What we have:
PαM⋅a where P is period, M is mass, and a is the separation of a two-body gravitational orbit.
What we know:
Because gravity is involved, we know G will be used, which is G=6.67x10−12cm3gs2.
We also know the units:
Period: T (time), M: M (mass), a: L (distance) and finally G: L3MT2 (a combination of the three).
So we can set up a dimensional analysis problem with only the exponents to work out:
Pw=Mx⋅ay⋅Gz→Tw=Mx⋅Ly⋅(L3MT2)z
For the units of time (T) to balance out on both sides of the equation, w must equal 2 and z must equal -1. With this inversion, for the units for distance to work out (L), y must equal 3. And finally, for mass to cancel (M), x must equal -1.
In conclusion, w=2, x=-1, y=3, and z=-1, which when put back into the first equation gives:
P2=M−1⋅a3⋅G−1
which cleans up to:
P2=a3M⋅G
All done!
P.S. Because I do not live on a desert island, I looked up the formula for Kepler's law:
P2=4π2a3MG
and I was only off by a constant!
Many thanks to Sean and Eden for working on this worksheet with me.
This is nice walk-through of the problem. And you missed a π. They are sneaky. They are fun because radians are technically dimensionless (you can take the sin of unit), so that are hard to find with dimensional analysis. Can you think of why it's 4π2 or (hint, hint) (2π)2)?
ReplyDeleteI fixed the pi. This makes sense because we are finding period over an entire circle, so the equation is really (P2π)2=a3M⋅G which simplifies to the final equation.
ReplyDelete