根据这些玻璃质微球粒的物理、表面结构构造及常量元素等特征，可认为是微玻璃陨石。
These spherulites are identified as glassy microtektites by their surficial texture, physical and optical properties, and common element contents.
从而认为，这些玻璃微粒并非为海底火山物质，而是典型的微玻璃陨石，并指出它们有可能起源于月球火山作用。
It is bilived that these glassy particles are not volcanic materials in ocean floor but are typical microtektites. It is suggested that they may be of lunar volcanic origin.
从而认为，这些玻璃微粒并非为海底火山物质，而是典型的微玻璃陨石，并指出它们有可能起源于月球火山作用。
It is bilived that these glassy particles are not volcanic materials in ocean floor but are typical microtektites. It is suggested that they may be of lunar volcanic origin.
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