<p><BR/>Replying to:<BR/><DIV CLASS='Discussion_PostQuote'>This is a basic understanding of black hole formation (since I'm not too good with this topic!):The most common formation of black holes is from collapsed stars. Typically, black holes form from high mass stars, much more massive than our Sun. Betelgeuse is an excellent example. Betelgeuse is a Red Super Giant, with a mass that is far greater than the Sun. When one of these colossal stars runs out of nuclear energy, they begin to collapse. Eventually, the star will collapse so far that nothing can prevent itself from collapsing under the pressure of its own gravity. After releasing its guts into interstellar space, the final result will often be a black hole. As for what happens inside a black hole, only theory and mathematics can tell us what may be taking place. Once you cross the event horizon (the point of no return), there is nothing that will stop you from being pulled to the gravitational singularity at the center. The event horizon is the barrier where on the outside, you still have a chance to escape the black hole, yet on the inside, your trip to the singularity is inevitable. Think of it this way: Once inside the event horizon, the roles of time and space are reversed. In other words, in normal 4D space, your forward progression in time is inevitable, there's nothing you can do to stop it; additionally, your movement through space is not dictated by any one direction. Yet, once inside the black hole, these two are reversed: Your forward progression through time will cease, yet your forward progression through space is inevitable, being dictated by the gravitational singularity. Are you following this? <br />Posted by weeman</DIV><br /><br />Just testing if I got everything right. The <em>star</em> doesn't really collapse more and more; at first its diameter goes up as fusion moves outwards through new layers. When the core has fused nucleuses to point where it's fusing iron, it can no longer gain energy surplus through fusion (as fusing elements heavier than iron <em>requires</em> energy); and now the core, and the core only, collapses since there is nothing left that now can withstand gravity. At this point, the star is going supernova. Depending on it's current mass, it will transform into either a neutron star or, if it's massive enough, a black hole.</p><p>The event horizon; that's the point where the escape velocity = c? </p> <div class="Discussion_UserSignature"> </div>