Sandford Scott A, Engrand Cecile, Rotundi Alessandra
NASA Ames Research Center, Moffett Field, CA, USA.
Centre de Sciences Nucléaires et de Sciences de la Matière-CSNSM Bat. 104, 91405 Orsay-Campus, France.
Elements (Que). 2016;12(3):185-189. doi: 10.2113/gselements.12.3.185. Epub 2016 Jun 1.
Organics are observed to be a significant component of cosmic dust in nearly all environments were dust is observed. In many cases only remote telescope observations of these materials are obtainable and our knowledge of the nature of these materials is very basic. However, it is possible to obtain actual samples of extraterrestrial dust in the Earth's stratosphere, in Antarctic ice and snow, in near-Earth orbit, and via spacecraft missions to asteroids and comets. It is clear that cosmic dust contains a diverse population of organic materials that owe their origins to a variety of chemical processes occurring in many different environments. The presence of isotopic enrichments of D and N suggests that many of these organic materials have an interstellar/protosolar heritage. The study of these samples is of considerable importance since they are the best preserved materials of the early Solar System available.
在几乎所有观测到尘埃的环境中,有机物都是宇宙尘埃的重要组成部分。在许多情况下,只能通过远程望远镜对这些物质进行观测,而且我们对这些物质性质的了解非常基础。然而,有可能在地球平流层、南极冰雪、近地轨道以及通过前往小行星和彗星的航天器任务获取地外尘埃的实际样本。很明显,宇宙尘埃包含各种各样的有机物质,其起源归因于许多不同环境中发生的各种化学过程。D和N的同位素富集表明,这些有机物质中的许多都有星际/原太阳的传承。对这些样本的研究具有相当重要的意义,因为它们是早期太阳系现存保存最完好的物质。