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D H said:And you didn't put that information on the table. That's what I was getting at.
I beg to differ:
Orodruin said:The relation is v = ωr. What does this tell you about the angular velocity if you keep v fixed and increase r?
Orodruin said:The angular momentum of the ball is conserved and given by mvr, where v is the horizontal component of the velocity. What does this tell you about the horizontal velocity as r increases? What does it tell you about the angular velocity?
I gave all of the information necessary for the OP to work this out for himself/herself rather than simply providing the answer.
Qualitatively, yes, your explanation does explain why there's a westward drift. Quantitatively, good luck. That's voko's approach. Invoking the concept of the Coriolis effect and assuming gravity doesn't vary with height and it's just a matter of high school level calculus to arrive at the quantitative result that the ball thrown straight up at the equator will land a distance d=\frac 4 3 \frac {\Omega v^3}{g} to the west.
If you reread the OP, you will see that it is not necessarily asking for a quantitative solution. I find it counter productive to meet a qualitative question of what happens and why with "there is this fictitious force in a rotating system", rather than trying to explain what is actually going on.
In addition, within your assumptions that the ball is not thrown to heights that require consideration of a varying g, it is also very easy to integrate the equations I supplied and arrive at the same result (assuming that your ##g## really should be ##g^2##, which is necessary to make the dimensions consistent):
Conservation of angular momentum gives:
$$
\omega(r) = \omega_0 \frac{r_0^2}{r^2} \simeq \omega_0 - 2 \omega_0 \frac {h(t)}{r_0}
\quad \Rightarrow \quad
\frac{d\phi}{dt} = \omega(r) - \omega_0 \simeq - 2 \omega_0 \frac {h(t)}{r_0}.
$$
Given that ##g## is constant
$$
h(t) = v t - \frac{gt^2}2.
$$
Integrating from 0 to ##2v/g## yields
$$
\phi = - \frac{4\omega_0 v^3}{3r_0 g^2}.
$$
Multiply with ##r_0## to get the distance rather than angle:
$$
d = - \frac{4\omega_0 v^3}{3 g^2}.
$$