煤渣
发表于 2025-4-1 02:59:24
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爱管闲事
发表于 2025-4-1 08:31:51
Lianet Camara,Mourik Bueno de Mesquitasolar nebula, by catalytic (Fischer-Tropsch) reactions of CO, H., and NH. at 360–400 K, ∼ 10. atm. The onset of these reactions was triggered by the formation of suitable catalysts (magnetite, hydrated silicates) at these temperatures. Such reactions may be a source of prebiotic carbon compounds on the inner planets, and interstellar molecules.