EE refers to Early Earth conditions, which can be simulated in a laboratory setting.
Heat is supplied to water, mimicking the sun's effect on ocean waters, causing evaporation.
The evaporated water moves to a bowled area representing the atmosphere.
Experiment runs using various combinations of gases such as methane, ammonia, and hydrogen.
These gases mimic volcanic output, simulating early atmospheric conditions.
Water vapor interacts with gases; electrodes create arcs simulating lightning strikes.
Cold water circulates around the atmosphere model to condense water vapor, forming clouds and rain.
This rain returns to the ocean, creating a cyclical model of water exchange.
There's criticism over what the ocean's composition would have been, as it's not assumed to be pure water.
Future technology could establish better understandings of ancient ocean and atmosphere characteristics.
In later studies, researchers discovered 60 different amino acids in the products of these simulated conditions.
Speculation suggests that RNA can be produced abiotically in conditions similar to early Earth, highlighting its potential role in life's origins.
RNA, while not alive, functions similarly to roles in biological processes, suggesting its importance in early life development.
It is clarified that life's origins are distinct from viruses.
Discussion transitions to the three domains of life: Eubacteria, Archaea, and Eukarya.
Eukarya, encompassing organisms with true nuclei (e.g., euglena, amoebas), is contrasted with prokaryotic domains.
Prokaryotes lack a nucleus and are responsible for various life forms, including extremophiles (e.g., bacteria in Yellowstone