Solving Problem 9: Smaller than Any of the Choices?

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Homework Help Overview

The discussion revolves around a problem related to orbital mechanics, specifically involving the application of Kepler's Laws to determine relationships between orbital period and radius for celestial bodies.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • The original poster attempts to solve a problem but is uncertain about assuming a circular orbit and questions potential errors in their work. Participants discuss the application of Kepler's Laws, particularly whether to use the orbital period and radius of one moon to find the mass of a planet.

Discussion Status

Participants are actively engaging in clarifying the application of Kepler's Laws, with some guidance provided on how to approach the problem without needing to solve for the planet's mass. There is a productive exchange regarding the use of ratios derived from the data of one moon to analyze another.

Contextual Notes

There is mention of specific data related to "moon II" and "moon III," which may be relevant to the calculations but are not detailed in the discussion.

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Homework Statement


see problem 9 attachment


Homework Equations


see problem 9 attempt attachment


The Attempt at a Solution


I come up with a solution that is much smaller than any of the choices. I do not know if I am to assume the orbital is circular. I do not know if there is another error besides that in my work.
 

Attachments

  • 1031-10871-problem 9.jpg
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  • 2899-33757-problem 9 attempt.jpg
    2899-33757-problem 9 attempt.jpg
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Hello,

You need not assume that the orbit is circular. Use one of Kepler's Laws (which applies for both circular and elliptical orbits).
 
ok if I use kepler's third law would I start by using moon II orbital period and radius to solve for the mass of the planet?
 
You don't need to solve for the planet's mass. Remember that R^3 is proportional to T^2, and that must hold for all objects orbiting a body. Hence R^3/T^2 = constant.
 
ok so I can find that ratio from moon II data and then multiply that ratio by T^2 of moon III?
 
yup, that is right
 
thank you for your help
 

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