion and Kepler's laws
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Students of physics, astrophysicists, and anyone interested in understanding the dynamics of planetary motion and the principles of angular momentum conservation.

Soren4
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I don't understand why the conservation of angular momentum can imply an acceleration, in absence of a force.

Consider for istance planetary motion. The angular momentum \vec{L} of the planets is conserved and that means \mid \vec{L} \mid=mr^2 \dot{\theta}=mrv_{\theta} is conserved too.

Consider the acceleration in polar coordinates
$$
\left( \ddot r - r\dot\theta^2 \right) \hat{\mathbf r} + \left( r\ddot\theta+ 2\dot r \dot\theta\right) \hat{\boldsymbol{\theta}} \ $$

The second term is zero since \vec{L} is constant. In fact the second term can be rewritten as <br /> a_{\theta}=\frac{1}{r}[\frac{d}{dt}(r^2 \dot{\theta})]=\frac{1}{r}[\frac{d}{dt}(\frac{L}{m})].
This means that there is no acceleration in the direction of \hat{\boldsymbol{\theta}}, which is clear since the gravitational force is a central froce.

But if the distance r decreases v_{\theta} (i.e. the velocity in the direction of \hat{\boldsymbol{\theta}}) must increase in order to keep \mid\vec{L} \mid constant.

How can v_{\theta} increase if there is no acceleration in the direction of \hat{\boldsymbol{\theta}}?

I understood that it happens because of the conservation of angular momentum but if there is an acceleration, necessarily a force is needed. I don't see where do this force come from.
 
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Speed changes because the force is not perpedicular to velocity, when the distance changess.
 

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