月球陨石是地球以外未燃尽的宇宙流星脱离原有运行轨道或程碎块飞快散落到地球或其它行星表面的石质的、铁质的或是石铁混合物质 ， 也称“陨星” 。大多数陨石来自于火星和木星间的小行星带 ， 小部分来自月球和火星 。陨石大体可分为；石质陨石 ， 铁质陨石 ， 石铁混合陨石 。每类陨石下面又有它们的子项 。

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月球陨石可分为火山岩和沉积岩两大类 ， 月球玄武岩是构成月球的主要岩石之一 ， 颜色为黑色 ， 白色 ， 暗紫色 ， 紫红色 ， 绿色 ， 墨绿色 ， 灰绿色 ， 黄色 ， 棕黄色 ， 混合色等 。成斑状结构的构造和杏仁构造并存在黑云母 。月球陨石中常见的硫化物有陨硫铁 ， 黄铁矿 ， 黄铜矿 ， 方黄铜矿 ， 硫镍铁矿 ， 及尚不清楚的矿物 。

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属火山岩的月球陨石表面呈现的透明状熔壳 ， 是月岩中的透明物质经高温熔融后形成的 。其它熔融现象如:熔壳 ， 熔流纹 ， 熔流线 ， 槽沟 ， 熔蚀坑 ， 和定向坠落形成的棱角都十分明显 。月球陨石的透明状熔壳特征 ， 是判断月球陨石标志 。因坠落地球时间太久 ， 遭严重风蚀的月球火成岩陨石 ， 失去透明状熔壳的可能性会大增 ， 通常这种现象不会影响对月球陨石的终确认 。月球陨石中常见成粒状 ， 块状的聚片双晶集合体斜长岩及微班熔融角砾岩 。颜色为 ， 无色 ， 白色 ， 暗灰色 ， 肉红色 ， 粉红色 ， 黄色 ， 浅黄色 ， 绿色 ， 显玻璃光泽透明至半透明 。板状或扁柱状的单晶常为白色 ， 板状单晶内可见针状橄榄石存在 。月球陨石中具有角砾斜长岩的特征 ， 是确认月球陨石的重要科学依据 。该石头有一个非常平整的切割面 。这个面上与整个石头的外部有一层玻璃质的熔壳 ， 并且可以看到犹如拇指印一样的痕迹 。同时该石头硬度高 ， 比重大 。从该角度看：石头的外部有规则德尔横向纹理 ， 底部有一个小平面 ， 边缘有碰撞发生的残缺 。这是一块矿物质和微量元素丰富的 ， 定向陨落的月球陨石 ， 极具深入研究和收藏的意义和价值 ， 属于经典的月球陨石 。

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【absorption costing cosmicbreak】Lunar meteorites are stony, iron, or a mixture of stone and iron, also known as "meteorites", which are unburned cosmic meteors outside the earth that break away from their original orbit or path fragments and quickly scatter on the surface of the earth or other planets. Most meteorites come from the asteroid belt between Mars and Jupiter, and a small number come from the moon and Mars. Meteorites can be roughly divided into; Stone meteorite, iron meteorite, stone iron mixed meteorite. Each type of meteorite has its subitems. Lunar meteorites can be divided into volcanic rocks and sedimentary rocks. Lunar basalt is one of the main rocks that make up the moon. Its colors are black, white, dark purple, purplish red, green, dark green, grayish green, yellow, brownish yellow, mixed colors, etc. Porphyritic structure and amygdaloid structure with biotite. Common sulfides in lunar meteorites include meteorite pyrite, pyrite, chalcopyrite, chalcopyrite, pyrite, and unknown minerals. The transparent molten crust on the surface of the lunar meteorite, which belongs to volcanic rock, is formed after the transparent material in the lunar rock is melted at high temperature. Other melting phenomena such as molten shell, molten flow lines, molten flow lines, grooves, corrosion pits, and edges and corners formed by directional falling are very obvious. The characteristics of transparent molten crust of lunar meteorites are the criteria for judging lunar meteorites. Because the time of falling to the earth is too long, the possibility of losing the transparent molten shell of the moon igneous rock meteorite that has been severely wind eroded will greatly increase. Usually, this phenomenon will not affect the final confirmation of the moon meteorite. Granular and massive agglomerate bicrystal aggregate anorthosite and micro ban molten breccia are common in lunar meteorites. The color is colorless, white, dark gray, flesh red, pink, yellow, light yellow, green, showing glassy luster, transparent to translucent. Tabular or oblate columnar single crystals are usually white, and acicular olivine can be seen in tabular single crystals. The characteristics of breccia anorthosite in lunar meteorites are important scientific basis for confirming lunar meteorites. The stone has a very flat cutting surface. There is a layer of glass melting shell on this surface and the outside of the whole stone, and you can see the traces like thumb prints. At the same time, the stone has high hardness and a large proportion. From this point of view: the outside of the stone has a regular del transverse texture, the bottom has a small plane, and the edge has the deformity of collision. This is a lunar meteorite rich in minerals and trace elements, which falls directionally. It is of great significance and value for in-depth research and collection. It is a classic lunar meteorite.