Earth's Rotation & g-Force Effects

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Discussion Overview

The discussion revolves around the effects of Earth's rotation on the apparent value of gravitational acceleration (g) at its surface, particularly considering the hypothetical scenario of the Earth stopping its rotation. Participants explore both direct and indirect influences of rotation on g, including centripetal acceleration and the Earth's shape.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants propose that the force of gravity would remain unaffected, but the apparent value of g might increase slightly due to the absence of centripetal acceleration.
  • Others argue that while the effect of rotation on g is small, it could be measurable through simple experiments, referencing historical observations of pendulum clocks running slower near the equator.
  • A participant explains that the Earth's rotation contributes to its oblate spheroid shape, and if the Earth were to stop rotating, it would likely relax to a spherical shape, affecting the distribution of g across different latitudes.
  • One participant provides specific formulae for calculating g at sea level, noting that the apparent gravitational acceleration would increase for latitudes less than 61.381° and decrease for more extreme latitudes.

Areas of Agreement / Disagreement

Participants express varying views on the effects of Earth's rotation on g, with no consensus reached regarding the magnitude or implications of these effects. Some agree on the basic principles but differ in their interpretations and conclusions.

Contextual Notes

Participants reference historical debates and observations, indicating that the discussion is informed by both theoretical and experimental perspectives. There are unresolved assumptions regarding the implications of the Earth's shape and the exact measurements of g.

Who May Find This Useful

This discussion may be of interest to those studying physics, particularly in the areas of gravitation, rotational dynamics, and geophysics, as well as individuals curious about the implications of Earth's rotation on physical phenomena.

phymatter
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if the Earth stops rotating , what will happen to the apparent value of g on its surface ?
 
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The force of gravity would be unaffected I believe. Without the rotation you might be able to measure a slightly higher amount of G on stationary objects on the ground since the surface isn't rotating anymore, but the amount would probably be negligible.
 
Drakkith said:
The force of gravity would be unaffected I believe. Without the rotation you might be able to measure a slightly higher amount of G on stationary objects on the ground since the surface isn't rotating anymore, but the amount would probably be negligible.

If you dropped something, it would have a slightly higher acceleration downward, because there would be no centripetal acceleration.
 
Drakkith said:
The force of gravity would be unaffected I believe. Without the rotation you might be able to measure a slightly higher amount of G on stationary objects on the ground since the surface isn't rotating anymore, but the amount would probably be negligible.

The effect is small but big enough measure with simple experiments. The early global explorers found that their pendulum clocks ran slower as they traveled towards the equator. The change in length of a pendulum with a period 1 second is a few mm, between the poles and the equator.

There was considerable debate as to the cause of this (one hypothesis was that gravity was temperature-dependent) before Newton sorted out the math.
 
Just like i thought then. :biggrin:
 
phymatter said:
if the Earth stops rotating , what will happen to the apparent value of g on its surface ?
The Earth's rotation affects g in two ways. Directly, g includes a centrifugal acceleration term. This will vanish should the Earth stop rotating, thereby increasing the apparent value of g except at the poles. Indirectly, the Earth's rotation makes the Earth have a shape of an oblate spheroid. The Earth would presumably relax to a spherical shape should the Earth stop rotating. This would bring equatorial regions closer to the center of the Earth but make polar regions move further from the center of the Earth.

Assuming the Earth's volume remains constant while it relaxes toward this spherical shape, the radius of the Earth would become a uniform 6371.0008 km sometime after the Earth stopped rotating. The product G*Mearth=398,600.4418 km3/s2 would remain unchanged (mass isn't lost), so g would become 9.82024802 m/s2 for all points on the new surface of the Earth at sea level.

A couple of formulae for computing the apparent value of g at sea level (with the Earth still rotating) are the 1967 Geodetic Reference System Formula

g_0 = 9.780327\,\left(1+0.0053024\sin^2\phi-0.0000058\sin^2(2\phi)\right)\,\frac{\mbox{m}}{\mbox{s}^2}

and the World Geodetic System 1984 equation

g_0 = 9.7803267714\,\frac{1+0.00193185138639\sin^2\phi}{\sqrt{1-0.00669437999013\sin^2\phi}}\,\frac{\mbox{m}}{\mbox{s}^2}

To seven places, both formulae yield an acceleration of 9.820248 at a latitude of 61.381°.Bottom line: Should the Earth stop rotating the apparent gravitational acceleration would increase for latitudes less than 61.381° but decrease for more extreme latitudes.
 

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