Is angular momentum of the planet conserved?

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SUMMARY

The discussion centers on the conservation of angular momentum in planetary motion, specifically addressing the equation mr(1)V(1)= mr(2)v(2), where "m" represents mass, "r" is the distance from the sun, and "v" is velocity. Angular momentum is generally conserved in the absence of external forces; however, the gravitational force from the sun acts as an external force on planets. While planets move in elliptical orbits, which complicates the conservation of angular momentum, the elliptical paths are sufficiently close to circular that angular momentum can be considered conserved for practical purposes.

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  • Understanding of basic physics concepts such as momentum and angular momentum.
  • Familiarity with the equation for angular momentum (L = mrv).
  • Knowledge of gravitational forces and their effects on planetary motion.
  • Basic comprehension of elliptical versus circular orbits.
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  • Study the principles of angular momentum conservation in closed systems.
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Astronomer107
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What is it meant by:

mr(1)V(1)= mr(2)v(2)
The quantity mrv is called the angular momentum of the planet. Is angular momentum of the planet conserved?

What do they mean conserved?? Thanks and sorry such short notice... my physics teacher soooo nicely gave us 2 days notice to finish all the labs for the 2nd marking period by tomorrow, which is in a half hour and I need some sleep, thanks.
 
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"mrv" is mass (m) times distance from the sun (r) times velocity (v).

Ordinary momentum itself is conserved (doesn't change as ambitwistor said) as long as there is no external force on the object.

That's not true for planets- the force of gravity from the sun is an external force.

Angular momentum is conserved if the force is perpendicular to the line of motion. Since planets move in ellipses rather than circles, that is not exactly true but the ellipses are so close to being circles that for most planets the difference is not very large.
 

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