Precession
Precession is a change in the orientation of the rotational axis of a rotating body. In an appropriate reference frame it can be defined as a change in the first Euler angle, whereas the third Euler angle defines the rotation itself. In other words, if the axis of rotation of a body is itself rotating about a second axis, that body is said to be precessing about the second axis. A motion in which the second Euler angle changes is called nutation. In physics, there are two types of precession: torquefree and torqueinduced.
In astronomy, precession refers to any of several slow changes in an astronomical body's rotational or orbital parameters. An important example is the steady change in the orientation of the axis of rotation of the Earth, known as the precession of the equinoxes.
Contents
Torquefree
Torquefree precession implies that no external moment (torque) is applied to the body. In torquefree precession, the angular momentum is a constant, but the angular velocity vector changes orientation with time. What makes this possible is a timevarying moment of inertia, or more precisely, a timevarying inertia matrix. The inertia matrix is composed of the moments of inertia of a body calculated with respect to separate coordinate axes (e.g. x, y, z). If an object is asymmetric about its principal axis of rotation, the moment of inertia with respect to each coordinate direction will change with time, while preserving angular momentum. The result is that the component of the angular velocities of the body about each axis will vary inversely with each axis' moment of inertia.
The torquefree precession rate of an object with an axis of symmetry, such as a disk, spinning about an axis not aligned with that axis of symmetry can be calculated as follows:^{[1]}
where ω_{p} is the precession rate, ω_{s} is the spin rate about the axis of symmetry, I_{s} is the moment of inertia about the axis of symmetry, I_{p} is moment of inertia about either of the other two equal perpendicular principal axes, and α is the angle between the moment of inertia direction and the symmetry axis.^{[2]}
When an object is not perfectly solid, internal vortices will tend to damp torquefree precession, and the rotation axis will align itself with one of the inertia axes of the body.
For a generic solid object without any axis of symmetry, the evolution of the object's orientation, represented (for example) by a rotation matrix R that transforms internal to external coordinates, may be numerically simulated. Given the object's fixed internal moment of inertia tensor I_{0} and fixed external angular momentum L, the instantaneous angular velocity is
Precession occurs by repeatedly recalculating ω and applying a small rotation vector ω dt for the short time dt; e.g.:
for the skewsymmetric matrix [ω]_{×}. The errors induced by finite time steps tend to increase the rotational kinetic energy:
this unphysical tendency can be counteracted by repeatedly applying a small rotation vector v perpendicular to both ω and L, noting that
Another type of torquefree precession can occur when there are multiple reference frames at work. For example, Earth is subject to local torque induced precession due to the gravity of the sun and moon acting on Earth's axis, but at the same time the solar system is moving around the galactic center. As a consequence, an accurate measurement of Earth's axial reorientation relative to objects outside the frame of the moving galaxy (such as distant quasars commonly used as precession measurement reference points) must account for a minor amount of nonlocal torquefree precession, due to the solar system’s motion.
Torqueinduced
Torqueinduced precession (gyroscopic precession) is the phenomenon in which the axis of a spinning object (e.g., a gyroscope) describes a cone in space when an external torque is applied to it. The phenomenon is commonly seen in a spinning toy top, but all rotating objects can undergo precession. If the speed of the rotation and the magnitude of the external torque are constant, the spin axis will move at right angles to the direction that would intuitively result from the external torque. In the case of a toy top, its weight is acting downwards from its center of mass and the normal force (reaction) of the ground is pushing up on it at the point of contact with the support. These two opposite forces produce a torque which causes the top to precess.
The device depicted on the right (or above on mobile devices) is gimbal mounted. From inside to outside there are three axes of rotation: the hub of the wheel, the gimbal axis, and the vertical pivot.
To distinguish between the two horizontal axes, rotation around the wheel hub will be called spinning, and rotation around the gimbal axis will be called pitching. Rotation around the vertical pivot axis is called rotation.
First, imagine that the entire device is rotating around the (vertical) pivot axis. Then, spinning of the wheel (around the wheelhub) is added. Imagine the gimbal axis to be locked, so that the wheel cannot pitch. The gimbal axis has sensors, that measure whether there is a torque around the gimbal axis.
In the picture, a section of the wheel has been named dm_{1}. At the depicted moment in time, section dm_{1} is at the perimeter of the rotating motion around the (vertical) pivot axis. Section dm_{1}, therefore, has a lot of angular rotating velocity with respect to the rotation around the pivot axis, and as dm_{1} is forced closer to the pivot axis of the rotation (by the wheel spinning further), because of the Coriolis effect, with respect to the vertical pivot axis, dm_{1} tends to move in the direction of the topleft arrow in the diagram (shown at 45°) in the direction of rotation around the pivot axis.^{[3]} Section dm_{2} of the wheel is moving away from the pivot axis, and so a force (again, a Coriolis force) acts in the same direction as in the case of dm_{1}. Note that both arrows point in the same direction.
