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彗星运送有机分子到早期的地球
C F Chyba1, P J Thomas, L Brookshaw
1Laboratory for Planetary Studies, Cornell University, Ithaca, NY 14853, USA.
概括
早期地球可能从小行星和彗星撞击中获得了先生物的有机分子. 密集的早期大气层允许完好无损的有机分子传递,这对生命起源至关重要.
科学领域:
- 天体生物学 天体生物学
- 行星科学 行星科学
- 地质化学 地质化学
背景情况:
- 猜测地球在重轰炸 (45亿至38亿年前) 期间从小行星和彗星撞击中增加了先生物有机分子.
- 之前了解大气进入和对有机分子生存的影响.
研究的目的:
- 研究从彗星和小行星到早期地球的先生物有机分子的生存和传递.
- 为了确定有机分子可以完好无损地交付的条件.
主要方法:
- 模拟彗星-小行星大气相互作用,包括空中制动和冲击热解.
- 在不同冲击速度和大气密度下分析有机分子生存率.
- 在早期地球上计算有机分子积聚率.
主要成果:
- 有机分子无法在超过大约10公里/秒的冲击中生存.
- 在1-bar大气层中的空中制动不足以减缓小彗星/小行星低于这个临界速度.
- 在45亿年前,可信的密度高 (10巴二氧化碳) 的早期大气层能够以每年106-107公斤的速度提供完整的彗星有机物.
结论:
- 密集的早期大气层对于从外星冲击中传递完整的先生物有机分子至关重要.
- 有机分子积累的速度随着时间的推移而下降,其半衰期约为108年.
- 这种传递机制为地球生命起源提供了有机物质的重要来源.
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