What are Black Holes?

Black Hole 2


Figure 2: Source UPI.2002 <http://web.a.ebscohost.com/ehost/detail/detail?sid=e7517dd2-ddd8-48a2-8ff4-4c0d8 7bd2aff%40sessi onmgr4003&vid=13&hid=4114&bdata=JnNpdGU9ZWhvc3Q tbGl2ZQ%3d %3d#db=aph&authdb=imh&AN=imh172790> viewed 2 February 2015.




     


                                                                                                                                                                            


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            Black holes can be thought of as condensed stars which have collapsed in on themselves to form a very dense ball of mass. There are stellar sized black holes and supermassive black holes.  Supermassive black holes have density approximately that of water, (Berman 2014). The reason a black hole is called a black hole is that gravity at a certain distance from this massive condensed matter is at a high enough acceleration that light cannot escape its grasp. The matter in a black hole is condensed, unlike matter here on earth and on the sun where the matter is at “normal” levels. A condensed object such as a black hole is one in which the matter has shrunk to a point that the gravity a certain distance from the object is stronger than the speed of light. This is why it is possible that our sun could become a black hole without any additional matter being fed into it. Bob Berman writes that:


"Because gas is easy to compress, it makes sense that the Sun's huge gravitational pull -- 333,000 times greater than Earth's -- someday could force our star to shrink much smaller. When the core's fusion factory shuts down, its outward-pushing gas pressure no longer will be able to counteract gravity's inward pull."

                                                                                                                                                                    (Berman, 2014)