A supernova (Image credit: NASA) |
Carl Sagan famously said we are all made of
stardust, and he was right on the money. Everything around us began in the
death of a star. Supernovas create giant clouds of matter which provide the
building blocks for new stars, planets, and the matter that makes up living and
inorganic substances.
The
Death of a Star
Stars produce energy by nuclear fusion. Each
star contains vast reserves of hydrogen, which fuses into helium. Toward the
end of its life, a star runs out of hydrogen. Without hydrogen, the star starts
fusing helium into heavier elements. The core of the star shrinks, but the
outer layers expand to create a red giant star, which often destroys
surrounding planets.
Eventually the star runs out of helium as well.
If it’s a small star, like our sun, fusion ends and the star, now a white
dwarf, slowly dies. Larger stars go through violent changes when they run out
of helium. The core collapses almost instantly.
Temperature within the collapsing core builds
in a matter of seconds to over 100 billion degrees Fahrenheit. The outer layer
collapses inwards, and then explodes outwards in a supernova. During the
supernova explosion, the dying star produces enough energy to fuse heavy
elements, such as uranium and gold. Any planets lucky enough to survive the
star’s expansion into a red giant are obliterated by the supernova.
As for the remains of the collapse star core,
if conditions are right it may become a black hole, an area where matter is
crushed under gravitational forces so strong even light cannot escape.
Star
Birth
The material expelled during the explosion sometimes
forms massive clouds of dust and gas called nebulae that float in the
interstellar void. Gravity causes nebulae material to clump together,
eventually giving birth to a protostar. As millions of years pass, the
protostar develops into a fully-formed star.
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