Post No. 2: Black Holes.
Black holes is an exciting topic. They are the most
important consequence of the Theory of Relativity even that Einstein never
expressed enthusiasm. The general relativity predicted the presence of a mass
deforms space-time in such a way that the paths taken by particles bend towards
the mass. At the event horizon of a black hole, this deformation becomes so
strong that there are no paths that lead away from the black hole.
There are many definitions of black hole as “black hole is a
place in space where gravity pulls so much that even light can not get out. The
gravity is so strong because matter has been squeezed into a tiny space. This
can happen when a star is dying.” (NASA)
The definition I found in Wikipedia says;” A black hole is a region of spacetime exhibiting such strong gravitational effects that nothing- not even particles and electromagnetic radiation such as light-can space from inside it.”
The first use of the term “black hole “ in print was by
science journalist Ann Ewing in her article “ Black Holes in Space” dated 18
January 1964, which was a report on a meeting of the American Association for the Advancement of Science
held in Cleveland in Ohio.
The defining feature of a black hole is the appearance of an
event horizon- a boundary in spacetime through which matter and light can only
pass inward towards the mass of the black hole. Nothing, not even light can
escape from inside the event horizon.
Stephen Hawking has compared crossing this boundary to going over
The photo shows a
spiral galaxy called Messier 106. NASA/ESA Hubble Space Telescope. It is located over 20 million Light-
years away. At his heart, as in most spiral galaxies, is a supermassive Black hole,
but this one is particularly active.
There are many scientists that had been investigating and
writing about this phenomenal topic but still are many concerns and is not easy
to understand.
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