奇克苏鲁布多环冲击盆地:根据重力分析得出的尺寸和其他特征
概括
奇克苏鲁布撞击结构可能比以前认为的要大得多. 对重力数据的新分析揭示了一个巨大的结构,可能是太阳系内部最大的结构之一.
科学领域:
- 行星地质学 行星地质学
- 撞击石坑研究研究.
- 地质物理学 地质物理学
背景情况:
- 奇克苏鲁布撞击结构与白-第三纪 (K-T) 边界层有关.
- 以前对结构大小的估计可能被低估了.
研究的目的:
- 重新评估奇克苏鲁布撞击事件的大小和结构.
- 分析地质物理数据,寻找撞击盆地形态的证据.
主要方法:
- 从北尤卡坦地区重力数据的再处理.
- 在埋藏的撞击盆地内分析环状结构.
主要成果:
- 在奇克苏鲁布结构中识别了三个主要环和第四个环的部分.
- 外环表明地形边缘直径近300公里.
- 环的距离与其他陆地多环冲击盆地相似.
结论:
- 奇克苏鲁布撞击结构明显大于此前估计的.
- 自从早期轰炸时期结束以来,奇克苏鲁布是太阳系内部最大的冲击结构之一.
- 这些发现为地球历史上重大冲击事件的规模提供了新的见解.
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