Earth's Rotation: Slowing Down?

In summary, the rotation of the Earth is slowing down due to a transfer of rotational momentum to the Moon's orbital momentum caused by tidal resistance. The period of rotation is increasing by 2 milliseconds per century. However, this change is also affected by internal changes in the Earth's inertia tensor, which can vary over shorter periods of time. The effect of tidal interactions on the Sun's rotation is negligible.
  • #1
Bjarne
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How fast is the rotation of the Earth slowing down ?
 
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  • #2
The period of rotation increases by 2 milliseconds per century.
 
  • #3
Janus said:
The period of rotation increases by 2 milliseconds per century.

Due to tidal resistance right ?
 
  • #4
What about the Suns rotation, do we know anything about that period too is increasing?
 
  • #5
it is due to a transfer of Earth's rotational momentum to the Moon's orbital momentum as tidal friction slows the Earth's rotation. for the sun, I believe it is the same.
 
  • #6
Janus said:
The period of rotation increases by 2 milliseconds per century.
Perhaps a bit misleading. For example, the length of a day decreased by 3.35 milliseconds over the last century. The excess length of day was 0.36 milliseconds for 2009, 3.71 milliseconds for 1909. Before you accuse you of cherry-picking: Guilty as charged. Excess length of day peaked in 1910.

The Earth's rotation rate also varies because of internal changes in the Earth. Over the short term (short here meaning hundreds or even thousands of years), these internal changes swamp the small but steady change due to transfer of angular momentum to the Moon's orbit. These internal changes arise from changes in the Earth's inertia tensor. They do not change the Earth's angular momentum. Over the long haul these internal changes average out to a null effect. The change in the Earth's rotation due to transfer of angular momentum to the Moon's orbit is a secular effect. Over millions of years or longer this is the only effect that stands out.

As far as the Sun goes, that effect is negligible. While tidal forces are inversely proportional to the cube of distance, the change in rotation rate due to tidal interactions is inversely proportional to distance6.
 

1. How does Earth's rotation slow down?

Earth's rotation is primarily slowed down by the tidal forces of the Moon and Sun. As these celestial bodies exert gravitational forces on the Earth, they cause the oceans to bulge out towards them. This creates a drag on the Earth's rotation, slowing it down over time.

2. How long does it take for Earth's rotation to slow down?

The exact amount of time it takes for Earth's rotation to slow down is not consistent, as it is affected by various factors such as the composition of the Earth's core and the distribution of landmasses. However, on average, Earth's rotation slows down by about 17 milliseconds every 100 years.

3. What are the effects of Earth's rotation slowing down?

As Earth's rotation slows down, the length of each day increases. This can have significant effects on the Earth's climate and weather patterns, as well as on the behavior of living organisms that rely on daylight for their daily activities. Additionally, the slowing of Earth's rotation can also cause changes in the Earth's magnetic field and potentially impact the accuracy of GPS systems.

4. Is there anything that can be done to prevent or reverse Earth's rotation from slowing down?

At this time, there is no known way to prevent or reverse Earth's rotation from slowing down. However, some scientists have proposed the idea of using large-scale engineering projects to artificially speed up the Earth's rotation. However, the feasibility and potential consequences of such projects are still being studied.

5. Will Earth's rotation eventually stop completely?

No, Earth's rotation will not stop completely. As long as the Earth continues to orbit the Sun, it will continue to rotate. However, it is possible that Earth's rotation could eventually become synchronized with its orbit around the Sun, resulting in one side of the Earth always facing the Sun (similar to how the Moon always shows the same face to the Earth).

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