塞雷斯上的石坑:对其地和演变的影响
H Hiesinger1, S Marchi2, N Schmedemann3
1Institut für Planetologie, Westfälische Wilhelms-Universität, Münster, Germany. hiesinger@uni-muenster.de.
概括
黎明航天器的观测显示,星球表面有大量的石坑,这与冰的预测相矛盾. 坑道形态表明冰岩组成混合, 年代可追溯到几亿年的光滑区域.
科学领域:
- 星球科学
- 地质学
- 天文地质学
背景情况:
- 热化学模型预测Ceres的内部有差异化和冰的地,撞击坑最小.
- 之前的模型表明,由于预期的冰表面有利于放松,因此缺乏大坑.
研究的目的:
- 来自"黎明"号探测器的观测数据.
- 根据火山口形态和分布,调查塞雷斯地的组成和地质历史.
主要方法:
- 分析来自"黎明"航天器的高分辨率图像.
- 对撞击坑的形态研究,包括形状,特征和分布.
- 使用火山口约会技术确定特定区域的绝对模型年龄 (AMA).
主要成果:
- 塞雷斯表面有大量的石坑,而且石坑分布不同,这与之前的预测相反.
- 坑道形态表明地既不是纯冰,也不是纯岩石,具有多边形,露台和倾斜等特征.
- 根据时间模型,Kerwan火山口附近的光滑区域的绝对模型年龄表明形成于5.5亿和7.2亿年前.
结论:
- 塞雷斯的表面比预期的要有更多的石坑,这表明地质历史更为复杂.
- 塞雷斯地的混合冰岩组成影响了火山口的形态和保存.
- 表面特征的约会为塞雷斯的地质演变提供了新的约束.
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