Welcome to4.6 billion years agoEarth. A barren world where we could not breathe. It was a time of extreme turmoil β rivers of lava flowed across the surface, and relentless meteor impacts scarred the land. By looking at the craters on the Moon, we can imagine the staggering landscape of early Earth.
4, NH3, H2O, H2, CO2 (no O2)
Energy Sources: Lightning, High Heat, UV Radiation
Nature's "Laboratory" for the Evolution of Life
The composition of the primitive atmosphere was vastly different from today's. It consisted of water vapor, hydrogen, ammonia, methane, carbon dioxide, hydrogen sulfide, and other gases released by volcanic eruptions. The most crucial point:There was absolutely no free oxygen in the primitive atmosphere. This reducing environment was the prerequisite for chemical evolution.
- Energy Trigger: Lightning in the sky, intense ultraviolet radiation, and the high temperatures generated by tectonic activity broke the chemical bonds of small inorganic molecules.
- Primordial Ocean: As the surface cooled, rainfall gathered to form the primordial ocean. Small organic molecules accumulated here with the rainwater, creating the famous "primordial soup."
Key Takeaway
The primordial ocean was the cradle of life. Here, over vast stretches of time and driven by energy, non-living matter gradually made the leap from inorganic to organic compounds, and from simple organic molecules to complex primitive life forms.