Everything that has a beginning has an end. We know how the
universe began, and how old it is (some 13.7 billion years), but we don’t know
the end. Or do we? To know the end of the universe is to acquire enough data to
compute a constant known as Omega.
Envision a
rocket leaving the planet, there is a certain speed that it must be going to
escape the gravity of the Earth, we call this escape velocity. Omega works off
a very similar idea. If the big bang imparted enough velocity to the galaxies
(escape velocity if you will) then the universe will continue to expand ever
onwards. However, if the galaxies are not fast enough, then think of them as a rocket
that has not achieved escape velocity. Eventually gravity would pull everything
back to the way it all was in the beginning, what scientists call “the big
crunch”, the converse of the big bang.
Whatever
fate awaits the universe one day can be determined by the numerical value of
Omega. Omega is the total amount of matter in the universe divided by the
minimum amount of matter needed to create the big crunch. If Omega is greater
than 1, the galaxies will fly apart forever, and if it is less, then someday
the big crunch will happen. Knowing that there are about five hydrogen atoms
per cubic meter of space, our best guess is that Omega is valued somewhere
between .98 and 1.1 so the fate of the universe remains a mystery.
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