恩塞拉多斯的重力场和内部结构
L Iess1, D J Stevenson, M Parisi
1Dipartimento di Ingegneria Meccanica e Aerospaziale, Sapienza Università di Roma, via Eudossiana 18, 00184 Rome, Italy.
概括
卡西尼号任务数据显示,恩塞拉多有一个地下海洋. 这个区域海,位于30-40公里深,解释了质量异常,并表明土星的内部差异化.
科学领域:
- 行星科学 行星科学
- 天文地质学 天文地质学
- 地质物理学 地质物理学
背景情况:
- 土星的一个小,活跃的卫星恩塞拉多斯是卡西尼号任务的关键目标.
- 了解其内部结构对于评估其潜在可居住性至关重要.
研究的目的:
- 为了确定恩塞拉多的四极重力场和半球不对称.
- 为了研究恩塞拉多的地下结构和内部组成.
主要方法:
- 分析了卡西尼号航天器三次飞越的多普勒数据.
- 计算四极子系数 (J2,C22) 和惯性矩.
主要成果:
- 在南极地区出现负质量异常,被正面的地下异常所补偿.
- 证据表明,在30-40公里的深处有一个区域地下海,延伸到~50°南.
- 轻微偏离水静平衡和惯性瞬间,暗示具有低密度核心的差异化物体.
结论:
- 引力场数据强烈支持恩塞拉多上存在地表下海洋的存在.
- 恩塞拉多表现出显著的内部差异化,这对其地质活动和进化有影响.
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