The article synthesizes what scientists know about early Earth from scarce “Hadean archives,” especially detrital zircons from Australia’s Jack Hills, and it contrasts those clues with experimental routes for making key molecular building blocks of life. Zircons are used as a record for when liquid water, early crust formation, and possible weathering may have occurred around 4.4 billion years ago, but major uncertainties remain about early surface conditions.

The review then evaluates several proposed habitats for the emergence of life, including tidal flats, small warm ponds, submarine alkaline hydrothermal systems, evaporative soda lakes, and reactor-like “nuclear reactor–geyser” scenarios, as well as ideas involving material delivered from space. While lab studies have shown plausible ways to form amino acids, nucleobases, sugars, fatty acids, thiols, phosphorylated intermediates, protometabolic networks, and membrane-like structures, the review concludes that no one setting fully explains how non-living chemistry became life.