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Bodies of meteoritic size (1-I00 cm) would survive atmospheric entry, and deliver their organic compounds intact. Larger bodies would vaporize on impact, causing any organic compounds to revert to CO and H 2. But on expansion and cooling of the gas ball, catalytic reactions might commence on the surfaces of dust grains. Apart from prebiotic organic matter, some portion of the Earth's petroleum may have originated by this route, as argued by Robinson (1966), Porfir'ev (1971), and others. 2 FTT Reactions on the Earth There are indications that FTT reactions also take place in petroleum deposits.

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