It's likely the single biggest part of a scientific instrument. (Not of an industrial tool... yet.)
It's likely the single biggest part of a scientific instrument. (Not of an industrial tool... yet.)
It's also reasonable to assume that more and more extreme physics is going to be harder and harder (if not practically impossible for any future humans) to come up with new gee-whiz uses.
https://chem.tufts.edu/answersinscience/relativityofwrong.ht...
I haven't double checked the calculations myself: too much other stuff to do. But glancing around at other people who have looked at the numbers, it seems pretty clear that spaghettification is expected to happen for macroscopic objects well outside the event horizon of a stellar-mass black hole. Wikipedia gives an example of a 10-solar-mass black hole: its event horizon radius is about 30km, but macroscopic objects will be spaghettified at a radius of about 320km. https://en.wikipedia.org/wiki/Spaghettification#Inside_or_ou... (That ratio is roughly reversed for a 10,000-solar-mass black hole.) There are some similar calculations shown in detail on this NASA math worksheet (which is for some reason still using cgs units): https://spacemath.gsfc.nasa.gov/blackh/4Page33.pdf