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

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To calculate the mass of Mars using Phobos' orbit, the gravitational force equation must be equated to centripetal force. The correct formula involves the radius cubed (r^3) rather than squared (r^2) when rearranging the equation. The orbital period must also be accurately converted to seconds for precise calculations. The expected mass of Mars is approximately 6.5 x 10^23 kg, which serves as a benchmark for verifying calculations. Understanding these principles is crucial for mastering the method of calculating planetary masses.
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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=centripital force=m\frac{v^2}{r} and the fact that v=\frac{2\pi r}{T}

so this is my attempt:

F_g=\frac{GMm}{r^2}=m(\frac{v^2}{r})

implies \frac{GMm}{r^2}=\frac{m4\pi^2r}{T^2}

implies M=\frac{4\pi^2r}{GT^2}

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.
 
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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=centripital force=m\frac{v^2}{r} and the fact that v=\frac{2\pi r}{T}

so this is my attempt:

F_g=\frac{GMm}{r^2}=m(\frac{v^2}{r})

implies \frac{GMm}{r^2}=\frac{m4\pi^2r}{T^2}

implies M=\frac{4\pi^2r}{GT^2}
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
 
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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\frac{GMm}{r^2}=\frac{m4\pi^2r}{T^2}
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 \frac{GMm}{r^2}=\frac{m4\pi^2r}{T^2}

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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