Stephen Hawking — "Wrong again, Albert."
Wrong again, Albert.
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More from Stephen Hawking
"We are in danger of destroying ourselves by our greed and stupidity. We cannot remain looking inwards at ourselves on a small and increasingly polluted and overcrowded planet."
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About Stephen Hawking (1942-2018)
British theoretical physicist whose Hawking radiation work and A Brief History of Time (1988) brought black-hole physics to a mass audience while he lived with ALS for 55 years. Closely associated with Roger Penrose (his collaborator on singularity theorems) and Carl Sagan (fellow popularizer who wrote Brief History's foreword). For an intellectual contrast, see William Lane Craig, American philosopher of religion — Craig's Kalam cosmological argument depends on the Big Bang requiring a divine first cause; Hawking's no-boundary proposal was specifically designed to remove the moment that would require one — the cleanest cosmology-vs-natural-theology contrast in modern thought.
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Understanding this quote
What it means
With playful confidence, this quote challenges the idea that even the greatest minds are infallible. It expresses the core engine of science: progress means correcting predecessors, regardless of their stature. Rather than reverence freezing inquiry, it suggests intellectual courage to declare genius can be wrong. The casual tone makes it radical—treating Einstein not as a sacred authority but as a fellow scientist who got some things demonstrably mistaken.
Relevance to Stephen Hawking
Hawking's entire career involved extending and overturning Einstein's intuitions. Einstein insisted 'God does not play dice,' rejecting quantum mechanics, but Hawking's 1974 discovery of Hawking radiation proved quantum effects reshape black holes Einstein thought were purely classical. Einstein doubted black holes were real; Hawking made them his life's work. Confined to a wheelchair by ALS yet rewriting physics, Hawking delivered such corrections with characteristic wit and zero deference.
The era
From the 1970s onward, physics faced its central crisis: Einstein's general relativity and quantum mechanics couldn't be reconciled. String theory, loop quantum gravity, and the Standard Model all probed beyond Einstein's classical framework. Hawking radiation in 1974 was the era's landmark—showing quantum effects operate at black hole event horizons, directly challenging Einstein's classical picture. The era also saw growing cultural veneration of Einstein, making Hawking's irreverent correction carry deliberate provocation.
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