Sir George Howard Darwin

Born in 1845, he was the second son of Charles Darwin and became one of Britain’s leading mathematical astronomers. He studied at Trinity College, Cambridge, where he later spent much of his career, and he is especially remembered for work on tides, the evolution of the Earth–Moon system, and the figures of rotating celestial bodies.

He served as Plumian Professor of Astronomy and Experimental Philosophy at Cambridge and was known for bringing deep mathematical analysis to problems in astronomy and geophysics. His research helped shape later thinking about tidal friction and the long-term development of planetary systems.

He was knighted for his scientific work and remained an important figure in British science until his death in 1912. Readers interested in the history of astronomy often find his career especially compelling because it sits at the meeting point of Victorian science, mathematics, and the Darwin family legacy.