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I'll start of with my (mis)understanding:

We have a planet orbiting around another body. The orbiting planet has infinitely many axes passing through it, but we're interested in two, $A_1$ and $A_2$. $A_1$ is the axis that is perpendicular to the planet's orbit, whereas $A_2$ is the one passing through its poles.

The planet is rotating around $A_1$. When $A_2$ is exactly superimposable onto $A_1$, then this is a rotation without precession. If $A_2$ is at an angle from $A_1$ however, we've got precession. Let's say that the point at the tip of $A_2$ is called $a_2$. When there is no nutation, $a_2$ orbits around $A_1$ in some elliptical path.

When there is nutation, then the that orbit is disturbed in a specific way. Let's define an abstract point, $p$, that orbits around $A_1$ identically to how $a_2$ would, if there was no nutation. So, the way I've understood nutation is that it's when $a_2$ orbits around $p$.

In the lower left, you see the orbit of $a_2$ around $p$ quite clearly. However, that is a contrived scenario where $p$ isn't moving. Thing is, $p$ is in orbit around $A_2$, which means that circle gets stretched out into a $2$D helix. We could make it into a $3$D helix by defining an axis $t$, and define integer values of $t$ as the time taken for $a_2$ to orbit around $p$ once. If you look at the first photo, that time step is demarcated onto the helix.

In this Math.SE post, I defined a function, $_rF_n(t)$, that gives us the coordinates that trace out the movement of $a_2$. It takes $t$ as the input, and outputs a two-dimensional value, corresponding to where $a_2$ exists at time $t$. If one looked at this function, it would be a $3$D helix. However, one could look at that $\Bbb R^3$ space in such a way so as to compress it into two dimensions. Basically, you position the observer's line of sight perpendicular to the $t$-axis (the $x$-axis in this photo). 2D helix

And this get's you the path traced out by a point orbiting around another point that is moving. The above picture was taken from user65203's answer to this Math.SE post. Now, in the second photo of this post, I defined $r$ as the distance between $a_2$ and $p$. Now, if $p$ moves a distance $\ge 2r$ per time step, that means that there will be no looping (by loops, I mean the loops you see in the above $2$D helix). When the velocity of $p$ exceeds $2r$ per time step $t$, you get a sinusoidal wave as the curve traced out by the movement of $a_2$. The reason is that $p$ moves too fast for $a_2$ to loop back on itself, for a lack of more precise wording. In other words, by the time $a_2$ has finished its orbit, $p$ has moved a distance of $2r$, thus meaning it has no chance of crossing over a point is has been before. To illustrate this, let me show the middle point between $n = 0$ and $n = 2r$, $n$ being the distance travelled by $p$ per time step $t$.

Here, $n = r$.


The question:

The thing is, whenever I look at pictures where nutation is illustrated, the path of $a_2$ never loops; it's sinusoidal (see this Wikipedia article for an example). So, that makes me think that nutation for some reason requires $n \ge 2r$. However, this belief is based on my current (mis)understanding. So, this leaves me with two questions:

  1. Is my understanding correct?
  2. If so, why is $n \ge 2r$?

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1 Answer 1

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I will give links to resources that I think will be of help to you.

(The stackexchange policy is that contributors should given standalone answers, using links only for corroboration. I support that policy, but writing a standalone answer here would be very time consuming.)

Experimental

Svilen Kostov and Daniel Hammer have conducted a tabletop experiment to verify experimentally that the onset of gyroscopic precession always involves nutation. (Generally the nutation dampens out quickly. Faster spin rate corresponds to faster nutation rate, and smaller nutation amplitude. In classroom demonstations: when the spin rate is fast the nutation generally goes unnoticed, and it rapidly dampens out.)

The title of their article is: It has to go down a little, in order to go around


Theoretical

There is a set of two articles by Eugene Butikov

About torque-free precession (also known as Feynman's wobbling plate):
Eugene Butikov "inertial rotation of a rigid body"

(I googled that title, and was able to obtain the article from the website researchgate.net, without having to create an account.)

Butikov points out that there is a particular way of representing the motion of torque-free precession geometrically. The motion of the axis of the wobbling body is moving in the way a cone rolls inside a wider cone.

The follow-up article applies the concepts laid out in the preceding article, presenting discussion of connection between nutation and precession:
Eugene Butikov "Precession and nutation of a gyroscope"

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