
Malcolm C.
asked 01/17/20What is the ratio of the speeds v1/v2?
Two satellites of masses m1 and m2 orbit a planet of mass M in circular orbits. The satellites travel in opposite directions with speeds v1 and v2. Their orbital radii are R1 and R2, respectively. Assume M>>m2>m1.
I know the answer is = square root(R2/R1)
But I don't know why.
1 Expert Answer

Daniel R. answered 01/17/20
Physics and Math are my specialties
This is tricky but with this problem you want to guess what kind of problem it's going to be to know where to start. We always want to start by writing down what we are given (even if there are no numbers).
We have
m1 m2 M R1 R2 v1 and v2
Now the key to what they gave in the problem is Circular Orbits which means that we can use the centripetal force equation. let's do that for satellite 1
Fc = m1 v12/R1
The centripetal force is equal to the net force on a moving satellite which is just the gravitational force
Fg = G M m1/R12
Now let's set them equal
Fc = Fg
m1 v12/R1 = G M m1/R12
Now let's pick out things we can cancel on either side, there's m1 and R1 on both sides so let's cancel these to get:
v12= G M /R1
Now let's rearrange this equation to get just G M on one side:
v12 R1 = G M
Now we can do the same exact steps with satellite 2 and we get:
v22 R2 = G M
Now these are both equal to G M so lets just set the left sides of our two equations equal to one another:
v12 R1 = v22 R2
Next we rearrange this to get
v12/v22 = R2/R1
Now we can square root both sides to get our solution:
v1/v2 = SQRT(R2/R1)
This is our solution, the part about opposite directions was just there to throw us off and make us think it's a momentum problem when in fact it is just a centripetal force problem
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Stanton D.
Try this relationship: for an object under gravitational attraction, a (acceleration) = G (universal gravitational constant) * M (mass of central body)/r (distance from central body)^2 [because mass of the object "drops out" from numerator and denominator]. Also, for an object in circular orbit, a (acceleration) = v (velocity)^2 / r (distance from central body) . So equate these two expressions for each object, and calculate the desired ratio of the question. Note that since the individual a's have disappeared, and the G's cancel, you have only functions of v's and r's in your ratio calculation. Good luck, -- Cheers, -- Mr. d.01/17/20