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The Big Bang
Consider something unbelievably tiny, unbelievably dense, and incredibly hot. Then, suddenly, space, time, and all molecular matter burst in ways that no words can express. What is known is that the Universe expanded at an unfathomable rate in a fraction of a second. Some recognised subatomic particles and fundamental forces emerged as a result of this expansion. The Universe then began to cool drastically, to around 1 billion degrees Celsius, allowing energy and ultimately matter (plasma of nuclei, electron and photons) to emerge.
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Cosmic Microwave Background (CMB)
3,80,000 years after The Big Bang
As the universe expanded, plasma grew cooler and cooler. The universe cooled down further to 3000 K, making it possible for the nuclei in the plasma to gain electrons and become full-fledged neutral Hydrogen and Helium atoms.
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First Stars Stabilises
The gravity that was trying to squash the star together was pushed back by the fusion at the center which created a balance. Within a few hundred million years after the Big Bang, the first generation of stars, known as Population III stars, were formed. After CMB, these stars were the first sour...
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First Stars
About 200 million years after The Big Bang
Due to gravity, hydrogen and helium clouds began to clump together. Tiny imperfections. Little knots, wrinkles, and flaws began attracting nearby particles of matter. The clumps grew, became more massive, and attracted more particles. Hence, it mad...
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Cosmic Dark Age
The entire universe was made up of Hydrogen and helium gas clouds with no stars and planets.
After the release of CMB, nothing in the Universe radiated light until around 200 million years after the Big Bang when the first stars began to form.
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The First Galaxies, clusters and superclusters
About 1 Billion years after The Big Bang
Stars formation happened almost everywhere in universe. Thus we have billions and billions of stars. Galaxies were formed out of these swirling clouds of stars and gas in space. Gravity sends these objects careening into one another...
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Threshold II: Formation of the First Stars
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