Kerridge J F, Mariner R, Flores J, Chang S
Institute of Geophysics, UCLA 90024, USA.
Orig Life Evol Biosph. 1989;19(6):561-72. doi: 10.1007/BF01808118.
Carbonaceous residues from a variety of laboratory syntheses yield release patterns for C and H isotopes during stepwise combustion that fail to mimic the striking patterns characteristic of meteoritic kerogen-like residues that otherwise superficially resemble them. It seems likely that the meteoritic material comprises a complex mixture of substances having different origins and/or synthesis conditions.
来自各种实验室合成的碳质残渣在逐步燃烧过程中产生的碳和氢同位素释放模式，无法模拟陨石类干酪根残渣所特有的显著模式，而这些陨石类干酪根残渣在表面上与它们相似。陨石物质似乎可能由具有不同起源和/或合成条件的物质的复杂混合物组成。
