A "laboratory" frame of reference is one that is attached to the surface of the Earth, and so it rotates along with the Earth. Normally we regard a laboratory frame as truly inertial, in which Newton's laws of motion can be applied in their simplest form. We generally do only that, as any errors that occur as a result are almost always small enough to be completely negligible.
Back on 4 October 2014 I posted Figure 1 above, showing how an object in a laboratory frame at the Earth's equator is seen to move as measured in a truly inertial frame set at the center of the Earth. (The Earth's orbital motion is disregarded). From a macro like this, or just from the basic physics involved, results can be derived for the upwards displacement and velocity for a truly inertial "weightless" mass initially placed on the equator (Fig 2). I used values of 0.00007292115 radians/sec for the Earth's rotational velocity, and 6,378,137 meters for its equatorial radius.
An observer in a laboratory frame who stays attached to the Earth would see the weightless mass rise upwards, and drift to the West, slowly at first, then ever more rapidly.
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Fig 2. Spreadsheet of data for a weightless mass "floating" up from a point on the Earth's equator. |
Energy extraction?
From Figure 2, if a weightless mass rises upwards at the equator for say 5 seconds, it could then impact at a velocity of 0.16958 m/s against any structure fastened to Earth, after having risen through a distance of 0.423946 m. If the mass was say 10kg, that impact would deliver
½ × 10 × 0.16958² = 0.14379 joules of energy. Could we really do that?
There are two problems:— achieving a weightless mass, and returning it back to the Earth's surface. The first could be easily solved e.g. with a constant-force spring from the mass to the earthed structure, but the second problem is much harder, if we hope to gain energy overall. We must distinguish carefully between a mass that is made weightless in a laboratory frame, which could be returned to the Earth's surface with no energy penalty, and one that is weightless in a truly inertial frame, which is required here. The latter would inevitably give an energy penalty equal to the centrifugal force caused by Earth's rotation (i.e. 0.033916 Newtons/kilogram at the equator) multiplied by the distance required to return it.
In the above case we would have a penalty of
0.033916 N/kg × 10 kg × 0.423946 m = 0.14379 N-m = 0.14379 joules.
So the energy gained equals the energy lost, and this particular idea is ruled out.
I think that anyone who looks seriously into the idea of extracting energy from the rotating Earth will soon become as familiar with that figure of 0.033916 N/kg for equatorial centrifugal force as they probably already are with 9.80665 N/kg for (standard) gravitational force! (Assuming they site their thought experiments and models at the equator, as I always do).
[Postscript] — Calculation
The centrifugal force caused by Earth's rotation on a 1kg mass at the equator can be calculated thus:—
Centrifugal force = mω²r = 1 × 0.00007292115² × 6378137 = 0.033916 N
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