Why is Kantās theory of solar-system formation called the Kant-Laplace hypothesis?
The term Kant-Laplace nebular hypothesis is used because the model combines the distinct but related theories of Immanuel Kant and Pierre-Simon Laplace regarding the origin of the solar system.1
In 1755, Kant proposed that the solar system emerged from a cloud of dispersed particles that were pulled together by gravity, eventually coalescing into the Sun and planets. Decades later, Laplace independently developed a model suggesting that the Sun and planets formed from a cooling, contracting nebula that shed rings of material, which then condensed into planets.123
Because both thinkers shared the fundamental concept that planets formed from the condensation of dispersed material within a rotating cloud, their approaches were synthesized into a single model. This combined theory, known as the Kant-Laplace nebular hypothesis, served as a widely accepted explanation for the formation of the solar system for approximately 100 years.1