Planets and satellites, law of periods circular orbit.

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Homework Help Overview

The discussion revolves around a problem involving a satellite in circular orbit around a planet, where the gravitational acceleration on the planet's surface is known. Participants are tasked with determining the radius of the planet based on given parameters such as the satellite's mass, orbital period, and radius.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning, Assumption checking

Approaches and Questions Raised

  • Participants explore the relationship between gravitational force and orbital mechanics, questioning the definitions of variables in their equations. There is discussion on using centripetal acceleration to find the planet's mass and radius, as well as the implications of Newton's laws in this context.

Discussion Status

Participants are actively engaging with each other's reasoning, providing guidance on the correct application of formulas. There is an ongoing exploration of the relationship between the satellite's orbit and the gravitational properties of the planet, with some participants correcting earlier misunderstandings regarding the equations used.

Contextual Notes

Some participants express uncertainty about the values and assumptions used in their calculations, particularly regarding the mass of the planet and the radius in relation to gravitational acceleration. There is a focus on ensuring that the equations are applied correctly, especially in light of the gravitational acceleration provided in the problem statement.

J-dizzal
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Homework Statement


A 15 kg satellite has a circular orbit with a period of 4.4 h and a radius of 3.5 × 106 m around a planet of unknown mass. If the magnitude of the gravitational acceleration on the surface of the planet is 1.2 m/s2, what is the radius of the planet?

Homework Equations

The Attempt at a Solution


20150719_221818_zpsyk9ccfhe.jpg

I think I am on the right track, but I am stuck finding the radius of the planet. in my equation at the bottom for radius what would i use for M and m?
 
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In your equation ##r=\sqrt{\frac{GMm}{F_g}}## r is the distance between the two objects, not the radius of the planet.

Try to use the centripetal acceleration to find the mass of the planet (only 1 mass will cause this orbit) and then try to find the radius (with the mass known, only 1 radius will cause that value of surface gravity).
 
Last edited:
Considering Newton's 2nd law, what does Fg /m represent?
 
Nathanael said:
In your equation r=GMmFg−−−−√r=\sqrt{\frac{GMm}{F_g}} r is the distance between the two objects, not the radius of the planet. That equation is really of no use.
would it work if M is the mass of the planet and m is a mass on the surface of the planet? the distance between them would be about the radius of the planet?

TSny said:
Considering Newton's 2nd law, what does Fg /m represent?
acceleration. But in my equation for r; Fg is the force of acceleration on the surface of the planet. would that work with the given a=1.2m/s2
 
J-dizzal said:
would it work if M is the mass of the planet and m is a mass on the surface of the planet? the distance between them would be about the radius of the planet?
Oh my bad, yes then it would work. You just need to find the mass of the planet first.
 
Nathanael said:
Oh my bad, yes then it would work. You just need to find the mass of the planet first.
Does my equation for M look ok, toward the top of my page M=946496.4kg?
If its ok, then would any value for m work in my equation for r?
 
J-dizzal said:
Does my equation for M look ok, toward the top of my page M=946496.4kg?
If its ok, then would any value for m work in my equation for r?
Sorry for ignoring your initial work, apparently I'm not so good at skimming pictures o0)

The equation is right but you didn't cube the radius when you solved it.
 
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Nathanael said:
Sorry for ignoring your initial work, apparently I'm not so good at skimming pictures o0)

The equation is right but you didn't cube the radius when you solved it.
In my equation for r, I am letting Fg=a. where a=1.2m/s/s is a given in the problem statement. I am guessing this is wrong because its the force on the satellite at distance r from the surface.
 
J-dizzal said:
In my equation for r, I am letting Fg=a. where a=1.2m/s/s is a given in the problem statement. I am guessing this is wrong because its the force on the satellite at distance r from the surface.
a is 1.2 m/s/s, not Newtons. Consider an object on the surface of mass m. If it accelerates at 1.2m/s/s, then what must the force on that object (of mass m) be?
 
  • #10
J-dizzal said:
acceleration. Yes, But in my equation for r; Fg is the force of acceleration on the surface of the planet. would that work with the given a=1.2m/s2
Fg = GMm/r2 gives the force of gravity on m as a function of r. Using this, you can derive an expression for FG /m as a function of r. Thus, you have an expression for the acceleration due to gravity as a function of r. Apply this for a point at the surface of the planet.
 
  • #11
Nathanael said:
a is 1.2 m/s/s, not Newtons. Consider an object on the surface of mass m. If it accelerates at 1.2m/s/s, then what must the force on that object (of mass m) be?
F=(15kg)(1.2m/s/s)=18N

TSny said:
Fg = GMm/r2 gives the force of gravity on m as a function of r. Using this, you can derive an expression for FG /m as a function of r. Thus, you have an expression for the acceleration due to gravity as a function of r. Apply this for a point at the surface of the planet.
Fg/M = Gm/r2 so this would be the acceleration of M?
 
  • #12
J-dizzal said:
Fg/M = Gm/r2 so this would be the acceleration of M?

Well, yes that would give the acceleration of the planet (M) due to the attraction of the satellite (m). But that would be extremely small and it is not of relevance to this problem.

However, Fg /m gives the acceleration of the satellite due to the attraction of the planet. This is what you would call the "acceleration due to gravity of the planet". You are given the acceleration due to gravity of the planet at the surface of the planet.

So you want to find an expression for Fg /m rather than Fg /M. Then apply the expression to a point near the surface of the planet.
 
  • #13
TSny said:
Well, yes that would give the acceleration of the planet (M) due to the attraction of the satellite (m). But that would be extremely small and it is not of relevance to this problem.

However, Fg /m gives the acceleration of the satellite due to the attraction of the planet. This is what you would call the "acceleration due to gravity of the planet". You are given the acceleration due to gravity of the planet at the surface of the planet.

So you want to find an expression for Fg /m rather than Fg /M. Then apply the expression to a point near the surface of the planet.
im getting R= sqrt(GM/a) =1.337x106 same answer i got before...
 
  • #14
R = sqrt(GM/a) is correct. What did you get for the mass of the planet, M, after correcting for cubing r as pointed out by Nathanael in post #7?
 
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  • #15
TSny said:
R = sqrt(GM/a) is correct. What did you get for the mass of the planet, M, after correcting for cubing r as pointed out by Nathanael in post #7?
I got 3.219x1022kg
 
  • #16
TSny said:
R = sqrt(GM/a) is correct. What did you get for the mass of the planet, M, after correcting for cubing r as pointed out by Nathanael in post #7?
ok i got it correct now thanks again.
 

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