Black Holes Slowly Evaporate — and the Last One Will Mark the End of Everything
Answers: “do black holes ever die?”
Nothing escapes a black hole — that’s the whole premise. Fall past the event horizon and you are, as far as the universe is concerned, gone forever.
Which is why Stephen Hawking’s 1974 calculation shocked physics: black holes leak. Slowly, imperceptibly, but inevitably, every black hole is evaporating — and will one day vanish in a flash.
The mechanism, now called Hawking radiation, comes from quantum physics. Empty space isn’t truly empty: pairs of “virtual” particles constantly flicker into existence and annihilate. But at the edge of an event horizon, a pair can be split — one particle falls in, the other escapes. To balance the books, the escaping particle carries away a sliver of the black hole’s mass-energy.
The black hole pays for the radiation with its own existence.
The timescales make geology look hasty:
- A black hole with the Sun’s mass would take about 10^67 years to evaporate — that’s a 1 followed by 67 zeros. The universe is currently 1.4 × 10^10 years old.
- Supermassive giants like TON 618 will take closer to 10^100 years
- As a black hole shrinks, it radiates faster — the process accelerates until the final moments, which end in a burst of energy like a cosmic firework
There’s a haunting cosmological postscript. In the unimaginably far future, after the last stars burn out and galaxies decay, black holes will be the final structures left — slowly evaporating in the dark. The disappearance of the last black hole may be the last event the universe ever hosts.
Hawking radiation has never been directly observed — it’s far too faint — but the theory is so robust that physicists overwhelmingly accept it. Hawking asked for its formula to be engraved on his tombstone. It is.