"In 1965, Antony Hewish and Samuel Okoye discovered "an unusual source of high radio brightness temperature in the Crab Nebula." - Wikipedia
Some more http://en.wikipedia.org/wiki/Neutron_star#Examples_of_neutron_stars" could be found here, have fun :smile:
As your traveling further and further into the gravitational well, there must be huge gravitational gaps among each millimeter taken, especially as your getting closer to the event horizon :smile:
I know this might be a rough explanation... but if your trying to get into a BH, you'll need to get pass the gravitational gaps and the huge amounts of disintegrating space junk traveling close to c first :biggrin:
According to widespread modern knowledge, the universe possesses about 0.4 of the required mass to collapse back into it's original state, in a sort of 'big crush',
As the current predictable future of the universe is to expand in an exhilarating speed while 'tearing up' the matter into the most...