The Fermi Paradox
The universe is ancient, enormous, and full of ordinary stars much like ours. So where is everybody?
1950 (Fermi's remark), 1975 (Hart's argument)22 min read
Italian-American physics
1901 – 1954
Architect of the first self-sustaining nuclear reactor and of the theory of beta decay, and famous for order-of-magnitude estimation from almost no data. Over lunch at Los Alamos in the summer of 1950 he interrupted a conversation about flying saucers to ask "Where is everybody?" — a question about the feasibility of interstellar travel that was later built into an argument he never published.
The universe is ancient, enormous, and full of ordinary stars much like ours. So where is everybody?
1950 (Fermi's remark), 1975 (Hart's argument)22 min read