Citat:
The point at which tidal forces destroy an object or kill a person depends on the black hole's size. For a supermassive black hole, such as those found at a galaxy's center, this point lies within the event horizon, so an astronaut may cross the event horizon without noticing any squashing and pulling, although it remains only a matter of time, as once inside an event horizon, falling towards the center is inevitable. For small black holes whose Schwarzschild radius is much closer to the singularity, the tidal forces would kill even before the astronaut reaches the event horizon.[4][5] For example, for a black hole of 10 Sun masses[6] and the above-mentioned rope at 1000 km distance, the tensile force halfway along the rope is 325 N. It will break at a distance of 320 km, well outside the Schwarzschild radius of 30 km. For a black hole of 10,000 Sun masses it will break at a distance of 3200 km, well inside the Schwarzschild radius of 30,000 km.
http://en.wikipedia.org/wiki/Spaghettification
Men tydligen är man inte längre säkra på vad som händer när man passerar händelsehorisonten, såg nåt avsnitt av sixtysymbols (nåt av brady iaf) där dom visade två nya papper där dom kom fram till att varje objekt skulle annihileras så fort händelsehorisonten passerats