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Finding a planet through calculation

Urbain Le Verrier

1811–1877

Le Verrier calculated an unknown planet’s position from discrepancies in Uranus’s orbit. In 1846 Neptune was observed close to his predicted position, a spectacular success for celestial mechanics.

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Urbain Le Verrier
Historical portrait of Urbain Le Verrier, engraving held by the Wellcome Collection.
Wellcome Collection — engraver not recorded · CC BY 4.0 · Portrait source
Resized and converted to WebP for this site.

A life of research

Educated at the École polytechnique, he began in chemistry before turning to celestial mechanics. Much of his career was associated with the Paris Observatory.

He sought improved theories and tables of planetary motion. Small differences between predictions and observations became physical clues rather than inconvenient errors to ignore.

Understanding the contribution

He attributed some anomalies in Uranus’s motion to the pull of a more distant planet. On 23 September 1846 Johann Galle and Heinrich d’Arrest found Neptune in Berlin, guided by his calculations.

John Couch Adams had independently studied the same problem. Later, Mercury’s anomaly resisted explanation by an extra planet and found its solution in general relativity.

What this work changed

His story illustrates two possible outcomes of a discrepancy: discovering a missing object or revising the theory used for prediction.

Sources and references