数字模拟表明小行星 (101955) Bennu 和 (162173) Ryugu 可能是第二代或更后一代的废墟堆
K J Walsh1, R-L Ballouz2, W F Bottke3
1Southwest Research Institute, Boulder, CO, USA. kwalsh@boulder.swri.edu.
Nature communications
|July 5, 2024
概括
接近地球的小行星Ryugu和Bennu很可能是第二代遗留物,而不是来自最初的小行星碰撞. 这解释了它们的表面年龄比它们的母小行星家族年轻.
科学领域:
- 小行星科学小行星科学
- 行星地质学 行星地质学
- 碰撞动态 碰撞动态
背景情况:
- 碎片堆小行星是灾难性碰撞的碎片.
- 接近地球的小行星Ryugu和Bennu与主要小行星带的小行星家族有关.
- 表面年龄数据表明Ryugu和Bennu比他们的家长家庭年轻.
研究的目的:
- 调查近地小行星Ryugu和Bennu的起源.
- 调和这些小行星及其假定家族之间的年龄差异.
- 确定传送到近地空间的小行星残骸的生成.
主要方法:
- 结合碰撞和动态进化模型.
- 对小行星家族成员的分析.
- 表面年龄和火山口保留年龄的比较.
主要成果:
- 瑞古和本努很可能是后来的破坏的第二代遗留物.
- 大约80%和60%的新波拉纳和尤拉利亚家族的小行星是第二代.
- 自上次破坏以来的年轻的中位数年龄与火山口保留年龄一致.
结论:
- 通过以后的破坏事件,可以将小行星年龄与家族成员身份相协调.
- 很大一部分近地小行星是第二代或后一代的遗骸.
- 这一发现影响了我们对小行星进化和传递机制的理解.
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