Classroom Working Blog

THIS IS A CLASSROOM WORKING BLOG. YOU MAY SEE MISTAKES OR ERRORS. THESE ERRORS WILL NOT BE CORRECTED BY THE TEACHER AS THIS IS WHERE THE CHILDREN ARE CURRENTLY WORKING. THIS BLOG WILL BE MONITORED BY THE CLASSROOM TEACHER. THANK YOU FOR VISITING OUR BLOG.

Sunday, November 14, 2010

Black Hole facts

Not even light can escape black holes.Once a giant star dies and a black hole has formed, all its mass is squeezed into a single point. At this point, both space and time stop.Black holes are the ends of stars at least 10 to 15 times as massive as the Sun. If a star that is massive or larger undergoes a supernova explosion, it may leave behind a fairly massive burned out remnant. With no outward forces to oppose gravitational forces, the remnant will collapse in on itself.Black holes are x-ray radiation that gets smaller and smaller until they disappear, or "evaporate".The gravity around the hole of a black hole is so strong that NOTHING can make its way back out after a critical distance.The critical distance at which nothing can escape is called the Event Horizon.If the Sun was magically crushed until it was about 1 mile in size, it would become a black hole, but the Earth would remain in its orbit. According to theory, there might be three types of black holes: stellar, super massive, and miniature black holes — depending on their size. Four billion years from now when the Sun runs out of the available nuclear fuel in its core, our Sun will die a quiet death. Stars of this type end their history as white dwarf stars.

Written by Alexandra and Laine

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