

A visionary who derived equations predicting an expanding universe from Einstein's theory, he laid the mathematical groundwork for the Big Bang.
In the turbulent aftermath of the Russian Revolution, Alexander Friedmann, a mathematician and dynamicist, performed a quiet act of cosmic prophecy. While others, including Einstein himself, believed the universe was static, Friedmann took Einstein's equations of general relativity and showed they could describe a universe that was dynamic—growing, shrinking, or cycling. His 1922 paper presented the Friedmann equations, the first rigorous mathematical model of an expanding cosmos. Tragically, he died of typhoid fever at 37, just three years after his groundbreaking work, never witnessing Edwin Hubble's observational proof of expansion. Friedmann's legacy is the fundamental framework upon which all modern cosmology is built, the first true scientific narrative of a universe with a beginning and a destiny.
1883–1900
Came of age during World War I. Disillusioned by the carnage, they rejected the certainties of the Victorian era and built modernism from the wreckage — in art, literature, and politics.
Alexander was born in 1888, placing them squarely in The Lost Generation. The events that shaped this generation — world wars, depression, and rapid industrialization — shaped the world they entered and the choices available to them.
The biggest hits of 1888
The world at every milestone
World's Columbian Exposition dazzles Chicago
Queen Victoria dies, ending the Victorian era
New York City opens its first subway line
San Francisco earthquake devastates the city
Robert Peary claims to reach the North Pole
World War I ends; Spanish flu pandemic kills millions
The Scopes Trial debates evolution in schools
He served as a bomber pilot and later a military meteorologist for the Russian air force during World War I.
Friedmann's expanding universe theory was initially dismissed by Einstein, who later acknowledged it as correct.
He undertook daring scientific balloon flights to collect atmospheric data, setting a Russian altitude record in 1925.
A crater on the far side of the Moon is named in his honor.
“The universe described by these equations is not static, but expanding.”