Black holes & exotica

Spaghettification

The stretch that pulls anything falling into a black hole into a long, thin strand

Artist's impression · drag to rotate
What it is stretching along the line to the black hole and squeezing sideways [1]
How it grows with the inverse cube of distance halve the distance and the stretch is 8 times stronger [1]
Stretch on Earth about 0.0000055 m/s² head to foot, for a 1.8 m person [3]
At a Sun-mass black hole's horizon about 19.6 billion m/s² the horizon is 2.9 km from the centre [3]
At a 100-million-Sun black hole's horizon about 0.0000019 m/s² less than Earth's tide on you [3]
Swallowed whole above about 100 million Suns a Sun-like star crosses the horizon before it is torn apart [6]
Torn-apart stars seen about 100 as of May 2024 [6]
Word in print by 1977 Nigel Calder; popularised by Stephen Hawking in 1988 [2]

About the image. Drawn as a black hole pulling a star into a long, glowing stream of gas that curls around it. Stars torn apart like this are seen only as unresolved points of light, so the shape of the stream follows simulations, and its colours and texture are imagined.

Spaghettification is what happens to anything that falls too close to a black hole. The end nearer to the black hole is pulled harder than the far end, so the object is stretched out along the line towards it and squeezed in from the sides, into a long, thin strand. The effect is the same tide that raises the oceans on Earth. Near a black hole it becomes strong enough to tear apart a person, a planet or a star.

Why size matters

The stretch depends on how quickly gravity changes over the length of your body, and it grows with the inverse cube of distance: halve the distance and it is eight times stronger. On Earth, the difference between the pull on your head and your feet is about 0.0000055 metres per second squared, far too small to notice.

At the event horizon of a black hole with the mass of the Sun, only 2.9 kilometres from its centre, the stretch on a 1.8-metre person would be about 19.6 billion metres per second squared. Nobody would get that far in one piece. Stellar-mass black holes, up to about 30 times the Sun’s mass, tear things apart well before they reach the horizon.

A huge black hole is gentler. The horizon of one with 100 million times the Sun’s mass lies 295 million kilometres out, and there the stretch is only about 0.0000019 metres per second squared, less than Earth’s tide on you. You could cross that horizon without feeling the stretch. “If you have the choice, you want to fall into a supermassive black hole,” said Schnittman of NASA, who in 2024 made a simulation of a fall into a black hole of 4.3 million Suns, like the one at the centre of the Milky Way. His virtual camera crossed the horizon intact and was spaghettified 12.8 seconds later, about 128 000 kilometres from the centre.

Stars torn apart

Spaghettification has never been seen happen to anything as small as a person, but it is seen happening to stars. When a star strays too close to a supermassive black hole, it is drawn out into long streams of gas. In 1988 Rees calculated that about half of the star stays bound to the black hole and the rest is flung away. The gas falling back lights up as a brilliant flare. About 100 of these tidal disruption events were known by May 2024. Around the very largest black holes, above about 100 million Suns, a star like the Sun crosses the horizon before it can be torn apart and is swallowed whole without a flare.

When ESO reported it in 2020, AT2019qiz was the closest such flare yet recorded, just over 215 million light-years away in a spiral galaxy in Eridanus. A star of about the Sun’s mass lost about half of it to a black hole more than a million times heavier, and gas streamed away at up to 10 000 kilometres per second. In 2024 Nicholl and colleagues reported that, years later, the spot was erupting in X-rays about once every 48 hours.

The word

Stephen Hawking made the word famous in A Brief History of Time in 1988, with his image of an astronaut stretched like spaghetti. It is older than his book: it appears in print in 1977, in Nigel Calder’s The Key to the Universe.

Gallery

A black sphere edged with a bright golden crescent of light, and a thin glowing stream of gas curling around its lower side, an impression of a star being stretched into a stream by a black hole. AI-generated painting.
A small rocky asteroid at the lower left trailing a long, thin, curving thread of glowing rubble that leads into a bright orange ring of light around a black hole, an impression of spaghettification. AI-generated painting.
Spaghettification, 3D artist's impression, rendered from the interactive model.
Spaghettification, 3D artist's impression, from another angle, rendered from the interactive model.
Spaghettification, 3D artist's impression, close-up, rendered from the interactive model.

Timeline

  1. 1975 Hills proposes that black holes tearing stars apart could power bright flares.
  2. 1977 The word spaghettification appears in Nigel Calder's The Key to the Universe.
  3. 1988 Hawking's A Brief History of Time makes it famous; Rees shows about half a torn star stays bound.
  4. 2020 ESO reports AT2019qiz, a Sun-like star torn apart 215 million light-years away.
  5. 2024 NASA's simulation of a fall into a Milky Way-sized black hole; AT2019qiz is found erupting in X-rays every 48 hours.

Questions people ask

Would you be spaghettified before reaching the event horizon?

It depends on the black hole. A stellar-mass black hole, up to about 30 times the Sun's mass, tears you apart before the horizon. At one of 100 million Suns the stretch at the horizon is smaller than what you feel on Earth.

How long would spaghettification take if you fell into a black hole?

In NASA's 2024 simulation of a black hole of 4.3 million Suns, like the Milky Way's, the camera crosses the horizon and is torn apart 12.8 seconds later, about 128 000 km from the centre.

Who came up with the word spaghettification?

Stephen Hawking made it famous in A Brief History of Time in 1988, but it was already in print in 1977, in Nigel Calder's The Key to the Universe.

Sources

  1. Wikipedia: Spaghettification
  2. Word Origins: spaghettify / spaghettification
  3. Astronomy magazine (2023), Ask Astro: Why are small black holes more dangerous than big ones?
  4. NASA Scientific Visualization Studio (2024), NASA Black Hole Visualization Takes Viewers Beyond the Brink
  5. NASA Science (2024), New NASA Black Hole Visualization Takes Viewers Beyond the Brink
  6. Wikipedia: Tidal disruption event (Hills 1975; Rees 1988; Gezari 2021)
  7. ESO (2020), Death by Spaghettification: ESO Telescopes Record Last Moments of Star Devoured by a Black Hole
  8. Nicholl et al. (2020), An outflow powers the optical rise of the nearby, fast-evolving tidal disruption event AT2019qiz, MNRAS 499, 482
  9. Chandra X-ray Center (2024), on Nicholl et al., Quasi-periodic X-ray eruptions years after a nearby tidal disruption event, Nature 634, 804
  10. Price et al. (2024), Eddington envelopes: The fate of stars on parabolic orbits tidally disrupted by supermassive black holes, ApJL 971, L46