What is the Orbital Period of Jupiter in Earth Years?

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Homework Help Overview

The discussion revolves around calculating the orbital period of Jupiter in Earth years, utilizing Kepler's Third Law of planetary motion. The original poster attempts to apply the formula T^2 = Kr^3, where they express confusion regarding the use of planetary radii versus orbital radii.

Discussion Character

  • Conceptual clarification, Assumption checking

Approaches and Questions Raised

  • Participants explore the application of Kepler's Third Law, questioning the necessity of using the physical radii of the planets instead of their orbital distances. There is a discussion about the correct interpretation of the variables in the equation.

Discussion Status

Some participants suggest alternative approaches to the problem, indicating that using the orbital distances rather than the physical radii may lead to a correct solution. There is acknowledgment of differing interpretations regarding the variables involved.

Contextual Notes

The original poster expresses uncertainty about the requirement to use the radii of the planets and the implications of treating planets as point masses in this context.

petern
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Jupiter is 5.2 times farther than Earth from the sun. Find Jupiter's orbital period in Earth years.

Equation to use is: T^2 = Kr^3

Radius of Earth is 6378100 m and radius of Jupiter is 71492000 m.

I rearrange the equation to K = T^2/r^3 and set k of Earth equal to k of Jupiter. I enter all of it including 5.2 times radius of Earth into the equation. I solve for t of Jupiter but I always end up with 16.457 years when it should be 11.86 years. What am I doing wrong?
 
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Can anyone help me?
 
petern said:
Radius of Earth is 6378100 m and radius of Jupiter is 71492000 m.

I rearrange the equation to K = T^2/r^3 and set k of Earth equal to k of Jupiter. I enter all of it including 5.2 times radius of Earth into the equation. I solve for t of Jupiter but I always end up with 16.457 years when it should be 11.86 years. What am I doing wrong?

I don't know where you got those radii from, but you don't need them.

Use 1 Earth year as T (earth) and 1 Earth orbit as R (earth). Use 5.2 Earth orbits as R (jupiter).

Plug these into T(earth)^2 / R(earth)^3 = T(jupiter)^2 / R(jupiter)^3

and solve for T(jupiter).
 
Last edited:
Thanks. Looks like it works but the only problem is that I know that I have to use the radii of the planets which is from the center to the edge of the planet. r stands for radius, not orbit so I don't understand why that's working.
 
The r stands for radius of an orbit, considered circular, not the radius of a planet! All planets are considered to be point masses in this treatment.
 

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