Precession of the earth's axis

In summary, the Earth has a precessional movement due to the Sun and Moon's pull on the Equatorial Bulge. The Chandler wobble is also caused by the Earth's non-spherical nature.
  • #1
Ulysees
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I remember an analogy with a child's spinning top, that does not rotate in a fixed axis but the axis makes a precessional movement.

But the spinning top is sitting on something, it's getting a force from below that's not aligned with its weight, so this force has a torque, etc etc (can't continue cause I don't really know how to :biggrin:)

But the Earth is not like this, there's no force from the bottom. Why does it have a precession then?

Would there be no precession without the moon?
 
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  • #2
Both the Sun and Moon contribute to the precession of the Earth.

The Earth is not an homogeneous sphere. It has an equatorial bulge. It is the Sun's and Moon's pull on this bulge that leads to precession.
 
  • #3
The reason a spinning top precesses is because gravity and the normal force collectively exert a torque on the top. The Sun and Moon similarly exert a torque on the Earth due to the non-spherical nature of the Earth. The result is the precession of the Equinoxes.

There are some smaller effects on top of this large precession. The Moon has an 18.6 year nodal precession, and this couples with the non-spherical nature of the Earth to create an 18.6 cycle equinoctial precession on top of the lunisolar precession. To confuse things, astronomers call this equinoctial precession on other planets but nutation on the Earth.

For any non-spherical object, the angular velocity vector cannot be constant in a torque-free situation unless the angular velocity is perfectly aligned with one of the object's eigenaxes. The Earth undergoes a very small precession, the Chandler wobble, as a result.

A detailed model of the Earth's rotational motion is necessarily numerical. The IERS uses a rather ad-hoc model with several fitted parameters to describe the orientation of the Earth to the milliarcsecond level.
 
  • #4
D H said:
The Sun and Moon similarly exert a torque on the Earth due to the non-spherical nature of the Earth. The result is the precession of the Equinoxes.

Now that I thought of it it has occurred to me that it is not the gravity that causes the torque but the gravity gradient. In other words, in a homogeneous field there would be no torque, no matter the shape of the earth. Presumably the gradient from the strongest to the weakest solar gravity, over the extent of the earth, is just sufficient to make the 25000 year cycle. And the moon adds a much weaker cycle on top of it, right? And the equinoctial precession adds an even weaker cycle on top, and the Chandler precession yet another, right?

If we imagine the sphere of "the heavens" with the Earth in the centre, does the axis trace a circle due to the sun, and another circle due to the moon, and another circle due to the equinoctial cycle, and another circle due to the Chandler wobble, so they all add up to make something wobbly? The cycle due to the sun probably dominates, tracing its circle?

Maybe we can compare the solar and lunar gradients to get a rough idea and confirm if the sun dominates the lunisolar cycle or not.
 
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1. What is precession of the earth's axis?

Precession of the earth's axis is the gradual change in the orientation of the Earth's rotational axis, where the axis traces out a cone shape over a period of approximately 26,000 years. This means that the North Pole and South Pole do not always point in the same direction in space.

2. What causes the precession of the earth's axis?

The precession of the earth's axis is caused by the gravitational forces exerted on the Earth by the Sun, Moon, and other planets. These forces cause the Earth's rotational axis to wobble slightly, leading to the gradual change in its orientation over time.

3. How does precession impact the Earth's climate?

Precession has a small but significant impact on the Earth's climate. As the axis of the Earth changes, the amount of sunlight received by different parts of the Earth changes. This can affect the distribution of heat and can potentially lead to changes in climate patterns over time.

4. How is precession measured and tracked?

Precession is measured using astronomical observations, such as the position of stars, to determine the changes in the Earth's rotational axis. This data is then analyzed and used to track the changes in the axis over time.

5. Is precession a slow or fast process?

Precession is a slow process that occurs over a period of approximately 26,000 years. This means that the changes in the Earth's axis are not noticeable in a human lifetime, but can be observed over many generations.

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