Can the Solar Nebular field be recorded through impacts?

太阳星云场可以通过撞击记录下来吗？

• 批准号: 2151024
• 金额: --
• 依托单位: Imperial College London
• 依托单位国家: 英国
• 项目类别: Studentship
• 财政年份: 2018
• 资助国家: 英国
• 起止时间: 2018 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=studentship-2151024
• 关键词: Solar; Nebular; field; recorded; through

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.

我正在研究早期太阳系小行星之间低速碰撞(&lt；2公里/S)的可能性，以记录下周围的磁场。利用牛津大学固体力学和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，展示低速撞击在行星状星云中的重要作用。