泰坦上的一个刚硬而经受天气侵蚀的冰
D Hemingway1, F Nimmo, H Zebker
1Department of Earth and Planetary Sciences, University of California Santa Cruz, 1156 High Street, Santa Cruz, California 95064, USA. djheming@ucsc.edu
Nature
|August 30, 2013
概括
泰坦 泰坦 泰坦 泰坦 泰坦
科学领域:
- 行星科学 行星科学
- 地质物理学 地质物理学
- 天体生物学 天体生物学
背景情况:
- 据信土星最大的卫星泰坦拥有全球地下海洋.
- 它外层冰的厚度估计在50至200公里之间.
- 以前的模型表明,薄弱的冰,可能由对流或静态补偿驱动.
研究的目的:
- 为了研究泰坦冰的结构性质.
- 为了协调长波长的重力和地形数据.
- 为了评估泰坦外的刚性和地质活动.
主要方法:
- 分析长波长的重力和地形数据,不包括潮和旋转效应.
- 冰内的质量异常的建模.
- 重力场与表面高度之间的相关性分析.
主要成果:
- 在长波长的重力和地形之间发现了显著的反向相关性.
- 负重力异常,归因于冰底部的加厚,主导了表面特征的正异常.
- 这些发现需要一个刚性冰,弹性厚度大于40公里,表面侵蚀/沉积量很大.
结论:
- 泰坦的冰实质上是刚性的,并且在地质上不活跃,刚度低.
- 观察到的重力-地形相关性是由冰底部的地加厚解释的.
- 泰坦的惯性瞬间可能高于先前估计的,这表明中心凝聚率较低.
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