The planets probably formed from debris cast off from our Sun following its condensation from interstellar gas and dust of a nebula about 5-7 BYA
Earth was semi-molten → gradually cooled enough to form a solid rock crust
Decay of radioactive elements of Earth caused partial melting of the planet's interior, with denser materials making up the core
Differential temperatures of the core and crust set convection currents in motion in the mantle
Gases released into the primitive atmosphere
ammonia = NH3
carbon monoxide = CO
hydrogen sulfide = H2S
methane = CH4
nitrogen = N2
water vapor = H2O
Water vapor condensed and fell through the atmosphere → dissolving gases; "poisonous" rain
Run-off of rainwater from the land carried dissolved minerals into a shallow proto-ocean
The collective materials in the proto-ocean formed a "hot, thin primordial soup"
Ribozyme
An RNA molecule capable of enzymatic actions, e.g., the self-splicing introns of some RNAs, which can excise themselves from the molecule without the help of protein enzymes
The earliest organism may have been no more than a ribozyme
Early Atmosphere probably contained CO2, CO, Nitrogen, Ammonia, Methane. No oxygen to support life
The Earth cooled down → enough for liquid water to form
3.8 BYA
Microscopic organisms → earliest life form
Preserved in the hard structures called "stromatolites"
Prokaryotes and anaerobic heterotrophs that fed on organic molecules in the primordial soup
Cyanobacteria (2.4 BYA) → Earth's first photo-synthesizers, making food using water and the Sun's energy and releasing oxygen as a result
Cyanobacteria catalyzed a sudden, dramatic rise in oxygen → killed microbes that could not tolerate oxygen (Great Oxidation Event)
The Great Oxidation Event was recorded on seafloor rocks → oxidation reaction caused bands of iron
Oxygen levels were lowered eventually → reduce in cyanobacteria number
Anaerobic respiration
C6H12O6 (glucose) → energy + C2H3OH (ethanol) + CO2
In the atmosphere, UV radiation
3CO2 + UV → O3 (ozone) + 3CO (carbon monoxide)
Animal bodies have various cells each doing a distinct job
Microbes are just single cells with no organelles and no nuclei to package their DNA
Eukaryotic organisms → true nucleus, DNA, and membrane-bound organelles evolved between 1.4 and 1.6 BYA
DNA became packaged in nuclei
The new complex cells ("eukaryotic cells") boasted specialized parts playing specialized roles that supported the whole cell
Cells also began living together → benefits (feed efficiently, grow bigger, protection)
Living collectively, cells began to support the needs of the group by each cell doing a specific job (specialization), similar to stem cells
Clusters of specialized, cooperating cells eventually became the first animals (800 MYA)
Poriferans (Sponges) were among the earliest animals
While chemical compounds from sponges are preserved in rocks as old as 700 million years, molecular evidence points to sponges developing even earlier
Oxygen levels in the ocean were still low compared to today, but sponges are able to tolerate conditions of low oxygen
Ediacaran Period aka Vendian Period → more organisms aside from sponges have proliferated
580 MYA
Fossil evidence of Ediacaran organisms can be found in sedimentary rocks around the world
Ediacaran Period → end of global Marinoan glaciation
Distinctive carbonate aka "cap carbonate" from glacial deposits
By the end of the Ediacaran, oxygen levels rose, approaching levels sufficient to sustain oxygen-based life
The early sponges may actually have helped boost oxygen by eating bacteria
Tracks of an organism named Dickinsonia costata suggest that it may have been moved along the sea bottom, presumably feasting on mats of microbes