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{{about|]'s and planets' nutation}}
{{See also|Nutation in plants}}
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'''Nutation''' (from ]: ''nūtāre'', to nod) is a rocking, swaying, or nodding motion in the ] of a largely axially symmetric object, such as a ], ], or ] ], or as an intended behavior of a mechanism. A pure nutation is a movement of a rotational axis such that the first ] (]) is constant.
==Astronomy==
The nutation of a planet happens because of ]s that cause the ] to vary over time so that the speed of precession is not constant. The nutation of the ] was discovered in 1728 by the British ] ], but this nutation was not explained in detail until 20 years later.<ref>The Nodding Sphere and the Bird's Beak: D'Alembert's Dispute with Euler </ref>
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Values of nutations are usually divided into components parallel and ] to the ]. The component that works along the ecliptic is known as the ''nutation in longitude''. The component perpendicular to the ] is known as the ''nutation in obliquity''. Celestial coordinate systems are based on an "equator" and "equinox," which means a great circle in the sky that is the projection of the Earth's equator outwards, and a line, the ] intersecting that circle, which determines the starting point for measurement of ]. These items are affected both by ] of the equinoxes and nutation, and thus depend on the theories applied to precession and nutation, and on the date used as a reference date for the coordinate system. In simpler terms, nutation (and precession) values are important in observation from ] for calculating the apparent positions of astronomical objects.
===Earth===
], the most northerly latitude which the Sun can reach directly overhead. All four ] that are defined by the Earth's tilt (both ] and both ]) will shift correspondingly.]]
In the case of the Earth, the principal sources of tidal force are the ] and ], which continuously change location relative to each other and thus cause nutation in Earth's axis. The largest component of Earth's nutation has a period of 18.6 years, the same as that of the precession of the ]. However, there are other significant periodical terms that must be calculated depending on the desired accuracy of the result. A mathematical description (set of equations) that represents nutation is called a "theory of nutation" (see, e.g., ). In the theory, parameters are adjusted in a more or less ''ad hoc'' method to obtain the best fit to data. As can be seen from the ] publication just cited, nowadays simple rigid-body ] do not give the best theory; one has to account for deformations of the solid Earth.
====Values====
The principal term of nutation is due to the regression of the moon's nodal line and has the same period of 6798 days (18.6 years). It reaches plus or minus 17″ in ] and 9″ in ]. All other terms are much smaller; the next-largest, with a period of 183 days (0.5 year), has amplitudes 1.3″ and 0.6″ respectively. The periods of all terms larger than 0.0001″ (about as accurately as one can measure) lie between 5.5 and 6798 days; for some reason they seem to avoid the range from 34.8 to 91 days, so it is customary to split the nutation into long-period and short-period terms. The long-period terms are calculated and mentioned in the almanacs, while the additional correction due to the short-period terms is usually taken from a table.
==In mechanical engineering==A nutating motion can be seen in a ] mechanism. In general, a nutating plate is carried on a skewed bearing on the main shaft and does not itself rotate, whereas a swashplate is fixed to the shaft and rotates with it. The motion is similar to the motions of coin or a tire wobbling on the ground after being dropped with the flat side down.The nutating motion is widely employed in ] and ]s. The displacement of volume for one revolution is first determined. The speed of the device in revolutions per unit time is measured. In the case of flowmeters, the product of the rotational speed and the displacement per revolution is then taken to find the flow rate.==In physiology==In upright vertebrates, the ] is capable of slight independent movement along the ]. When you bend backward the top (base) of the sacrum moves forward relative to the ]; when you bend forward the top moves back.<ref>Maitland, J (2001). ''Spinal Manipulation Made Simple.'' Berkeley: North Atlantic Books, p. 72.</ref> The anterior motion of the sacral base is called nutation, and the posterior motion is counter-nutation.<ref>{{cite web|author=Joseph D. Kurnik, DC|url=http://www.chiroweb.com/archives/14/26/18.html|title=The AS Ilium Fixation, Nutation, and Respect}}</ref>==External links==*
==References==
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Revision as of 11:15, 28 July 2012
This article is about Earth's and planets' nutation. For other uses, see Nutation (disambiguation).
Rotation (green), Precession (blue) and Nutation in obliquity (red) of the Earth
Nutation (from Latin: nūtāre, to nod) is a rocking, swaying, or nodding motion in the axis of rotation of a largely axially symmetric object, such as a gyroscope, planet, or bulletin flight, or as an intended behavior of a mechanism. A pure nutation is a movement of a rotational axis such that the first Euler angle (precession) is constant.
The nutation of a planet happens because of tidal forces that cause the precession of the equinoxes to vary over time so that the speed of precession is not constant. The nutation of the axis of the Earth was discovered in 1728 by the British astronomerJames Bradley, but this nutation was not explained in detail until 20 years later.
Because the dynamic motions of the planets are so well-known, their nutations can be calculated to within arcseconds over periods of many decades. There is another disturbance of the Earth's rotation called polar motion that can be estimated for only a few months into the future because it is influenced by rapidly and unpredictably varying things such as ocean currents, wind systems, and motions in the liquid nickel-ironcore of the Earth.
Values of nutations are usually divided into components parallel and perpendicular to the ecliptic. The component that works along the ecliptic is known as the nutation in longitude. The component perpendicular to the ecliptic is known as the nutation in obliquity. Celestial coordinate systems are based on an "equator" and "equinox," which means a great circle in the sky that is the projection of the Earth's equator outwards, and a line, the Vernal equinox intersecting that circle, which determines the starting point for measurement of right ascension. These items are affected both by precession of the equinoxes and nutation, and thus depend on the theories applied to precession and nutation, and on the date used as a reference date for the coordinate system. In simpler terms, nutation (and precession) values are important in observation from Earth for calculating the apparent positions of astronomical objects.
Earth
Nutation makes a small change to the angle at which the Earth tilts with respect to the Sun, thereby moving the location of the Tropic of Cancer, the most northerly latitude which the Sun can reach directly overhead. All four major circles of latitude that are defined by the Earth's tilt (both Tropical Circles and both Polar Circles) will shift correspondingly.
In the case of the Earth, the principal sources of tidal force are the Sun and Moon, which continuously change location relative to each other and thus cause nutation in Earth's axis. The largest component of Earth's nutation has a period of 18.6 years, the same as that of the precession of the Moon's orbital nodes. However, there are other significant periodical terms that must be calculated depending on the desired accuracy of the result. A mathematical description (set of equations) that represents nutation is called a "theory of nutation" (see, e.g., ). In the theory, parameters are adjusted in a more or less ad hoc method to obtain the best fit to data. As can be seen from the IERS publication just cited, nowadays simple rigid-body mechanics do not give the best theory; one has to account for deformations of the solid Earth.
Values
The principal term of nutation is due to the regression of the moon's nodal line and has the same period of 6798 days (18.6 years). It reaches plus or minus 17″ in longitude and 9″ in obliquity. All other terms are much smaller; the next-largest, with a period of 183 days (0.5 year), has amplitudes 1.3″ and 0.6″ respectively. The periods of all terms larger than 0.0001″ (about as accurately as one can measure) lie between 5.5 and 6798 days; for some reason they seem to avoid the range from 34.8 to 91 days, so it is customary to split the nutation into long-period and short-period terms. The long-period terms are calculated and mentioned in the almanacs, while the additional correction due to the short-period terms is usually taken from a table.
References
The Nodding Sphere and the Bird's Beak: D'Alembert's Dispute with Euler
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