How Does Satellite Motion Work?

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SUMMARY

Satellite motion is defined by the balance between gravitational force and centrifugal force, which establishes a fixed speed for any given orbit radius. While circular orbits are often referenced, they are not commonly found in nature or artificial constructs, with most planets, except Mercury and Pluto, maintaining nearly circular orbits. The dominant force acting on a satellite is gravity, allowing satellites to "fall" indefinitely when positioned above a certain altitude, specifically above 16,000 km. Additionally, satellites follow conic sections, primarily elliptical orbits as described by Kepler's first law.

PREREQUISITES
  • Understanding of gravitational forces and centrifugal forces
  • Familiarity with orbital mechanics concepts
  • Knowledge of Kepler's laws of planetary motion
  • Basic physics principles related to motion and forces
NEXT STEPS
  • Study Kepler's laws of planetary motion in detail
  • Explore the mathematical modeling of elliptical orbits
  • Research the effects of gravitational perturbations on satellite trajectories
  • Learn about the different types of satellite orbits and their applications
USEFUL FOR

Aerospace engineers, astrophysicists, students of physics, and anyone interested in understanding the principles of satellite dynamics and orbital mechanics.

ColterMacK
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1. What is Satellite Motion?



2. What are the main concepts of Satellite Motion?


I googled these for 6 hours yesterday and never came up with any solid answers. I have also checked the school library and have found no solid answers either. All that I get is a bunch of experiments that Newton did about Satellite Motion but not a definition.
 
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Not sure it's specifically for satelites but for any object in orbit - the centrifugal force outward balances the gravitiational force inward.
This sets a fixed speed for any orbit radius.
 
mgb_phys said:
Not sure it's specifically for satelites but for any object in orbit - the centrifugal force outward balances the gravitiational force inward.
This sets a fixed speed for any orbit radius.

That is only true for circular orbits, and which circular orbits never occur in nature -- or artificially. That said, except for Mercury and Pluto, the planets are in nearly circular orbits.

One key main concept of satellite motion is that gravity is by far the dominant force on a satellite. The same is true for an arrow. An arrow and a satellite differ in that the arrow falls for a short time before it hits the ground. A satellite falls for a long, long time before hitting the ground. Satellites with perigee above 16,000 km or so will essentially fall forever.

Ignoring perturbations, another key concept of satellite motion is that they follow a conic section.
 
ColterMacK said:
1. What is Satellite Motion?
I think you mean elliptical orbits which are predicted by Kepler's first law.
 

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