Chaves Laura C, Thompson Michelle S
Department of Earth, Atmospheric, and Planetary Sciences, 550 Stadium Mall Drive, West Lafayette, IN 47907 USA.
Earth Planets Space. 2022;74(1):124. doi: 10.1186/s40623-022-01683-6. Epub 2022 Aug 9.
Transmission electron microscopy analyses of the polymineralic regolith particle RC-MD01-0025 show microstructural and microchemical characteristics indicative of space weathering on the surface of asteroid Itokawa. The depletion of sulfur and nickel was identified in space weathered rims on troilite and pentlandite minerals. This corresponds to the first report of nickel depletion in samples returned from asteroid Itokawa by the Hayabusa mission. Microstructurally, the sulfide minerals present crystalline rims and the olivine presents both crystalline and amorphous zones in the rim. These results suggest that sulfides might be more resistant to amorphization caused by solar wind irradiation. The space weathering features identified in the regolith particle analyzed here are likely formed via solar wind irradiation. Additionally, the differences in the space weathering features in olivine, pentlandite, and troilite suggest that silicates and sulfides respond differently to the same space weathering conditions in interplanetary space.
对多矿物月壤颗粒RC-MD01-0025的透射电子显微镜分析显示,其微观结构和微化学特征表明丝川小行星表面存在空间风化。在陨硫铁和镍黄铁矿矿物的空间风化边缘发现了硫和镍的损耗。这与隼鸟号任务从丝川小行星带回的样本中首次报告的镍损耗情况相符。在微观结构上,硫化物矿物呈现出结晶边缘,而橄榄石在边缘既有结晶区又有无定形区。这些结果表明,硫化物可能对太阳风辐照引起的非晶化更具抗性。此处分析的月壤颗粒中识别出的空间风化特征可能是通过太阳风辐照形成的。此外,橄榄石、镍黄铁矿和陨硫铁中空间风化特征的差异表明,硅酸盐和硫化物在行星际空间中对相同的空间风化条件反应不同。