Closest stable orbit of a body around earth

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SUMMARY

The discussion focuses on calculating the closest stable orbit of the Moon around Earth, incorporating eccentricity to model an elliptical orbit. Key parameters include the mass of the Moon (7.348x10^22 kg), the mass of Earth (5.97x10^24 kg), and the gravitational constant (6.674x10^-11 m^3 kg^-1 s^-2). The gravitational parameter for the Moon is calculated as u = 4.03x10^14 m^3 s^-2. The participant seeks guidance on whether calculating the velocity of the Moon or the acceleration due to gravity is the best approach for determining this stable orbit.

PREREQUISITES
  • Understanding of gravitational parameters and their calculations
  • Familiarity with orbital mechanics and elliptical orbits
  • Knowledge of calculus, particularly in relation to velocity and acceleration
  • Experience with simulation tools like Universe Sandbox
NEXT STEPS
  • Research the equations of motion for elliptical orbits in celestial mechanics
  • Learn how to apply the gravitational parameter in orbital calculations
  • Explore the effects of atmospheric drag on low Earth orbits
  • Investigate simulation techniques in Universe Sandbox for modeling orbits
USEFUL FOR

Students in physics or mathematics, hobbyists interested in celestial mechanics, and anyone looking to model orbital dynamics using simulation software.

AndrewC
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Homework Statement


This is a problem I picked for my calculus one class that I would like to solve, then model the solution using the sandbox video game universe sandbox. I would like to calculate the closest stable orbit of the moon, if possible allowing for some eccentricity in the orbit making it an ellipse. If this is the wrong forum to post this in I apologize.
mass of moon = 7.348x10^22kg
Mass of Earth = 5.97x0^24kg
Gravitational constant = 6.674x10^-11m^3kg^-1s^-2
Gravitational parameter of moon = G(m1+m2) = u = 4.03x10^14[/B]

Homework Equations


V=sqrt(u ((2/r)-(1/a)))
r = current distance from parent body
a = semi major axis of orbiting body
u = Gravitational parameter = GM if orbiting body's mass is small compared to parent body.
u = G (m1+m2) if orbiting body's mass is comparable to parent body.

The Attempt at a Solution


I'm not sure calculating velocitiy of tge moon or acceleration due to gravity is the best way to find the closest stable orbit? Looking for any input.[/B]
 
Last edited:
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By stable orbit, it this considering low Earth orbits are affected by the outer fringes of the atmosphere, so they are slowed down and the orbit is not "stable"?
 
Sorry I needed to update all of the info. I'm specifically thinking of the moon. So this is not a very real world problem. It's so e thing I picked for fun for a math project.
 

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