The study of how life's building blocks formed and became available on early planets.The origin of life is the scientific inquiry into how non-living chemical compounds on early Earth (or other planets) assembled into the first self-replicating, metabolically active structures. This field bridges chemistry, geology, and biology, seeking to explain the transition from simple organic molecules to the first cells. Research in this area often focuses on the conditions of early planetary environments, such as the availability of water, energy sources, and organic building blocks like amino acids and nucleotides.
The modern scientific study of abiogenesis began with the Miller-Urey experiment in 1953, which demonstrated that amino acids could form spontaneously under simulated early Earth conditions. Earlier ideas date back to Darwin's 'warm little pond' hypothesis and Oparin's 1924 proposal of a 'primordial soup'.
Scientists investigate prebiotic chemistry by simulating early Earth conditions in the lab, such as lightning discharges in a reducing atmosphere (the Miller-Urey experiment) or hydrothermal vents on the ocean floor. The key steps involve the formation of organic monomers, their polymerization into larger molecules like RNA, and the eventual emergence of self-replicating systems. Recent work also considers the role of meteorites delivering organic compounds and the potential for life to arise in diverse environments, including those with high radiation or extreme pH.
Understanding the origin of life informs astrobiology, guiding the search for habitable exoplanets and biosignatures, and also inspires synthetic biology efforts to create artificial life-like systems.
Cyanide, often considered a deadly poison, is now recognized as a likely key player in prebiotic chemistry, as it can catalyze the formation of nucleotides and amino acids under early Earth conditions.
























