Quantization of Earth's angular momentum

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SUMMARY

The discussion centers on the quantization of Earth's angular momentum in its orbit around the Sun, comparing it to the quantized states of a hydrogen electron. The calculated quantum number for Earth is approximately 2.523 x 1074. The energy transition between quantum states was derived using gravitational and kinetic energy equations, resulting in a formula for energy release during transitions. The participant identified the need for the mass of the Sun to complete their calculations.

PREREQUISITES
  • Understanding of classical mechanics, specifically angular momentum
  • Familiarity with quantum mechanics concepts, particularly quantization
  • Knowledge of gravitational forces and energy equations
  • Proficiency in algebra and calculus for solving equations
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  • Research the implications of angular momentum quantization in celestial mechanics
  • Study gravitational potential energy and its applications in astrophysics
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Students and professionals in physics, particularly those focusing on astrophysics, celestial mechanics, and quantum mechanics. This discussion is beneficial for anyone interested in the intersection of classical and quantum theories in planetary motion.

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Homework Statement


If the angular momentum of Earth in its motion around the Sun were quantized like a hydrogen electron, what would Earth's quantum number be? How much energy would be released in a transition to the next lowest level? Would that energy release be detectable? What would be the radius of that orbit?

Homework Equations


L = mvr = nħ
F = GMm/r2 = mv2/r
En = -E0/n2

The Attempt at a Solution


I found Earth's quantum number by solving mvr = nħ for n, with m = 5.972 x 1024 kg, r = 149.7 x 109 m and v = 29.78 x 103 m/s.

n = 2.523 x 1074

The second part is what gets me.
In order to express the energy of a energy level in terms of a planet, I used
F = GMm/r2 = mv2/r
and E = KE + PEg = mv2/2 - GMm/r
to get:

E = -GMm/2r

I then plugged in v = (GM/r)1/2 to r = nħ/mv getting r = n2ħ2/m2GM

And then plugged this into E getting:

E = -G2M2m3/2n2ħ2

The energy of a transition would equal: En+1 - En = -E0/(n+1)2 + E0/n2

Which I could solve with a super huge/super small online calculator. I already assume that the energy will be super small and the orbit won't noticeably change. My issue is...what do I plug in for m? Or should I do it a completely different way? Please help!
 
Last edited:
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Oh duh, I went through all that work and didn't realize I need the mass of the sun as well as the Earth.
 

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