Why falling into a supermassive black hole is safer than a small one

What would we see if we fell into a Black Hole? · 14:53 · Video: ScienceClic English · Watch at the source

In short: If you were to fall into a stellar-mass black hole, tidal forces would stretch you like a noodle before you ever reached the center. However, plunging into a supermassive giant offers a different, albeit still fatal, journey through the warped physics of general relativity.

The experience of approaching a black hole is defined by the extreme curvature of spacetime described by Einstein's general theory of relativity. For an observer falling toward a stellar-mass black hole—which can contain up to about 30 solar masses—the difference in gravitational pull between your head and your feet becomes lethal very quickly. This phenomenon, known as spaghettification, occurs because the gravity is significantly stronger on the side closer to the mass, literally stretching objects into long, thin strands. Conversely, different physical principles apply to supermassive black holes, exemplified by the Milky Way's central entity possessing a mass 4.3 million times that of our Sun. Because these monsters are so vast, their event horizons are much larger and the tidal forces near the boundary are relatively weaker.

This means an astronaut could theoretically cross the 'point of no return' without being instantly shredded, allowing them to witness the bizarre optical effects of warped light before their fate is sealed. To make these difficult-to-imagine processes visible, astrophysicists like Jeremy Schnittman at NASA’s Goddard Space Flight Center use supercomputers to bridge the gap between complex mathematics and visual reality. By simulating a camera as a stand-in for an astronaut, researchers can map out how light behaves near the horizon. These visualizations help us understand the consequences of relativity in our universe, showing what happens when an object briefly orbits or plunges into the most extreme gravitational wells in existence.

Note: While these simulations provide a visual guide to the physics of the event horizon, they are theoretical models based on the equations of general relativity.

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