Understanding Planetary Motion: Correcting a Common Misconception

AI Thread Summary
The discussion revolves around the formula for planetary motion derived from Kepler's third law, specifically addressing a perceived error in the original equation. The formula in question is (T_A/T_G)^2=(R_A/R_B)^3, where T represents the period and R the radius of the planets. The user suggests that T_G, representing Kepler's constant, may be incorrectly applied, and proposes that the correct form should be (T_A/T_B)^2=(R_A/R_B)^3 when comparing two planets of the same mass. This correction aligns with the principle that the square of the period is proportional to the cube of the radius. The discussion emphasizes the importance of accurately applying Kepler's laws in understanding planetary motion.
mormreed
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I just need an explanation of a formula, and I think part of it is wrong, so here is the formula:

(T_A/T_G)^2=(R_A/R_B)^3


so T is the period and T_A is the period of planet A
then below it is what I think is wrong, T_G G is the Kepler's constant, I'm not sure what that really is
=
[text]R_A[/tex] which is radius of planet A over radius of planet B cubed, this side is right, any help is appreciated thanks
 
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I comes from Kepler's third law which states that

T^2 \propto R^3


So if two planets have the same mass, in your case planet A and G.

then T_A^2= k R_A^3 and T_G^2= kR_G^3

so just divide them and you'll get the formula
 
I think I found the answer after some searching, which I did try before which brought me here, but I think it is (T_A/T_B)^2=(R_A/R_B)^3
 
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