Question:

What happens to the magnetic susceptibility (\(k\)) and remanent magnetization (\(I_r\)), when the molten rock undergoes rapid cooling?

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Rapid cooling produces fine, single-domain-like grains: these are magnetically 'hard' — low induced susceptibility but strong, stable remanent magnetization.
Updated On: Jul 21, 2026
  • \(k\) increases and \(I_r\) decreases
  • \(k\) decreases and \(I_r\) increases
  • Both \(k\) and \(I_r\) decrease
  • Both \(k\) and \(I_r\) increase
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The Correct Option is B

Solution and Explanation

When molten rock (magma/lava) cools, its magnetic minerals (mainly magnetite/titanomagnetite) crystallise and grow. The rate of cooling directly controls the grain size of these magnetic minerals:

Rapid cooling (e.g. lava chilled at the surface or against cold rock) leaves very little time for crystal growth, so the magnetic grains that form are very small — close to the single-domain (SD) or pseudo-single-domain (PSD) size range, with few or no internal domain walls.

Susceptibility (\(k\)): bulk magnetic susceptibility in an applied field is largely controlled by how easily domain walls can move within multidomain (MD) grains — MD grains respond strongly to a weak applied field because their walls shift readily, giving a high induced susceptibility. Fine, near single-domain grains lack mobile domain walls (a SD grain is a single, uniformly magnetized domain), so the induced/bulk susceptibility of a rock dominated by fine grains is comparatively low. Hence rapid cooling → smaller grains → lower \(k\).

Remanent magnetization (\(I_r\)): single-domain and pseudo-single-domain grains are magnetically far more efficient at recording and, crucially, at *retaining* a stable thermoremanent magnetization (TRM) than multidomain grains, because there are no internal domain walls to later relax or realign and demagnetize the grain. As the fine grains cool quickly through their Curie/blocking temperature in the ambient (Earth's) field, they lock in a strong, stable remanence. Hence rapid cooling → fine SD/PSD grains → higher, more stable \(I_r\).

So rapid cooling produces a rock with lower susceptibility but higher (more stable) remanent magnetization — exactly option (B).

\(\boxed{k \text{ decreases}, \; I_r \text{ increases}}\)

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