How Do You Calculate the Density of a Planet Based on Satellite Orbit Time?

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Homework Help Overview

The discussion revolves around calculating the density of a planet based on the orbital period of a satellite close to its surface. The problem involves concepts from gravitational physics and circular motion, specifically focusing on the relationship between mass, radius, and density.

Discussion Character

  • Exploratory, Mathematical reasoning, Assumption checking

Approaches and Questions Raised

  • The original poster attempts to apply various gravitational equations but expresses uncertainty about how to proceed with the formulas. They question how to isolate mass and incorporate density into their calculations.
  • Some participants point out errors in the original equations and suggest corrections, questioning the validity of the original poster's approach.
  • There is discussion about the need to eliminate certain variables from the equations to simplify the problem.

Discussion Status

The conversation is ongoing, with participants providing feedback on the original equations and suggesting corrections. There is a focus on clarifying the relationships between the variables involved, but no consensus has been reached on a specific method to solve the problem.

Contextual Notes

Participants are working under the assumption that the planet has a constant density and that the satellite's orbit is circular. There are indications of confusion regarding the application of gravitational equations and the definitions of the variables involved.

shadowice
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Homework Statement


A satellite is in a circular orbit very close to the surface of a spherical planet. The period of the orbit is 2.50 hours. What is density of the planet? Assume that the planet has a constant density.

R= radius
G= gravational constant = 6.6742x10^-11
M = mass of
m = mass of
T = period = 9000 seconds
M = mass of earth
m = mass of planet
w= angular velocity
P = density

Homework Equations


(GmM)/R^2 = Rw^2
GPv/R^3 = W^2
w = 2pi/T
volume = 4/3pi*R^2
P= M/V

The Attempt at a Solution



i have lots of formulas and not really sure how to go about using them all
i know to start with

(GmM)/R^2 = Rw^2 then sub for w divide by r
(GmM)/R^3 = (2pi/T)^2 from here I am not sure what to do to get mass then use my M/(4/3pi*R^2)
 
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Hi shadowice,

There are some erros in your equations that appear to causing some problems:

shadowice said:

Homework Statement


A satellite is in a circular orbit very close to the surface of a spherical planet. The period of the orbit is 2.50 hours. What is density of the planet? Assume that the planet has a constant density.

R= radius
G= gravational constant = 6.6742x10^-11
M = mass of
m = mass of
T = period = 9000 seconds
M = mass of earth
m = mass of planet
w= angular velocity
P = density

Homework Equations


(GmM)/R^2 = Rw^2

This formula is not correct; you have a force on the left side and an acceleration on the right side of the equation.

GPv/R^3 = W^2
w = 2pi/T
volume = 4/3pi*R^2

This last one is also not correct; the volume is (4/3) pi R^3. Once you correct these two, do you see what to do now?
 
so your saying to change this

(GmM)/R^2 = Rw^2

to

(GmM)/R^3 =w^2 to solve for a number which would be m = Mr^3*(2pi/T)^2

and set that to be the top and (4/3) pi R^3 to be the bottom and cancel out the r's and substitute numbers in. But where do i get rid of the M i see no way to remove it from the equation

[Mr^3*(2pi/T)^2]/[(4/3) pi R^3]
 
shadowice said:
so your saying to change this

(GmM)/R^2 = Rw^2

to

(GmM)/R^3 =w^2

No, because that does not correct the equation. If you look in your book, you will see that you either have one one too many mass factors on the left side, or you are missing a mass on the right side. Once you make that small change you will almost be done with the problem.



to solve for a number which would be m = Mr^3*(2pi/T)^2

This expression cannot be right, since the units are not the same on each side of the equation.



Once you correct your first equation from this post, you will find that one of the masses cancels out and you will be left with an equation with only one mass to deal with.


After that, the goal is to put the density in the formula. You already have that:

P = M / V

so you can use this to eliminate the M in your equation.
 

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