Does the moon orbit as a classical particle?

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SUMMARY

The discussion centers on the moon's orbit around Earth and whether it behaves as a classical particle. The moon orbits at a radius of 3.84E8 m, with a mass of 7.35E22 kg, while Earth has a mass of 5.98E24 kg. To determine if the moon's behavior aligns with classical particle theory, participants suggest using De Broglie's equation to calculate the moon's matter wavelength and compare it to its orbital radius. The relevant equations include λ=h/(mv) and v=sqrt(GM/r), which are essential for this analysis.

PREREQUISITES
  • Understanding of De Broglie's equation
  • Familiarity with gravitational force equations (F=GMm/r^2)
  • Basic knowledge of classical mechanics, particularly orbital motion
  • Ability to perform dimensional analysis and compare magnitudes
NEXT STEPS
  • Calculate the moon's velocity using v=sqrt(GM/r)
  • Determine the moon's matter wavelength using λ=h/(m*sqrt(GM/r))
  • Compare the calculated wavelength to the orbital radius of 3.84E8 m
  • Research the implications of wave-particle duality in classical mechanics
USEFUL FOR

Students of physics, astrophysicists, and anyone interested in the principles of orbital mechanics and wave-particle duality.

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Thread moved from a technical forum, so homework template missing
The moon orbits Earth at a radius of 3.84E8 m. To do so as a classical particle, its wavelength should be small. But small relative to what? Being a rough measure of the region where it is confined, the orbit radius is certainly a relevant dimension against which to compare the wavelength. Compare the two. Does the Moon indeed orbit as a classical particle? (MEarth=5.98E24 kg and MMoon=7.35E22 kg)

I know I need to use De Broglies equation but I don't know what it means by "compare the two". How do I compare the moon's matter wavelength to its orbit? And how do I, from this determine whether it orbits as a classical particle?

Relevant equations: λ=h/(mv), F=mv^2/r, F=GMm/r^2

Do I solve for V and then use that in the wavelength equation? How does that tell me how small it is in relation to the orbit.

v=sqrt(GM/r) λ=h/(m*sqrt(GM/r))
 
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You have two values, the orbit radius and the wavelength, which have the same units. Are they the same order of magnitude? Do they differ by a small factor (2? π?). Or is one incredibly small compared to the other?
 

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