Can the Solar Nebular field be recorded through impacts?

我正在研究早期太阳系中小行星之间低速撞击（<2公里/秒）的可能性，以记录环境磁场。使用牛津大学固体力学与材料工程小组精心设计的实验，我们能够在磁场中撞击球粒陨石前体类似物，然后进一步检查样品的磁性。我们希望为陨石的磁化提供另一种解释，展示行星状星云中低速撞击的重要作用。

I am studying the potential for low-velocity impacts (<2km/s) in the early solar system between asteroids to have recorded an ambient magnetic field. Using carefully designed experiments with the Solid Mechanics & Materials Engineering group at Oxford, we are able to impact a chondrite precursor analog within a magnetic field and then further examine the sample's magnetic properties. We hope to offer an alternative explanation to the magnetisation of meteorites, displaying the significant role of low-velocity impacts in planetary nebulae.