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自从蒙格(Monge)等人对1806年3月15日降落在法国的阿拉斯碳质球粒陨石含碳化合物进行了测定以后,一个多世纪以来,鉴定各类陨石中的有机化合物和研究它们的成因越来越引起人们的兴趣。因为陨石的物质组成和成因与太阳系原始星云密切相关,所以研究陨石有机化合物的成因可以帮助我们认识太阳系的演化过程,深入了解地球独立成行星前、后的有机质的产生和状态以及这种最原始的有机化合物对发展地球上有
Since Monge et al. Determined the carbonaceous compounds of Arrasian carbonaceous chondrites that landed in France on March 15, 1806, for more than a century, identifying and studying organic compounds in various types of meteorites The causes of more and more aroused people’s interest. Because the material composition and genesis of meteorites are closely related to the original solar nebula, studying the genesis of meteorite organic compounds can help us understand the evolution of the solar system, understand the formation and state of organic matter before and after the Earth’s independent planets, and the most primitive The development of organic compounds on the earth there