Calculating Jupiter's Mass from Log10(a) vs Log10(P) Graph

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The discussion focuses on calculating Jupiter's mass using a log10(a) vs log10(P) graph of its satellites. The user has created the graph and identified a trend line with a slope of 3/2 but is unsure how to derive Jupiter's mass from it. They attempted to use the equation m1+m2=(4*P^2*a^3)/(G*P^2) with Io's values but encountered issues with large results that didn't utilize the graph. A correction was provided, indicating the correct form of the equation should be m1+m2=(4*π^2*a^3)/(G*P^2). The discussion emphasizes the importance of rearranging Kepler's equation and correctly applying logarithmic properties for accurate calculations.
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my problem involves creating a graph of log10(a) vs log10(P) of the Galilean satellites and 3 others, then calculate the mass of Jupiter from the graph. P= period of the satelite, a is the semi-major axis

I have created the graph and it seems to be right since the of the trend line is 3/2. My problem is that I am unsure how to go about calculating the mass from the graph.

to get the equation y = 1.5012x - 8.1973

I have tried using m1+m2= (4*P^2*a^3)/(G*P^2)G being the universal gravitational constant 6.67206 x 10-11 m3/kg s2. I used P and A values of Io. unfortunately that produced a rather large value and doesn't utilize the graph at all.

Any help or nudges in the right direction would be greatly appreciated, Thanks!
 
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You can neglect the masses of the satellites I think, since Jupiter is so much more massive than its satellites. Remember that the gradient is just effectivelylog_{10}(a) / log_{10}(p).
Start by rearranging the kepler equation so you can the gradient part on one side, then take the log remembering log_b(x^y) = ylog_b(x)

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bemc said:
I have tried using m1+m2= (4*P^2*a^3)/(G*P^2)

You have miscopied the equation. That is not the Kepler law equation. You should have written
m1+m2= (4*PI^2*a^3)/(G*P^2)

where PI stands for the number 3.14...
 

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