Earth orbit -- geosynchronous orbit calculation

AI Thread Summary
The discussion revolves around calculating geosynchronous orbit parameters using Newton's laws and centripetal acceleration. The initial approach incorrectly applies angular velocity and does not utilize the correct relationships between speed, radius, and gravitational forces. Participants emphasize the need to derive centripetal acceleration and gravitational force equations to establish the correct relationship. Key corrections include recognizing that centripetal acceleration is expressed as ω²r and clarifying the gravitational force formula. Overall, the conversation focuses on refining the method for determining the radius of a geosynchronous orbit through proper application of physics principles.
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Homework Statement


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Homework Equations



ε= r_max - r_min / r_max + r_min
= r*v2 / gRE

The Attempt at a Solution


I first find that 1 revolution is 2π rad , the angular velocity ω = 2π rad / 24h = π/43200 rad /s
so v = rω where r is the unknown
ε = 0 (circular orbit)

r*(rω)2 / g RE = 0Correct route?
 
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Your approach is incorrect. You need to use Newton's 2nd law to find a relation between speed and radius in a circular orbit.
 
st
kuruman said:
Your approach is incorrect. You need to use Newton's 2nd law to find a relation between speed and radius in a circular orbit.
start with F= ma, then integrate?
 
No need for integration. Remember that the acceleration here is centripetal. What is an expression for F?
 
F=ma then a is gravity?
 
No, a is the centripetal acceleration. What is an expression for it? F is the force of gravitational attraction between two masses according to Newton's law of gravitational attraction.
 
GmM/ r2
 
That's F. What about a on the other side of the equation?
 
m (r'' + rω) because it is the angular movement ?
 
  • #10
Centripetal acceleration is ω2r, not ωr. Also, what is r'' for a satellite in a circular orbit?
 
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