# Can we measure the "Tilt-A-Whirl" effect of the Earth+Sun orbiting the galactic hub?

You've probably ridden on the fairground ride called the "Tilt-A-Whirl", or--as Disneyland calls it--the "Spinning Teacups", as well as other fairground rides that employ epicycles. You can really feel the centrifugal force strongly when your car spins complementary to the spin of the main rotor.

Now, can that extra force be measured on Earth as our orbit around the Sun complements the Sun's orbit around the galactic hub? Has anyone done it?

• Are you talking about tidal forces? Jan 10, 2011 at 0:01
• Centrifugal acceleration is $v^2 / r$. I suggest you plug in the relevant numbers. Short story: galactic distances are far too huge for that acceleration to be anything but negligible. Jan 10, 2011 at 0:16
• Mark: that didn't occur to me, but it sounds like an effect that could be measured. The Arabs built entire buildings to measure the tides precisely (by connecting vast tanks to the sea by tunnels, then marking a column that ran through the middle), and perhaps the fact of galactic orbit could be evidenced if the tidal levels coincided with predictions made by theory and astronomical observations. Of course, now I'm wondering if you could measure the effect by the moon's distance to Earth, too. Jan 10, 2011 at 0:33
• @Mark, not exactly, but ties are the only uncompensated term left after you realize that all the bodies involved are freely falling. Of course they go by $d\frac{m_1 m_2}{r^3}$ (where $d$ is the separation from the free-falling center), so that effect is even more trivial than Marek suggests. Jan 10, 2011 at 1:25