Solve Satellite Velocity Homework: Find Moon's Velocity

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SUMMARY

The discussion focuses on calculating the velocity of a moon in circular orbit around a planet with a gravitational acceleration of 20 m/s² and a radius of 8.0 × 106 m, at a height of 300,000 m above the surface. The correct approach involves using Newton's law of universal gravitation, represented by the equation GM/r = v², to derive the moon's orbital velocity. The final calculated velocity is approximately 12,421.5 m/s, after determining the planet's mass using the gravitational constant G and the provided parameters.

PREREQUISITES
  • Understanding of Newton's law of universal gravitation (F = GMm/r²)
  • Knowledge of circular motion and centripetal acceleration (a = v²/r)
  • Familiarity with gravitational acceleration and its implications in orbital mechanics
  • Basic algebra for manipulating equations and solving for variables
NEXT STEPS
  • Learn how to derive orbital velocity using the formula V = √(GM/(R + r))
  • Study the implications of gravitational acceleration on satellite motion
  • Explore the concept of escape velocity and its calculations
  • Investigate the relationship between mass, radius, and gravitational force in celestial mechanics
USEFUL FOR

Students studying physics, particularly those focusing on mechanics and gravitation, as well as educators seeking to clarify concepts related to orbital dynamics and gravitational calculations.

physicaled
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Homework Statement


On the surface of a distant planet, objects experience an acceleration due to gravity of 20 m/s2. The distance from the center of the planet to its surface is 8.0 * 106 m. Find the velocity of a moon that is circular orbit about the planet at a height of 300,000 m above the planet's surface.

Homework Equations


a = v2/r

The Attempt at a Solution


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20 = v2/(8e6 + 300,000) = 12,884.1

I know this isn't right because my teacher said the acceleration due to gravity should not be 20. But I don't know how to solve it another way. Could anyone shed some insight?
 
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The acceleration is caused by the gravity of the planet. Can you write the equation for gravitational acceleration at the specified height?
 
Bandersnatch said:
The acceleration is caused by the gravity of the planet. Can you write the equation for gravitational acceleration at the specified height?

The only formula I can think to use would be a = v2/r which would leave me with a = v2/ (8e6 + 300,000) and then I'm still completely lost
 
What equations were introduced when you talked about gravity in class? Look in your notes, or use the internet. Here's a hint: it's all Newton's idea.
 
I suppose you mean the F = GMm/r2 equation? My teacher doesn't really teach so it's mostly us students trying to guess at things. So it would become:
GM/r = v2 leaving me with (6.67e-11)(M)/(8e6+300,000) = v2?

I'm sorry thank you for your patience
 
Actually could you solve it so that:

a= v2/r
20= v2/8e6
v2= 160,000,000
v= 12,649.1 m/s

GM/r= v2
(6.67e-11)(M)/8e6 = 12649.12
6.67e-11M= 1.28e15
M = 1.92e25

GM/r = v2
(6.67e-11)(1.92e25)/(8e6+300,000)= v2
154293975.9 = v2
12421.5 m/s = v

Was this what you were getting at? I was staring at it a little more and the idea came to mind but I'm not really sure if it works out.
 
physicaled said:
I'm not really sure if it works out.
That's pretty much what I had in mind, yes. :)
Looks about right. I'll go over the numbers later, though, I have to go now. But should be fine.
 
Bandersnatch said:
That's pretty much what I had in mind, yes. :)
Looks about right. I'll go over the numbers later, though, I have to go now. But should be fine.
No worries! Thank you so much for your help!
 
Yup, numbers look good too.
Myself, I'd probably write ##ma=\frac{GMm}{R^2}##, get the mass of the planet from there, and then plug it into ##V=\sqrt{\frac{GM}{R+r}}##. Saves you an equation, and is more straightforward reasoning-wise.

Do you understand why you used those equations?
 

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