How Do You Calculate the Mass of Mars Using Phobos' Orbit?

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Homework Help Overview

The discussion revolves around calculating the mass of Mars using the orbital characteristics of its moon, Phobos. The problem involves concepts from gravitational physics and orbital mechanics.

Discussion Character

  • Exploratory, Mathematical reasoning, Assumption checking

Approaches and Questions Raised

  • Participants discuss the relationship between gravitational force and centripetal force, exploring the equation involving mass, radius, and orbital period. There are attempts to derive the mass of Mars using the formula involving gravitational constant and orbital parameters.

Discussion Status

Several participants have provided feedback on the original poster's approach, pointing out potential errors in the algebra and the need to reconsider the power of the radius in the final equation. There is an ongoing exploration of the correct formulation and calculations, with some participants expressing concern about their understanding of the method.

Contextual Notes

Participants are working under the constraints of homework guidelines, which may limit the extent of direct assistance. There is a shared focus on learning the method rather than simply obtaining the answer.

Saladsamurai
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The Martian satellite Phobos travels in an approx circular orbit with r=9.4*10^6 meters and period 7h 39min. Find the mass of mars.

I am supposed to use the concept of gravitational F=centripetal force[tex]=m\frac{v^2}{r}[/tex] and the fact that [tex]v=\frac{2\pi r}{T}[/tex]

so this is my attempt:

[tex]F_g=\frac{GMm}{r^2}=m(\frac{v^2}{r})[/tex]

implies [tex]\frac{GMm}{r^2}=\frac{m4\pi^2r}{T^2}[/tex]

implies [tex]M=\frac{4\pi^2r}{GT^2}[/tex]

Should this not work? or am I just putting these numbers into my calculator wrong. I have T in seconds=275405

Text says it is 6.5*10^23 kg

Casey

ps I am more concerned with learning the method here.
 
Last edited:
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You reasoning is fine just two small mistakes. Look at the radius in your final equation again and ask if it should be to that power, and calculate your time in seconds again.
 
Saladsamurai said:
The Martian satellite Phobos travels in an approx circular orbit with r=9.4*10^6 meters and period 7h 39min. Find the mass of mars.

I am supposed to use the concept of gravitational F=centripetal force[tex]=m\frac{v^2}{r}[/tex] and the fact that [tex]v=\frac{2\pi r}{T}[/tex]

so this is my attempt:

[tex]F_g=\frac{GMm}{r^2}=m(\frac{v^2}{r})[/tex]

implies [tex]\frac{GMm}{r^2}=\frac{m4\pi^2r}{T^2}[/tex]

implies [tex]M=\frac{4\pi^2r}{GT^2}[/tex]
You should have a factor r^3 on the RHS instead of r

Should this not work? or am I just putting these numbers into my calculator wrong. I have T in seconds=275405

Text says it is 6.5*10^23 kg

Casey

ps I am more concerned with learning the method here.
 
should it be r^3 ...I am messing up my algebra here...wow...
T=7h 39 min= (7*3600)+(39*60)=27540...dont know where that last 5 came from! Thanks

Casey
 
Last edited:
Yes. Go to the previous step and ask yourself how you move the r2 term from the left to the right.
 
Sorry for butting in-- I was rather late! Glad you've got it though, Casey :smile:
 
Kurdt said:
Yes. Go to the previous step and ask yourself how you move the r2 term from the left to the right.

Yeah, I'm a stooge. I treated the equals sign in this[tex]\frac{GMm}{r^2}=\frac{m4\pi^2r}{T^2}[/tex]
like it was a multiplication sign!

I love making up my own rules!

Casey
 
cristo said:
Sorry for butting in-- I was rather late! Glad you've got it though, Casey :smile:

Feel free to butt in anytime:wink:
 
Yeah, I'm a stooge. I treated the equals sign in this [tex]\frac{GMm}{r^2}=\frac{m4\pi^2r}{T^2}[/tex]

like it was a multiplication sign!

I love making up my own rules!

Casey
No problem. We've all made that mistake and we all will again unfortunately. :smile:
 
  • #10
Saladsamurai said:
should it be r^3 ...I am messing up my algebra here...wow...

If you solve your expression for T^2, you'll see that you've derived Kepler's Third Law for Mars, so you have that a check on your algebra. (I'm assuming you've seen Kepler's Law of Celestial Motion in your course by this point.)
 

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