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Evidence of space weathering in regolith breccias II: Asteroidal regolith breccias

机译:go石角砾岩的空间风化证据II:小行星的re石角砾岩

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Space weathering products, such as agglutinates and nanophase iron-bearing rims are easily preserved through lithification in lunar regolith breccias, thus such products, if produced, should be preserved in asteroidal regolith breccias as well. A study of representative regolith breccia meteorites, Fayetteville (H4) and Kapoeta (howardite), was undertaken to search for physical evidence of space weathering on asteroids. Amorphous or npFe0-bearing rims cannot be positively identified in Fayetteville, although possible glass rims were found. Extensive friction melt was discovered in the meteorite that is difficult to differentiate from weathered materials. Several melt products, including spherules and agglutinates, as well as one irradiated rim and one possible npFe0-bearing rim were identified in Kapoeta. The existence of these products suggests that lunar-like space weathering processes are, or have been, active on asteroids.
机译:太空风化产物,例如凝集物和含铁的纳米相轮辋,很容易通过石化保存在月球长角砾岩角砾岩中,因此,如果产生此类产品,也应保存在小行星角砾岩角砾岩中。进行了代表性代表性的巨石角砾岩陨石,费耶特维尔(H4)和卡普埃塔(钙矾石)的研究,以寻找小行星上空间风化的物理证据。尽管发现了可能的玻璃轮辋,但在费耶特维尔仍无法正确鉴定出非晶或带有npFe0的轮辋。在陨石中发现了广泛的摩擦熔体,很难与风化材料区分开。在卡波埃塔(Kapoeta)中发现了几种熔融产品,包括小球和凝集物,以及一个辐照轮辋和一种可能的含npFe0的轮辋。这些产品的存在表明类似月球的空间风化过程已经或已经在小行星上活跃。

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