The same reasoning applies for the bottom half of the wheel, but there the arrows point in the opposite direction to that of the top arrows. Combined over the entire wheel, there is a torque around the gimbal axis when some spinning is added to rotation around a vertical axis.
It is important to note that the torque around the gimbal axis arises without any delay; the response is instantaneous.
In the discussion above, the setup was kept unchanging by preventing pitching around the gimbal axis. In the case of a spinning toy top, when the spinning top starts tilting, gravity exerts a torque. However, instead of rolling over, the spinning top just pitches a little. This pitching motion reorients the spinning top with respect to the torque that is being exerted. The result is that the torque exerted by gravity – via the pitching motion – elicits gyroscopic precession (which in turn yields a counter torque against the gravity torque) rather than causing the spinning top to fall to its side.
Precession or gyroscopic considerations have an effect on bicycle performance at high speed. Precession is also the mechanism behind gyrocompasses.
Classical (Newtonian)
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Precession is the change of angular velocity and angular momentum produced by a torque. The general equation that relates the torque to the rate of change of angular momentum is:
where and are the torque and angular momentum vectors respectively.
Due to the way the torque vectors are defined, it is a vector that is perpendicular to the plane of the forces that create it. Thus it may be seen that the angular momentum vector will change perpendicular to those forces. Depending on how the forces are created, they will often rotate with the angular momentum vector, and then circular precession is created.
Under these circumstances the angular velocity of precession is given by:^{[citation needed]}
where I_{s} is the moment of inertia, ω_{s} is the angular velocity of spin about the spin axis, m is the mass, g is the acceleration due to gravity and r is the perpendicular distance of the spin axis about the axis of precession. The torque vector originates at the center of mass. Using ω = 2π/T, we find that the period of precession is given by:^{[citation needed]}
Where I_{s} is the moment of inertia, T_{s} is the period of spin about the spin axis, and τ is the torque. In general, the problem is more complicated than this, however.
There is an easy way to understand why gyroscopic precession occurs without using any mathematics. The behavior of a spinning object simply obeys laws of inertia by resisting any change in direction. A spinning object possesses a property known as rigidity in space, meaning the spin axis resists any change in orientation. It is the inertia of matter comprising the object as it resists any change in direction that provides this property. Of course, the direction this matter travels constantly changes as the object spins, but any further change in direction is resisted. If a force is applied to the surface of a spinning disc, for example, matter experiences no change in direction at the place the force was applied (or 180 degrees from that place). But 90 degrees before and 90 degrees after that place, matter is forced to change direction. This causes the object to behave as if the force was applied at those places instead. When a force is applied to anything, the object exerts an equal force back but in the opposite direction. Since no actual force was applied 90 degrees before or after, nothing prevents the reaction from taking place, and the object causes itself to move in response. A good way to visualize why this happens is to imagine the spinning object to be a large hollow doughnut filled with water, as described in the book "Thinking Physics" by Lewis Epstein. The doughnut is held still while water circulates inside it. As the force is applied, the water inside is caused to change direction 90 degrees before and after that point. The water then exerts its own force against the inner wall of the doughnut and causes the doughnut to rotate as if the force was applied 90 degrees ahead in the direction of rotation. Epstein exaggerates the vertical and horizontal motion of the water by changing the shape of the doughnut from round to square with rounded corners.
