From some of my previous posts you know that objects don’t just have size, they have mass. A three-foot diameter ball of loosely packed feathers, for example, has far less mass than a three-foot diameter ball of lead. But if you keep compressing feathers into that three-foot sphere, keep squeezing and squeezing them in, you’ll eventually have as much mass as the lead sphere. Once the two spheres are of equal mass you only need to squeeze in one more feather and, suddenly you have a three-foot sphere of feathers that is more massive than the three-foot sphere of lead.Now imagine you have an unimaginably powerful feather-squeezing gizmo and could keep squeezing in feathers. If you kept squeezing them in, your feather ball would become more and more massive. Eventually it would be so massive that it would have measurable gravity. Sooner or later it would become so massive that you could walk around on it just like the Earth but not as large.
Because your feather squeezing gizmo is so powerful you’d keep squeezing feathers in until the sphere had as much gravity as the Sun, then more than the Sun. Eventually it would have so much mass and its gravity would be so powerful that even light would bend a little when it passed too close to it. And after that? Well, it would become so massive that anything, including light, would fall right into it and be unable to escape if it passed too close.
And just like that, you’d have created a black hole. A black hole is simply an object of so much mass that its gravity prevents the escape of anything, even light. Black holes of varying mass exist at the center of many galaxies (including our own, it is believed) and in the space beyond. They are formed by the death of very large stars or by the joining of enough mass (in the form of stars, gas and other matter until the inward gravitational pull of the object exceeds any outward forces imparted by spin or (in the case of stars) by the energy of fusion. At this point, the object collapses in size until an unbelievable amount of mass is compressed into an unimaginably small area of space.
When you think about black holes you’re actually thinking about two things - the object or mass in the middle and the area of influence that object exerts. (though both are depicted in the image to the left, remember they’d both actually be completely invisible until you get out to the event horizon). The area of influence can be further broken down into two components - the event horizon and everything outward beyond the event horizon out to a point where the gravitational effect is no longer notable (represented by the green fog). We’ve already described the mass in the middle. It is simply all the matter (gas, rocks, ice, feathers, squirrels or anything of sufficient quantity) that has been packed together until it is massive enough to have an area of influence that prevents the escape of everything, including light.
If you could measure out from the edge of the massive object, there is a sphere of space-time. If an object passes far enough away from that sphere of influence at a constant speed as in the image to the left then it has every chance of continuing on its path without even noticing the effects of the black hole. Super sensitive instruments might read a subtle fluctuation in gravity in the direction of the hole. Perhaps a subtle course correction might be required. But the point is, despite its awesome power, even a black hole has limits. The primary weapon in its arsenal, gravity, dissipates over distance.
If the object flies closer to the black hole then its direction of travel might be influenced. It would, in effect, be pulled towards the black hole rather than traveling forward in a straight line. It might even be slowed a bit until it escaped the gravitational influence assuming it is applying constant force.
An object (a rocket, for example) has two choices to minimize the influence of the black hole it passes near. It can increase its speed to limit its time in the black hole’s gravity well or it can increase its distance from the gravity well as in the first example.
Fly too close, though, and the object might be captured by the black hole’s gravitational influence. It might then be held in a permanent orbit around the black hole, not falling in but not escaping. If it could increase thrust, it might escape. If it ran out of fuel, it is doomed to eventually fall past the event horizon. Once it falls past the event horizon, all bets are off. Remember, that current theory holds that nothing can move faster than light. Since even light is incapable of finding its way back out from the inner side of the event horizon, no rocket or spaceship could either. The event horizon is where the black hole begins to appear black. That’s because light can’t escape to reach our eye so, effectively, nothing from that point inward appears to exist.
Black holes are some of the strangest things you can find in space. Physics gets really weird when you throw black holes in the mix. A black hole literally warps both space and time. If you’re interested in reading more about black holes, super massive black holes, or micro black holes, eat a good breakfast, get plenty sleep the night before and make sure you bring your thinking cap with you. Then go to Ted Bunn’s absolutely wonderful FAQ about black holes and read until your brain hurts.
If you have flash enabled, I also strongly recommend visiting ThinkTechnologies.com and enjoying a very well put together flash presentation on the bizzare nature of black holes.