fr en es pt
Astronomy
Asteroids and Comets Black Holes Children Constellations Earth Eclipses Environment Equations Evolution Exoplanets Galaxies Light Matter Moons Nebulas Planets and Dwarf Planets Probes and Telescopes Scientists Stars Sun Universe Volcanoes Zodiac New Articles Shorts Archives
Contact the author
RSS astronoo
Follow me on Bluesky
Follow me on Pinterest
English
Français
Español
Português
 


Last update 23 March 2016

The First Second of Our History

CHANGE

The Zero Moment of the Universe

About 13.8 billion years ago, in a fraction of a second, the universe was born. The mystery of creation is hidden in this first second after the Big Bang.

How, when there was nothing, no energy, no matter, no time, did a tremendous explosion suddenly give birth to space, matter, and time?

From this first second, chaos emerged from nothingness, burning with unimaginable heat. An informal mush expanded, stretched in all directions, and slowly cooled.

This "initial moment" is ours, the beginning of our clock. Even today, we capture in the sky the trace of the first moments (380,000 years after the first second) called "cosmic microwave background radiation" or "background radiation." This low-temperature microwave radiation, close to absolute zero, reaches the Earth's surface from all directions of the cosmos.

The cosmic microwave background is part of the background of all radio sources detected by our radiotelescopes since its discovery by Arno Penzias and Robert Wilson in 1965. It is proof that our observable Universe had a beginning. The first second of our Universe remains the greatest mystery of modern science. It seems that our mathematical formulas shatter against the wall of creation. In the beginning, there was nothing, no matter, no void, time and space did not exist. The explosion of a luminous point smaller than an atom and of infinite heat gave birth to the universe.

Everything begins an infinitesimal fraction of a second after the original explosion, the Big Bang. Time begins to unfold, and within a second, the entire cosmos takes shape. There is no zero time; before time did not exist. The cosmic clock strikes its first beat at 10-43 seconds.

The universe at this moment is an energy-dense boiling void, incredibly hot. Then, it is assumed to inflate suddenly, which is cosmic inflation. At 10-32 seconds, during this short period, the Universe filled with particles of all kinds. Elementary particles and their antiparticles emerged from the rapidly expanding space.

The first elements of matter, accompanied by antimatter, quarks, electrons, neutrinos, and photons, bathed in a cosmic soup. At 10-6 seconds, or one millionth of a second later, the first force, the strong nuclear force, comes into play. This force pulls quarks out of the void in threes to form protons and neutrons and create hydrogen and helium nuclei. After this mysterious first second, a very long and even more mysterious history will unfold, that of our existence.

"To understand our place in the universe, we must go back to the very beginning and see how it all formed." Professor Lawrence Krauss (Case Western Reserve University).

Articles on the same theme

How can we say that the Universe has an age? How can we say that the Universe has an age?
First Proof of the Expansion of the Universe First Proof of the Expansion of the Universe
Space-time slices of the observable Universe Space-time slices of the observable Universe
Dark Ages of the Universe Dark Ages of the Universe
Alternative theories to the accelerated expansion of the universe Alternative theories to the accelerated expansion of the universe
The primitive atom of Abbot Georges Lemaître The primitive atom of Abbot Georges Lemaître
Great walls and filaments: the great structures of the Universe Great walls and filaments: the great structures of the Universe
Always closer to the Big Bang Always closer to the Big Bang
Lyman-alpha bubbles Lyman-alpha bubbles
The mystery of gamma bursts The mystery of gamma bursts
Eternal inflation, string theory and dark energy Eternal inflation, string theory and dark energy
The Planck Universe: the Image of the Universe Becomes Clearer The Planck Universe: the Image of the Universe Becomes Clearer
The sky is immense with Laniakea The sky is immense with Laniakea
Abundance of chemical elements in the Universe Abundance of chemical elements in the Universe
The Symmetries of the Universe: A Journey Between Mathematics and Physical Reality The Symmetries of the Universe: A Journey Between Mathematics and Physical Reality
The geometry of time The geometry of time
How to measure distances in the Universe? How to measure distances in the Universe?
Do nothingness and emptiness exist? Do nothingness and emptiness exist?
Mystery of the Big Bang, the problem of the horizon Mystery of the Big Bang, the problem of the horizon
The first second of our history The first second of our history
Does dark matter exist? Does dark matter exist?
Metaverse, the next stage of evolution Metaverse, the next stage of evolution
The multiverse long before the Big Bang The multiverse long before the Big Bang
What is recombination in cosmology? What is recombination in cosmology?
The cosmological and physical constants of our Universe The cosmological and physical constants of our Universe
Thermodynamics of the sand pile Thermodynamics of the sand pile
What does the equation E=mc2 really mean? What does the equation E=mc2 really mean?
The engine of the accelerated expansion of the Universe The engine of the accelerated expansion of the Universe
The Universe of X-rays The Universe of X-rays
The oldest galaxies in the universe The oldest galaxies in the universe
Fossil radiation in 1992 Fossil radiation in 1992
Hubble constant and expansion of the Universe Hubble constant and expansion of the Universe
Dark energy is needed Dark energy is needed
Gravitational waves Gravitational waves
How big is the universe? How big is the universe?
The vacuum has considerable energy The vacuum has considerable energy
Paradox of the dark night Paradox of the dark night
Paradoxes in physics Paradoxes in physics

1997 © Astronoo.com − Astronomy, Astrophysics, Evolution and Ecology.
"The data available on this site may be used provided that the source is duly acknowledged."
Contact −  Legal mentions −  English Sitemap −  Full Sitemap −  How Google uses data