Evolution: Cosmology & Planetary Science
[Before ~4.0 BYA]
Proposed Origin: The observable universe evolved from an early hot, extremely dense state.
This pre-origin theory is acceptable for ΛCDM cosmology. But if tied to metaphysics, it should be separated.
The Big Bang Theory
The start of cosmic expansion
Energy/particle epochs: fractions of a second onward
Atoms (recombination): ~13.7996 BYA
Cosmic Dark Ages: ~13.8 to ~13.6 BYA
First stars form: ~13.6–13.7 BYA
Ignition of First stars (Pop III): Population III stars remain theoretical unobserved despite strong indirect evidence.
Reionization begins: the ultraviolet light from early stars ionizes hydrogen.
First galaxies: Forms from dark matter halos.
Galaxies grow: Through mergers and star formation.
First generations of stars: Synthesis of heavy elements (carbon, oxygen, iron) via nuclear fusion and supernovae.
Heavy elements: Seed future planetary systems.
The Milky Way: Forms and evolves during this period.
Star formation rate: Peaks and then declines.
Spiral galaxies (like Milky Way): Develop stable structures.
Multiple generations of stars: Enriched interstellar space with metals. Conditions for rocky planets become common.
Solar system forms: ~4.57 BYA →
A region of the Milky Way collapses into a protoplanetary disk.
The Sun ignites at the center.
Planets, moons, asteroids, and comets form from remaining material.
Earth forms: ~4.54 BYA
Earth accretion and differentiation
Magma oceans and intense volcanism
Heavy meteoritic bombardment
Moon formation
Early atmosphere from outgassing
Evidence of liquid water (zircons)
Zircon crystals and meteorites as primary evidence