Overview

The inner core is the very center of Earth, a dense, primarily metallic sphere that is distinct from the overlying fluid outer core. It is small compared with the whole planet but plays an outsized role in deep-Earth processes. Estimates from seismic data put its radius at roughly 1,220 km and its temperature near several thousand kelvins. Its composition is believed to be dominated by iron with a significant admixture of nickel and lighter elements.

Structure and physical conditions

The inner core is mechanically solid, while the surrounding outer core is liquid. That contrast in physical state produces characteristic signatures in seismic records and sets up the boundary that separates different types of wave propagation. Pressure at the center of the planet is enormous, and the combination of extreme pressure and temperature determines whether iron can remain crystalline. Under core conditions the melting temperature of iron rises, allowing a solid phase to exist despite temperatures comparable to the hot parts of the Sun's surface.

How we know: seismology and discovery

Information about the inner core comes almost entirely from seismic waves generated by earthquakes and other large seismic sources. Waves that travel through Earth are bent, slowed or blocked by changes in material and state; careful analysis reveals a small, distinct central region. The solid inner core was inferred by Danish seismologist Inge Lehmann in 1929 when she noted puzzling arrivals from a large earthquake in New Zealand. Her interpretation of seismic travel times led to the two-part core model (solid inner, liquid outer) that is now well established.

Composition, temperature and pressure

Laboratory experiments, mineral physics, and geochemical arguments point to an iron–nickel alloy as the main constituent of the inner core. Light elements such as sulfur, silicon, oxygen or hydrogen may be present in smaller amounts. Estimates of temperature at the inner-core boundary are in the thousands of kelvins, and central pressures are on the order of millions of atmospheres; these factors together control phase relations and the behavior of metals under core conditions.

Dynamics, role and open questions

The inner core grows slowly as the liquid outer core solidifies at the inner-core boundary, releasing latent heat and chemical buoyancy that help drive convection in the outer core and sustain Earth’s magnetic field. Seismologists have also detected subtle anisotropy (direction-dependent seismic speeds) and differences between the outermost and innermost parts of the inner core, leading to hypotheses of an "inner inner core" or variations in crystal alignment. Other active research topics include the precise age of the inner core, whether it rotates slightly differently from the mantle, and how its evolution ties to Earth’s thermal history.

Key points and resources

Further reading