Science. 1970 Jan 30;167(3918):691-3. doi: 10.1126/science.167.3918.691.
A breccia sample (10023) from the moon was found to have a strong and fairly stable remanent magnetization. If this sample was not magnetized by local fields in the spacecraft or in the lunar receiving laboratory, it must have been magnetized on the moon. This could have happened in a variety of ways, such as cooling through the Curie temperature, by comitinuous thermal cycling, or by impact, but all of these require the presence ofr a magnetic field. Such a field could have been of internal origin in the moon, or it could have been a residual effect from the earth's magnetic field at a time when the moon and the earth were much closer together. Thermomagnetic studies identify the presence of iron with about 1 percent nickel (igneous). iron with abiout 5 to 10 percent nickel (meteoritic), iron with about 33 percent or more nickel (meteoritic), and ilmenite.
一块取自月球的角砾岩样本(10023)显示出很强且相当稳定的剩余磁化强度。如果这个样本不是在航天器或月球接收实验室中的局部场中被磁化的,那么它一定是在月球上被磁化的。这种磁化可能通过多种方式发生,例如通过居里温度冷却、连续热循环或撞击,但所有这些都需要磁场的存在。这样的磁场可能是月球内部的起源,也可能是月球和地球距离较近时地球磁场的残余效应。热磁研究确定了存在约 1%镍的铁(火成岩)、约 5%至 10%镍的铁(陨石)、约 33%或更多镍的铁(陨石)和钛铁矿。