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塔吉什湖陨石中的有机小球体:原太阳盘的遗迹。

Organic globules in the Tagish Lake meteorite: remnants of the protosolar disk.

作者信息

Nakamura-Messenger Keiko, Messenger Scott, Keller Lindsay P, Clemett Simon J, Zolensky Michael E

机构信息

Robert M. Walker Laboratory for Space Science, Astromaterials Research and Exploration Science Directorate, NASA Johnson Space Center, Houston, TX 77058, USA.

出版信息

Science. 2006 Dec 1;314(5804):1439-42. doi: 10.1126/science.1132175.

Abstract

Coordinated transmission electron microscopy and isotopic measurements of organic globules in the Tagish Lake meteorite shows that they have elevated ratios of nitrogen-15 to nitrogen-14 (1.2 to 2 times terrestrial) and of deuterium to hydrogen (2.5 to 9 times terrestrial). These isotopic anomalies are indicative of mass fractionation during chemical reactions at extremely low temperatures (10 to 20 kelvin), characteristic of cold molecular clouds and the outer protosolar disk. The globules probably originated as organic ice coatings on preexisting grains that were photochemically processed into refractory organic matter. The globules resemble cometary carbon, hydrogen, oxygen, and nitrogen (CHON) particles, suggesting that such grains were important constituents of the solar system starting materials.

摘要

对塔吉什湖陨石中有机球粒进行的透射电子显微镜和同位素测量显示,它们的氮-15与氮-14的比率(是地球的1.2至2倍)以及氘与氢的比率(是地球的2.5至9倍)有所升高。这些同位素异常表明在极低温度(10至20开尔文)下的化学反应过程中发生了质量分馏,这是冷分子云及原太阳外部圆盘的特征。这些球粒可能起源于先前存在颗粒上的有机冰涂层,这些涂层经光化学作用转化为难熔有机物质。这些球粒类似于彗星的碳、氢、氧和氮(CHON)颗粒,这表明此类颗粒是太阳系起始物质的重要组成部分。

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