Can life be built from silicon rather than carbon? This essay stages the question as a trial. The prosecution assembles the terrestrial case against silicon — the atomic geometry that denies it stable double bonds, the tyranny of oxygen that turns its chains to sand, and the "monotony problem" that starves its molecular vocabulary of the variety a genome needs. The defense then walks the length of that wall and finds it ends at the edge of Earth's warm, wet, oxygenated conditions: on cold anoxic worlds like Titan, in Venus's acid clouds, and in the crushing heat of planetary interiors, the fitness landscape redraws itself and silicon's liabilities become assets. Laboratory milestones — the kinetically stabilized silicon double and triple bonds once thought impossible, and Frances Arnold's directed evolution of an enzyme that forges carbon–silicon bonds inside living cells — show the boundary between life and silicon to be permeable rather than sealed. Yet stability is not origination, and the unsolved mystery of how life began humbles confident verdicts in either direction. The essay closes on suspension: the honest recognition that silicon life is chemically permitted in genuinely existing conditions we have barely begun to examine — a question held open, pointing outward, worth the instruments to answer.
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Alexandru C. Stan (2026) studied this question.
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