Now imagine the object to be a spinning bicycle wheel, held at both ends of its axle in the hands of a subject. The wheel is spinning clockwise as seen from a viewer to the subject’s right. Clock positions on the wheel are given relative to this viewer. As the wheel spins, the molecules comprising it are traveling exactly horizontal and to the right the instant they pass the 12o'clock position, vertically downward the instant they pass 3 o'clock, horizontally to the left at 6 o'clock, vertically upward at 9 o’clock and horizontally to the right again at 12 o'clock. Between these positions, each molecule travels components of these directions. Now imagine the viewer applying a force to the rim of the wheel at 12 o’clock. For this example’s sake, imagine the wheel tilting over when this force is applied; it tilts to the left as seen from the subject holding it at its axle. As the wheel tilts to its new position, molecules at 12 o’clock (where the force was applied) and those at 6 o’clock still travel horizontally; their direction did not change as the wheel was tilting. Nor is their direction different after the wheel settles in its new position; they still move horizontally the instant they pass 12 and 6 o’clock. BUT, molecules passing 3 and 9 o’clock were forced to change direction. Those at 3 o’clock were forced to change from moving straight downward, to downward and to the right as viewed from the subject holding the wheel. Molecules passing 9 o’clock were forced to change from moving straight upward, to upward and to the left. This change in direction is resisted by the inertia of those molecules. And when they experience this change in direction, they exert an equal and opposite force in response AT THOSE LOCATIONS3 AND 9 O’CLOCK. At 3 o’clock, where they were forced to change from moving straight down to downward and to the right, they exert their own equal and opposite reactive force to the left. At 9 o’clock, they exert their own reactive force to the right, as viewed from the subject holding the wheel. This makes the wheel as a whole rotate counterclockwise as viewed from directly above. Thus, as the force was applied at 12 o’clock, the wheel behaved as if that force was applied at 3 o’clock, which is 90 degrees ahead in the direction of rotation. Or, you can say a force from the opposite direction was applied at 9 o'clock, 90 degrees prior to the actual force.
In summary, when you apply a force to a spinning object to change the direction of its spin axis, you are not changing the direction of the matter comprising the object at the place you applied the force (nor at 180 degrees from it); matter experiences zero change in direction at those places. Matter experiences the maximum change in direction 90 degrees before and after that place, and lesser amounts closer to that place. The equal and opposite reaction that occurs 90 degrees before and after then causes the object to behave as it does. This principle is demonstrated in helicopters. Helicopter controls are rigged so that inputs to them are transmitted to the rotor blades at points 90 degrees prior to and 90 degrees after the point at which the change in aircraft attitude is desired. The effect is dramatically felt on motorcycles. A motorcycle will suddenly lean and turn in the opposite direction the handle bars are turned.
Precession causes another phenomenon for spinning objects such as the bicycle wheel in this scenario. If the subject holding the wheel removes a hand from one end of its axle, the wheel will not topple over, but will remain upright, supported at just the other end. However, it will immediately take on an additional motion; it will begin to rotate about a vertical axis, pivoting at the point of support as it continues spinning. If you allowed the wheel to continue rotating, you would have to turn your body in the same direction. If the wheel was not spinning, it would topple over and fall when one hand is removed. The initial action of the wheel beginning to topple over is equivalent to applying a force to it at 12 o'clock in the direction toward the unsupported side (or a force at 6 o’clock toward the supported side). When the wheel is spinning, the sudden lack of support at one end of its axle is equivalent to this same force. So, instead of toppling over, the wheel behaves as if a continuous force is being applied to it at 3 or 9 o’clock, depending on the direction of spin and which hand was removed. This causes the wheel to begin pivoting at the one supported end of its axle while remaining upright. Although it pivots at that point, it does so only because of the fact that it is supported there; the actual axis of precessional rotation is located vertically through the wheel, passing through its center of mass. Also, this explanation does not account for the effect of variation in the speed of the spinning object; it only illustrates how the spin axis behaves due to precession. More correctly, the object behaves according to the balance of all forces based on the magnitude of the applied force, mass and rotational speed of the object. Once it is visualized why the wheel remains upright and rotates, it can easily be seen why the axis of a spinning top slowly rotates while the top spins as shown in the above illustration. A top behaves exactly like the bicycle wheel due to the force of gravity pulling downward. The point of contact with the surface it spins on is equivalent to the end of the wheel axle that is supported.
Relativistic (Einsteinian)
The special and general theories of relativity give three types of corrections to the Newtonian precession, of a gyroscope near a large mass such as Earth, described above. They are:
 Thomas precession a special relativistic correction accounting for the observer's being in a rotating noninertial frame.
 de Sitter precession a general relativistic correction accounting for the Schwarzschild metric of curved space near a large nonrotating mass.
 Lense–Thirring precession a general relativistic correction accounting for the frame dragging by the Kerr metric of curved space near a large rotating mass.
Astronomy
In astronomy, precession refers to any of several gravityinduced, slow and continuous changes in an astronomical body's rotational axis or orbital path. Precession of the equinoxes, perihelion precession, changes in the tilt of Earth's axis to its orbit, and the eccentricity of its orbit over tens of thousands of years are all important parts of the astronomical theory of ice ages. (See Milankovitch cycles.)
