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Mathematician of celestial mechanics

Pierre-Simon Laplace

1749–1827

Pierre-Simon Laplace applied mathematical analysis to gravity and planetary motion. He sought to explain irregularities in the Solar System through interactions among its different bodies.

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Pierre-Simon Laplace
Painted portrait of Laplace by Johann Ernst Heinsius.
Johann Ernst Heinsius · Public domain · Portrait source
Resized and converted to WebP for this site.

A life of research

Born in Normandy, he moved to Paris and built a scientific career during a period of major political change. His research extended across mechanics, probability and mathematical physics.

He assembled much of his work in the Treatise on Celestial Mechanics, published from 1799 to 1825. It developed Newton's laws into powerful methods for calculating the behaviour of systems containing multiple objects.

Understanding the contribution

Planets feel not only the Sun's attraction but also each other's gravity. Laplace studied these perturbations to explain changes in their orbits and investigate the stability of the Solar System over long periods.

In 1796 he also proposed a hypothesis for planetary formation from a rotating nebula. This historical picture differs in important ways from modern models, but it sought a common physical origin for the system.

What this work changed

His legacy is an approach connecting observations, calculations and general laws. Modern investigations of chaos have since clarified the limitations of conclusions about stability over exceptionally long timescales.

Sources and references