来自InSight无线电跟踪的火星旋转状态和深层结构
Sébastien Le Maistre1,2, Attilio Rivoldini3, Alfonso Caldiero3,4
1Royal Observatory of Belgium, Brussels, Belgium. sebastien.lemaistre@oma.be.
Nature
|June 14, 2023
概括
视觉任务
科学领域:
- 星球科学
- 地质学
- 天文地质学
背景情况:
- 了解火星的内部结构和大气是形成和演变的关键.
- 由于行星内部无法直接进入,因此难以解释全球地质数据.
- 美国宇航局的InSight任务提供了重要的地震和无线电科学数据.
研究的目的:
- 确定火星核心,地幔和大气层的基本特性.
- 用无线电科学数据分别描述火星的核心和地幔.
- 调查火星内部的异常和旋转速度.
主要方法:
- 精确测量火星行星的旋转.
- 在正常模式下检测共振.
- 分析了InSight的无线电跟踪数据.
主要成果:
- 确定液体核心半径 (1.835±55公里) 和密度 (5.9556.290公斤/m3).
- 在核心-地幔边界 (1,6902,110 kg m−3) 呈现密度增加.
- 这表明地幔质量异常.
- 发现火星旋转速度缓慢加速的证据.
结论:
- 探测器的数据使得火星内部结构的详细描述成为可能.
- 结果表明火星地幔内存在内部质量异常.
- 观察到的旋转加速可能与内部动力学或大气/冰盖变化有关.
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