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

In summary: Note that the formula for the volume of a sphere is:V = (4/3) pi R^3so you can rearrange it to:M = V * P / (4/3) piIf you substitute this into your first equation, you will get a formula with P as the only variable. Then you can solve it for P (the density) and that will be the answer to your problem.In summary, we use the equation (GmM)/R^2 = Rw^2 to find the mass of the planet, which cancels out and leaves us with an equation containing only the density, P. Using the formula P = M/V, we can eliminate the remaining mass variable and solve
  • #1
shadowice
26
0

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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  • #2
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?
 
  • #3
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]
 
  • #4
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.
 

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

1. What is planetary motion density?

Planetary motion density refers to the distribution and movement of celestial bodies, such as planets, moons, comets, and asteroids, within a specific area of space.

2. How is planetary motion density calculated?

The planetary motion density is calculated by dividing the mass of all celestial bodies in a specific area by the volume of that area. This gives us a measure of how much mass is present in a given space.

3. Why is planetary motion density important?

Studying the planetary motion density can provide valuable insights into the formation and evolution of our solar system. It can also help us understand the dynamics of other planetary systems in the universe.

4. How does planetary motion density affect the gravitational pull between celestial bodies?

The closer the celestial bodies are to each other, the stronger their gravitational pull will be. This means that areas with higher planetary motion density will experience stronger gravitational forces compared to areas with lower density.

5. What factors can influence planetary motion density?

Planetary motion density can be influenced by various factors, such as the size and mass of celestial bodies, their distance from each other, and the presence of other gravitational forces, such as from neighboring stars or black holes.

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