Matter is much older than life. Billions of years before the sun and earth even formed, atoms were being synthesized in the insides of hot stars and then returned to space when the stars blew themselves up. Newly formed planets were made of this stellar debris, the earth and every living thing are made of star stuff (Carl Sagan).
About ten
million years after the Big Bang, enough cooling and expansion had occurred to
fill the universe with a mist of particles, containing mostly hydrogen and some
helium, as also some types of elementary particles (including neutrinos), some
electromagnetic radiation, and perhaps some other, unknown, particles. The
universe was just cold, dark, and formless at that stage.
Then, when
enough cooling had occurred, some quantum-mechanical primordial fluctuations in
the densities of the particles resulted in a clumping of some of the particles,
rather like the nucleation that precedes the growth of a crystal from a fluid. The presence
of such clumped particles brought the gravitational forces into prominence, resulting
in a cascading effect. Portions of the mist began collapsing into large
swirling clouds. Over a period of a few hundred million years, huge galaxies,
each containing billions of young stars of various sizes, formed and began to
shine. The formless darkness of the initial period was gone.
The large
superstars among these were strongly bright spheres, the brightness coming from
the nuclear fusion of hydrogen and helium in their interiors, made possible by
the prevailing extreme temperatures and pressures. This is how many of the
heavier elements got formed in the interiors of these large stars.
The emergence
of heavier elements by the process of nuclear fusion continued steadily until
the element iron (Fe) started forming. The iron nucleus is the most stable of
them all, having the largest binding energy per nucleon. [Protons and neutrons
inside the nucleus are jointly called nucleons; and 'binding energy' is defined
as the amount of energy required to extract a nucleon from inside the nucleus
and take it far away from it]. Therefore iron cannot fuse with one or more
nucleons and release radiative energy of the nuclear process; such a process
would not lower the potential energy and the free energy. Consequently, the
presence of iron acts as a 'poison' for the nuclear fusion process. Thus
the appearance of iron marked the beginning of the end of the available nuclear
fuel, and therefore the end of the life of the star. In due course, the smaller
among such stars simply ceased to shine, shrinking into cold and dead entities.
But a very
different fate awaited the larger stars. No longer able to sustain their size
because of the progressively decreasing processes of nuclear fusion of
elements, they began to collapse under their own immense gravitational
pull. A rapid change occurred in their interiors. Under the immense squeezing
generated by the collapse, the iron-element core imploded. This resulted in a
new state of matter as the electrons and the protons in the atoms were squeezed
together. The dominant process of interaction was the electroweak interaction: p+
+ e- → n0 + νe
(i.e., protons and electrons combined to produce neutrons and
electron-neutrinos).
Thus, this collapse
led to a compression of the star to an extremely dense ball of pure neutron
matter, with the neutrino cloud bursting outwards, resulting in an explosion of
the outer shell of the star (the 'SUPERNOVA EXPLOSION'). This is how the
synthesized elements (up to the atomic number (Z) for iron), residing in the
outer shell of the star, were scattered into the universe, accompanied by a
brilliant flash of light.
A consequence
of such supernova explosions (which still occur from time to time, and illuminate
the galaxies with brilliant flashes of light) was the emergence of clouds of
dust and gas and the debris containing heavy elements. These clouds encircled
the galaxies in spiraling arms. THE INTENSITY OF THE SUPERNOVA EXPLOSIONS AND
THE TEMPERATURES INVOLVED WERE SO HIGH THAT ELEMENTS HEAVIER THAN IRON WERE
ALSO SYNTHESIZED AND SCATTERED INTO SPACE.
The chemical
elements in our bodies have come from that star stuff: In the outer portions of
the spirals occurred a condensation of the dust, the clouds and the debris,
resulting in the formation of the second generation of (smaller) stars
(including our Sun), as also planets, moons, comets, asteroids, etc.
Our solar
system was formed when the universe was ~9 billion years old. In the initial
period, our Earth underwent several violent upheavals (bombardment by comets
and meteors, as also huge earthquakes and volcanic eruptions). By the time the
Earth was ~2.5 billion years old, its continents had formed. Life appeared in
due course, which further influenced the ecosphere in a major way. In
particular, free oxygen (as opposed to oxygen chemically bound with other
elements) was liberated as a waste product by the algae that consumed carbon
dioxide present in the atmosphere and in the oceans.
Two billion
years ago, our Earth was extremely radioactive as well. The heavier-than-iron
elements produced in the outer shell of the exploding stars during the
supernova explosion were/are radioactive, as their binding energy per nucleon
was lower than that of iron: Such elements can increase their binding energy
per nucleon (and thus attain a more stable state) by undergoing nuclear fission,
either spontaneously or with the assistance of free neutrons. Uranium was among
the heaviest elements produced during the last few seconds of the supernova
explosion. Thus this element was a part of the Earth right from the beginning.
Watch this video for an interesting visualization of our cosmic and terrestrial history:
Watch this video for an interesting visualization of our cosmic and terrestrial history:
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