Currently the most widely accepted scientific explanation for the origin of the Universe, supported by observational evidence.
- Singularity: About 13.8 billion years ago, all matter and energy in the universe were concentrated in a tiny point of infinite density and temperature.
- Initial Expansion: This 'primeval atom' expanded rapidly. It was an expansion of space itself, not an explosion inside empty space.
- Cooling & Matter: As it expanded, the temperature dropped. Energy converted into subatomic particles (protons, neutrons), which formed hydrogen and helium during the first few minutes (nucleosynthesis).
- Redshift: Light from distant galaxies is shifted toward red wavelengths, showing they are moving away from us (Hubble Expansion).
- CMBR: Cosmic Microwave Background Radiation is the faint thermal echo of the hot Big Bang, discovered in 1964. It is uniform across the sky at 2.7 Kelvin.
- Abundance of Light Elements: The observed ratio of 75% hydrogen and 25% helium matches calculations of early universe cooling.