Physics Asked by π times e on June 25, 2021
Let’s say an object is at rest in Earth’s reference frame. We know that Earth’s reference frame is non inertial. If we were to observe that object from an inertial frame, we would see three forces acting on it (ignoring resistive forces like air drag, etc). The three forces are gravity $mg$, Normal reaction $N$, and a 3rd force which imparts a centripetal acceleration to the object which makes it spin (along with the Earth). Which force provides that centripetal acceleration? Is it friction or some other force?
Edit : Ignoring Earth’s revolution around the Sun in this case and just taking into account its spin about its axis of rotation
The details of this setup depend on where on earth you are.
On either of the geographical poles, the object would simply spin around its axis along with earth, no centripetal force occurs. On the equator, the centripetal force keeping it on the earth and making it spin along with it is purely gravity. The centrifugal (apparent) force is pointing straight up, gravity is pointing straight down. A stationary object on the surface will experience a much greater gravitational force than centrifugal force, so the object stays on the ground and spins along with the earth.
The situation is a bit more complicated anywhere in between these points. I will describe the abstract situation in which the earth is a perfect sphere. Other answers also address its actual oblate geometry.
Between the poles and the equator, gravity is pointing straight down, but the centrifugal force is pointing outwards perpendicular to the rotational axis. This means, standing on the ground, the centrifugal force is pointing diagonally up, where its horizontal component (the one parallel to the surface) is directed at the closest point on the equator (or, equivalently, the more distant pole). The vertical component is again cancelled by gravity, but the horizontal part would have to be compensated by some frictional force. If the earth was a perfect sphere with a frictionless surface, all objects left alone on it would collect at the equator. As other answers correctly point out, this effect is counteracted by the oblate shape of the actual earth.
Answered by noah on June 25, 2021
The diagram below depicts the source of the centripetal force.
Every rotating celestial body that is large enough to pull itself into an energy minimizing shape has an equatorial bulge. (Over geologic time scale the solid rock of the Earth's tectonic plates is ductile. )
The diagram shows a celestial body with a far larger equatorial bulge than the Earth; for clarity the equatorial bulge is exaggerated.
Any buoyant object is subject to a normal force (red arrow).
When a celestial body has an equatorial bulge the gravitational force is not exactly opposite in direction to the normal force. So there is a resultant force. From here on I will refer to that resultant force as the poleward force.
In the case of the Earth: polar radius is 6357 kilometer, equatorial radius is 6378 kilometer. The difference is 21 kilometer.
This means that from the equator to the pole is a downhill slope. If that slope would not be there then the water of the Earth would flow to the Equator. The Earth's equatorial bulge prevents that.
Example: at 45 degrees latitude the slope is 0.1 degree. That slope provides the required centripetal force to remain co-rotating with the Earth. At 45 degrees, to find the amount of required centripetal force you divide by 580, that is the ratio.
Divide your own weight by 580, that is how much centripetal force is required for you (at 45 degrees latitude). If you have a weighing utensil you can push: that will give you a feel for it.
I noticed that other answers suggest that the required centripetal force is provided by friction. That is a whopping mistake.
70 percent of the Earth's surface is ocean, and it is not the case that the oceans are deeper at the equator. There are differences in ocean depth, but they are not correlated with latitude.
For the water in the oceans there is no friction available. The oceans are the same depth at the equator because the equatorially bulged shape of solid Earth provides just the right amount of poleward force.
About the process that arrived at the current equatorial bulge:
Prior to formation the material that was about to form the Earth was distibuted in the form of a proto-planetary disk. As the planet formed the blob of material became more and more spherical. Geologists have reconstructed that shortly after formation the rotation period of the Earth was about 6 hours; 4 times faster than today.
When a forming celestial body contracts to a more spherical form there is release of gravitational potential energy. That gravitational potential energy turns into rotational kinetic energy. That is: the contraction tends to speed up the rate of rotation. At some point the celestial body cannot contract further, as that would cost more energy than would be released.
Tidal interactions with the Moon have been slowing down the Earth's rotation thoughout the Earth's existence. Over geologic time scale the Earth as a whole is sufficiently ductile to act effectively as a fluid. A very, very viscous fluid, but fluid. For more on that: see the pitch drop experiment
In celestical mechanics the shape of a rotating celestial body is referred to as 'hydrostatic equilibrium'. With hundreds of millions of years available to adjust a celestial body has the same shape as a celestial body that is entirely an easy flowing fluid.
Answered by Cleonis on June 25, 2021
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