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81P/怀尔德2号彗星尘埃与彗星际尘埃的比较。

Comparison of comet 81P/Wild 2 dust with interplanetary dust from comets.

作者信息

Ishii Hope A, Bradley John P, Dai Zu Rong, Chi Miaofang, Kearsley Anton T, Burchell Mark J, Browning Nigel D, Molster Frank

机构信息

Institute of Geophysics and Planetary Physics, Lawrence Livermore National Laboratory, Livermore, CA 94550, USA.

出版信息

Science. 2008 Jan 25;319(5862):447-50. doi: 10.1126/science.1150683.

Abstract

The Stardust mission returned the first sample of a known outer solar system body, comet 81P/Wild 2, to Earth. The sample was expected to resemble chondritic porous interplanetary dust particles because many, and possibly all, such particles are derived from comets. Here, we report that the most abundant and most recognizable silicate materials in chondritic porous interplanetary dust particles appear to be absent from the returned sample, indicating that indigenous outer nebula material is probably rare in 81P/Wild 2. Instead, the sample resembles chondritic meteorites from the asteroid belt, composed mostly of inner solar nebula materials. This surprising finding emphasizes the petrogenetic continuum between comets and asteroids and elevates the astrophysical importance of stratospheric chondritic porous interplanetary dust particles as a precious source of the most cosmically primitive astromaterials.

摘要

星尘号任务将已知的外太阳系天体——81P/怀尔德2号彗星的首个样本带回了地球。该样本预计与球粒多孔星际尘埃颗粒相似,因为许多乃至可能所有此类颗粒都源自彗星。在此,我们报告称,球粒多孔星际尘埃颗粒中最丰富且最易识别的硅酸盐物质在返回的样本中似乎并不存在,这表明81P/怀尔德2号中本地的外星云物质可能很稀少。相反,该样本类似于来自小行星带的球粒陨石,主要由内太阳系星云物质组成。这一惊人发现强调了彗星和小行星之间的成因连续体,并提升了平流层球粒多孔星际尘埃颗粒作为宇宙中最原始天体物质珍贵来源的天体物理学重要性。

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