The study of paleomagnetism is possible because
iron-bearing minerals such as
magnetite may record past polarity of Earth's magnetic field. Magnetic signatures in rocks can be recorded by several different mechanisms.
Thermoremanent magnetization Iron-titanium oxide minerals in
basalt and other
igneous rocks may preserve the direction of 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 , whereas most basalt and
gabbro are completely crystallized at temperatures below . Hence, the mineral grains are not rotated physically to align with Earth's magnetic field, but rather they may record the orientation of that field. The record so preserved is called a thermoremanent magnetization (TRM). Because complex
oxidation reactions may occur as igneous rocks cool after crystallization, the orientations of 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
oceanic 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. Although the
Māori people of
New Zealand do not make pottery, their 700- to 800-year-old steam ovens, or
hāngī, provide adequate archaeomagnetic material.
Detrital remanent magnetization 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 remanent magnetization. If the magnetization is acquired as the grains are deposited, the result is a depositional detrital remanent magnetization; if it is acquired soon after deposition, it is a post-depositional detrital remanent magnetization.
Chemical remanent magnetization In a third process, magnetic grains grow during chemical reactions and record the direction of the magnetic field at the time of their formation. The field is said to be recorded by
chemical remanent magnetization (CRM). A common form is held by the mineral
hematite, another
iron oxide. Hematite forms through chemical oxidation reactions of other minerals in the rock including magnetite.
Red beds,
clastic sedimentary rocks (such as
sandstones) are red because of hematite that formed during sedimentary
diagenesis. The CRM signatures in red beds can be quite useful, and they are common targets in magnetostratigraphy studies.
Isothermal remanent magnetization Remanence that is acquired at a fixed temperature is called
isothermal remanent magnetization (IRM). Remanence of this sort is not useful for paleomagnetism, but it can be acquired as a result of lightning strikes.
Lightning-induced remanent magnetization can be distinguished by its high intensity and rapid variation in direction over scales of centimeters. IRM is often induced in
drill cores by the magnetic field of the steel core barrel. This contaminant is generally parallel to the barrel, and most of it can be removed by heating up to about 400 °C or demagnetizing in a small alternating field. In the laboratory, IRM is induced by applying fields of various strengths and is used for many purposes in
rock magnetism.
Viscous remanent magnetization Viscous remanent magnetization is remanence that is acquired by
ferromagnetic materials influenced by a magnetic field for some time. In rocks, this remanence is typically aligned in the direction of the modern-day geomagnetic field. The fraction of a rock’s overall magnetization that is a viscous remanent magnetization is dependent on the magnetic mineralogy. == Sampling ==