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Close Encounters (of the Cosmic Kind)
Back to The Dating Game
Right now, in our atmosphere, there are countless numbers of
nitrogen atoms floating high above the Earth's surface. These
atoms are, in a sense, vulnerable.
Cosmic radiation, in the form of neutrons, zips through the
atmosphere at a high rate of speed. Occasionally, and purely
by chance, some of these neutrons collide with the nuclei of
some of the nitrogen atoms.
The nucleus of each nitrogen atom contains seven protons and
seven neutrons. That is, it does until a collision happens.
The incoming neutron hitting the nucleus causes a proton to
shoot out of the nucleus, just as a cue ball on a pool table,
hitting one of two balls that are touching, might cause the
ball that it hits to stay in place and the other ball to shoot
off.
The nitrogen atom now has six protons and eight neutrons. This
means two things. One, with this arrangement of protons and
neutrons, it's unstable. In other words, it's radioactive. And
two, it's no longer nitrogen. The reason is that the number of
protons an atom contains determines what that atom is. Since
it now contains six protons, it's carbon. Carbon usually has
six neutrons as well—in this form it's called carbon-12
(6+6=12). The unstable, eight-neutron version, however, is
carbon-14 (6+8=14).
All radioactive atoms will eventually decay, or change, in
some way. When a carbon-14 atom decays, one of its eight
neutrons turns into a proton, emitting an electron (with a
charge of -1) in the process. The atom is now stable. And with
seven protons and seven neutrons, it is again nitrogen-14.
Next:
Eating It and Eating It...
Does Race Exist? |
Meet Kennewick Man
Claims for the Remains
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