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Comet 81P/Wild 2 under a microscope.

机译:彗星81P / Wild 2在显微镜下观察。

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摘要

The Stardust spacecraft collected thousands of particles from comet 81P/Wild 2 and returned them to Earth for laboratory study. The preliminary examination of these samples shows that the nonvolatile portion of the comet is an unequilibrated assortment of materials that have both presolar and solar system origin. The comet contains an abundance of silicate grains that are much larger than predictions of interstellar grain models, and many of these are high-temperature minerals that appear to have formed in the inner regions of the solar nebula. Their presence in a comet proves that the formation of the solar system included mixing on the grandest scales.
机译:星尘号飞船从81P / Wild 2彗星中收集了数千个粒子,并将其返回地球进行实验室研究。对这些样品的初步检查表明,彗星的不挥发部分是太阳和太阳系起源的不平衡物质。彗星含有大量的硅酸盐晶粒,比星际晶粒模型的预测要大得多,而且其中许多是似乎已在太阳星云内部形成的高温矿物。它们在彗星中的存在证明了太阳系的形成包括了最大尺度的混合。

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