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Seismology 1906

The Constitution of the Interior of the Earth, as Revealed by Earthquakes

Richard Dixon Oldham

Time the trembles that cross the planet — and a hidden core appears at its heart.

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In depth · the introduction

An earthquake on one side of the world arrives, faintly, on the other — and in exactly how late it arrives, Oldham found a core hidden at the centre of the Earth.

A heart at the centre of the Earth

When a great earthquake strikes, it sends waves racing clear through the planet, not just around its surface. Two kinds travel through the deep rock: fast push–pull waves and slower side-to-side waves. By 1906, seismographs scattered across the globe were catching these waves after their long journeys, each arrival stamped with a time.

Richard Oldham lined those times up against distance and noticed something off. Waves that had to pass through the very deepest part of the Earth showed up late — later than they should if the planet were the same stuff all the way down. The simplest explanation: a distinct core at the centre, of denser material through which the waves travel more slowly. The Earth had a hidden heart, and you could hear it in the timing.

From an Indian earthquake to the Earth's centre

Oldham was an Anglo-Irish geologist who had spent years with the Geological Survey of India. His turning point was the catastrophic 1897 Assam earthquake, which he documented in unprecedented detail; from its records he learned to read the separate arrivals of different wave types — a skill most of his contemporaries lacked.

Back in England, he gathered seismograms of distant earthquakes from the world's growing network of stations and did the patient bookkeeping: which wave, how far, how long. The late arrivals at the greatest distances were the clue. Rather than dismiss them as error, he followed them to a startling conclusion and published it in 1906 — the first time anyone had shown, from earthquakes alone, that the Earth has a core.

Why it mattered

Nobody can dig to the centre of the Earth; the deepest borehole barely dimples the crust. Oldham proved that we don't have to. The waves from earthquakes go everywhere a drill cannot, and they report back in their timing. He turned the whole planet into something you could examine from the outside — and found its largest interior division, the boundary between mantle and core, on which every later picture of the deep Earth is built.

Like knocking to find the beam behind a wall

Knock along a wall and listen: the sound changes where a wooden beam hides behind the plaster, and you can map what you can't see by how the knock comes back. Oldham knocked on the Earth with earthquakes and listened with seismographs. Where the returning knock came late, he knew the wave had crossed something different deep inside — and traced that delay to a core no one could ever reach.

A cross-section of the Earth with a mantle and a central core, an earthquake at the top, and a travel-time graph alongside. A slider moves a station around the globe and a checkbox removes the core. A straight ray is drawn to the station; on the graph, a dashed line shows what a coreless Earth predicts and a solid line shows the real travel time, which climbs late once the wave's path crosses the core.

Where it sits

Oldham opened a relay that read the deep Earth from its tremors: he found the core in 1906, Andrija Mohorovičić found the crust–mantle boundary in 1909, Beno Gutenberg measured how deep the core lay, Harold Jeffreys showed its outer part is liquid, and Inge Lehmann — also in this Library — found a solid inner core within. It stands beside the other ways this Library's scientists learned to read the planet: Hutton and Lyell in the slow time of rocks, Wegener and Hess in the moving sea floor. Together they turned the Earth from an opaque ball into a body with a known anatomy.

The original document
Original source text
Richard Dixon Oldham · The Constitution of the Interior of the Earth, as Revealed by Earthquakes · Quarterly Journal of the Geological Society of London 62 (1906): 456–475
The instrument: a worldwide clock of trembles
By 1906 a network of sensitive seismographs around the world recorded the same great earthquake at many distances. Oldham's raw material was the arrival times on those records, set against the angular (epicentral) distance from each shock — a global stopwatch on waves that had threaded the whole planet.
Three arrivals on every record
Oldham insisted on separating three distinct arrivals that earlier workers had blurred together: a first phase of fast compressional waves (today's P), a slower second phase of shear waves (today's S), and the still-slower large waves that run around the surface. Timing each phase apart was the key that let the interior speak.
The anomaly: waves that arrive too late
Plotted against distance, the first two phases followed a smooth curve out to roughly 120°. Beyond that, the waves whose paths plunged through the deepest interior arrived markedly later than a uniform planet would allow. Something near the centre was holding them back.
The conclusion: a central core
Oldham read the delay as the signature of a distinct central core — of materially different, lower wave-speed constitution than the rock above it — occupying roughly the inner two-fifths of the radius. The Earth was not uniform to its centre: it had a heart.
[ … ]
Oldham's core was real, but his measure of it was rough: the modern core–mantle boundary sits deeper, at 2891 km (core radius 3480 km, 0.55 R). His size estimate, his velocities, and his reliance on the second phase were all refined or corrected within decades — by Gutenberg (1913), Jeffreys (1926) and Lehmann (1936). The full memoir, tables and plates included, is at the source below.
Geological Society of London · 1906