- The study of the remanent magnetization in rocks.
- The earth's magnetic field as it existed in the past.
Dictionary:
pa·le·o·mag·net·ism (pā'lē-ō-măg'nĭ-tĭz'əm) ![]() |
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The study of the direction and intensity of the Earth's magnetic field through geologic time. Paleomagnetism has been, and continues to be, an important tool in unraveling the past movements of the Earth's, tectonic plates. By studying the records of the ancient magnetic field left in rocks, earth scientists are able to learn how the continental and oceanic plates have moved relative to the Earth's, spin axis and relative to one another. In addition, the global reference frame of the Earth's, magnetic field provides a very useful basis for temporal correlation of rocks on a local or global geographic scale (magnetostratigraphy). See also Geomagnetism; Plate tectonics.
Many rocks acquire remanent magnetizations at or about the time they are formed. These magnetizations are nearly always parallel to the direction of the Earth's, magnetic field at the locality where the rock formed. See also Rock magnetism.
In paleomagnetic studies a suite of carefully oriented samples spanning a time interval long enough to average magnetic secular variations is collected. For magnetostratigraphy, an ordered suite of samples spanning the stratigraphic section of interest are collected. The samples are taken to the laboratory, where they are cut into small upright cylinders and their magnetization is measured by using a sensitive magnetometer.
The end product of the laboratory experiments is a suite of magnetization vector directions from the collected samples. These directions are specified by the inclination I, the angle that the magnetization vector makes with the horizontal, and the declination D, the angle that the projection of the magnetization vector upon a horizontal plane makes with true north, reckoned positive clockwise from north. Provided that the sample collection represents a sufficiently long time span to average out secular variation, representative mean D and I values and an associated uncertainty in direction may be calculated by using statistical techniques. The mean declination and inclination, together with the inclination-latitude relationship mentioned earlier and some elementary spherical trigonometry, allow the calculation of a representative paleomagnetic pole from the rock unit. By connecting paleomagnetic poles of different ages in an ordered time sequence, an apparent polar wander path (APWP) may be constructed for a particular tectonic plate. The APWP specifies the displacement history of a plate or continent with respect to the spin axis, and can be directly compared with APWPs from other plates or continents to determine whether relative movements have occurred.
The end product of a magnetostratigraphic study is a set of normal (N) and reversed (R) magnetizations from the stratigraphic section under investigation. The positioning and frequency of occurrence of these N-to-R and R-to-N transitions is highly diagnostic in many cases, and by using these data together with other local geologic information, such as the position of major unconformities, one stratigraphic section can be correlated with another over considerable distances. The method can also be used over intracontinental and intercontinental distances. However, because the field has only two possible states (N or R), correlation over longer distances where tectonics and sedimentation rates may vary is correspondingly less accurate.
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Paleomagnetism is the study of the record of the Earth's magnetic field preserved in various magnetic minerals through time. The study of paleomagnetism has demonstrated that the Earth's magnetic field varies substantially in both orientation and intensity through time.
A paleomagnetist is a scientist who studies the ancient magnetic field by measuring the orientation of magnetic minerals in rocks and sediments, acquired at the time of their formation (remnant magnetization), then using methods similar to geomagnetism to determine what configuration of the Earth's magnetic field may have resulted in the observed orientation.
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Paleomagnetism is studied on a number of scales:
The study of paleomagnetism is possible because iron-bearing minerals such as magnetite may record past directions of the Earth's magnetic field. Paleomagnetic signatures in rocks can be recorded by three different mechanisms.
First, iron-titanium oxide minerals in basalt and other igneous rocks may preserve the direction of the Earth's magnetic field when the rocks cool through the Curie temperatures of those minerals. The Curie temperature of magnetite, a spinel-group iron oxide, is about 580°C, whereas most basalt and gabbro are completely crystallized at temperatures above 900°C. Hence, the mineral grains are not rotated physically to align with the Earth's field, but rather they may record the orientation of that field. The record so preserved is called a thermal remnant magnetization (TRM). Because complex oxidation reactions may occur as igneous rocks cool after crystallization, the orientations of the Earth's magnetic field are not always accurately recorded, nor is the record necessarily maintained. Nonetheless, the record has been preserved well enough in basalts of the ocean crust to have been critical in the development of theories of sea floor spreading related to plate tectonics. TRM can also be recorded in pottery kilns, hearths, and burned adobe buildings. The discipline based on the study of thermoremanent magnetisation in archaeological materials is called archaeomagnetic dating.[1]
In a completely different process, magnetic grains in sediments may align with the magnetic field during or soon after deposition; this is known as detrital remnant magnetization (DRM). If the magnetization is acquired as the grains are deposited, the result is a depositional detrital remnant magnetization (dDRM); if it is acquired soon after deposition, it is a post-depositional detrital remnant magnetization (pDRM).
In a third process, magnetic grains may be deposited from a circulating solution, or be formed during chemical reactions, and may record the direction of the magnetic field at the time of mineral formation. The field is said to be recorded by chemical remnant magnetization (CRM). The mineral recording the field commonly is hematite, another iron oxide. Redbeds, clastic sedimentary rocks (such as sandstones) that are red primarily because of hematite formation during or after sedimentary diagenesis, may have useful CRM signatures, and magnetostratigraphy can be based on such signatures.
Paleomagnetic evidence, both reversals and polar wandering data, was instrumental in verifying the theories of continental drift and plate tectonics in the 1960s and 70s. Some applications of paleomagnetic evidence to reconstructing histories of terranes have continued to arouse controversies. Paleomagnetic evidence also is used in constraining possible ages for rocks and processes and in reconstructions of the deformational histories of parts of the crust.
Reversal magnetostratigraphy is often used to estimate the age of fossil and hominin bearing sites.[2]
Paleomagnetic studies are combined with geochronological methods to determine absolute ages for rocks in which the magnetic record is preserved. For igneous rocks such as basalt, commonly used methods include potassium-argon and argon-argon geochronology.
The oldest magnetizations early paleomagnetic studies were able to measure were approximately 250 Ma old (the oldest oceanic crust). Today refined methods can be used to provide field information for dating of rocks as old as four Ga.
One of the pioneering scientists who studied paleomagnetism was the British physicist P.M.S. Blackett.
Edward A. Irving, a Canadian paleomagnetism specialist, used paleomagnetic studies to support plate tectonics in the 1950s. The method of identifying polar reversals by examination of oceanic crust was further developed by Frederick John Vine.
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