Delivery of Organic Matter to the Early Earth

被引:3
|
作者
Martins, Zita [1 ,2 ]
Pasek, Matthew A. [3 ]
机构
[1] Univ Lisbon, Inst Super Tecn, Inst Mol Sci, Ctr Quim Estrutural, P-1049001 Lisbon, Portugal
[2] Univ Lisbon, Inst Super Tecn, Dept Chem Engn, P-1049001 Lisbon, Portugal
[3] Univ S Florida, Sch Geosci, 4202 E Fowler Ave NES 204, Tampa, FL 33620 USA
关键词
organic matter; exogenous delivery; early Earth; prebiotic molecules; MONOCARBOXYLIC ACIDS; EXOGENOUS DELIVERY; SHOCK SYNTHESIS; AMINO-ACIDS; MICROMETEORITES; CHONDRITES; MOLECULES; COMETARY; ORIGIN;
D O I
10.2138/gselements.20.1.19
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The inner Solar System-including the planet Earth-was heavily bombarded by comets, asteroids, and their fragments (i. e., meteorites, micrometeorites, and interplanetary dust particles) from 4.56 to about 3.5 billion years ago. This bombardment resulted in a rich assortment of organics delivered to the Earth, as comets and many asteroids contain carbonaceous material. These organic compounds were likely further processed on the early Earth (e.g., by impact-shock reactions), providing a feedstock of prebiotic molecules to the crust and oceans. In this chapter, we review the mechanisms of organic matter delivery to the primitive Earth, further reactions and processing, and the importance of exogenous material in the evolution of our planet and life.
引用
收藏
页码:19 / 23
页数:5
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