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Microstructural Indications For Protoenstatite Precursor Of Cometary Mgsio_3 Pyroxene: A Further High-temperature Component Of Comet Wild 2

机译:Mgsio_3 y彗星原钙钛矿前体的微观结构指示:野彗星2的另一个高温成分

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摘要

Microstructural studies by transmission electron microscope (TEM) techniques of a microtomed cometary enstatite (Mg/Si 0.858; Fe/Si 0.027; Ca/Si 0.01; Al/Si 0.009; Cr/Si 0.01) from Wild 2 sampled during NASA's Stardust mission were conducted. The enstatite is characterized by high stacking disorder parallel (100) which includes alternating clinoenstatite (CLEN) and orthoenstatite (OREN) lamellae and (100) twins. In addition a widespread occurrence of 4.5 A wide half-planes parallel (100) are detected, which leads to 13.5 and 22.5 A polytypes of the structure. These microstructural features are indicative of the direct transformation from a protoenstatite (PEN) precursor, which requires temperatures of more than 1275 K and rapid cooling (>10 K hr~(-1)). Our finding represents a further high-temperature component originally present in the cold icy region where comet Wild 2 was formed.
机译:美国国家航空航天局(NASA)的星尘任务期间从野生2中取样的微米级彗星顽辉石(Mg / Si 0.858; Fe / Si 0.027; Ca / Si 0.01; Al / Si 0.009; Cr / Si 0.01)的透射电子显微镜(TEM)显微组织研究是进行。顽辉石的特征在于高堆积无序平行体(100),其包括交替的斜铁辉石(CLEN)和正辉石(OREN)的薄片和(100)孪晶。另外,检测到广泛存在平行于(100)的4.5A宽半平面,这导致结构的13.5A和22.5A多型。这些微观结构特征指示了从原生钙钛矿(PEN)前体的直接转变,这需要温度超过1275 K和快速冷却(> 10 K hr〜(-1))。我们的发现代表了最初存在于形成Wild 2彗星的冰冷地区的另一个高温成分。

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