Momentum Principle Related to Velocity

Click For Summary
SUMMARY

The discussion centers on applying the Momentum Principle to calculate the speed of a satellite with a mass of 2500 kg orbiting the Earth at a radius of 8.3 x 106 m. The relevant equations include the Momentum Principle, expressed as Pfinal = Pinitial + Fnet * ΔT, and the gravitational force equation GMm/r2. The solution involves recognizing that the satellite's circular motion allows for the expression of velocity in terms of gravitational parameters, leading to the conclusion that v = √(G * Mearth / r).

PREREQUISITES
  • Understanding of the Momentum Principle in physics
  • Knowledge of circular motion dynamics
  • Familiarity with Newton's Second Law
  • Basic grasp of gravitational force equations
NEXT STEPS
  • Study the derivation of the Momentum Principle in circular motion
  • Learn about gravitational force calculations using GMm/r2
  • Explore the relationship between velocity and orbital radius
  • Investigate the concept of orbital period and its calculation
USEFUL FOR

Students in physics, particularly those studying mechanics and orbital dynamics, as well as educators looking to explain the application of the Momentum Principle in real-world scenarios.

cowmoo32
Messages
121
Reaction score
0

Homework Statement



You will need to use the Momentum Principle to do the first part of this problem, and the Energy Principle to do the second part.

A satellite of mass 2500 kg orbits the Earth in a circular orbit of radius of 8.3 106 m (this is above the Earth's atmosphere).The mass of the Earth is 6.0 1024 kg.
What is the speed of the satellite?
I have the 2nd part of the problem, so all I need is the momentum principle


Homework Equations



Pfinal = Pinitial + Fnet*DeltaT
GMm/r^2

The Attempt at a Solution


I'm not sure how to start this one. The directions say that I'm supposed to use the momentum principle, but I'm not given the speed of the satellite. I was thinking maybe the derivative form of the momentum principle and find the perpendicular component of dP/dT, but I'm not sure how long it takes for the satellite to go around th earth. I'm completely stuck.
 
Physics news on Phys.org
I have no idea what you mean by the "momentum principle". If you mean conservation of momentum, I don't see how that is relevant.

Instead, apply Newton's 2nd law to the satellite, recognizing that its motion is circular.
 
By momentum principle I mean DeltaP = Fnet*DeltaT
 
OK, I see. Your initial thought was correct: Use F = dP/dt. (Note that this is another way of stating Newton's 2nd law.)

Use what you know (or should know) about circular motion to evaluate d(mv)/dt = m dv/dt.
 
Here's the problem I have with using dP/dt: In order to find the velocity, or the change in momentum, I need to know the time it takes for one rotation around the earth...that's why I didn't use that formula in the first place. v = dr/dt, but again, I don't have dt.
 
Call the speed "v" and express dP/dt in terms of it (along with other known variables).
 
v= dr/dt I can find dr because I know the radius of orbit, but I have no way of finding dt.
 
You can express the period (if you need it) in terms of v, since you know the radius of the orbit.
 
I don't understand how you can express the period in terms of v if you don't know the time.
 
  • #10
Ok, I figured out the problem.

v = sqrt(G*Mearth/r)
 
  • #11
Excellent.
 

Similar threads

  • · Replies 9 ·
Replies
9
Views
1K
  • · Replies 6 ·
Replies
6
Views
3K
Replies
5
Views
3K
Replies
3
Views
6K
  • · Replies 1 ·
Replies
1
Views
8K
  • · Replies 2 ·
Replies
2
Views
3K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 6 ·
Replies
6
Views
2K
Replies
1
Views
8K
Replies
1
Views
6K