The Cold War secret that revealed the universe's most powerful explosions

Gamma-Ray Bursts: Crash Course Astronomy #40 · 14:05 · Video: CrashCourse · Watch at the source

In short: In 1963, the U.S. Air Force launched satellites to monitor nuclear weapons tests. Instead of finding forbidden bombs, they stumbled upon something far more massive: gamma-ray bursts, cosmic explosions so energetic they can outshine a million trillion suns.

Gamma-ray bursts (GRBs) were discovered by accident during the Cold War. The Vela satellites, designed to ensure compliance with nuclear testing treaties between the U.S., UK, and Soviet Union, began detecting high-energy light from deep space. By 1/2/1967, the Vela 4A satellite recorded the first GRB, though the findings were not declassified and published until 1973. Scientists at Los Alamos National Laboratory eventually proved these bursts were not local, but originated from beyond our solar system.

These events are categorized into two main types based on their duration. Collisions involving a black hole and a neutron star, or two neutron stars, initiate brief pulses under two seconds. Long bursts, lasting two seconds or longer, occur when a massive star undergoes a hypernova, leading to a core collapse and the birth of a black hole. These explosions are incredibly luminous; a single burst can emit as much energy in seconds as our Sun will in its entire 9-billion-year lifetime.

While some feared a nearby GRB could wipe out life in a galaxy, modern evidence suggests they act more like lighthouses than bombs, channeling energy into narrow, collimated jets. While anything within 200 light years of a beam might be vaporized, our Solar System is safe, as no nearby stars are destined for such an explosion. Today, these bursts serve as cosmic laboratories, helping researchers study the formation of heavy elements like gold and platinum.

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