How Do You Calculate Orbital Period with Limited Data?

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SUMMARY

The discussion focuses on calculating the orbital period of Moon I using limited data, specifically its orbital radius of 5E7 meters. Participants emphasize the application of Kepler's Third Law to establish a ratio between the orbital periods of Moon I and Moon II, which has known period and radius information. The consensus is that the orbital period of Moon I is approximately 1.24 x 10^5 seconds, derived from the established ratios. The conversation highlights the importance of understanding orbital mechanics and the assumptions regarding planetary mass.

PREREQUISITES
  • Understanding of Kepler's Laws of planetary motion
  • Basic knowledge of gravitational force equations
  • Familiarity with orbital mechanics terminology
  • Ability to manipulate ratios and solve equations
NEXT STEPS
  • Study Kepler's Third Law in detail
  • Learn how to calculate gravitational force using Newton's Law of Universal Gravitation
  • Explore the relationship between orbital radius and period in celestial mechanics
  • Investigate the mass of celestial bodies and its impact on orbital dynamics
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Astronomy students, physics enthusiasts, and anyone interested in celestial mechanics and orbital calculations will benefit from this discussion.

blackbyron
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Homework Statement


An Earth station receives data transmitted back in time from a future intergalactic expedition. The table summarizes the data for the moons of a planet that will be discovered in a distant galaxy.


Moon 1: only has orbital radius = 5E7 meters
Just only this information.


Question: the orbital period of Moon I is closest to:

Homework Equations


Using Kelpers Law

Force = GMeM/R^2


The Attempt at a Solution



How do I find out the orbital period if I don't know that acceleration, and the mass, and what's the difference between radius and orbital radius? I just don't understand what to do.
 
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hi blackbyron! :smile:

what are the possible answers?

my guess is that you're expected to assume that the planet's mass is somewhere between Mercury's and Jupiter's
 
Hi, tiny-tim, thanks for your reply.

No, I don't believe the moon on the mass has something to do with mercury and jupiter.
It only talks about the 3 moons.

Here is the table, that might make sense to you.


1zf1qx5.jpg







The possible answer is 1.2 *10^5s. Not sure if that asks you a question.
 
You have period and radius information for Moon II. You could use Kepler's 3rd law to solve for the orbital period of Moon I by setting up the appropriate ratios.
 
ohhh :rolleyes:

then can't you find the orbital period of moon I from the orbital period of moon II ?
 
@tiny-tim
hmm, I probably would give it a try, but I don't know if I'm going to to do it right. haha

gneill said:
You have period and radius information for Moon II. You could use Kepler's 3rd law to solve for the orbital period of Moon I by setting up the appropriate ratios.
Alright, so I use the ratio of Time to solve for time 2 using the Kepler's 3rd law.

So For example,

Tm1/Tm2 = kepler's third law?
m1 = moon 1
m2 = moon 2

Is that right?
 
I think I got it. Finding out the ratio of Tm1/Tm2 gives me the right answer.

So, I think I did it right. My answer is 1.24e5. Do you guys agree? :)
 
The value looks fine.
 
Thank you so much guys. It's very helpful.
 

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