Axial precession (precession of the equinoxes)
Axial precession is the movement of the rotational axis of an astronomical body, whereby the axis slowly traces out a cone. In the case of Earth, this type of precession is also known as the precession of the equinoxes, lunisolar precession, or precession of the equator. Earth goes through one such complete precessional cycle in a period of approximately 26,000 years or 1° every 72 years, during which the positions of stars will slowly change in both equatorial coordinates and ecliptic longitude. Over this cycle, Earth's north axial pole moves from where it is now, within 1° of Polaris, in a circle around the ecliptic pole, with an angular radius of about 23.5°.
The ancient Greek astronomer Hipparchus (c. 190120 BC) is claimed to be the earliest known astronomer to recognize and assess the precession of the equinoxes at about 1° per century (which is not far from the actual value for antiquity, 1.38°).^{[4]} Caltech's Swerdlow disputes Hipparchus's knowledge of precession because Hipparchus apparently did not necessarily indicate anything like a motion of the entire sphere of the fixed stars with respect to the equinoxes.^{[5]} In ancient China, the Jindynasty scholarofficial Yu Xi (fl. 307345 AD) made a similar discovery centuries later, noting that the position of the Sun during the winter solstice had drifted roughly one degree over the course of fifty years relative to the position of the stars.^{[6]} The precession of Earth's axis was later explained by Newtonian physics. Being an oblate spheroid, Earth has a nonspherical shape, bulging outward at the equator. The gravitational tidal forces of the Moon and Sun apply torque to the equator, attempting to pull the equatorial bulge into the plane of the ecliptic, but instead causing it to precess. The torque exerted by the planets, particularly Jupiter, also plays a role.^{[7]}
Apsidal precession
The orbits of planets around the Sun do not really follow an identical ellipse each time, but actually trace out a flowerpetal shape because the major axis of each planet's elliptical orbit also precesses within its orbital plane, partly in response to perturbations in the form of the changing gravitational forces exerted by other planets. This is called perihelion precession or apsidal precession.
In the adjunct image, Earth's apsidal precession is illustrated. As the Earth travels around the Sun, its elliptical orbit rotates gradually over time. The eccentricity of its ellipse and the precession rate of its orbit are exaggerated for visualization. Most orbits in the Solar System have a much smaller eccentricity and precess at a much slower rate, making them nearly circular and stationary.
Discrepancies between the observed perihelion precession rate of the planet Mercury and that predicted by classical mechanics were prominent among the forms of experimental evidence leading to the acceptance of Einstein's Theory of Relativity (in particular, his General Theory of Relativity), which accurately predicted the anomalies.^{[8]}^{[9]} Deviating from Newton's law, Einstein's theory of gravitation predicts an extra term of A/r^{4}, which accurately gives the observed excess turning rate of 43″ every 100 years.
The gravitational force between the Sun and moon induces the precession in Earth's orbit, which is the major cause of the climate oscillation of Earth that has a period of 19,000 to 23,000 years. It follows that changes in Earth's orbital parameters (e.g., orbital inclination, the angle between Earth's rotation axis and its plane of orbit) is important to the study of Earth's climate, in particular to the study of past ice ages.
Nodal precession
Orbital nodes also precess over time.
See also
References
 ^ Schaub, Hanspeter (2003), Analytical Mechanics of Space Systems, AIAA, pp. 149–150, ISBN 9781600860270, retrieved 1 May 2014
 ^ Boal, David (2001). "Lecture 26 – Torquefree rotation – bodyfixed axes" (PDF). Retrieved 20080917.
 ^ Teodorescu, Petre P (2002). Mechanical Systems, Classical Models. Springer. p. 420.
 ^ DIO 9.1 ‡3
 ^ Swerdlow, Noel (1991). On the cosmical mysteries of Mithras. Classical Philology, 86, (1991), 4863. p. 59.
 ^ Sun, Kwok. (2017). Our Place in the Universe: Understanding Fundamental Astronomy from Ancient Discoveries, second edition. Cham, Switzerland: Springer. ISBN 9783319541716, p. 120; see also Needham, Joseph; Wang, Ling. (1995) [1959]. Science and Civilization in China: Mathematics and the Sciences of the Heavens and the Earth, vol. 3, reprint edition. Cambridge: Cambridge University Press. ISBN 0521058015, p. 220.
 ^ Bradt, Hale (2007). Astronomy Methods. Cambridge University Press. p. 66. ISBN 978 0 521 53551 9.
 ^ Max Born (1924), Einstein's Theory of Relativity (The 1962 Dover edition, page 348 lists a table documenting the observed and calculated values for the precession of the perihelion of Mercury, Venus, and Earth.)
 ^ An even larger value for a precession has been found, for a black hole in orbit around a much more massive black hole, amounting to 39 degrees each orbit.
External links
Wikibooks has a book on the topic of: Rotational Motion 