Falling into a black hole has long been one of science fiction's most popular tropes. But what would actually happen if a spacecraft ventured too close to such an object? Sergei Pilipenko, a senior researcher at the Astrospace Center of the Lebedev Physical Institute (FIAN), explained the effects that would await the crew and how supermassive black holes differ from their stellar-mass counterparts.
Time Would Accelerate DramaticallyIn an interview with RIA Novosti, the scientist explained that when falling into a supermassive black hole, time aboard the spacecraft would speed up so drastically relative to an outside observer that the crew could witness processes that under normal conditions take millions of years. The motion of stars and even entire galaxies would become visible "before their very eyes."
This is one of the relativistic effects of general relativity. The closer an object gets to the event horizon, the more time slows down for an external observer. For those falling inward, the picture is different: the external Universe would begin to rapidly "fast-forward."
Supermassive vs. Stellar-Mass – A Crucial DifferenceThe size of the black hole plays a major role. For supermassive objects, which reside at the centres of galaxies and have masses of millions to billions of Suns, tidal forces near the event horizon are relatively weak. As a result, a spacecraft could theoretically cross the horizon intact, without being torn apart.
However, even in this case, seeing the centre itself—the singularity—would be impossible. According to Pilipenko, between the spacecraft and the black hole's centre there would be another horizon, from which light simply could not reach the observers.
A very different fate awaits those approaching a stellar-mass black hole. There, tidal forces are immense. The difference in gravitational pull between different parts of the object becomes so strong that the spacecraft—or any body—would most likely be destroyed before ever crossing the event horizon.
What Remains Beyond the FrameThe subject of black holes continues to be an active area of research. Cosmologists have previously suggested that primordial black holes, which formed before the Big Bang, could have survived it and persisted to the present day. Such ideas are linked to models of a "cosmic bounce," in which the Universe first contracted and then began to expand.
For now, the main practical takeaway remains the same: supermassive black holes theoretically allow us to "look" beyond the event horizon, albeit with very unusual consequences for the perception of time and space.
In BriefAstrophysicist Sergei Pilipenko explained that when falling into a supermassive black hole, a spacecraft's crew, owing to relativistic time acceleration, would be able to observe the motion of stars and galaxies—changes that outside observers would see unfold over millions of years. The craft could cross the event horizon, but the black hole's centre would still remain invisible. In the case of a stellar-mass black hole, an object would most likely be destroyed by tidal forces before reaching the horizon.
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